Masses and radii of Earth and Moon are $M_1, M_2$ and $R_1, R_2$ respectively. The distance between their centers is $d$. The minimum velocity given to a mass $m$ from the midpoint of the line joining their centers so that it escapes the gravitational field of both is:

  • A
    $\sqrt{\frac{4G(M_1 + M_2)}{d}}$
  • B
    $\sqrt{\frac{4G}{d} \frac{M_1 M_2}{(M_1 + M_2)}}$
  • C
    $\sqrt{\frac{2G}{d} \left(\frac{M_1 + M_2}{M_1 M_2}\right)}$
  • D
    $\sqrt{\frac{2G}{d} (M_1 + M_2)}$

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