Due 30 Mar. 1999
(3 points) A star of mass M = 2×1030 kg and radius R0= 7×108 m rotates with angular velocity . Suddenly the star collapses under the force of its own gravity, and its radius is reduced to R1= 104 m. For this problem, "collapse" means that the radius is reduced while the mass remains constant. Assume that the star remains spherical with a uniform mass density.
What is the angular velocity of the collapsed star? You can look up the moment of inertia of a uniform sphere.
Stability of the collapsed star demands that for an element of mass, dm, at the surface of the collapsed star, the gravitational acceleration exceeds the centripetal acceleration. Use this fact to derive a limit on the angular velocity after collapse, w1.