Step 1: The angular momentum \( J \) is related to the kinetic energy \( K \) and the radius \( R \) by the formula:
\[ J = mRv \]
where \( v \) is the velocity of the satellite.
Step 2: The total kinetic energy is given by:
\[ K = \frac{1}{2} mv^2 \]
From the relationship \( J = mRv \), we can solve for \( v \) and substitute it into the equation for kinetic energy to get:
\[ K = \frac{J^2}{2mR^2}. \]
Step 3: The total energy \( E \) of the satellite in orbit is the sum of its kinetic and potential energy. The potential energy is \( U = -\frac{GMm}{R} \), where \( G \) is the gravitational constant and \( M \) is the mass of the Earth. The total energy is then:
\[ E = K + U = \frac{J^2}{2mR^2} - \frac{GMm}{R}. \]
Therefore, the correct answer is \( K = \frac{J^2}{2mR^2} \) and \( E = -\frac{J^2}{2mR^2} \).
Match the LIST-I with LIST-II
\[ \begin{array}{|l|l|} \hline \text{LIST-I} & \text{LIST-II} \\ \hline \text{A. Gravitational constant} & \text{I. } [LT^{-2}] \\ \hline \text{B. Gravitational potential energy} & \text{II. } [L^2T^{-2}] \\ \hline \text{C. Gravitational potential} & \text{III. } [ML^2T^{-2}] \\ \hline \text{D. Acceleration due to gravity} & \text{IV. } [M^{-1}L^3T^{-2}] \\ \hline \end{array} \]
Choose the correct answer from the options given below:

A quantity \( X \) is given by: \[ X = \frac{\epsilon_0 L \Delta V}{\Delta t} \] where:
- \( \epsilon_0 \) is the permittivity of free space,
- \( L \) is the length,
- \( \Delta V \) is the potential difference,
- \( \Delta t \) is the time interval.
The dimension of \( X \) is the same as that of: