$A$ planet of mass $m$ moves in an ellipse around the sun of mass $M_S$ such that its maximum and minimum distances are $r_1$ and $r_2$ respectively. The angular momentum of the planet relative to the center of the sun is

  • A
    $\sqrt{\frac{2GM_Sr_1}{r_1 + r_2}}$
  • B
    $\sqrt{\frac{2GM_Sm^2r_1r_2}{r_1 + r_2}}$
  • C
    $\sqrt{\frac{GM_Sr_1r_2}{r_1 + r_2}}$
  • D
    $\sqrt{\frac{2GM_S}{r_1r_2(r_1 + r_2)}}$

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