Gravitation
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Consider a star of mass m 2 k g revolving in a circular orbit around another star of mass m 1 k g with m 1 ≫ m 2 . The heavier star slowly acquires mass from the lighter star at a constant rate of γ k g ∕ s . In this transfer process, there is no other loss of mass. If the separation between the centers of the stars is r , then its relative rate of change
(in s − 1 ) is given by:
[JEE Adv 2025 P2]
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