Concept:
At terminal velocity, the loss of gravitational potential energy per second is completely converted into heat due to viscous drag.
Hence,
\[
\frac{dQ}{dt}
=
F_{\text{viscous}}\,v_t.
\]
According to Stokes' law,
\[
F_{\text{viscous}}
=
6\pi\eta r v_t.
\]
Step 1: Write the expression for terminal velocity.
For a sphere moving in a viscous liquid,
\[
v_t
=
\frac{2r^2(\rho-\sigma)g}{9\eta}.
\]
Therefore,
\[
v_t\propto r^2.
\]
Step 2: Express the viscous force in terms of \(r\).
Since
\[
F_{\text{viscous}}
=
6\pi\eta r v_t,
\]
and
\[
v_t\propto r^2,
\]
we get
\[
F_{\text{viscous}}
\propto r^3.
\]
Step 3: Calculate the rate of heat production.
\[
\frac{dQ}{dt}
=
F_{\text{viscous}}\,v_t.
\]
Substituting the proportionalities,
\[
\frac{dQ}{dt}
\propto r^3\times r^2.
\]
\[
\frac{dQ}{dt}
\propto r^5.
\]
Step 4: Write the final answer.
\[
\boxed{\frac{dQ}{dt}\propto r^5}
\]
\[
\boxed{\text{Answer = (B)}}
\]