Step 1: Understanding the Concept:
We need to find a relationship between the orbital velocity of a satellite at a specific altitude and the escape velocity from the surface of the Earth. Step 2: Key Formula or Approach:
1. Escape Velocity (\( V_e \)) from the surface of the Earth (radius R, mass M): The minimum velocity needed to escape Earth's gravity.
\[ V_e = \sqrt{\frac{2GM}{R}} \]
2. Orbital Velocity (\( V_o \)) of a satellite in a circular orbit at a radius r from the center of the Earth:
\[ V_o = \sqrt{\frac{GM}{r}} \]
Step 3: Detailed Explanation:
The satellite is at a height H=R from the surface. The orbital radius 'r' is the distance from the center of the Earth.
\[ r = R + H = R + R = 2R \]
Now, let's write the expression for the orbital velocity at this radius:
\[ V_o = \sqrt{\frac{GM}{2R}} \]
We want to express this in terms of \( V_e = \sqrt{\frac{2GM}{R}} \).
From the escape velocity formula, we can write \( GM = \frac{V_e^2 R}{2} \). Let's substitute this into the orbital velocity formula.
\[ V_o = \sqrt{\frac{1}{2R} \left( \frac{V_e^2 R}{2} \right)} \]
\[ V_o = \sqrt{\frac{V_e^2 R}{4R}} = \sqrt{\frac{V_e^2}{4}} \]
\[ V_o = \frac{V_e}{2} \]
This result matches the provided correct answer. My initial thought about \(V_e/\sqrt{2}\) was for an orbit close to the surface (r=R).
Step 4: Final Answer:
The orbital velocity is \( \frac{V_e}{2} \).