Aryabhata wrote the Aryabhatiya in 499 CE, a compact text that used a place value number system, gave an approximation of pi accurate to five significant figures, and set out rules for solving linear and quadratic equations. In astronomy he stated that Earth rotates on its axis, producing the daily motion of the stars, and explained lunar and solar eclipses as the shadows of the Earth and Moon rather than as omens, a genuinely physical account centuries ahead of much of the world. This description is adapted from Wikipedia contributors under CC BY-SA 4.0; changes were made. https://creativecommons.org/licenses/by-sa/4.0/
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Birth YearSourced to the subject's own account FieldSourced to the subject's own accountMathematics and astronomy 1 Notable Work Notable Work Notable Work Notable Work Field
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Sources
1. Aryabhata (Wikipedia)
WikipediaLead sectionQuote, Lead section
Aryabhata (Sanskrit: आर्यभट, IAST: Āryabhaṭa) or Aryabhata I (476-550 CE) was the first of the major mathematician-astronomers and early physicist from the classical age of Indian mathematics and Indian astronomy.
2. Aryabhata (Wikidata)
P570 (date of death): year
+0550-01-01T00:00:00Z
P20 (place of death): Pataliputra, India
Q389755
P19 (place of birth): Pataliputra, India
Q389755
P800 (notable work): Āryabhaṭīya
Q3518429
P800 (notable work): Arya Siddhanta
Q124799996
P800 (notable work): Āryabhaṭa numeration
Q140783
P800 (notable work): Āryabhaṭa's sine table
Q8079604
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