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Q. A satellite $A$ of mass $m$ is at a distance of r from the surface of the earth. Another satellite $B$ of mass $2m$ is at a distance of $2r$ from the earth's centre. Their time periods are in the ratio of

AIPMTAIPMT 1993Gravitation

Solution:

Time period does not depend on the mass.
As $T^{2} \propto r^{3}$.
$\frac{T_{A}}{T_{B}}=\frac{r^{3 / 2}}{2^{3 / 2} r^{3 / 2}}=1: 2 \sqrt{2}$