सामग्री पर जाएँ
सर्वकोश
ब्राह्मस्फुटसिद्धान्त (ब्रह्मगुप्त - शून्य, कुट्टक, बीजगणित एवं सम्पूर्ण २१ अध्याय सान्वय सटीक)

ब्राह्मस्फुटसिद्धान्त (ब्रह्मगुप्त - शून्य, कुट्टक, बीजगणित एवं सम्पूर्ण २१ अध्याय सान्वय सटीक)

Brahmasphuta Siddhanta of Brahmagupta with Commentary

आचार्य ब्रह्मगुप्त द्वारा

DevanagariHindipublished737 पृष्ठ

पृष्ठ 150, कुल 737 में से

संदर्भ में पढ़ें
पृष्ठ 150

110 INDIAN LUNI-SOLAR ASTRONOMY
chapter on शशि-दर्शनम् or the fiirst visibility of the crescent. It is
thus clear that the practice was to observe the Moon when very
near the Sun.
Again Āryabhaṭa says that 'रवीन्दुयोगात् प्रसाधितश्चेन्दुः',
"the Moon was determined from her conjunctions with the Sun."
The Moon was observed by him at the time of solar eclipses, or
at the time of the first visibility of the crescent.
Even up to the time of Pṛthūdaka, the accuracy in lunar
astronomy was chiefly aimed at the time of eclipses. Thus in
his commentary on the Khaṇḍakhādyaka. IV, he makes the
following introductory remarks :—
"All knowledge relating to (luni-solar) astronomy is desired
by the wise (or cultured) specially for knowing the right instants
of opposition or conjunction ; these instants are, however, not
visible to the eye. Of other things such as tithis, nakṣatras and
Karaṇas, as the planets, the Sun and the Moon, are not clearly
observed, their beginnings and ends are not visible. Men see
the agreement between calculation and observation at the times
of solar and lunar eclipses. Hence the word of the astronomers
is esteemed amongst men even in respect to such things as tithis,
etc."¹
Thus the chief aim of the ancient Indian astronomers was
to calculate the eclipses accurately and the Moon was observed
chiefly at lunar or solar eclipses, though the time for observation
related also to the fiinding of the first visibility of the crescent.
This latter phenomena did not perhaps lead them to directly
observing the Moon's position at such times by using instruments.
Moon's Mean Motion
The practice of observing the Moon at the time of the
eclipses alone led to the determination of the synodic month
with the following results :—
(i) Mean synodic month according to the Āryabhaṭīya
= 1577917500 / (57753336—4320000) days,
=29.530582 days.

  1. बाहुल्येन पर्व्वज्ञानार्थं सकलं ज्ञानमिष्यते शिष्टैः । तेषां च पर्व्वणां दर्शनं नास्ति ।
    अन्येषामपि तिथिनक्षत्रकरणानां तस्मात् तेषां शशिभास्करयोरव्यक्तित्वात् । शशिभास्कर-
    ग्रहणयोर् 'ग् गणितैक्यं लोकः पश्यति । तस्मात् तिथ्यादिष्वप्यर्थेषु दैवज्ञं वाक्यं लोके आद्रियते ।