$A$ body of mass $m$ starts falling from a distance $3R$ above the Earth's surface. When it reaches a distance $R$ above the surface of the Earth (radius $R$,mass $M$),its kinetic energy is:

  • A
    $\frac{2}{3} \frac{GMm}{R}$
  • B
    $\frac{1}{3} \frac{GMm}{R}$
  • C
    $\frac{1}{2} \frac{GMm}{R}$
  • D
    $\frac{1}{4} \frac{GMm}{R}$

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