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A pair of stars rotates about a common centre of mass. One of the stars has a mass Mand the other has mass m such that =2m. The distance between the centres of the stars is d ( d being large compare to the size of eithe star). The period of rotation of the stars about their common centre of mass ( in terms of d,m,G) is |
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Answer» `sqrt((4 PI^(2))/(GM)d^(3))` |
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