(a) The change in potential energy in gravitational field is given by $\mathrm{\Delta}E = GMm\left( \frac{1}{r_{1}} - \frac{1}{r_{2}} \right)$
In this problem; $r_{1} = R$ and $r_{2} = nR$
$\mathrm{\Delta}E = GMm\left( \frac{1}{R} - \frac{1}{nR} \right)$
$= \frac{GMm}{R}\left( \frac{n - 1}{n} \right)$
$= mgR\left( \frac{n - 1}{n} \right)\ \ \left( \because g = \frac{Gm}{R^{2}}\ \right)$