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7.Gravitation
normal
A body of mass $m$ is situated at a distance equal to $2R$ ($R-$ radius of earth) from earth's surface. The minimum energy required to be given to the body so that it may escape out of earth's gravitational field will be
A
$mgR$
B
$\frac{mgR}{3}$
C
$\frac{mgR}{2}$
D
$\frac{mgR}{4}$
Solution
$\mathrm{E}_{\mathrm{es}}=-\mathrm{PE}$
$\Rightarrow \mathrm{PE}=-\frac{\mathrm{GMm}}{3 \mathrm{R}}$
$\Rightarrow \mathrm{PE}=-\frac{\mathrm{mgR}}{3} \Rightarrow \quad \mathrm{Ees}=\frac{\mathrm{mgR}}{3}$
Standard 11
Physics