The additional kinetic energy to be provided to a satellite of mass $m$ revolving around a planet of mass $M$ to transfer it from a circular orbit of radius $R_1$ to another of radius $R_2$ $(R_2 > R_1)$ is:

  • A
    $GMm \left( \frac{1}{R_1^2} - \frac{1}{R_2^2} \right)$
  • B
    $\frac{GMm}{2} \left( \frac{1}{R_1} - \frac{1}{R_2} \right)$
  • C
    $2GMm \left( \frac{1}{R_1} - \frac{1}{R_2} \right)$
  • D
    $\frac{GMm}{R_1} - \frac{GMm}{R_2}$

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