Step 1: Orbit radius at the given point.
Altitude \(=600\ \text{km}\Rightarrow r = R_E+600 = 6400+600 = 7000\ \text{km} = 7.0\times10^{6}\ \text{m}.\)
Step 2: Circular and escape speeds at \(r\).
Circular speed: \(V_c=\sqrt{\mu/r}\), \(\mu=GM_E=3.98\times10^{14}\). \[ V_c=\sqrt{\frac{3.98\times10^{14}}{7.0\times10^{6}}} =\sqrt{5.6857\times10^{7}}\approx 7.54\times10^{3}\ \text{m/s}=7.54\ \text{km/s}. \] Escape speed: \(V_{\mathrm{esc}}=\sqrt{2\mu/r}=\sqrt{2}\,V_c\approx 10.67\ \text{km/s}.\)
Step 3: Classify using speed range (or energy sign).
Given \(V=9\ \text{km/s}\) satisfies \(V_c(7.54) < V(9) < V_{\mathrm{esc}}(10.67)\).
Equivalently, specific mechanical energy \(\varepsilon=\tfrac{V^2}{2}-\tfrac{\mu}{r}\) is negative (bound) but not the special circular case.
Hence the conic is a bounded ellipse (non-circular). \[ \boxed{\text{Elliptic trajectory}} \]
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).
