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सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

सिद्धान्तशिरोमणि: गणिताध्याय (भास्कराचार्य - ग्रहगणित, मध्यमाधिकार व स्पष्टाधिकार सटीक)

Siddhanta Shiromani Ganitadhyaya of Bhaskaracharya with Commentary

भास्कराचार्य द्वितीय द्वारा

DevanagariHindipublished573 पृष्ठ

पृष्ठ 86, कुल 573 में से

संदर्भ में पढ़ें
पृष्ठ 86

66
Rule. If the Ahargaṇa be x days then the Śīghra will
be 4x° + (4x × 3') / 130 + Dhruvaka. Proof. For x days, the mean
motion is x × 4° + x × (0-5′-32″-18‴-28⁗). The second
part is taken to be 4x × 3° / 130 ie x × 12° / 130 = x × 6/65° for
6/65 of a degree = 0-5′-32″-18‴-"28"". The fraction 6/65 can
be seen to be a convergent of the remainder for 5′-32″-
18‴-28⁗ = 299077° / 3240000 = 1/(10 +) 1/(1 +) 1/(4 +) 1/(1 +) 1/9968 of which the
penultimate convergent is 6/65.
Verse 19. The Ahargaṇa divided by 12 and by 71
gives respectively the positive degrees and negative minutes
to be added to the Dhruvaka of Jupiter.
Comm. If x be the Ahargaṇa x° / 12 − x' / 71 + Dhruvaka =
Guru.
The mean daily motion of Jupiter is 0-4-59-9.9 = 0-5′
minus 0-0-0-50-51. Evidently 0-5′ × x = x° / 12. The
remainder 0-0-0-50-51 = 61′ / 4320 of which the continued
fraction is 1/(70 +) 1/(1 +) 1/4. A very approximate convergent
is 1/71 as given.
Verse 19 contd. To obtain the position of the Śīghra
of venus.
The Ahargaṇa multiplied by 10 and divided by 6 and
155 respectively gives degrees positive and negative to be
added to the Dhruvaka of Venus to give his position.
Comm. The formula is 10 x / 6 − 10 x / 155. The mean daily
motion of the Śīghra of Venus is 1°-36′-7″-44‴-35⁗ =