$A$ satellite is revolving around a planet in a circular orbit close to its surface. Let $\rho$ be the mean density and $R$ be the radius of the planet; then the period of the satellite is $(G = \text{Universal constant of gravitation})$

  • A
    $\sqrt{3\pi/\rho G}$
  • B
    $\sqrt{2\pi/\rho G}$
  • C
    $\sqrt{\pi/\rho G}$
  • D
    $\sqrt{4\pi/\rho G}$

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