Step 1: Recall the formula for total energy of a satellite.
The total mechanical energy of a satellite in circular orbit is
\[
E=-\frac{GMm}{2r}
\]
where
\[
G=\text{gravitational constant},
\]
\[
M=\text{mass of earth},
\]
\[
m=\text{mass of satellite},
\]
and
\[
r=\text{orbital radius}
\]
Step 2: Find the initial total energy.
Let the initial orbital radius be
\[
r
\]
Then initial total energy is
\[
E_i=-\frac{GMm}{2r}
\]
Step 3: Find the final total energy.
The orbital radius is reduced to half:
\[
r_f=\frac{r}{2}
\]
So,
\[
E_f=-\frac{GMm}{2(r/2)}
\]
\[
E_f=-\frac{GMm}{r}
\]
Now compare with
\[
E_i=-\frac{GMm}{2r}
\]
Thus,
\[
E_f=2E_i
\]
Hence, the magnitude of total energy becomes double.
Step 4: Calculate percentage change.
Initial magnitude of energy:
\[
|E_i|
\]
Final magnitude of energy:
\[
|E_f|=2|E_i|
\]
Increase in magnitude:
\[
2|E_i|-|E_i|=|E_i|
\]
Therefore,
\[
\text{Percentage change}
=
\frac{|E_i|}{|E_i|}\times 100
\]
\[
=100\%
\]
Step 5: Final conclusion.
Hence, the change in total energy is
\[
\boxed{100\%}
\]