Concept:
For heights comparable to Earth's radius, acceleration due to gravity is not constant. Use conservation of mechanical energy:
\[
\frac{1}{2}mv^2 = mgh \text{ (invalid for large h)}
\]
Correct approach:
\[
\frac{1}{2}mv^2 = GMm\left(\frac{1}{R} - \frac{1}{R+h}\right) = mgR^2\left(\frac{1}{R} - \frac{1}{R+h}\right)
\]
where \(GM = gR^2\).
Step 1: Energy conservation equation.
\[
\frac{1}{2}mv^2 = mgR^2\left(\frac{1}{R} - \frac{1}{R+h}\right)
\]
Cancel \(m\) and simplify:
\[
\frac{v^2}{2} = gR^2\left(\frac{R+h - R}{R(R+h)}\right) = gR^2\left(\frac{h}{R(R+h)}\right) = \frac{gRh}{R+h}
\]
Step 2: Solve for \(h\).
\[
\frac{v^2}{2} = \frac{gRh}{R+h}
\]
\[
v^2(R+h) = 2gRh
\]
\[
v^2R + v^2h = 2gRh
\]
\[
v^2R = h(2gR - v^2)
\]
\[
h = \frac{v^2R}{2gR - v^2}
\]
Step 3: Substitute values.
\[
v = 4 \, km/s = 4000 \, m/s
\]
\[
R = 6400 \, km = 6.4 \times 10^6 \, m
\]
\[
g = 9.8 \, m/s^2
\]
\[
h = \frac{(4000)^2 \times (6.4 \times 10^6)}{2 \times 9.8 \times (6.4 \times 10^6) - (4000)^2}
\]
\[
= \frac{16 \times 10^6 \times 6.4 \times 10^6}{2 \times 9.8 \times 6.4 \times 10^6 - 16 \times 10^6}
\]
\[
= \frac{102.4 \times 10^{12}}{(125.44 - 16) \times 10^6}
\]
\[
= \frac{102.4 \times 10^{12}}{109.44 \times 10^6}
\]
\[
= \frac{102.4}{109.44} \times 10^6 \, m
\]
\[
\approx 0.935 \times 10^6 \, m = 935 \, km
\]