From: Thomas Hockey et al. (eds.). The Biographical Encyclopedia of Astronomers, Springer Reference. New York: Springer, 2007, pp. 1110-1111 |
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Sulaymān ibn
ʿIṣma: Abū
Dāwūd Sulaymān
ibn ʿIṣma al‐Samarqandī
Giuseppe Bezza
Flourished Samarqand,
(Uzbekistan), second half of the 9th century
Much of our information on Sulaymān ibn ʿIṣma comes from the remarks of Bīrūnī.
According to Bīrūnī, Sulaymān made observations in Balkh
(Afghanistan) in 888–890 for determining the obliquity of the ecliptic. For
this purpose, he used a mural quadrant (libna) provided with an alidade,
the diameter of the quadrant being about 8 cubits (dhirāʿ), approximately 4 m. He found the meridian solar altitude
at the winter solstice to be 29° 46' and at the summer solstice 76° 54'. From this he determined
that the obliquity of the ecliptic was 23° 34', 1 min less than the result of Battānī.
Bīrūnī also tells us of Sulaymān's determination of the
length of Spring and Summer, and attributes to Sulaymān a zīj
(astronomical handbook) dealing with the Sun and Moon (Zīj al‐nayyirayn),
as well as a book on the construction of an instrument for determining the
visibility of the crescent (Qānūn II, p. 654). Nasawī
claims that Sulaymān also wrote a commentary on the Almagest.
Finally,
Sulaymān composed a commentary on the tenth book of Euclid's Elements,
which is still extant.
Al‐Bīrūnī, Abū al‐Rayḥān
Muḥammad b. Aḥmad (1954–1956). al‐Qānūn al‐Masʿūdī. Hyderabad.
Ali, Jamil (trans.)
(1967). The Determination of the Coordinates of Cities: Al‐Bīrūnī's
Taḥdīd al‐Amākin.
Beirut: American University of Beirut.
Kennedy, E. S. (1973).
A Commentary upon Bīrūnī's Kitāb Taḥdīd
al‐Amākin. Beirut: American University of Beirut.
Rosenfeld, B. A. and Ekmeleddin Ihsanoğlu (2003). Mathematicians,
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Sayılı, Aydın (1960). The Observatory in Islam.
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Oskar (1926/1927). “Studien zur Astronomie der Araber.” Sitzungsberichte
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Fuat (1978). Geschichte des arabischen Schrifttums. Vol. 6, Astronomie, p. 170. Leiden: E. J. Brill.
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