write Newton's three equation for gravitation
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The one most people know describes Newton's universal law of gravitation: F = Gm1m2/r2, where F is the force due to gravity, between two masses (m1 and m2), which are a distance r apart; G is the gravitational constant
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Newton's Universal Law of Gravitation. Newton's equation first appeared in the Philosophiæ Naturalis Principia Mathematica, July 1687. ... Theequation says that the force (F) between two objects is proportional to the product of their masses (m1 and m2), divided by the square of the distance between them.
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