నీలకంఠ సోమయాజి: కూర్పుల మధ్య తేడాలు
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K.Venkataramana (చర్చ | రచనలు) |
K.Venkataramana (చర్చ | రచనలు) |
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పంక్తి 58:
==ఖగోళ శాస్త్రం==
In his ''Aryabhatiyabhasya'', a commentary on Aryabhata's ''[[Aryabhatiya]]'', Nilakantha developed a computational system for a partially [[heliocentrism|heliocentric]] planetary model in which Mercury, Venus, [[Mars]], [[Jupiter]] and [[Saturn]] orbit the [[Sun]], which in turn orbits the [[Earth]], similar to the [[Tychonic system]] later proposed by [[Tycho Brahe]] in the late 16th century. Most astronomers of the Kerala school who followed him accepted this planetary model.<ref name=Joseph/><ref>K. Ramasubramanian, M. D. Srinivas, M. S. Sriram (1994). "[http://www.physics.iitm.ac.in/~labs/amp/kerala-astronomy.pdf Modification of the earlier Indian planetary theory by the Kerala astronomers (c. 1500 AD) and the implied heliocentric picture of planetary motion]", ''[[Current Science]]'' '''66''', p. 784-790.</ref>
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