The angular velocity of rotation of star (of mass M and radius R) at which the matter start to escape from its equator will be [MH CET 1999]

\[\sqrt{\frac{2G{{M}^{2}}}{R}}\]

There will be repulsion between A and B and also x and y

The angular velocity of rotation of star (of mass M and radius R) at w

1.	The angular velocity of rotation of star (of mass M and radius R) at which the matter start to escape from its equator will be [MH CET 1999]
A.	\[\sqrt{\frac{2G{{M}^{2}}}{R}}\]
B.	\[\sqrt{\frac{2GM}{g}}\]
C.	There will be repulsion between A and B and also x and y
D.	\[\sqrt{\frac{2GR}{M}}\]
Answer» D. \[\sqrt{\frac{2GR}{M}}\]