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An extremely small and dense neutron sta...

An extremely small and dense neutron star of mass M and radius R is rotating with angular velocity `omega`. If an object is placed at its equator, then it will remain stuck to it due to gravity, if

A

`Mgt(Romega)/(G)`

B

`Mgt(R^2omega^2)/(G)`

C

`Mgt(R^3omega^3)/G`

D

`Mgt(R^2omega^2)/G`

Text Solution

Verified by Experts

The correct Answer is:
C
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