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Question

Physics Question on mechanical properties of fluid

If the potential energy of a body on a planet is numerically UU and the escape velocity for the same body be vev_{e} for the same planet then U/veU / v_{e} will be :

A

Uve=mGM2R\frac{U}{v_{e}}=m \sqrt{\frac{G M}{2 R}}

B

Uve=mGM2R\frac{U}{{{v}_{e}}}=m\sqrt{\frac{GM}{2R}}

C

Uve=m2GMR\frac{U}{{{v}_{e}}}=m\sqrt{\frac{2GM}{R}}

D

Uve=mGMR\frac{U}{{{v}_{e}}}=m\frac{GM}{R}

Answer

Uve=mGM2R\frac{U}{{{v}_{e}}}=m\sqrt{\frac{GM}{2R}}

Explanation

Solution

The work obtained in bringing a body from infinity to a point in a gravitational field is called the gravitational potential energy of the body at that point.
U=GMmR...(1)U=-\frac{G M_{m}}{R}\,\,\,...(1)
where GG is gravitational constant, MM is mass of earth RR its radius and mm is mass of body.
Also for a body projected upwards at a certain velocity of projection the body will go out of the gravitational field of the earth and will never return to the earth, this initial velocity is called escape velocity.
ve=2GMR...(2)v_{e}=\sqrt{\frac{2 G M}{R}}\,\,\,\,...(2)
Since, work is required to take a body from earth's surface to infinity, we have
U=+GMmR....(3)U=+\frac{G M_{m}}{R}\,\,\,\,....(3)
Dividing E (3) by (2), we get
Uve=mGM2R\frac{U}{v_{e}}=m \sqrt{\frac{G M}{2 R}}