The correct answer is (a) True.
Explanation:
The time period of a satellite in orbit around a planet (like Earth) is independent of the mass of the satellite. This can be understood from Kepler's Third Law and the gravitational formula for orbital motion.
The orbital time period TTT of a satellite is given by the formula:
T=2πr3GMT = 2\pi \sqrt{\frac{r^3}{GM}}T=2πGMr3
where:
- rrr is the radius of the orbit (distance from the center of the planet to the satellite),
- GGG is the gravitational constant,
- MMM is the mass of the central body (e.g., the Earth),
- TTT is the orbital period.
Notice that the mass of the satellite does not appear in this formula. The time period depends on the radius of the orbit and the mass of the planet around which the satellite orbits, but not the mass of the satellite itself.
Thus, regardless of whether the satellite is large or small, the time period for completing one orbit remains the same for a given orbital radius. This is why the time period of a satellite is independent of the satellite's mass.