Step 1: Using the relation between acceleration and radius.
The acceleration due to gravity is related to the radius and density of the planet by the formula:
\[
g = \frac{G M}{R^2}
\]
Where \( M \) is the mass of the planet, \( R \) is the radius, and \( G \) is the gravitational constant. The mass of a planet is related to its density \( \rho \) by \( M = \rho V \), where \( V = \frac{4}{3} \pi R^3 \).
Step 2: Comparing gravity on Earth and Moon.
The gravity on the moon is given by:
\[
\frac{g_m}{g_e} = \frac{1}{6}
\]
Thus, comparing the gravity on Earth and the moon, we get:
\[
\frac{R_m}{R_e} = \frac{5}{18}
\]
Thus, the radius of the moon is \( \frac{5}{18} R_e \), corresponding to option (C).