Naked Science Forum
Non Life Sciences => Physics, Astronomy & Cosmology => Topic started by: syhprum on 08/06/2010 20:46:03
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I could not resist this follow up from the previous question "How did scientists calculate the radius of the Earth and Sun"
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A set of experiments was done on earth to measure the gravitational attractions between balls of various masses. This defined the gravitational constant which was found to be the same fro an equal mass of any material.
The distances and orbital periods of the earth moon and sun have been known from earlier measurements and therefore using Newtons law of gravitation and the gravitational constant it is possible to calculate the masses of the earth moon and sun.
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If I have done the maths right:
Mass of the sun = ω²*r³/G
Where r is distance from sun to planet and ω is angular speed (= 2πf)