State Kepler's third law of planteray motion
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Kepler's third law of planetary motion states that
the cube of the mean distance of a planet from the sun is proportional to the square of its orbital period T. or,
r³/T² = constant
the cube of the mean distance of a planet from the sun is proportional to the square of its orbital period T. or,
r³/T² = constant
shakib0:
i ask it's definition or state it not ask it's deviation or formula anyways thank you
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