- Also called:
- Aryabhata I or Aryabhata the Elder
- Born:
- 476, possibly Ashmaka or Kusumapura, India
- Notable Works:
- âAryabhatiyaâ
Aryabhata
How did Aryabhata become famous?
What did Aryabhata discover?
What was Aryabhataâs legacy?
Aryabhata (born 476, possibly Ashmaka or Kusumapura, India) was an astronomer and the earliest Indian mathematician whose work and history are available to modern scholars. He is also known as Aryabhata I or Aryabhata the Elder to distinguish him from a 10th-century Indian mathematician of the same name. He is believed to have lived and worked at Kusumapuraânear Pataliputra (present-day Patna), then the capital of the Gupta dynasty. Aryabhata is known as the author of Aryabhatiya, composed about 499 ce. A second work, the Aryabhatasiddhanta (also called the Arya-siddhanta), is mentioned by later writers but did not survive as an independent text.
Aryabhatiya
Aryabhatiya is a treatise written in Sanskrit verse particularly popular in southern India, where numerous mathematicians over the ensuing millennium wrote commentaries. The work was written in verse couplets and deals with mathematics and astronomy. Aryabhatiya is divided into four padas (âsectionsâ). The opening pada, âGitikaâ (âVersesâ), also called âDasagitikaâ (âTen Versesâ), comprising ten core verses, sets out basic astronomical parameters, units of time, and numerical constants. It also introduces Aryabhataâs system of alphabetic numeration, in which numbers are represented by syllables formed from consonants and vowels. This system made it possible to encode large numerical values in verse form and was widely used by later astronomers. The remaining padas are âGanitaâ (âMathematicsâ), âKalakriyaâ (âTime Calculationsâ), and âGolaâ (âSphereâ).
Aryabhataâs work was widely studied in India, where it gave rise to scholarly commentaries that explained and elaborated on his methods and further mathematical development. Aryabhatiya was translated into Arabic in the early 9th century under the title ZÄ«j al-Arjabhar, helping to introduce Indian mathematical and astronomical methods into the Islamic world.
Mathematics
In the âGanitaâ pada Aryabhata names the first 10 decimal places and gives algorithms for obtaining square and cubic roots using the decimal number system. Then he treats geometric measurementsâemploying 62,832/20,000, yielding a value of 3.1416, for pi, very close to the actual value 3.14159âand develops properties of similar right-angled triangles and of two intersecting circles.
Using the Pythagorean theorem, Aryabhata obtained one of the two methods for constructing his table of sines. He also realized that second-order sine difference is proportional to sine. Mathematical series, quadratic equations, compound interest (involving a quadratic equation), proportions (ratios), and the solution of various linear equations are among the arithmetic and algebraic topics included. Aryabhataâs general solution for linear indeterminate equations, which Bhaskara I called kuttakara (âpulverizerâ), consisted of breaking the problem down into new problems with successively smaller coefficientsâessentially the Euclidean algorithm and related to the method of continued fractions.
Astronomy and time calculation
With the âKalakriyaâ pada Aryabhata turned to astronomyâin particular, treating planetary motion along the ecliptic. The topics include definitions of various units of time, eccentric and epicyclic models of planetary motion (see Hipparchus for earlier Greek models), planetary longitude corrections for different terrestrial locations, and a theory of âlords of the hours and daysâ (an astrological concept used for determining propitious times for action).
Spherical astronomy
Aryabhatiya ends with spherical astronomy in the âGolaâ pada, where he applied plane trigonometry to spherical geometry by projecting points and lines on the surface of a sphere onto appropriate planes. Topics include prediction of solar and lunar eclipses and an explicit statement that the apparent westward motion of the stars is due to the spherical Earthâs rotation about its axis. Aryabhata also correctly ascribed the luminosity of the Moon and planets to reflected sunlight.
Aryabhatasiddhanta
Aryabhatasiddhanta circulated mainly in the northwest of India and, through the SÄsÄnian dynasty (224â651) of Iran, had a profound influence on the development of Islamic astronomy. Its contents are preserved to some extent in the works of Varahamihira (flourished c. 550), Bhaskara I (flourished c. 629), Brahmagupta (598âc. 665), and others. It is one of the earliest astronomical works to assign the start of each day to midnight.
