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b. There are two planets A and B having masses mi and m respectively.around the Sun in circular orbit. The orbital radius of A from the sun isorbital radius of B. The mass of A is twice that of mass of B. Compare th

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let the gravitational force on a be g×2b/4b^2 and on b the force is gb/r^2 now divide force of b by a 4/2 = 2 times therefore the gravitational force on b is twice of a



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