Step 1: Angular momentum \( J \) relates to kinetic energy \( K \) and radius \( R \) as:
\[ J = mRv \]
where \( v \) is the satellite's velocity.
Step 2: Total kinetic energy is:
\[ K = \frac{1}{2} mv^2 \]
Using \( J = mRv \), solve for \( v \) and substitute into the kinetic energy equation to get:
\[ K = \frac{J^2}{2mR^2}. \]
Step 3: Total energy \( E \) of the satellite is the sum of kinetic and potential energy. Potential energy is \( U = -\frac{GMm}{R} \), where \( G \) is the gravitational constant and \( M \) is Earth's mass. Total energy is then:
\[ E = K + U = \frac{J^2}{2mR^2} - \frac{GMm}{R}. \]
Thus, the correct answer is \( K = \frac{J^2}{2mR^2} \) and \( E = -\frac{J^2}{2mR^2} \).