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112<br />

Astronomy<br />

Like other disciplines of Indian thought, astronomy and its origins<br />

may be genetically related back to the Vedas. The Vedic Aryans<br />

were well acquainted with the natural routine cycles of heavenly<br />

bodies. The vault of the sky, for example, was seen as being<br />

governed by the eternal ordinances of an inherent universal<br />

principle, Rita (literally, the course of things), which determines<br />

the paths and phases of the moon and the planets, the day/night<br />

cycle and occurrences of eclipses.<br />

The Jyotisha Vedanga and the Surya Prajnapati (c. 400 BC-AD 200)<br />

record the earliest Hindu astronomical statements. In early times,<br />

astronomy developed out of pragmatic speculations which were<br />

necessary and therefore of paramount importance for the careful<br />

calculation of appropriate times for rituals and sacrifices. The<br />

important treatises on Indian astronomy were the Gargi-samhita (c.<br />

AD 230), the Aryabhattiya of Aryabhata (AD 499), the Siddhantasekhara<br />

of Sripati, and the Siddhanta-Siromani of Bhaskara II (AD<br />

1114-1160).<br />

By the beginning of the Christian era, a great upsurge in the<br />

astronomical search was formalized in a number of methodical<br />

studies; many works of great importance, such as the five<br />

Siddhantas, of which the Surya Siddhanta is probably the best<br />

known, were compiled and later summarized by the sixth-century<br />

astronomer and mathematician Varaha-Mihira in his Panchasiddhantika<br />

(The Five Astronomical Systems), written about AD 550.<br />

In his outstanding work, the Brihat-samhita (The Great Compendium),<br />

he describes the motions and conjunctions of celestial<br />

bodies and their significance as omens.<br />

The classical period of ancient Indian astronomy is considered<br />

to have ended with Brahmagupta who wrote the Brahmasiddhanta,<br />

in AD 628, and the Khandakhadyaka, a practical treatise on<br />

astronomical calculations, in AD 664. Aryabhata's new epicyclic<br />

theory, and his postulates regarding the sphericity of the earth, its<br />

rotation upon its axis and revolution around the sun, as well as his<br />

formulae for the determination of the physical parameters of<br />

various celestial bodies (such as the diameters of the earth and the<br />

moon), and the prediction of eclipses and the correct length of the<br />

year by means of mathematical calculation, were significant<br />

achievements which anticipated and agree with the modern ideas.<br />

Aryabhata also gave the first fundamental definition of trigonometric<br />

functions and was responsible for pointing out the<br />

importance of zero.

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