The radius of the orbit of a geostationary satellite is (mean radius of the earth is $R$,angular velocity about its axis is $\omega$,and acceleration due to gravity on the earth's surface is $g$).

  • A
    $\left(\frac{g R^{2}}{\omega^{2}}\right)^{1 / 3}$
  • B
    $\frac{g R^{2}}{\omega^{2}}$
  • C
    $\left(\frac{g R^{2}}{\omega^{2}}\right)^{2 / 3}$
  • D
    $\left(\frac{g R^{2}}{\omega^{2}}\right)^{1 / 2}$

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