Habash al-Hasib

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Template:Short description Script error: No such module "Template wrapper".Template:Main otherScript error: No such module "Check for clobbered parameters". Ahmad ibn 'Abdallah al-Marwazi,[1][2] known as Habash al-Hasib (Template:Langx,[1][2][3] died Template:Circa 869Template:Sfn) was a Persian[4][2] astronomer,[5] geographer, and mathematician from Merv in Khorasan, who discovered the trigonometric ratios tangent, and cotangent.[6] Al-Biruni who cited Habash in his work, expanded his astronomical tables.[3]

Habash al-Hasib flourished in Baghdad, and died a centenarian some time between 864 and 874[2][3][7] possibly in Abbasid Samarra.Template:Sfn The title "Habash" (Abbyssian) may refer to dark skin color.[3] He worked under two Abbasid caliphs, al-Ma'mun and al-Mu'tasim.[3]

Habash al-Hasib developed a trigonometric algorithm to solve problems related to parallax, which was later rediscovered by Johannes Kepler in 1609 and it is now known as Kepler's equation.[8][9]

Habash is the father of the astronomer Abu Ja'far ibn Habash.[3]

Work

Habash Hasib made astronomical observations from 825 to 835, and compiled three zijes (astronomical tables): the first were still in the Hindu manner; the second, called the "tested" tables, were the most important; they are likely identical with the "Ma'munic" or "Arabic" tables and may be a collective work of al-Ma'mun's astronomers; the third, called tables of the Shah, were smaller.

Apropos of the solar eclipse of 829, Habash gives us the first instance of a determination of time by an altitude (in this case, of the sun); a method which was generally adopted by Muslim astronomers.

In 860, he seems to have introduced the notion of "shadow", umbra (versa), equivalent to our tangent in trigonometry, and he compiled a table of such shadows which seems to be the earliest of its kind. He also introduced the cotangent, and produced the first tables of for it.[10][11]

The Book of Bodies and Distances

Habash al-Hasib conducted various observations at the Al-Shammisiyyah observatory in Baghdad and estimated a number of geographic and astronomical values. He compiled his results in The Book of Bodies and Distances (Template:Transliteration),[7] in which some of his results included the following:[12]

Earth
Moon
  • Moon's diameter: 1886.8 miles (3036.5 km)
  • Moon's circumference: 5927.025 miles (9538.622 km)
  • Radius of closest distance of Moon: 215,208;9,9 (sexagesimal) miles
  • Half-circumference of closest distance of Moon: 676,368;28,45,25,43 (sexagesimal) miles
  • Radius of furthest distance of Moon: 205,800;8,45 (sexagesimal) miles
  • Diameter of furthest distance of Moon: 411,600.216 miles (662,406.338 km)
  • Circumference of furthest distance of Moon: 1,293,600.916 miles (2,081,848.873 km)
Sun
  • Sun's diameter: 35,280;1,30 miles (56,777.6966 km)
  • Sun's circumference: 110,880;4,43 miles (178,444.189 km)
  • Diameter of orbit of Sun: 7,761,605.5 miles (12,491,093.2 km)
  • Circumference of orbit of Sun: 24,392,571.38 miles (39,256,038 km)
  • One degree along orbit of Sun: 67,700.05 miles (108,952.67 km)
  • One minute along orbit of Sun: 1129.283 miles (1817.405 km)

See also

Notes

Template:Reflist

References

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External links

Template:Islamic mathematics Template:Islamic astronomy Template:People of Khorasan Template:Authority control

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  4. General Cartography Template:Webarchive : "The Iranian geographers Abū Muhammad al-Hasan al-Hamdānī and Habash al-Hasib al-Marwazi set the Prime Meridian of their maps at Ujjain, a center of Indian astronomy"
  5. Islamic Desk Reference, ed. E. J. Van Donzel, (Brill, 1994), 121.
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  11. Jacques Sesiano, "Islamic mathematics", p. 157, in Script error: No such module "citation/CS1".
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