The total mechanical energy \( E \) of a satellite in a circular orbit is given by the sum of its kinetic energy and gravitational potential energy:
\[ E = K + U \]
where:
The kinetic energy \( K \) of the satellite is given by:
\[ K = \frac{1}{2} m v^2 \]
Substituting \( m = 10 \) kg and \( v = 200 \) m/s:
\[ K = \frac{1}{2} \times 10 \times (200)^2 \]
\[ K = 5 \times 40000 = 200000 \text{ J} \]
The gravitational potential energy \( U \) for an object in orbit is given by:
\[ U = -\frac{GMm}{r} \]
where:
For a circular orbit, the gravitational force provides the centripetal force required for the satellite’s circular motion:
\[ \frac{GMm}{r^2} = \frac{m v^2}{r} \]
Solving for \( r \):
\[ r = \frac{GM}{v^2} \]
Substituting this into the potential energy equation:
\[ U = -\frac{1}{2} m v^2 \]
Thus, the total energy is:
\[ E = K + U = \frac{1}{2} m v^2 - \frac{1}{2} m v^2 = -\frac{1}{2} m v^2 \]
Substituting \( m = 10 \) kg and \( v = 200 \) m/s:
\[ E = -\frac{1}{2} \times 10 \times (200)^2 \]
\[ E = -5 \times 40000 = -200000 \text{ J} \]
\[ E = -200 \text{ kJ} \]
The total energy of the satellite is \(-200\) kJ.