Gravitational force between the moon and the planet is "F = G \\frac{m M}{R^2}", where "m" is the mass of the moon, "M" is the mass of the planet, R is the distance between the two, G is the gravitational constant.
Since the motion of the moon is along the circular path, this force is equal to centripetal force "F = m \\frac{v^2}{R}". Equating last two equations, obtain "G \\frac{M m}{R^2} = m \\frac{v^2}{R}", from where "v^2 = \\frac{G M}{R}", and "R = \\frac{G M}{v^2} \\approx 1.3 \\cdot 10^8 m".
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