To find the additional kinetic energy required to transfer a satellite from a circular orbit of radius $R_1$ to another orbit of radius $R_2$, we proceed as follows.
- Start by recalling the formula for the total energy of a satellite in a circular orbit. The total energy \(E\) is given by:
$$E = -\frac{G m M}{2R}$$
where $G$ is the gravitational constant, $m$ is the mass of the satellite, $M$ is the mass of the planet, and $R$ is the radius of the orbit.
- The kinetic energy $K$ of the satellite is one half of the magnitude of the total energy:
$$K = -\frac{E}{2} = \frac{G m M}{2R}$$
- The problem asks for the additional kinetic energy required for moving the satellite from radius $R_1$ to $R_2$. We calculate the difference in kinetic energy:
$$\Delta K = K_2 - K_1 = \frac{G m M}{2R_2} - \frac{G m M}{2R_1}$$
- Simplifying the expression for $\Delta K$:
$$\Delta K = \frac{G m M}{2} \left(\frac{1}{R_2} - \frac{1}{R_1}\right)$$
or equivalently:
$$\Delta K = \frac{1}{2} G m M \left(\frac{1}{R_1} - \frac{1}{R_2}\right)$$
This expression matches the option:
$\frac{1}{2} G m M \left(\frac{1}{R_1} - \frac{1}{R_2}\right)$
Hence, the correct answer is:
$\frac{1}{2} G m M \left(\frac{1}{R_1} - \frac{1}{R_2}\right)$
This is the amount of additional kinetic energy that must be provided to the satellite to move from an orbit of radius $R_1$ to $R_2$.