सामग्री पर जाएँ
सर्वकोश
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 55, कुल 573 में से

संदर्भ में पढ़ें
पृष्ठ 55

35
by dividing the product of the number of lunations in
a Kalpa and (12 x + y) 30 + t where x is the number
of elapsed years, y the number of elapsed lunations t
the number of elapsed tithis in the current lunar month
at the time when the Ahargaṇa is being computed and
S the number of Solar days in a Kalpa. The form
of the Avama-Sesha was formerly stated as R / T. The
procedure given is as follows. In the first place, we are
asked to assume that the number of elapsed solar days is
equal to the number of elapsed tithis from the beginning of
Chaitra ie the beginning of the luni-Solar year, since we do
not know when the Solar year began; so, at the rate of 1°
per a Solar day (A Solar day is not a mean solar day,
Vide definition given before under verse 8. Bhagaṇādh-
yāya) the Sun’s position is given by as many degrees as
there are elapsed tithis; and the Moon’s position must be
13 times the same since each tithi means an increase of
12° in the elougation and if x° be the Sun’s position, the
Moon’s position must be 12 x° ahead of the Sun ie 13 x°.
Having got thus approximate positions of the Sun and the
Moon, we have to make amends for the roughness of the
assumption made. In assuming that the longitude of the
Sun is equal to the number of elapsed tithis, we have over-
estimated the longitude since it has to begin from the
beginning of the solar year. The time in between the
beginnings of the luni-Solar year and the solar year is
known as the Adhimāsa-Sesha at the time of the beginning
of the solar year, measured in tithis; also, we have com-
mitted an error in assuming the Sun’s rate to be 1° per tithi.
This also is due to Adhimāsa-Sesha subsequent to the
beginning of the Solar year upto the day concerned- Thus
the entire error committed by assuming the Sun’s longitude
to be as many degrees as there are elapsed tithis from the
beginning of the luni-Solar year. is no other than the Adhi-
māsa-Sesha at the day concerned, But this Adhimāsa-
Sesha is of the form (R′ × 30) / S as mentioned and is in tithis.