Step 1: Understanding the Energy of a Satellite in Orbit
- The total mechanical energy of a satellite in a circular orbit is given by:
\[
E_{\text{total}} = KE + PE = -\frac{GMm}{2r}.
\]
- The kinetic energy of the satellite is given by:
\[
KE = \frac{GMm}{2r}.
\]
- The potential energy of the satellite in orbit is:
\[
PE = -\frac{GMm}{r}.
\]
- The total energy of the system is:
\[
E_{\text{total}} = KE + PE = \frac{GMm}{2r} - \frac{GMm}{r} = -\frac{GMm}{2r}.
\]
- Since we are given that kinetic energy is \( E \), we write:
\[
KE = E = \frac{GMm}{2r}.
\]
Thus, the total energy of the satellite is:
\[
E_{\text{total}} = -E.
\]
Step 2: Energy Required for Escape
- For the satellite to escape Earth's gravitational field, its total energy must be zero (i.e., it must reach infinity with zero velocity).
- The energy required to remove the satellite from orbit is:
\[
E_{\text{required}} = 0 - E_{\text{total}}.
\]
Substituting \( E_{\text{total}} = -E \),
\[
E_{\text{required}} = 0 - (-E) = E.
\]
Thus, the minimum energy required to make the satellite escape from the Earth is:
\[
\boxed{E}.
\]