The velocity of a satellite in orbit around Earth can be determined by the formula for orbital velocity, which is given by:
\[ v = \sqrt{\frac{GM}{r}} \]
where:
- \( v \) is the orbital velocity,
- \( G \) is the gravitational constant,
- \( M \) is the mass of the Earth, and
- \( r \) is the distance from the center of the Earth to the satellite.
The altitude of a satellite is measured from the Earth's surface, so to find the radius \( r \), you need to add the Earth's radius (approximately 6371 km) to the altitude.
For Satellite A:
- Altitude = 500 km
- Radius \( r_A = 6371 , \text{km} + 500 , \text{km} = 6871 , \text{km} \)
For Satellite B:
- Altitude = 800 km
- Radius \( r_B = 6371 , \text{km} + 800 , \text{km} = 7171 , \text{km} \)
Now, we can see how the velocities compare:
- Since \( r_B > r_A \), then \( \sqrt{r_B} > \sqrt{r_A} \).
- Consequently, since the orbital velocity is inversely proportional to the square root of the radius, it follows that \( v_A > v_B \).
Thus, the velocity of Satellite A is greater than the velocity of Satellite B.
The correct conclusion is:
The velocity of Satellite A is greater than the velocity of Satellite B.