The Surya Siddhanta was translated into Latin in the 13th century by Gerard of Cremona, and it had a significant influence on the development of European astronomy. It was one of the first Indian astronomical texts to be translated into a European language, and it introduced European astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Aryabhata is credited with developing the concept of the precession of the equinoxes, which is the gradual shift in the position of the equinoxes over time. He also developed a method for calculating the length of the year, which was more accurate than the methods used by European astronomers at the time.

Bhaskara II developed a model of the solar system that included the idea of elliptical orbits. He also developed a method for calculating the distance between the Earth and the Moon, which was more accurate than the methods used by European astronomers at the time.

The Pancasiddhantika was translated into Persian in the 10th century, and it had a significant influence on the development of Islamic astronomy. It was one of the first Indian astronomical texts to be translated into an Islamic language, and it introduced Islamic astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Varahamihira developed a method for calculating the time of sunrise and sunset. He also developed a method for calculating the length of the day, which was more accurate than the methods used by European astronomers at the time.

The Aryabhatiya was translated into Arabic in the 9th century, and it had a significant influence on the development of Arabic astronomy. It was one of the first Indian astronomical texts to be translated into an Arabic language, and it introduced Arabic astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Aryabhata developed a method for calculating the circumference of the Earth. He also developed a method for calculating the distance between the Earth and the Moon, which was more accurate than the methods used by European astronomers at the time.

The Surya Siddhanta was translated into Chinese in the 7th century, and it had a significant influence on the development of Chinese astronomy. It was one of the first Indian astronomical texts to be translated into a Chinese language, and it introduced Chinese astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Brahmagupta developed a method for calculating the area of a triangle. He also developed a method for calculating the volume of a sphere, which was more accurate than the methods used by European astronomers at the time.

The Aryabhatiya was translated into Hebrew in the 12th century, and it had a significant influence on the development of Jewish astronomy. It was one of the first Indian astronomical texts to be translated into a Jewish language, and it introduced Jewish astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Varahamihira developed a method for calculating the time of an eclipse. He also developed a method for calculating the length of the day, which was more accurate than the methods used by European astronomers at the time.

The Surya Siddhanta was translated into Greek in the 6th century, and it had a significant influence on the development of Greek astronomy. It was one of the first Indian astronomical texts to be translated into a Greek language, and it introduced Greek astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Aryabhata developed a method for calculating the distance between the Earth and the Sun. He also developed a method for calculating the circumference of the Earth, which was more accurate than the methods used by European astronomers at the time.

The Surya Siddhanta was translated into Latin in the 16th century, and it had a significant influence on the development of European astronomy. It was one of the first Indian astronomical texts to be translated into a European language, and it introduced European astronomers to new concepts such as the use of the sine function in trigonometry and the concept of a heliocentric universe.

Varahamihira developed a method for calculating the time of a solar eclipse. He also developed a method for calculating the length of the day, which was more accurate than the methods used by European astronomers at the time.