Ancient Indian Astronomy Key Discoveries : Calculation of Earth’s circumference First concept about gravity First concept of relativity Determining the number of planets in the Solar System Concept and calculation of solar and lunar eclipses Determining sidereal day and year , close to the actual one The earliest concept of a heliocentric model of the solar system Figure 3: A page from the book ‘Pancha-Sidhanta’ or ‘FivePrinciples’ written in 400-500 AD. [Shows how eclipses are to be calculated] Figure 2: A stone etching from Burzahom, Kashmir. [a hunting scene, with two bright objects in the sky, preferably the sun and the moon Figure 1: Rock art from Chillas, Kashmir. [Sun god with the disk of the Sun just behind him.] The division of the disk into four quadrants is probably indicative of the four seasons. Book ARYABHATIYA - By Astronomer-Mathematician Aryabhatta (476–550 CE) Key Contribution: • Proposed mathematical heliocentric model of solar system[1], mentioned in his book “Aryabhatia” , chapter “Gola”. Also mentioned that earth spins on its axis. • Calculated the circumference of earth equal to 24835 miles, which differs by 66 mi from the actual result, 24901 miles [2]. • Calculated length of the day as 23 hours, 56 minutes, and 4.1 seconds[3]; the actual value is 23:56:4.091 hours. Length of sidereal year 365.25858 days; the actual value is 365.25636 days; error of 3 minutes & 20 seconds over the length of a year [4]. • Provided explanation of lunar and solar eclipse . In his book, he mentioned 1,582,237,500 rotations of the Earth equal to 57,753,336 lunar orbits [4]. • Explained the cause of rising and setting of star and also the concept of relativity [4] saying the same way that someone in a boat going forward sees an unmoving Figure 4: Astronomer-Mathematician Aryabhatta; India’s 1st satellite was [object] going backward, so [someone]on the equator sees the unmoving stars named after him going uniformly westward. • A great mathematician, proposed the place-value system numbering system, provided approximation of Pi (correct to 4 decimal), sinusoidal function. Reference : 1. Translation from K. S. Shukla and K.V. Sarma, K. V. Āryabhaṭīya of Āryabhaṭa, 2. http://www.livemint.com/Sundayapp/8wRiLexg1N2IOXjeK2BKcL/How-Aryabhata-got-the-earths-circumference-right-millenia-a.html 3. Encyclopaedia of the history of science, technology, and medicine in non-western cultures http://www.springer.com/us/book/9781402044250 4. Gola chapter, Book Aryabhatia Continuation of Aryabhatta’s Concepts Brahmagupta (598-668 AD) : Brahmagupta, in the book Brahmasphuta Siddhanta (AD 628), explained heliocentric system of Aryabhata (AD 476–550) [1] stating that - all heavy things are attracted towards the center of the earth. Bhaskaracharya (1114-1185 AD) : 6th Sloka from Sidhanta Shiromani, Bhuvanakosa“akrsta saktisca mahi taya yat svastham guru svabhimukham svasaktya akrsyate tatpatativa bhati same samantat kva patatviyam khe”. It means every object falls on the ground due to earth’s force of attraction. This force allows the sun, earth, moon and constellations to stay in the orbit. Mention of astronomy in Indian mythology: In a prayer, to the Hindu God ‘Hanuman’ , named as ‘Hanuman-Chalisa’, by poet Tulsidas, the distance between the earth and sun has been mentioned as – “Juga X Sahastra X jojan’ =12000 X 1000 X 8 miles = 9,60,00,000 miles, (near to the actual value) . Figure 5: Astronomical Influence in megalithic structures; Sun dial in 13thcentury CE Sun Temple at Konark in Orissa, India. References: 1. https://www.cs.mcgill.ca/~rwest/link-suggestion/wpcd_2008-09_augmented/wp/g/Gravitation.htm
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