Given that the terminal velocity \( V \) of a sphere falling in a viscous fluid is given by Stokes' law:
\[
V = \frac{2}{9} \frac{R^2 (\rho_s - \rho_f) g}{\eta}
\]
Where:
- \( V \) is the terminal velocity,
- \( R \) is the radius of the sphere,
- \( \rho_s \) and \( \rho_f \) are the densities of the sphere and the fluid respectively,
- \( g \) is the acceleration due to gravity,
- \( \eta \) is the coefficient of viscosity of the fluid.
### Step 1: Set up the equation for both spheres.
For sphere 1:
\[
V = \frac{2}{9} \frac{R_1^2 (2\rho - \rho)}{\eta}
\]
For sphere 2, with terminal velocity \( 8V \):
\[
8V = \frac{2}{9} \frac{R_2^2 (3\rho - \rho)}{\eta}
\]
### Step 2: Relate the two equations.
Dividing the second equation by the first equation:
\[
\frac{8V}{V} = \frac{R_2^2 (3\rho - \rho)}{R_1^2 (2\rho - \rho)}
\]
This simplifies to:
\[
8 = \frac{R_2^2 (2\rho)}{R_1^2 ( \rho)}
\]
\[
8 = \frac{R_2^2}{R_1^2} \cdot 2
\]
Thus,
\[
\frac{R_2^2}{R_1^2} = 4
\]
Taking the square root of both sides:
\[
\frac{R_2}{R_1} = 2
\]
Therefore,
\[
R_1 = \frac{R_2}{8}
\]
Thus, \( R_1 \) is \( \frac{1}{8} \) of \( R_2 \).