$A$ body (mass $m$) starts its motion from rest from a point distant $R_0$ $(R_0 > R)$ from the centre of the Earth. The velocity acquired by the body when it reaches the surface of the Earth will be ($G =$ universal constant of gravitation,$M =$ mass of Earth,$R =$ radius of Earth).

  • A
    $2 GM \left( \frac{1}{R} - \frac{1}{R_0} \right)$
  • B
    $\left[ 2 GM \left( \frac{1}{R} - \frac{1}{R_0} \right) \right]^{\frac{1}{2}}$
  • C
    $GM \left( \frac{1}{R} - \frac{1}{R_0} \right)$
  • D
    $2 GM \left[ \left( \frac{1}{R} - \frac{1}{R_0} \right) \right]^{\frac{1}{2}}$

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