The mass and radius of the Earth and Moon are $M_1, R_1$ and $M_2, R_2$ respectively. Their centres are at a distance $d$ apart. The minimum speed with which a body of mass $m$ should be projected from a distance $\frac{2d}{3}$ from the centre of $M_1$ so as to escape to infinity is:

  • A
    $\left[\frac{3 G(M_1+2 M_2)}{d}\right]^{\frac{1}{2}}$
  • B
    $\left[\frac{3 G(M_1-M_2)}{2 d}\right]^{\frac{1}{2}}$
  • C
    $\left[\frac{6 G(M_1-M_2)}{2 d}\right]^{\frac{1}{2}}$
  • D
    $\left[\frac{6 G(M_1+M_2)}{d}\right]^{\frac{1}{2}}$

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