Varahamihira, a renowned astronomer and mathematician from the 6th century CE, made significant contributions to the study of eclipses and other celestial phenomena.

Ancient Indian astronomers primarily relied on observation and recording of historical eclipse data to predict future eclipses.

The term 'Sandhi' was used in ancient Indian astronomy to describe the moment of totality during a solar eclipse.

The Surya Siddhanta, an influential astronomical text from ancient India, contains detailed descriptions and predictions of eclipses.

In ancient India, studying eclipses was primarily aimed at predicting future events and outcomes, often associated with astrology and religious beliefs.

Aryabhata, a renowned mathematician and astronomer from the 5th century CE, developed a mathematical model to calculate the timing and duration of eclipses.

In ancient India, eclipses held religious significance and were associated with divine omens, specific deities, astrological influences, misfortune, and the determination of auspicious dates.

Aryabhata was the first ancient Indian astronomer to propose that the Earth's shadow caused lunar eclipses.

The term 'Grahana' was used in ancient Indian astronomy to describe the moment of totality during a lunar eclipse.

The Brihat Samhita, an encyclopedic text by Varahamihira, contains detailed descriptions of various types of eclipses and their astrological significance.

Ancient Indian astronomers primarily relied on naked-eye observations to observe and record eclipses.

Aryabhata developed a method to calculate the size and shape of the Earth's shadow during a lunar eclipse.

In ancient Indian astronomy, studying eclipses served multiple purposes, including predicting future events, understanding celestial movements, performing religious rituals, and calculating the length of the year.

Aryabhata was the first ancient Indian astronomer to propose that the Moon's shadow caused solar eclipses.

The term 'Samyoga' was used in ancient Indian astronomy to describe the moment of totality during a solar eclipse.