ASTRONOMY

            In the light of

        ISLAM 

 

 

CONTENTS.

 

            Preface                                                                       11

 

CHAPTER 1: SOME IMPORTANT TERMS AND THEIR EXPLANATIONS.

 

1.1       Geography and our Students                                   13

            Useful Geographic Information                                               14

Diameter and radius of Earth                                       16

Continents of the World                                                          16

Oceanography                                                             19

Well known rivers of continents                                              21

Famous mountains of continents                                             22

1.2       Changes in The earth                                               23

Seasons                                                                                    24

Refraction                                                                    27

The Dead Sea                                                              28

Aurora                                                                         30

The Snow Fall                                                              32

The soil                                                                                    33

Atmosphere of the earth                                                          34

Wind system and rain                                                  35

World Distribution of Rain Fall                                               37

Storms and their Types                                                            38

1.3       Interior of the earth                                                  38

Mountain Building . and Ocean Building                     39

Movements of the Earth                                                          41

Theory of continental drift                                          41

1.4       Latitudes and longitudes                                          44

1.5       Coordinate system and their explanation               47

International Date Line                                                            49

Changes in lengths of day and night                            51

Horizontal Coordinate System                                     52

1.6       Some terms and their explanations                          52

Time of Transit                                                                        52

Diurnal Circle                                                              52

Horizon                                                                       53

Great Circle                                                                 54

Declination of the Sun                                                 55

Zones                                                                           55

Normal and abnormal regions                                      55

1.7       Solar and Lunar Eclipses                                         56

Solar Eclipse                                                                56

Lunar Eclipse:                                                              58

Tides                                                                            59

Physical data about the earth                                       60

 

CHAPTER 2: DIRECTIONS

 

2.1       Directions                                                                   61

Cardinal Points                                                                        62

Basic Directions                                                           62

The Geographic North                                                 63

The Magnetic North                                                     63

The True North                                                                        63

The Grid North                                                                        63

Magnetic Declination                                                   64

2.2       Determination of Directions                                     64

With the help of The Pole Star                                     64

Pole Star                                                                      65

The Great Bear                                                                        65

With the help of the Sun                                                          66

            With the help of shadow                                              67

With the help of clock                                                 67

With the help of magnetic compass                             68

Method of finding the sun’s altitude                            69

To find the latitude of any place                                              69

2.3              Behavior of the Holy Prophet (peace be

upon him) and Sahabah towards Qibla                  69

Sun Shadow Method to determine the Qibla direction 71

2.4       Time and Calendar                                                   72

Mean solar day                                                                        73

Sidereal day                                                                 74

Apparent day or apparent solar day                             75

Local Time and Standard Time                                                77

2.5       Calendar                                                                    80

Lunar calendar                                                             80

Hijri calendar                                                               80

Solar or Gregorian calendar                                         80

Luni Solar calendar                                                      82

Solar Hijri calendar                                                      82

 

CHAPTER 3: COMPALATION AND COMPOSITION OF PRAYER TIMES.

 

3.1              Mathematical Method For Finding

Prayer Times and Qibla Direction.              83

Geometry, Trigonometry and Spherical
Trigonometry.                                                              83

Angle                                                                           83

Triangle                                                                       84

Trigonometric ratios                                                     85

Solution of a triangle                                                   86

Spherical triangle                                                         86

3.2       Calculations of Prayer Times.                                  86

Dawn, Isha and Fajar Times.                                       87

Maghrib and Sunset                                                     88

Sharaie Sunrise                                                                        89

Zohar                                                                           90

Declination of the Sun                                                 91

Equatorial Coordinate System                                      92

3.3       Celestial Sphere                                                         92

Right ascension, Vernal and Autumnal

Equinoxes                                                                    92

3.4       Method to Find the Time of Transit                        93

Examples                                                                     94

Basic Formulae                                                                        95

Method to Find Dawn and Isha Time.                          96

Examples                                                                     97

 

Time of Misle Awwal (Asar e Shafi) and

Misle Sani (Asar e Hanfi)                                            103

Examples                                                                     103

            Formula for Dawn                                                      112

Formula for Sunrise and Sunset                                  113

3.5       Altitude Correction Factor                                       114

3.6       Aneroid and Mercurial Barometer                         115

3.7       Tables for altitude correction                                   116

 

CHAPTER 4: ASTRONOMY

 

4.1       Introduction, need and Importance

of Astronomy.                                                            122

Light Year                                                                   123

4.2       Solar System                                                              123

Life on planets                                                             124

Motions of the sun                                                       124

Motion of planets                                                        125

Motions of the earth                                                    126

The sun (The centre of the solar system)                                 127

4.3       Expanse of the Universe                                           127

Some astronomical terms                                             128

4.4       The Planets                                                                130

Mercury                                                                       130

About Iron                                                                   131

Venus                                                                          131

The Earth                                                                     131

Mars                                                                            132

Jupiter                                                                          134

Saturn                                                                          135

Uranus                                                                         137

Neptune                                                                       148

Pluto                                                                            139

Comets, meteors and asteroids                                     140

Some famous stars                                                       141

4.5       Circles on Celestial Sphere                                       144

Great Circle                                                                 144

Small Circle                                                                 144

Celestial Equator                                                          145

Ecliptic                                                                                    145

Horizon                                                                       146

Right ascension and declination                                               147

 

CHAPTER 5: SUBAHE SADIQ AND SUBAHE KAZIB

 

5.1       Subh-e-Sadiq and Subh-e- Kazib                            148

Ancient charts (calendars) for Prayer Times

and Dawn                                                                    150

5.2       Determination of prayer timings                             151

Non Muslim Astronomer’s appreciation                                  154

Guidance through the Holy Qur’an                              155

Astronomical explanation of the term Twilight                        156

5.3       AI Fajrus Sadiq'                                                        157

5.4       AI Fajrul Kadhib'                                                     159

Interplanetary dust within the Zodiacal belt                 161

Types of Fajar                                                             164

5.5       Duration between sunset and Total Darkness or

between Total Darkness and sunrise                       166

5.6       Saying of scholars of ancient past                            171

5.7       An Invitation to Think and Ponder                         172

5.8       A misconception regarding the interval

between dawn and sunrise                                       176

5.9       Time difference due to altitude                                176

A mistake in difference of time in Jantaries                177

An important point to note                                           179

5.10     Nautical Almanac, Astronomical Ephemeris

and Non Muslim Astronomers                                 180

5.11     Further discussion about dawn and false dawn     181

 

 

 

 

CHAPTER 6: PHASES AND SIGHTING OF THE MOON.

 

6.1       The Moon                                                                  183

Physical data of the moon                                           185

Motions of The moon                                                  185

Length of lunar year                                                    186

Longitudinal motion of the moon                                187

Delay in the moonrise                                                  187

6.2       Phases of the moon                                                   187

Web Based Resources of Moon Sighting                                 188

Sharaie Ruet e Hilal .                                                   189

6.3       Use of modern instruments for the

Sighting of the moon                                                 190

6.4       View of Islam about scientific inventions                191

Eid and Eid ul Azha are not our festivals but

occasions of worship                                                   193

6.5       New moon, conjunction                                            198

Existence of the moon                                                 199

Chances of sighting                                                     201

Opinion of experienced observers                               202

Useful facts (To be noted)                                           203

Sighting of the Moon, a Very Unique Question.                      204

6.6       Gregorian calendar and its roots                             205

 

CHAPTER 7: MATHEMATICAL METHOD OF FINDING DIRECTION OF QIBLA

 

7.1       Formula for direction of Qibla                                207

Examples                                                                     207

7.2       Another formula for Qibla                                       210

Examples                                                                     211

7.3                  Method to find The North with the

              help of the sun.                                                        212

 

 

            CHAPTER 8: PLACES WHERE

TWILIGHT DOES NOT END

 

8.1       Regions near the poles of the earth                         214

8.2       The Issues                                                                  215

            The Normal Period and Normal Areas                         216

Abnormal Areas and Different Conventions in Use.   221

8.3       ISTAFTA (Questionnaire)                                       223

Nights in which twilight does not end                          225

Days when the sun does not set                                               225

Days when the sun does not rise                                              225

Appearance of twilight in places near poles

during long nights                                                        226

The shortest day and the longest night                         226

The longest day and the shortest night                         227

The calendar for prayer times for London                   228

8.4       The answer                                                                229

8.5       Tables                                                                         235

8.6       A new method for finding times of prayer in

regions near the poles                                               240

8.7              An Important Proposal                                            241

 

CHAPTER 9: DIRECTION OF QIBLA AND MUSLIMS OF AMERICA

 

9.1       Great circle and Rhumb line for finding

Direction of Qibla                                                      243

9.2       Gnomonic projection                                                248

9.3       Some Important Information                                   251

Measurements, distances, weights, sharaie journey etc            251

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

BLANK

 

 

 

 

 

 

 

 

 

 

PREFACE

In this book an attempt has been made to acquaint the students of formal and religious institutions with elementary but important knowledge of Geography, Astronomy, and Calculations of prayer times, to find direction of Qibla and Ruet e Hilal and teach them these subjects by an easy method. Many books have been consulted. Data and pictures have been taken from various books. This book is a part of a series of books in which prayer times have been compiled and composed for innumerable countries and cities of the world.

            The world known personality of Hazrat Maulana Muhammad Umer Palanpuri (R.A.) is the instigating force behind this work. He, realizing the necessity that since our delegations will visit all parts of the world to learn and teach the religion, direction of Qibla and prayer times will be needed, chose me for the job and guided me through every step. It is due to his affection, love, guidance, advice, and blessings that books containing prayer times have been compiled composed and some of them printed. These prayer timing tables and books were prepared separately for more than 75 countries. Most of the delegations that travel abroad for religious missions are taking advantage from them. May Allah (s.w.t.) accept this effort and make it a means for spreading the religion - Islam.

ACKNOWLEDGMENTS

I have used abstracts and data from many books. Some of them are as follows:

“Fahamul Falkiat” by Hazrat Maulana Shabbir Ahmed Kakakhel, “Falkiat e Jadeedah” by Hazrat Maulana Sameeruddin of Britain, Articles by Dr. Kamal Abdali of America and by Dr. Muhammad Ilyas of Malaysia, an article in Arabic by Dr. Kamaluddin of Riyadh, Saudi Arabia etc.

            In addition, data and text from many other books have been included according to the needs of the students so that they may find convenience in understanding this difficult subject. I regard it my moral responsibility to thank all from the core of my heart as the compilation of this book was possible as a result of their efforts. May Allah (s.w.t.) bless them with good reward. (Amin)

I thank Prof. Syed Shafaat Ali, former Chairman, Department of Mathematics for his assistance in translating my Book “Tasheel-ul Falkiyat”and Mr Riyaz Hassan of Edinburgh for proof reading.

            By the blessing and grace of Allah (s.w.t.), I had the honour of teaching and guiding the students of Jamia Ashrafia, Lahore, Jamia Farooqia, Shah Faisal Colony, Jamia Islamia Allama Binori Town, Karachi; Jamia Binoria, Site, Karachi; Jamia Imdadul Uloom, Nazimabad, Karachi and respectable Mufti Shaheban and teachers of various religious Institutions. Recently I was invited to deliver lectures on these topics by the Madrasatul Islam of Glasgow, Scotland. I had the honour of acquainting them with the art of composition and compilation of prayer times and direction of Qibla. On their advice and demand this book is being presented.

            May Allah (s.w.t.) bless my late parents and my late elder brothers Abdul Hafeez Qureshi and Abdul Majeed Qureshi and award a place under His protection. I was able to start work on this book due to their blessings. I am also thankful to my brothers Gulzar Muhammad Qureshi, Prof.Anwar Muhammad Qureshi and Izhar Muhammad Qureshi whose blessings and good wishes assisted to continue this task. May Allah (s.w.t.) give them great reward.

 

Abdul Lateef

Karachi, 2, August 2011, 1st Ramzan 1432

 

 

CHAPTER 1

SOME IMPORTANT TERMS AND THEIR EXPLANATIONS

 

1.1       Geography and our Students

It is my personal experience that the students of our religious institutions and different colleges and universities of Pakistan are unaware of the elementary information about Geography. When a cricket team came to tour Pakistan, I said to the students that this team has come from West Indies or New Zealand and asked them to tell me where West Indies or New Zealand is situated. No one knew. And if some one gave an answer, it was wrong. Our students are completely ignorant about it.

            This is my personal observation that students of Pakistani schools and colleges are being, intentionally or unintentionally, kept in the dark about geographical locations and distances of other countries from us. Maybe it is a part of our education policy. A subject Social Studies (consisting of many subjects) have been included in school curriculum. Students can neither learn Geography from it nor History. Most of the students do not even know where East Pakistan was and what the distance between East and West Pakistan was. They were astonished struck when informed that we traveled over a thousand miles from Karachi to Decca in an aero plane over India via Delhi and that former East Pakistan was surrounded by India.

            Our students do not even know the geography of our own country. They were amazed when informed that boundaries of Jammu and Kashmir touch five countries. That boundary of Jammu and Kashmir touches on one side with Pakistan, on the other it meets India; in the north east is the border of China, in the West, across a few mountains, Afghanistan and in the north former Russia. After dissolution of U.S.S.R., there are many Muslim states in that region. You can imagine the standard of our students. How much geography they know? The countries that gained independence from U.S.S.R. include East Germany, Poland, Hungary, Czechoslovakia, Albania, Romania, Bulgaria, Herzegovina, Tajikistan, Turkmenistan, Azerbaijan, Kazakhstan etc. India and Pakistan gained independence in 1947. In 1961 Sindh Taas Pact (Indus Water Treaty) was signed. In 1971 after the fall of East Pakistan, Bangladesh was formed.

 

Useful Geographic Information

فَلِلَّهِ ٱلۡحَمۡدُ رَبِّ ٱلسَّمَـٰوَٲتِ وَرَبِّ ٱلۡأَرۡضِ رَبِّ ٱلۡعَـٰلَمِينَ (٣٦) وَلَهُ ٱلۡكِبۡرِيَآءُ فِى ٱلسَّمَـٰوَٲتِ وَٱلۡأَرۡضِ‌ۖ وَهُوَ ٱلۡعَزِيزُ ٱلۡحَكِيمُ (٣٧)  {الجاثية 45}           

  

Translation:   Then Praise be to Allah Lord of the heavens and Lord of the earth Lord and Cherisher of all the worlds! (36) To Him be Glory throughout the heavens and the earth: and He is Exalted in Power, Full of Wisdom! (37)

 

Some basic and useful information about the earth

29% of the earth’s area consists of dry land and 71% is sea and water i.e. there are three parts of water and one part of dry land. The study of the earth’s geography is divided in three parts:

i. Lithosphere: In this part we study the landscape form, shape, high and low parts (mountains, plane areas, plateaus, topography), surface of the earth, shape of the earth, earthquakes, volcanoes, motions of the earth, mountain and ocean building, natural resources, mineral resources, rocks etc. This is called physical geography.

 

ii. Hydrosphere: In this part, we study oceans, water reservoirs, rivers, lakes, water resources etc.

 

iii. Atmosphere: In this we study atmospheric pressure, wind velocities, wind directions, temperature, weather conditions, insulation heat of the sun, clouds, thunder, lightning in clouds, rain, snow, hail, cyclones, anticyclones etc.

Geology: In this subject we study about the inner layers of the earth, internal structure, inner natural resources (petroleum, natural gas), rocks, minerals (Iron, silver, gold, copper, diamonds, coal etc.). The earth is spherical in shape.

 

 وَٱلۡأَرۡضَ بَعۡدَ ذَٲلِكَ دَحَٮٰهَا (٣٠) {النَّازعَات 79}         

 

Translation: And the earth, moreover; hath He extended (to a wide expanse): (30)

 

Maximum circumference of the earth is at the equator which is 24901.55 miles or 40075.16 km. long. The polar circumference is 24859.82 miles or 40008 km.

The equator divides the earth in two equal parts. The northern part is called the northern hemisphere and the other the southern hemisphere. The latitude at all points on the equator is zero degrees. The north and the south latitudes are measured from the equator.

 

 

 

 

 

 

 


Diameter and radius of the earth

Diameter means a well dug through the centre of the earth which reaches the surface on the other side. The depth up to the centre is called the radius of the earth. The diameter of the earth at the equator is 7926.41 miles or 12756.32 km. The diameter from the North Pole to the South Pole is 7899.83 miles or 12713.54 km.

 

The highest and the lowest places on the earth

Mount Everest (in Nepal) of the Himalayan Range is the highest point on the earth having a height 8848 meters. The deepest part of the earth is 399 meters (about 1,309 ft) below the sea level in the Dead Sea.

 

The hottest and the coolest place on the earth

The hottest place is the place called Al Aziziyah in Libya, Africa. The temperature there reaches 58o C. The coolest place is Vostok in Antarctica near the South Pole. The temperature there falls down to – 89.6o C.

 

ٱلَّذِى خَلَقَ ٱلسَّمَـٰوَٲتِ وَٱلۡأَرۡضَ وَمَا بَيۡنَهُمَا فِى سِتَّةِ أَيَّامٍ۬ ثُمَّ ٱسۡتَوَىٰ عَلَى

ٱلۡعَرۡشِ‌ۚ ٱلرَّحۡمَـٰنُ فَسۡـَٔلۡ بِهِۦ خَبِيرً۬ا (٥٩)  {الفُرقان 25 }             

Translation: He Who created the heavens and the earth and all that is between in six days, and is firmly established on the Throne (of authority): Allah Most Gracious: ask thou, then, about Him of any acquainted (with such things). (59)

Continents of the World

Large masses of lands are called continents. There are seven continents in the world:  

i. Asia         ii. Europe             iii. Africa         iv. Australia          v. North America               vi. South America

vii. Antarctica

 

Important countries and cities of continents:

 

1. Asian Continent.

 

  • The Middle East (The Arabian Peninsula): Saudi Arabia, (Mecca Mukarrama, Medina  Munawwara.); Syria (Damascus), Jordan (Oman), Yemen (Aden), Palestine. Kuwait, Iraq (Baghdad), Bahrain. Gulf States: Dubai, Sharjah, Qatar, Abu Dhabi, Doha, Al Amarat.

 

  • South Asia: Pakistan, India, Sri Lanka, Bangladesh, Myanmar (Burma), Nepal (Katmandu), Maldeep, Bhutan.

 

  • South East Asia: Thailand (Bangkok), Vietnam, Cambodia, Singapore, Malaysia, Indonesia etc.

 

Central Russia and Independent Muslim States:

 

  • Uzbekistan – Fargana Toshkent, Nmangan
  • KyrgyzstanOsh
  • Kazakhstan – Almaty, Shymkent, Astana
  • TajikistanDushanbe
  • Turkmenistan – Ashhgabat
  • Astrakhan -  Astrakhan
  • AzerbaijanBaku
  • Chechnya – Groznyey
  • Bosnia and Herzegovina -Sarajevo

.

East Asia: China (Beijing), Japan (Tokyo), Korea (Seoul), Hong Kong etc.

2. European Continent:

·         Spain (Madrid), France (Paris), Germany (Berlin), Poland, Bulgaria, Rumania, Albania, Britain, Finland, Russia, Norway, Sweden, Denmark, Holland, Italy, Czechoslovakia, Chechnya, Bosnia, Herzegovina, Turkey (Ankara) etc.

 

3. African Continent:

·         There are about 48 countries in Africa. Some of them are: Egypt, Libya, Morocco, Mali, Sudan, Ethiopia, Nigeria, Tanzania, South Africa, Zimbabwe, Somalia, Togo, Benin, Niger, Madagascar, Mauritius, Jazeeratul Qamar (Comoros Island), Mozambique, Congo, Central African Republic etc.

 

4. The north American Continent:

 

·         Canada, U.S.A., Mexico, Panama and other Central American countries. 

5. The south American Continent:

 

·         Brazil, Lima, Lampas, Chile, Peru, Falkland Islands, Guyana etc.

6. Australian Continent:

 Australia was known as terra incognita (land unknown)

·         Australia (Sydney, Melbourne, Canberra), New Zealand.

 

What we study in Geography

In this subject we study, in detail, Physical aspects of the land known as topography, land forms, atmospheric conditions, Oceanography, Geomorphology, anthropology, some aspects of Meteorology, Cartography, Statistics, Agricultural, industrial,  Commercial and Economic Geography, demography, town planning , Land use, map making, Urban and rural Geography etc.

 

Oceanography                          

Oceans of the world

Atlantic Ocean: Europe and Africa are situated on the East of this ocean; North and the South America are on its West.

Pacific Ocean: North and The South America are on its East side and Australasia and Asia are on its West.

Indian Ocean: Australasia is located on its east, Africa on the west and the Arabian Sea, Bay of Bengal and South Asian countries (India, Pakistan) are on its north.

Arctic Ocean: It is the frozen sea near northern Europe, the north Canada and the North Pole.

Antarctic Ocean: It is the frozen area near the South Pole.

Mediterranean Sea: Europe lies on its north and Africa on its south.

Black Sea and Caspian Seas are located in Europe.

Arabian Sea, Red Sea and Persian Gulf are in the Middle East.

 

Depth of Oceans

Scientific research has divided the oceans into three main parts according to depth.

i.          Bathal Zone

Its depth is 6560 feet or 2000 meters. There is sufficient sunlight in it. Fish live in this zone and ships travel in it.

ii.         Abyssal Zone

It lies below the Bethel Zone. Its depth ranges from 2000 meters to 6000 meters. Or from 6560 feet to 19690 feet. The suns rays cannot reach this part, so it remains dark.

iii.        Hadal Zone

It is below Bethel and Abyssal zones. Absolutely no sunlight reaches here. There is complete darkness in this region. Only those creatures are found in this zone that can live under these extreme conditions. Its depth ranges from 6000 meters i.e. 19690 feet to the bottom of the ocean.

 

أَوۡ كَظُلُمَـٰتٍ۬ فِى بَحۡرٍ۬ لُّجِّىٍّ۬ يَغۡشَٮٰهُ مَوۡجٌ۬ مِّن فَوۡقِهِۦ مَوۡجٌ۬ مِّن فَوۡقِهِۦ سَحَابٌ۬‌ۚ ظُلُمَـٰتُۢ بَعۡضُہَا فَوۡقَ بَعۡضٍ إِذَآ أَخۡرَجَ يَدَهُ ۥ لَمۡ يَكَدۡ يَرَٮٰهَا‌ۗ وَمَن لَّمۡ يَجۡعَلِ ٱللَّهُ لَهُ ۥ نُورً۬ا فَمَا لَهُ ۥ

 مِن نُّورٍ (٤٠)       {النُّور 24}                                                         

Translation:  Or (the Unbelievers' state) is like the depths of darkness in a vast deep ocean overwhelmed with billow topped by billow, topped by (dark) clouds: depths of darkness one above another: if a man stretches out his hand, he can hardly see it! For any to whom Allah giveth not light there is no light! (40)

 

Deepest Ocean

The place Guam in the sea called Mariana in the Pacific Ocean is believed to be the deepest sea. Its depth is believed to be 11033 meters. Usually the depth of sea is 3730 meters.

 

Ocean Currents

Water of oceans appears to be stationary but there are rivers several miles long and wide flowing in them. These are called ocean currents. There are two types of ocean currents:

i. Warm ocean currents           ii. Cold ocean currents

If an ocean current is warm, it heats the nearest shore and causes rain in that region. Since the rays of the sun fall vertically near the equator all year round, they heat the ocean water which travels in the form of a current to distant cold countries. This goes on continuously. When a current flows, it appears that a huge river is flowing in the ocean. Water travels with large waves. Following are some of the reasons for ocean currents:

·         Fast moving wind in the same direction.

·         Difference of salt in ocean water at different places

·         Earthquakes and volcanoes in oceans

·         Tides

Ocean currents have different names. They are named after the places through which they pass. Near the equator it is called warm equatorial current. The current in the Atlantic Ocean which moves from the equator to Europe is called Warm Gulf current or Gulf Stream. Water in the western shore of Europe does not freeze due to it and remains open to ships all year round. The harbor Archangel in northern Russia remains functional throughout the year due to this current.

 

Gulf Stream

When warm water flows from the Gulf of Mexico (America) to Britain and Europe in the north east direction, it warms the entire region. It travels in the Atlantic Ocean as if a large river is flowing. This stream travels 160 km or 110 miles in a day. Its width is 60 km. or 37 miles and depth is 600 meters or 2000 feet. Its water is very prominent in the ocean.

 

وَهُوَ ٱلَّذِى مَرَجَ ٱلۡبَحۡرَيۡنِ هَـٰذَا عَذۡبٌ۬ فُرَاتٌ۬ وَهَـٰذَا مِلۡحٌ أُجَاجٌ۬ وَجَعَلَ

بَيۡنَہُمَا بَرۡزَخً۬ا وَحِجۡرً۬ا مَّحۡجُورً۬ا (٥٣)  {الفُرقان25}             

Translation: It is He Who has let free the two bodies of flowing water: one palatable and sweet and the other salt and bitter; yet has He made a barrier between them, a partition that is forbidden to be passed. (53)

 

Well known rivers of continents

Asia: In Pakistan there are 5 rivers in Punjab; Sutlej, Bias, Ravi, Chanab and Jhelum. The sixth is the Indus River. According to Sindh-Taas pact (Indus Water Treaty), 3 eastern rivers (Sutlej, Bias and Rave) are owned by India and the western rivers Chanab, Jhelum and Indus are owned by Pakistan. Swat and Kabul rivers are also in Pakistan. Warsaw dam was built on Kabul River. The famous city of Lahore is situated at the bank of Ravi River. Mangla Dam is on the river Jhelum in Azad Kashmir.

India: Ganga, Jamuna, Narbada, Tapti, Krishna, Kowari and Gadavari are famous rivers of India. Delhi is on the bank of Jamuna. Allahabad city is located at the junction of Ganga and Jamuna.

Iraq: Rivers Dajla and Farat are in Iraq. The famous city of Baghdad is situated at the place where these rivers merge.

Bangladesh: Rivers Brahamputra and Budiganga flow in Bangladesh. Decca city is situated on the bank of Budiganga.

Australia: Rivers Murray and Darling flow in Australia.

Europe: Famous Rivers of Europe are Volga, Volta, Dnieper, Dniester etc. Ob, Yenisey and Lena flow into Russia.

River Thames flows in Britain. London is on its bank. River Seine is in France. Paris is on its bank. River Po is in Italy.

Africa: The longest river is the world in the river Nile. It flows in Africa and passes through many countries including Egypt. Other African rivers are river Niger, Congo River, river Limpopo, river Zambezi etc.

North America: Mississippi river and Missouri Rivers are famous rivers of U.S.A.

South America: River Amazon in Brazil is the largest river in the world.

 

Famous mountains of continents

أَلَمۡ نَجۡعَلِ ٱلۡأَرۡضَ مِهَـٰدً۬ا ( ٦ )  وَٱۡجِبَال أَوۡتَادً۬ا(٧)  {النّبَإِ 78}         
Translation: Have we not made the earth as a wide expanse, (6) and the mountains as pegs? (7)

وَٱلۡجِبَالَ أَرۡسَٮٰهَا (٣٢) {النَّازعَات 79}                             

Translation: And the mountains hath He firmly fixed― (32)

 

The highest mountain in the world is the Himalayas in Asia. It has many branches (Mt. Sewalek, Mt. Murrey, Mt. Hindu Kush, Mt. Karakoram, Mt. Laddakh, Mt. Suleman etc.) All these mountain ranges are from the east to the west and are all parallel to each other. There are valleys between them in which rivers flow. All rivers in Pakistan emerge from these mountains. They all flow in Kashmir from the east to the west, turn to the south and enter Sindh passing through Punjab. Finally they fall into the Arabian Sea near Keti Bandar, east of Karachi forming a delta. Many dams and bridges are made on these rivers. Canals from these dams supply water for agriculture to plane areas of Sindh and Punjab. The irrigation system of Pakistan is one of the largest in the world. If we add the lengths of all the rivers and canals of Pakistan, the sum is about 75,000 miles. Compare that to the circumference of the earth which is 25,000 miles. Thus rivers and canals of Pakistan can be wrapped round the earth three times. Many problems arise due to the irrigation system. Soil salinity and water logging are the most important problems. It is estimated that a hundred thousand square miles of land becomes useless for agriculture because of salinity and water logging. Work is in progress to overcome this problem.

Famous mountains of Europe are Mount Alps, Mount Quaff,  Mount Atlas, and Mount Ural etc. On the western part of the North America Rocky Mountain is stretched from the north to the south. On the western coast of South America Andes Mountain range runs north to south.

 

1.2       Changes in the Earth

Continuous changes are taking place in the earth since it was formed. Besides motion of the earth, flowing lava, flowing water, storms, hurricanes, gusts of winds, glaciers, earth quakes, volcanoes, ocean waves, flood etc. are continuously changing the shape of the earth. Rivers, glaciers and wind move land from one place to another. The rocks keep expanding and shrinking due to heat and cold for thousands of years. This process breaks them into pieces which are spread over wide areas by rain and wind. Men and animals also change the shape of the earth according to their needs. They plough the land at places, build large dams at other places; they dig canals and make large buildings. Since the formation of the earth, different processes are busy in changing its form.

 

Seasons: The earth moves round the sun in its orbit once a year. This annual motion causes changes in seasons. Some times the sun rises over the tropic of Cancer, and some times over the tropic of Capricorn. It keeps moving between them all year round. When the sun rises over the tropic of Cancer, it is summer in the northern hemisphere and when it rises over the tropic of Capricorn, it is summer in the southern hemisphere.

 

Solstices and change of declination: The earth changes its direction of motion twice a year while moving round the sun. But since it appears to us that the sun is moving round the earth, we can say that the sun changes its direction twice a year. Firstly it moves from the equator towards the north. After moving up to 23.5 degrees north, it changes direction and starts moving towards the south. The point where it changes the direction of motion to the south is called Summer Solstice. It occurs on 21st June. Then moving south it crosses the equator again and keeps moving south up to 23.5 degrees south on 22nd December and again reverses the direction of motion to the north. This point is called Winter Solstice.

 

Vernal and Autumnal Equinoxes

The point where the sun crosses the equator moving from the south to the north is called Vernal Equinox. It occurs on 21st March. The point where the sun crosses the equator moving from the north to the south is called Autumnal Equinox. It occurs on 21st September.

 

Seasons

21st June: On 21st June the sun is in the northern hemisphere over Tropic of Cancer. It is summer season in the northern hemisphere. It is called Summer Solstice. It is very hot in June, July. The days are longer than the nights. The inclination of the axis of the earth towards the sun is shown in the figure on next page.

 

21st December: On 21st December the sun is over the Tropic of Capricorn in the southern hemisphere. It is winter in the northern hemisphere. This is called Winter Solstice. The rays of the sun fall obliquely on the northern hemisphere. Days are short and nights are long. The inclination of the axis of the earth towards the sun is shown in the figure on next page.

 

21st March: On 21st March the sun is over the equator again. The rays of the sun fall equally on both hemispheres. It is spring season in the northern hemisphere. The weather is pleasant. Fruits start ripening. It is called Vernal equinox. Lengths of days and nights are equal. The position of the earth’s axis is shown in the figure below.

 

21st or 22nd September: Somewhere on 21st or 22nd September the sun is again over equator but is moving towards the south. The rays of the sun fall equally on both hemispheres. It is autumn season in the northern hemisphere. Summer ends and winter is about to begin. The leaves of trees start falling. Lengths of days and nights are equal. It is called autumn equinox. The position of the earth’s axis is shown in the figure 1 below.

 

 

 

 

                                                                Zenith

 


                                          23.5o                                      North Pole

 

 

                   

                                – 23.5                                                      Horizon

                                                                        Summer solstice

 

                                                                                                     Equator

                                                                                    

                                                                Winter solstice

Fig. 1

 

 

 

 


                                                                                                                   Sun

 

 

 

                                                   

                                21st March and 21st September : Sun rays falling on equator

 

 

 

 

 


                                                                                                                         Sun

                               

 

 

                                21st June : Sun rays falling on Tropic of Cancer

 

 

 

 


                                                                                                                           Sun

 

 

 

 

 

 

                                21st December: Sub rays falling on Tropic of Capricorn

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Fig.2 The seasons result because the tilted earth’s axis keeps a constant orientation in space as the earth revolves about the sun.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Refraction (allusion of eye) and Sharaie Sunrise and Sunset

The sun is a disc of light whose average width is equivalent to about 32 minutes of arc as seen from the earth. Sunrise is defined as the instant of appearance of the upper rim – called upper limb of the sun’s disc above the horizon, and sunset is defined as the instant of total disappearance of the upper limb below the horizon.

Theoretically it rises and sets when its centre reaches at 0° on the horizon. But practically it does not rise or sets at this altitude. The light rays reaches to the eyes of the observer due to the refraction of light. The sun practically rises and sets as well when its centre is at 50º below the horizon in which 34´ are the horizontal refraction of light and 16΄ due to the semi-diameter of the sun.

Geographical and astronomical sun rise and sun set is different from the Sharaie rise and set. When the upper limb (which was visible due to refraction) disappears and completely goes beneath the horizon the time of Maghrib starts.  In like manner when the upper limb appears due to refraction, according to Sharaia, it is considered as the time of sunrise  

 

The Dead Sea                  

Arabic al-Bahr al-Mayyit also called the Salt Sea is a salt lake bordering Jordan to the east and Palestine and the West Bank to the west. Its surface and shores are 423 meters (1,388 ft) below sea level, the lowest elevation on the Earth's surface on dry land. The Dead Sea is 399m (1,309 ft) deep, the deepest hypersaline lake in the world. With 33.7% salinity, it is also one of the world's saltiest bodies of water. It is 8.6 times saltier than the ocean. This salinity makes for a harsh environment in which animals cannot flourish, hence its name.

 


The Causes of Its Depth

Usually we do not understand and recognize, but it is a reality that when people go astray and knowingly indulge in sinful activities without the fear of life after death or the doomsday and do not care for the commands of their Creator Allah subhanaho wa taala (Lord of the entire universe) they deserve a curse, and sever punishment from the Heavens.

Allah (s.w.t) clearly invited the attention, in the holy Qur’an, of every one and particularly of those who have wisdom, to ponder and think what has been written therein. The events of the past nations that are mentioned in the holy Qur’an are the lessons for the entire humanity.

 

Prophet Lut (Alyhis Salam)

The Dead Sea is near the land in which the Prophet Lut (Alayhis Salam) lived. According to the teachings of Islam the people in this area were extremely wicked for their acts of homosexuality, robbery and murder. By the command of Allah (s.w.t), Prophet Lut (AS) preached to his people to repent and turn to Allah. They arrogantly refused to leave their wicked ways, sinful, shameful and dirty  habits and they continuously rejected the preaching of Prophet Lut (AS), except for a very few.

Every message that was brought to them, they flipped it to satisfy their own wicked way of life. The People of Lut (AS) received many warnings to repent or be punished but they did not take any notice seriously. They were committing blunder, and were not ready to listen to the warnings. Finally Allah sent three angels as handsome young men to be guests of Prophet Lut (AS), when the people heard of this they rushed to Lut's home. The people demanded that these young men be given to them as they wanted to perform their wicked acts with them as well. One of the angels, angel Jibrail (AS), gave Prophet Lut the warning to leave the town with his band of believers and do not look back. The entire town and its people were lifted up by angel Jibrail and flipped upside down and were sent smashing down to earth, causing the ground to cave in. Thus, the lowest land on Earth was formed because of this punishment. This event is an eye opening incident for all those who have some wisdom.

Dimentions

The Dead Sea is 67 kilometers (42 mi) long and 18 kilometers (11 mi) wide at its widest point. It lies in the Jordan Rift Valley, and its main tributary is the Jordan River.

The Punishment

The town and all the wicked people were thrown in the newly formed cave and submerged under this extremely salty and dense sea.

Nearly eight times as salty as the ocean, the Dead Sea contains at a depth of 305 m (1,000 ft) some 27 percent solid substances: sodium chloride, (common salt) magnesium chloride, calcium chloride, potassium chloride, magnesium bromide, and many other unknown substances.

Streams: The Jordan River is the only major water source flowing into the Dead Sea, although there are small perennial springs under and around the Dead Sea, creating pools and quicksand pits along the edges. There is no outlet Rainfall is scarcely 100 mm (4 in) per year in the northern part of the Dead Sea and barely 50 mm (2 in) in the southern part. The Dead Sea zone's aridity is due to the rain shadow effect of the Judean Hills. The highlands east of the Dead Sea receive more rainfall than the Dead Sea itself.

Climate

The Dead Sea's climate offers year-round sunny skies and dry air. It has less than 50 millimeters (2 in) mean annual rainfall and a summer average temperature between 32 and 39°C (90 and 102°F). Winter average temperatures range between 20 and 23°C (68 and 73° F). The region has weakened ultraviolet radiation, particularly the UVB (erythrogenic rays), and an atmosphere characterized by a high oxygen content due to the high barometric pressure.

 

Dead Sea

Coordinates:                31°20’ N 35°30’ E

Lake type:                   Endorheic hypersaline

Primary inflows:          Jordan River

Primary outflows:       None

Catchment area:          41,650 km2 (16,080 sq mi)

Aurora                   

Extremely beautiful and colorful clouds, arches, bands, luminous and attractive forms near the poles

 

What Do We Mean By Aurora?

An aurora is a natural light display in the sky, particularly in the Polar Regions, caused by the collision of charged particles directed by the Earth's magnetic field. An aurora is usually observed at night and typically occurs in the ionosphere. It is also referred to as a polar aurora or, collectively, as polar lights. These phenomena are commonly visible between 60 and 72 degrees north and south latitudes, which place them in a ring just within the Arctic and Antarctic polar circles.

In northern latitudes, the effect is known as the aurora borealis (or the northern lights). They are most visible closer to the poles due to the longer periods of darkness and the magnetic field. Typically the aurora appears either as a diffuse glow or as "curtains" that approximately extend in the east-west direction. At some times, they form "quiet arcs"; at others ("active aurora"), they evolve and change constantly. Each curtain consists of many parallel rays, each lined up with the local direction of the magnetic field lines, suggesting that auroras are shaped by Earth's magnetic field.

 

Some shapes and forms of aurora

The auroras assume an endless variety of forms including:

 the filaments diverging towards the zenith, and beautiful curtains, fans, flames or streamers of various shapes. the aurora arch, a luminous arc lying across the magnetic meridian, the aurora band, generally boarder and much more irregular than the arch, filaments and streamers at right angle to the arch or band, the corona, a luminous circle near the zenith, aurora clouds, indistinct nebulous masses, which may occur in any part of the heavens. The aurora glow, a luminous appearance high in the sky

 

“…The aurora borealis shines above Bear Lake Red and green aurora in Fairbanks, Alaska Northern lights with very rare blue light over Moskosel, Lapland in Sweden” From Wikipedia, the free encyclopedia

 

The Snow fall and the beautiful forms and designs of snow flakes

Precipitation results when air rises and is adiabatically cooled below the dew point so rapidly that not only do clouds form, but rain, hail or snow produced as well.

As a matter of fact precipitation results when condensation is occurring rapidly within a cloud. Snow consists of masses of crystals of ice, grown directly from the water vapour of the air, where air temperature is below freezing. Individual snow crystals, which can be carefully caught upon a black surface and examined with a strong magnifying glass, develop in six-sided, flat crystals, or as prisms. They display infinite variation, shapes and beautiful designs, in their extremely beautiful symmetrical pattern. Following is a picture of tiny snow fakes. Countless beautiful designs and formation can be seen through extraordinary strong magnifying glass, Allah (s.w.t) is the Creator and see how the beauty of these snow flakes are produced by Him.  The following figure shows snowflakes which are made up of aggregates of tiny hexagonal ace crystal such as these (photo by Ewing Galloway).

Snow

 

 

The Soil                                                         

Many of us think of the soil as a lifeless, residual layer, which has somehow accumulated over a long period of time and which merely holds a supply of ingredients necessary for plant growth.

It is very interesting to note Muslims and particularly the Arab Muslims were the first who introduced the subject of SOIL SCIENCE. Their work and research contributions were presented, for the first time, by them in the Arabic language. Later on their marvelous and novel work was translated in Russian Language, which was taken by the western scientists for translation in English language. Now because of their work, we have, in almost all the countries, a number of Soil Science laboratories.

In soil science we study sand, clay and loam’s texture, tint, size and the presence of organic and inorganic material – known as Humus. Soil constitution covers such properties as compactness, stickiness, porosity, and consistency. Detailed study and its survey provide sufficient information for the selection of seeds and to decide what to grow, and what are the deficiencies of ingredients required for a particular plantation.

 

Atmosphere of the earth

Although we are not constantly aware of it, Allah s.w.t. blessed us with the most vital need – wind- without which life is impossible. Air is a tangible material substance. At sea level, the atmosphere exerts a pressure of about fifteen pounds per square inch on every solid or liquid surface exposed to it. Its unique quality is that in an upward direction, both density and pressure of the air fall off rapidly.

Force of gravity is present every where in the Universe. Due to this force the heavenly bodies retain their positions and planets revolve around their parent star in fixed orbits. On the other hand air, oxygen, water vapors, moderate heat and cold needed for existence of human beings and animals are available only on the earth up to a limited height. This sphere of air is called the earth’s atmosphere. When anyone travels in space beyond the earth, they have to wear special space suits and have to carry oxygen to breath.

 

 

The scientists divide the atmosphere in five parts.

i.          Exosphere       ii.         Thermosphere 

iii.        Mesosphere     iv.        Stratosphere   

v.         Troposphere

 

These five layers of gas, water vapors etc. envelopes the earth. It appears that the earth has been wrapped in five sheets consisting of these layers. The earth and every thing on it are fixed inside these spheres. It is the greatness of Allah (s.w.t.) that when the earth travels with high speed around the sun, these five layers travel with it at the same speed. No matter how fast the earth moves or rotates around its axis, nothing can leave the earth or fall off due to pressure of these layers and gravitational pull of the earth. If something escapes the gravitational force of the earth, it is suspended in space and revolves round the earth. This is the principle on which artificial satellites and space ships revolve round the earth without any fuel. They cannot return to the earth without external force.

 

Wind system and rain

أَلَمۡ تَرَ أَنَّ ٱللَّهَ أَنزَلَ مِنَ ٱلسَّمَآءِ مَآءً۬ فَسَلَكَهُ ۥ يَنَـٰبِيعَ فِى ٱلۡأَرۡضِ ثُمَّ يُخۡرِجُ بِهِۦ زَرۡعً۬ا مُّخۡتَلِفًا أَلۡوَٲنُهُ ۥ (٢١)  {الزُّمَر  39}                                    

Translation: Seest thou not that Allah sends down rain from the sky, and leads it through springs in the earth? Then He causes to grow, therewith produce of various colours: (21)

 

وَيُنَزِّلُ مِنَ ٱلسَّمَآءِ مَآءً۬ فَيُحۡىِۦ بِهِ ٱلۡأَرۡضَ بَعۡدَ مَوۡتِهَآ‌ۚ إِنَّ فِى ذَٲلِكَ لَأَيَـٰتٍ۬ لِّقَوۡمٍ۬ يَعۡقِلُون (٢٤)  {الرُّوم 30}                                                          

           Translation: and He sends down rain from the sky and with it gives life to the earth after it is dead: verily in that are Signs for those who are wise. (24)

 

وَأَنزَلۡنَا مِنَ ٱلسَّمَآءِ مَآءَۢ بِقَدَرٍ۬ فَأَسۡكَنَّـٰهُ فِى ٱلۡأَرۡضِ‌ۖ وَإِنَّا عَلَىٰ ذَهَابِۭ بِهِۦ   لَقَـٰدِرُونَ (١٨) {المؤمنون 23 }                                       

Translation: And we send down water from the sky according to (due) measure, and we cause it to soak in the soil; and we certainly are able to drain it off (with ease). (18)

 

Wind system: It is our observation that steam rises up from a cup of hot tea. Hot air is light and light things move up. On the other hand, cold air is heavy and it moves down from the upper atmosphere. The wind system is due to difference in temperatures. In hot regions, the air becomes warm. The atmospheric pressure decreases due to lighter air. On the other hand, in colder regions, the air is heavier and thus pressure increases. The air comes down from the upper layers.

Let us take Karachi as an example. When the weather is hot, the land becomes very hot. It is difficult to walk bare footed in open parts of a mosque at the time of Zohar. But if some one puts his hand in the water of the sea at the same time, he will feel that the water is not so hot. Thus on dry land, due to heat air becomes hot, light and moves up creating low pressure whereas over the sea, the air is cold and heavier creating high pressure. When the air moves up on dry land, it creates a vacuum. It is the law of nature that no place can be without air, therefore the wind starts blowing from the sea to the land. The wind blowing from the sea to the land is called Sea breeze.

It is a rule that wind always blows from high pressure to low pressure regions.

            In winter when it is very cold in Karachi, the sea water is not as cold as dry land. Thus the air on land is heavier and has higher pressure. At the same time sea water is not so cold, so the air is warmer, lighter and has low pressure. The wind starts blowing from the land to the sea. Such winds are called Land breeze.

            The winds blow all over the world under the same system i.e. there will be high pressure on colder areas and low pressure on warmer areas, the wind blows from high pressure to low pressure regions.

            The sea breeze brings clouds and causes rain. There are many causes for rain. There are many types of clouds as well. Regions near the equator are very hot; the air becomes heated and moves up usually up to 3 or 4 O’clock in the evening. Clouds are formed and heavy rain falls almost every day in the evening. Due to extreme heat, daily rain and productive earth, there are dense forests in these regions. Usually the trees are hundreds of feet high. The forests are so dense that the sun light cannot reach the earth.

 

World Distribution of rain fall

Equatorial regions

Rain fall is very heavy, more than 80 inches, in this zone, where high temperature, and great oceanic expanse, large amount of water vapor unstable weather conditions persist. Virtually rainfall, in this region, is called rainfall of convectional type.

 

Subtropical Zone

In this zone rainfall is very light .The deserts of North Africa, Arabia and Iran lie along this zone as well as those of Australia, South Asia - Pakistan, India and Sri Lanka, South Africa and west coast of South America.

The monsoon winds of Asia largely control rainfall of this zone. Monsoons are the seasonal winds. Winds blow from High Presser to Low Presser. Winds entering into this zone bring rainfall from the oceans.

 

Middle Latitudes

Precipitation in the middle latitudes shows clearly the effect of the prevailing westerly winds. Western continental coasts within the latitude range 35 to 60 degrees appears as a narrow strip of heavy precipitation.

Rain shadow deserts

Rain shadow deserts are developed in the westerly wind belt, in the lee of coastal range. The best example is the Great Basin Desert of Nevada.

Arctic region

In Arctic regions, precipitation is very small in terms of total inches annually. The atmosphere here is at prevailing low temperature and thus does not hold large quantities of water vapors from which precipitation can be produced.

Storms and Their Types

Thunderstorms may be classified into several types, based on the mechanism or cause of initial lift of the air column that sets off the spontaneous growth of the storm.

One type is the thermal, or air mass thunderstorm. The torrential monsoon rains of the Asiatic and East Indian mountain ranges are largely of this type. For example, Cheerapunji, a hill station, facing the summer monsoon, air drift in north east India, results in an average 426 inches of rainfall annually.

 

1.3       Interior of the Earth

Earthquakes and Volcanoes

Four parts of the earth: Geologists study the interior of the earth. They say that there are many parts of the interior. The major ones are

·               Crust        

·               Mantle

·               Outer Core

·               Inner core

 

Crust: The outer most layer of the earth is called the crust. At the ocean basins its thickness is up to 6 km or 4 miles and in the mountainous regions the thickness is up to 64 km or 40 miles. It is believed that when the earth cooled, the outer parts solidified like the skin of a fruit. There is still lava which is very hot and molten, under the crust. The crust is floating on this molten lava and is attached to it like the skin of an orange.

            The thickness of the crust varies from 2 to 4 miles or more. It consists of silicon and aluminum (si + al). Life of Humans and all sorts of agricultural activities are possible on it. As we move down the earth the temperature increases. There are pockets of lava. The lava erupts from these magma chambers from places where it finds holes or cracks to form volcanoes. Fig.4 shows different layers in the Interior of the earth

 

 

 

 


                                Crust

 

                                                                                                Mantle

                                                               inner

                           Outer                           core

                            core

 

 

 

 

 

 

 

Fig. 4                                       Inner Layers of The earth

 

 

Mountain Building and Ocean Building

            How were mountains and oceans formed? The crust of the earth is not smooth. There are oceans and high mountains on it. Similarly the thickness of the crust is not uniform everywhere. Under oceans it is about 6 km and near mountains up to 64 km thick. Scientists give some reasons how these deep and high mountains were formed.

  • When the gas and molten material cooled on the surface of the earth, they became uneven like a dried date.
  • There is a layer of silicon and magnesium (si + ma) under the crust, it is called mantle. This part is very hot. It is believed that it is like molten wax. Places where molten lava pushes the earth it raised the crust to become a mountain and in places where the lava sinks deeper, the crust became ocean.
  • The central part of the earth is called the core. It consists of iron and nickel (fe + ni). This part is very hot. After 9 years of research on earthquakes and waves, it has been recently proved that this part is rotating rapidly inside the earth.         
  • The crust of the earth is broken. It has cracks on it. There were 15 large continents in the past. These continents move slowly on molten lava. At some places they collided or moved away. At such places the molten lava shoots up from these cracks to form a volcanic eruption. This situation is in the Pacific Ocean. Constant volcanic activities go on in the Pacific. It appears that there is a wide fire ring round this ocean. At some places these continents collide and slide on one another. At such places high mountains are formed. The Himalayas of Asia, the Andes of South America and Rocky mountains of North America were formed in this way. This is another reason for the formation of mountains and oceans in the crust. The Himalayas, the Andes and Rocky mountains were formed by collision of continents.

 

Continents: Initially the crust of the earth was just one huge piece. Later it cracked and was broken into 15 pieces which scientists call continents. The Holy Quran refers to them as “Rawasi”. These continents are still in contact with one another. As described earlier, at places where they move apart, lava erupts and volcanic mountains form there. In Japan lava keeps erupting repeatedly, so there are many volcanoes there.

            At places these continents are moving away and at others they are sliding over each other. These continents carry the living beings on their backs. If they sink in molten mantle, everything on the surface of the earth will sink and the entire population of that continent will be exterminated. The Holy Quran has pointed towards this and has said:

 

وَأَلۡقَىٰ فِى ٱلۡأَرۡضِ رَوَٲسِىَ أَن تَمِيدَ بِڪُمۡ (١٥) { النّحل 16 }            

Translation: And He has set up on the Earth Mountains standing firm, lest it should shake with you;

 

Maybe near the Day of Judgment these pieces might separate from each other and the hot lava will come out. The Holy Quran refers to it as:

وَإِذَا ٱلۡبِحَارُ سُجِّرَتۡ (٦)  {التّکویر 81 }                 

Translation: When the oceans boil over with a swell; (6)

 

Movements of the Earth

Slow and sudden movements of the earth: The rotation of the earth is different from Movements of The earth. Rotation means the movement of the earth around its axis and movements means abrupt motion of the earth slowly or suddenly. If the earth moves suddenly, we call it earthquake. Earthquake is not only felt but it causes wide spread destructions. This is called sudden movement. Many changes are caused in the earth due to any type of movement. Scientists so far have not been able to explain the reasons of sudden movements of the earth. The reason has been told by the Creator of the Universe that when the people become astray various divine punishments fall on them.

            These movements cause mountain and ocean building. New fountains, new islands emerge, volcanoes erupt, and lands slides occur, thousands, sometimes millions of people lose their lives. An example is the recent earthquake in our country in which approximately 300,000 people of Balakot, Muzzafarabad etc. lost their lives.

 

Theory of continental drift

وَجَعَلۡنَا فِى ٱلۡأَرۡضِ رَوَٲسِىَ أَن تَمِيدَ بِهِمۡ (٣١) { الاٴنبیَاء 21 }         

Translation: And we have set on the Earth Mountains standing firm lest it should shake with them. (31)

 

            The continents which appear stationary on the surface of the earth are actually floating on molten lava in the interior of the earth. It has been proved that they move and change their positions. Allah (s.w.t.) almighty, referring to their motion has said that we have inserted mountains as pegs in the earth.

            Whenever the molten lava in the interior of the earth gets an outlet or crack, it erupts from it. This is volcanic activity. There is no definite opinion about the reasons of earthquakes. Prediction of the earthquakes is also impossible. No one can predict where and when an earthquake will occur and what will be its intensity. One opinion is that besides calcium carbonate, gas, molten lava, minerals and radioactive particles having high energy are there inside the earth. Perhaps their energy moves continents resulting in earthquakes. In fact it is due to our deeds


The Holy Qur'an says

إِنَّ ٱللَّهَ لَا يَظۡلِمُ ٱلنَّاسَ شَيۡـًٔ۬ا وَلَـٰكِنَّ ٱلنَّاسَ أَنفُسَہُمۡ يَظۡلِمُونَ   (٤٤)  {یُونس 10}       

Translation: Verily Allah will not deal unjustly with man in aught: it is man that wrongs his own soul. (44)                                

 

The crust of the earth is broken at many places. There are cracks between them forming large continents. The famous 7 continents are among them. These continents slowly move on molten lava. At places these continents move apart forming a gulf. High mountains emerge due to their collisions. Such mountains are called Newly Folded Mountains.

The Himalayas of Asia, Andes of South America and Rocky Mountains of North America were formed in this way. Two large continents moving in opposite directions collide and slide over one another forming high mountain ranges. The highest peak is in the Himalayas having a height of 8848 meters or 29028 feet above sea level. Frequent earthquakes occur near newly folded mountains.

The present scientists and geologists believe that when the earth was formed, all continents were joined together. There was a shallow ocean between them. It was called Tytheses Sea. Later due to movements of the earth these continents started floating and drifted apart.

Experts of Geomorphology cut the continents from the map of the world and made maps of ancient world by joining them to show where these continents were in remote past and what their shapes were in early history of the world. The following figure represents the world of that era. In the Holy Qur'an the Creator of the Universe has clearly stated that the earth was moving so we inserted pegs on it in the forms of mountains.

The continent that was on the north was called Angara Land and the one in the south was called Gondwana land.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Fig. 5 According to the Wegner’s theory of continental drift all the continents were joined in the (jig-saw fitting) form as shown in the figure above. Later on they were drifted apart. 

 

 

 

 

Data regarding major earthquakes..

 

Date                        Place                       No. of           Rector                Reason for

                                                                casualties     Scale   casualties.

 

May 30, 1935          Queta, Pakistan        30,000 to    7.5     Completely

                                                                60,000                  destroyed

Mar, 23, 1893          Ostan e Ardabi         150,000  

Sep 1, 1923             Kanto, Japan            143,000      7.9

Oct 5, 1948              Tuekmenistan          110,000      7.3

Dec 28, 1908           Messine, Italy          70,000 to    7.2

                                                                100,000

Sep  1290                Hebel, China            100,000

Nov 18, 1727          Tabriz, Iran              77,000

Nov. 1, 1755           Lisbon, Portugal      70,000        8.7        Great Tsunami

Dec. 25, 1932          Gansu, China           70,000        7.6

May, 31, 1970         Peru                         66,000        7.9        Rock slide, flood

 

1268                        Cillicia, Asia Minor  60,000

Jan 11, 1693            Sicily, Italy              60,000

June 20, 1990          Iran                          50,000        7.7        Land slides

Jan 23, 1556            Shaanxi, China         830,000      8.0

July 24, 1976           Tang Shan, China     255,000 to                  7.5

                                                                655,000

Aug. 9, 1138            Aleppo, Syria           230,000

May 22, 1927          Xining, China           200,000      7.9        Heavy fractures

Dec 22, 1856           Damghan, Iran         200,000  

Dec 20, 1920           Ganau, China           2000,000    8.6

Dec 26, 2004           Near Sumatra           153,000      9.0        Tsumani

 

May 22, 1960          Chile                                           9.5

Feb 1, 1938             Banda, Indonesia                        8.5

Aug 15, 1950           Tibet, Assam                              8.6

Oct 8, 2005              Punjab, NWFP         More than                    7.6       Earth quake

                                Pakistan                   3 million

                                                                NWFP 300,000

 

Balakot Bagh, Mansehra, Muzaffarabad and most parts of Azad Kashmir were completely destroyed

 

1.4       Latitudes and Longitudes

Latitude: Imaginary lines drawn on the surface of the earth are called latitudes and longitudes. Some are drawn from left to right and some from top to bottom in such a way that the globe is divided into squares. The lines that are from left to right i.e. horizontal lines are called latitudes. The lines from top to bottom are called longitudes. The figure below shows latitudes. The middle line which divides the world in two equal parts is called the equator.

Equator: This is the line of zero degree latitude. It divides the world into two equal parts. The upper part is called the northern hemisphere and the lower part the Southern hemisphere. Latitudes are measured from 0o to 90o North and from 0o to 90o South, thus there are 180 degrees of latitudes.LATITUDES                             Parallels               

Fig. 6 - Lines are parallel to each other from the Equator to the North and to the South Pole.

 

Width of latitudes: The distance from latitude to the next degree latitude is 69.05 miles or 111.13 km. The arc distance from one pole to the next and back is 24859.82 (approximately 25,000) miles or 40008 km. This circumference is 41.73 miles or 67.16 miles less than the equatorial circumference.

 

The Tropic of Cancer and the Tropic of Capricorn

            The parallel of latitude 23½o north is called tropic of Cancer and the one at 23½o South is called tropic of Capricorn. The sun travels between them all the year round. The sun rises daily from a different point due to its annual motion. Twice a year when the sun is exactly over equator, it rises exactly from the east. During a year the earth moves about 47o from the tropic of cancer to the tropic of Capricorn due to its motion round the sun. The angle 23.44o or roughly 23½o is called the tilt of the axis.

Longitude: A city or a place cannot be located by only knowing its latitude. There are many cities on the same latitude. We need to know the other line, from the north to the south. These lines from top to bottom like lines on a melon are called longitudes. The central line is taken as 0o longitude. It divides the globe in two parts, Eastern hemisphere and The Western hemisphere. The line of 0o longitude is called Greenwich meridian or central meridian. Greenwich is the name of a locality in London where the Royal Observatory is located. In 1844 the line through Greenwich was taken as 0o longitude. Longitudes are shown in the figure below. Longitudes are measured from 0o to 180o east and from 0o to 180o west. The total longitudes are 360o. The line where 180p east and 180o west coincide is called International Date Line. The date changes across this line. If there is Thursday on one side of this line, it will be Friday on the other.

 

                            Meridians         

Fig .7 - Meridians or The Longitudes Central meridian is called Greenwich

 

Width of longitudes: The distance from one degree of longitude to the next is different at different latitudes. Maximum distance at equator is 69.17 miles or 111.31 km. The total length of 360o of longitude at equator is 24,901.55 miles or 40,075.16 km. As we move north or south, the distance from one longitude to the next decreases.

The distances between two longitudes at different latitudes is given in the following table.

Distance between two longitudes at different latitudes

 

Latitude

Width

In miles

Width

In km.

Circumference

in miles

Circumference.

in km.

90

0.00

0.00

0.00

0.00

80

7.68

12.36

2766.83

4452.79

70

15.37

24.74

5533.68

8905.59

60

23.50

37.10

8300.52

13358.39

50

30.74

49.47

11067.36

17811.18

40

38.42

61.84

13834.19

22263.98

30

46.11

74.20

16601.03

26716.77

20

53.79

86.57

19367.87

31169.57

10

61.48

98.94

22134.71

35622.36

0

69.17

111.31

24901.55

40075.16

 

1.5       Coordinate System and Their Explanation

            It is easy to find the positions of any place with the help of latitude and longitude. For example, if we want to find the position of Karachi, we see from the map that Karachi is on longitude 67o east of Greenwich and at a latitude of 25o north. Its location will be described as “Karachi lies on longitude 67o east and latitude 25o north.” Similarly the location of any place can be found. This system is called spherical coordinate system.

 

Zone: The region of the earth between two longitudes is called a zone.

 

Gore: The region between two latitudes is called a gore.

 

Graticule: The square region between two latitudes and two longitudes is called a graticule.

 

                            latitude_longitude

Fig.8 – Positions on the globe

 

Greenwich: As described earlier, Greenwich is the central longitude. It is called central meridian. The time of all places in the world is fixed with reference to Greenwich Time. For countries lying to the east of Greenwich, the time is ahead of Greenwich Time and in places lying west of Greenwich the time is behind Greenwich Time.

Note: Since the times of Arabs till 1844, i.e. for centuries, the 0o longitude passed through Khaldaat Islands now called Canary Islands. Some details are given below.

 

Present Greenwich and ancient Khaldaat Islands

            The contributions of Arab Muslim astronomers, mathematicians and experts in geography are known even today all over the world. The formulae of mathematics and astronomy derived by them are still in use and are found to be accurate. They believed that Khaldarat Islands, now known as Canary Islands, was the west corner (the last corner) of the earth. Al Beruni drew latitudes and longitudes regarding it as 0o longitude. Al Idreesi also regarded it as 0o longitude. In 1844 there was a chaos in Europe. Every country regarded itself superior to others. The head of every country had started declaring the longitude of their capitol as 0o longitude. There was no standard left. In such chaotic conditions a conference was held in 1844 in Washington. After lengthy discussions, it was declared that 00 longitude which was taken by Al Beruni and Al Idreesi as longitude of Canary Islands would be shifted to the locality of Greenwich in London where the Royal Meteorological Observatory was located. It was declared as 0o longitude. Thus the 0o longitude we use today which divides the world into the east and the west hemispheres was decided in the conference in1844 in Washington. Before this declaration no one had even heard about Greenwich.

There is a difference of 26o in longitudes of Al Beruni and Al Idreesi and the present longitudes i.e. longitude of Khaldaat Islands is further 26o west of Greenwich. If some one uses old maps, he will find a difference of 26o in longitudes of old and new maps.

The Westerners have been trying to exterminate all signs of Muslims; accordingly they shifted the place 0o longitude to their own city. (Reference: Research book “Al Beruni wa Jugrafia e Alam wa Qanoon e Massodi” by Maulana Abul Kalam Azad)

International Date Line

            We have learnt that longitudinal lines are from top to bottom like the lines on a water melon. The central line is 0o longitude. It divides the world in the eastern and the western hemispheres. Longitudes are measured from 0o to 180o east and 0o to 180o west. 0o longitude is called Greenwich longitude or central meridian.

            The line where 180o east and 180o west merge is called International Date Line. A new day begins here and date changes. If there is Thursday on one side, there will be Friday on the other. Just think that a new day must begin somewhere on the globe. On the globe of the world if Greenwich meridian is in front, then the International Date Line will be at its back.

Date Line International            This line passes through the Pacific Ocean near Fiji Islands This line is bent at places so that it may not divide and pass through any country. It is now a common experience that travelers traveling east from Hong Kong, Japan etc to North America set one day back on crossing this line. When traveling from the east to the west set one day forward i.e. while traveling east Friday will become Thursday on crossing this line. When traveling to the west Friday will become Saturday as soon as the International Date Line is crossed.

 

Fig. 9   The International Date Line.

 

Changes in lengths of day and night

 

أَلَمۡ تَرَ أَنَّ ٱللَّهَ يُولِجُ ٱلَّيۡلَ فِى ٱلنَّهَارِ وَيُولِجُ ٱلنَّهَارَ فِى ٱلَّيۡلِ

Translation: Seest thou not that Allah merges Night into Day and He merges Day into Night. (29)

 

 خَلَقَ ٱلسَّمَـٰوَٲتِ وَٱلۡأَرۡضَ بِٱلۡحَقِّ‌ۖ يُكَوِّرُ ٱلَّيۡلَ عَلَى ٱلنَّہَارِ وَيُكَوِّرُ ٱلنَّهَار   

َ عَلَى ٱلَّيۡلِ‌ۖ  (٥)  {الزُّمَر 39}                                                   

Translation: He created the heavens and the earth in true (proportions): He makes the Night overlap the Day, and the Day overlap the Night. (5)

 

Our observation is that sometimes days are long and sometimes night. But on the equator day and night are almost equal all year round. There is hardly a difference of an hour or half an hour in several months. North and south of the equator, up to the tropics of Cancer and Capricorn, the difference gradually increases and decreases. But from 48.5o north to the North Pole and from 48.5o south to the South Pole there is considerable difference between the lengths of day and night. These regions are called abnormal regions. In these regions, in summer days are very long and nights are very short. In the winter season days are very short and night are very long. Near poles, the sun does not rise for months in winter and it is perpetual night. In summer the sun does not set for months and it is perpetual day there. At poles days and nights are of six months durations.

وَهُوَ ٱلَّذِى خَلَقَ ٱلَّيۡلَ وَٱلنَّہَارَ وَٱلشَّمۡسَ  وَٱلۡقَمَرَ‌ۖ كُلٌّ۬ فِى فَلَكٍ۬ يَسۡبَحُونَ (٣٣) 

 {الاٴنبیَاء 21}                                                                       

Translation: It is He Who created the Night and the Day, and the sun and the moon: all (the celestial bodies) swim along each in its rounded course. (33)

 

 

 

                              Winter Solstice

Fig. 10   Duration of day and night – and winter solstice

 

 

لَا ٱلشَّمۡسُ يَنۢبَغِى لَهَآ أَن تُدۡرِكَ ٱلۡقَمَرَ وَلَا ٱلَّيۡلُ سَابِقُ ٱلنَّہَارِ‌ۚ وَكُلٌّ۬ فِى فَلَكٍ۬

يَسۡبَحُونَ (٤٠)  {یسٓ 36}                                                  

 

Translation: It is not permitted to the Sun to catch up the Moon, nor can the Night outstrip the Day: each (just) swims along in (its own) orbit (according to Law). (40)

Horizontal Coordinate System: The coordinate system in which the position of a heavenly body is located by height above horizon or depth below horizon is called Horizontal Coordinate System.

 

1.6       Some Terms and Their Explanations

Time of Transit: When the sun is at the highest point in the sky (on the observer’s meridian), it is called Time of Transit. The shadow of every body is the least in length at this time. This shadow is called real shadow.

Diurnal Circle: The path in which the sun appears to move daily due to the earth’s rotation is called diurnal circle. Its part on which the sun moves from rising till setting is called the day arc and the remaining part (below the horizon) on which the sun travels at night after setting till rising is called the night arc.

            The parts of the earth from 48.5o north to the North Pole and from 48.5o south to the South Pole are called abnormal regions by astronomers. In these regions day arc and night arcs are not equal but there is a large difference between their lengths.

Horizon: By standing in an open ground, you will see a large circle where the sky and the earth seem to meet. This is called the “horizon”. Observations show that the disc of the sun takes about 3 minutes to cross the horizon at the time of sunset and sunrise.

Zenith: The point on the sky directly over our head is called zenith. It is at an angular distance of 90o from the horizon.

Nadir: The point on the sky directly below our feet is called Nadir. It is diametrically opposite zenith.

Angle of Altitude: The angle a heavenly body makes above the horizon towards zenith is called “angle of altitude” or simply the “altitude of the body”. The angle between zenith and the body is called the “zenith distance” of the body.

Angle of depression: The angle of a body below the horizon is called its angle of depression.

            With the help of altitude and angle of depression we get an idea about the position of the body (star). If the altitude of a body is 30o we know that it will be 30o above horizon. If the depression of the sun is 18o we know that it is 18o below horizon. But by this information alone we cannot locate the exact position of the body. By altitude we know the height of the body above the horizon but we do not know in which direction to look for it. Thus we need direction also. There are four basic directions reckoned from the north. The north direction is taken as a basis. If a body is exactly toward the north we say that its direction is 0o, if towards the south its direction is 180o, the direction of the east is 90o and that of the west is 2700.   

 

Coordinate System

            To fix the position of a body (any star) on the sky we need to know its altitude and its direction i.e. it is necessary to know its angle from the north. For example if the direction of a star is 230o from the north and its altitude is 50o, its coordinates will be described as “such and such star is 230o east of the north and has an altitude of 50o”. If a star is below the horizon, it will be represented by its angle of depression.

Great Circle: If we draw a straight line touching the globe it at one point it is called a tangent. We cannot draw a straight line on a sphere using a scale. If we want to join two points on a globe, we have to use a string or a piece of thread. Put the ends of the strings or threads at the points and taut the string. The arc formed is part of a circle called “a great circle”. A great circle arc is the least distance between two points on a sphere. All ships travel on great circles because it is the minimum distance between two points.

            If we draw a circle on a sphere a radius equal to the radius of the sphere, it will divide the sphere in two equal parts. Such circles are called great circles. All lines of longitude on the globe of the earth are great circles. The equator is also a great circle but other parallel of latitudes are not because they do not divide the sphere in two equal parts. They are called small circles.

 

Figure from page 49.

 

 

 

Fig.11

Declination of the Sun

The celestial latitude of the sun is called its declination. On 21st March and 21st September the sun is on the equator, so its declination on these days is zero degree.

            On 21st June the sun is on the Tropic of Cancer so its declination is + 23.5o north. On 21st September the sun is on the Tropic of Capricorn so its declination is    – 23.5o south.

 

Zones On the basis of Temperature

According to weather conditions the earth is divided in five zones.

  • Torrid Zone (Very hot region): This is between the Tropics of Cancer and the Tropic of Capricorn. It is called “Tropical Belt”.
  • The North Temperature Zone: From the tropic of Cancer to 66.5o North.
  • The South Temperature Zone: From the tropic of Capricorn to 66.5o South.
  • Arctic Zone (very cold and frozen region): From 66.5o N to the North Pole.
  • Antarctic Zone (very cold and frozen region): From 66.5o S to the South Pole.

 

Normal and abnormal regions

Normal regions: The parts of the earth from the equator to 45.5o north and 45.5o south are called normal regions by astronomers. In this region the sun rises and sets and white and red twilights also rise and set all the year round.

Abnormal regions: The parts of the earth from 45.5o north to the North Pole and from 45.5o south to the South Pole are called abnormal regions. The conditions in these areas are different from other areas. In winter the sun rises and sets, twilight begins and ends but in summer, near the Arctic and Antarctic circles, the sun does not rise or set and twilight does not begin and end every day.

            Twice a year the sun crosses the equator. In these days the sun rises exactly in the east and sets in the west. On these days all over the world, day and night are equal. The day is about 12 hours long and so is the night. These days are 21st March and 21st September.

 

1.7       Solar and Lunar Eclipses

Solar Eclipse: If some thing comes in between our eye and the object which we want to see, the object will be totally or partially hidden from us. The same situation happens at solar eclipse. When the moon comes in between the earth and the sun, the sun is partially or totally hidden. The moon blocks the light of the sun, so the sun is not visible. This is called solar eclipse.

Remember that the paths of the sun and the moon are different. If they were not different, the moon would not have been visible to us during the day along with the sun. You may have observed that sometimes the moon is visible during day although they are both traveling in their separate orbits. The sun appears to move round the earth. The path in which it moves is called ecliptic. The moon is also revolving round the earth. Its orbit is towards the north south of the ecliptic. The orbit of the moon intersects the orbit of the sun in two points which are called Nodes. The point where the moon crosses the ecliptic moving towards the north is called the Ascending Node and the point where it crosses the ecliptic while traveling south is called the Descending Node.

            Whenever the sun, the moon and the earth come in a straight line, with the moon at the middle and near a node, the moon will block the light of the sun causing a solar eclipse. If the moon covers the entire disc of the sun, it is called total solar eclipse, and if a part of the solar eclipse is covered, it is called partial solar eclipse. There is another type of solar eclipse in which the central part of the sun is covered by the moon and edges of the sun are visible as a bright ring. It is called annular solar eclipse.

At the time of the new moon (conjunction), the sun, the moon and the earth are in a straight line with the moon between the earth and the sun. The shadow of the moon falls on the earth causing a solar eclipse in that area.

Conjunctions occur once in every lunar month. Naturally a question arises that why don’t we have a total solar eclipse in every new moon? Why eclipses are there only 2 or 3 times in a year? The answer is that there are two conditions for solar eclipse to take place:

 

  • The sun, the moon and the earth come in a straight line in such a way that the shadow of the moon falls on the earth. If the shadow of the moon does not fall on the earth but passes beyond the earth’s edge, then there will be no eclipse.

 

  • The shadow narrows down as the distance increases. So the moon should be near enough to the earth so that its shadow reaches the earth. If the shadow ends before it reaches the earth, then in that part annular eclipse will take place.

 

 

Fig. 12 – Total and Annular eclipse

                                                                Total Solar Eclipse

 

                         Sun                            Moon                                       Earth

 

 

                                                                Partial Solar eclipse

 

 

 


                         Sun                   Moon                                                    Earth

 

 

                                                                Annular solar eclipse

 

Lunar Eclipse: When the earth comes in between the sun and the moon, we get a lunar eclipse. It does not take place every month. It can take place only when the moon is near one of its nodes at the time when the earth comes between it and the sun. The moon enters the shadow of the earth; the sunlight cannot reach that part of the moon. This is called lunar eclipse. If part of the moon enters the earth’s shadow and the remaining part is outside, we get a partial lunar eclipse; if the entire moon enters the shadow a total lunar eclipse takes place. Lunar eclipse can only take place on 13th or 14th of a lunar month because in these days the earth is between the sun and the moon. But lunar eclipse cannot take place at every full moon. It occurs only when at full moon; it is near one of its nodes.

At the time of full moon the earth suddenly slides in between it and the sun blocking the light of the sun from falling on the moon. The shadow of the earth falls on the moon and its brightness disappears. This falling of the earth’s shadow on the moon is the lunar eclipse.

There are two conditions for lunar eclipse (same as for solar eclipse).

 

i. The shadow of the earth reaches the moon.

ii. The sun, the moon and the earth come in line in such a way that shadow of the earth falls on the moon, and it does not escape from its edge. If the earth’s shadow escapes the moon and falls beyond its edge there will be no eclipse.

            Since the earth is much bigger than the moon, its shadow is much longer than the moon’s shadow. So the earth’s shadow always reaches the moon. From any given place more lunar eclipses are visible than solar eclipses.

 

Fig.13 – Partial solar eclipse

 

                                                                                No eclipse

 

 

                                                        Partial Lunar Eclipse

                                                                                                     Moon

 

                Sun                                                     Earth                  Moon

 

 

                                                                Total Lunar eclipse

 

                                                                   Moon’s Orbit

 

 

 

Tides:  Due to attractions of the sun and the moon, the level of sea water increases. This is called high tide. When the level falls it is called low tide. This rising and falling of sea water level twice a day is called tides. Both the sun and the moon have gravitational pulls. They exert attractive force on that part of the earth over which they pass. The dry part of the earth is solid and is not affected by the pull. Since water is fluid, the gravitational pull has an appreciable affect on it.

            Due to its large distance from the earth, the sun’s gravitation has very little effect even on water. The moon is much nearer the earth than the sun, so its gravity has more effect on water. The water rises several feet in the place over which the moon passes. This is called “high tide”. When the moon moves away, the water level falls causing low tide. Since the moon reaches the same place 48.76 minutes late every day, the high tides also occur 48.76 minutes late every day. There is another high tide at a place diametrically opposite to the place over which the moon is passing. The reason is that when the water is pulled under the moon, due to the reaction of the earth, the water is pushed up on the other side.

Spring Tides: At the time of new moon and full moon, the earth, the moon and the sun are in the same straight line. The gravitational pulls of the sun and the moon add up to cause high tides higher than normal. Such high tides are called spring tides. At spring tides water level rises by 6 to 8 feet.

Neap tides: On 7th and 21st of a lunar month, the lines joining the sun to the earth and the moon to the earth are perpendicular to one another. Their gravitational pulls are subtracted. The high tides on these days are lower than normal high tides. These are called neap tides.

 

Physical Data about the earth

 

Equatorial radius                                 = 6.378 km.

Equatorial Inclination                        = 23.5o.

Mass                                                      = 5.97 x 1024 kg.

Average density                                   = 5.5 gm/cm3.

Rotational period                                = 0.997 day.

Orbital period                                       = 365.2422 days.

Average distance from the sun         = 149.6 million km.

Perihelion                     do                    = 147.1 million km.

Aphelion                       do                   = 152.1 million km.

Orbital eccentricity                              = 0.0167o.

Inclination                                            = 0.0003o.

 

 

 

 

 


 

CHAPTER 2

 

2.1 Directions

            We know from child hood that the direction from which the Sun rises is called The East and where it sets is called The West. Precise concept of directions is necessary to recognize stars, planets and other heavenly bodies.

The concept of determining directions with the help of the Pole star has been known since ancient times. The direction of the Pole star is the standard direction of the north. The other three directions the east, the west and the South are fixed with reference to the north. Later magnetic compass was used to determine the directions. The property of a magnetic needle to point north south is used. Since then the concept of directions has made rapid progress.

For more exactness in directions, four more directions were inserted between the standard directions. They were South East, South West, North East and North West. Later more subdivisions like North North East, South South West etc. were introduced.

Later more points representing directions were introduced. The complete circle representing directions was divided in 360 degrees. Zero degree coincides with the north. Moving clockwise (towards right) the east is at 90 degrees, South at 180o, and the west at 270o. In Arabic this system of measuring directions in terms of angles is called ‘Assimt’. The English word azimuth is derived from it. The As-simt or azimuth of the Pole star is 0o. It remains zero all the time whereas the azimuth of all other stars, planets, the Moon, the Sun and all other heavenly bodies continuously keep changing with time.

To fix the position of a point in the sky, we need to know its azimuth and height above the horizon. To determine the azimuth we face the North Star and turn right till we face the required star. The angle we turn around is the azimuth of the star.

 

Cardinal Points or Directions

It is very easy to determine directions. There are several methods for it. For students of geography it is necessary to know the following facts to understand a map and to determine the direction of Qibla.

When early Muslims traveled to spread Islam, they needed to know the direction of Qibla to offer prayers. They prepared accurate maps of the world and introduced the concepts of latitude and longitude. Today entire world has been benefiting from their research.

 

Basic Directions (Cardinal Points)

There are four basic directions, the east, the west, the north and the south. If a person faces the setting sun, the west is in his front, the east is behind him, the north is towards his right and the south towards his left. In maps the north is upwards, the east to the right, the west to the left and the south downwards.                        

 

                                                                 NORTH 360 º

 

 


                           WEST 270 º                                              EAST 90 º

 

                                            

                                            

                                                                 SOUTH 180 º

 

The Geographic North

The children play with the top which rotates around the nail. This is called the axis of the top. Similarly the earth is rotating around its axis. The upper end of the axis is called the North Pole and the lower end the South Pole. Both are called the poles of the earth. The Geographic north of a place is the direction of the North Pole from that place. The lines passing through a place and the poles is called the MERIDIAN of that place.

The Magnetic North

The direction indicated by the north end of the needle of a magnetic compass is called its magnetic north. The other end of the needle points towards the south which is called the magnetic south.

The True North

The north determined by the pole star is called the true north. It is the same as the geographic north. The north on a map determined by longitudinal lines is called the True North.

The Grid North

Note that the true north and the magnetic north are not the same. The Magnetic north is in the north of the Hudson Bay whereas the geographic north lies in Bothia Land. Only on the line joining South Carolina and Lake Superior, called the agonic line where the true and the magnetic north coincide. On either side of the agonic line there is an angular difference between the true and the magnetic north. In the east of this line, the magnetic north is west of the true north and in the west of it somewhat to the east.

Magnetic Declination

The angular difference between the true and the magnetic north is called the magnetic declination. It is different for different places and it varies slightly every year. It can be calculated with the known annual rate of change.

 


2.2       Determination of Directions

Following are some methods of determining the north:

·         With the help of the pole star.

·         With the help of magnetic compass.

·         With the help of the Sun.

·         With the help of a clock.

·         With the help of altitude of the Sun.

·         With the help of longitudes in maps.

The directions of the north obtained by different methods are not always the same. There are two types of north; the true north determined by the pole star (the grid north found by longitudes) and the magnetic north determined with the help of a compass.

 

Fig. 14

                                                True

                                                North

                                Grid                         Magnetic      

                               North                        North

 

 

                                                                

 

 

 

1.         Pole Star

            Determination of the geographic north with the help of pole star is very simple. In clear weather a constellation of seven stars, called Great Bear or Plough, is visible in the sky towards the north in the northern hemisphere. Five of the stars form an arc. Other two stars are called the pointers. If we extend the line joining the pointers, we observe a bright star which is the Pole Star. The direction towards the pole star is the true north.

 

 

 


                    Pointers

 

 

 

 

 

 

 

 

 

Pole Star

                                                Great Bear

 

 

Pole star: Pole star occupies a central position for the earth. Direction of the north and direction of Qibla are determined with its help. This star is at a distance of 1085 light years from the earth and its declination (the angular distance from the celestial equator) is always 90o.

About 5000 years ago the North Star was star Thuban in the constellation of Draco. About 12000 years from now the bright star Vega in the constellation of Lyra will be the North Star. 26000 years from now again the present pole star in Great Bear will be the North Star. The reason of this change is that the axis of the earth is not fixed but rotates and completes one complete revolution in 26000 years. To sum up, the north end of the axis of the earth points towards a star which is the North Star. These days the North Star is the pole star in the constellation known as the Great Bear.

 

The Great Bear: It is a constellation of seven stars which rotates anticlockwise once every day round the North Pole. If we observe it at different times at night it will sometimes appear to the left, sometimes to the right, sometimes up and below the pole star but its distance from the pole does not change.

It is not difficult to identify it at night. With the help of its two pointer stars, the pole star can be located easily. Since ancient times, navigators used it, as a guide during their journey. Pole star itself moves within a small circle but it is always very close to the centre of the circle. Its motion can be neglected and can be taken as the north.

On the opposite side of the Great Bear with respect to the pole there is another constellation of five stars called Cassiopeia. Joining the stars in order we get two angles. The bisector of the smaller angle points towards the pole star, as shown in the figure below.

 

 

                                                                   Polestar

 

 

 

 

 

 

 

 


                                    Cassiopeia

 

 

2.         The Sun

            Twice a year the Sun rises exactly at the east and sets exactly at the west. If we observe the points of rising and setting on 21st March and on 22nd or 23rd September, we can determine the exact directions of the east and the west. The true north can then be determined.

 

 

3.         Shadow

Direction can be easily determined with the help of a shadow. Draw a circle on level ground. At the centre of the circle fix a rod vertically. When the shadow of the rod reaches the circle, before noon, mark the point. After the mid day, when the shadow again reaches the circle, mark the second point. Join these points to the centre of the circle. The bisector of the angle thus formed is the direction of South. The advantage of this method is that we do not have to consider the local time. The disadvantage of this method is that the north determined does not coincide exactly with the geographical north. The reason is that the sun does not rise exactly at the east nor sets exactly at the west everyday. Another disadvantage is that it cannot be used in cloudy weather.

                                         Rod

 

                                 Shadow

       Before noon

 

       Bisector                                                                North

 

         Shadow

         After noon

 

 

4.         Clock

  • In the northern hemisphere: Synchronize the clock with local time and put it horizontally such that its hour needle points towards the sun. The bisector of the angle formed by the line joining 12 to the centre and the hour needle towards the sun points towards the south. The other direction of the bisector represents the north.
  • In the southern hemisphere set the 12 of the clock towards the sun. The bisector of the angle formed by the line joining 12 to the centre and the hour needle points towards the north. The disadvantage of this method is that it can be used only in day time and in clear weather.

 

 

 

Picture page 67 top

 

 

 

5.         Magnetic Compass

            Magnetic compass is a well known instrument. Its needle points towards the magnetic north and south. The needle remains parallel to the magnetic poles of the earth. Only the magnetic north can be determined with its help. To find the geographic north we need to know the magnetic declination of the place. If magnetic declination is known, the geographic north can be obtained as explained below:

Example: If the magnetic declination of a place is 4.8o west, find the magnetic north and draw a line 4.8o west. It represents the geographic north.

If the magnetic declination is west, then the geographic north is west of the magnetic north and if the declination is east the geographic north is east of the magnetic north.

The method of determining the north with the magnetic compass has been in use since ancient times. This is the easiest and the best method because it can be used at all times and in all types of weather. Here are two disadvantages. Firstly it does not give the geographic north directly and secondly the geographic north cannot be found if magnetic declination is not known.

 

 

 

 

 

 

 

 

Picture page 68

 

 

Method of finding the sun’s altitude

            If we fix a bamboo vertically on the ground, it will cast a shadow on the earth. If we draw a line from the end of the shadow towards the sun, the angle of this line with the shadow represents the altitude of the sun.

 

 

                                                               A

 

                                                                Bamboo

 

 

                                                              Altitude

                                              C                                                       B

            Shadow       

 

For example AB is the bamboo with the end B on the ground, BC is the shadow, then the angle ACB is the altitude of the sun.

 

To find the latitude of any place: If we subtract the altitude of the sun on March 21 or September 23 from the 90o we get the latitude of the place.

 

2.3       Behavior of the Holy Prophet (P.B.U.H) and Sahabah towards Qibla

i.          It is well known fact that the first Masjid (mosque) constructed after Baitullah is the Masjid-e- Quba. (Quba is the name of a famous place near Madinah) This mosque was founded when the Qibla of the Muslims was Baitul Maqdas. When the verse about the change of Qibla was revealed, a Sahabah reached the mosque at a time when a prayer was being offered. On hearing this news, the Prayer Leader (Emam) and all the worshippers turned towards the Baitullah. This event is quoted in books of Tafseer and Ahadith. When the Holy Prophet (P.B.U.H) was informed of this He (P.B.U.H) approved it.

Evidently the direction adopted by the worshippers, in the past during prayer was not determined by astronomical instruments. Nor, perhaps, was any magnetic compass or star used. The direction was adopted by intuition (Tahharee). Even after the prayer no mathematical calculations or other methods were used to determine the direction of Qibla.

 

ii.         Hazrat Umer Farooq during his tenure of caliphate instructed all provincial heads of Islamic States to construct mosques in each locality. Heads of states obeyed the orders but neither Hazrat Umar nor the personnel of the government used any instrument or mathematical calculations. The direction of Qibla was determined by intuition.

 

iii.        There is a difference of opinion in Muslim scholars about the direction of Qibla determined by instruments and calculations. The reason is that even a small error in determination of latitude and longitude may result in a considerable error in the direction of Qibla.

            Scholars agree that the directions of most of the Masajid – (mosques) in the world were determined by calculations but, it is said, the direction of Qibla of Masjid e Nabvi was set by Revelation (Wahi). Therefore the direction of Masjide Nabvi is most exact without any doubt.


Sun-Shadow Method to Determine the Qibla Direction

For the benefit of Muslim brothers and to facilitate all those who are interested to find out most accurate Qibla direction in any country of the world, consult the Tables given in the appendix. Table No.1 is for Pakistan with the following explanation

For other countries of the world please see the attached Table 2 for 28th May and Table 3 for 16th July respectively.

 

·         It is very astonishing to note that every year, according to the astronomical calculations, the sun reaches exactly at the top of Haram Sharif (centre of  Baitulah Sharif) particularly on the 28th May at 18 past 2 according to Pakistan Standard time  (It is the time of  (ZAWAL) Nisfun-Nahar  at Mecca Mukarramah  (known as  Midday). 

·         It is the time when one can find out the QIBLA DIRECTION in any part of Pakistan by adopting the following method.

·         On this particular date and time that is on 28th May at 18 past 2 P.M. erect a pole or a mast or any straight stick in an open place, ground or in the courtyard.

·         Exactly at 18 past 2 p.m.  mark the shadow of the pole on the ground

·         And this line of shadow (shadow of the pole) will show you the exact QIBLA DIRECTION

·         Please remember, on the line of shadow - The Qibla direction will be towards the pole.

·         If you failed to mark this shadow on the 28th May, you can mark the shadow on the next date that is on 29th May. as the difference will be negligible.

In order to facilitate Muslim Ummah it is requested that its copies may kindly be forwarded to the daily “NEWS PAPERS” and to the MEDIA and Journals for maximum circulation.

2.4                Time and Calendars

هُوَ ٱلَّذِى جَعَلَ ٱلشَّمۡسَ ضِيَآءً۬ وَٱلۡقَمَرَ نُورً۬ا وَقَدَّرَهُ ۥ مَنَازِلَ لِتَعۡلَمُواْ عَدَدَ    

 ٱلسِّنِينَ وَٱلۡحِسَابَ‌ۚ مَا خَلَقَ ٱللَّهُ ذَٲلِكَ إِلَّا بِٱلۡحَقِّ‌ۚ يُفَصِّلُ ٱلۡأَيَـٰتِ لِقَوۡمٍ۬ يَعۡلَمُونَ (٥)  {یُونس10}

Translation: It is He who made the sun to be a shining glory and the moon to be a light (of beauty), and measured out stages for it: that ye might know the number of years and the count (of time). No wise did Allah create this but in truth and righteousness. (Thus) doth He explain His Signs in detail, for those who understand? (5)

 

The system with which we keep track of time is called calendar. With its help we keep track of days, weeks, months and years.

       

وَجَعَلۡنَا ٱلَّيۡلَ وَٱلنَّہَارَ ءَايَتَيۡنِ‌ۖ فَمَحَوۡنَآ ءَايَةَ ٱلَّيۡلِ وَجَعَلۡنَآ ءَايَةَ ٱلنَّہَارِ مُبۡصِرَةً۬ لِّتَبۡتَغُواْ فَضۡلاً۬ مِّن رَّبِّكُمۡ وَلِتَعۡلَمُواْ عَدَدَ ٱلسِّنِينَ وَٱلۡحِسَابَ‌ۚ وَڪُلَّ شَىۡءٍ۬ فَصَّلۡنَـٰهُ تَفۡصِيلاً۬ (١٢)  {بنیٓ اسرآئیل / الإسرَاء 17 }                           

Translation: the Night and the Day as two (of Our) Signs: the Sign of the Night have We obscured, while the Sign of the day We have made to enlighten you; that ye may seek bounty from your Lord, and that ye may know the number and count of the years: all things have We explained in detail. (12).

 

We use a clock to keep track of hours, days and nights. Day and night is one unit. The earth is rotating around its axis causing days and nights to follow each other. The earth makes one complete rotation around it’s axis in 24 hours. This is called a solar day.

The earth makes one complete revolution around the sun in about 365 days. Due to the difference in times of transit of the sun, all days are not of equal lengths. Seasons change and repeat after completion of one revolution. This larger period of 365 days is called a year.

            Generally, in normal regions within Tropics, the length of a day and a night is 24 hours. Accurate measurements show that:

  • On 1st January a solar day is 24 hours and 29 seconds in length.
  • On 1st April 23 hours 59 minutes and 42 seconds.
  • On 1st July 24 hours 12 seconds and
    On 1st October 23 hours 59 minutes and 41 seconds in length.

Thus the length of a solar day varies. The change is sometimes positive and sometimes negative. Thus the time of transit of the sun on 1st February is 12 hours 13 minutes and 32 seconds local time and on 1st November it is 11 hours 44 min and 20 sec. Four times a year the sun transits exactly at 12 O’clock, the local noon.

Mean solar day: When we talk about 24 hours, we have a certain period in mind. What is one hour? The average length of a day for the entire year is taken as 24 hours, called mean solar day. Every hour has 60 minutes and a minute has 60 seconds. Thus there are 86400 seconds in a mean solar day. A mean solar day begins at 12 O’clock midnight. The time of transit is thus 12 O’clock noon but except 4 days in a year it never takes place at exactly 12 O’clock. The difference is called the equation of time. It may be positive or negative.

            In every day life we follow the time reckoned with the sun. The time can also be reckoned with the help of the moon as it varies from a crescent to full moon and back to crescent. As Allah (s.w.t). Has said:

 

وَٱلۡقَمَرَ قَدَّرۡنَـٰهُ مَنَازِلَ حَتَّىٰ عَادَ كَٱلۡعُرۡجُونِ ٱلۡقَدِيمِ (٣٩)  {یسٓ 36}

 

Translation:  We have measured for it mansions (to traverse) till it returns like the old (and withered) lower part of date-stalk. (39)

           

The moon takes the form of crescent 12 times in a year. So a year is divided in 12 months. It stated the concept of month and year. Following this lead a solar year is also divided in 12 months. Reckoning time with the sun and the moon is mentioned in the Holy Quran. In Surah Kahaf Allah (s.w.t). Says:

 

وَلَبِثُواْ فِى كَهۡفِهِمۡ ثَلَـٰثَ مِاْئَةٍ۬ سِنِينَ وَٱزۡدَادُواْ تِسۡعً۬ا (٢٥) {الکهف  18}

Translation: d in their Cave three hundred years, and (some) add nine (more). (25)

 

It indicates that 300 solar years are equal to 309 lunar years. Islam is a natural religion (deen e fitrat). It follows the lunar calendar so that Muslims have no problem. There is vividly clear reason and wisdom behind it. Fasting and Hajj are easier in lunar time. If a person fasts for 33 years of his life time then he has fasted on every single day of the year. It is the greatness of Allah (s.w.t). Who has blessed his followers?

 

Day: Astronomers call a day and a night i.e. 24 hours a day. There are three types of days: Sidereal day, apparent day and mean day.

 

1.         Sidereal day: It is used for observation of stars. The earth has two types of motions.

·                     Annual motion in which it makes one complete revolution around the sun in one year which causes changes in seasons.

·                      Rotation about its axis in 24 hours. Day and night change due to this motion.

Due to these motions, the earth rotating on its axis also moves forward every day. As a result, if a star is visible today at a place, the next day it will appear at the same place after 23 hours and 56 minutes. This is called a sidereal day. After 24 hours it will appear one degree to the west.

Accordingly if a constellation is visible overhead today, after three months it will have moved 6 hours to the west and will be visible on the western horizon as a setting constellation.

Part of the earth facing the sun faces it again after 24 hours. But stars return to their position after 23 hours and 56 minutes. So their time is different from our time. There are clocks which complete one day in 23 hours 56 minutes. Their speed is slower than the speed of our clocks. Such clocks are called Sidereal clocks and are used in navigation and in astronomical observatories.

Technically the interval between two consecutive transits of a fixed star across a meridian is a sidereal day. It is the time in which the earth makes one complete rotation around its axis. It is 3 minutes 56 seconds shorter than our usual day. The clocks which keep the sidereal time complete a day in 23 hours and 56 minutes and 4 seconds, are called star chronometers. They are used in astronomical calculations. Nowadays sensitive electronic and computerized clocks are used.

 

2.         Apparent day or apparent solar day: The interval between two consecutive transits of the sun across a meridian is called “apparent day” or “apparent solar day”. If the earth were not revolving round the sun, the apparent day and sidereal day would be equal. But the earth is moving round the sun from the west to the east in an elliptic orbit called the ecliptic. It completes one revolution in 365 days 5 hours and 46 minutes. Due to it the earth moves 0.835 degree towards the east each day. Thus we observe the sun to move by an equal amount. Thus in one rotation of the earth one sidereal day is complete but an apparent solar day is not because the sun has moved about a degree to the east on the ecliptic. The earth has to rotate a further angle between the present meridian and the meridian on which the sun has moved. This arc is called the solar lag. When the earth covers this angle the sun transits i.e. an apparent solar day has elapsed. Thus the time taken by the earth to rotate through the angle (360 + solar lag) is an apparent solar day. Apparent solar day is always greater than the sidereal day.

The arc lengths traveled by the sun on the ecliptic each day are not equal so the lengths of apparent solar days are also not equal. Apparent time is found with the help of solar clocks.

4. Mean solar day: Since the arc lengths traveled by the sun on the ecliptic each day are not equal the lengths of apparent solar days are also not the same. To remove this discrepancy the astronomers have assumed a fictitious sun which travels with uniform velocity in the same time period as the actual sun. The interval between two consecutive transits of this fictitious sun across a meridian is called a mean solar day. It is the time in which the earth rotates 360.83559 degrees. An apparent day is sometimes longer, sometimes shorter and sometimes equal.

Declination of the sun

The earth moves round the sun in the ecliptic, so the sun appears to move round the earth in the ecliptic. The ecliptic does not coincide with the celestial equator. They intersect at two points called vernal equinox and autumnal equinox. The angle of intersection is 23o 27 ́. Half of the ecliptic is towards the north of the celestial equator and the other half south of it. Any point on the ecliptic which is not at equinoxes will be either north of equator or south of it. The angular distance of the sun from the equator is called the declination of the sun. It can have a maximum value 23o 27 ́ north (positive) or south (negative). When the declination of the sun is positive, day is longer than the night and when negative, night is longer than the day. The value of declination of the sun at any particular day varies slightly but the rate is very small 0.0503 seconds per year. It is quite negligible and will become appreciable in centuries.

Local Time and Standard Time

Standard Time: We use standard time in every day life. As far as local time is concerned, in our daily life, we neither need it nor do we care for it. So when local time is mentioned with standard time we are surprised. Standard time means the time which is used and is the same throughout the country. When we say that in Pakistan it is 8 p.m. that means that the standard time throughout Pakistan is 8 p.m.

Local Time: Local time in the eastern parts of Pakistan is different from that of the western parts. The reason is that the sun first rises in the eastern parts than in the western parts. The earth is rotating round its axis and its different parts keep facing the sun and keep moving away from it completing one complete rotation in 24 hours. There are 1440 minutes in 24 hours. Thus in 1440 minutes 360 degrees of the earth faces the sun and moves away from it. Dividing 1440 by 360 we see that after every 4 minutes one degree of longitude faces the sun. Thus in every degree the time differs by 4 minutes. So in 15 degrees the time changes by one hour. It takes one hour for 15 degrees of the earth to pass in front of the sun. To conclude, it can be said that there is a difference of 4 minutes in every degree of longitude.

It is clear that if at Greenwich (longitude 0o) the time is 12 noon then at 1o E the time will be 12.04 p.m. On the other hand 1o W the time will be 11.56 a.m. So at 15o E the time will be 1 p.m. because in the east the time is ahead. At 15o W the time will be 11 a.m. because the time is slow and behind towards the west.

 

 

          Hours

 

                    Time Relations             

     TimeZone

2.5       Calendars

There are four types of calendar:

i.          Lunar calendar            ii.         Solar calendar

iii.        Luni-solar calendar     iv.        Solar- Hijri calendar

 

i.                    Lunar calendar      

            As the name suggests, it depends on the phases of the moon (change in shape from crescent to full and back) and on rising and setting of the moon. This is the oldest, most accurate and the simplest calendar. Ancient people counted days and months with the help of a new moon. A month begins with a new moon. A lunar month is 29 or 30 days in length. There are 354 or 355 days in a lunar year.

Hijri calendar: Lunar calendar has been in use since ancient times. At the time of the Holy Prophet (peace be upon him), Arabs used it. But it was the practice of the locals to alter or change the months without any consideration of the irregularity or consequences. Sometimes one month was made equal to two months and sometimes they used to drop one month. In the Holy Quran this wrong practice is named ‘nasi ‘(Surah Taubah verse 37). Anyway up to Hajatul Widah (The last Pilgrimage) all months of the year were of the present order. Thus the present Hijri Calendar was founded at the time of Hajatul Widah (The last Pilgrimage). Hazrat Umar formally introduced it during his tenure of caliphate. In this version Muharramul Haram was declared the first month of the year and the year of migration of the Holy Prophet (P.B.U.H) was declared to be the beginning of the calendar.

ii.         Solar or Gregorian calendar

It is based on the revolution of the earth round the sun. Seasons change due to the revolution. Care has been taken to ensure that all seasons begin every year on fixed dates. Sometimes the earth comes closer to the sun and sometimes moves away from it. In lunar calendar a day begins at the sunset whereas in solar calendar a day begins at mid night. Since the beginning of a month does not depend on visibility of the moon, the number of days of each month in solar calendar are assigned before hand. It is predetermined that which month will contain how many days. Special attention is paid to months and seasons so that seasons always begin on the same date each year. For example every year it will be summer in June and July and winter in November and December. In this calendar a year has 365 days. Some months are of 30 days, some have 31 days except February which is of 28 days. After every four years February has 29 days. This year is called leap year. January, March, July, August and December have 31 days whereas April, June, September and November have 30. February has 28 days but in a leap year it has 29 days..

During the days of Pope Gregory XIII the calendar became out of phase with the seasons. On the advice of astronomers he dropped 10 days in October. Thus the date following 15th October was 25th October. Even today these 10 days are missing in the calendar of that year (1582). If after every four years a day is not added, the calendar will again become out of phase with seasons. In comparison the lunar calendar does not need addition or subtraction of any day. May Allah (s.w.t). guide us to use it in every day life. It is a conspiracy according to which propaganda is made that the Muslims cannot celebrate Eid on the same day and keep fighting on the moon and that lunar calendar is baseless and is not fit for use.


Reason for leap year

The earth makes one complete revolution round the sun in about 365 days and 6 hours. The addition of 6 hours has compelled the founders of solar calendar to compensate it. Six hours per year amount to 24 hours in 4 years i.e. a day in 4 years. Thus if a day is added every fourth year, in the next year (the fifth year) begins in accordance with seasons.

iii.        Luni Solar calendar

This calendar is the basis for the Jewish calendar. Solar year is 10 or 11 days longer than the lunar year. Thus after 3 lunar years a difference of one month occurs with the solar calendar. They added a month in the lunar calendar after every 3 years and called it “inter calary month”. Since this calendar uses both types of calendars it is called luni solar calendar.

iv.        Solar Hijri Calendar

This calendar is not practically in use today. Some Muslim astronomers have introduced its concept. It differs from the solar calendar in the following aspects:

  • The calendar will begin from the year of migration of the Holy Prophet (P.B.U.H).
  • The names of months will be on important places or events which were at the time of the Holy Prophet (peace be upon him). The order will be Hira, Mairaj, Sur, Quba, Badar, Uhad, Ahzab, Rizwan, Khaiber, Fatah, Hunain, and Tabuk. The present names of months are unislamic and mythological.
  • In the leap year a day will be added in the last month i.e. Tabuk. The advantage is that being the last day of the year; it will have no effect on other days.

 

In the presence of lunar calendar solar calendar is also a need because in some matters the solar calendar is used, for example in the calculations of times of prayers and times of sehar and iftar. If these times are calculated for example for 1st January, then they will remain the same on that day for all years to come.

 

 


 

CHAPTER 3

                           

Compilataion and Composition of Prayer Times

 

3.1       Mathematical Method of Prayer Times and Qibla Direction

It is necessary to have some basic elementary knowledge of mathematics for finding the times of prayers and direction of Qibla.

  • Spherical trigonometry is used for calculations. Very elementary knowledge is sufficient as we use computers or scientific calculators.
  • Latitude and longitude of the place (it can be found with the help of an atlas.)
  • The longitude of the particular place according to which the standard time of the place is kept. (page        ) (For example the standard time of Pakistan is kept according to longitude 75o E.)
  • Declination of the sun on for all dates of the year. (Table on page        ).
  • Time of Zawal (Transit time) for all dates of the year ( Table on page         )
  • Altitude or depression of the sun at the required prayer time. (E.g. for dawn 18o below horizon.
  • Difference between standard and local times.

Geometry, Trigonometry and Spherical Trigonometry

Angle: Angle is obtained when two lines meet at a point forming a V shape. For example needles of a clock. The needles are called the arms of the clock. There are three types of angles

Right angle: The two arms of the needles of a clock at 3 O’clock. This angle is called a right angle = 90o.

 

Acute angle: An angle which is less than 90o is called an acute angle.

Obtuse angle: An angle whose which is more than 90o is called an obtuse angle.

 

 

 

 

 

 


Right                           Acute                                    Obtuse

                Angle                          angle                                     angle

 

There are 360o in a complete circle. If it is divided in 4 equal parts each part is equal to 90o or a right angle.

 

Triangle: It is a figure bounded by three sides. It has 3 angles. A triangle is represented by the figure ABC. The three sides are AB, BC and AC and three angles are X, Y and Z. If one angle of the triangle is a right angle, it is called a right angled triangle. The horizontal side is called its base, the vertical side the perpendicular and the side facing the right angle is called the hypotenuse.

 

 

                                          A

                                      x

                                                   Perpendicular                 hypotenuse

                             y        z

                   B                            C

                                                                                Base

 

                          Triangle                            Right angled triangle

 

The sum of the three angles of a plane triangle is 180o. So a plane triangle cannot have more than one right angle and two obtuse angles.

There are three types of triangles:

i.          If all sides of a triangle are equal it is called equilateral triangle.

ii.         If two sides of a triangle are equal. It is called an isosceles triangle.

iii.        If all three sides are unequal, it is called a scalene triangle.

 

Trigonometric ratios:

 

                                                                                        C

 

 

                                                                               

                                                       

               θ                                   90

                                A                                                    B

 

 

Let ABC be a right angled triangle. ABC = 90o and    BAC = θ (theta). AB is the base also called the adjacent side, BC is the perpendicular, also called the opposite side and AC is the hypotenuse.

 

There are six trigonometric ratios:

 

Sin θ = ,            cos θ = 

 

tan θ =  ,           cosec θ =

 

sec θ =  ,           cot θ =

 

These ratios refer to a triangle formed in a plane which is called a plane triangle.

 

Solution of a triangle: A triangle has 3 sides and 3 angles. These six quantities are called the elements of a triangle. If some elements of a triangle are known, the process of finding other elements is called the solution of the triangle. It is done with the help of the trigonometric ratios.

 

Spherical triangle: If instead of in a plane, a triangle is drawn on the surface of a sphere; its sides are arcs instead of lines. Such a triangle is called a spherical triangle. In astronomy all heavenly bodies, the sun, the moon, the stars appear to move on the sky and move on arcs of circles. Their motions are studied with the help of spherical trigonometry. A spherical triangle also has same six trigonometric ratios.

 

3.2       Calculations of Prayer Times

            Prayer times are explained in the books of fiqah. According to them

  • the time of Fajar starts from dawn (subah e sadiq),
  • time of Zohar from the time of transit (zawal),
  • time of Maghrib from the sunset and
  • time of Isha from the end of red twilight,
  • according to Sahibain (Imam Yousuf and Imam Humbel) Isha is permissible to offer at the end of the white twilight
  • according to Hanafi Maslak. Time of Asar begins at Misle-Sani (when the shadow of a body is twice the length of the body and the length of its minimum shadow)
  • According to Sahibain (Imam Yousuf and Imam Humbl) Asar e Shafi begins at masal e Awwal (when the shadow of a body is the sum the length of the body and the length of its minimum shadow).

 

Prayers should be offered at times determined by these criteria. It is necessary that prayer times should be calculated with the help of clocks especially as due to high buildings, the determination of time according to the above criteria is difficult.

It is necessary to know the altitude and depressions of the sun for different prayers in order to solve the mathematical calculations.

 

Dawn (Subah E Sadiq), Isha and Fajar Times

In his book “Mayarul Auqat As-Seam wo Salat”, Prof. Abdul Wasey says, “that dawn (subh e sadiq) is that light which is visible before the sunrise due to reflection and diffraction on the eastern horizon. When the sun approaches the horizon its rays are reflected from upper atmospheric layers to reach the earth (according to law of reflection: angle of reflection is equal to angle of incidence.) and we observe a vertical pillar of light. As the sun nears the horizon, this light narrows at the top and spreads near the horizon. As the sun further nears the horizon, dispersed light also merges with it and brightens it. The white light gradually becomes red and then yellow. After this the sun starts to rise.”

Evening twilight (shafaq) is that light which is visible after sun set on the western horizon. The reasons for it are the same as for dawn. The changes are same but in the opposite order. i.e. first the light is yellow then it becomes red and then white. It spreads on the horizon and gradually narrows at the bottom and becomes vertical. Astronomically both the phenomena are called twilight. The morning twilight begins and the evening twilight ends when the centre of the sun is 18o below the horizon.

When the sun is 18o below the horizon before rising it is dawn (subh-e-sadiq) which indicates the beginning of Fajar time. When the centre of the sun is 18o below the horizon after setting, the time of Isha begins. The methods of finding the time for the beginning of the morning twilight and end of the evening twilight are the same as for finding times of sun rise and sun set except that the zenith distance of the sun is taken 108o instead of 91o.

Dawn starts when the centre of the sun is 18o below horizon. The scholars have adopted 18o below horizon and we will also accept it. According to this rule when the sun is 18o below the eastern horizon before rising, it is dawn. On the other hand after setting when it goes 18o below the western horizon Isha time begins. Thus both for dawn and Isha the depression of the sun is the same (i.e. 18o) but in Fajar it is before sun rise and in Isha after sunset.

 

In mathematical formulae to calculate the times of dawn and Isha, the zenith distance of the sun is taken 90 + 18 = 108o.

Maghrib and Sunset

When the sun completely sets, it is the starting time for Maghrib prayer. What is the zenith distance of the sun at that time? The detailed discussion for the answer follows.

When we say that the sun is at such and such distance it means that the centre of the sun is at that distance. If the sun is at a distance of 90o towards the west, it means that half the sun is below the horizon and half is visible. Practically we know that the sun sets when it goes completely below the horizon. The diameter of the sun is 32 minutes so half of the diameter is 16 minutes. So the sun will set when its zenith distance is 90o

16 ́ W.

 

 

 

 


                                Sun                                         Horizon

 

                                                                        Sun

               

                Astronomical sun set      Real Sunset

 

            If we place a coin in a glass or a vessel full of water and observe it from the side, the coin appears higher than its actual position. It happens because the rays of light enter our eyes from a denser to a rarer medium and are bent. This phenomenon is called refraction. The atmosphere of the earth also behaves in the same way. As a result the sun is visible to us even when its centre is below 90o 16 ́. Refraction of the sun is found to be 34 ́. It means that the sun has still to go 34 minutes further down to set. Thus its zenith distance should become 90o 50 ́ for it to be practically below the horizon. This is sharaie (Islamic) sunset. Converting to decimals the zenith distance of the sun at sun set and sunrise must be 90.8333o.

            Prof. Abdul Wasey says, “That according to the astronomers, the sun rises and sets when its centre is on the horizon. Zenith distances of the sun on both these occasions are 90o. In the absence of refraction, half the disc of the sun should be visible on both occasions. But due to refraction it appears 32 ́ higher. The maximum diameter of the sun is 32.5 ́. When the centre of the sun is on the horizon it appears 32 ́ higher i.e. the lower limb is 7 ́ above horizon. When the centre of the sun is 32 ́ below, its centre appears on the horizon. This is astronomical sunrise or sunset. At this time the zenith distance of the sun is 90o 32́.”

Sharaie Sunrise:  Sharaie sunrise occurs when the upper limb of the sun just touches the eastern horizon. And the entire disc of the sun is below horizon. Similarly at sharaie sun set upper limb of the sun touches the western horizon and the entire disc is below it. Thus at both these times the zenith distance of the sun should be 900 50 ́. The value of refraction used is the average value. It is safer to take the zenith distance 91o. Sharaie sun rise occurs a little bit earlier than astronomical sunrise and Sharaie (Islamic) sunset occurs a bit later.

 

                Slanting Path


ZOHAR

            The time of Zohar begins immediately after transit. When the sun rises, the shadows are very long. As the altitude of the sun increases, the lengths of shadows of any pole or mast decrease. When the sun is at transit, the length of shadow is minimum. This is called real shadow. After it the lengths of shadows begin to increase again. As soon as the lengths of shadows start increasing, the time of transit ends. This is the time in which the sun has traveled half its journey from the east to the west.

            To find the time of transit, first find the difference between the times of sunrise and sunset, divide it by two and add to the time of sun rise. This will be the time of real shadow. At this time the sun is on the observer’s meridian. This time is prohibited for prayer. Zohar time starts after it.

 

Example: On 13th January, the sun rises in Karachi at 6:06 a.m. and sets at 6:08 p.m.

The difference is 12 hours and 2 minutes. Half of it is 6 hours and 1 minute. Adding it to the time of sun rise we get   6:06 + 6:01 = 12:07.

Thus transit time in Karachi on 13th January is 12:07 noon. After five minutes the time for Zohar starts.

            We also need to know, along with other data, the time of transit and the declination of the sun for the day for which the prayer times are to be found. They are involved in all calculations leading to determination of prayer times.

Declination of the Sun

Declination of the sun is its distance from the celestial equator. Since the sun is on the celestial equator on 21st March and 21st September, their declination on these dates is zero. On 21st June the sun is above the tropic of Cancer and its declination is maximum about 23.5o North or + 23.5o. On 21st December it is on the tropic of Capricorn and its declination is minimum 23.5o South or – 23.5o.

Equatorial Coordinate System

The system in which right ascension and declination of a heavenly body are used to locate its position is called the equatorial coordinate system. It is explained below.

 

3.3       Celestial Sphere

A very large imaginary sphere whose centre is at the centre of the earth is called the celestial sphere. It also has the northern and the southern hemispheres. Its north pole is called the Celestial North Pole and the South Pole is called the Celestial South Pole. Its equator is called celestial equator. The lines parallel to the equator are lines of declination (corresponding to latitudes on the earth). Its longitudinal lines are called meridians or time lines because the time for a heavenly body to reach a given point is determined with their help.

Two coordinate are needed to determine the position of a heavenly body (1) Right ascension and (2) declination.

 

Right ascension, Vernal and Autumnal equinoxes:

 

The celestial equator intersects the ecliptic at two points called Vernal and autumnal equinoxes.

Vernal equinox is taken as origin or base. The distance along the celestial equator measured towards the east from vernal equinox to the meridian through a body is called its right ascension. It is measured in terms of time. For example if a body is 150 east from vernal equinox it’s right ascension is 1 hour.

Thus the distance of a heavenly body measured from vernal equinox measured east wards is its right ascension.

 

Declination

The distance of a heavenly body from celestial equator measured north or south along a meridian is called its declination. It is positive for bodies north of equator and negative in the south.

The right ascension and declination of stars are constant but for the sun they change. But at a given time the right ascension and declination of the sun all over the world are the same. For example whatever the declination of the sun is on 25th July in Pakistan, it is the same on that day all over the world.  Declination of the sun is needed for calculations of prayer times.

            Times of transit of the sun and its declination are given in the table beginning from page         .

Tables from page 99 to 104

 

3.4       Method to Find Time of Transit (Zawal Time)

The formulae used in computer or calculators to calculate the time of transit are explained below.

Time of transit: In calculating prayer times, first of all we have to find the time of transit. Other times are obtained on its basis. First we discuss in some details about the time of transit.

Half of the time interval between sunset and sunrise is called the time of transit. Transit is also called upper culmination. This is the time when the sun reaches observer’s meridian. At this time the shadow of everybody is the least and it is called real shadow. Zohar time begins after upper transit. On the other hand half the time between sunset and dawn is called sharaie transit. It is related only with fasting. The intention (niyat) of fast must be made before sharaie transit.

(Note): The time of transit of the sun on a particular day is the same all over the world. The difference is only due to the difference between local and standard times. Find the difference between the standard and local times and add or subtract according to the criteria in the time of transit given in GMT or Universal Time to get the local time of transit. Local and standard times have already been discussed on page       .

For example, Pakistan standard time corresponds to the longitude 75o E and longitude of Karachi is 67o E. The difference is 75 – 67 = 8o = 8x4 =32 minutes.

           

The tables on page ……  give the UT for transit for any day of the year. Time of transit at any place can be found as explained below:

 

Example 1: Find the time of transit in Karachi on 1st January.

From the table on page     the time of transit is 12:03 UT.

Longitude of Karachi = 67o E.

Longitude of Standard time = 75o E.

Difference = 75 – 67 = 8o = 8 x 4 = 32 minutes.

Formula: Time of transit = UT + difference

= 12:03 + 0:32 = 12:35.

So the sun transits in Karachi at 35 minutes past 12 noon on 1st January.

 

Example 2: Find the time of transit in Chiniot on 22nd December.

Time of transit from the table = 11:58:29 UT.

Longitude of Chiniot = 73o E.

Longitude of Standard time = 75o E.

Difference = 75 – 73 = 2o = 2 x 4 = 8 minutes.

Formula: Time of transit = UT + difference

            = 11:59:29 + 0: 08:0 = 12:06:29.

I.e. the time of transit at Chiniot on 22nd December is 6 minutes past 12 noon.

 

Example 3: Find the time of transit at Tokyo (Japan) on 22nd December.

Time of transit from table = 11:58:29 UT.

Longitude of Tokyo = 139o 45 ́ E. = 139 + 45/60 = 139.75o E.

Longitude of Standard time of Japan = 135o E.

Difference = 135 – 139.75 = - 4.75o = - 4.75 x 4 = - 19 minutes.

Formula: Time of transit = UT + difference

            = 11:59:29 – 0:19:0 = 11:39:29.

I.e. the time of transit at Tokyo on 22nd December is 11:39 am.

 

  • In order to find out prayer times for, we first have to find the time of transit and then other times are found according to the following rules:
  • Subtract the calculated value of H for dawn (subah e sadiq) from the time of transit to get the correct time for dawn. H means hour angle.
  • Add the calculated value of H for Isha to the time of transit to get the correct time of Isha.
  • Subtract the calculated value of H for sunrise from time of transit to get the correct time of sunrise
  • Add the calculated value of H for sunset to time of transit to get the correct time of sunset
  • Add the calculated value of H for misle Awwal to time of transit to get the correct time of Asar e Shafi.
  • Add the calculated value of H for misle Sani to time of transit to get the correct time of Asar e Hanafi.

In these formulae H is the hour angle of the sun found by formulae given below.

 


Basic Formulae

The hour angle H of the sun used in the above rules is determined by the following formulae. In these formulae X stands for the declination of the sun on the given date and Y for the latitude of the place.

 

For dawn (Subh-e-sadiq) and Isha:

H =

For sunrise and sunset:

 

H =

 

For Misle Awwal

 

a = 1 + tan | X – Y |; A = ; G = sin ( tan – 1 A)

 

H =

 

For Misle Sani

 

a = 2 + tan | X – Y |; A = ; G = sin ( tan – 1 A)

H =

 

 

Method to Find Dawn and Isha Time

To calculate the time of prayers of any place we need to know the following:

  • Latitude and longitude of the given place (can be found from any atlas).
  • The longitude corresponding to the standard time of the place (table on page         ) e.g. standard time of Pakistan corresponds to longitude 75o E.
  • Declination of the sun on the given date.                   (table on page         )
  • Transit time for the given date (table on page        )
  • Altitude or depression of the sun for the given time (e.g. for dawn 180 below horizon,
  • for sunset and sunrise zenith distance 90.833o )
  • The difference between standard and local time.

 

Example 1: Find the time for dawn and Isha prayer for Karachi on 1st January.

Longitude of Karachi = 67o E.

Latitude of Karachi = Y = 24.9o N.

Longitude of Standard time of Pakistan =  75o E.

Declination of the sun on 1st January = X = – 23.12o.

Time of transit on 1st January 12.05554 = 12:03.

Difference between local and standard time = 75 – 67

= 8o = 8 x 4 = 32 minutes.

Transit time of Karachi on 1st January = UT + 32 min

= 12:03 + 0:32 = 12 : 35.

 

Formula for dawn and Isha

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 6.661262 hours

    = 6 hours 39 minute.

Time of dawn = transit time – H = 12:35 – 6:39

= 5:55.

Thus the end of time for Sehar and beginning of time for Fajar prayer in Karachi on 1st January is 5:55 am.

 

Time for Isha = transit time + H

= 12:35 + 6:39 = 19:14.

The Isha time begins at 7:14 pm in Karachi on 1st January.

 

Example 2: Find the time of dawn and Isha for Harper (Hazara) on 1st January.

Longitude of Haripur = 73o E.

Latitude of Haripur = Y = 34o N.

Longitude of Standard time of Pakistan =  75o E.

Declination of the sun on 1st January = X = – 23.12o.

Time of transit on 1st January 12 : 03 = 12.05554.

Difference between local and standard time = 75 – 73

= 2o = 2 x 4 = 8 minutes.

Transit time at Haripur on 1st January = UT + 8 min

= 12:03 + 0:08 = 12 : 11.

 

Formula for dawn and Isha

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 6.4491348 hours

    = 6 hours 26 minute 56 seconds = 6:27.

Time of dawn = transit time – H = 12:11 – 6:27

= 5:44.

Thus the end of time for Sehar and beginning of time for Fajar prayer in Haripur on 1st January is 5:44 am.

 

Time for Isha = transit time + H

= 12:11 + 6:27 = 18:38.

The Isha time begins at 6:38 pm in Haripur on 1st January.

 

Example 3: Find the time for dawn and Isha prayer for Peshawar on 26th October.

Longitude of Peshawar = 71o 40’ E. = 71.67o.

Latitude of Peshawar = Y = 34o N.

Longitude of Standard time of Pakistan =  75o E.

Declination of the sun on 26 October = X = – 12.713o.

Time of transit on 26 October 11.73 = 11: 44.

Difference between local and standard time = 75 – 71.67

= 3.33o = 3.33 x 4 = 13 minutes.

Transit time at Peshawar on 26th October = UT + 13 min

= 11:44 + 0:13 = 11 : 57.

 

Formula for dawn and Isha

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 6.882403 hours

    = 6 hours 53 minute.

Time of dawn = transit time – H = 11:57 – 6:53

= 5:04.

Thus the end of time for sehar and beginning of time for Fajar prayer in Peshawar on 26th October is 5:04 am.

 

Time for Isha = transit time + H

= 11:57 + 6:53 = 18:50.

The Isha time begins at 6:50 pm Peshawar on 26th October

 

Example 4: Find the time of sunrise and sunset at Karachi on 1st January.

Longitude of Karachi = 67o E.

Latitude of Karachi = Y = 24.9o N.

Longitude of Standard time of Pakistan =  75o E.

Declination of the sun on 1st January = X = - 23.12o.

Time of transit on 1st January 12.05554 = 12:03..

Difference between local and standard time = 75 – 67

= 8o = 8 x 4 = 32 minutes.

Transit time at Karachi on 1st January = UT + 32 min

= 12:03 + 0:32 = 12 : 35.

 

Formula for sunrise and sunset

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 5.3030626 hours

    = 5 hours 18 minute.

Time of sunrise = transit time – H = 12:35 – 5:18

= 7:17.

Thus the sun rises in Karachi on 1st January at 7:17 am.

 

Time for sunset = transit time + H

= 12:35 + 5:18 = 17:53.

The sun sets at 5:53 pm in Karachi on 1st January.

 

Time of Misle Awwal (Asar E Shafi) and Misle Sani

(Asar E Hanafi)

If a rod (AB) is fixed vertically, at the time of transit it’s shadow is minimum called real shadow (BC).

Suppose the length of a rod is 6 feet and length of its real shadow is 1 ft. When the length shadow 6 + 1 =7 ft. long, it is misle Awwal i.e. Asar e Shafi begins (BD). When the length of shadow becomes 2 x 6 + 1 = 13 ft. long it is Misle Sani i.e. Asar e Hanafi begins (BE).

Misle Awwal means the length of the shadow of the body and the real shadow. According to Imam Shafi Zohar time ends and Asar time begins at this instant. Misle Sani is the time when the length of the shadow is the sum of the real shadow and twice the length of the body. According to Hanafi Maslak Zohar time ends and Asar begins. According to Quiz Abu Yousuf Zohar time ends at misle Awwal and Asar begins at misle Sani.

 

 

                                  A

 

 

 

                                  B           C                D                          E

 

Example 5: Find the time for Asar e Shafi at Karachi on 1st January

Transit time for Karachi on January 1 = 12:35.

Latitude of Karachi = Y = 24.9o N.

Declination of the sun on 1st January = X =    23.12o.

 

 

Formula: a = 1 + tan | X – Y |; A = ; G = sin ( tan – 1 A)

 

H =

a = 1 + tan | 24.9 – (–  23.12)| = 1 + tan 48.02

   = 1 + 1.11139 = 2.11139.

A = 1/a = 1/(2.11139) = 0.4736216.

G = sin( tan – 1 0.4736216) = sin( 25.343248) = 0.428042.

 

H =

 

H =

 

H =

 

H =

 

H = = H =

 

=  = 2.97723 hours = 2:58.

Time of Asar e Shafi = Transit time + H

                        = 12:35 + 2:58 = 3:33 pm.

 

Example 6: Find the time for Asar e Hanafi for Karachi on 1st January

Transit time of Karachi on January 1 = 12:35.

Latitude of Karachi = Y = 24.9o N.

Declination of the sun on 1st January = X = –  23.12o.

Formula : a = 2 + tan | X – Y |; A = ;

G = sin ( tan – 1 A)

 

H =

a = 2 + tan | 24.9 – (– 23.12)| = 2 + tan 48.02

   = 2 + 1.11139 = 3.11139.

A = 1/a = 1/3.11139 = 0.3213996..

G = sin( tan – 1 0.3213996) = sin( 17.817393)

= 0.3059843.

 

H =

 

H =

 

 

H =

 

H =

 

H = = H =

 

=  = 3.7065833 hours = 3:42.

Time of Asar e Hanafi = Transit time + H

                        = 12:35 + 3:42 = 16:17.

 

Thus the time for Asar e Hanafi in Karachi on 1st January is 4:17pm.

 

Example 7: Find the time of dawn for Glasgow on 1st January.

Longitude of Glasgow = 4o 15’ W. = 4.25.

Latitude of Glasgow = Y = 55o 51’ N.= 55.85.

Longitude of Standard time =  0o .

Declination of the sun on 1st January = X = – 23.12o.

Time of transit on 1st January 12 : 03 = 12.05554.

Difference between local and standard time = 0 – (– 4.25) = 4.25o = 4.25 x 4 = 17 minutes.

Transit time at Glasgow on 1st January = UT + 17 min

= 12:03 + 0:17 = 12 : 20.

 

Formula for dawn

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 5.88208 hours

    = 5 hours 52 minute 55 seconds = 5:53..

Time of dawn = transit time – H = 12:20 – 5:53

= 6:27.

Thus the end of time for Sehar and beginning of time for Fajar prayer in Glasgow on 1st January is 6:27 am.

 

 

Example 8: Find the time of sunrise and sunset at Moscow on 1st March.

Longitude of Moscow = 37o 36’E = 37.6.

Latitude of Moscow = Y = 55o 45’N = 55.75.

Longitude of Standard time =  45o E.

Declination of the sun on 1st March = X = – 7.278o.

Time of transit on 1st March 12.05554 = 12:12.

Difference between local and standard time = 45 – 37.6

= 7.4o = 7.4 x 4 = 30 minutes.

Transit time at Moscow on 1st March = UT + 30 min

= 12:12 + 0:30 = 12 : 42.

 

Formula for sunrise and sunset

 

H=

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 5.3763276 hours

    = 5 hours 23 minute.

Time of sunrise = transit time – H = 12:42 – 5:23

= 7:19.

Thus the sun rises in Moscow on 1st March at 7:19 am.

 

Time for sunset = transit time + H

= 12:42 + 5:23 = 18:05.

The sun sets at 6:05 pm in Moscow on 1st March

 

Example 9: Find the time of beginning of Fajar prayer for Johannesburg on 1st May.

Longitude of Johannesburg = 28o 02’ E. = 28.0333.

Latitude of Johannesburg = Y = 26o 12’ S.= – 26.2.

Declination of the sun on 1st May = X = 11.950o.

Time of transit on 1st May  = 11.9501 = 11:57.

Difference between local and standard time = 2 minutes.

Transit time at Johannesburg on 1st May = UT + 2 min

= 11:57 + 0:02 = 11 : 59.

 

Formula for dawn

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 6.9568449 hours

    = 6 hours 57 minute 24 seconds = 6:57..

Time of dawn = transit time – H = 11:596:57

= 5:02.

Thus the end of time for Sehar and beginning of time for Fajar prayer in Johannesburg on 1st May is 5:02 am.

 

Example 10: Find the time of beginning of Fajar prayer for Beijing on 1st September.

Longitude of Beijing = 116o 23’ E. = 116.3833.

Latitude of Beijing = Y = 39o 54’ N.=  39.9.

Declination of the sun on 1st September = X = 7.979o.

Time of transit on 1st September  = 12:00.

Difference between local and standard time = 14 minutes.

Transit time at Beijing on 1st September = UT + 14 min

= 12:00 + 0:14 = 12 : 14.

 

Formula for dawn

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 7.167082 hours

    = 7 hours 10 minute 22 seconds = 7:10..

Time of dawn = transit time – H = 12:147:10

= 5:04.

Thus the end of time for Sehar and beginning of time for Fajar prayer in Beijing on 1st September is 5:04 am.

 

Example 11: Find the time of beginning of Fajar Prayer and  times for sunrise and sunset for New York on 1st November.

Longitude of New York = 74o W.

Latitude of New York = Y = 40o 42’ N.= 40.7.

Longitude of Standard time =  75o .

Declination of the sun on 1st November.= X = – 14.682o.

Time of transit on 1st November. 11 : 44

Difference between local and standard time = 75 – (74)

= 1o = 1 x 4 = 4 minutes.

Transit time at New York on 1st November. = UT + 4 min

= 11:44 + 0:04 = 11 : 48.

 

Formula for dawn

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 6.75357 hours

    = 6 hours 45 minute 12 seconds = 7:45..

Time of dawn = transit time – H = 11:48 – 6:45

= 5:03.

Thus the end of time for Sehar and beginning of time for Fajar prayer in New York on 1st November. is 5:03 am.

 


Formula for sunrise and sunset

 

H =

 

   =

 

Find and substitute the values of sin and cos from calculator

H =

 

Perform multiplication

 

H =

 

Perform addition

 

H =  . Perform division

 

H = . Take cos inverse

H =  = 5.206218 hours

    = 5 hours 13 minute.

Time of sunrise = transit time – H = 11:48 – 5:13

= 6:35.

Thus the sun rises in New York on 1st November. at 6:35 am.

 

Time for sunset = transit time + H

= 11:48 + 5:13 = 17:01

The sun sets at 5:01 pm in New York on 1st November.

 

3.5              Altitude Correction Factor

Astronomers and other experts who are mainly concerned with the tabulation of prayer timings are of the opinion that any FLAT surface with

* Sufficiently extended unobstructed area of any height

* Clearly visible horizon will be considered for the calculation of sun-rise or sun-set, as a normal area, as if it is a FLAT COASTAL PLANE.

Abdul Majeed Khan, a weather expert and Meteorologist of Pakistan Meteorological Department considers it as a debatable issue as he added the correction factor for all the places and towns of Pakistan including Lahore and Islamabad by keeping in view the height of the place above mean sea level.
On the contrary, the observations reveal that any Plateau shaped unobstructed flat surface, of any altitude does not need any correction factor to apply particularly for the calculations of sun-rise and sun-set timings. It seems strange but it is a reality.

 

 In other words it can be concluded that:

*…..any obstructed surface of any height,

*…..or any place located on a conical shaped hill top

*… .Or an escarpment having a steep slope, certainly needs some difference of time correction to apply – same is the case with journey by a plane or space ship.

 

It may be remembered that the difference in time is not uniform everywhere. It differs from Latitude to Latitude and at every latitude from date to date. So computed tables (Shown below) are composed in such a way that right from Zero degree Equator to 60 degrees, correction of time for various altitudes have been shown from 1000 to 11000 feet., and also from 30,000 to 40,000 feet for 1st  and 15th of each month of a solar calendar. The two dates are enough to depict the picture for the entire month. 

Tables are computed for every 5th degree of Latitude up to 60th parallel these tables show the difference of time at various altitudes from 1000 to 11000 feet and 30,000 to 40000 feet with a few exceptions.

During our journey by a jet plane, which usually flies between 30000 to 40000 ft. above mean sea level, we need to know the difference of time of sun-rise and sun-set for our prayers, Iftar and Maghrib, as, due to the difference of Horizon, the time at this height will be different from the ground.

During our journey, we do not calculate the height of the plane from the ground but from the above mean sea level, particularly for finding the timings of sunrise & sunset. This we need due to the difference of horizon. Only at the time of landing and take off the pilot needs to know the height of the plane from the run way (to which we call ground) or local surface.

But in the sky, during the flight, we need to know the height of the plane from the sea level and certainly not from the ground above which it is flying. To facilitate the air passengers and the compilers of prayer time tables, the following tables of time difference will prove helpful. It is vital to check the difference in time with reference to altitude, latitude and date everywhere.

 

3.6       Aneroid or Mercurial Barometer

Aneroid or mercurial barometer is used to find out the (air) atmospheric pressure and the height. At any place a barometer by registering the pressure of the atmosphere indicates the height of that place from the sea level. Generally heights up to 20,000 feet can be measured. As the height increases the pressure of the atmosphere decreases and thus if the pressure decreases it is clear that height has increased. As a general rule it can be said that pressure decreases by ONE inch for every 1000 feet. This generalization is, however, not universally applicable, because the atmospheric pressure changes as a result of the presence of a number of disturbances and depressions in the air, so that the reading from the instrument will not be an absolutely true indication of height. 

(2) Murree is about 7000 ft high from sea level. If you want to calculate the timings of sunrise and sun-set of Hill Tops of this hilly station, obviously you need to have a point of reference as to wherefrom you will calculate its height.

Do you think that one should find out the height from the ground level of Islamabad or Rawalpindi which is the nearest ground level from this hill top? If not what is your opinion?

Certainly the horizon of this hill top is different from the horizon of Islamabad and also from the mean sea level. Wherefrom one should determine its height? It may be measured from the sea level.

As far as the time of Subhe-Sadiq is concerned we need not to apply any Altitude Correction up to the height of 3000 feet elevation.

 

3.7       Tables for Altitude Correction

To find the altitude correction for any Latitude and Height at any particular Date, reference to Table 1 and Table 2 given below is necessary:

First of all find the column in Table 1 corresponding to the desired Latitude and row in the same table corresponding to its desired height. If the entry in that row and column is a number (digit) that is the correction in time in minutes due to altitude. If the entry in the column corresponding to desired height and latitude in Table No.1 is an alphabet then refer to Table No.2.

Look for the entry in the column corresponding to the respective alphabet and the row corresponding to the date. The entry in the column is the correction in time in minutes.  

 

 

 

 

 

TABLE      1

.LATITUDES IN DEGREES

HEIGHT

IN

 

 

 

 

 

 

 

 

 

 

 

 

 

FEET

0o

5o

10o

15o

20o

25o

30o

35o

40o

45o

50o

55o

60o

1000

2

2

2

2

2

2

3

3

3

3

4

5

F

2000

3

3

3

3

3

3

4

4

4

5

5

6

G

3000

4

4

4

4

4

4

4

5

5

6

7

B

H

4000

4

4

4

5

5

5

5

5

6

7

7

B

H

5000

5

5

5

5

5

5

6

6

7

7

8

C

I

6000

5

5

5

6

6

6

6

7

7

8

9

C

I

7000

6

6

6

6

6

6

7

7

8

9

10

C

J

8000

6

6

6

6

7

7

7

8

8

9

A

D

J

9000

7

7

7

7

7

7

8

8

9

10

A

D

K

10000

7

7

7

7

7

8

8

9

10

10

A

D

K

11000

7

7

7

8

8

8

8

9

10

11

A

E

L

30000

12

12

12

12

13

13

14

15

N

O

P

S

V

31000

12

12

12

13

13

14

14

15

N

O

P

S

V

32000

12

12

13

13

13

14

14

M

N

O

P

S

V

33000

13

13

13

13

14

14

15

M

N

O

Q

S

W

34000

13

13

13

13

14

14

15

M

N

O

Q

S

W

35000

13

13

13

14

14

14

15

M

N

O

Q

T

W

36000

13

13

13

14

14

15

15

M

N

O

Q

T

X

37000

13

14

14

14

14

15

16

M

N

O

Q

T

X

38000

14

14

14

14

15

15

6

M

O

P

Q

T

X

39000

14

14

14

14

5

15

16

M

O

P

Q

T

Y

40000

14

14

14

15

15

15

16

M

O

P

R

U

Y

                                                               

 

 

 

TABLE     2

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

NORTH

SOUTH

A

B

C

D

E

F

G

H

I

J

K

L

M

1-Jan

2-Jul

12

9

12

14

16

6

9

12

15

17

19

20

17

15-Jan

17-Jul

12

9

11

13

15

6

8

11

14

16

18

18

17

1-Feb

4-Aug

11

8

10

12

14

5

7

10

12

14

15

16

16

15-Feb

19-Aug

11

8

9

11

13

5

6

9

11

13

14

15

16

1-Mar

3-Sep

10

7

9

11

12

4

6

8

10

12

13

14

15

15-Mar

17-Sep

10

7

9

11

12

4

6

8

10

12

13

14

15

1-Apr

4-Oct

10

7

9

11

12

4

6

8

10

12

13

14

15

15-Apr

18-Oct

11

8

9

11

13

4

6

9

11

13

14

15

16

1-May

3-Nov

11

8

10

12

14

5

7

10

12

14

16

17

16

15-May

16-Nov

12

9

11

14

15

6

8

11

14

16

18

19

17

1-Jun

2-Dec

13

10

12

15

17

7

10

13

16

19

22

23

17

15-Jun

16-Dec

13

10

13

16

18

7

10

14

17

21

23

26

18

1-Jul

1-Jan

13

10

13

16

17

7

10

14

17

21

23

25

18

15-Jul

13-Jan

12

9

12

15

16

6

9

12

16

18

21

22

17

1-Aug

29-Jan

12

9

11

13

15

5

8

10

13

16

18

18

17

15-Aug

11-Feb

11

8

10

12

13

5

7

9

12

14

15

16

16

1-Sep

27-Feb

10

7

9

11

12

4

6

9

11

12

14

15

16

15-Sep

12-Mar

10

7

9

11

12

4

6

8

10

12

13

14

15

1-Oct

29-Mar

10

7

9

11

12

4

6

8

10

12

13

14

15

15-Oct

12-Apr

10

7

9

11

12

4

6

8

10

12

13

14

15

1-Nov

29-Apr

11

8

10

12

13

5

7

9

11

13

15

15

16

15-Nov

14-May

11

8

10

13

14

5

7

10

12

14

16

17

16

1-Dec

30-May

12

9

11

14

15

6

8

11

14

16

18

19

17

15-Dec

14-Jun

12

9

12

16

6

9

12

15

17

19

20

17

 

 

 

TABLE 2 Contd.

NORTH

SOUTH

N

O

P

Q

R

S

T

U

V

W

X

Y

 

1-Jan

2-Jul

18

20

21

23

24

26

28

29

33

34

36

37

 

15-Jan

17-Jul

17

19

21

22

24

25

17

28

30

32

33

34

 

1-Feb

4-Aug

17

18

19

21

22

23

25

26

27

28

29

30

 

15-Feb

19-Aug

16

18

19

20

21

22

23

24

25

26

27

28

 

1-Mar

3-Sep

16

17

18

20

21

21

22

23

23

25

26

27

 

15-Mar

17-Sep

16

17

18

19

20

20

22

23

23

24

25

26

 

1-Apr

4-Oct

16

17

18

20

21

21

22

23

24

25

26

27

 

15-Apr

18-Oct

16

18

19

20

21

22

23

24

25

26

28

29

 

1-May

3-Nov

17

19

20

22

23

24

26

27

29

30

31

33

 

15-May

16-Nov

18

20

21

23

24

26

28

29

33

35

36

38

 

1-Jun

2-Dec

18

21

23

25

26

29

31

33

41

43

45

47

 

15-Jun

16-Dec

19

21

24

26

27

31

33

35

46

48

51

53

 

1-Jul

1-Jan

19

21

23

26

27

30

33

34

45

47

50

52

 

15-Jul

13-Jan

18

20

22

25

26

28

31

32

39

41

43

45

 

1-Aug

29-Jan

17

19

21

23

24

26

27

28

32

33

35

36

 

15-Aug

11-Feb

17

18

20

21

22

23

25

26

28

29

30

32

 

1-Sep

27-Feb

16

17

19

20

21

21

23

24

25

26

27

28

 

15-Sep

12-Mar

16

17

18

19

21

21

22

23

23

24

26

27

 

1-Oct

29-Mar

16

17

18

19

20

20

22

23

23

24

25

26

 

15-Oct

12-Apr

16

17

18

20

21

21

22

23

24

25

26

27

 

1-Nov

29-Apr

16

18

19

21

22

22

24

25

26

27

28

29

 

15-Nov

14-May

17

18

20

22

23

24

25

26

28

29

30

32

 

1-Dec

30-May

18

19

21

23

24

25

27

28

31

33

34

35

 

15-Dec

14-Jun

18

20

22

23

25

26

28

29

33

35

36

38

 

 

 

 

 

Example 1: Find the correction for a place at a height of 9000 feet located in a latitude of 40o N

 

In table 1 look under the column of 40 and the row of height 9000. The number is 9. Thus 9 minutes should be subtracted from the time of sunrise, Sehar and Fajar and added to the time of sunset, Maghrib and Isha.

 

Example 2: Find the difference for an aero plane flying at a height of 33000 feet at latitude of 50o on 15th May.

 

In table 1 the cell in column of 55o and row of 33000 contains the alphabet Q. Now in table 2 look in the column of Q and row of 15th May. The entry is 23. Thus sunrise, Sehar and Fajar are 23 minutes earlier and sunset, Maghrib and Isha are 23 minutes later.

 

 

 

 

 

 

 

 

 

 

CHAPTER 4

 

ASTRONOMY

 

4.1       Need and Importance of Astronomy

The study of positions, motions, sizes, distances etc. of heavenly bodies is called Astronomy. According to scholars it is desirable and good to study astronomy as many secrets of the universe are revealed and we recognize the greatness of Allah (s.w.t.). The Holy Quran, in various verses, directs us to ponder about the heavenly bodies. It becomes easier to understand and preach religious matters by the study of astronomy e.g. times of prayers, direction of Qibla etc.  

It must be noted that astrology is different from astronomy. Astrologers forecast the future with the help of stars. There is no room in Islam for this. It is entirely base less, haram and shirks. On the other hand astronomy is a formal branch of science and that studies with the help of mathematics. We appreciate, and recognize the greatness and power of Allah (s.w.t.) by studying it.

It depends on the intention by which knowledge is obtained. If the intention is good, then with the blessing of Allah (s.w.t.) the knowledge becomes a tool to understand and spread the message of Allah (s.w.t.) and the Quran.

The study of astronomy is good but to relate it with fortune telling is unislamic and leads to kufar.

Hazrat Ibrahim was born in a tribe which worshipped stars and idols. There were many idols in the temple of Namrood. Hazrat Ibrahim used a very simple logic to guide them to accept the presence of Allah (s.w.t.) as one and only one creator – Allah (s.w.t.) is immortal; He is Nourisher, cherisher and sustainer. Hazrat Ibrahim said to his people that since stars, the sun and the moon all set, so these are helpless useless and perishable things. The omni present is only Allah (s.w.t.) who is present since eternity and will always last. I do not recognize the perishable material as God the Creator and you should also do the same. Look at the sky. The innumerable galaxies, billions of stars, the sun, and the moon could not be created by themselves. There must be a creator and how powerful he must be.

 

سبحان الله وبحمده سبحان الله العظيم                         

 
Light year: Students of Physics and Astronomy know very well that light travels at a speed of 186,000 miles or 299,792 km per second. The distance traveled by light in one year is called a light year. A light year is 9 trillion 46 billion kilometers long. The diameter of our galaxy is 100,000 light years. The galaxy NGC 2207 in our cluster of galaxies is at a distance of 1 billion 141 million light years away. You can imagine the vastness of our universe and the greatness of Allah (s.w.t.) who created it. Although as compared to the vastness and expansion of the Universe and Cosmos our position is insignificant, but the entire Universe and each and every thing has been created for us. So we should think and decide what for we have been created and how long we are going to stay in this perishable and tiny world and what is our final destination where we will live forever and for ever after our worldly life.

 

 سبحان الله وبحمده سبحان الله العظيم                     

 

4.2       Solar System

The surface temperature of the sun is 5500o C. At the centre its temperature is 15,000,000o C. Its gravity is 27 times the gravity of the earth. There are thousands of galaxies containing billions of stars like the sun. In our galaxy there are about 5 billion stars.

There are 9 planets revolving around the sun. The nearest planet is Mercury. Other planets in order of their increasing distance from the sun are Venus, The earth, Mars, Jupiter, Saturn, Uranus, Neptune and Pluto.

The sun and all the bodies revolving around it due to its gravitation form the solar system. The sun is a hot star. Hydrogen gas is being converted in its centre into Helium gas creating atomic energy. The sun is 1.3 million times larger than the earth. The average distance between the earth and the sun is 150,000,000 km. All the planets revolve around the sun due to its attraction. There are about 44 satellites (moons) that revolve around planets. Thousands of asteroids and comets also revolve around the sun. All these objects form the solar system which in Urdu is called “Nizam e Shamsi”.

Life on planets: Recent research indicates that there is no possibility of life anywhere other than the earth. In some planets the atmosphere is too thin or too dense. Some planets are extremely cold while some are very hot e.g. on Mercury the temperature on the night side is – 289o F and on the sun lit side 801o. In some planets all life will freeze and on others it will be burned to ashes. Mars is the only planet on which some sort of life may exist. But nothing can be said with certainty. We do not know where and how many solar systems Allah (s.w.t.) has created in the universe.

Heat of the sun does not reach to the outer planets so extreme cold persists there. On Pluto temperature is always – 387o F. Thus the earth is the only planet on which life is possible. Allah (s.w.t.) sent the Holy Prophet (peace be upon him) here for the benefit of entire mankind.

Motions of the sun: It is our experience that when we travel in a train all the trees appear to us as running backwards. Actually the trees are not running but we are traveling forward. Similarly we observe that the sun is moving. But actually the earth is moving. Every one knows that the sun rises in the east, comes overhead and sets in the west causing day and night. According to astronomers day and night are not caused due to the motion of the sun but due to the rotation of the earth.

 

وَٱلشَّمۡسُ تَجۡرِى لِمُسۡتَقَرٍّ۬ لَّهَا‌ۚ ذَٲلِكَ تَقۡدِيرُ ٱلۡعَزِيزِ ٱلۡعَلِيمِ (٣٨ ) { یسٓ 36}

Translation: And the Sun runs his course for a period determined for him: that is the decree of (Him) the Exalted in Might, the All-Knowing. (38)

 

            The sun has three types of motions:

  1. Motion with the galaxy (The Milky Way)
  2. Its own motion inside the galaxy
  3. Rotation around its axis

 

Motion with galaxy: The galaxy in which our sun is located (the Milky Way) is rotating around its centre like a gigantic wheel. The sun is moving with it at a speed of 250 km/sec.

 

Motion inside Milky Way: All stars inside a galaxy are moving, so is the sun. Inside the Milky Way the sun is moving with a speed of 19 km/sec i.e. 68,400 km/hour.

 

Axial rotation: The sun is rotating around its axis as well completing one rotation in a period of 25.4 days.

It takes the sun 220 billion years to make one complete revolution around the centre of the galaxy. It is called a galactic year.

 

Motion of planets

The planets also have three types of motions.

 

  • Motion along with the sun around the galaxy and inside it.
  • Motion around the sun in elliptic orbits. The time taken by a planet to make one complete revolution around the sun is called its sidereal period or length of year for that planet. The speed with which they move around the sun is called orbital speed.
  • Rotation around their axes. The time taken by a planet to make on complete rotation on its axis is called the rotation period and the speed with which a point on its equator moves is called rotational speed.

 

Motions of the earth

 The earth also has three types of motions.

  • Motion around its axis (daily rotation of the earth
  • Motion with the sun around the galaxy with a speed of 250 km/sec.

·         Motion around the sun in elliptic orbit. The length of the orbit is 569,610,000 miles or 959,000,000 km. When it is nearest the sun, its distance is 91.5 million miles or 147.1 million kilometers. When the earth is farthest from the sun, the distance becomes 94.5 million miles or 152.1 million kilometers. There is summer on that part of the earth which is tilted towards the sun and winter on the other part.

Orbital speed: The earth is moving around the sun with a speed of 18.51 miles/sec or 29.79 km/sec which amounts to 66636 miles/hour or 107244 km/hour.

Solar year: The earth makes one complete revolution around the sun in 365 day 6 hours 9 minutes and 9.54 seconds. This is called a solar year. The earth is traveling with a speed of 18.5 miles/sec completing one revolution in about 365 days and 6 hours. After 4 years the 6 hour difference combines to form a day. So every fourth year is a leap year having 366 days.

 

3. Rotation around axis. The earth is almost a sphere rotating around its axis once in 24 hours causing day and night. At any given time the rays of the sun fall on half the earth where there is day. The other side, the night side, is dark. Each part of the earth gradually comes in front of the sun causing the day to begin and another part moves away from it causing night. The earth rotates through 360 degrees in 24 hours. Every part moves one degree in 4 minutes.

Rotating speed

A point on the earth at equator is moving at a speed of 17.29 miles/sec (27.82 km/sec) or 103756 miles/hour (166979 km/sec).

The plane in which the earth is moving around the sun is called ecliptic. It appears to us that the sun is moving around the earth in the ecliptic.

 

The sun (The centre of the solar system):

 

Average distance from the earth                      92.96 million miles

                                                                                149.6 million km.sec

Orbital speed                                                        250 km/sec

Rotation period                                                    25.04 earth days.

Distance from galactic centre                           30.000 light years.

Temperature at centre                                        15 million degrees C.

Temperature at surface                                      5500o C.

Volume                                                                  1,300,000 times the earth.

Time in which light travels to the earth           8 minutes 20 seconds.

Mass                                                                      330,000 times the earth.

Gases                                                                     75% Hydrogen,

                                                                                25% Helium.

Speed of light                                                       186,000 miles/sec.

Number of major planets                                  9.

 

4.3       Expanse of the Universe

Changes are continually taking place in the universe. Usually we decide the volume, area etc. of a body by its length, breadth and height. But for a star or a cluster of stars only its length, breadth and height are not sufficient. To measure the universe we have to consider the time along with these dimensions because whenever an event takes place in a star, we have to consider both space and time to describe it completely.

The universe is so vast that the usual units of length which we use on the earth are too small. We use the following two units to measure the distances in the universe:

1. Light Year

2. Parsec

A light year has been explained. A parsec is 3.6 light years long. The universe has been seen through telescopes up to 2 billion light years. The Universe is not static, it is continuously in motion. The galaxies are moving away from each other with very high speeds. Even if we make a telescope a thousand times larger then the 200 inch telescope, we will not be able to see to the extreme of the universe. It can be said that the universe is infinite. Its end has not yet been discovered. You can imagine the vastness of the universe. Our galaxy is 100,000 light years across. There are billions of such galaxies in the universe. Allah (s.w.t.) is great. His greatness is beyond our imagination.

 


Some astronomical terms

Stars: Stars are the heavenly bodies that emit their own light.

Planets: They do not emit their own light but reflect the light of the sun e.g. the earth, Mars, Saturn etc.

Moons: Bodies revolving around planets are called the moons or

Satellites: There is one moon around the earth. There is more than one moon around Mars, Jupiter, Saturn etc. All the moons are smaller than their parent planet.

Comets: It is a body which has a long tail. A comet has a nucleus and a very long tail.

Meteorites: They are small stony objects revolving around the sun. When a meteorite comes near the earth, it is attracted to the earth, falls towards it and starts burning in the atmosphere due to friction of the air. They emit a streak of light. A common person assumes that a star is falling. Mostly they are burnt in the atmosphere but a few larger one reach the surface of the earth. They are called meteoroids.

The Milky Way: The system of several billion stars of which the sun is also a member is called the Galaxy or the Milky Way. In clear night it is visible as a white band across the sky. Our galaxy is rotating around its centre completing one rotation in 200 billion years. There are billions of similar galaxies in the universe.

Sunspots: At some places on the surface of the sun the temperature become less than the surroundings. These parts look like dark black circles (spots) on the sun. They are called the sun spots. In size some of them are many times larger than the earth. Sometimes signal transmission on the earth is disturbed by them. They disturb the radio transmission. They also interfere with telegraph and television signals. They produce changes in weather and magnetic field of the earth as well.

Solar flares: Some parts of the sun suddenly increase in brightness up to 10 times the normal surface. This brightness spreads rapidly to several thousand miles. They are called solar flares. They also affect the transmission system on the earth.

Solar Prominences: The sun ejects hot gases with high velocities. The gases rise thousands of miles from the surface of the sun and then fall back forming a loop. They are called solar prominences. In 1947 a prominence erupted from the sun with a speed of 400,000 miles /hour and reached a height of 250,000 miles in about half an hour.

 

4.4       The Planets

The scale of the solar system can be imagined from the following model:

If the distance between the sun and Mercury be 30 feet, then Venus will be 55 feet, the earth 80 feet, Jupiter 400 feet, Saturn 740 feet, Uranus 1565 feet, Neptune 2330 feet and Pluto will be 3085 feet away. The diameter of the solar system is 7,400,000,000 miles.

Mercury: This planet is closest to the sun. It shows phases like the moon. It is the second smallest planet after Pluto. Its average distance from the sun is 36 million miles. Due to closeness to the sun the temperature on the side facing the sun is very high. Due to its small size, it does not have enough gravity to posses an atmosphere. Its diameter is 3100 miles. It completes one complete revolution around the sun in 88 days which is the length of its year. It completes one rotation around its axis in 58.6 days which is the length of the day on Mercury. Thus on Mercury there are 3 days in 2 years. Its orbital speed is 30 miles/sec. Its orbit is highly elliptic. Its maximum distance from the sun is 43 million miles and minimum distance 29 million miles. It is nearer to the sun than the earth, so is visible immediately after sunset as evening star or immediately before sunrise as a morning star. Its axis is perpendicular to its orbital plane so there are no seasons on Mercury. Temperature on day side rises up to 872o F and on night side falls down to -298oF. The day side is very hot and the night side is very cold.

There being no atmosphere, the meteorite fall on the surface. Mercury has more iron ratio than any other planet. According to mass it has 65% to 70% iron and according to volume 45%. Its core is made up of iron. The core is surrounded by 700 km of thick layer of rock. Its average density is about the density of the earth. It is the only planet where magnetic field exists though it is weaker than the earth’s magnetic field.

It shows phases. When nearer to the earth it looks like a crescent and when farthest its phase is full. It has no moon.

About Iron: In the Holy Qur'an, the last revealed book of Allah (s.w.t.), it is clearly mentioned that Iron was sent down. In other words, iron is not a material of the earth. It was dropped from the other heavenly body. The Qur’an is perfect and true. There is no ambiguity. This is a fact which is now proved by the modern scientists and research scholars- it is a fact.

Venus: It is the second planet of the solar system and our nearest neighbour planet. It is the brightest planet. It is also visible only as an evening or a morning star at sufficient altitude. It also shows phases. Its diameter is 7850 miles and average distance from the sun is 67 million miles. It completes one revolution around the sun in 225 days with a speed of 22 miles/sec. When it comes closest to the earth, it is said to be at inferior conjunction and when farthest at superior conjunction. A few days before inferior conjunction it becomes so bright that it casts shadows on the earth and it is possible to see it in day time near the sun.

The Earth: The earth is almost spherical and moves around the sun and around its own axis. If we travel in an aero plane to the west, we will reach USA, China, India and back to Pakistan. It is no longer unimaginable or unrealistic occurrence for us. At an average speed of modern aero planes it is about 50 hour’s journey. It was not possible for our ancestors a few hundred years ago to believe it.

The equatorial radius of the earth is 6378 km and the polar radius is 6357 km. It is not a complete sphere. It is a flattened near the poles. Its ellipticity is 1/297 { (6378 – 6357)/6378}. The earth is moving around the sun with an average speed of 29.8 km/sec (18.51 miles/sec). At least 11.2 km/sec speed is needed to escape from the gravity of the earth. The earth completes one rotation around its axis in 23 hours 56 minutes.

Mars: Mars and the remaining planets have their own orbits outside the orbit of the earth. They are called superior planets. All such planets have two special positions.

·         The sun comes in between the planet and the earth. The planet is behind the sun and is not visible. Its distance from the earth is maximum. The planet rises at day time and is always very close to the sun therefore it cannot be seen. This position is called superior conjunction.

·         The earth is in between the planet and the sun. The distance of the planet from the earth is minimum. When the sun sets, the planet rises; it is visible all night, transits at mid night and has maximum brightness. This position is called opposition.

 

Mars is the nearest superior planet. Its diameter is 4270 miles and average distance from the sun is 142 million miles. Its orbit is elliptic. Its minimum distance from the sun is 141.5 million miles and maximum distance 143.5 million miles. It comes closest to the earth (in opposition) after about every two years. Its minimum distance from the earth varies between 35 and 65 million miles due to elliptic orbit. At opposition sometimes it appears very bright (called favourable oppositions) and sometimes dimmer. Favourable oppositions occur after every 15 to 17 years in August or September. This planet is called red planet.

Its rotation period is 24.5 days. A day on Mars is 37 minutes longer than the day on the earth. It moves around the sun with a speed of 15 miles/sec completing one revolution in 687 days. It has a very rare atmosphere having a maximum height of 8 miles. Its surface has many craters. Ice caps have been observed in Polar Regions. Air, Oxygen and water are present in very small quantity. Human life is not possible on Mars.

Its equator is inclined to the ecliptic at an angle of 1.9o and its axis makes an angle 25.2o. Its atmosphere consists of a very thin layer of carbon dioxide having traces of Nitrogen, Oxygen, Argon and Xenon gases. Surface temperature varies between – 6o F to – 191o F. Water vapors in the atmosphere of Mars is one thousandth part of that on the earth. Even then, they form thin clouds and fog in the morning. The surface indicates that there was water on it in remote past. There are remains of lakes, rivers and falls. There are short lasting storm in its atmosphere.

The apparent angular diameter of Mars varies from 3.5 ` to 2.5` due to changes in distance from the earth. When it is nearest the earth, it is 55 times brighter than the pole star. Except Venus, no planet or star can compete with it.

It moves around the sun east wards. For about a year it appears to move east relative to stars. When its elongation becomes 137o it appears to stop. This is called stationary point. Then it starts moving backwards i.e. west wards called retrograde motion. At opposition retrograde motion becomes very rapid. Then it slows down, again becomes stationary and then starts moving east wards. It is due to the fact that orbital speed of Mars is less than that of the earth. All superior planets have stationary point and retrograde motions.

It also shows phases but its phase never becomes less than ½ i.e. it never becomes crescent.

The year of Mars is longer than that of the earth. So the lengths of seasons are also longer. Spring season is 191 days long, Summer 181 days, Autumn 149 and Winter season is 147 days long. Like the surface of the earth, the surface of Mars has mountains and volcanoes. The Martian mountains are as high as 20.18 miles. Its poles have a thin ice cap. So far no life has been discovered on Mars.

Mars has two moons. One is called Phobos. It is 6 km in diameter. Its distance form Mars is 5500 miles. It completes one revolution in 7 hours and 39 minutes. It rises in the west and sets in the east. The second moon is called Deimos. Its diameter is 3 km and completes a revolution in 30 hours 21 minutes.

Mass of Mars is 10.8% that of the earth and density 37.6% of the earth.

Jupiter: It is the largest planet in the solar system. It is 480 million miles from the sun even then it appears very bright due to its large size. It appears equally bright almost throughout the year. Despite its distance, it competes with Venus in brightness.  In telescope, clouds are visible in its atmosphere consisting mostly of Hydrogen gas. These are clouds of ammonia gas and methane and not of water vapors. This atmosphere is not suitable for any type of life. Some surface features including a red spot are visible through telescopes. Diameter of Jupiter is 89300 miles and it moves around the sun with a speed of 8 miles/sec completing one revolution in 12 years. It has 12 moons (more have been discovered by space ships. They are very small). In an ordinary telescope four of them are visible. The volume of Jupiter is 1300 times that of the earth and its mass is 318 times. Its density is one fourth compared to the density of the earth. It is the fifth planet in order of distance from the sun but first in order of size.

There is a large space between Mars and Jupiter. Some astronomers believe that there was once a planet in this region which was smashed to pieces for some unknown reasons. The pieces are rotating around the sun and are called asteroids. Some of them fall on the earth. It gets heated due to friction in the earths sphere, starts burning and appear as falling stars.

Diameter of Jupiter at equator is 142,984 km and at poles133, 875 km. In a telescope it appears flattened at the poles. The atmosphere of Jupiter consists of 89% hydrogen and 11% helium. Some other gases are also present in small quantities. In 100,000 parts there are 2000 parts of methane, 200 parts ammonia, 205 parts deuterium Isotope of hydrogen) and one part water vapors. In such unfriendly atmosphere the possibility of life is almost nil. Atmospheric pressure is 100 times that on the earth.

In a telescope, lines parallel to its equator are visible together with some other spots. The great red spot is very famous. It is 3 times larger than our earth and is an object of research for several years.

Saturn: It is the sixth planet of the solar system and second according to size. It was known since ancient times and was famous for its yellow color and slow motion among stars. It is perhaps the most beautiful object in the universe.

Three flat bright rings are rotating around its equator. Each of them consists of millions of particles and pieces of rocks, dust and ice. The atmosphere of this planet is very high. It is colder than Jupiter and possibility of life is very remote. There are 9 moons revolving around it. (More have been discovered by space ships. They are very small).

Its diameter is 75,000 miles and mean distance from the sun is 886 million miles. Moving with 6 miles/sec, it makes one revolution around the sun in 30 years. It also moves eastwards, stops, starts retrograde motion backwards (west wards), again stops and changes the direction of motion again. Due to its slow speed other planets keep overtaking it.

Volume of Saturn is 820 times the volume of the earth and mass is 95 times that of the earth. Its density is 1/8th density of the earth i.e. less than density of water. If a piece of Saturn is put in a vessel of water, it will float in it.

The width of the 3 rings is 40,000 miles but their thickness is not more than 10 miles. The rings appear very beautiful through telescope.

Saturn is the second largest planet in the solar system but it is smaller than Jupiter. Its equatorial diameter is 119980 km (74552 miles) and polar diameter 107982 km. (67097 miles). Like Jupiter it is also flattened at the poles. Its axis is inclined to its orbital plane at an angle of 26.75o. Its orbit makes an angle 2.5o with the ecliptic.

It rotates around its axis in 10 hours and 14 minutes near the equator. The period is less in higher latitudes. The earth is solid so it rotates with same speed at all points but Saturn is not solid so its rotational speed is not constant. The weight of a body on Saturn is 7% more than its weight on the earth.
Its albado is 0.5. Ten moons revolve around it (more have been discovered by space ships. They are very small). One of its moons, Titan, is almost twice as large as the earth’s moon. It completes one revolution around Saturn in 16 days. Astronomers believe that its atmospheric conditions on Titan resemble those of the earth in primitive stage.

Due to large distance of Saturn from the sun its temperature is very low.  Its surface temperature is – 179o C and atmospheric pressure is 60% more than that on the earth.

 

Axis of Saturn makes an angle 27o with its plane. Almost for 15 years we see the upper parts of the rings and for 15 years the lower part. Twice in 30 years the rings almost disappear as they appear only as a line. When the rings are wide, Saturn is the most beautiful object to observe with a telescope. It is called the prince of heavenly bodies. In 2002 the rings were wide open.

Initially three rings were known but the space ship Pioneer discovered four more in 1979. The newly discovered rings are so dim that they cannot be observed from the earth. The nearest D ring begins at a distance 66711 km from Saturn, B ring at 92000, C ring at a distance 64520 km, a ring at 122170, F ring at 140180 and G ring at 166000 km. The rings are not named according to their distances from Saturn but in order of their discovery. There are gaps in the rings visible in a telescope called Cassini’s divisions. If the photographs of the rings taken from space ships from close range are seen, it is observed that there are hundreds of rings. The classification in seven rings is a rough one.

Uranus: Uranus was discovered by William Hershel in 1781. Its diameter is 32600 miles and average distance from the sun is 178 million miles (287 million km.). Travelling with speed of 4 miles/sec, it completes one revolution around the sun in 84 years. It rotates around its axis once in 17.24 hours. Five moons revolve around it (more have been discovered by space ships. They are very small).

It is dimly visible to the naked eye. Early astronomers knew planets only up to Saturn. In astrology only planets up to Saturn are used. Uranus was the first planet to be discovered. Up to 1781, Uranus was regarded a star. In ancient Bermese book of astrology a planet Radho is mentioned along with sun, the moon, Mercury, Venus, Mars, Jupiter and Saturn. Perhaps it was Uranus. But Europeans, knowingly or unknowingly, have credited William Herschel with its discovery.

William Herschel was a musician in England and was interested in astronomy. He made a telescope with the help of his sister Caroline. When he was testing his telescope in 1781, he observed a star which looked different from others. He increased the magnification of his telescope and found that the star had become larger. It is known that stars become brighter but not larger in a telescope by increasing magnification. This object could be either a planet or a comet. Observing it continuously, he confirmed that it was a new planet. He named it Georgium Sidus on the name of his employer the king of England. Later in accordance with the policy of naming planets according to Greek Mythology, the name was changed to Uranus (in Greek mythology Uranus is the father of Saturn). William Herschel was given the title of Sir on this discovery.

Its equatorial diameter is 32600 mile (50791 km) and polar diameter is 31045 miles (48354 km) Its mass is 14.54 times the earth’s mass and density 30% that of the earth. Its axis makes an angle of 97.9o with its orbital plane. Thus it almost lies on its orbital plane. Its orbital plane is inclined to the ecliptic at an angle 0.77o.

Neptune: Mathematicians found that the orbit of Uranus was slightly different from the orbit calculated mathematically. They thought that some other planet was disturbing it. They calculated the orbit and position of the unknown planet. The planet Neptune was observed telescopically at the predicted position.

Its diameter is 30900 miles and average distance from the sun is 279 million miles. Eight moons revolve around it (more have been discovered by space ships. They are very small). It completes one rotation around its axis in 19 hours. Moving with a speed of 3 miles/sec, it completes one revolution around the sun in 165 years. Cloud formation can be seen on it.

Discovery of Neptune created a sensation in the history of astronomy. Mathematicians observed the discrepancies in the orbit of Uranus and using Newton’s law of gravity calculated the mass and position of an unknown planet causing it without seeing it. A young mathematician John Adam calculated the position and informed the Astronomer Royal and asked to look for the ninth magnitude object in constellation of Gemini. But the Astronomer Royal had no faith in a young mathematician. He neglected the information. At the same time a French mathematician also calculated the position and he also informed not only the Astronomer Royal but also the director of Berlin Observatory. The Astronomer Royal recalled Adam’s letter, noted that the position is the same and discovered the planet in the predicted position.

Equatorial diameter of Neptune is 48766 km and its volume is 5774 times that of the earth but its mass is only 17.147 times that of the earth. This is due to low density of Neptune which is 0.2976 times that of the earth. Its axis makes an angle 29.6o with its plane and the orbital plane makes an angle 1.77o with ecliptic.

Pluto: It was discovered in 1930. It has a diameter of 1413 miles. Its average distance from the sun is 370 million miles. Its orbital speed is 1.5 miles/sec. It makes one revolution around the sun in 250 years. It is the only planet whose orbital plane is vastly different from the rotational planes of other planets.

The existence of Neptune did not explain completely the discrepancies in orbit of Uranus. Mathematicians suspected another planet, calculated its mass and position. They calculated the position the ninth planet. But this time their predictions were wrong. Pluto was discovered but not exactly at the predicted position. The orbit of Neptune is also not exactly in accordance of calculations. Astronomers and mathematicians suspect that there is a tenth planet having a mass at least 5 times the mass of the earth. Let us see how far they are right this time.

The mass of the earth is 400 times that of Pluto. It rotates around its axis in 6 days. It has one moon. Its orbit is highly elliptic having eccentricity 0.248. It is thought that Pluto is the outer most planets. But its orbit intersects the orbit of Neptune. In 1979 it crossed the orbit and Pluto came closer to the sun than Neptune. In March 1999, it again crossed the orbit of Neptune to become the outer most planets.

Pluto appears as a star of magnitude 13.7. Its atmosphere consists of Nitrogen. There is 0.5% to 1.5% methane and some carbon dioxide. Its axis is tilted at an angle of 122o. Its distance from the sun is 40 times the distance of the earth from the sun. From Pluto the sun appears as a bright star. The size of the sun as seen from Pluto is 1/40th of the size of the full moon as seen from the earth. The sunlight on Pluto is 1/1500 times the sunlight on the earth.

If the mass of the earth is 1000 units, the mass of Pluto is about 3 units. It is a completely frozen world having a rocky core.

Comets/Meteors and asteroids

Comet:  The word comet is derived from Latin word cometa meaning long haired. Comets are not stars. They do not have their own light. They keep changing their positions relative to stars and move around the sun in highly elliptic orbits. Some times they come very close to the sun and at others move further away than Pluto. When they come nearer the sun their speed increases in accordance with Kepler’s law, and when they move away from the sun their speed decreases.

 

A comet has three parts:

  • Head 
  • Nucleus and
  • Tail.

Nucleus is the central part and consists of solid matter. It is surrounded by gases forming the head or coma. The tail is made up of gas and dust. It is millions of mile long and has a very low density. It is so rare that stars are visible through it. The tail always points away from the sun and becomes longer as the comet comes closer to the sun.

Asteroids or minor planets: These are thousand of rocky objects moving around the sun between the orbits of Mars and Jupiter. Their diameters vary from a few feet to a few miles. When an asteroid comes near the earth, it enters the earth’s atmosphere and starts burning due to the resistance of air. It is called a meter or a falling star, Shahabus- Saqib. If it reaches the earth it is called a meteorite.

Some famous stars:

Pole star: It is situated in the constellation of small bear (Ursa Minor). The constellation consists of 7 stars which form the shape of a bear. The pole star is at the tail of the small bear. In astronomy it is called Alpha Ursa minoris. The entire sky appears to rotate around it.

Opposite it is another constellation (Binatun- Nash) called Great Bear (Ursa Major). It also looks like a bear or a plough. Two of its stars called pointers always point towards the pole star.

Canopus: It is a bright star in the constellation of Carina. Carina begins from 53o S and extends further south. Canopus is visible from Karachi. Its right ascension is 6 hour 22.8 min. and declination is – 52o 40’. It is one of the brightest yellow stars. It is 650 years from us and is 80,000 times brighter than the sun. Its speed is + 13.5 miles/sec. The tribe Tai of Arab were the worshippers of Canopus.

 

Procyan: It is the brightest star in the constellation of Canis Minor (Small Dog). This constellation is visible in winter. It transits after mid night in mid January. The constellation Orion is east of it, Gemini in the north, Canis Major (Big Dog) in its south and Leo to its west.

 

Table of minimum and maximum distances of planets from the earth in km/miles

 

                        The moon                                                Saturn

Max.        407,000 (253,000)                  1,646,000,000 (1,023,000,000)

Min          357,000 (222,000)                  1,244,000,000 (773,000,000)

 

                                Mercury                                   Uranus

Max.        220,317,000 (136,900,000)    3,132,000,000 (1,946,000,000)

Min.         79,000,000 (49,100,000)        2,565,000,000 (1,594,000,000)

 

                                Venus                                      Neptune

Max.        259,000,000 (160,900,000)    4,652,580,000 (2,891,000,000)

Min.         39,750,000 (24,700,000)        4,271,000,000 (2,654,000,000)

 

                                Mars                                        Pluto

 

Max         397,500,000 (247,000,000)    7,251,500,000 (4,506,000,000).

Min.         55,000,000 (34,000,000)        4,192,300,000 (2,605,000,000)

                                Jupiter

Max         960,700,000 (597,000.000).

Min.         582,600,000 (362,000,000)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Table of Planetary Data   (from p 179 of book)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

4.5       Circles on the Celestial Sphere

            There are two types of circles on a sphere:

1. Great Circles: The circles whose planes pass through the centre of the sphere are called great circles. Every great circle divides the sphere in two equal parts. All meridians of longitude are great circles.

 

2. Small circles: Circles whose planes do not pass through the centre of the sphere are called small circles.

All great circles have the same centre, same radius and same circumference. But small circles do not have these properties. All parallel of latitudes and parallel of declinations except the equator are small circles.

A line through the centre of the circle perpendicular to its plane intersects the sphere in two points called the poles of the circle.

A great circle passing through the poles of another great circle is called secondary circle. A great circle and its secondary intersect at right angle.

 

 

                                                                C

 


                                             R                                      P

                                                               

                                                                                Q

 

                                  B                            O                             A

 

                                                                           E

 

 

 

 

                                                                 D

 

 

In the above figure AB is a great circle. C and D are its poles. CED is the secondary circle of AB. PQR is a small circle.

 

Some important great circles on Celestial Sphere which are used in calculation of prayer times and determination of direction of Qibla are given below:

1. Celestial Equator: The plane perpendicular to axis of rotation of the earth intersects the celestial sphere in a great circle called celestial equator. Its pole in the north hemisphere is called the North Pole and the one in the south hemisphere, the South Pole. When the sun is on the celestial equator lengths of days and night are equal. The North Pole is almost at the pole star. The celestial equator passes through the east and the west points. Its plane intersects the earth in a great circle called terrestrial equator. In the following figure AB is equator. N is the north pole, S the South Pole.

Diurnal circles: These are small circles parallel to celestial equator. All heavenly bodies appear to move on these small circles due to the earth’s rotation. PQ is a diurnal circle.

2. Ecliptic: The plane in which the sun appears to move around the earth intersects the celestial sphere in a great circle called the ecliptic. In the figure CD is the ecliptic.

The sun, the moon and planets move on or near the ecliptic. The ecliptic and celestial equator intersect at two points called equinoxes (E and F). The point E where the sun passes from the south to the north of the equator is called Vernal Equinox and the point F where the sun passes from the north to the south is called Autumnal equinox. The points where the sun is at maximum distance from equator are called solstices. C is the summer solstice and D is the winter solstice. The 12 zodiacal constellations are spread around the ecliptic.

Small circles parallel to the ecliptic are called parallels of celestial latitude. RS is a parallel of celestial latitude.

3. Four Polar Circle: The great circle passing through the four poles, two of ecliptic and two of equator is called Four Polar Circle. It is the circle ACBDP in the following figure. Its poles are the equinoxes. It is the secondary circle of both the ecliptic and the equator and intersects both at right angles.

The arc of the great circle between the ecliptic and the equator i.e. arc AC is called the obliquity of the ecliptic. Its present value is 23o 27’.

 

                                                     N

                                                                      R

 

                                                                                   C

                           S                      F                                    Ecliptic

                                                                                            Obliquity of

                        B                                                         A         ecliptic

                          D                         E

 

                                  Q                                           P

 

                                                       S

4. Horizon: The plane of horizon intersects the celestial equator in a great circle called observer’s horizon or simply horizon. One of its poles is exactly over the head of the observer called the zenith. The other pole is called Nadir. It divides the celestial sphere in two parts. All heavenly bodies above the horizon are visible to us and bodies below the horizon are hidden. The horizon intersects the celestial equator in the East and the West points.

If an observer stands on a level ground, the perpendicular to the ground through the head of the observer intersects the celestial sphere in Zenith. The other point of intersection below his feet is Nadir.

 

 

                     Arctic Circle

 

Right ascension and declination

To find the position of a heavenly body, we take a reference point and a reference circle on the celestial sphere and locate the body by means of distances from the point and the circle. Vernal equinox is taken as the reference point and celestial equator as reference circle.

Declination of a body is the arc measured along the meridian through the body from the equator to the body.

Right ascension is the arc length measured from Vernal equinox along the equator to the point where the meridian through the body intersects the equator. It is measured from 0o to 360o east or from 0 hour to 24 hours.

 

                                Z  (zenith)                                                               P (North Celestial Pole)

 

                                                                                             Star    *

                Diurnal Circle

                                                                                          Ecliptic

                                                Equator                    Equator

 

                                   Horizon                                                      A

                                                                       Vernal Equinox           Declination

 

                             Sun sets                                                           Right Asension

 

     Sun rises            N (Nadir)                                              Q (South C. Pole)

 

 

CHAPTER 5

 

Subahe sadiq and subahe kazib

                                                           

 

PHOTOGRAPH OF ZOIDIACAL LIGHT

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

5.1 Subahe Sadiq and Subahe Kazib

In all the following discussions and in the remaining book Subahe Sadiq will be referred to as dawn and Subah e Kazib as false dawn.

 

The Problem:  Signs of dawn have been described by our Holy Prophet (peace be upon him) in Ahadees e Nabvi. In this context let us discuss the following:

At what time azan (call for prayer) for Fajar prayer (following ancient charts) is given in Indo Pak sub continents for centuries?

What is the form and shape of the light on the horizon at dawn when azan e Fajar is given?

How far the light appearing at that time agrees with the signs of dawn?

  • What is the time that can be taken as dawn, the beginning of time of Fajar and end of Sehar?
  • What is false dawn? What is the difference between dawn and false dawn? What is the shape of light at false dawn?

 

                                                                                  

 

 

                                                                      Elongate tail like

                                                Reflected light of

                                                False dawn.                       Zodiacal light

 

                Observer

 

 

                                                               

                                                                               Sun more than 18o below

                                                                                                Horizon

 

 

                                                                                            

If we discuss the above questions critically in the light of observations, comments and explanations of scholars, it will be helpful in understanding and solving the problem. Answers to these questions are given in following pages.

Ancient Charts (Calendars) For Prayer Times and Dawn

In all charts and calendar used in Indo Pak, one thing is common. They take the time of dawn (beginning time for Fajar and end time of Sehar) when the centre of the sun is 18o below horizon.

In common man’s language, the time in ancient charts for dawn is the time when the centre of the sun is at a point below the horizon from where it has to travel another 18o in order to reach the horizon. At this time some light reaches the horizon by reflection.

This instant when the sun is 18o below horizon and its light spreads on the horizon by reflection in the atmosphere, is called the beginning of astronomical twilight. All recent and ancient astronomers take this instant as the beginning of day.

It is important to note that in the holy cities of Mecca and Medina, the payer charts in use also consider as the instant of beginning of astronomical twilight when the centre of the sun is 18o below horizon as beginning time for Fajar.

Ancient and recent astronomers have described the time of beginning of astronomical twilight as:

 

انحطاط الشمس تحت الأفق متى كان ثمانية عشر جزء

وكان ذالك وقت طلوع الفجر في المشرق                                                          Translation: The degeneration of the sun under the horizon when he was eighteen parts and that was the dawn time in the East.

                                                                                       

Abu Rehan Al Beruni Has Described This Time as Dawn

Famous astronomer and mathematician Al Beruni had 1000 years ago defined the instant when the sun is 18o below horizon as the beginning of day. In Encyclopedia Britannica it is clearly written that since the 11th century no one, despite their full efforts, has been able to alter the fact that the day begins when the sun is 18o below the horizon.

 

Astronomers have given special emphasis to the time when the sun is 18o below the horizon. They have described the light appearing on the eastern horizon at this instant as:

  • As soon as the centre of the sun reaches 18o below horizon, a light appears on the eastern horizon.
  • At that instant a light in the form of an arc or semi circular in shape spreads on the horizon after being reflected from the earth’s atmosphere.
  • There is a dim red tint in the light.
  • The light appearing at that instant continuously increases. The brightness of the light and the brightness in the region increases. The intensity of the light also increases without any fluctuation.
  • At this instant the light is and was never been in the form of a conical pillar or in the shape of a pyramid of Egypt nor like a tail or a rectangle.
  • This light is slightly reddish in color which increases continuously.
  • Internationally, this instant of 18o below horizon has been recognized as the time which separates day from the night. So “it is the instant or point of separation between day and night”.

5.2       Determination of Prayer Timings

             When we trace historical records we find that Muslims were the first who attempted to determine the timings of'    AI Fajru 'I Kadhib', &   Al  Fajru's Sadiq' , sunrise, sunset and mid-day timings etc., because it was their utmost need. The first " obligatory service “Salatul Fajr”  is performable from the appearance of the  'Subhe Sadiq' i.e., the 'True dawn' to which modern astronomers consider to be the time of the beginning of  ‘Astronomical Twilight'.

This is the time when the first signs of light, as has been described and explained in the Holy Qur’an and traditions of the Prophet, (peace be upon him), just begin to appear all along the eastern horizon. At this particular moment illumination appears just like a white thread on the eastern horizon, quite distinct from the black thread of the dark background of the night sky. This is the time when (at the most initial beginning time of astronomical twilight), indirect, diffracted and scattered light of the morning sun spreads on the eastern horizon. This illumination constantly increases without any break till sunrise.

Prayer timings

·         Although, the 'Salatul Fajr' can be offered up to the time of sunrise, it is, therefore, a must for Muslims to know and accurately determine the exact initial time  of Subhe-Sadiq. Moreover 'Sowm' (i.e., fasting particularly during the Holy Month of Ramadan) too, begins from the time of  ‘AI Fajrus Sadiq' and ends at the time of sunset. It also invited the immediate attention of Muslims to ascertain the timings of 'Subhe Sadiq', sunrise and sunset.

·         Similarly, for Salatu-Zuhr (afternoon prayer), which is also a mandatory prayer, it is necessary for Muslims to determine the time of Ephemeris Transit - i.e., the time of 'Zawal'  , when the sun reaches its zenith and when the shadow of any object is at its least This is also known as 'Saya-Asli' or the 'Real Shadow'. Prayers are forbidden at the time of Zawal. Since the time of Salatu-Zuhr begins after Zawal, the time of mid-day is also a matter of prime importance for Muslims to determine.

·         'Misl-e-Awal' is the time when the shadow of a stick or any object is equal to its size plus the length of the least shadow cast by it at the time of Zawal. This is the time of ASR.

·         As for 'Misl-e-Sani'  , it is the time when the shadow of the stick or any object is equal to double its size plus the least shadow cast at the time of Zawal (mid-day).

·         The Salatul Isha (night mandatory prayer) too, is offered when the reddishness of the evening twilight disappears. According to the Hanafi Maslak, the time of Isha prayer begins when all sorts of illumination of twilight (Both red and white Shafaq-e-Ahmer & Sha-faq-e-Abyed) disappears from the western horizon.

So we observe that all the mandatory and obligatory prayers are in some way or the other, related with the timings. This practice develops the habit of punctuality, regularity, and devotion and sub-mission to Allah Almighty.

            As for the time of' AI-Fajrus Sadiq', there is a necessity to accurately observe the commencement of 'Dawn' i.e., 'True Dawn' - 'Subhe, Sadiq' and distinguish with any other phenomena that may be mistaken for it.

Muslims gave different names to these different types of illuminations. In Arabic 'AI Fajrul Kadhib' or 'As-Subh-e-Kazib' is termed  'Zanabus Sirhan' - identical in meaning with 'Dum-e-Gurg'    of Persian. The Qamus explains it as wolf’s tail by its synonym the 'False Dawn'. The Turkish translation of the Qamus, however, is somewhat more explicit.

             It adds to 'Fajru Kazib', in explaining 'Zanabus Sirhan'  the gloss 'Shafq-e-MustateeI', the longish or tallish twilight. Under Fajr it explains: "...there are two dawns, one the false dawn, makes its appearance under a longish or tallish form, and what is termed the wolf's tail. The other shows itself later, and is spread along the horizon, when this takes place, he who is about to fast may no longer eat or drink lawfully". It is the 'True Dawn'.

Non Muslim Astronomer’s appreciation

In the recent past non Muslim astronomers admitted that - the Muslims and particularly the Arab Muslims were the first to recognize and distinguish between the two different types of illumination - one like a wolf’s tail   and the other like a white thread quite distinct from the black thread (streaks of light) that appears on the eastern horizon well before sunrise.

It was only in the beginning of the 17th century A.C., according to the Astronomical Treatise which teaches Europeans, that the illumination like a wolf’s tail - which appears on the eastern horizon in the morning was first observed by Cassini (in 1683) he first named it 'The Zodiacal Light'. It clearly shows how much and how early the phenomena of 'False Dawn' and 'True Dawn' interested the Muslims.         

Some times in 1877, a paper was presented before the members of the Royal Asiatic Society, wherein it was accepted that Muslims were the first who observed  the conical pyramid shaped light before the true dawn. In this paper a suggestion was also made that the natural phenomenon known to Muslims of every clime as “FALSE DAWN”    was no other than what is known in Europe by the name of “Zodiacal Light”. 

In the recent past, it was first observed by Kepler, who supposed it to be the solar atmosphere. Later it was described by Dominic Cassini, who gave it the name by which it is now (Astronomically) known, as 'Zodiacal light'. It is visible before sunrise and - after sunset immediately in the place where the Sun is about to appear or has just dropped below the horizon. It has a flat lanticular form extending from the horizon obliquely upwards, and following the course of the ecliptic or rather of the sun's equator. The most favorable time for observing it are in the months of April or May in the evening or at the opposite season of the year -. (October & November) before sunrise.

Muslim authors and eastern Lexicons make no mention of a 'wolfs tail' as seen at night after the evening twilight. This circumstance constitutes a difficulty in theoretically identifying the 'False Dawn' with the 'Zodiacal light’. But it may be partly explained by the fact that though Muslim astronomers and earth scientists were fully aware of it there was no mandatory prayer to be offered after the end or beginning of the conical shaped 'Zodiacal Light'.

Guidance through the Holy Qur’an

In the Holy Qur’an, for our guidance, it is clearly mentioned: (you are permitted to) eat and drink till the white thread (illumination of true dawn i.e., Subhe Sadiq in the form of white thread) and the black thread (i.e., the black streak of the night sky) is distinctly distinguished.

Muslims were fully familiar with these natural phenomena. Muslim scholars and astronomers, on the basis of their personal observations and findings contributed a number of articles on this issue. Since non-Muslim astronomers were not concerned with these phenomena, they never paid any attention to it.

Astronomical explanation of the term Twilight Definitions

This section describes several optical and celestial phenomena which may occur at, before, during or after twilight. Many of these can be seen all throughout the year, except for a few.  In this text, the phenomena are explained in the order they occur, particularly, during the Morning Twilight. For evening twilight, the order is of course reversed. Some phenomena (for example Zodiacal light  and Astronomical twilight occur predominantly in the morning, while others have a fair chance to be seen in the evening.

Before sunrise and again after sunset there are intervals of time, twilight, during which there is natural light provided by the upper atmosphere, which does receive direct sunlight and reflects parts of it towards the Earth's surface. Some outdoor activities may be conducted without artificial illumination during these intervals, and it is useful to have some means to set limits beyond which a certain activity should be assisted by artificial lighting.

The major determinants of the amount of natural light during twilight are the state of the atmosphere generally and local weather conditions in particular. Atmospheric conditions are best determined at the actual time and place of events. Nevertheless, it is possible to establish useful, though necessarily approximate, limits applicable to large classes of activities by considering only the position of the Sun below the local horizon. Reasonable and convenient definitions, therefore, have been evolved.

According to the General Astronomy there are three kinds of twilight:

 

·         civil twilight                        

·         nautical twilight                   

·         Astronomical twilight   

5.3       'AI Fajrus Sadiq'    

             It is defined to begin in the morning, and to end in the evening when the center of the Sun is geometrically 18 degrees below the horizon. That is, at the dark limit of astronomical twilight, the center of the Sun is geometrically 18 degrees below a horizontal plane. Before the beginning of astronomical twilight in the morning  and after the end of astronomical twilight in the evening the Sun does not contribute to sky illumination; for a considerable interval after the beginning of the morning twilight and before the end of the evening twilight, sky illumination is so faint that it is practically imperceptible.

When the sun reaches -18 degrees altitude (18 degrees below the horizon), astronomical twilight starts. This is (for middle latitudes like 30-50 degrees) usually, (but not always)   to the order of 90 to 75 minutes before sunrise. It varies from latitude to latitude and depends upon a number of factors including the atmospheric conditions.

At the time of beginning of Astronomical Twilight, you will note that the eastern horizon starts to glow faintly, and the zodiacal light merges into a bright white area on the horizon. 20 minutes later or so, you will notice that the developing twilight starts to show colors. It will get pale red at the horizon, and yellow just above it (very hard to detect at first).

When and where to observe it

It spreads all along the eastern horizon, and is followed by sunrise. There can be no mistake as to what this really is. It is the daybreak, the morning twilight with which the time of 'Sehr' & 'Tahajjud' ends and 'Salatul Fajr' begins.  This subject enjoyed sufficient importance with the Muslim astronomers and scientists, as the two phenomena helped in determining the times of some prayers and fasting.

Near the Equator, where the Sun appears and disappears at a steeper angle than it does in the mid latitudes or near the poles, the zodiacal light may be observed throughout the year.  Zodiacal light is sometimes referred to as the after glow of day or the false dawn. Under favorable conditions, the zodiacal light is as bright as the Milky Way, and it can be seen 30 to 40 degrees up from the horizon - about 1/3 of the way to the zenith.

In the morning when the sun is 18 degrees below the horizon direct sunlight cannot reach above the horizon. But sunlight as reflected and diffracted by the earth's atmospheric layers, illuminates places above the local horizon.

The instant when the solar depression angle (SDA) is 18 degrees has been chosen by astronomers as the time of the 'Beginning of Astronomical Twilight'. The instant of 18 degrees SDA is universally regarded as a point of separation between the completely dark background and discernable background illumination. It is thus generally accepted that in order to have a completely dark background the SDA must be at least 18 degrees. At the beginning of morning twilight SDA 18 degrees the entire horizon is illuminated with extremely faint reddish (almost white) light. It is distributed all along the eastern horizon, in a slightly semi-circular form of distribution rather than in a conical or rectangular form. It is also important to note that light intensity and reddishness constantly increases without any apparent change in the form of distribution

Findings of Muslim Scientists and Astronomers

We know that the greatest Muslim scientist and writer on optics Ibn-ul-Haitham determined that twilight begins or ceases when the sun is 19 degrees below the horizon. He also attempted to measure the height of the atmosphere.

Abu Rayhan Muhammad Bin Ahmad AI- Biruni (D.440 AH-I048 AD), some one thousand years ago, dealt with the subject in ‘Maoala Al-Biruni’.  He informs us that this phenomena occurred when the sun is 18 degrees below the horizon. He adds that "Some people determine it as 17 degrees. The former result corresponds exactly with the best modern researches." Evidently both the results are slightly different from Ibn-ul- Haitham's, findings and are based on independent researches.  We know that optics was one of AI-Biruni's favourite subjects in which he left some original and most remarkable researches.

It is' AI Fajrus-Sadiq' for which the word 'beginning of astronomical twilight' is used in nautical almanacs. I hereby suggest to all those who compute the prayers schedules or coin software for prayer timings, for any particular city or for the whole world, to consider the instant of 18 degrees SDA to be the right time of ‘AI Fjrus-Sadiq' as this 18 degrees SDA is universally regarded as the time when illumination spreads all along the eastern horizon, in the morning, resembling exactly in shape, form and Intensity to ‘Subhe - Sadiq'.

5.4       AI Fajrul Kadhib'

‘AI Fajrul Kadhib’ is in modern astronomy termed 'Zodiacal light'. It is also sunlight but it is reflected by interplanetary gas and dust (and not by the earth's atmosphere). 'Zodiacal light' in astronomy, is a faint nebulous aurora which surrounds the sun In the plane of Its equator, is somewhat whitish in colour and confined within the zodiacal belt around the ecliptic and thus lies streaming upwards. In favourable circumstances it is visible as a cone of light extending above the eastern horizon when the SDA is more than 18 degrees. It sometimes gives the impression of 'False Dawn'. Its shape looks like a wolf's tail or a pyramid. In the tropics where the ecliptic is nearly perpendicular to the horizon it may be seen after the end of twilight on every clear evening, and before the twilight on every clear morning, unless blotted out by the moon light. But as day approaches, however, matters are quite different. The 'Zodiacal light' is the reflection of the sun's rays in the sphere of inter-planetary dust and gases. It is narrow and tall like a tail. As the sun comes nearer to the eastern horizon in the morning, at 18 degrees SDA its light spreads all along the eastern horizon like a white thread. This is 'True Dawn' known as ‘AI Fajrus Sadiq'. A similar appearance is made in the evening in the west, when the sun is as far below the horizon as it was in the morning, when the false and true dawns appeared respectively.

Zodiacal light' was first observed by the Arab Muslims as a wolf’s tail - 'Zanabus-Sirhan'   to which they first gave the name 'False dawn or the ‘Al-Fajr-el Kazib’.

Sometimes in 1879, the Sultan of Zanzibar observed the phenomena and explained: “…..when I watched the light known as Fajrul Kadhib, it seemed to me very like the “Zodiacal Light” of the evening, rising in the east in a cone, and inclined considerably to the North. It was not so distinct as to allow me to measure its apex; but from what I saw, there is little doubt in identifying with the ‘Zodiacal Light’. There was no fading of this light as the ‘True Dawn’ - ‘Subhe Sadiq’ spread over the horizon; but it became lost in the rising light”.

When Twilight ends

Twilight does not really end until the Sun is 18 degrees below the horizon; this is called astronomical twilight. In some areas this happens about 90 minutes after sunset (or before sunrise) and its duration differs from place to place and from latitude to latitude. Only when astronomical twilight has ended, is the sky considered truly dark (assuming the Moon isn't above the horizon!)

After the end and beginning of astronomical twilight, at certain times of year in the right locations, a faint cone of light appears in the predawn sky for lucky viewers in dark locations. This eerie glow is the Zodiacal Light. It is best seen before daybreak, generally two to three hours before sunrise in the eastern sky. But it’s also visible in the west at certain times of the year.
            Over the centuries countless individuals have been fooled into thinking the Zodiacal Light was the first vestige of morning twilight. In fact, the Persian astronomer, mathematician and poet Omar Khayyam, who lived around the turn of the 12th Century, made reference to it as a "false dawn" in his one long poem, The
Rubaiyat-E-Omer Khayyam.

What it is

It was once thought to be solely an atmospheric phenomenon: perhaps reflected sunlight shining on the very high atmosphere of the Earth.

We now know, however, that while the phenomenon indeed involves reflected sunlight, it is being reflected not off our atmosphere, but rather off a non uniform distribution of space debris left over from the formation of the planets some 4.5 billion years ago.

These countless millions of particles -- ranging in size from meter-sized mini asteroids to micron-sized dust grains -- seem densest around the immediate vicinity of the Sun, but extend outward, beyond the orbit of Mars and are spread out along the plane of the ecliptic (the path the Sun follows throughout the year).

Inter planetary dust particles within the Zodiacal Belt:

The explanation for the zodiacal light is that meteoric dust particles (sub millimeter or micron size) found in the plane of the solar system scatter sunlight in such a way that it's faintly visible from Earth.

“This dust mainly comes from asteroids and comets that periodically drop off debris on their way around the Sun. Over the eons, thousands of comets have replenished the solar system with dust, most of which is concentrated along the plane of the solar system. The diffuse light scattered by the dust particles can only be seen during the evening or morning twilight”

 “Zodiacal light is more readily seen at those times of the year when the Sun rises or sets more abruptly - the spring and fall.”

“The smallest dust particles are blown out of the solar system by the sun’s radiation. The larger dust particles gradually spiral inwards towards the sun, and together form a flattened disc in the ecliptic plain in the inner part of the solar system. This disc of dust is composed of dust particles with sizes between 0.1 and 100 micrometer.”

From a dark secluded location, this disc of dust is visible from earth at night. A very faint band of light stretches over the sky following the path of the ecliptic ("Zodiak").

Hence the reason for the name "zodiacal"  light, is because it is usually seen projected against the zodiacal constellations, which were conjured by astronomers and poets to fit the ecliptic.

When to see it

The best time to see the Zodiacal Light is when the ecliptic appears most nearly vertical to your local horizon.

For those in the Northern Hemisphere, this occurs in the western evening sky after sunset from early February to late March. The best morning view in the eastern sky comes from late September into the early part of November. Conversely, for those who live in the Southern Hemisphere, the best view in the western evening sky comes after sunset from early August to late September, while the best morning view in the eastern sky comes from late March into the early part of May.

Those who live in the tropics or at the equator are the luckiest of all, since it has been said that the Zodiacal Light is bright and very conspicuous from these regions.

This is probably because the ecliptic is always favorably oriented there, allowing views of the Zodiacal Light both in the western evening sky and eastern morning sky all year long.

For its observation above 40 degrees latitudes the following conditions are absolutely necessary:

·         A very dark observing location

·         Dark horizon

·         Lacking light pollution,

·         A moonless night

·         Cloudless clear weather and sky

If you are interested to see and personally observe these phenomena in the morning, it is advisable to start your observations about 2 to 3 hours before sunrise. During the fall season (for people on the northern hemisphere), you will have a chance to see the (sometimes stunning) zodiacal light column rise steeply from the eastern horizon.

“There is some interval of time after the end of the zodiacal light and the beginning of astronomical twilight. There is no light on the horizon unless the centre of the sun reaches 18o below horizon.” Jawaid Qamar, Chairman, Observatory, University of Karachi.)

What it looks like

To the discerning eye, its diffuse shape resembles almost a tilted cone, wedge or slanted pyramid. At the base of the cone, the light may extend some 20 to 30 degrees along the horizon (a fist on your outstretched arm covers about 10 degrees of sky).

At its best, the display can approach or even equal the Milky Way in brightness, yet it is typically so faint that even a small amount of atmospheric haze can obscure it. On exceptionally clear nights, the tapering cone might be seen to stretch more than halfway to the zenith, an imaginary point in the sky directly overhead from wherever you are.

When the sun reaches -18 degrees altitude (18 degrees below the horizon), astronomical twilight starts. This is (for middle latitudes like 30-50 degrees) usually, (but not always)   to the order of 90 to 75 minutes before sunrise. It varies from latitude to latitude and depends upon a number of factors including the atmospheric conditions.

At the time of the beginning of the Astronomical Twilight, you will note that the eastern horizon starts to glow faintly, and the zodiacal light merges into a bright white area on the horizon.  20 minutes later or so, you will notice that the developing twilight starts to show colors. It will become pale red at the horizon, and yellow just above it (very hard to detect at first).

Types of Fajar

There are three types of Fajar.

i.        First, narrow vertical light called false dawn. It is  

Described as tail of a wolf. No prayer time, act or habit is associated with it.

ii.      Second type is the extended light in a semi circle form

along the eastern horizon which brightens the world. Animals and human wake up according to their habit and worship (ibadat) time is also associated with it.

iii.    Third type is the red light before sun rise. This is similar

to the first type in sharia.

 

Evening Twilight: Like morning twilight, evening twilights are also of three types but their order is opposite.

·         First type is reddish light immediately after sunset.

·         Second is spread white light. There is a dispute among modern Scientist and scholars as to which should be treated as evening twilight, (either Red or white twilight.(Both are subjects of discussion.

·         Third is the vertical light like the tail of a wolf. People are unaware of it due to their work and being at home at this time. In the morning when people wake up from their sleep they make preparations for their work, walk around to wait for the morning, so they observe it in the morning but not in the evening.

The following rules are devised for the morning and evening twilights as they are needed for prayers:

When the sun is 18o below horizon before raising it is dawn. As it cannot be mistaken from false dawn, some times it is taken as 17o. The time described by Abu Rehan Al Beruni, the astronomer and mathematician corresponding to 18o below horizon is certainly dawn. It is entirely wrong to consider it false dawn or not to consider it as dawn. If an ordinary person confuses it, it is tolerable but not for scholars.

Abu Rehan Al Beruni in his detailed discussion described the three types of Fajar. He emphasized that people’s daily and religious activities depend only on dawn. Since people depend on it, scholars have agreed to fix its time when the sun is 18o below horizon. On the other hand false dawn has nothing to do with daily or religious activities. Thus the time of that Fajar which is agreed on is the dawn when the sun is 18o below horizon.

5.5       Period between sunset and total darkness or between total darkness and sunrise

“Total darkness does not occur immediately when the sun sinks below the horizon because light from the sun that strikes the atmosphere is scattered (both by the air itself and by suspended matter, e.g., dust and smoke). Civil twilight ends when the center of the sun is 6° below the horizon. Although it is still not very dark, it is necessary to use artificial light to carry out most activities. Nautical twilight ends when the sun's center is 12° below the horizon; at about this time the light is too dim for the user of a sextant to see a sharp horizon. Astronomical twilight ends when the sun's center is 18° below the horizon; by this time even the faintest stars overhead can be seen. (Similar definitions apply to morning twilight.) During twilight, Venus or Mercury is often seen as the evening star or morning star. The length of twilight depends on latitude and the time of year. Twilight is generally shorter at the equator, where the sun's path towards the horizon is more vertical than at higher latitudes.”**

** The Columbia Encyclopedia, Fifth Edition, Columbia University Press. “

This is now becoming a debatable issue as to which twilight angle should be used in the calculation of Fajar/Isha. For a discussion on the subject refer to Dr. Ilyas’ book “Astronomy of Islamic Times for the Twenty-first Century”. Here is a brief extract from chapter five of this book.

            “In modern times astronomical twilight (18 degrees) has come to be widely used for the determination of Isha and Fajar times. As the average intensity curve of evening twilight indicates, the flux decreases to a minimum level, and thus it would seem appropriate that even for Islamic purposes, this should indicate a reasonable starting value for the end of ‘gastro-Islamic twilight’ (ATI). Indeed, 18 degree depression was a commonly used value for Fajar and Isha in the medieval period, when it must have been based on careful observations. Nevertheless, slight variations from this value- between 16 degrees and 20 degrees- were also used during the medieval period. According to King, 20 degrees and 16 degrees were the parameters used by Ibne Yunus for morning and evening AIT respectively, whereas 19 degrees and 17 degrees were the parameters used by various Egyptian Astronomers. Nasr also refers to 19 degrees being used in the Islamic world for the Fajar and Isha times. King has confirmed that although Muslim astronomers widely used 18 degrees/18 degrees symmetrical values or a slight variation to 19 degrees.17 degrees (morning/evening)-and in a few (earlier)cases even 20 degrees/16 degrees values were adopted- no record has been found of the use of a value as small as 15 degrees. This is of specific interest to us because a few years ago, values of 15 degrees/15 degrees for both AITs were proposed by Bagvi on the authority of Maulana Rashid Ahmed Ludianvi of Karachi, who is reported to have made observations personally. Indeed, I myself followed Bagvi in preparing the first South Australian Islamic Time Table, although I did consider the need to examine the matter very carefully and introduced a distinct term for it. Subsequently, this 15 degrees proposition has come under criticism and is apparently not proved by others’ observations made in recent years in that particular area (Karachi). Concern on this matter is obviously understandable, because an erroneous delay in the beginning of Fajar would have serious implications for the beginning of the fast. One of the useful studies arguing against this 15 degrees depression for AIT is that of Latiff, who claims to have conducted some observational work. Unfortunately Latiff has argued for a fixed 18 degrees/18 degrees case for all over the globe-no less and no more. This, it seems, may not be the true situation either as there seems to be room for geographical variability and perhaps 18 degrees serves as a good upper limit only. The value for morning AIT has widely been used as 18 degrees, although a practice of using 20 degrees prevails in Egypt and Indonesia/Malaysia (under Egyptian influence, apparently owing to the concerned persons having been trained there). Possibly, 20 degrees is taken as a safeguard because of the sanctification of the Fast. On the other hand, the use of smaller values than 18 degrees for India and Yemen has been reported to me in personal communications by Abdul Hafiz Manyar of Surat, India, and Dr. M. M. Quraishi of Islamabad, Pakistan, respectively. However, as we have noted elsewhere, in general, at 18 degrees depression, no detectable trace of twilight flux will be found, meaning that 18 degrees represents an upper limit.”

             Duration of Twilight

 

            Following is the summary of the observations and research of astronomers and scholars about zodiacal light:

 

·         Zodiacal light is triangular in shape

·         It is like a tail

·         Its shape resembles pyramids of Egypt or a rectangular

      tower

·         It has a white tint

·         It is spread near the horizon i.e. distributed over a large area but has a vertex at the top. It appears to climb up. It is a triangular shaped light.

·         It is such a bright light that it creates the impression of dawn.

·         In tropical regions zodiacal light can be observed throughout the year. The reason for its observation throughout the year in tropical regions is that the ecliptic is almost perpendicular to the horizon in these regions. It is especially visible before dawn in the autumn season.

            It has been proved spectroscopicaly that zodiacal light is not the light itself but it is sunlight reflected by gas and dust particles in the atmosphere.

A picture of zodiacal light taken from internet is given below. It is the false dawn producing such a bright light even before the beginning of astronomical twilight.

 

                                       

 

 

 

 

 

 

 

 

 

 

 

 

 

Picture page 186

 

5.6              Saying of Scholars of Ancient Past

Following are sayings of some scholars of ancient past:
Ibne Bashir Maliki says: It is the light of the sun and appears when the sun reaches near the horizon. When the eyes get used to it, it gives the impression that it disappears although it does not actually disappear.

Abash Ibrahim quotes some persons that this light disappears after appearing and it again becomes dark as night.

Abu Jaffer Al Basari describes it as:  two hours are left; this light appears up to quarter sky in a rectangular shape and is like a pillar. In summer when the atmosphere is polluted and dusty, this light does not appear. Its upper part is narrow and lower part is wide. Below it there is darkness. Behind it there is again light which is dominated and spreads. He contradicted it and said that he has been observing it for 50 years but never saw it disappeared. He further explained it: This light steps downwards and merges with the light which appears horizontally and all merge in the light of dawn.

            The concept that the light disappears and reappears again is either personal opinions or the changes in it due to seasons giving the deception of disappearance.

The sayings of scholars show that their observations and research have one thing in common that the light of the false dawn is exactly like the zodiacal light. They confirm that the false dawn and zodiacal lights are the two names of the same light.

In Tafseer of Alshqaq, Khalil bin Ahmed has quoted that I observed twilight (bayaz) from the tower of Alexandria and observed that it keeps moving from one horizon to another. I observed it to disappear. Ibne Abu Owais says that twilight is always present till dawn.

Mohasshi (interpreter) says that the observation of the author does not contradict that of Khalil because Khalil observed it from a high tower and the author saw it from the desert. If it disappears for some one on the ground, it is not necessary that it should also disappear to a person observing from a height because there is a difference in altitude of the two observers.

Imam Zelee in his book “Tabbyanul Haqayaq” says that the person observing the sun from the tower of Alexandria will see as if it disappears later than the person who is observing it on the ground. The discussion shows that the stated byaz (twilight) remains on the sky up to dawn and if it disappears for some observer, it does not actually disappear.

Now let us consider what present astronomers say about it. When Royal Greenwich Observatory was contacted, they sent a few pages of a book with their answer. It is stated: when the sun is 19 or 20 degrees below horizon it appears that the part of pyramidal zodiacal light near the eastern horizon has extended further. The extension increases the brightness of the light. When the sun reaches 17 or 18 degrees, the light of astronomical twilight appears clearly.

It can be inferred that the zodiacal light that appeared at 20o or further below horizon remains present till the astronomical twilight appears at 18o. In other words the zodiacal light does not disappear but its base extends and merges with twilight.

            A Professor of the Institute of Astronomy, Cambridge University, has written “…that the light appearing as twilight at 18o depression continuously rises above the horizon. If the atmosphere is polluted, it will be reddish and if the atmosphere is clear and observed from a height it will be pale yellow like the sun.”

 


5.7       An Invitation to Think and Ponder

The times for fasting, Eid and prayers described by the Holy Prophet (P.B.U.H) depend only on visibility of the moon and observations. He (peace be upon him) described such simple, easy and definite criteria which can be used by every one. There was no problem to identify the times of dawn and false dawn. There is still no problem today. Recent research has shown that the course taken by ancients was correct and the tables of prayer times prepared by them were accurate. There is no doubt about it.

People used to find the times of dawn and false dawn by their personal experience. Not only religious people and scholars were expert in recognizing the dawn and times but elder people of the villages were also well versed with it. These aged simple people used to recognize the time of dawn by their observations and on their directive azan e Fajar was given in the mosques. With azan e Fajar, sehar time ends. In those days there were no bright electric lights which cause hindrance and interference in conducting observations. There were no prayer charts in every village. Time of sehar used to end with azan e Fajar given at the instructions of these elderly people.

Even today the villagers stop sehar on hearing Azaan e Fajar . These simple people, even when they settle in cities continue to stop sehar on hearing azan e Fajar as a habit. They regard it appropriate. Charts and calendars of prayer and Ramzan times are used for years in the Subcontinent. Our ancestors have been using them. The learned elders had prepared the tables for their regions for the benefit of common Muslims. These elders were very careful, serious, pious and sensible about it. They were far better Muslims than us. It can not be imagined that they would have prepared the charts without continued observations, serious thought and confirmation. If someone was to say that they were not serious and cautious, it would be a base less allegation against them.

Offering prayers is obligatory and so is the knowledge of their correct time. It will be a serious allegation to say that these people did not prepare the charts without proper care, research and observations. These charts have been in practice since a long time. It cannot even be thought that they prepared the charts irresponsibly and did not take proper care in testing and verifying the times. They were more determined, careful, dedicated than us. These charts are accurate and there is no room for doubting them. If anyone has any doubt that wrong times of dawn etc. were compiled and listed, he may contact any of the following national or international agencies for their satisfaction and confirmation of charts and tables.

  • International, local or overseas Astronomical Research Centres.
  • Local or overseas meteorological offices.
  • Specialists and navigators of Navy or Air force.
  • Astronomy Department of any University or expert astronomers.
  • Royal Astronomical Observatory of Greenwich.

 

Confirm from the above sources and/or satisfy yourself by your personal observations that:

  • As soon as the sun reaches 18o below horizon a horizontal light appears on the eastern horizon and day begins.
  • The horizon remains dark until the sun reaches 18o below horizon. This instant is the limit between day and night.
  • The light appearing at this instant keeps increasing without any fluctuation. Neither it disappears after appearing nor does it become dark again.
  • This light spreads horizontally on the entire eastern horizon and keeps spreading in neighbouring parts of the sky.
  • At that time there is no question of any light appearing on the eastern horizon in the shape of an elongated tail like or conical or pyramidal or rectangular or pillar like form. (This has been proved not only by recent and ancient research but also by observations.)
  • This light is not purely white but it has a slightly dim imperceptible reddish tint which gradually increases.
  • A semi circular light appears on the eastern horizon at this instant and it spreads rapidly.
  • On the other hand the zodiacal light has a conical shape or the shape of a wolf’s tail, pyramid or rectangular like a pillar.
  • It disappears and merges with the light of dawn as the sun reaches 18o below horizon.
  • Zodiacal light is also the sun’s light which appears before the beginning of the morning twilight under suitable conditions.
  • Zodiacal light has white tint and is so bright and clear that it gives the deception of dawn.
  • Zodiacal light is the light that appears at night before dawn. It has exactly the same shape as described for false dawn. It gives the deception of dawn.
  • It is misleading to think that the horizontally spread light appears on the horizon only when the sun reaches 15o below the horizon and that it is preceded by a long pointed light.
  • It is surely misleading and against research and observation to say that the reddish tint appears in the light only when the sun reaches 15o below horizon.
  • It is certainly wrong that the semi circular light appears only when the sun reaches 15o below horizon.

Despite the fact that zodiacal light is pointed, tail like, conical and exactly in accordance with the signs described for false dawn, it is wrong to think that it has nothing to do with the code of shariat.  It can be confirmed that this is the light which gives the deception of dawn in the darkness of the night. Its light is several times brighter than the light of a galaxy.

After considering the sayings of scholars, it cannot be denied that dawn begins when the sun reaches 18o below the horizon and that zodiacal light is false dawn.

 

5.8       A Misconception Regarding the Interval between Dawn and Sunrise

Usually people know that it takes the sun 4 minutes to travel one degree but do not consider the direction in which it travels. Is it along latitude or longitude? It is to be remembered that it takes 4 minutes for the sun to travel 1o for every longitude but not for latitude. If the sun crosses 1o latitude perpendicular to it, then it will take 4 minutes but the more obliquely it crosses, the longer it takes. Mostly the sun moves along latitudes obliquely. Thus it is wrong to consider that since the sun has to travel 18o between dawn and sunrise, it will always take 18 x 4 = 72 minutes. Thus it is wrong to think that there is always an interval of 1 hour and 12 minutes between dawn (subah e sadiq) and sunrise. This is simply due to ignorance. Similarly since the angular difference between white and red twilights is 3o it is wrong to think that it always lasts for 3 x 4 = 12 minutes. It is without any doubt incorrect to think and against the reality.

If the sun travels 18o in 1 hour and 12 minutes at the equator, it will travel the same distance in several hours in Britain in summer which lies between 51o N to 58o N latitudes. This example is enough to illustrate the statement.

Thus if the sun travels 18o in 72 minutes at a place, it is wrong to consider that it will travel between the same distance at all places and in all seasons and will take the same time. Similarly it is wrong to say that there are always 12 minutes difference between white and red twilights.

Thus it is clear that the sun does not travel between two latitudes in equal times.

5.9       Time Difference Due to Altitude

Altitude correction factor is very important. There is a difference in times of sunrise, dawn, and sunset due to height and curvature of the earth. Because of height the time of sun rise and dawn are several minutes earlier and the time of sunset is later. So we have to consider the height of the place for calculation of payer times and times for Ramzan (particularly the time of sunset).

The following table shows the time which has to be subtracted from the time of dawn, astronomical twilight and sunrise and to be added to the time of sunset.

 

Table showing the difference to be subtracted from the time of subha sadiq.

 

            Height (feet)       Time

            50                    35 seconds

            100                  50 seconds

200                  1 min. 10 sec.

500                  1 min. 50 sec.

1000                2 min. 36 sec.

2000                3 min. 40 sec.

5000                5 min. 48 sec.

 


A mistake in time difference in Jantaries (calendars)

In payer charts and jantaris, it is noted that the difference of time is sometimes written in margins for various cities and places. But it is not taken into account whether they are on the same latitude or not. The times of prayers of the same date are different for different latitudes. For example if in the jantary of one city the time difference is written for another city, it is observed that on the same date the time difference between dawn is different from that of transit which also differs from that of the sunset. Thus the stated difference is wrong and misleading.

The following facts should be noted:

  • The difference in time of transit is due to the difference in longitude only.
  • The difference in other times, dawn, sunrise, sunset etc. depend on difference of longitude as well as latitude.
  • The lengths of day at different places on different latitudes are also different.

Considering these difficulties, if the difference is written for a given day for all cities located on the same latitude, it will be good for all places. The only difference will be due to the change in longitude. Without keeping in view the latitude of different places, if the time difference is noted on the margins of prayer timetables, it will be misleading.

 

Example: In the timetable published of Lahore the difference for Karachi is written as +27 minutes.

Comparing the chart of Lahore prepared by late Maulana Karim Bakhsh (Professor Arabic, Government college Lahore) and chart for Karachi by Maulana Qari Shareef Ahmed, we observe the following difference in times.( All times are in minutes):

 


Difference of time for Karachi from the prayer’s table of Lahore

 

1st Jan.    1st April      1st July     1st Sept.

Dawn         17           32               53             31

Sun rise      15           33               44             27

Transit       15           12              18               12

Sunset        44           27              15               31

Isha            45           27              10               31

 

The above table is given only for 1st of January, April, July and September. It illustrates that writing the 27 minute difference is not sufficient. It would have been better to write the differences for places located on the same latitude so that tables can be used with confidence.

 

Example 2: If it is desirable to write the differences without considering the latitude, then the differences should be written at intervals of five days as Prof. Abdul Wasey has done in the chart of Hydrabad (Deccan) for use in Aurangabad having different latitude.

 

The difference of Aurangabad from Hydrabad (Deccan):

 

Date       Dawn    Sunrise   Zohar     Asar    Sunset    End of Twilight

1st Jan.      +16       +17         +13         +4           +8           +9

10th  June +16       +8           +13         +16         +17         +19

 

The difference for Aurangabad is not written as a single entry but date wise difference is given due to the change of latitude.

 

An important point to note: The Meteorological Department prepares charts in the month of Ramazan every year for sehar and iftar times. In these charts the locality Jacobabad is taken as the centre of Karachi for the calculations of times. Karachi is a vast city. One side of it extends to Hub Chauki and Somiani touching Baluchistan and the other side extends to Landi, Korangi and Pipri. The time differences in the eastern and the western parts vary from ± 1 – 2 to ± 1 – 3 minutes from the centre Jacobabad. Due to this small difference, it is necessary to prepare separate charts for eastern and the western parts but the residents of near by regions e.g. Thatta, Sajawal, Tandu Muhammad Khan, Hydrabad, Gaddap, Pasni, Turbat etc. should not use these charts of Karachi. Necessary corrections must be applied. Many cities of Pakistan which were once very small have how largely expanded e.g. Lahore, Multan, Faisalabad, Gujranwala etc. In these cities similar care should be taken.

 

5.10     Nautical Almanac, Astronomical Ephemeris and Non Muslim Astronomers

Non Muslim astronomers have benefited from the work, experience and research of Muslim astronomers but they do not care to acknowledge it. They could not deviate from the laws and principles derived by the expert Abu Rehan Al Beruni. For example without referring to dawn and false dawn the western astronomers after their research on twilight remarked “ Despite all efforts and observations since 11th century no one is able to alter the fact that the day begins when the sun reaches 18o below horizon. (Encyclopedia Britannica, Vol 22 p. 637).

Among books of astronomy, Nautical Almanac and Astronomical Ephemeris are the two books of the west in which they publish astronomical data. They publish the data after updating it every year. In it the starting time of astronomical twilight are tabulated for every day for various north and south latitudes. Tables are given below.  These times are in fact the times of dawn for these latitudes because astronomical twilight and dawn are the names of the same instant. Similarly the times listed for the end of the evening twilight for various latitudes are the times for the beginning of Isha. When the sun reaches 18o below the horizon after setting, the night begins and evening twilight ends. This is the beginning time of Isha.

The times of the beginning of morning and end of evening twilight are available for all latitudes. Taking into consideration the standard and local times of the place, the times of dawn and Isha can be calculated. These books also publish data about declination of the sun, motion of the moon and other astronomical bodies. The times of sunset and sunrise are also given. The times when the centre of the sun is 18o, 12o and 6o below horizon before rising and after setting are also given. These are called astronomical. Nautical and civil twilights.

5.11     Further Discussion about Dawn and False Dawn

1. When the sun reaches 15o below horizon, illumination of light expands so much on the ground and the horizon that even a person even with weak eyesight can feel that it is daytime. When the sun is at 18o and dawn breaks out, it is the time when dark and white lines can be distinguished. This instant of dawn can be recognized only by an experienced eye. After it the intensity of light brightens and when the sun reaches 15o every one can say that the day has broken out.

2. Arrangements for observing dawn were made. Scholars of Jamia Al Uloom Islamia, Binori Town and Darul Uloom, Korangi themselves conducted observations and were satisfied that dawn begins when the sun is 18o below horizon. (The details of observation and conclusions can be seen in the book “Subah e Sadiq WA Subah e Kazib” **).

 

** “Subhe Sadiq and Subahe Kazib”, Latif, A., 1982

3. If we search “zodiacal light” on the internet, we get 1100 sites where articles and essays by experts are available. They have clearly stated that before the sun reaches 18o below horizon in the morning, a light appears on the horizon having the shape of a wolf’s tail, triangular and conical. Several articles have been published which can be seen on internet. This light is false dawn.

4. Before sunrise, when the sun reaches 18o below horizon, it is called the beginning of astronomical twilight. This is the time of dawn, the day breaks from night, and the light continuously increases. The light spreads horizontally on the eastern horizon. If we look towards the east the light spreads left and right. At this instant the light is neither conical nor of the shape of a wolf’s. tail. You are advised to search on “Google” ”Astronomical Twilight”. You will find at least 2000 sites containing articles by experts of astronomy. You will also find many photographs. It is clearly written that this light appears on the eastern horizon when the sun reaches 18o below the horizon. It spreads horizontally. Before it, zodiacal light appears which is called false dawn. There is no doubt that zodiacal light is conical in shape and is exactly like false dawn.

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

CHAPTER 6

 

Phases and sighting of the moon

 

Phases of the Moon

 

 

 

6.1  The Moon

The paths (orbits) of the moon and the sun are different. If they were the same, we could never see the moon during day light. You may have observed that sometimes during the day the moon is visible along with the sun. When we see the moon for Ramzan or Eid, first the sun sets on the western horizon and then the moon. So it is a decided fact that the moon will be only visible when it sets after the sunset. . Thus on the first of a lunar month the sun sets earlier than the moon. On that day we see the moon before it sets. On the second day the moon sets later. On the 14th of a lunar month, the sun sets in the west and at the same time the moon rises in the east.

Physically there are troughs and crests on the moon. There are many mountains, hills, several miles wide large craters, cracks and holes. When the sun light falls on the moon, it looks bright and beautiful. All its beauty is due to the sun. Actually the surface of the moon is rougher than the surface of the earth.

Our Holy Prophet (P.B.U.H) divided the moon in two parts by pointing towards it with His finger. The signs of this event known as Shaqqul Qamar still exist on the moon. A straight crack is visible in photographs of the surface of the moon. This straight crack is the witness that it cannot be due to the moon quake, but because it was divided in two parts. There is an island near Africa called Jazeera tul Qamar. The westerners have deformed and renamed it to Comoros Island. This island is near Mozambique. A large number of Muslims live there. It is conjectured that it was named Jazeera tul Qamar because its inhabitants saw the moon breaking in two parts. They were the witness to this miracle. Shaqqul Qamar was also witnessed by the ruler of the south Indian state Malabar who got it confirmed by sailors and tourists. It is said that he accepted Islam.

There is neither air nor water on the moon. Thus there are no traces of life there. If two people speak on the moon, they will see their lips moving but will not hear any sound because there is no air to transmit the sound. Due to the absence of air we cannot talk on the moon.

 

Physical data of the moon

  • Average distance between the earth and the moon = 384,365 km (238,840 miles).
  • Diameter of the moon =  3476 km. (2160 miles)
  • The earth’s diameter   = 12,745 km. (7926 miles)
  • Density of the moon   = 3.3 times that of water.
  • Density of the earth    = 5.5 times that of water.
  • Sidereal period around the earth = 27.3 days (approx.)
  • Synodic period (new moon to new moon) = 29.5 days (approximately)

Motions of the Moon

            The moon has three types of motions all from the west to the east.

1. Motion with the earth

2. Revolution around the earth

3. Rotation around its axis

 

1. Motion with the earth: The earth is moving around the sun. The moon also moves with it. The time in which the earth completes one revolution around the sun is called its orbital period.

2. Revolution around the earth:  The moon moves around the earth in an elliptic orbit. The time in which it completes one revolution around the earth is called a lunar month.

3. Rotation around its axis

 

 

 

 

 

Lunar months:  There are two types of lunar months.

  • Sidereal Month. When the moon returns to the same point of its orbit after making one revolution, it is called Sidereal Month. Its length is 27 days 7 hours 43 minutes and 11.5 seconds.
  • Syndic month. It is the interval between two new moons. Its duration is 29 days 12 hours 44 minutes 2.9 seconds. This is the religious month. It is 2 days 5 hours 51.4 seconds longer than the sidereal month.

Reason for its difference: The moon returns to the same point of its orbit after 27.32 days. But during this time the earth has moved considerable further in its orbit around the sun. The moon takes another 2.2 days to face the earth. Thus the religious month becomes 29.53 days in length.

The moon moves 51 minutes (on the average) east every day i.e. if the moon passes a star at 10 O’clock, the next day it will pass it at 10:51. The same average delay of 51 minutes occurs in the moon set and the moon rise. If the moon has risen today at 7 pm, tomorrow it will rise at 7:51 pm.

Length of lunar year

When the moon makes 12 complete revolutions around the earth a lunar year has elapsed. Thus a lunar year is 12 synodic months long i.e. 354 days and 8 hours approximately. A lunar year is 10 days 21 hours 20 minutes 35.46 seconds shorter than solar year. This is the reason that lunar months keep moving in solar year. Every three years it moves one month backwards. After 33 years 198.22 days the lunar year will again come back on the same dates.  For example if Ramzan begins in January this year after 33 years 198.22 days, it will again begin in January.

            The lunar months are:

1. Muharram                            2. Safar

3. Rabi ul Awwal                    4. Rabi us Sani

5. Jamadi ul Awwal                6. Jamadi us Sani

7. Rajab                                   8. Shaban

9. Ramzan                               10. Shawwal

11. Ziqad                                 12. Zilhaj

Longitudinal motion of the moon: Out of 360 degrees of longitude the moon travels 12.19o daily and in 29.53 days completes 360o to make one complete revolution around the earth. Thus the moon travels one degree of longitude in 1.96 hours.

Delay in the moonrise

In its monthly motion the moon moves towards the east, so it rises 48.76 minutes late every day. Due to elliptic orbit this time varies, but the average time is 48.76 minutes i.e. 48 minutes and 45 seconds.

  • The average distance between the earth and moon is 384,000 km.
  • The length of the moon’s orbit is 3,060,000 km. long
  • The moon is traveling in its orbit with a speed of 1 km/sec completing one revolution around the earth in 27.5 days.
  • The moon is revolving around the earth from the west to the east.

6.2    Phases of the moon

The moon does not have its own light. It appears bright due to reflected sun light. If it had its own light, it would always appear as a full moon. Half of the moon faces the sun and this face is bright. The other half is dark. Half of the moon always faces us and the other half is hidden from us. It can never be seen from the earth as the rotation and revolution periods of the moon are equal. When the entire bright portion faces us, it is full moon. If half the bright portion is visible, it is called quadrature. There are various phases relative to quadrature.

            Let us first consider what scientific information about the moon is provided to us by experts. Astronomers keep record of the data about the moon for every second. Especially the following information is monitored continuously:

 

  • What is the path of the moon i.e. from which parts will it pass today?
  • What will be the altitude of the moon i.e. what will be its height above horizon?
  • What will be the distance of the moon?
  • What will be the strength of its magnetic field?
  • What will be its elongation?
  • What will be the lamination towards the earth?
  • What will be the time of moon rise and moon set at any given place?
  • What will be the time of first visibility of the moon?
  • In which part of the world will it be sighted first?

 

All types of information can be obtained at any time from astronomical observatories or meteorological offices. We can use this information and judge the witness about sighting of the moon in the light of this information.

Web based resources for probability of moon sighting

A program   “Accurate Times” written by Mohammad Odeh of Jordon (a member of Jordanian Astronomical Society – JAS) is available from the

Web site: http://www.jas.org/software/index.html#

 

This software calculates the Islamic prayer times, the Qiblah direction and the Hijri – Gregorian date conversion. This program runs under MS – Windows. The program also use the NAO Technical Note 69 for providing information on moon’s earliest possible visibility and the position of moon (Lunar position), in the sky at any instance.

Since it is a tested program, it is advisable to visit this web site for satisfaction and calculating the most probable date of visibility of moon for beginning of Ramdhan and Eid etc.

            Prof. Dr. Triq Munier of Edinburgh UK contributions “Our Solar System and its position within the universe and a program for computation of Islamic Pray Times” his contribution is remarkable.

            A visual basic program for obtaining prayers times for the entire year is available. (Visit his web site: http://www.jas.org.jo/munir)

            Dr. Mohammad Ilyas from Malaysia is providing Maximum material on the topic of possibilities of moon sighting. He introduced IIDL – (that is- International Lunar Date Line) and drawn circles along the latitudes to show the probability of visibility of moon that decreases to the east of IILD and increases to the west of IILD as shown in the following figure.

Sharaie Ruet E Hilal (Islamic moon sighting)

Islam is a religion for the entire humanity. A large population of Muslims live in villages, mountains and islands. It is difficult to acquaint all of them with mathematical calculations. So Islam has made sighting by eye as a base instead of calculations. Its use is possible by every literate or illiterate person.

There is only one way of sighting the moon, seeing it with the eye. The Holy Prophet (P.B.U.H) said:

 

 ‏عن‏ ‏عبد الله بن عمر ‏ ‏رضي الله عنهما                          

‏أن رسول الله ‏ ‏صلى الله عليه وسلم ‏ ‏ذكر رمضان فقال

 ‏ ‏لا تصوموا حتى تروا الهلال ولا تفطروا حتى تروه فإن ‏ ‏غم ‏ ‏عليكم فاقدروا له       Narrated Abdullah bin Umar (RA):
Allah's Apostle mentioned Ramadan and said, "Do not fast unless you see the crescent (of Ramadan), and do not give up fasting till you see the crescent (of Shawwal), but if the sky is overcast (if you cannot see it), then act on estimation (i.e. count Sha'ban as 30 days).

Another saying emphasizes completing 30 days by calculation. Its words are:

 

فإن ‏غم ‏عليكم فأكملوا العدة ثلاثين                                     .

Translation: And if the sky is overcast, then complete Sha'ban as thirty days.

 

Note: Along with hadith we have to consider the intention of the Holy Prophet (P.B.U.H).

 

In Islam it is not prohibited to get help from astronomical calculations regarding the sighting of the moon. But it is wrong and against the will of the Holy Prophet (peace be on Him) to make the decision on its basis. If calculations are in favour of the visibility but the moon is not seen by any eye for any reason, then it is not right to trust and decide on the basis of mathematical calculations.

 

6.3       Use of Modern Instruments for the Sighting of the Moon

Abstract from “Ruet e Hilal” by Hazrat Maulana Mufti Muhammad Shafi. (Explanations of Hazrat Maulana Mufti Muhammad Shafi expressed in the magazine “Ruet e Hilal” are presented below so that it may become clear that the religious scholars and Mufti Sahebaan do not regard the use of scientific and technical instruments improper)

 

The difference of opinion in this regard is the reason that some people think that since it is possible to ascertain the position of the moon in the sky with the help of instruments and calculations, so why not use them for sighting so that there is no need to see by any eye or any witnesses for sighting. Further why not believe the news of the radio, television and wireless as the entire world depends on them for every matter.

 

6.3    View Of Islam About Scientific Inventions

All instruments prepared by science, modern or ancient, are blessings of Allah (s.w.t.) and should be used thankfully. To discard and dislike them is neither an act of religion nor wisdom. However both religion and common sense require that they must not be used for disobedience of Allah (s.w.t.) and at wrong places and for improper purposes. There is no hindrance in their use where any religious principle is not violated.

It is stated in the Holy Quran

 

هُوَ ٱلَّذِى خَلَقَ لَكُم مَّا فِى ٱلۡأَرۡضِ جَمِيعً۬ا  (٢٩){البَقَرَة 2}             

Translation: It is He Who hath created for you all things that are on earth.

        

The purpose of science, modern or ancient, is to make use of the things created by Allah (s.w.t.). Science does not create anything, it only teaches the use of things created by Allah (s.w.t.).

As the new discoveries and invention are needed in the world, Allah (s.w.t.) teaches the people of that time new methods to use them. In ancient times every region was self sufficient in their requirements, the members of a family were not distributed in different countries, so there was no need for speedy vehicles, radio, wireless, telephone, telegraph etc. But when countries started depending on one another, members of a family dispersed to different countries, the problem of communication aroused and Allah (s.w.t.) guided people to invent necessary audio video techniques. He guided them to use petrol for vehicles like motor cars, aero planes etc. This was also forecasted in the Holy Quran. After referring to vehicles driven by horses, camels, donkeys etc. used in those days it is stated

 

وَيَخۡلُقُ مَا لَا تَعۡلَمُونَ (٨) {النّحل 16}                                 

Translation: And He creates (other) things of which you have no knowledge (8)

 

If names of motor cars, aero planes etc. were mentioned in that place, the people of that time would not understand them and would become confused. So instead on naming them, it was simply said that various types of vehicles will appear. When vehicles to reach the moon are invented, they are also included in it. Thus inventions of science are also blessings of Allah (s.w.t.) and should be used thankfully.

However, Islam restricts that these inventions may not be used for disobedience and improper and sinful deeds by which principles of Islam are violated. This is why when guns, cannons, tanks and different types of bombs were invented; no scholar or pseudo scholars even thought that their use in modern war is a sin. When aero planes flew, Muslims used them freely not only for their worldly but even for their religious needs.. Similarly wireless, telephones, telegraphs, radios; loudspeakers were used extensively for religious and worldly affairs. Scholars took care to restrict their use to the extent that it does not violate any principle of Quran or Sunnah (shariah). No scholar prohibited loudspeakers to be used for azan, khutba, speech etc. The only dispute was about its use during prayer. This was due to debatable and conflicting opinions of scientists. Some scientists described the voice coming from a loudspeaker as the actual voice of the person using it and some described it as an artificial voice created by machine. This dispute continues even today. Decision is not due to ignorance, like or dislike about modern inventions but as a matter of principle. All scholars undisputedly agree to believe in the news on recent media as far as news is concerned. But when there is a need to provide witness, no court in the world accepts it unless the witness is present personally.

It is therefore wrong to say that the scholars reject the recent inventions due to their ignorance, but when they appear as reality, they are compelled to use them. It is possible that there may be some doubts about a new invention due to incomplete information about it, but when the doubts are cleared and removed and it is proved that they do not conflict with religious principles it is considered permissible. It is not correct to blame or accuse them for waiting initially and then permitting it.

It is not correct to consider them fools; instead it is an indication of their openheartedness and wisdom to accept the truth.

No one has any objection in using new inventions in sighting the moon to the extent that it does not violate any Islamic principle. It is necessary, before any discussion, to study the Islamic principles with open mind and then decide whether the use of instruments violates it or not.

Eid and Eid ul Azha are not our festivals but occasions of worship. First of all it should be clearly understood that whether it is fasting or Eid or Eid ul Azha, they are not festivals in the sense of the rest of the world. These are the occasions of our worships. The purpose of worship is the obedience and submission to the will of Allah (s.w.t.). The commandants of Allah (s.w.t.) are to be obeyed without any hesitation or opinion. All conditions and restrictions for any worship have to be followed by the same rule. For example why are there five prayers daily why not more or less? Why they have to be performed at their prescribed times why not at any other time? If prayer is offered whole heartedly and with full faith at any other time, why are they not advisable? Why 2 rakats in Fajar, 4 in Zohar and 3 in Maghrib? What if some one offers 5 or 6 rakats?

The only answer to all these questions is that it is the will of Allah (s.w.t.) and worshipping is obeying Him unconditionally. It is not permissible and proper to make any increase or decrease or change the time. Similarly fasting is to be done from dawn to sunset. What is the sin if some one fasts up to Isha? What if some one fasts for 31 days instead of 29 or 30? Why is it not acceptable to fast in any month other than Ramzan? Why is it wrong to fast for 30 days even if the moon is sighted on 29th, or to fast for 29 days even if the moon is not visible? Only the acts performed according to the will and instruction of Allah (s.w.t.) are fit to be called worships. If human opinion is used in it, it is not worship.

Similarly if it is disputed that the moon is sighted on 29th or not, it can not be resolved by the opinion or votes. Its solution has to be found in the teachings of Allah (s.w.t.) and the Holy Prophet (peace be upon him) because rising or setting of the moon or the sun is not the basis of our worships, but our worship depends on fulfilling orders of Allah (s.w.t.). Practically it will not affect the duration of fast if sehri and iftar are taken five minutes later than prescribed times to such an extent that all the effort of the entire day is declared null and void. However if a person performs iftar five minutes before sun set, he has committed a great blunder and his fast is nullified.

The problem is not the presence of the moon but its sighting and witness (shahadat).

 

First of all it is necessary to find the criteria of sharia whether it is enough for the moon to be above the horizon or its sighting is necessary by normal human eye.

Every literate person knows that the moon is never non existent. It is always present at some point of its orbit and can be seen even on 28th, 29th, or 30th of a month by telescopes which block the sun light from high altitudes. If the problem were only the existence of the moon, condition for 29 or 30 would be irrelevant. Thus the sharai requirement is not for the moon to be above the horizon but its sighting by normal human eye. Not only Ramzan and Eid but thousands of other matter of Islamic Sharaia depend on it. It also affects marriage, divorce, iddat etc. If Islamic calendar is used as in Saudi Arabia, it also affects the beginning of dates on which working of offices and all institutions depend. It can not be applicable and permissible on any day like a ceremony or a festival.

It is thus clear that sighting or non sighting of the moon on 29th is not a casual matter like a festival or a national ceremony, but it is the end of a worship and beginning of another. For example 29th Ramzan means that fast and other worships of Ramzan have ended and worship of Eid has started, months of Hajj have started which affects many ahkam e shariah.

It should be understood what is meant by sighting or not sighting of the moon according to Quran and Holy Prophet ((peace be upon him) Is the presence of the moon above the horizon enough according to Sharaia or sighting by a human eye will decide it i.e. is the presence of the moon enough for Ramzan and Eid or is sighting and witness is needed. To decide it look at the quotation of the Holy Prophet ((peace be upon him). Shih Bukhari is a well known book of hadith which is credible second only to the holy Qur’an. In it the Holy Prophet (peace be upon him) is quoted:

 

عن‏ ‏عبد الله بن عمر ‏ ‏رضي الله عنهما ‏                                            
‏أن رسول الله ‏ ‏صلى الله عليه وسلم ‏ ‏ذكر رمضان فقال ‏ ‏لا تصوموا حتى تروا الهلال ولا تفطروا حتى تروه فإن ‏ ‏غم ‏ ‏عليكم فاقدروا له                              .

Narrated Abdullah bin Umar (RA):

Allah's Apostle mentioned Ramadan and said, "Do not fast unless you see the crescent (of Ramadan), and do not give up fasting till you see the crescent (of Shawwal), but if the sky is overcast (if you cannot see it), then act on estimation (i.e. count Sha'ban as 30 days).

Another hadith says:

‏عن ‏عبد الله بن عمر ‏ ‏رضي الله عنهما
‏أن رسول الله ‏ ‏صلى الله عليه وسلم ‏ ‏قال ‏ ‏الشهر تسع وعشرون ليلة فلا تصوموا حتى تروه فإن ‏ ‏غم ‏ ‏عليكم فأكملوا العدة ثلاثين
.

Narrated Abdullah bin Umar (RA):

Allah's Apostle said, "The month (can be) 29 nights (i.e. days), and do not fast till you see the moon, and if the sky is overcast, then complete Sha'ban as thirty days."

Both these Ahadith are present in all other books of Ahadith. No scholar has disputed them. In both, the basis of fasting and Eid is on sighting of the moon. The word “Ruet” is an Arabic word and it means seeing by eye. Any other meaning assigned to it is not real but virtual. The gist of the quotation of the Holy Prophet ((peace be upon him) is that all matter depending on the moon depend on sighting of the moon by normal eye. Thus the criteria is not presence of the moon above horizon but sighting of the moon. If the moon is present above the horizon but is not sighted due to any reason, then its presence cannot be relied upon.

 

The meaning of the hadith has been further clarified by the last phrase which says that if the moon is hidden from you then complete 30 days. It is not said that in this case find the birth and presence of the moon by calculations and follow it, or see it by telescope or other astronomical instruments but said that

فإن ‏غم ‏عليكم فأكملوا العدة ثلاثين                                               .


Translation: And if the sky is overcast, then complete Sha'ban as thirty days.


            i.e. if the moon is hidden, then complete 30 days of the month. The word “Ghummah” needs special attention. Its literary meaning in Arabic dictionary (Qamoos) is hidden from the eye.

It is said at a time when cloud or some other object hinders the view and the moon cannot be seen. Thus the Holy Prophet ((peace be upon him) has ordered it by accepting the presence of the moon, only on its sighting by the eye, because for something to be hidden its presence is necessary. If something is not present it cannot be called hidden. It is also clear that there may be several reasons for the moon being hidden. Whatever the reason, if it is hidden from the eye and is not visible, then Sharaia instruction is that fasting and Eid can not be celebrated.

It is further confirmed by another hadith of Sahi Muslim. It is stated that some Sahabah left for Umrah. They saw the moon during their journey. Observing its large size they discussed it. Some said it is the moon of 2nd, some said it is of 3rd. Hazrat Abdullah bin Abbas asked them when they saw it first. It was informed that it was seen on such and such night. Ibne Abbas said:

“The Holy Prophet) peace be upon him) has emphasized the sighting of the moon, therefore it should be regarded the moon of the night in which it was sighted.”

 

From this it is clear that the problem is not the presence of the moon but sighting it by the common eye. To see the hidden moon with a telescope or to see it from an aero plane flying over the clouds is not a replacement of sighting. The problem of seeing an object has nothing to do with science or meteorological department or astronomy. If a person claims to see an object at a particular time and a particular place and others say that they were also present there at that time and did not see it, then the decision does not lie with meteorological department or astronomy or mathematicians. The judgement can be given in Islamic states by Qazi (jurist) and in others by a Muslim judge. He will examine the witnesses and give the decision. If the problem is only of its presence then it is not a matter of a Qazi (jurist) or Muslim judge, it has to be decided by an astronomer. If a judge or a Qazi (jurist) has to give a decision, he can and will seek the advice of astronomers too.

 

6.5       New Moon Conjunction

The moon is revolving around the earth. Every lunar month, there is a position in its orbit when the moon comes in between the earth and the sun i.e. all the three bodies come in a straight line. There is no fixed time for this event every month. Sometimes it occurs at midday, some times 3 O’clock at night. Experts can calculate the time of each month, but the time of its conjunction is different in different months. This instant when they are in the same line is called new moon or conjunction. At this instant the dark side of the moon is towards the earth and the bright side towards the sun. So it is in no way possible to see the crescent at this time because the crescent has not yet been born. Astronomers regard this instant as the beginning of a lunar month. But the Islamic lunar month begins with sighting. The crescent is visible 20 to 22 hours after the birth of the new moon.

 

Existence of the moon

After the birth of the new moon, there can be the following possibilities:

·         The moon sets before the sunset

·         First the sun sets and then the moon

·         Both set together

 

On the first of a lunar month if the moon remains above the horizon even for one minute (whether visible or not), the astronomers call it existence or presence of the moon. Many Arab countries that use the lunar calendar in their business and government work use the existence of the moon to prepare their calendars and use it to regulate their official business and work and trade. But according to Islamic principles the lunar date does not begin with the new moon of this nature.

We have nothing to do with the existence of the moon. For example if on 29th Ramzan the sky is cloudy, the moon is neither visible nor is there any possibility of its being seen, then we are advised to complete 30 fasts and do not celebrate Eid despite the existence of the moon. The calendars prepared on this basis are wrong. If an Arab country prepares a lunar calendar or gets it prepared by an expert on the basis of existence of the moon and announces the beginning of Ramzan or Eid on its basis, we should reject their claim. But if the moon is sighted in an Arab country and they declare its visibility it should be accepted by the inhabitants of their locality.

 

(Abstract from  “ Ruete Hila ka Masla Asre Hazir ke Wasayal aur Taraqqiyat ki Roshni Men” by Hazrat Maulana Burhanuddin Sambhali, Sadar, Shoba e Hadees Shareef, Darul Uloom Nidwat ul Ulma, Lukhnow.

            According to principles and observations of Astronomy, every month the moon comes in a line with the sun for some time (called conjunction). It is impossible to see it at that instant. Gradually it moves away. After about 17 to 20 hours, it becomes possible that the moon may be visible. When the moon just moves away from conjunction, it is called new moon or birth of the moon. Islamic shariah also agree with it. (e.g. see the famous book of Fiqah Hanafi  (Shami Vol 1, p289).

It has been proved by observations that the moon is sight able at least 17 hours (usually 20 to 22 hours) after the new moon (not a single contradiction has been reported for several years.). Obviously it can be seen only after it is sightable not before it.

He further writes: The famous sharah of the most credible hadith book Bukhari, Hafiz Ibne Hajar has written the following important point to ponder:

In this hadith of the Holy Prophet (peace be upon him) it has been ordered to complete 30 days in case of non sighting of the moon. It has not been said to consult mathematicians. The wisdom is that to begin the next month by completing 30 days is easy for every one (on the other hand not many people know mathematics). Thus there will be no dispute.

The point of view of scholars about the beginning of a new lunar month is by sighting with the eye and not by mathematical calculations. Hafiz Ibne Hajar has also, with reference to Allama Baji has quoted the consensus of previous religious scholars.

 

From the above discussion it becomes very clear that the beginning of month does not depend on calculations or instruments but only on sighting of the moon by the human eye. It is not enough for the moon to be present on the horizon. It is also clear that the new moon found by calculations or instruments does not fulfill the share (Islamic principles and laws) requirements.

Chances of sighting: The moon can never be sighted at the birth of the moon. If the moon moves about 12o away from the sun about 7% of its bright portion faces us and is sufficiently away from bright rays of the sun. If the weather is clear and the atmosphere is not polluted, the chances of visibility become stronger i.e. the moon can be seen by the human eye. This time is called “Possible sighting time”. The sharai Islamic new moon begins at this instant. Fast, Eids and other religious occasions depend on this crescent.

There are three important conditions for the sighting of the moon.

 

1. Elongation of the moon. The elongation of the moon should be at least 12o for sighting then it is possible.

2. Altitude of the moon.

3. The moon should have moved sufficiently away from the sun so that its sufficient bright part faces the earth.

 

                        Moon

 

 

 

 

 

 

 

 

 

 

                                 Elongation

              Horizon                                   12o                  Observer

 

       Sun

 

 

 

 

Maulana Sameeruddin from UK has listed the data available at Royal Greenwich Observatory, London for minimum times when the moon was sighted.

 

  • When observed with a telescope, it was found that when elongation of the moon becomes 6.87 and its age 13.47 hours i.e. 13 hours and 28 minutes, it was visible through binoculars not by naked eye.
  • After seeing it with binoculars, it was then seen with naked eye when its elongation became 8.1o and age 15.53 days i.e. its age was 15 hours and 32 minutes. It was visible to the naked eye with great difficulty and was seen very rarely.
  • Usually the moon is visible at elongation 10o. All the three old books of astronomy

“Attasreeh p 52, Sharah e Chaghmani  p 90 and the famous book Al Qanun al Masoodi part 2 p 952” agree that

 

 The crescent is visible when the moon is 12o from the sun and its age is 23 hours 31 minutes.

 

Opinion of experienced observers

Experienced observers are of the opinion that if the age of the moon is about 18 hours and the weather is clear then shahadat (witness) of sighting can be accepted without much investigation.

Sighting is common (by a good number of observers) in clear weather when age is greater than 25 hours. The shahadat of sighting before the age is 17 hours is not trustable.

 


Altitude

The second condition for sighting is that the moon should be sufficiently high above the horizon to be seen. Even if the elongation of the moon is 30o but the moon sets before the sun or at sunset its height above the horizon is very small, the thin crescent cannot be seen. Thus for six months when the moon is in the south, it sets before the sun in  abnormal regions as its altitude is very low. For this reason the crescent is not visible in those regions for several days.

 

Useful facts

  • Altitude of the moon should be 10o for sighting.
  • The moon cannot be seen immediately after sunset due to bright light and red twilight (shafaq e ahmer) in the atmosphere.
  • After sunset when the sun has moved 5o below horizon (about 15 to 20 minutes) and the Sun light has become dim and at that time the moon is at least 5o above horizon, the crescent can be seen.

 

 

Moon

 

 

 

 


                                                                                       Horizon

                Earth                 100

                                               

 

 

                        

                                                                                Sun

 

Conjunction:  When the sun, the moon and the earth come together in the same line, it is called conjunction. As soon as the moon moves away, it is called new moon by astronomers. It can take place at any time during the day or night. Sighting of the moon on 1st of a lunar month is different from the birth of the new moon. The situation at conjunction is given below.

 

 

        Earth                        Moon                                              Sun

 

 

 

 


.

SIGHTING OF THE MOON a unique question

– From the author’s article Published in “Saudi Gazette”:

 

            The day is not too far when some Muslim, after reaching on the moon may ask us from the MOON:

            …O ! You Gentleman, the dweller of the tiny world ..Please let me know have you sighted the new moon so that I may start Fasting”

            My dear Muslim brothers: ….With the rapid advancement of modern day technology we should now keep ourselves ready to answer such questions and to face such situations. There is no doubt that the solution of every problem is available in the Holy Qur’an and Ahadees-e-Nabwi Sharif. It is for us to recite, learn, understand, practice and preach to others the teachings of Holy Qur’an and the way of Prophet Mohammad (Sallaho-alyhe-wa-sallam). May ALLAH Almighty give us Taufiq and Hidayah to do so.   Aameen. 

(Abstracts from my article - published in the Saudi Gazette Jeddah, KSA – Monday August 1986 in its Hajj Edition)

 

6.6 Gregorian Calendar and Its Roots

Unfortunately we condemn our lunar calendar and are satisfied with the solar calendar hanging on the wall. We find it very simple to see the date in it although the innocent looking calendar hanging on the wall has several defects.

 

How many of us know the name of the calendar hanging on the wall and why is it named so. From where this Gregorian calendar had come? We have to relate thousands of years old history of it so that its defects can be brought forward.

Do you know that this Gregorian calendar based on the sun’s annual motion changes every year? It becomes obsolete and every year a new calendar has to be printed.

  • It does not divide the year in equal number of days.
  • In a leap year the number of days is even.
  • In these years the 366 days can be divided in two halves of 183 days.
  • In normal years 365 days cannot be divided in 2 equal halves.
  • Neither can the year be divided in 4 equal parts.
  • 365 or 366 days can not be divided in equal number of weeks of 7 days.

Thus this calendar is deprived of several useful properties.

In 46 BC the Roman king Julius Caesar modified the Roman calendar by increasing a day in February every fourth year. In 13th century a defect in Julian calendar founded by ancient Romans was detected. When the calendar was founded, the period of revolution of the earth around the sun was known as 365.25 days. Later better calculations showed that the actual period is 365.2422 days. The difference is 0.0078 days per year. Usually such a small difference is neglected. But in 100 years it becomes 0.78 days, in 200 years 1.56 days, in 300 years 2.34 days and 400 years 3.12 days. Thus in 400 years the Julian calendar became longer by 3 days.

With passing years this difference kept on mounting. In 16th century, in 1582, on the advice of astronomer and mathematician Christopher Clavius, Pope Gregory XIII made another reform in the calendar and it was called Gregorian calendar which we use today. To correct the cumulative error, he shortened the month of October. The following 4th October 1582 was not the 5th October but was declared to be the 15th October 1582. Thus it was the longest night of history. People slept in the evening of 4th October and woke up in the morning of 15th October.

Gregory changed the rule of leap years also. Till then every fourth year was a leap year. The centuries 1700, 1800, 1900, 2000 were all leap years in Julian calendar. But according to Gregory all centuries are not leap years. Only those centuries are leap years which are divisible by 400. Thus 2000 was a leap year but 1700, 1800 and 1900 were not, nor will be 2100.

This is the calendar which we use today without any doubt, but the lunar calendar does not have these defects.

 

 

 

 

 

 

 

 

 

 

 

 

                             CHAPTER 7

 

MATHEMATICAL METHOD FOR FINDING THE DIRECTION OF QIBLA

 

7.1       Formula for Direction of Qibla

The following information is needed to find the direction of the Qibla from a given place:

a = latitude of the place.

b = latitude of Mecca Mukarramah = 21o 25’ 16” N.

c = longitude of the place.

d = longitude of Mecca Mukarramah = 39o 49’ 29.1” E.

Formula:

 

            Cot A =

 

Where A is the angle of Qibla from the north. If A turns out to be add 180o to it.

 

Example 1: Find the direction of Qibla from a place whose latitude is 33o 17’ 12” N and longitude is 73o 02’ 25” E.

 

Solution:         a = latitude of place = 33o 17’ 12”.    

b = latitude of Mecca = 21o 25’ 16”

c = longitude of place = 73o 02’ 25”.

d = longitude of Mecca = 39o 49’ 29.2”.

 

Formula Cot A =

 

Put the value of a, b, c and d and take sin, cos and tan with the help of calculator.

Cot A =

 

Multiply the terms

Cot A  =  . Subtract

 

Cot A  =  = – 0. 2540800

 

Take reciprocal:          

tan A =  =  – 3.9357683.

 

Take tan -1 with calculator

A = tan -1 (– 3.9357683) = – 75o 44’ 38”.

    = – 75o 44’ 38”. + 180

    = 104o 15’ 22” West of The north or

255o 44’ 38” East of The north

.

 

Example 2: Find the direction of Qibla for the city Den Haag of Netherland.

Solution:         a = latitude of place = 52o 22’ 0” N.  

b = latitude of Mecca = 21o 25’ 16” N

c = longitude of place = 4o 53’ 0”E.

d = longitude of Mecca = 39o 49’ 29.2” E.

 

Formula Cot A =

 

Put the value of a, b, c and d and take sin, cos and tan with the help of calculator.

 

Cot A =

 

Multiply the terms

Cot A  =  . Subtract

 

Cot A  =  = – 0. 6113121

 

Take reciprocal:          

tan A =  =  – 1.6358257.

 

Take tan -1 with calculator

A = tan -1 (–1.6358257) = – 58.5621.

    = – 58.5621 + 180 = 121.438.

    = 121o 26’ East of The north or

 

Example 3: Find the direction of Qibla from Karachi.

 

Solution:         a = latitude of place = 24o 50’ N.      

b = latitude of Mecca = 21o 25’ 16” N

c = longitude of place = 67o 03’ E

d = longitude of Mecca = 39o 49’ 29.2”.E

 

Formula Cot A =

 

Put the value of a, b, c and d and take sin, cos and tan with the help of calculator.

 

Cot A =

 

Multiply the terms

Cot A  =  . Subtract

 

Cot A  =  = – 0. 040523

 

Take reciprocal:          

tan A =  =  – 24.6773105.

 

Take tan -1 with calculator

A = tan -1 (–24.6773105) = – 87.6795.

    = – 87.6795 + 180

    = 92.32 = 92o 19’ West of The north or

267o 41’East of The north

.

7.2       Another Formula for Qibla

Find the latitude of the place, latitude of Mecca and difference of longitudes of Mecca and the place.

Formula:

A =

Example 1: Find direction of Qibla from Rahim Yar Khan.

Solution:  Put the value in above formula

 

A =

 

   =

 

   =

   =  = tan – 1 ( – 7.94408657)

   = - 82.8253 + 180 = 97.17

   = 97o19’ West of The north

   = 262o 41’ East of The north.

 

 

Example 2: Find direction of Qibla from Islamabad.

Solution:         Longitude of place = 73.0833o E.

                        Latitude of place    = 33.716676o N.

                        Longitude of Mecca = 39.75o E.

                        Latitude of Mecca   = 21.4499986o N.

                        Diff of longitudes = 73.0833 – 39.75

                                                 = 33.333

 

Formula: A =

Put the value of the angles

A =

A =

 

A =

 

   =   =  tan – 1 ( – 4.012193)

   = – 76.004o + 180 = 103.996o..

So direction of Qibla from Islamabad is 104o West of The north.

 

7.3       Method to find the North with The Help of the Sun

On a sheet of paper draw a line NS.

If it is 4 pm draw the angle NBC (15o for each hour after midnight) = 240o towards the east.

Fix the paper horizontally and put a pencil perpendicular to the plane of the paper at C.

Rotate the paper so that the shadow of the pencil coincides with the line CB. NS will represent the North and the South

                                                                         N

 

 

 


                                                                            B

 

 

                                     Pencil

                                                           Shadow

 

                                                 C

                                                                           S

 

CHAPTER 8

 

PLACES WHERE TWILIGHT NEVER ENDS

 

Six months long day and night

Abnormal regions

 

8.1 Regions near the Poles of the Earth

The conditions in places near the poles are different from other places. These places are called abnormal regions and the countries located in such regions are called abnormal countries.

In such abnormal regions day and nights are of six months duration. Near the poles and in adjacent regions. White twilight and sometimes red twilight does not disappear for months. The reason is explained below.

The earth is rotating round its axis which causes day and night. Its axis of rotation is tilted at an angle 23.5o. Allah (s.w.t.) almighty has created the earth in such a way that thousands of our requirements are fulfilled without our efforts.

 

 

 

 

 


    night  day                                                                                day     night

                                                                      Sun



 

                                                   Orbit

 

 

Besides the rotation of the earth around its axis it is also revolving round the sun in the elliptic orbit. The above diagram illustrates that when the earth is at one extremity of its orbit, due to tilt of axis, the northern hemisphere is tilted towards the sun so that the rays of sun fall perpendicularly on Tropic of Cancer. At this time there is summer in the northern hemisphere and at the North Pole and adjoining areas it is continuously day time. After six months when the earth reaches the other end of the orbit due to annual motion, the southern hemisphere is tilted towards the sun. The sun ray fall perpendicularly on Tropic of Capricorn, causing summer in the southern hemisphere and is the cause of lengthy days at and around the South Pole. In summer days are long and nights are short.

            When it is perpetual day for six months at and near the North Pole, there is perpetual night at and around the South Pole. After six months when there is perpetual day at and around the South Pole, there remains perpetual night at and near the North Pole.

 

8.2       The Issues

Let us tackle the issue separately.

All of us know that there are two separate regions and period in the world.

·         Normal areas.  

Normal areas are between (48 ½) degrees North Latitude to (48 ½) degrees South Latitude; while beyond 48 ½) degrees up to poles are abnormal areas.

·         Abnormal period and area.  

 

During the summer season when Twilight never ends in the areas beyond (48 ½) degrees North Latitude and (48 ½) degrees South Latitude up to poles, are considered as abnormal areas & abnormal periods. During this period neither Shafaq abyadh nor Ahmar ends or where neither sun rises nor sets.

 

The Normal period and normal areas

In this connection we have to refer to the actual words of the Holy Quran. It is clearly mentioned to distinguish between: 

·         White thread and black thread. (Line – khat-e-abyad and khat-e-aswad)

·         Allah s.w.t. used the word THREAD of the morning  (and not the white and black ROPE

      or broad spectrum)

We have to distinguish between the two.

We must look towards the intention of the Holy Quran.

Think – why the word Thread is used – what is the intention behind it.

And Think of the thickness of the thread (KHAT) or line or thread.

We have not been guided to wait till the lamination (light) spreads all around us. 

 

All the Ulamas, Alhumdo-llillah, know very well its meaning and also the intention of Allah s.w.t. and the intension of our Holy Prophet p.u.h.

What is to be emphasized?

White and black thread appears and is visible vividly and only recognizable in the very initial stage when the night breaks and the day light starts spreading. It happens at the beginning of astronomical Twilight. This is the time when we have to stop our Sehri and this is the actual time of Subhe Sadiq.

With the passage of time, every one knows, the illumination –that is light intensity constantly increases and spreads and covers a broad area till the sun rises.

The two Threads of Fajr can be distinguished, recognized, and differentiated by only those experienced persons who constantly watch and regularly observe these threads in the very initial time of its appearance. And by those who know its shape, direction, and time of appearance.

Certainly its observation depends upon:

  • eye sight of the observer- (most important)
  • If the eye sight is weak, observations of the line (having thickness of a thread) will be impossible.     
  • Light free & Clear atmosphere – no snow fall/ rainfall -  (most important) Cloud, moist, fog and dust free environment  -  (most important)constant observations – necessary and
  • Observations without knowing the time of beginning of Astronomical Twilight – must.

As far as Astronomical Terminologies are concerned

Experts talk about the range:

  • The duration of Civil Twilight is between 0 to 06 degrees.
  • The duration of Nautical Twilight is between 6 to12 degrees.
  • The duration of Astronomical Twilight is between 12 to18 degrees.

 

It is now clear that we are not concerned with the range – or the transitional Zone

 

We have been clearly and specifically taught by the Holy Quran and asked to distinguish between the Black and white threads of the morning.

 


It can be confirmed from any Astronomical Observatory that:

·         18 degrees stage is the point of separation - at this time in the morning black darkness of night ends and illumination of day starts. It is the time when, on the eastern horizon and all around, one can find within the DARK night sky :

·         A dark Black cap just like a black TAWWA  on the head of the observer – one edge of the cap, ending on the eastern horizon, shows a black semi circular line (Black streak) – quite distinct from the white streak of light coming up from the bottom.

·         This white streak of light is quite vivid from the black streak.  

     

How it looks like

The white Thread appears in a semi circular form of which the upper limb pushes the black thread upwards – and constantly the light intensity increases with the increase in size of the semi circular white glow. These are the distinguishable Black and white threads of the morning. 

During  the Normal period (in winter) when Twilight (both Shafaq-Abyed and Ahmar) appears and disappears in areas beyond the (48 ½) degrees North, particularly in Europe, any one expert or any one who recognizes the Subhe-Sadiq  can observe the Black and white threads, in favorable weather conditions, in its most initial stage.

Shafaq (twilight) remains for a longer period in the higher latitudes - and in abnormal seasons (in summer) for weeks or months and sometimes it never ends. It is correct but during the normal seasons the shape at its initial stage and appearance remain the same throughout the whole world.

At this time the shape of illumination never appears like a wolf’s tail- This statement can be confirmed from any Meteorological or Astronomical observatory.

Illumination like a pyramid, pillar, and conical shaped elongated light appears only before the beginning of astronomical twilight in the morning –it appears in the Zodiac-and known as zodiacal light 

The duration between the sun set and Shafaq-Abyed on any particular date is the same as the duration between sun-rise and Subhe-sadiq. If it is difficult to ascertain the time of Subhe-Sadiq, it is advisable to watch and observe, after the sunset, the time when Shafaq Abyed ends.

Shabbir Ahmad Kakakhel from Islamabad, observed these phenomena for six months, and noted the ending time of Shafaq Ahmar and Abyed. He observed and recorded the timings. According to his findings he always observed the end of shafaq Ahmar when the sun was between 15 and 16 degrees below horizon – Obviously shafaq abyed ends after Shafaq-e-Ahmar as Shafaq Ahmar can never end before shafaq abyed.

 

(Ref:  Fahmul-Falkiyat   Shabbir Ahmad Kakakhel) 

All the Ulamas, Alhumdo-llillah, also know:

If in a country or a locality the moon is sighted by a group of people and Ulamas are satisfied, they issue the Fatwa of Eid or Ramzan.

Likewise, if a group of God fearing people observe and sincerely say we have seen and distinguished the white and black thread of Fajr in its initial stage, it becomes necessary for all others to accept and follow their findings.

If a person says no I shall believe only on what and when I and only I personally have observed – it means every individual will follow and go according to his own findings – which is neither acceptable nor sensible.

References in support of 18 degrees are available. But instead of giving any importance to observations of others, unfortunately Moulana Yaqoob Fathavi from UK quoted and mentioned the reference of Tusi alone. While Tusi was a Shia Aalim

It is amazing that on the basis of the following ground Dr Omar Afzal from USA coined the opinion that the time of Fajr begins at Nautical Twilight (depression angle 6°).

He wrote: “For Isha a good gauge is found in Surah Yusuf. The brothers of Yusuf (AS) returned to their home by “Isha” to tell their father about the ‘event’ of Hazrat Yousuf (AS) disappearance. They waited in the open desert and returned when the normal daytime activities were possible... they returned - at the time of Civil twilight (sun’s depression ).”

Remember: The brothers of Yusuf (AS) returned to their home by “Isha” to tell their father about the ‘event’ of his disappearance. But don’t forget they were not bringing any good news to their father. They committed a blunder and were all guilty. They tried to hide their faces from the general public, and returned to their home late (quite late) in the night. So how we can assume they returned - at the time of civil twilight as suggested by Dr.Afzal.

 

Is it  not very strange that, in  order to facilitate and to avoid  hardship,  unfortunately (some Muslims, consider ( it ) sun’s depression at 6 degrees time to be the time of Subhe-Sadiq., and depending upon this assumption and on the basis of this event, they are eating and drinking in Sehri till  the time of Civil Twilight.

 

               For a valid visual observation of Fajr al-Mustateel and Faj al-Mustateer, like Shafaq al-Ahmar and Shafaq al-Abyad the observers must prepare methodically. A valid observation should be done at a location away from well-lighted cities, by observers who do not know the local prayer schedules, or the direction (where to observe), and should not have watches, etc. A time-keeper with a watch and a compass should merely note down the details given by each observer (about when he noticed the first light, in what direction, when the light started spreading horizontally, the time lag, etc.), without making any comments or corrections.

            So during our observations we must keep in mind the above conditions. In abnormal conditions religious scholars particularly Muftees (Jurists) may be consulted to give their final opinion.

Alhamdo-llillah Muftian karam are very cautious in this respect. They are guiding and assisting Muslim brothers to pray all five obligatory prayers and compiling Sehar and Iftar Time Tables on the basis of Ijtehad - (FAQDEROO) Taqdeer -   

 

Abnormal areas & different conventions in use

In various countries, people are using different convention, for the compilation and composition of Prayers Timetables particularly for Fajr and Isha. The different methods used by different organizations are as follows.

 

 

Organisation

Fajr

Twilight

 angle

Isha – twilight

 Angle

Region

 

University of Islamic

Sciences, Karachi

18°

18° degrees

below  horizon

Pakistan,Bangladesh,India  India, Afghanistan, parts of Europe

 

Islamic Society of

North America (ISNA)

15°

15° -Incorrect

don’t use it it is

 debatable

Parts of USA & Canada,

parts of UK

 

World Islamic League

18°

17°

Europe, Far East,

parts of USA

 

Um Ul-Qura, Makkah

19°

90 mines after

 Maghrib, 120

 min in Ramazan

Arabian Peninsula

 

Egyptian General

Organisation of Surveying

19.5

17.5

Africa, Syria, Iraq,

Lebanon, Malaysia,

parts of USA

 

Convention:  In the abnormal areas and also in the extreme northern and southern latitudes, during the summer months, the twilight may persist between sunset and the next sunrise for certain months of the year. In these months the sun does not go below the horizon to abolish twilight. Hence we can say these are the abnormal regions where there is no true night. Under these circumstances, Fajr and Isha times may be calculated using one of the following four agreed principles. These conventions are commonly known to the Ulmas 

i.          Nearest latitude (Aqrab Al-Balad)

Since conditions differ from Lat 48:30 in both the hemispheres add the interval between sunset and isha for a location on latitude 48 degrees (the nearest Latitude) to the local sunset time to obtain time for local isha. Similarly the interval between fajr and sunrise for a location on latitude 48 degrees is subtracted from local sunrise to obtain local fajr time.

ii.         Nearest day (Aqrab Al-Ayyam)

Use fajr and isha times from the last day, for the abnormal period, when it was possible to determine and calculate these times in the normal way for that location.

iii.        Middle of night (Nisf Al-Lail)

Split interval between sunrise and sunset into two halves. Isha may be offered before the midpoint (e.g. 15 minutes before midnight) and fajr may be offered, obviously before sun rise, after the midpoint.

 

iv.            One seventh of night (Sube Al-Lail)

Split interval between sunset and sunrise into seven segments. Isha may be offered after the first segment and fajr may be offered after the sixth segment

From latitude of 48.5o north to the North Pole and from 48.5o south to the South Pole white and red twilights do not end for several months in summer. We consider these regions as abnormal regions too. They include European countries specially France, Britain, Belgium, North Russia, Poland, Lithonia, Norway, Sweden, Netherlands, Canada and Alaska. For such areas, different conditions were recorded to and compiled as istafta

A fatwah was obtained from Mazahar ul Uloom, Saharanpur (India) with the efforts of Hazrat Maulana Mohammad Umer Palanpuri. It was published by Haztar Maulana Muhammad Yousuf Ludhianvi in the monthly magazine “Al Bayyenat” of Jama Islamia, Binori Town, Karachi,. This proposal, fatwah and tables are given below:

 

8.3       Istafta (Questionnaire)

Respectable Hazrat Mufti Saheb

Assalam Alaikun wa Rahmatullah wa Barkatuhu

Hope by the grace of Allah (s.w.t.) that you are well. These lines are written for the solution of a very important problem. Between the latitudes of 48½ degrees north and south, the days and nights continue all year round with changes in durations. But in higher latitudes on some days there is not complete night i.e. the twilight does not end. It creates some problems and confusion as to when Maghrib and Isha prayers each be offered and to decide when the time of sehri ends.

 

Since Muslim countries are located between 48 ½ degrees north and south, there was no practical problem in this context. Guidance was provided by scholars in some rare cases for these regions but in general it was not needed for a common person. Now the situation is different. There are millions of Muslims in some cities of the western countries There are thousands villages. Without exaggeration, the number of Muslim residing in these areas is in tens of millions. Now as Ramazan is coming in July and the interest and trend of prayers in Ramazan also increases in Muslims, there are great difficulties in those areas where twilight does not end. There is great dispute in such areas in finding times of Isha and Fajar. Different times are followed in different mosques of the same city. It becomes an easy way for lazy people who seek ways to avoid religious practices. Various situations faced are given below in detail. Some more similar situations may be known to you.

Kindly provide the guidance towards principles which are definite according to sharia and on which the Islamic community agrees.

Wassalam

Abdul Latif

Muharram 3, 1402 H

 

Some important problems are as follows

There are places where twilight does not end and places where there is continuously daylight or continuously night. There are some places where either the sun does not rise or does not set for several months. Muslims living in such places face problem in fixing times for prayers, sehar and iftar. Thousands of Muslims live in such places. There are local Muslims and other Muslims who have settled in such places from other parts of the world.  The following reflects the problems faced by them in determining the times of prayers.

 

1. Nights in which twilight does not end. In places from 48½ o N to the North Pole and from 48½ o S to the South Pole the twilight does not end and white or red twilight remains visible on the sky throughout the night in summer. The list of such places is given in table 1 on page

The problems in these places are

 

Question No.1

(a) How to fix the time of Isha prayer?

(b) How to fix the time of beginning of Fajar and end of shear?

 

2. Days when the sun does not set: (i.e. where it is perpetual day).

            In the northern hemisphere at latitude of 66oN the sun rises on 12th June and does not set (remains above the horizon) for 19 days i.e. it is continuously day time. In higher latitudes, this duration is longer. On 75o N the sun rises on 28th April and sets on 15th August after a long day of 3 months and 19 days in length. (Table 2 page       ). At further north latitudes and at the North Pole the sun does not set for six months in the northern hemisphere. While in the southern hemisphere there is six months day in summer. (Table 4 page    )

The problems for these places are:

 

Question No. 2

(a) How to fix the times for all five prayers?

(b) How to find times for sehar and iftar?

 

3. Days when the sun does not rise (i.e. perpetual night)

            On the latitude 68oN when the sun sets on 8th December at 12:15 noon, then it rises on 3rd January at 11:55 a.m. after a long night of 25 days in length. During this period it is continuously night. In higher latitudes this length of night gradually increases. On 75o N there is a 3 months long night from 1st November to 5th February. At the North Pole and the South Pole it is night for 6 months in winter. (Table 3 page     ).

The problems in these places are:

 

Question No.3

(a) How to fix the times for all the five prayers?

(b) How to find times for sehar and iftar?

 

4. Appearance of twilight in places near poles during long nights

            In places near poles where there is perpetual night, the twilight is visible above the horizon for several hours every day. The twilight appears on the horizon when the sun is 18o below horizon. The light of twilight keeps increasing every hour. It neither vanishes nor ends. It remains visible throughout north south for hours. The details are given in table 4 page  

(The number of hours for which the twilight is visible from 68o N to 75o N is given in table 5 page   .)

In these places the problems are:

 

Question No. 4

(a) Will beginning of twilight be treated as beginning of Fajar and end of sehar?

(b) The sun does not rise at all. How the interval of twilight be treated? Will it be regarded as part of day or night?

(c) How will prayer times be set in these days?

 

5. The shortest day and the corresponding longest night

            In winter season, especially on 21st December, the length of the day decreases continuously from 60o N to 67o N. At 66o the day is 2 hours 45 minutes long and at 67o it becomes 1½ hour long and the night becomes 22½ hour long.

Just imagine that at 67oN, during a 1½ hour short day,

 

Time of sun rise                       = 11:13 morning.

Transit time                             = 11:58 morning.

Time of sun set                        = 12:43 noon.

Dawn (end of sehri)                = 6:34 morning.

Beginning of time of Isha       = 5:22 evening.

The question is that in 1½ hour short day

 

Question No. 5

(a) Transit time is 45 minutes after sunrise. Will Zohar be offered immediately after transit and since?

(b) As a 45 minute interval is in between transit and sunset, will Asar prayer also be offered in the same interval?

(c) There is an interval of 1½ hours between sunrise and sunset, so will Maghrib prayer also be offered at the end of 1½ hours?

 

Muslims living there have a very short period available to them, will the prayers be offered as described above or they will have to fix the times in these short days as for those places where no day time is available?

 

6. The longest day and the corresponding shortest night

In The northern hemisphere 21st December is the shortest day in winter. On the other hand in summer 21st June is the longest day. On this date at 60o N latitude this day is 19 hours long. Further north it increases. On the same date at latitude of 65o N the day is about 22 hours long. The corresponding night is hardly of 2 hours. At latitude 66o N and further north, the sun does not set on that day and it is continuously day. At latitude of 66o N, the twilight does not end continuously for 5 months and 1 day.

Just imagine: in the 2 hour short night period at latitude 66o N on 21st June,

Time of sunset             = 23:03.

Time of sun rise           = 01:00.

Dawn: Twilight does not end throughout the night.

Transit time                 = 12:02 pm

Time of Isha: Twilight does not end all night.

 

Thus Muslims living at this latitude get 2 hours short night in which even twilight does not end after sunset.

In these two hours duration after sun set:

(a) Iftar is to be done.

(b) Maghrib prayer is to be offered.

(c) Isha and traveeh during Ramzan are to be offered.

(d) Sehri is to be done.

(e) After sehri Fajar prayer is to be offered before sunrise.

Remember that this night corresponding to the longest day is only of two hours duration in length.

The problems are:

 

Question No. 6

(a) Will the short night be divided according to the usual rules?

(b) Will some rule be devised as for those regions where the sun    

      does not rise or set

(c) How will the time of Fajar and end of sehar be decided?

 

7. The calendar for prayer times published from London

London city, from which 0o Greenwich longitude passes, is located at 51.5o N. Millions of Muslims from all over the world live there. Due to high altitude, the twilight does not end there from 23rd May to 19th July i.e. for one month and 28 days (almost two months). Many other cities are located on the same latitude e.g. Bristle, Cardiff, famous city of Canada Canderlay, parts of Sekchwan, Enderhoven, Valkil, Netherlands  etc. In these cities twilight does not end for two months as in London.

In a calendar of prayer times published from London, the time of Isha is shown one hour after Maghrib every day. Time of Fajar for every day from 23rd May to 15 th July is shown (more or less) 2 hours before sunrise.

 

The problems are:

 

Question No. 7

(a) Is it correct to offer Isha prayer one hour after Maghrib in  

      places where twilight does not end?

(b) In places where twilight does not end, is it correct to offer

      Fajar prayer two hours before sunrise?

(c) Is it correct to end sehri two hours before sunrise in such

      places?

(d) Is the calendar published from London wrong?

(e) How will the times of prayers, sehar and Iftar be determined

      in such places?                     

 

8.4       Answers

i.          In the case where twilight does not end all night, Isha prayer can be offered one hour after Maghrib prayer   

Arabic text p 302

Its clear meaning is that if a person offers prayer in congregation even before the end of white twilight it is correct without any objection and will not be a matter of dispute or to condemn.

Thus if there is no harm in it without any hindrance or objection and is not condemnable, then in stated latitudes it will not be objectionable due to valid and unavoidable reasons and conditions. It is advisable to consider it in mosques.

The rule is that the interval between dawn and sunrise is the same as the interval between Maghrib and Isha. If the first interval is known, the second will be considered as the same.

 

The sign of dawn is that in the east a long light appears i.e. at the place of sunrise it looks like a high pillar. This is false dawn. Later this light almost disappears and another light appears in the sky in the north south directions. It is a must to end sehri before the beginning of this light and Fajar time begins at its appearance. And after sunset till a similar light remains, i.e. white twilight, Isha should not be offered. When this light disappears, Isha can be offered.

It is not difficult to find dawn and white twilight because it has a special characteristic. The darkness of the night is evident and the illumination of light in the east or west against it is also evident. Till this light is towards the west, it is time for Maghrib, when it disappears, it is time for Isha. And till such light does not appear on the east, it is night and when it appears in the east, it is dawn. It is Fajar time between dawn and sunrise. End sehri before dawn; do not continue it after dawn.

If the stated procedure is difficult, Fajar should be offered 1½ hours before sunrise. Offer Isha prayer one hour after Maghrib.

 

ii.         In places where the sun does not rise and set daily but for several days or several months it remains risen or set as at and near poles, in such regions the sun completes one circle daily in 24 hours i.e. it leaves a place one day and after almost 24 hours returns to the same point. It can be regarded as one circuit which is equivalent to the sum of a day and a night and the times of the five prayers can be guessed and offered accordingly. The time of start of day-night cycle may be taken as the sunset of the nearest place where it rises immediately after setting.

In places where the sun rises immediately after setting, the interval between sunset and sunset be treated as the sum of day-night. First half (12 hours after sunset) be treated as night. Maghrib should be offered at the start of this period. Isha time should be regarded after 1½ hours and Isha should be offered as soon as possible.

Then half hour before the end of first half (which was regarded as night) offer Fajar. After elapsing half the time of the second half, which is regarded as day, i.e. after three quarters of the time regarded as day-night, Zohar time be declared and Zohar prayer may be offered as soon as possible.

Then about 1½ hours before the end of the 24 hour circuit, i.e. 1½ hours before sunset, the time of Asar be taken. Then after sunset the next day-night is considered and the next day’s Maghrib be offered soon after sunset. Then times of Isha, Fajar and other prayers be fixed regarding the sum of day-night as a day. The schedule of daily prayers is made accordingly.

If it is difficult, then it will be easier to regard 24 hours as a day-night from the time the sun rises and does not set for several days. The first 24 hours be regarded as one day-night and the five prayers be distributed as described. Next 24 hours be regarded as next day.

In regions where the sun does not rise or set daily, but remains above or below the horizon for several days or months, as at and near the poles of the earth, the complete 24 hour circuit of the sun be treated as sum of a day-night. The second half be treated as day. Keep fast in it. Stop eating sehri 1½ hours before beginning of this half and keep fast after making intention. First half is treated as night. Offer Maghrib, Isha, Taraveeh in it. When the next day starts after the sum of day-night period ends, perform iftar and offer Maghrib. Then in the first half of the next day which is treated as night, you can eat, drink and offer all prayers of night. 1½ hours before the beginning of next half which is treated as day, eat sehri and perform intention of fast. Keep following it until the situation lasts.

 

iii.        When the sun does not rise daily, the sun is not present continuously for several days and remains set as at or near poles, then in such places every 24 hours will be treated as a day-night period. The first half will be treated as night and the second half as day provided the sun does not rise after setting and remains continuously set. In this case the 5 prayers will be offered as in answer (2).

The beginning of the day-night period be taken as sunrise of the nearest place where the sun sets immediately after rising. In this case the first half will be treated as day and the second half as night. In this case follow the routines of (2) until continuous setting does not end. The times of fasting in (3) will be the same as in (2).

 

iv.        In case of continuous night, every 24 hours of time will be treated as a day-night period. First half is treated as night and second half as day.

See the direction in which the twilight if it appears. If it appears in the west it will be treated as white or red evening twilight and if it begins elongated towards the east, i.e. it is like a pillar in the place of sunrise, it is false dawn. Later it almost disappears and another light spreads on the sky stretching along north south. After it Fajar time begins. This is taken as dawn.

If above mentioned signs are visible then it will be taken as evening white or red twilight or dawn. Otherwise again a 24 hour period will be regarded as equivalent to a day-night and prayers may be offered as in (3).

 

v.         When the length of a day becomes too small and it is difficult to determine and distinguish misl and malain , offer Zohar as soon as possible and well before sunset (i.e. Isteqrar e Shams)  offer Asar. When the day becomes so short that even transit cannot be determined definitely and agreed upon, then offer Zohar after half the day has passed and before Isteqrar e Shams offer Asar so that there is a little difference of time between the two prayers. There is no harm even if there is too little difference.

 

vi.        When night is short and day is long but the sun rises and sets daily, time of transit and time of Asar may be separately determined. Every prayer should be offered at its actual time. However Asar must be offered before (Isteqrar e Shams) otherwise the prayer will be makrooh.

If the night is two hours long, offer Maghrib after sunset and Isha half an hour later. Offer Fajar half an hour before sunrise. One hour’s time remains between Isha and Fajar, in which Taraveeh and sehri can be done easily.

In places where the sun rise and sunset occur daily all the year round but there is not enough time after sun set till dawn that according to the ayat:

 

وَكُلُواْ وَٱشۡرَبُواْ حَتَّىٰ يَتَبَيَّنَ لَكُمُ ٱلۡخَيۡطُ ٱلۡأَبۡيَضُ مِنَ ٱلۡخَيۡطِ             

ٱلۡأَسۡوَدِ مِنَ ٱلۡفَجۡرِ‌ۖ ثُمَّ أَتِمُّواْ ٱلصِّيَامَ إِلَى ٱلَّيۡلِ‌ۚ (٨٧ ) {البَقَرَة 2}     

Translation: And eat and drink until the white thread (light) of dawn appears to you distinct from the black thread (darkness of night), then complete your Saum (fast) till the nightfall.

 

Food and drinks can be taken and then fast can be completed till Maghrib, then for these places the length of fast will not be determined with hours. But exactly the same the days of the month will be fixed for fasts. As without eating and drinking satisfactorily, a whole month fast is intolerable so in these days keep fast by giving gaps according to courage and limit. The fasts in lieu of gaps may be completed in other months according to courage and power again by giving gaps.

If it is not possible due to physical weakness then gives fidiya equal to one sadqa e fitr and if it is not possible due to poverty, then keep repenting and try to leave such a place as soon as possible.

 

In places where sunrise and sunset occur daily and between sunset and dawn there is enough time all the year in which the night prayers can be offered and food taken easily and enough time is left for rest, then for persons in these regions fasting is obligatory and necessary in Ramzan and fast should be started with dawn. The duration of fast will be long, but due to cold country, it will be well within tolerable limits and should not be avoided.

 

vii.       In this case to offer Isha prayer one hour after Maghrib is correct. Offer Fajar prayer 1¼ hours before sunrise. To be on the safe side, end sehri two hours before sun rise. Offer remaining prayers at their scheduled times. If Ramzan occurs during this period then fasting is obligatory. Obligatoriness is not invalid and cancelled because in such days fast is 16 or 17 hours long which is not beyond human endurance.

 

 Yahyah                       Mazaharul Uloom, Saharanpur

                                    7, Jamadiul Awwal, 1402

 

Note: Evidently the answers to above questions are not given in books of Fiqah in detail. Some scholars have written explainations and answers in their fatawa like Muntakhibat e Nizamul Fiqah,   Ahsanul Fatawa.  Imdadul Fatwa etc., that is written.  May be some     scholar disputes. It should be shown to other scholars as well. We have written after consulting Hazrat Mufti Mahmood Hasan Gangohi  -  Yahya GG

 

 

 

 

 

 

 

Table 1

 

The places where twilight does not end in summer.

 

North

latitude

Days when twili-

ght does not end

No of

such days

Length day

night 21 June

Affected regions/

Places

degree

 

Mnth

    day

Night    day

h  m      h  m

 

 

49

 

50

 

51

 

52

53

54

55

56

57

58

59

60

61

62

63

64

65

66

67

68

69

70

71

72

73

74

75

11 Jun - 1 July

 

1 Jun - 11 July

 

25 May - 17 July

 

21 May - 21 July

15 May – 27 July

11 May – 31 July

9 May – 3 Aug

5 Mat – 7 Aug

1 May – 11 Aug

27 Apr – 13 Aug

25 Apr – 17 Aug

21 Apr – 19 Aug

19 Apr – 23 Aug

17 Apr – 25 Aug

13 Apr – 29 Aug

11 Apr – 1 Sep

7 Apr – 3 Sep

5 Apr – 5 Sep

3 Apr – 9 Sep

31 Mar – 11 Sep

29 Mar – 13 Sep

25 Mar – 17 Sep

23 Mar – 19 Sep

21 Mar – 21 Sep

19 Mar – 23 Sep

15 Mar – 27 Sep

13 Mar – 29 Sep

0    21

 

1   11

 

1   23

 

2    1

2   13

2   21

2  26

3    3

3   11

3   18

3   24

4    0

4    5

4    9

4   17

4   22

4   28

5    1

5    7

5   12

5   16

5   24

5   28

6    1

6    5

6   13

6   17

7  47    16  13

 

7  37    16  23

 

7  27     16  33

 

7  16     16  44

7  02     16  58

6  51     17  09

6  37     17  23

6  22     17  38

6  06     17  54

5  49     18  11

5  29     18  21

5  07     18  53

4  43     19  17

4  15     19  45

3  41     20  19

2  58     21  02

1  57     22  03

0  00     24  00

0  00     sun

0  00   

0  00     does

0  00   

0  00     not

0  00

0  00    set

0  00

0  00

France, Germany,Canda

British Columbia,

Britain, Mangolia, Ukrain,

Canada, Belgium

Russia, Canada, Brussels,

London. Cardiff,, Holland

Warsa, Poland, Betal Harbor

Hudson Bay,Russia

British Clumbia, Humburg

Canada, Newfound Land

Denmark, Glascow, Dundy

Russia

Russia

Russia

Finland, Alaska, Greenland

Norway, Sweden, Finland

              Do            

Russia, Alaska, Canada

          Do               ,Iceland,

Iceland, Norway, Sweden

              Do     , N. Russia

Greenland,  Finland, Canada

N. Norway, Sweden, Greenl

               do

Belgium, Netherlands, Alask

N.Russia, Greenland, Canada

               do

               do

               do

               do

 

 

 

 

 

 

 

 

 

 

Table 2

Places where sun does not set

(Perpetual day)

 

N. Lat

Degre.

Date of no sunset

perpetual day

Duration of

Perpet. day

Famous places / regions

 

Rises           Sets

Months   Days

 

66

67

68

69

70

71

72

73

74

75

12 June     30 June

2 June      11 July

26 May    17 July

21 May    23 July

16 May    27 July

12 May    31 July

  8 May     4 Aug

  5 May     8 Aug.

  1 May    11 Aug

28 Apr      15 Aug

0         19

1         10

1         22

2           3

2          13

2          20

2          28

3            4

3           11

3           19

Norway, Sweden, Finland, Russia

                       do

                       do

                       do

Alaska, N. Russia, Greenland

                       do

                       do

                       do

                       do

                       do

 

 

 

 

Table 3

Places where sun does not rise

(Perpetual night)

 

N. Lat

Degrees.

Date of no sunrise

perpetual night

Duration of

Perpet. Night

Duration of Twilight

Minimum      Maximum

 

Sets       Rises

Mon     Days

Hr.    Min        Hr.   Min

68

69

70

71

72

73

74

75

 8 Dec    3 Jan

 1 Dec   11 Jan

26 Nov  17 Jan

21 Nov  22 Jan

17 Nov  26 Jan

12 Nov  30 Jan

 9 Nov    2 Feb

 6 Nov    6 Feb

0            26

1            11

 1        23

 2          2

 2         10

 2         18

 2         25

 3           1

5       20           5      26

5       16           5      20

5       12           5      38

5         8           5      51

5         3          6         1

4       58          6        13

4       53          6        25

4       46          6        42

Times for 76o onwards are in next table.

 

 

 

 

 

 

 

 

 

 

Table 4

Six months long day and night

Appearance of twilight in long nights

 

North

Latitude

Days when sun light or

Twilight remains

Continuous night but

Twil. Begins and ends

Continuous night

Duration of twilight(1)

 

From              To

From           To

 

76

 

77

 

78

 

79

 

80

 

81

 

82

 

83

 

84

 

85

 

86

 

87 – 90

 9 March     2 Oct

 

 7 March     4 Oct

.

 4 March     8 Oct

 

 2 March     9 Oct

 

 1 March     12 Oct

 

25 Feb        15 Oct

 

23 Feb        18 Oct

 

20 Feb        20 Oct

 

16 Feb        24 Oct

 

14 Feb        26 Oct

 

10 Feb        29 Oct

 

day is longer in

these days

 3 Oct     8,10 Mar

 

 5 Oct     6,8 Mar

 

 8 Oct     3,5 Mar

 

10 Oct    1,3 Mar

 

13 Oct      28 Feb,

                  1 Mar

16 Oct    24,26 Feb

 

19 Oct      22,24 Feb

 

21 Oct      19,21 Feb

 

25 Oct      17,19 Feb

 

27 Oct     13,15 Feb

 

30 Oct     8,10 Feb

 

night is longer

in these days

72o to 87o twilight

does not set for 6

hours. (Jan), date 26

 

Twilight does not set

For 4 to 5 hours daily

From 76o to 800.(Jan)

 

80o day starts to rise

from 1 March

76o night begins from

1, Oct.

76o to 81o twilight does

not set for 5 to 9 hours

on 16 Oct.

 

16 Nov. twilight does

not set for 6 hours

from75o to 85o.

 

10 Jan. twilight does

not set for 4 hours

from 75o to 80o.

 

 

(1) Light of twilight appears for different durations at different times at different latitudes. Some data is given above as a sample.

 

 

 

 

 

 

 

 

 

 

 

 

Table 5

Days in which it is perpetual night

Hours for which twilight is visible

Degrees in North latitudes

 

Date/Month

68

69

70

71

72

73

74

75

 

H   M

H  M

H  M

H  M

H  M

H  M

H  M

H  M

 7 Nov

 9 Nov

13 Nov

17 Nov

21 Nov

27 Nov

  1 Dec

  2 Dec

  9 Dec

15 Dec

23 Dec

  1 Jan

  7 Jan

  9 Jan

15 Jan

21 Jan

25 Jan

29 Jan

  1 Feb

  5 Feb

 

 

 

 

 

 

 

 

5  26

5  22

5  20

5  25

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

5  28

5  23

5  18

5  16

5  21

5  28

5  31

 

 

 

 

 

 

 

 

 

 

 

5  38

5  31

5  27

5  19

5  14

5  13

5  18

5  25

5  28

5  39

 

 

 

 

 

 

 

 

 

5  49

5  35

5  27

5  24

5  15

5  10

5  08

5  14

5  22

5  25

5  37

5  51

 

 

 

 

 

 

 

5  59

5  47

5  32

5  24

5  20

5  11

5  05

5  04

5  10

5  18

5  21

5  34

5  49

6  01

 

 

 

 

 

6  10

5  57

5  45

5  29

5  20

5  16

5  07

5  01

4  58

5  05

5  14

5  17

5  31

5  47

6  00

6  13

 

 

 

6  25

6  10

5  56

5  43

5  26

5  16

5  12

5  02

4  55

4  53

4  59

5  09

5  13

5  27

5  45

5  58

6  13

6  24

 

6  34

6  25

6  09

5  54

5  40

5  22

5  12

5  07

4  56

4  49

4  46

4  54

5  04

5  08

5  24

5  42

5  57

6  12

6  25

6  42

 

 

 

                    Twilight Diagram

 

 

 

(insert the duration of Astronomical twilight from its beginning to sunrise from  the sunset to its end)

 

 

8.6       A New Method for Finding Times of Prayer in Regions near the Poles

The transit time (at any date) is the same all over the world.

Strange and interesting

Allah (s.w.t.) almighty put a very useful idea in my mind by which the problem of prayer, sehar and iftar can be easily solved in places where the sun does not rise and set for six months. All praises to the almighty Allah (s.w.t.) who put this idea in my mind. It is a fact which most people are unaware of. Perhaps religious scholars also have not thought about it.

 

i.          All over the world, in every country, every city, on every latitude and longitude (at any given date, and place) the time of transit is the same. It is a known fact to which astronomers agree and confirm. There is nothing extraordinary about it.

 

ii.         For example today 1st of April, the time of transit in Glasgow and Pakistan is 12:00 hrs Universal Time. The same time of transit is in Tokyo, Moscow, New York, London, South Africa, Fiji Islands i.e. in every part of the world the time of transit is the same. This Universal time of transit is called Ephemeris Transit or mid day (waqt e zawal).

 

iii.        The apparent difference in the time of transit (zawal) observed by us in different places and countries, is due to the standard time of the country and due to the difference between standard and local times. The standard time of Pakistan is reckoned by longitude 75oE. The local time of this longitude is regarded as the time of all parts of Pakistan. This is called Pakistan standard time. Besides it, there is a local time for every place which is never used by us and we are not even aware of it. Except the time of transit, all other times e.g. time of sun rise, sun set, misle awwal, misle sani are different for different latitudes and longitudes.

 

iv.        Some further explanations

 

To form charts of prayer times we need to know the difference in standard and local times. This has already been discussed in detail on pages    .

  • When the sun is on observer’s meridian, it is transit time which is the same all over the world on the same day.
  • Just as the time of transit is the same all over the world on the same day similarly the time of dawn, i.e. for beginning and end of astronomical twilights is also at the same instant, when the sun is 18o below horizon. It is another matter that when red and white twilights do not end, there is no question of beginning or end of dawn. These days are called abnormal days and the regions in which it occurs are called abnormal regions.

 

8.7       An Important Proposal

(Hopefully religious scholars will ponder over this and give their valuable opinion).

It is a universal truth that the time of zawal (transit) is the same all over the world for any date of the solar calendar. We can use this fact (known time of transit) safely for compiling and composing of Prayer Timings etc. for the regions where the sun neither rises nor sets for several months. We have to convert the Universal Time of transit in to local time to know the exact time of zawal for the place for which we are going to calculate the times of prayers. When we have calculated the time, it can be used as a standard. The 24 hours day and night duration may be divided by this standard which is the middle point of 24 hour day and night duration.

For example if the middle point is 12 hours, the first half that is 6 hours may be regarded as time of sunrise and the second half from this standard time that is 18 hours may be considered as the time of sunset. All the prayers may be scheduled with this reference.

This is most simple and easy to use method for calculating the timings. After sunset Maghrib and Isha may be offered, and before sunrise Fajar. In between time of transit and sunset, Asar may be offered two hours before sunset. (Lateef)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 


 

                           CHAPTER 9

 

Direction of Qibla and Muslims of America

 

9.1    Details About Great Circle and Rhumb Line of Mercator’s Projection for Finding Direction Of Qibla

Some people living in Canada and America, due to their ignorance, are getting confused themselves and are confusing others about the direction of Qibla. Two terms, great circle and Rhumb line of Mercator’s projection are repeatedly used in this connection. Let us consider them in detail.

Our earth is a sphere. So a globe can accurately represent it. But it is not possible to carry a globe everywhere and at all the times. We have to use maps drawn on plain papers. Some method or device has to be adopted to transfer lines of latitude and longitude from the globe to the paper. A method by which latitudes and longitudes on the globe are transferred to a plain paper is called map projection. Projection means shadow or image. We assume that the lines of latitude and longitude are made of steel wires i.e. it is a spherical cage made of wires. Wrapping a photographic paper round the globe and lighting a bulb at the centre of the globe the images of wires are transferred on the paper.

If the paper is wrapped in the shape of a cylinder, the image will be cylindrical. The image will appear rectangular when the paper is unwrapped i.e. all lines in length and breadth will be equally spaced, which is entirely different from the real globe. Such projection is called cylindrical projection. It is a deformed form of the map. Mercator’s projection is similar. Neither shape nor area is represented correctly. The line on it is called Rhumb line or Loxodrome.

There are many types of projections. We can wrap the paper in various ways according to our requirement and get latitudes and longitudes transferred on the paper. Some of them are:

·                     Projection showing equal areas.

·                     Projection showing equal shapes.

·                     Projection showing equal distances and

·                     Projection showing equal sizes.

 

We use different types of projection for equatorial regions, Polar Regions, tropical regions and mid latitude regions (European countries)

 

Types of Projections

 

1. Cylindrical projection.

2. Conical projection.

3. Zenithical projection.

4. Conventional projection.

5. Molowide projection.

6. Gnonomic projection,

7. Ortographic projection

8. Stereographic Projection

9. Azimuthal Projection

 

 

 

 

Pictures of conical and cylindrical page 313

 

 

 

 Map on page 314

 

 

 

 

 

 

 

 

 

 

 

 

 

Mercator’s projection is a technique of map making as are other types of projections. Map making is a branch of geography called cartography. In it, using mathematics and taking into consideration various requirements of map making, beautiful maps of different regions are designed. One of the projections is Gnomonic projection. The people unaware of this art think that Mercator’s projection is the only projection from which the direction of Qibla can be found. This is due to the lack of knowledge about the art of map making.

In Gnomonic projection, all the lines joining two points are straight lines whereas they are great circles. In Mercator’s projection a great circle becomes an arc where as Rhumb line or Loxodrome is shown as a straight line. In Gnomonic projection Rhumb line is in the shape of an arc and great circles are straight lines.

To sum up, in sharia neither Gnomonic projection is mentioned nor is it dependable. Similarly Mercator’s projection is neither mentioned nor is advised to determine the direction of Qibla. There is a simple rule to turn your face towards Baitullah where ever you are.

We cannot draw a straight line on a globe. If two places are to be joined it can be done only with the help of a thread or a string. Put the ends of a string at the two places that will make an arc on the globe. This forms a great circle which is also the line of sight and also of the minimum distance.

 

Rhumb line or Loxodrome on Mercator’s projection

When the Rhumb line or Loxodrome on Mercator’s projection is drawn on the globe, it is a zigzag line. On the other hand the great circle is straight.

Pakistan International Airlines has set up a training centre at Karachi for training their navigation staff. On page 58 of its Training Manual # AV- 31N-01, both Rhumb line of Mercator’s projection and great circle are drawn on a globe for comparison. The Rhumb line becomes zigzag on the globe whereas great circle is straight. The figure is given below:

 

 

Picture page 316

 

 

 

 

 

 

In Gnomonic projection the curve joining two places is a straight line which is great circle.

 

 

             polar

 

 

 

                Equatorial

 

 


9.2       Gnomonic Projection

            If direction of Qibla is to be found by a map, use Gnomonic projection for correct direction. According to the great circle route, the direction of Qibla, in North America and Canada, is the north east.

 

       Construction Equatorial Position

 

 

           Oblique

 

Following map is Mercator’s projection. Note the form and shape of lines of latitudes here. In it the distance between all the latitudes near the pole are as far apart as on equator (24000 miles). In this projection all parallel of latitudes are equal. This is its greatest drawback. The actual distance between parallels of latitudes measured north south are the same, but as we move north or south, the distance on the map increases. Thus Mercator’s projection is defective and do not represent the globe correctly.

 

     Equatorial Mercator Projection

 

 

 

 

 

 

 

 

9.3       Some Important Information

Measurements, distances, weights, Sharaie journey etc.

 

One mile has 8 furlongs and one furlong has 220 yards. Thus a mile has 1760 yards.

A yard has 3 feet and each foot has 12 inches. Thus a yard has 36 inches.

British system of units yard, feet, inches, sair, mond, chattak, Fahrenheit etc were used in India and Pakistan during British Rule. Now metric system is being used in which the units are meter, kilogram, litre, Centigrade etc.

The unit of length is a meter. It was initially defined as a ten millionth part of the distance from the equator of earth to the North Pole. Now a law has been passed according to which one yard is equivalent in length to 0.9144 meter.

 

10 meters         = 1 decameter

100 meters       = 1 hectometer

1000 meters     = 1 kilometer

1/10 meter       = 1 decimeter

1/100 meter = 1 centimeter

1.1000 meter = 1 millimeter

 

Units of weight

 

10 grams          = 1 decagram

100 grams        = 1 hectogram

1000 grams      = 1 kilogram

1/10 gram        = 1 decigram

1/100 gram      = 1 centigram

1/1000 gram    = 1 milligram

100 kilogram   = 1 tonne or 1 metric tonne

Linear measures (measures of length)

1 centimeter    = 0.39370 inch.

1 meter            = 1.0936143 yards.

1 kilometer      = 0.62137 miles.

1 inch              = 2.54 centimeter.

1 mile              = 1.609344 kilometers.

 

One Sharaie mile is 240 yards longer than a British mile.

 

1 yard              = 0.9144 meter

1 furlong         = 201.168 meters.

1 square mile   = 2.58998 square kilometers.

1 acre               = 4840 square yards.

 

9 inches                       = 1 balisht

2 balisht                       = 18 inch = 1 haath (Hand).

2 haaths                       = 1 yard = 3 feet = 36 inches.

1 zara e masahat          = I yard 6 inches = 42 inches.

1 zara e karbas             = 1,5 feet = 18 inches.

 

According to "Fuqahaa" one mile is 4000 yards of 24 fingers yard. Thus one Sharaie mile is 2000 English yards because the 24 fingers zara is one hath i.e. 1.5 feet or 18 inches.

 

Mile: In Arabic dictionary "Mustapha e Baser" is called a mile and according to "Fiqah" a mile is one third of a "Forsake". Fiqah have different opinions about magnitude of "Farsakh".

 

Farsakh = distance of 3 miles and

 

Bareed = distance of 4 fasakh or 12 miles.

 

In Nihaya, Ibne Aseer says that this word is the abbreviation of Persian word Bereedadam. Breedadam donkeys were used to distribute post. It was abbreviated to "Bareed" and then the rider was also called “Bareed”. Ultimately the distance traveled by the rider was also called “Bareed”.

 

(Extract from book “Jawahar Ul Fiqah” by Hazrat Maulana Mufti Muhammad Shafi)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

CHAPTER 10

 

WHAT THE QUR’AN SAYS ABOUT ASTRONOMY

1) Big Bang - Creation of the heavens and earth:
"To Him is due the primal origin of the heavens and the earth; when He decrees a matter He said to it: "Be"; and it is." (2:117)

2) Stars are fixed to guide the travelers in the land and the sea:
"And it is He who ordained the stars for you that you may be guided thereby in the darkness of the land and the sea." (6:97)

3) Judgment Day:
"One day the Earth will be changed to a different Earth and so will be the Heavens and (men) will be marshalled forth before Allah the One the Irresistible." (14:48)

4) Constellations:
"And verily in the skies We have set constellations and beautified it for beholders." (15:16)

5) Stars and other signs to be used for directions:
"And marks and sign-posts and by the stars, (men) guide themselves." (16:16)

6) Creation of Mankind and Heavens By Allah:
"See they not that Allah Who created the heavens and the earth has power to create the like of them (anew)?...." (17:99)

7) Big Bang:
"Don't the Unbelievers see that the universe was once joined together, then We burst it apart. We made from water every living thing. Will they not then believe." (21:30)

8) Sun Moon Stars subjected to His Law:
"If indeed thou ask them who has created the heavens and the earth and subjected the sun and the moon (to His Law); they will certainly reply Allah." (29:61)

9) Sun is moving:
"And the sun runs towards its destination (resting place) ...." (36:38)

10) Gaseous state of universe:
"Then He turned to the sky when it had been gas and said to it and the earth, condense willingly or unwillingly. And they said, "We condensed willingly." (41:11)

11) Creation of the heavens and earth, not mere idle play:
"We have not created the heaven and the earth and all that is between them in mere idle play. None of this have We created without an inner truth: but most of them understand it not." (44:38-39)

12) Expansion of the universe:
"And the universe, we constructed with power and skill and verily we are expanding it." (51:47)

13) Sirius (the Mighty Star):
"And He is the Lord of Sirius (the Mighty Star)" (53:49)

14) Space flight:
"O assembly of Jinns and men when you can penetrate regions of the heavens and the earth, then penetrate them! Not without power (or authority) will you be able to pass." (55:33)

15) Other galaxies:
"God is the One Who created seven heavens and of the earth a similar number. The command descends upon them so that you know that God has power over all things and comprehends all things in His knowledge." (65:12)

16) Seven Heavens, Stars, and the skies:
"He Who created the seven heavens, one above another: No want of proportion will you see in the creation of Most Gracious, so turn your face again; Do you see any flaw ....... And We have adorned the lowest heaven with lamps ...." (67:3-5)

17) Seven Heavens:
"See ye not how Allah has created the seven heavens one above another." (71:15)

18) Signs of Qiyamah (Judgment Day):
"When the stars are put out and when the sky is cleft asunder." (77:8-9)

19) Seven Heavens and the Sun:
"We have built above you seven strong (heavens) and placed a blazing lamp." (78:12-13)

20) Creation of Mankind and Heavens By Allah:
What! are ye the more difficult to create, Or the heaven (above)? (Allah) has constructed it; On high has He raised its canopy and He has given it order and perfection; Its night does He endow with darkness and its splendor does He bring out (with light). (79:27-29)

21) Signs of Qiyamah (Judgment Day):
"When the sun is folded up and when the stars loose their lustre." (81:1-2)

22) Planets (Retrograde Motion):
"So verily I call to witness the planets that recede." (81:15)

23) Signs of Qiyamah (Judgment Day):
"When the sky is cleft asunder and the planets are scattered and the oceans are forced to join." (82:1-3)

24) Signs of Qiyamah (Judgment Day):
"When the sky is split asunder and attentive to her lord, and it must do so." (84:1-2)

25) Constellations:
"Consider the sky full of great constellations." (85:1)

26) Moon, Stars, and Planets:
"By the sky and the night-visitant; and what do you know what the night-visitant is? It is the star of piercing brightness." (86:1-3)

27) Sky Raised High:
"And at the Sky how it is raised high?" (88:18)

 

 

WHAT THE QUR’AN SAYS ABOUT THE MOON

1) Crescent moon as the standard to be used for reckoning of time:
"They ask you about the waxing and waning phases of the crescent moons, say they are to mark fixed times for mankind and Hajj." (2:189)

2) Moon is not my Lord:
"When he saw the moon rising in splendor He said: "This is my Lord." but when the moon set he said: Unless my Lord guide me I shall surely be among those who go astray." (6:77)

3) Sun and Moon to be used for reckoning of time:
"And He who made the night for rest and sun and moon for reckoning of time. This is the decree of the Exalted, the All-knowing." (6:96)

4) Sun, moon, and the stars governed by laws:
"Allah is He, who created the sun, the moon, and the stars (all) governed by laws under His commandment." (7:54)

5) Moon is the measure of month:
"The number of months in the sight of Allah is twelve (in a year) so ordained by Him the day He created the heavens and the earth; of them four are sacred; that is the straight usage.......Verily the transposing (of a prohibited month) is an addition to unbelief: the unbelievers are led to wrong thereby: for they make it lawful one year and forbidden another year in order to adjust the number of months forbidden by Allah and make such forbidden ones lawful. The evil of their course seems pleasing to them. But Allah guideth not those who reject faith." (9:36-37)

6) Sun is source of light and Moon is just light:
"It is He who made sun a lamp, and moon a light and measured stages so you know number of years and count (of time)." (10:5)

7) Joseph's Dream:
"Behold Joseph said to his father: O my father! I did see eleven stars and the sun and the moon: I saw them prostrate themselves to me!"

8) Sun and moon continue in an orbit to their destiny:
"Allah is He who raised heavens without pillars that you can see; Then He established Himself on the throne; And He subjected the sun and the moon (to his law); each one runs its course for a term appointed." (13:2)

9) Allah created Sun and moon, and He made them subject to you:
"It is Allah Who hath created the heavens and the earth and sendeth down rain from the skies......... He has made subject to you, the night and the day; the sun and the moon; and the stars in subjection by His command." (14:32-33)

10) Day and night, sun and moon, and stars made for you:
"He has made subject to you, the night and the day; the sun and the moon; and the stars in subjection by His command." (16:12)

11) Sun bright - Moon dark (no light):
"We made night and day two signs. The sign of night we made dark and sign of day we made bright. That ye may seek bounty from your lord and ye may know number of years and count (of time)." (17:12)

12) Orbits of celestial bodies:
"It is He who created the night and the day, and the sun and the moon, all (the celestial bodies) swim along, each in its orbit." (21:33)

13) All things bow down to Allah:
"See you not that to Allah bow down in worship all things in the heavens and on earth, the sun, the moon, the stars." (22:18)

14) Moon is reflected light of the sun:
"Blessed is He who made constellations in the skies, and placed therein a lamp and a moon reflecting light (25:61)

15) Sun and moon are subjected to Allah's laws
If indeed thou asl them Who has created the heavens and the earth and subjected (to His Law), they will certainly reply, "Allah". How are they then deluded away (from the truth)? (29:61)

16) Sun and moon continue in an orbit to their destiny:
"See you not Allah merges night into day and day into night; And subjected the sun and the moon (to His Law); each one runs its course for a term appointed." (31:29)

17) Sun and moon continue in an orbit to their destiny:
"He merges night into day and day into night; And subjected the sun and the moon (to His Law); each one runs its course for a term appointed." (35:13)

18) Ordained orbits of celestial bodies:
"And the moon, we have measured for her mansions (to traverse) till she returns like the old, (withered, and curved-up like a sickle) date-palm. It is not permitted for sun to catch-up the moon, nor can the night outstrip the day; each swims along in (its own) orbit." (36:39-40)

19) Sun and moon continue in an orbit to their destiny:
"He created heavens and the earth in true proportions; He makes night overlap day and day overlap night and subjected the sun and the moon (to His Law); each one runs its course for a term appointed." (39:5)

20) Do not Prostrate to the Sun and Moon:
"Among His Signs are the Night and the Day and the sun and moon. Prostrate not to the Sun and the Moon but Prostrate to Allah Who created them if it is Him ye wish to serve." (41:37)

21) Moon is split asunder:
"The hour (of Judgment) is near and the moon is split asunder." (54:1)

22) Celestial bodies tied to orbits:
"The sun and the moon follow courses exactly computed." (55:05)

23) Sun is source of light and Moon is just light:
"And made the moon a light in their midst and made the sun as a (Glorious) lamp." (71:16)

24) Swear by the Moon:
"Nay verily: by the Moon." (74:32)

25) Signs of Qiyamah (Judgment Day):
"And the moon is buried in darkness. And the sun and moon are joined together." (75:8-9)

26) Moon becomes full:
"And the moon when it becomes full." (84:18)

27) Moon follows the sun:
"By the sun and its radiant brightness; By the moon as she follows him." (91:1-2)

 

 

 

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