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) T2 ∝ \(\frac{1}{R^3}\)
(2) T2 ∝ R
(3) T ∝ R
(4) T2 ∝ R3