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 \( E = -\frac{J^2}{2mR^2} \).
Net gravitational force at the center of a square is found to be \( F_1 \) when four particles having masses \( M, 2M, 3M \) and \( 4M \) are placed at the four corners of the square as shown in figure, and it is \( F_2 \) when the positions of \( 3M \) and \( 4M \) are interchanged. The ratio \( \dfrac{F_1}{F_2} = \dfrac{\alpha}{\sqrt{5}} \). The value of \( \alpha \) is 

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