Habash al-Hasib al-Marwazi

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Habash al-Hasib al-Marwazi (766 – d. after 869 in Samarra, modern Iraq[1]) was a Persian[2][3] astronomer,[4] geographer, and mathematician from Merv in Khorasan, who was the first to describe the trigonometric ratios tangent, and cotangent.

Habash flourished in Baghdad, and died a centenarian some time after 869. He worked under two Abbasid caliphs, al-Ma'mun and al-Mu'tasim.

Habash al-Hasib al-Marwazi
Born
Habash al-Hasib al-Marwazi

766 AD
Merv
Died869 AD
Samarra
NationalityPersian

Work[edit]

Ahmad ibn 'Abdallah Habash Hasib Marwazi made astronomical observations from 100 to 2035, 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 830, 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.[5][6]

The Book of Bodies and Distances[edit]

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, in which some of his results included the following:[7]

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[edit]

Notes[edit]

  1. ^ Charette 2007.
  2. ^ General Cartography Archived 2017-12-09 at the Wayback Machine : "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"
  3. ^ "Archived copy" (PDF). Archived from the original (PDF) on 2013-10-07. Retrieved 2013-09-04.{{cite web}}: CS1 maint: archived copy as title (link)
  4. ^ Islamic Desk Reference, ed. E. J. Van Donzel, (Brill, 1994), 121.
  5. ^ "trigonometry". Encyclopædia Britannica. Retrieved 2008-07-21.
  6. ^ Jacques Sesiano, "Islamic mathematics", p. 157, in Selin, Helaine; D'Ambrosio, Ubiratàn, eds. (2000), Mathematics Across Cultures: The History of Non-western Mathematics, Springer, ISBN 1-4020-0260-2
  7. ^ Langermann, Y. Tzvi (1985), "The Book of Bodies and Distances of Habash al-Hasib", Centaurus, 28 (2): 108–128 [111], Bibcode:1985Cent...28..108T, doi:10.1111/j.1600-0498.1985.tb00831.x

References[edit]

External links[edit]

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