The time period of revolution of a satellite close to the planet’s surface is 80 minutes. The time period of another satellite which is at a height of 3 times the radius of the planet from the surface is:
Show Hint
Kepler’s third law states that the time period of a satellite increases as the cube root of the orbital radius. The farther the satellite, the longer its revolution time.
Step 1: Use Kepler’s Third Law
Kepler’s third law states that the square of the orbital period \( T \) is proportional to the cube of the semi -major axis \( R \):
\[
T^2 \propto R^3
\]
Step 2: Calculate the Ratio of Time Periods
For a satellite near the planet’s surface:
\[
T_1 = 80 \text{ minutes}
\]
The radius of the second satellite’s orbit is:
\[
R_2 = R + 3R = 4R
\]
Using Kepler’s law:
\[
\left( \frac{T_2}{T_1} \right)^2 = \left( \frac{R_2}{R_1} \right)^3
\]
\[
\left( \frac{T_2}{80} \right)^2 = \left( \frac{4R}{R} \right)^3 = 4^3 = 64
\]
\[
T_2 = 80 \times 8 = 640 \text{ minutes}
\]