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Q. The time period T of the moon of planet mars (mass $M_m$) is related to its orbital radius R (G = Gravitational constant) as

KEAMKEAM 2011Gravitation

Solution:

Time period $T=\frac{2\pi r}{v_o}$
$T=\frac{2\pi R}{\sqrt{GM_m}}$ $\left(\therefore v_o=\sqrt{\frac{GM}{R}}\right)$
$T^2=\frac{4\pi^2R^3}{GM_m}$