derive newtons law of gravitation using kepler's 3rd law
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In Kepler's third law of gravitation is the cube of the mean distance of a planet from the sun is directly proportional to the square of time it takes to move around the sun.
r3 is directly proportional to T2
r3=constant. T2
r3\T2= constant
r3 is directly proportional to T2
r3=constant. T2
r3\T2= constant
debasish9:
i needed the derivation
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