The mass density of a spherical galaxy varies as over a large distance from its centre

PHYSICS · Single correct · AP · Physics C: Mechanics · Force and Translational Dynamics · Force and Translational Dynamics

Problem

The mass density of a spherical galaxy varies as Kr\frac{K}{r} over a large distance rr from its centre. In that region, a small star is in a circular orbit of radius RR. Then the period of revolution, TT depends on RR as : (1) T2∝RT^2 \propto R (2) T2∝R3T^2 \propto R^3 (3) T2∝1R3T^2 \propto \frac{1}{R^3} (4) T∝RT \propto R

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