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 \( E = -\frac{J^2}{2mR^2} \).
The height from Earth's surface at which acceleration due to gravity becomes \(\frac{g}{4}\) is \(\_\_\)? (Where \(g\) is the acceleration due to gravity on the surface of the Earth and \(R\) is the radius of the Earth.)