MCQ
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
- A$\sqrt {\frac{{2G{M^2}}}{R}} $
- B$\sqrt {\frac{{2GM}}{g}} $
- ✓$\sqrt {\frac{{2GM}}{{{R^3}}}} $
- D$\sqrt {\frac{{2GR}}{M}} $
