Al-Battani

Who was Al Battani? Biography, breakthroughs, IQ analysis, and intellectual legacy — curated by Geniuses.club's editors. Read more on Geniuses.club.

Nobody is known in Islam who reached similar perfection in observing the stars and scrutinizing their motions.

Abu ʿAbd Allah Muḥammad ibn Jabir ibn Sinan al-Raqqi al-Ḥarrani as-Sabiʾ al-Battani was an Arab astronomer, and mathematician. He introduced a number of trigonometric relations, and his Kitab az-Zij was frequently quoted by many medieval astronomers, including Copernicus. Often called the "Ptolemy of the Arabs", al-Battani is perhaps the greatest and best known astronomer of the medieval Islamic world.

Life

Little of al-Battani's life is known other than his birthplace in Harran near Urfa, in Upper Mesopotamia, today in Turkey and his father's fame as a maker of scientific instruments. Ibn Khallikan expresses ignorance on the question of his Muslim faith, and points out that his epithet as-Sabi’ suggests possible Sabian-sect ancestry. The Encyclopedia Britannica Eleventh Edition stated that he had noble origins as an Arab prince, but traditional Arabic biographers make no mention of this. Between 877 and 918/19, over a forty-year period, he lived in the ancient city of Raqqa, in north central Syria, recording his astronomical observations. He is said to have died while returning to Baghdad at a fortress called Kasr al-Hadr, which was near either Tikrit, or Samarra.

Astronomy

One of al-Battani's best-known achievements in astronomy was the determination of the solar year as being 365 days, 5 hours, 46 minutes and 24 seconds, which is only 2 minutes and 22 seconds off.

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The twelfth-century Egyptian encyclopedist al-Qifṭī, in his biographical history Ta’rikh al-Hukama’, mentions al-Battani’s contribution to advances in astronomical observation and calculations based on Ptolemy’s Almagest.

Al-Battani amended some of Ptolemy's results and compiled new tables of the Sun and Moon, long accepted as authoritative. Some of his measurements were more accurate than ones taken by Copernicus many centuries later and some ascribe this phenomenon to al-Battani's location lying closer to the equator such that the ecliptic and the Sun, being higher in the sky, are less susceptible to atmospheric refraction. Al-Battani observed that the direction of the Sun's apogee, as recorded by Ptolemy, was changing.

De scientia stellarum, 1645

Al-Battani's work was instrumental in the development of science and astronomy. Copernicus, in his book that initiated the Copernican Revolution, the De Revolutionibus Orbium Coelestium, quotes his name no fewer than 23 times, and also mentions him in the Commentariolus. Tycho Brahe, Riccioli, Kepler, Galileo and others frequently cited him or his observations. His data is still used in geophysics. The major lunar crater Albategnius is named in his honor.

Among his Innovations

Mathematics

In mathematics, al-Battani produced a number of trigonometrical relationships:

He also solved the equation sin x = a cos x discovering the formula:

He gives other trigonometric formulae for right-angled triangles such as:

Al-Battani used al-Marwazi's idea of tangents "shadows" to develop equations for calculating tangents and cotangents, compiling tables of them. He also discovered the reciprocal functions of secant and cosecant, and produced the first table of cosecants, which he referred to as a "table of shadows" in reference to the shadow of a gnomon, for each degree from 1° to 90°.

Using these trigonometrical relationships, Al-Battānī created an equation for finding the qibla, which Muslims must face in each of the five prayers they practice everyday. The equation he created did not give accurate directions, as it did not take into account the fact that Earth is a sphere. The relationship Al-Battānī used was fairly precise when a person is in Mecca, or close to Mecca, but resulted in more and more inaccurate results as one gets more distant from Mecca. However, it was still a widely used method at the time. The equation is as follows:

Works

In popular culture

A ship in Star Trek: Voyager is named after Al-Battani, known as the USS Al-Batani, on which Kathryn Janeway originally served.

Top questions

Who was Al-Battani?

Al-Battani was the greatest Arab astronomer of the medieval period and one of the most important astronomers in the history of science. Born around 858 CE, probably in Harran, he made most of his observations at Raqqa, on the Euphrates in what is now Syria, and died in 929 CE near Samarra.

What is Al-Battani best known for?

Al-Battani corrected errors in Ptolemy's Almagest, determined the length of the solar year with extraordinary accuracy and developed trigonometric methods that influenced European mathematics into the Renaissance. His Kitab az-Zij, a book of astronomical tables, was translated into Latin in the twelfth century and became a standard reference for European astronomers.

How accurately did Al-Battani measure the solar year?

He determined the solar year to be 365 days, 5 hours, 46 minutes and 24 seconds, an error of only about 2 minutes and 22 seconds from the modern value. He observed systematically for more than forty years, from 872 to 918 CE, using instruments of his own design, including an improved gnomon, mural quadrant and parallactic ruler.

What did Al-Battani contribute to trigonometry?

Al-Battani introduced the use of sines in place of the Greek chords, advancing the development of modern trigonometry. He developed the concept of what is now called the cotangent and produced detailed trigonometric tables. The mathematician Regiomontanus later used his trigonometric tables.

Which astronomers did Al-Battani influence?

Copernicus cited Al-Battani by name several times in De Revolutionibus in 1543 and used his observational data. Tycho Brahe used his measurements to calibrate his own observations, and Galileo cited him. Renaissance astronomers treated him as an authority on par with Ptolemy, and a lunar crater, Albategnius, is named after him.

How did Al-Battani correct Ptolemy?

He demonstrated that the distance between the earth and the sun varies through the year, a correction to Ptolemy's model with implications for the geometry of solar eclipses. He also measured the positions of stars and planets, the obliquity of the ecliptic and the precession of the equinoxes with remarkable accuracy.

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