Step 1: Orbital radius from period.
For a circular orbit
\[
T=2\pi\sqrt{\frac{r^3}{\mu}}, \mu=GM_E.
\]
Hence
\[
r=\Big(\mu\,(T/2\pi)^2\Big)^{1/3}.
\]
Step 2: Substitute.
\[
\mu=6.67\times10^{-11}\times 5.98\times10^{24}=3.986\times10^{14}\ \text{m}^3\!/\text{s}^2,
\]
\[
T=90\times60=5400\ \text{s},
r=\Big(3.986\times10^{14}\,(5400/2\pi)^2\Big)^{1/3}=6.654\times10^6\ \text{m}.
\]
Step 3: Altitude.
\[
h=r-R_E=6.654\times10^6-6.370\times10^6=2.840\times10^5\ \text{m}
\Rightarrow \boxed{h\approx 284\ \text{km}}.
\]
F and G denote two points on a spacecraft’s orbit around a planet, as indicated in the figure. O is the center of the planet, P is the periapsis, and the angles are as indicated in the figure. If \( OF = 8000 \, {km} \), \( OG = 10000 \, {km} \), \( \theta_F = 0^\circ \), and \( \theta_G = 60^\circ \), the eccentricity of the spacecraft's orbit is __________ (rounded off to two decimal places).
F and G denote two points on a spacecraft’s orbit around a planet, as indicated in the figure. O is the center of the planet, P is the periapsis, and the angles are as indicated in the figure. If \( OF = 8000 \, {km} \), \( OG = 10000 \, {km} \), \( \theta_F = 0^\circ \), and \( \theta_G = 60^\circ \), the eccentricity of the spacecraft's orbit is ___________ (rounded off to two decimal places).
