The angular velocity of rotation of a star (of mass M and radius R) at which matter will…
Physics · NEET · NTA Exams — Gravitation
The angular velocity of rotation of a star (of mass M and radius R) at which matter will start escaping from its equator is
- \(\sqrt{\frac{2 C R}{M}}\)
- \(\sqrt{\frac{2 C M}{R^{3}}}\)
- \(\sqrt{\frac{2 \mathrm{CM}}{\mathrm{R}}}\)
- \(\sqrt{\frac{2 G M^{2}}{R}}\)
Answer
(B) 2 C M R^ 3
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