When a spherical object falls through a viscous medium, three forces act:
1. Gravitational force: \( mg = \frac{4}{3} \pi r^3 \rho g \), where \( \rho \) is the density of the object, \( r \) is radius, \( g \) is gravitational acceleration.
2. Buoyant force: \( \frac{4}{3} \pi r^3 \sigma g \), where \( \sigma \) is the density of the medium.
3. Viscous drag (Stokes’ law): \( F_d = 6 \pi \eta r v \), where \( \eta \) is the viscosity, \( v \) is velocity.
At terminal velocity \( v_t \), net force is zero:
\[
\frac{4}{3} \pi r^3 \rho g = \frac{4}{3} \pi r^3 \sigma g + 6 \pi \eta r v_t.
\]
Simplify:
\[
\frac{4}{3} \pi r^3 g (\rho - \sigma) = 6 \pi \eta r v_t.
\]
\[
v_t = \frac{2 r^2 g (\rho - \sigma)}{9 \eta}.
\]
Answer: \( v_t = \frac{2 r^2 g (\rho - \sigma)}{9 \eta} \).