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Answer: According to Kepler's third law, The square of orbital period of revolution T of a planet around a star is directly proportional to the cube of the mean distance R of the planet from the star. Thus, for a planet, at a distance of 2R from the star, its period of revolution will be √8 T.
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Answer:
According to Kepler thirdthird law the square of orbitalperiod of revelution t of a planet around
a star is directly proportional to the cube of the mean distance r of the planet from the star for a planet at a distance of 2r from the star it's period of revelation will be √8 t
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