Let the acceleration due to gravity at a depth \( d \) be \( g_d \). The acceleration due to gravity at a height or depth from the surface of the Earth is given by the formula:
\[
g_d = g \left( \frac{R}{R + d} \right)^2
\]
where \( g \) is the acceleration due to gravity at the Earth's surface, and \( R \) is the radius of the Earth.
We are given that at a depth \( d \), the gravity becomes \( \frac{g}{n} \). So, we can equate the expression for gravity at depth to \( \frac{g}{n} \):
\[
\frac{g}{n} = g \left( \frac{R}{R + d} \right)^2
\]
Dividing both sides by \( g \), we get:
\[
\frac{1}{n} = \left( \frac{R}{R + d} \right)^2
\]
Taking the square root of both sides:
\[
\frac{1}{\sqrt{n}} = \frac{R}{R + d}
\]
Rearranging this to solve for \( d \):
\[
R + d = R \sqrt{n}
\]
\[
d = R \sqrt{n} - R
\]
\[
d = R \left( \sqrt{n} - 1 \right)
\]
Thus, the depth \( d \) is:
\[
d = \frac{R(n - 1)}{n}
\]
Thus, the correct answer is:
\[
\boxed{\frac{R(n - 1)}{n}}
\]