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In the history of astronomy, Islamic astronomy or Arabic astronomy refers to the astronomical developments made in the Islamic world, particularly during the Islamic Golden Age (8th-13th centuries), and mostly written in the Arabic language. These developments mostly took place in the Middle East, Central Asia, Al-Andalusmarker, and North Africa, and later in Chinamarker and India. It closely parallels the genesis of other Islamic sciences in its assimilation of foreign material and the amalgamation of the disparate elements of that material to create a science. These included Sassanid, Hellenistic and Indian works in particular, which were translated and built upon. In turn, Islamic astronomy later had a significant influence on Indian, Byzantine and European astronomy (see Latin translations of the 12th century) as well as Chinese astronomy and Malianmarker astronomy.

A significant number of stars in the sky, such as Aldebaran and Altair, and astronomical terms such as alhidade, azimuth, and almucantar, are still today recognized with their Arabic names. A large corpus of literature from Islamic astronomy remains today, numbering approximately 10,000 manuscripts scattered throughout the world, many of which have not been read or catalogued. Even so, a reasonably accurate picture of Islamic activity in the field of astronomy can be reconstructed.

Islam and astronomy

Islam has affected astronomy directly and indirectly. A major impetus for the flowering of astronomy in Islam came from religious observances, which presented an assortment of problems in mathematical astronomy, specifically in spherical geometry.


In the 7th century, both Christians and Jews observed holy days, such as Easter and Passover, whose timing was determined by the phases of the moon. Both communities had confronted the fact that the approximately 29.5-day lunar months are not commensurable with the 365-day solar year. To solve the problem, Christians and Jews had adopted a scheme based on a discovery made in circa 430 BC by the Athenianmarker astronomer Meton. In the 19-year Metonic cycle, there were 12 years of 12 lunar months and seven years of 13 lunar months. The periodic insertion of a 13th month kept calendar dates in step with the seasons.

On the other hand, astronomers used Ptolemy's way to calculate the place of the moon and stars. The method Ptolemy used to solve spherical triangles was a clumsy one devised late in the first century by Menelaus of Alexandria. It involved setting up two intersecting right triangles; by applying Menelaus' theorem it was possible to solve one of the six sides, but only if the other five sides were known. To tell the time from the sun's altitude, for instance, repeated applications of Menelaus' theorem were required. For medieval Islamic astronomers, there was an obvious challenge to find a simpler trigonometric method.

Islamic attitude towards astronomy

Islam advised Muslims to find ways of using the stars. The Qur'an says: "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." On the basis of this advice Muslims began to develop better observational and navigational instruments, thus most navigational stars today have Arabic names.

Other influences of the Qur'an on Islamic astronomy included its "insistence that the Universe is ruled by a single set of laws" which was "rooted in the Islamic concept of tawhîd, the unity of God", as well its "greater respect for empirical data than was common in the preceding Greek civilization" which inspired Muslims to place a greater emphasis on empirical observation, in contrast to ancient Greek philosophers such as the Platonists and Aristotelians who expressed a general distrust towards the senses and instead viewed reason alone as being sufficient to understanding nature. The Qur'an's insistence on observation, reason and contemplation ("see", "think" and "contemplate"), on the other hand, led Muslims to develop an early scientific method based on these principles, particularly empirical observation. Muhammad Iqbal writes:

There are also several cosmological verses in the Qur'an (610-632) which some modern writers have interpreted as foreshadowing the expansion of the universe and possibly even the Big Bang theory:

Don't those who reject faith see that the heavens and the earth were a single entity then We ripped them apart?
And the heavens We did create with Our Hands, and We do cause it to expand.

Several hadiths attributed to Muhammad also show that he was generally opposed to astrology as well as superstition in general. An example of this is when an eclipse occurred during his son Ibrahim ibn Muhammad's death, and rumours began spreading about this being God's personal condolence. Muhammad is said to have replied:

"An eclipse is a phenomenon of nature.
It is foolish to attribute such things to the death or birth of a human being."

Islamic rules

There are several rules in Islam which lead Muslims to use better astronomical calculations and observations.

The first issue is the Islamic calendar. The Qur'an says: "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." Therefore Muslims could not follow the Christian or Hebrew calendars and they thus had to develop a new one.

The other issue is moon sighting. Islamic months do not begin at the astronomical new moon, defined as the time when the moon has the same celestial longitude as the sun and is therefore invisible; instead they begin when the thin crescent moon is first sighted in the western evening sky. The Qur'an says: "They ask you about the waxing and waning phases of the crescent moons, say they are to mark fixed times for mankind and Hajj."This led Muslims to find the phases of the moon in the sky, and their efforts led to new mathematical calculations and observational instruments, as well as a special science being formed specifically for moon sighting.

Muslims are also expected to pray towards the Kaabamarker in Meccamarker and orient their mosques in that direction. Thus they need to determine the direction of Mecca from a given location. Another influencing factor is the time of Salah. Muslims need to determine from celestial bodies the proper times for the prayers at sunrise, at midday, in the afternoon, at sunset, and in the evening.

Necessity of spherical geometry

Predicting just when the crescent moon would become visible is a special challenge to Islamic mathematical astronomers. Although Ptolemy's theory of the complex lunar motion was tolerably accurate near the time of the new moon, it specified the moon's path only with respect to the ecliptic. To predict the first visibility of the moon, it was necessary to describe its motion with respect to the horizon, and this problem demands fairly sophisticated spherical geometry (invented by Hipparchus and freely drawn on by Ptolemy. Finding the direction of Meccamarker and the time of Salah are the reasons which led to Muslims developing spherical geometry. Solving any of these problems involves finding the unknown sides or angles of a triangle on the celestial sphere from the known sides and angles. A way of finding the time of day, for example, is to construct a triangle whose vertices are the zenith, the north celestial pole, and the sun's position. The observer must know the altitude of the sun and that of the pole; the former can be observed, and the latter is equal to the observer's latitude. The time is then given by the angle at the intersection of the meridian (the arc through the zenith and the pole) and the sun's hour circle (the arc through the sun and the pole).


Pre-Islamic Arabian knowledge of stars was empirical; their knowledge was what they observed regarding the rising and setting of stars. The rise of Islam is claimed to have provoked increased Arab thought in this field. The foundations of Islamic astronomy closely parallels the genesis of other Islamic sciences in its assimilation of foreign material and the amalgamation of the disparate elements of that material to create a science that was essentially Islamic. These include Indian, Sassanid and Hellenistic works which were translated and built upon.

The science historian Donald Routledge Hill has divided the history of Islamic astronomy into the four following distinct time periods in its history:
  • Assimilation and syncretization of earlier Hellenistic, Indian and Sassanid astronomy (700—825 AD)
  • Vigorous investigation, and acceptance and modification to the Ptolemaic system (825—1025 AD)
  • Flourishing of a distinctive Islamic system of astronomy (1025—1450 AD)
  • Stagnation, where few significant contributions were made (1450—1900 AD)


From the beginning, Muslim community in Medina sight new moon to determine the lunar months especially Ramadan and holy days.

In approximately 638 A.D, Caliph Umar introduced a new lunar calendar which is known as lunar calendar was made on the basis of Islamic view point. This calendar has twelve lunar months, the beginnings of which are determined by the sighting of the crescent moon. This calendar is about 11 days shorter than the solar year. This calendar is still in use for religious purposes among Muslims.


This period was most notably the period of assimilation and syncretization of earlier Hellenistic, Indian and Sassanid astronomy occurred during the eighth and early ninth centuries.


Historians point out several factors that fostered the growth of Islamic astronomy. The first was the proximity of the Muslim world to the world of ancient learning. Much of the ancient Greek, Sanskrit and Middle Persian texts were translated into Arabic during the ninth century. This process was enhanced by the tolerance towards scholars of other religions.

Another impetus came from Islamic religious observances, which presented a host of problems in mathematical astronomy. In solving these religious problems the Islamic scholars went far beyond the Greek mathematical methods.

Ancient influences and translation movement

During this period, a number of Sanskrit and Middle Persian texts were first translated into Arabic. The most notable of the texts was Zij al-Sindhind, based on the Surya Siddhanta and the works of Brahmagupta, and translated by Muhammad al-Fazari and Yaqūb ibn Tāriq in 777. Sources indicate that the text was translated after an Indian astronomer visited the court of Caliph Al-Mansur in 770. The most notable Middle Persian text translated was the Zij al-Shah, a collection of astronomical tables compiled in Sassanid Persia over two centuries.

Fragments of text during this period indicate that Arabs adopted the sine function (inherited from Indian trigonometry) instead of the chord of arc used in Hellenistic mathematics. Another Indian influence was an approximate formula used for timekeeping by Muslim astronomers.

A page from Ptolemy's Almagest.
Islamic interest in astronomy ran parallel to the interest in mathematics. Especially noteworthy in this regard was the Almagest (c. 150) of the astronomer Ptolemy (c. 100-178). The Almagest was a landmark work in its field, assembling, as Euclid's Elements had previously done with geometrical works, all extant knowledge in the field of astronomy that was known to the author. This work was originally known as The Mathematical Composition, but after it had come to be used as a text in astronomy, it was called The Great Astronomer. The Islamic world called it The Greatest prefixing the Greek work megiste (greatest) with the article al- and it has since been known to the world as Al-megiste or, after popular use in Western translation, Almagest. though much of the Almagest was incorrect, even in premise, it remained a standard astronomical text in both the Islamic world and Europe until the Maragha Revolutionmarker and Copernican Revolution. Ptolemy also produced other works, such as Optics, Harmonica, and some suggest he also wrote Tetrabiblon.

The Almagest was a particularly unifying work for its exhaustive lists of sidereal phenomena. He drew up a list of chronological tables of Assyrian, Persian, Greek, and Roman kings for use in reckoning the lapse of time between known astronomical events and fixed dates. In addition to its relevance to calculating accurate calendars, it linked far and foreign cultures together by a common interest in the stars and astrology. The work of Ptolemy was replicated and refined over the years under Arab, Persian and other Muslim astronomers and astrologers.


The period throughout the ninth, tenth and early eleventh centuries was one of vigorous investigation, in which the superiority of the Ptolemaic system of astronomy was accepted and significant contributions made to it. Astronomical research was greatly supported by the Abbasid caliph al-Mamun. Baghdadmarker and Damascusmarker became the centers of such activity. The caliphs not only supported this work financially, but endowed the work with formal prestige.

Observational astronomy

In observational astronomy, the first major original Muslim work of astronomy was Zij al-Sindh by al-Khwarizimi in 830. The work contains tables for the movements of the sun, the moon and the five planets known at the time. The work is significant as it introduced Indian and Ptolemaic concepts into Islamic sciences. This work also marked the turning point in Islamic astronomy. Hitherto, Muslim astronomers had adopted a primarily research approach to the field, translating works of others and learning already discovered knowledge. Al-Khwarizmi's work marked the beginning of non-traditional methods of study and calculations.

In 850, al-Farghani wrote Kitab fi Jawani ("A compendium of the science of stars"). The book primarily gave a summary of Ptolemic cosmography. However, it also corrected Ptolemy's Almagest based on findings of earlier Iranian astronomers. Al-Farghani gave revised values for the obliquity of the ecliptic, the precessional movement of the apogees of the sun and the moon, and the circumference of the earth. The books were widely circulated through the Muslim world, and even translated into Latin.

Muhammad ibn Jābir al-Harrānī al-Battānī (Albatenius) (853-929) discovered that the direction of the Sun's eccentric was changing, which in modern astronomy is equivalent to the Earth moving in an elliptical orbit around the Sun. His times for the new moon, lengths for the solar year and sidereal year, prediction of eclipses, and work on the phenomenon of parallax, carried astronomers "to the verge of relativity and the space age." Around the same time, Yahya Ibn Abi Mansour carried out extensive observations and tests, and wrote the Al-Zij al-Mumtahan, in which he completely revised the Almagest values.

In the 10th century, Abd al-Rahman al-Sufi (Azophi) carried out observations on the stars and described their positions, magnitude, brightness, and colour and drawings for each constellation in his Book of Fixed Stars (964). He also gave the first descriptions and pictures of "A Little Cloud" now known as the Andromeda Galaxy. He mentions it as lying before the mouth of a Big Fish, an Arabic constellation. This "cloud" was apparently commonly known to the Isfahanmarker astronomers, very probably before 905 AD. The first recorded mention of the Large Magellanic Cloud was also given by Abd Al-Rahman al-Sufi.

Ibn Yunus observed more than 10,000 entries for the sun's position for many years using a large astrolabe with a diameter of nearly 1.4 meters. His observations on eclipses were still used centuries later in Simon Newcomb's investigations on the motion of the moon, while his other observations inspired Laplace's Obliquity of the Ecliptic and Inequalities of Jupiter and Saturn's.

Abu-Mahmud al-Khujandi relatively accurately computed the axial tilt to be 23°32'19" (23.53°),.In 1006, the Egyptianmarker astronomer Ali ibn Ridwan observed SN 1006, the brightest supernova in recorded history, and left a detailed description of the temporary star. He says that the object was two to three times as large as the disc of Venus and about one-quarter the brightness of the Moon, and that the star was low on the southern horizon. Monks at the Benedictine abbey at St. Gallmarker later corroborated bin Ridwan's observations as to magnitude and location in the sky.

Early heliocentric models

In the late ninth century, Ja'far ibn Muhammad Abu Ma'shar al-Balkhi (Albumasar) developed a planetary model which some have interpreted as a heliocentric model. This is due to his orbital revolutions of the planets being given as heliocentric revolutions rather than geocentric revolutions, and the only known planetary theory in which this occurs is in the heliocentric theory. His work on planetary theory has not survived, but his astronomical data was later recorded by al-Hashimi, Abū Rayhān al-Bīrūnī and al-Sijzi.

In the early eleventh century, al-Biruni had met several Indian scholars who believed in a heliocentric system. In his Indica, he discusses the theories on the Earth's rotation supported by Brahmagupta and other Indian astronomers, while in his Canon Masudicus, al-Biruni writes that Aryabhata's followers assigned the first movement from east to west to the Earth and a second movement from west to east to the fixed stars. Al-Biruni also wrote that al-Sijzi also believed the Earth was moving and invented an astrolabe called the "Zuraqi" based on this idea:

In his Indica, al-Biruni briefly refers to his work on the refutation of heliocentrism, the Key of Astronomy, which is now lost:


In contrast to ancient Greek philosophers who believed that the universe had an infinite past with no beginning, medieval philosophers and theologians developed the concept of the universe having a finite past with a beginning (see Temporal finitism). This view was inspired by the creation myth shared by the three Abrahamic religions: Judaism, Christianity and Islam. The Christian philosopher, John Philoponus, presented the first such argument against the ancient Greek notion of an infinite past. However, the most sophisticated medieval arguments against an infinite past were developed by the early Muslim philosopher, Al-Kindi (Alkindus); the Jewish philosopher, Saadia Gaon (Saadia ben Joseph); and the Muslim theologian, Al-Ghazali (Algazel). They developed two logical arguments against an infinite past, the first being the "argument from the impossibility of the existence of an actual infinite", which states:

"An actual infinite cannot exist."
"An infinite temporal regress of events is an actual infinite."
".•. An infinite temporal regress of events cannot exist."

The second argument, the "argument from the impossibility of completing an actual infinite by successive addition", states:

"An actual infinite cannot be completed by successive addition."
"The temporal series of past events has been completed by successive addition."
".•. The temporal series of past events cannot be an actual infinite."

Both arguments were adopted by later Christian philosophers and theologians, and the second argument in particular became more famous after it was adopted by Immanuel Kant in his thesis of the first antimony concerning time.

Experimental astronomy, astrophysics, celestial mechanics

In the 9th century, the eldest Banū Mūsā brother, Ja'far Muhammad ibn Mūsā ibn Shākir, made significant contributions to astrophysics and celestial mechanics. He was the first to hypothesize that the heavenly bodies and celestial spheres are subject to the same laws of physics as Earth, unlike the ancients who believed that the celestial spheres followed their own set of physical laws different from that of Earth. In his Astral Motion and The Force of Attraction, Muhammad ibn Musa also proposed that there is a force of attraction between heavenly bodies, foreshadowing Newton's law of universal gravitation.

In the 10th century, Muhammad ibn Jābir al-Harrānī al-Battānī (Albatenius) (853-929) introduced the idea of testing "past observations by means of new ones". This led to the use of exacting empirical observations and experimental techniques by Muslim astronomers from the eleventh century onwards.

In the early 11th century, Ibn al-Haytham (Alhazen) wrote the Maqala fi daw al-qamar (On the Light of the Moon) some time before 1021. This was the first attempt successful at combining mathematical astronomy with physics and the earliest attempt at applying the experimental method to astronomy and astrophysics. He disproved the universally held opinion that the moon reflects sunlight like a mirror and correctly concluded that it "emits light from those portions of its surface which the sun's light strikes." In order to prove that "light is emitted from every point of the moon's illuminated surface," he built an "ingenious experimental device." Ibn al-Haytham had "formulated a clear conception of the relationship between an ideal mathematical model and the complex of observable phenomena; in particular, he was the first to make a systematic use of the method of varying the experimental conditions in a constant and uniform manner, in an experiment showing that the intensity of the light-spot formed by the projection of the moonlight through two small apertures onto a screen diminishes constantly as one of the apertures is gradually blocked up."

Ibn al-Haytham, in his Book of Optics (1021), was also the first to discover that the celestial spheres do not consist of solid matter, and he also discovered that the heavens are less dense than the air. These views were later repeated by Witelo and had a significant influence on the Copernican and Tychonic systems of astronomy.

Ibn al-Haytham also refuted Aristotle's view on the Milky Way galaxy. Aristotle believed the Milky Way to be caused by "the ignition of the fiery exhalation of some stars which were large, numerous and close together" and that the "ignition takes place in the upper part of the atmosphere, in the region of the world which is continuous with the heavenly motions." Ibn al-Haytham refuted this by making the first attempt at observing and measuring the Milky Way's parallax, and he thus "determined that because the Milky Way had no parallax, it was very remote from the earth and did not belong to the atmosphere."

Also in the early 11th century, Abū Rayhān al-Bīrūnī introduced the experimental method into astronomy and was the first to conduct elaborate experiments related to astronomical phenomena. He discovered the Milky Way galaxy to be a collection of numerous nebulous stars. In Afghanistanmarker, he observed and described the solar eclipse on April 8, 1019, and the lunar eclipse on September 17, 1019, in detail, and gave the exact latitudes of the stars during the lunar eclipse.


During this period, a distinctive Islamic system of astronomy flourished. It was Greek tradition to separate mathematical astronomy (as typified by Ptolemy) from philosophical cosmology (as typified by Aristotle). Muslim scholars developed a program of seeking a physically real configuration (hay'a) of the universe, that would be consistent with both mathematical and physical principles. Within the context of this hay'a tradition, Muslim astronomers began questioning technical details of the Ptolemaic system of astronomy. Most of these criticisms, however, continued to follow the Ptolemaic astronomical paradigm, remaining within the geocentric framework. As the historian of astronomy, A. I. Sabra, noted:

Some Muslim astronomers, however, most notably Abū Rayhān al-Bīrūnī and Nasīr al-Dīn al-Tūsī, discussed whether the Earth moved and considered how this might be consistent with astronomical computations and physical systems. Several other Muslim astronomers, most notably those following the Maragha schoolmarker of astronomy, developed non-Ptolemaic planetary models within a geocentric context that were later adapted by the Copernican model in a heliocentric context.

Refutations of astrology

The first semantic distinction between astronomy and astrology was given by the Persian astronomer Abu Rayhan al-Biruni in the 11th century, though he himself refuted astrology in another work. The study of astrology was also refuted by other Muslim astronomers at the time, including al-Farabi, Ibn al-Haytham, Avicenna and Averroes. Their reasons for refuting astrology were often due to both scientific (the methods used by astrologers being conjectural rather than empirical) and religious (conflicts with orthodox Islamic scholars) reasons.

Ibn Qayyim Al-Jawziyya (1292-1350), in his Miftah Dar al-SaCadah, used empirical arguments in astronomy in order to refute the practice of astrology and divination. He recognized that the stars are much larger than the planets, and thus argued:

Al-Jawziyya also recognized the Milky Way galaxy as "a myriad of tiny stars packed together in the sphere of the fixed stars" and thus argued that "it is certainly impossible to have knowledge of their influences."

Astrophysics and celestial mechanics

In astrophysics and celestial mechanics, Abū Rayhān al-Bīrūnī described the Earth's gravitation as:

Al-Biruni also discovered that gravity exists within the heavenly bodies and celestial spheres, and he criticized the Aristotelian views of them not having any levity or gravity and of circular motion being an innate property of the heavenly bodies.

In 1121, al-Khazini, in his treatise The Book of the Balance of Wisdom, states:

Al-Khazini was thus the first to propose the theory that the gravity or gravitational potential energy of a body varies depending on its distances from the centre of the Earth. This phenomenon was not proven until the 18th century, following Newton's law of universal gravitation.

Beginning of hay'a tradition

Between 1025 and 1028, Ibn al-Haytham (Latinized as Alhazen), began the hay'a tradition of Islamic astronomy with his Al-Shuku ala Batlamyus (Doubts on Ptolemy). While maintaining the physical reality of the geocentric model, he was the first to criticize Ptolemy's astronomical system, which he criticized on empirical, observational and experimental grounds, and for relating actual physical motions to imaginary mathematical points, lines and circles:

Ibn al-Haytham developed a physical structure of the Ptolemaic system in his Treatise on the configuration of the World, or Maqâlah fî hay'at al-‛âlam, which became an influential work in the hay'a tradition. In his Epitome of Astronomy, he insisted that the heavenly bodies "were accountable to the laws of physics."

In 1038, Ibn al-Haytham described the first non-Ptolemaic configuration in The Model of the Motions. His reform was not concerned with cosmology, as he developed a systematic study of celestial kinematics that was completely geometric. This in turn led to innovative developments in infinitesimal geometry. His reformed model was the first to reject the equant and eccentrics, separate natural philosophy from astronomy, free celestial kinematics from cosmology, and reduce physical entities to geometrical entities. The model also propounded the Earth's rotation about its axis, and the centres of motion were geometrical points without any physical significance, like Johannes Kepler's model centuries later. Ibn al-Haytham also describes an early version of Occam's razor, where he employs only minimal hypotheses regarding the properties that characterize astronomical motions, as he attempts to eliminate from his planetary model the cosmological hypotheses that cannot be observed from Earth.

Early alternative models

In 1030, Abū al-Rayhān al-Bīrūnī discussed the Indian planetary theories of Aryabhata, Brahmagupta and Varahamihira in his Ta'rikh al-Hind (Latinized as Indica). Biruni stated that Brahmagupta and others consider that the earth rotates on its axis and Biruni noted that this does not create any mathematical problems.

Abu Said al-Sijzi, a contemporary of al-Biruni, suggested the possible heliocentric movement of the Earth around the Sun, which al-Biruni did not reject. Al-Biruni agreed with the Earth's rotation about its own axis, and while he was initially neutral regarding the heliocentric and geocentric models, he considered heliocentrism to be a philosophical problem. He remarked that if the Earth rotates on its axis and moves around the Sun, it would remain consistent with his astronomical parameters:

In 1031, al-Biruni completed his extensive astronomical encyclopaedia Kitab al-Qanun al-Mas'udi (Latinized as Canon Mas’udicus), in which he recorded his astronomical findings and formulated astronomical tables. In it he presented a geocentric model, tabulating the distance of all the celestial spheres from the central Earth, computed according to the principles of Ptolemy's Almagest. The book introduces the mathematical technique of analysing the acceleration of the planets, and first states that the motions of the solar apogee and the precession are not identical. Al-Biruni also discovered that the distance between the Earth and the Sun is larger than Ptolemy's estimate, on the basis that Ptolemy disregarded the annual solar eclipses.

In 1070, Abu Ubayd al-Juzjani, a pupil of Avicenna, proposed a non-Ptolemaic configuration in his Tarik al-Aflak. In his work, he indicated the so-called "equant" problem of the Ptolemic model, and proposed a solution for the problem. He claimed that his teacher Avicenna had also worked out the equant problem.

Andalusian Revolt

In the 11th-12th centuries, astronomers in al-Andalusmarker took up the challenge earlier posed by Ibn al-Haytham, namely to develop an alternate non-Ptolemaic configuration that evaded the errors found in the Ptolemaic model. Like Ibn al-Haytham's critique, the anonymous Andalusian work, al-Istidrak ala Batlamyus (Recapitulation regarding Ptolemy), included a list of objections to Ptolemic astronomy. This marked the beginning of the Andalusian school's revolt against Ptolemaic astronomy, otherwise known as the "Andalusian Revolt".

In the late 11th century, al-Zarqali (Latinized as Arzachel) discovered that the orbits of the planets are elliptic orbits and not circular orbits, though he still followed the Ptolemaic model.

In the 12th century, Averroes rejected the eccentric deferents introduced by Ptolemy. He rejected the Ptolemaic model and instead argued for a strictly concentric model of the universe. He wrote the following criticism on the Ptolemaic model of planetary motion:

Averroes' contemporary, Maimonides, wrote the following on the planetary model proposed by Ibn Bajjah (Avempace):

Ibn Bajjah also proposed the Milky Way galaxy to be made up of many stars but that it appears to be a continuous image due to the effect of refraction in the Earth's atmosphere. Later in the 12th century, his successors Ibn Tufail and Nur Ed-Din Al Betrugi (Alpetragius) were the first to propose planetary models without any equant, epicycles or eccentrics. Al-Betrugi was also the first to discover that the planets are self-luminous. Their configurations, however, were not accepted due to the numerical predictions of the planetary positions in their models being less accurate than that of the Ptolemaic model, mainly because they followed Aristotle's notion of perfect circular motion.

Maragha Revolution

The "Maragha Revolution" refers to the Maraghehmarker school's revolution against Ptolemaic astronomy. The "Maragha school" was an astronomical tradition beginning in the Maragheh observatorymarker and continuing with astronomers from Damascusmarker and Samarkandmarker. Like their Andalusian predecessors, the Maragha astronomers attempted to solve the equant problem and produce alternative configurations to the Ptolemaic model. They were more successful than their Andalusian predecessors in producing non-Ptolemaic configurations which eliminated the equant and eccentrics, were more accurate than the Ptolemaic model in numerically predicting planetary positions, and were in better agreement with empirical observations. The most important of the Maragha astronomers included Mo'ayyeduddin Urdi (d. 1266), Nasīr al-Dīn al-Tūsī (1201-1274), 'Umar al-Katibi al-Qazwini (d. 1277), Qutb al-Din al-Shirazi (1236-1311), Sadr al-Sharia al-Bukhari (c. 1347), Ibn al-Shatir (1304-1375), Ali al-Qushji (c. 1474), al-Birjandi (d. 1525) and Shams al-Din al-Khafri (d. 1550).

Some have described their achievements in the 13th and 14th centuries as a "Maragha Revolution", "Maragha School Revolution", or "Scientific Revolution before the Renaissance". An important aspect of this revolution included the realization that astronomy should aim to describe the behavior of physical bodies in mathematical language, and should not remain a mathematical hypothesis, which would only save the phenomena. The Maragha astronomers also realized that the Aristotelian view of motion in the universe being only circular or linear was not true, as the Tusi-couple showed that linear motion could also be produced by applying circular motions only.

Unlike the ancient Greek and Hellenistic astronomers who were not concerned with the coherence between the mathematical and physical principles of a planetary theory, Islamic astronomers insisted on the need to match the mathematics with the real world surrounding them, which gradually evolved from a reality based on Aristotelian physics to one based on an empirical and mathematical physics after the work of Ibn al-Shatir. The Maragha Revolution was thus characterized by a shift away from the philosophical foundations of Aristotelian cosmology and Ptolemaic astronomy and towards a greater emphasis on the empirical observation and mathematization of astronomy and of nature in general, as exemplified in the works of Ibn al-Shatir, al-Qushji, al-Birjandi and al-Khafri.

Other achievements of the Maragha school include the first empirical observational evidence for the Earth's rotation on its axis by al-Tusi and al-Qushji, the separation of natural philosophy from astronomy by Ibn al-Shatir and al-Qushji, the rejection of the Ptolemaic model on empirical rather than philosophical grounds by Ibn al-Shatir, and the development of a non-Ptolemaic model by Ibn al-Shatir that was mathematically identical to the heliocentric Copernical model.

Mo'ayyeduddin Urdi (d. 1266) was the first of the Maragheh astronomers to develop a non-Ptolemaic model, and he proposed a new theorem, the "Urdi lemma". Nasīr al-Dīn al-Tūsī (1201-1274) resolved significant problems in the Ptolemaic system by developing the Tusi-couple as an alternative to the physically problematic equant introduced by Ptolemy, and conceived a plausible model for elliptical orbits. Tusi's student Qutb al-Din al-Shirazi (1236-1311), in his The Limit of Accomplishment concerning Knowledge of the Heavens, discussed the possibility of heliocentrism. 'Umar al-Katibi al-Qazwini (d. 1277), who also worked at the Maragheh observatory, in his Hikmat al-'Ain, wrote an argument for a heliocentric model, though he later abandoned the idea.

Ibn al-Shatir (1304–1375) of Damascusmarker, in A Final Inquiry Concerning the Rectification of Planetary Theory, incorporated the Urdi lemma, and eliminated the need for an equant by introducing an extra epicycle (the Tusi-couple), departing from the Ptolemaic system in a way that was mathematically identical to what Nicolaus Copernicus did in the 16th century. Unlike previous astronomers before him, Ibn al-Shatir was not concerned with adhering to the theoretical principles of natural philosophy or Aristotelian cosmology, but rather to produce a model that was more consistent with empirical observations. For example, it was Ibn al-Shatir's concern for observational accuracy which led him to eliminate the epicycle in the Ptolemaic solar model and all the eccentrics, epicycles and equant in the Ptolemaic lunar model. His model was thus in better agreement with empirical observations than any previous model, and was also the first that permitted empirical testing. His work thus marked a turning point in astronomy, which may be considered a "Scientific Revolution before the Renaissance". His rectified model was later adapted into a heliocentric model by Copernicus, which was mathematically achieved by reversing the direction of the last vector connecting the Earth to the Sun. In the published version of his masterwork, De revolutionibus orbium coelestium, Copernicus also cites the theories of al-Battani, Arzachel and Averroes as influences, while the works of Ibn al-Haytham and al-Biruni were also known in Europe at the time.

An area of active discussion in the Maragheh school, and later the Samarkandmarker and Istanbulmarker observatories, was the possibility of the Earth's rotation. Supporters of this theory included Nasīr al-Dīn al-Tūsī, Nizam al-Din al-Nisaburi (c. 1311), al-Sayyid al-Sharif al-Jurjani (1339-1413), Ali al-Qushji (d. 1474), and Abd al-Ali al-Birjandi (d. 1525). Al-Tusi was the first to present empirical observational evidence of the Earth's rotation, using the location of comets relevant to the Earth as evidence, which al-Qushji elaborated on with further empirical observations while rejecting Aristotelian natural philosophy altogether. Both of their arguments were similar to the arguments later used by Nicolaus Copernicus in 1543 to explain the Earth's rotation (see Astronomical physics and Earth's motion section below).

Islamic astronomy in China

Muslim astronomers were brought to Chinamarker work on calendar making and astronomy during the Yuan Dynastymarker. Kublai Khan brought Iranians to Beijing to construct an observatory and an institution for astronomical studies. Jamal ad-Din, a Persian astronomer, presented Kublai Khan with seven Persian astronomical instruments, including a Persian globe and an armillary sphere, in 1267. Several Chinese astronomers also worked at the Maragheh observatorymarker in Persia.

Islamic astronomy in Europe

During this period, Islamic-ruled regions of Europe, such as Al-Andalusmarker, the Emirate of Sicily, and southern Italy, were slowly being reconquered by Christians. This led to the Arabic-Latin translation movement, which saw the assimilation of knowledge from the Islamic world by Western European science, including astronomy. In addition, Byzantine astronomers also translated Arabic texts on astronomy into Medieval Greek during this time. In particular, Gregory Choniades translated several Zij treatises, including the Zij-i Ilkhani of the Maragheh observatorymarker, and may have played a role in the transmission of their work (such as the Tusi-couple) to Europe, where it eventually influenced Copernican heliocentrism.


This period was considered the period of stagnation, when the traditional system of astronomy continued to be practised with enthusiasm, but with decreasing innovation. It was believed there was no innovation of major significance during this period, but this view has been rejected by historians of astronomy in recent times, who argue that Muslim astronomers continued to make significant advances in astronomy through to the 16th century and possibly after this as well. After the 16th century, there appears to have been little concern for theoretical astronomy, but observational astronomy in the Islamic tradition continued in the three Muslim gunpowder empires: the Ottoman Empire, the Safavid dynasty of Persia, and the Mughal Empire of India.

Astronomical physics and Earth's motion

The work of Ali al-Qushji (d. 1474), who worked at Samarkandmarker and then Istanbulmarker, is seen as a late example of innovation in Islamic theoretical astronomy and it is believed he may have possibly had some influence on Nicolaus Copernicus due to similar arguments concerning the Earth's rotation. Before al-Qushji, the only astronomer to present empirical evidence for the Earth's rotation was Nasīr al-Dīn al-Tūsī (d. 1274), who used the phenomena of comets to refute Ptolemy's claim that a stationery Earth can be determined through observation. Al-Tusi, however, eventually accepted that the Earth was stationery on the basis of Aristotelian cosmology and natural philosophy. By the 15th century, the influence of Aristotelian physics and natural philosophy was declining due to religious opposition from Islamic theologians. Under this influence, Al-Qushji, in his Concerning the Supposed Dependence of Astronomy upon Philosophy, rejected Aristotelian physics and completely separated natural philosophy from astronomy, allowing astronomy to become a purely empirical and mathematical science. This allowed him to explore alternatives to the Aristotelian notion of a stationery Earth, as he explored the idea of a moving Earth. He also observed comets and elaborated on al-Tusi's argument. He took it a step further and concluded, on the basis of empirical evidence rather than speculative philosophy, that the moving Earth theory is just as likely to be true as the stationary Earth theory and that it is not possible to empirically deduce which theory is true. His work was an important step away from Aristotelian physics and towards an independent astronomical physics.

Despite the similarity in their discussions regarding the Earth's motion, there is uncertainty over whether al-Qushji had any influence on Copernicus. However, it is likely that they both may have arrived at similar conclusions due to using the earlier work of al-Tusi as a basis. This is more of a possibility considering "the remarkable coincidence between a passage in De revolutionibus (I.8) and one in Ṭūsī’s Tadhkira (II.1[6]) in which Copernicus follows Ṭūsī’s objection to Ptolemy’s “proofs” of the Earth’s immobility." This can be considered as evidence that not only was Copernicus influenced by the mathematical models of Islamic astronomers, but may have also been influenced by the astronomical physics they began developing and their views on the Earth's motion.

In the 16th century, the debate on the Earth's motion was continued by al-Birjandi (d. 1528), who in his analysis of what might occur if the Earth were rotating, develops a hypothesis similar to Galileo Galilei's notion of "circular inertia", which he described in the following observational test (as a response to one of Qutb al-Din al-Shirazi's arguments):

Planetary theory

It was traditionally believed that Islamic astronomers made no more advances in planetary theory after the work of Ibn al-Shatir in the 14th century, but recent studies have shown that there were several significant advances in planetary theory through to the 16th century, after George Saliba studied the works of a 16th century astronomer, Shams al-Din al-Khafri (d. 1550), a Safavid commentator on earlier Maragha astronomersmarker. Saliba wrote the following on al-Khafri's work:

Ali al-Qushji also improved on al-Tusi's planetary model and presented an alternative planetary model for Mercury.

Ottoman observational astronomy

Another notable 16th century Muslim astronomer was the Ottoman astronomer Taqi al-Din, who built the Istanbul observatory of al-Din in 1577, where he carried out astronomical observations until 1580. He produced a Zij (named Unbored Pearl) and astronomical catalogues that were more accurate than those of his contemporaries, Tycho Brahe and Nicolaus Copernicus. Al-Din was also the first astronomer to employ a decimal point notation in his observations rather than the sexagesimal fractions used by his contemporaries and predecessors. He also invented a variety of astronomical instruments, including accurate mechanical astronomical clocks from 1556 to 1580.

Earlier in 1574, al-Din used astrophysics to explain the intromission model of vision. He stated since the stars are millions of kilometers away from the Earth and that the speed of light is constant, that if light had come from the eye, it would take too long for light "to travel to the star and come back to the eye. But this is not the case, since we see the star as soon as we open our eyes. Therefore the light must emerge from the object not from the eyes."

After the destruction of the Istanbul observatory of al-Din in 1580, astronomical activity stagnated in the Ottoman Empire, until the introduction of Copernican heliocentrism in 1660, when the Ottoman scholar Ibrahim Efendi al-Zigetvari Tezkireci translated Noël Duret's French astronomical work (written in 1637) into Arabic.

Islamic astronomy in India

Meanwhile in the Mughal Empire, the 16th and 17th centuries saw a synthesis between Islamic and Indian astronomy, where Islamic observational techniques and instruments were combined with Hindu computational techniques. While there appears to have been little concern for theoretical astronomy, Muslim and Hindu astronomers in India continued to make advances in observational astronomy and produced nearly a hundred Zij treatises. Humayun built a personal observatory near Delhimarker, while Jahangir and Shah Jahan were also intending to build observatories but were unable to do so. After the decline of the Mughal Empire, however, it was a Hindu king, Jai Singh II of Amber, who attempted to revive the Islamic tradition of astronomy in India. In the early 18th century, he built several large observatories called Yantra Mandirsmarker in order to rival the famous Samarkand observatory, and in order to update Ulugh Beg's Zij-i-Sultani with more accurate observations. The instruments and observational techniques used at the observatory were mainly derived from the Islamic tradition, and the computational techniqes from the Hindu tradition. In particular, one of the most remarkable astronomical instruments invented by Muslims in Mughal India is the seamless celestial globe (see Globes below).

Jai Singh also invited European Jesuit astronomers to his observatory, who had bought back the astronomical tables compiled by Philippe de La Hire in 1702. After examining La Hire's work, Jai Singh concluded that the techniques and instruments used in the European tradition were inferior to the Islamic and Indian traditions. It is uncertain whether Islamic astronomers in India were aware of the Copernican Revolution via the Jesuits, but it appears they were not concerned with theoretical astronomy, hence the theoretical advances in Europe did not interest them at the time.


In the 20th and 21st centuries, Muslim astronomers have been making advances in moon sighting, while Muslim astronauts and rocket scientists have been involved in research on astronautics and space exploration.

Astronautics and space exploration

Kerim Kerimov from Azerbaijanmarker (then part of the Soviet Unionmarker) was one of the most important key figures in early space exploration. He was one of the founders of the Soviet space program, one of the lead architects behind the first satellite (Sputnik 1) and first human spaceflight (Vostok 1), and responsible for the launch of the first space docks (the Cosmos 186 and Cosmos 188) and the first space stations (the Salyut and Mir series).

Farouk El-Baz from Egyptmarker worked for the rival NASAmarker and was involved in the first Moon landings with the Apollo program, where he was secretary of the Landing Site Selection Committee, Principal Investigator of Visual Observations and Photography, chairman of the Astronaut Training Group, and assisted in the planning of scientific explorations of the Moon, including the selection of landing sites for the Apollo missions and the training of astronauts in lunar observations and photography.

In the late 20th and early 21st centuries, there have also been a number of Muslim astronauts, the first being Sultan bin Salman bin Abdulaziz Al Saud as a Payload Specialist aboard STS-51-G Space Shuttle Discovery, followed by Muhammed Faris aboard Soyuz TM-2 and Soyuz TM-3 to Mir space station; Abdul Ahad Mohmand aboard Soyuz TM-5 to Mir; Talgat Musabayev (one of the top 25 astronauts by time in space) as a flight engineer aboard Soyuz TM-19 to Mir, commander of Soyuz TM-27marker to Mir, and commander of Soyuz TM-32marker and Soyuz TM-31 to International Space Station (ISS); and Anousheh Ansari, the first woman to travel to ISS and the fourth space tourist.

In 2007, Sheikh Muszaphar Shukor from Malaysiamarker traveled to ISS with his Expedition 16 crew aboard Soyuz TMA-11 as part of the Angkasawan program during Ramadan, for which the National Fatwa Council wrote Guidelines for Performing Islamic Rites (Ibadah) at the International Space Station, giving advice on issues such as prayer in a low-gravity environment, the location of Meccamarker from ISS, determination of prayer times, and issues surrounding fasting. Shukor also celebrated Eid ul-Fitr aboard ISS. He was both an astronaut and an orthopedic surgeon, and is most notable for being the first to perform biomedical research in space, mainly related to the characteristics and growth of liver cancer and leukemia cells and the crystallization of various proteins and microbes in space.

Other prominent Muslim scientists involved in research on the space sciences and space exploration include Essam Heggy who is working in the NASA Mars Exploration Program in the Lunar and Planetary Institute in Houston, as well as Ahmed Salem, Alaa Ibrahim, Mohamed Sultan, and Ahmed Noor.

New efforts in moon sighting

According to Islam, Muslims should observe religious duties during special days on the basis of the Islamic lunar calendar. Therefore, moon sighting is an important issue for Muslims. In recent years, due to global communication and using modern technologies to see the new moon, a new trend has formed among Muslims in this field and new religious questions have emerged.

In 2005, Ayatollah Ali Khamenei, religious scholar and supreme leader of Iranmarker, issued a fatwa to use modern technologies for moon sighting. The Islamic Society of North America in Plainfield, Ind., followed suit last year. Muslims are scrambling for a technological edge in the annual moon-hunting ritual.

Ayatollah Khamenei has established a Moon Observation Committee, composed of clerics who pore over sightings reported to centers. Scientists note the moon's angle, position, and illumination, and compare the sightings from the field with computerized charts that pinpoint where the moon should be. In Iran, groups of astronomers accompanied by a cleric are dispatched across the country, some using night vision gear lent by the military of Iran and high-definition telescopes from the universities. Iran also sends up a chartered airplane with an astronomer aboard. The plane is loaded with sensitive observation and photographic equipment, along with a laptop. Iranian mapmakers at the National Geography Organization in Tehranmarker have created a three-dimensional map of the country identifying 70 locations where the new moon might best be seen. There are similar efforts in other Muslim countries as well.

There is also a competition among astronomers to see the younger moon with naked eyes. According to the Islamic lunar calendar in Iran, the new "World Record for Lunar Crescent Sighting" has been established on September 7, 2002 (Jamadi-al Thani 29, 1423 AH) by Mohsen Ghazi Mirsaeed on the north-west heights (2,110 meters ) of Zarand in Rashk Bala village (31°, 04' N , 56°, 28' E). The record for the moon age at the moment of first visibility with naked eyes is 11 hours and 42 minutes.


The modern astronomical observatory as a research institute (as opposed to a private observation post as was the case in ancient times) was first introduced by medieval Muslim astronomers, who produced accurate Zij treatises using these observatories. The Islamic observatory was the first specialized astronomical institution with its own scientific staff, director, astronomical program, large astronomical instruments, and building where astronomical research and observations are carried out. Islamic observatories were also the first to employ enormously large astronomical instruments in order to improve the accuracy of their observations.

The medieval Islamic observatories were also the earliest institutions to emphasize group research (as opposed to individual research) and where "theoretical investigations went hand in hand with observations." In this sense, they were similar to modern scientific research institutions.

Early observatories

The first systematic observations in Islam are reported to have taken place under the patronage of al-Ma'mun, and the first Islamic observatories were built in 9th century Iraqmarker under his patronage. In many private observatories from Damascusmarker to Baghdadmarker, meridian degrees were measured, solar parameters were established, and detailed observations of the Sun, Moon, and planets were undertaken.

In the 10th century, the Buwayhid dynasty encouraged the undertaking of extensive works in Astronomy, such as the construction of a large scale instrument with which observations were made in the year 950. We know of this by recordings made in the zij of astronomers such as Ibn al-Alam. The great astronomer Abd Al-Rahman Al Sufi was patronised by prince 'Adud al-Dawla, who systematically revised Ptolemy's catalogue of stars. Abu-Mahmud al-Khujandi also constructed an observatory in Ray, Iranmarker where he is known to have constructed the first huge mural sextant in 994 AD. Sharaf al-Daula also established a similar observatory in Baghdadmarker. Reports by Ibn Yunus and al-Zarqall in Toledomarker and Cordobamarker indicate the use of sophisticated instruments for their time.

It was Malik Shah I who established the first large observatory, probably in Isfahanmarker. It was here where Omar Khayyám with many other collaborators constructed a zij and formulated the Persian solar calendar, a.k.a. the jalali calendar, the most accurate solar calendar to date. A modern version of this calendar is still in official use in Iranmarker today.

Late medieval observatories

The more influential observatories, however, were established beginning in the 13th century. The Maragheh observatorymarker was founded by Nasīr al-Dīn al-Tūsī under the patronage of Hulegu Khan in the 13th century. Here, al-Tusi supervised its technical construction at Maraghehmarker. The facility contained resting quarters for Hulagu Khan, as well as a library and mosque. Some of the top astronomers of the day gathered there, and their collaboration resulted in important alternatives to the Ptolemaic model over a period of 50 years. The observations of al-Tusi and his team of researchers were compiled in the Zij-i Ilkhani.

In 1420, prince Ulugh Beg, himself an astronomer and mathematician, founded another large observatory in Samarkandmarker, the remains of which were excavated in 1908 by Russian teams. Ulugh Beg, alongside his team of researchers that included Jamshīd al-Kāshī and Ali Qushji, compiled the results of their observations in the Zij-i-Sultani (1437). In 1577, Taqi al-Din bin Ma'ruf founded the large Istanbul observatory of al-Din, which was on the same scale as those in Maragha and Samarkand as well as those of his contemporary Tycho Brahe.

In the Mughal Empire, Humayun built a personal observatory near Delhimarker in the 16th century, while Jahangir and Shah Jahan were also intending to build observatories but were unable to do so. After the decline of the Mughal Empire, the Hindu king Jai Singh II of Amber built several large observatories called Yantra Mandirsmarker inspired by the famous Samarkand observatory. The instruments and observational techniques used at the observatory were mainly derived from the Islamic tradition, and the computational techniqes from the Hindu tradition.

Modern observatories

In modern times, many well-equipped observatories can be found in Jordanmarker, Palestine, Lebanonmarker, UAEmarker, Tunisiamarker, and other Arab states are also active as well. Iranmarker has modern facilities at Shiraz University and Tabriz Universitymarker. In December 2005, Physics Today reported of Iranian plans to construct a "world class" facility with a 2.0 meter telescope observatory in the near future.


Modern knowledge of the instruments used by Muslim astronomers primarily comes from two sources. First the remaining instruments in private and museum collections today, and second the treatises and manuscripts preserved from the Middle Ages.

Muslims made many improvements to instruments already in use before their time, such as adding new scales or details, and invented many of their own new instruments. Their contributions to astronomical instrumentation are abundant. Many of these instruments were often invented or designed for Islamic purposes, such as the determination of the Qibla (direction to Meccamarker) or the times of Salah prayers.

Astrolabes and planisphere

Brass astrolabes were developed in much of the Islamic world, often as an aid to finding the qibla. The earliest known example is dated 315 AH, (927/8 CE). The first person credited for building the Astrolabe in the Islamic world is reportedly Fazari. Though the first astrolabe to chart the stars was invented in the Hellenistic civilization, al-Fazari made several improvements to the device. The Arabs then took it during the Abbasid Caliphate and perfected it to be used to find the beginning of Ramadan, the hours of prayer (Salah), the direction of Meccamarker (Qibla), and over a thousand other uses.

In the 10th century, Al-Sufi first described over 1000 different uses of an astrolabe, in areas as diverse as astronomy, astrology, horoscope, navigation, surveying, timekeeping, Qibla, Salah, etc.

Large astrolabe

Ibn Yunus in the 10th century accurately observed more than 10,000 entries for the sun's position for many years using a large astrolabe with a diameter of nearly 1.4 meters.

Mechanical geared astrolabe

The first mechanical astrolabes with gears were invented in the Muslim world, and were perfected by Ibn Samh (c. 1020). One such device with eight gear-wheels was also constructed by Abū Rayhān al-Bīrūnī in 996. These can be considered as an ancestor of the mechanical clocks developed by later Muslim engineers.

Navigational astrolabe

The first navigational astrolabe was invented in the Islamic world during the Middle Ages, and employed the use of a polar projection system.

Orthographical astrolabe

Abu Rayhan al-Biruni invented and wrote the earliest treatise on the orthographical astrolabe in the 1000s.

Universal astrolabe (Saphaea)

The first astrolabe instruments were used to read the rise of the time of rise of the Sun and fixed stars. The first universal astrolabes were later constructed in the Islamic world and which, unlike their predecessors, did not depend on the latitude of the observer and could be used anywhere on the Earth. The basic idea for a latitude-independent astrolabe was conceived in the 9th century by Habash al-Hasib al-Marwazi in Baghdad and the topic was later discussed in the early 11th century by Al-Sijzi in Persia.

The first known universal astrolabe to be constructed was by Ali ibn Khalaf al-Shakkaz, an Arabic herbalist or apothecary in 11th century Al-Andalusmarker. His instrument could solve problems of spherical astronomy for any geographic latitude, though in a somewhat more complicated fashion than the standard astrolabe. Another, more advanced and more famous, universal astrolabe was constructed by Abū Ishāq Ibrāhīm al-Zarqālī (Arzachel) soon after. His instrument became known in Europe as the "Saphaea". It was a universal lamina (plate) which "constituted a universal device representing a stereographic projection for the terrestrial equator and could be used to solve all the problems of spherical astronomy for any latitude."


The Zuraqi is a unique astrolabe invented by Al-Sijzi for a heliocentric planetary model in which the Earth is moving rather than the sky.


In the early 11th century, Abū Rayhān al-Bīrūnī invented and wrote the first treatise on the planisphere, which was an early analog computer. The astrolabe was a predecessor of the modern planisphere.

Linear astrolabe

A famous work by Sharaf al-Dīn al-Tūsī is one in which he describes the linear astrolabe, sometimes called the "staff of al-Tusi", which he invented.

Astrolabic clock

Ibn al-Shatir invented the astrolabic clock in 14th century Syriamarker.

Analog computers

Various analog computer devices were invented to compute the latitudes of the Sun, Moon, and planets, the ecliptic of the Sun, the time of day at which planetary conjunctions will occur, and for performing linear interpolation.


The Equatorium was an analog computer invented by Abū Ishāq Ibrāhīm al-Zarqālī (Arzachel) in al-Andalusmarker, probably around 1015 CE. It is a mechanical device for finding the longitudes and positions of the Moon, Sun, and planets, without calculation using a geometrical model to represent the celestial body's mean and anomalistic position.

Mechanical geared calendar computer

Abu Rayhan Biruni also invented the first mechanical lunisolar calendar computer which employed a gear train and eight gear-wheels. This was an early example of a fixed-wired knowledge processing machine.


The volvelle, also called a wheel chart, is a type of slide chart, paper constructions with rotating parts. It is considered an early example of a paper analog computer. The volvelle can be traced back to "certain Arabic treateses on humoral medicine" and to Biruni (c. 1000) who made important contributions to the development of the volvelle. In the 20th century, the volvelle had many diverse uses.


Jabir ibn Aflah (Geber) (c. 1100-1150) invented the torquetum, an observational instrument and mechanical analog computer device used to transform between spherical coordinate systems. It was designed to take and convert measurements made in three sets of coordinates: horizon, equatorial, and ecliptic.

Castle clock with programmable analog computer

In 1206, Al-Jazari invented his largest astronomical clock, the "castle clock", which is considered to be the first programmable analog computer. It displayed the zodiac and the solar and lunar orbits. Another innovative feature of the clock was a pointer which traveled across the top of a gateway and caused automatic doors to open every hour.

Mechanical astrolabe with geared calendar computer

In 1235, Abi Bakr of Isfahanmarker invented a brass astrolabe with a geared calendar movement based on the design of Abū Rayhān al-Bīrūnī's mechanical calendar computer. Abi Bakr's geared astrolabe uses a set of gear-wheels and is the oldest surviving complete mechanical geared machine in existence.

Plate of Conjunctions

In the 15th century, al-Kashi invented the Plate of Conjunctions, a computing instrument used to determine the time of day at which planetary conjunctions will occur, and for performing linear interpolation.

Planetary computer

In the 15th century, al-Kashi also invented a mechanical planetary computer which he called the Plate of Zones, which could graphically solve a number of planetary problems, including the prediction of the true positions in longitude of the Sun and Moon, and the planets in terms of elliptical orbits; the latitudes of the Sun, Moon, and planets; and the ecliptic of the Sun. The instrument also incorporated an alhidade and ruler.

Astronomical clocks

The Muslims constructed a variety of highly accurate astronomical clocks for use in their observatories.

Water-powered astronomical clocks

Al-Jazari invented monumental water-powered astronomical clocks which displayed moving models of the Sun, Moon, and stars. His largest astronomical clock was the "castle clock", which is considered to be the first programmable analog computer (see Castle clock with programmable analog computer above).

Spring-powered astronomical clock

Taqi al-Din invented the first astronomical clock to be powered by springs, first described in his The Brightest Stars for the Construction of Mechanical Clocks (1556-1559).

Mechanical alarm clock

Taqi al-Din invented the first mechanical alarm clock, which he described in The Brightest Stars for the Construction of Mechanical Clocks (Al-Kawākib al-durriyya fī wadh' al-bankāmat al-dawriyya) in 1559. His alarm clock was capable of sounding at a specified time, which was achieved by means of placing a peg on the dial wheel to when one wants the alarm heard and by producing an automated ringing device at the specified time.

Mechanical observational clock

Taqi al-Din invented the "observational clock", which he described as "a mechanical clock with three dials which show the hours, the minutes, and the seconds." This was the first clock to measure time in seconds, and he used it for astronomical purposes, specifically for measuring the right ascension of the stars. This is considered one of the most important innovations in 16th-century practical astronomy, as previous clocks were not accurate enough to be used for astronomical purposes. He further improved the observational clock, as described in his Sidrat al-muntaha, using only one dial to represent the hours, minutes and seconds. He describes this observational clock as "a mechanical clock with a dial showing the hours, minutes and seconds and we divided every minute into five seconds."


Muslim astronomers and engineers invented a variety of dials for timekeeping, and for determining the times of the five daily prayers.


Muslims made several important improvements to the theory and construction of sundials, which they inherited from their Indian and Hellenistic predecessors. Al-Khwarizmi made tables for these instruments which considerably shortened the time needed to make specific calculations. Muslim sundials could also be observed from anywhere on the Earth. Sundials were frequently placed on mosques to determine the time of prayer. One of the most striking examples was built in the 14th century by the muwaqqit (timekeeper) of the Umayyad Mosquemarker in Damascusmarker, Ibn al-Shatir. Muslim astronomers and engineers were the first to write instructions on the construction of horizontal sundials, vertical sundials, and polar sundials. , in

Since ancient dials were nodus-based with straight hour-lines, they indicated unequal hours — also called temporary hours — that varied with the seasons, since every day was divided into twelve equal segments; thus, hours were shorter in winter and longer in summer. The idea of using hours of equal time length throughout the year was the innovation of Abu'l-Hasan Ibn al-Shatir in 1371, based on earlier developments in trigonometry by Muhammad ibn Jābir al-Harrānī al-Battānī (Albategni). Ibn al-Shatir was aware that "using a gnomon that is parallel to the Earth's axis will produce sundials whose hour lines indicate equal hours on any day of the year." His sundial is the oldest polar-axis sundial still in existence. The concept later appeared in Western sundials from at least 1446.

Navicula de Venetiis

This was a universal horary dial invented in 9th century Baghdadmarker. It was used for accurate timekeeping by the Sun and Stars, and could be observed from any latitude. This was later known in Europe as the "Navicula de Venetiis", which was considered the most sophisticated timekeeping instrument of the Renaissance.

Compass dial

In the 13th century, Ibn al-Shatir invented the compass dial, a timekeeping device incorporating both a universal sundial and a magnetic compass. He invented it for the purpose of finding the times of Salah prayers.


Armillary sphere

An armillary sphere had similar applications to a celestial globe. No early Islamic armillary spheres survive, but several treatises on “the instrument with the rings” were written.

Spherical astrolabe

The spherical astrolabe was first produced in the Islamic world. It was an Islamic variation of the astrolabe and the armillary sphere, of which only one complete instrument, from the 14th century, has survived.

Terrestrial globe

The first terrestrial globe of the Old World was constructed in the Muslim world during the Middle Ages, by Muslim geographers and astronomers working under the Abbasid caliph, Al-Ma'mun, in the 9th century.

Celestial globes

Celestial globes were used primarily for solving problems in celestial astronomy. Today, 126 such instruments remain worldwide, the oldest from the 11th century. The altitude of the sun, or the Right Ascension and Declination of stars could be calculated with these by inputting the location of the observer on the meridian ring of the globe.

In the 12th century, Jabir ibn Aflah (Geber) was "the first to design a portable celestial sphere to measure and explain the movements of celestial objects."

Seamless celestial globe

The seamless celestial globe invented by Muslim metallurgists and instrument-makers in Mughal India, specifically Lahoremarker and Kashmirmarker, is considered to be one of the most remarkable feats in metallurgy and engineering. All globes before and after this were seamed, and in the 20th century, it was believed by metallurgists to be technically impossible to create a metal globe without any seams. It was in the 1980s, however, that Emilie Savage-Smith discovered several celestial globes without any seams in Lahore and Kashmir. The earliest was invented in Kashmir by the Muslim metallurgist Ali Kashmiri ibn Luqman in 998 AH (1589-90 CE) during Akbar the Great's reign; another was produced in 1070 AH (1659-60 CE) by Muhammad Salih Tahtawi with Arabic and Sanskrit inscriptions; and the last was produced in Lahore by a Hindu metallurgist Lala Balhumal Lahuri in 1842 during Jagatjit Singh Bahadur's reign. 21 such globes were produced, and these remain the only examples of seamless metal globes. These Mughal metallurgists developed the method of lost-wax casting in order to produce these globes.

These seamless celestial globes are considered to be an unsurpassed feat in metallurgy, hence some consider this achievement to be comparable to that of the Great Pyramid of Gizamarker which was considered an unsurpassed feat in architecture until the 19th century.

Optical instruments

Observation tube
The first reference to an "observation tube" is found in the work of al-Battani (Albatenius) (853-929), and the first exact description of the observation tube was given by al-Biruni (973-1048), in a section of his work that is "dedicated to verifying the presence of the new crescent on the horizon." Though these early observation tubes did not have lenses, they "enabled an observer to focus on a part of the sky by eliminating light interference." These observation tubes were later adopted in Latin-speaking Europe, where they influenced the development of the telescope.

Experimental device with apertures
In order to prove that "light is emitted from every point of the moon's illuminated surface," Ibn al-Haytham (Alhazen) built an "ingenious experimental device" showing "that the intensity of the light-spot formed by the projection of the moonlight through two small apertures onto a screen diminishes constantly as one of the apertures is gradually blocked up."

Magnifying lens
The first optical research to describe a magnifying lens used in an instrument was found in a book called the Book of Optics (1021) written by Ibn al-Haytham (Alhazen). His descriptions helped set the parameters in Europe for the later advances in telescopic technology and his additional work in light refraction, parabolic mirrors, as well as the creation of other instruments such as the camera obscura, also helped spark the Scientific Revolution.

Taqi al-Din describes a long-distance magnifying device in his Book of the Light of the Pupil of Vision and the Light of the Truth of the Sights around 1574, which may have possible been an early rudimentary telescope. He describes his device as an instrument that makes objects located far away appear closer to the observer, and that the instrument helps to see distant objects in detail by bringing them very close. Taqi al-Din states that he wrote another treatise (which has not survived to the present day) explaining the way this instrument is made and used. There is some confusion as to what he was describing since he also said his invention was similar to one used by ancient Greeks at the Tower of Alexandriamarker.


A number of mural instruments, including several different quadrants and sextant, were invented by Muslim astronomers and engineers.

Sine quadrant

The sine quadrant, invented by Muhammad ibn Mūsā al-Khwārizmī in 9th century Baghdadmarker, was used for astronomical calculations. Also known as the "Sinecal Quadrant" (the Arabic term for it is "Rubul Mujayyab"), it was used for solving trigonometric problems and taking astronomical observations. It was developed by al-Khwarizmi in the 9th century and remained prevalent until the 19th century. Its defining feature is a graph paper like grid on one side that is divided into sixty equal intervals on each axis and is also bounded by a 90 degree graduated arc. A cord was attached to the apex of the quadrant with a bead at the end of it to act as a plumb bob. They were also sometimes drawn on the back of astrolabes.

Horary quadrant

The first horary quadrant for specific latitudes, was invented by Muhammad ibn Mūsā al-Khwārizmī in 9th century Baghdad, center of the development of quadrants. It was used to determine time (especially the times of prayer) by observations of the Sun or stars. The horary quadrant could be used to find the time either in equal or unequal (length of the day divided by twelve) hours. Different sets of markings were created for either equal or unequal hours. For measuring the time in equal hours, the horary quadrant could only be used for one specific latitude while a quadrant for unequal hours could be used anywhere based on an approximate formula. One edge of the quadrant had to be aligned with the sun, and once aligned, a bead on the end of a plumbline attached to the centre of the quadrant showed the time of the day.

Universal horary quadrant (Quadrans Novus)

The universal horary quadrant was an ingenious mathematical device invented by al-Khwarizmi in 9th century Baghdadmarker and which was later known as the "Quadrans Vetus" (Old Quadrant) in medieval Europe from the 13th century. It could be used for any latitude on Earth and at any time of the year to determine the time in hours from the altitude of the Sun. This was the second most widely used astronomical instrument during the Middle Ages after the astrolabe. One of its main purposes in the Islamic world was to determine the times of Salah.

Astrolabic/Almucantar quadrant (Quadrans Vetus)

The astrolabic or almucantar quadrant was invented in the medieval Islamic world, and it employed the use of trigonometry. The term "almucantar" is itself derived from Arabic. The almucantar quadrant was originally modified from the astrolabe. It was invented in Egyptmarker in the 11th or 12th century, and was later known in Europe as the "Quadrans Vetus" (New Quadrant). It was intended as a simplified alternative to the astrolabe serving a specific latitude. According to David King:

Universal quadrant (Shakkāzīya)

The universal (shakkāzīya) quadrant was used for solving astronomical problems for any latitude. These quadrants had either one or two sets of shakkāzīya grids and were developed in the 14th century in Syriamarker. Some astrolabes are also printed on the back with the universal quadrant like an astrolabe created by Ibn al-Sarrāj. The Shakkaziya quadrant produced by Jamal al-Din al-Maridini was an analog computer for solving problems of spherical astronomy. By the time of the Mamluk Sultanatemarker, Muslim astronomers "developed the quadrant to all conceivable limits; it virtually replaced the astrolabe in Syria and Egypt in Mamluk and Ottoman times."


Mural sextant

The first sextant was constructed in Ray, Iranmarker, by Abu-Mahmud al-Khujandi in 994. It was a very large mural sextant that achieved a high level of accuracy for astronomical measurements, which he described his in his treatise, On the obliquity of the ecliptic and the latitudes of the cities.

Fakhri sextant

In the 15th century, Ulugh Beg constructed the Fakhri sextant, which had a radius of approximately 36 meters. Constructed in Samarkandmarker, Uzbekistanmarker, the arc was finely constructed with a staircase on either side to provide access for the assistants who performed the measurements.

Framed sextant

At the Istanbul observatory of al-Din between 1577 and 1580, Taqi al-Din invented the mushabbaha bi'l manattiq, a framed sextant with cords for the determination of the equinoxes similar to what Tycho Brahe later used.

Other instruments

Various other astrononmical instruments were also invented in the Islamic world:

  • Astronomical compass: The first astronomical uses of the magnetic compass is found in a treatise on astronomical instruments written by the Yemenimarker sultan al-Ashraf (died 1296) in 1282. This was the first reference to the compass in astronomical literature.
  • Dry compass: In 1282, al-Ashraf also developed an improved compass for use as a "Qibla indicator" instrument in order to find the direction to Meccamarker. Al-Ashraf's instrument was one of the earliest dry compasses, and appears to have been invented independently of Peter Peregrinus.
  • Alhidade: The alhidade was invented in the Islamic world, while the term "alhidade" is itself derived from Arabic.
  • Compendium instrument: A compendium was a multi-purpose astronomical instrument, first constructed by the Muslim astronomer Ibn al-Shatir in the 13th century. His compendium featured an alhidade and polar sundial among other things. Al-Wafa'i developed another compendium in the 15th century which he called the "equatorial circle", which also featured a horizontal sundial. These compendia later became popular in Renaissance Europe.
  • Orthogonal and regular grids: Islamic quadrants used for various astronomical and timekeeping purposes from the 10th century introduced orthogonal and regular grids and markings that are identical to modern graph paper.
  • Qibla indicators: In 17th century Safavid Persia, two unique brass instruments with Meccamarker-centred world maps engraved on them were produced primarily for the purpose of finding the Qibla. These instruments were engraved with cartographic grids to make it more convenient to find the direction and distance to Mecca at the centre from anywhere on the Earth, which may be based on cartographic grids dating back to 10th century Baghdadmarker. One of the two instruments, produced by Muhammad Husayn, also had a sundial and compass attached to it.
  • Shadow square: The shadow square was an instrument used to determine the linear height of an object, in conjunction with the alidade, for angular observations. It was invented by Muhammad ibn Mūsā al-Khwārizmī in 9th century Baghdad.

List of notable treatises

Zij treatises


The word "Almanac" is an Arabic word. The modern almanac differs from earlier astronomical tables (such as the earlier Babylonian, Ptolemaic and Zij tables) in the sense that "the entries found in the almanacs give directly the positions of the celestial bodies and need no further computation", in contrast to the more common "auxiliary astronomical tables" based on Ptolemy's Almagest. The earliest known almanac in this modern sense is the Almanac of Azarqueil written in 1087 by Abū Ishāq Ibrāhīm al-Zarqālī (Latinized as Azarqueil) in Toledomarker, Al-Andalusmarker. The work provided the true daily positions of the sun, moon and planets for four years from 1088 to 1092, as well as many other related tables. A Latin translation and adaptation of the work appeared as the Tables of Toledo in the 12th century and the Alfonsine tables in the 13th century.

Treatises on instruments

In the 12th century, al-Khazini wrote the Risala fi'l-alat (Treatise on Instruments) which had seven parts describing different scientific instruments: the triquetrum, dioptra, a triangular instrument he invented, the quadrant and sextant, the astrolabe, and original instruments involving reflection.

In 14th century Egyptmarker, Najm al-Din al-Misri (c. 1325) wrote a treatise describing over 100 different types of scientific and astronomical instruments, many of which he invented himself.

In 1416, al-Kashi wrote the Treatise on Astronomical Observational Instruments, which described a variety of different instruments, including the triquetrum and armillary sphere, the equinoctial armillary and solsticial armillary of Mo'ayyeduddin Urdi, the sine and versine instrument of Urdi, the sextant of al-Khujandi, the Fakhri sextant at the Samarqandmarker observatory, a double quadrant Azimuth-altitude instrument he invented, and a small armillary sphere incorporating an alhidade which he invented.

Other works

  • Ja'far Muhammad ibn Mūsā ibn Shākir (Latinized as Mohammed Ben Musa) (800-873)
    • Book on the motion of the orbs
    • Astral Motion
    • The Force of Attraction
  • Ahmad ibn Muhammad ibn Kathīr al-Farghānī (Latinized as Alfraganus) (d. 850)
    • Elements of astronomy on the celestial motions (c. 833)
    • Kitab fi Jawami Ilm al-Nujum
  • Ibn al-Haytham (Latinized as Alhacen) (965-1039)
    • On the Configuration of the World
    • Doubts concerning Ptolemy (c. 1028)
    • The Resolution of Doubts (c. 1029)
    • The Model of the Motions of Each of the Seven Planets (1029-1039)
  • Abū Rayhān al-Bīrūnī (973-1048)
    • Kitab al-Qanun al-Mas'udi (Latinized as Canon Mas’udicus) (1031)
  • Abu Ubayd al-Juzjani (c. 1070)
    • Tarik al-Aflak (1070)
  • Al-Istidrak ala Batlamyus (Recapitulation regarding Ptolemy) (11th century)
  • Al-Khazini (fl. 1115-1130)
    • Risala fi'l-alat (Treatise on Instruments)
  • Nasīr al-Dīn al-Tūsī (1201-1274)
    • Al-Tadhkirah fi'ilm al-hay'ah (Memento in astronomy)
  • 'Umar al-Katibi al-Qazwini (d. 1277)
    • Hikmat al-'Ain
  • Qutb al-Din al-Shirazi (1236-1311)
    • The Limit of Accomplishment concerning Knowledge of the Heavens
  • Ibn al-Shatir (1304–1375)
    • A Final Inquiry Concerning the Rectification of Planetary Theory
  • Ali al-Qushji (d. 1474)
    • Concerning the Supposed Dependence of Astronomy upon Philosophy
  • Shams al-Din al-Khafri (d. 1525)
    • The complement to the explanation of the memento

Arabic star names

Many of the modern names for numerous stars and constellations are derived from their Arabic language names. Examples include: Acamar, Aldebaran, Algol, Altair, Baham, Baten Kaitos, Caph, Dabih, Edasich, Furud, Gienah, Hadar, Izar, Jabbah, Keid, Lesath, Mirak, Nashira, Okda, Phad, Rigel, Sadr, Tarf, and Vega, as well as a number of other stars. Some of these names originated in the pre-Islamic Arabian Peninsula, but many came later, as translations of Ancient Greek descriptions.


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See also


  • , in
  • (cf. )
  • , June 2003
  • , June 2003
  • , June 2004

External links

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