Step 1: Understanding the Energy of a Satellite in Orbit
The total mechanical energy of a satellite in a stable circular orbit is the sum of its kinetic and potential energies. These are defined as:
- Kinetic Energy (KE):
\[
KE = \frac{GMm}{2r}
\]
- Potential Energy (PE):
\[
PE = -\frac{GMm}{r}
\]
- Total Energy (Etotal):
\[
E_{\text{total}} = KE + PE = \frac{GMm}{2r} - \frac{GMm}{r} = -\frac{GMm}{2r}
\]
If the satellite’s kinetic energy is given as \( E \), then:
\[
KE = E = \frac{GMm}{2r}
\]
Using this, we can express total energy in terms of \( E \):
\[
E_{\text{total}} = -E
\]
Step 2: Energy Required for Escape
To make the satellite escape Earth’s gravity completely, it must reach a point infinitely far away with zero residual velocity, meaning its total energy must become zero:
\[
E_{\text{final}} = 0
\]
Therefore, the minimum energy required to escape is the amount needed to raise its total energy from \( -E \) to \( 0 \):
\[
E_{\text{required}} = E_{\text{final}} - E_{\text{total}} = 0 - (-E) = E
\]
Final Answer:
Hence, the minimum energy that must be supplied to the satellite in orbit to escape Earth’s gravity is:
\[
\boxed{E}
\]