सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)
Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary
भास्कराचार्य द्वितीय द्वारा
पृष्ठ 143, कुल 573 में से
संदर्भ में पढ़ें123 beginning of the Madhyādhikāra, Bhagaṇādhyaya in verses 1 to 6. Even Bhāskara gave such a proof as appealed to Āgama ie. 'Authority', which proof therefore will not be acceptable to a student of Modern Astronomy, who is likely to question how the Āgama came into existence. How the Āgama came to formulate the number of sidereal revolutions of the grahas, we shall now see. The forefathers of Hindu Astronomy (have been re- ported to be eighteen in number in the famous verses " सूर्यः पितामहो व्यासो वसिष्ठोऽत्रिः पराशरः कश्यपो नारदो गर्गो मरीचिर्मनु- रङ्गिराः लोमशः पौलिशश्चैव च्यवनो यवनो भृगुः, शौनकोऽष्टादशैतेस्युः ज्योतिषशास्त्रप्रवर्तकाः " Of these Brahmagupta mentions Brahma-Siddhānta, which he reports to have resuscitated. Varāha Mihira gave a version of the old Sūryasiddhānta, mentioning that it accorded with observations. Āryabhata says that he revived his system from the then existing ocean of knowledge both good and spurious. The fact that none of these outstanding astronomers mentioned that they had derived their systems from a foreign source, and the reasonableness in presuming that all these three could not be impostors, make the author of this work feel strongly that there should have been some works in the name of Āgamas extant long before these Acharyās. The argument that the crude Vedānga-jyotiṣa alone should have existed before Āryabhata, simply because, no other work worth the name has been discovered, may not be correct. It is quite possible that crude works could exist side by side with advanced scientific works, just as even nowadays we have thinkers and works of a primitive type existing along with highly advanced thinkers as well as scientific works). Bhagaṇopapatti. In the first place, the forefathers of Hindu Astronomy must have noticed very easily that the Moon has a motion among stars, for, this could be detected