Thank you for reporting, we will resolve it shortly
Q.
Two satellites of masses $M$ and $9M$ are orbiting a planet in a circular orbit of radius $r$ . Their frequency of revolution will be in the ratio of
NTA AbhyasNTA Abhyas 2020Gravitation
Solution:
Using Kepler's IIIrd law of planetary motion,
$T=2\pi \sqrt{\frac{r^{3}}{GM}}$ or $T^{2} \propto r^{3}$
Frequency, $f=\frac{1}{T}=\frac{1}{2 \pi }\sqrt{\frac{GM}{r^{3}}}$
Frequency is independent of the mass of the satellite.
Hence, required ratio $= 1 : 1$