$A$ certain planet completes one rotation about its axis in time $T$. The weight of an object placed at the equator on the planet's surface is a fraction $f$ ($f$ is close to unity) of its weight recorded at a latitude of $60^{\circ}$. The density of the planet (assumed to be a uniform perfect sphere) is given by

  • A
    $\left(\frac{4-f}{1-f}\right) \cdot \frac{3 \pi}{4 G T^2}$
  • B
    $\left(\frac{4-f}{1+f}\right) \cdot \frac{3 \pi}{4 G T^2}$
  • C
    $\left(\frac{4-3f}{1-f}\right) \cdot \frac{3 \pi}{4 G T^2}$
  • D
    $\left(\frac{4-2f}{1-f}\right) \cdot \frac{3 \pi}{4 G T^2}$

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