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+1 vote
81.0k views
in Physics by (48.7k points)

The mass density of a spherical galaxy varies as \(\frac{k}{r}\) over a large distance ‘r’ from its centre. In that region, a small star is in a circular orbit of radius R. Then the period of revolution, T depends on R as

(1)  T∝ \(\frac{1}{R^3}\)

(2)  T∝ R

(3)  T ∝ R

(4)  T2 ∝ R3

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