Step 1: Using Stefan–Boltzmann law.
The rate of radiation from a body is given by:
\[
E = \varepsilon \sigma A T^4
\]
where $\varepsilon$ is emissivity, $\sigma$ is Stefan constant, $A$ is surface area and $T$ is absolute temperature.
Step 2: Radiation from sphere $S_1$.
For $S_1$,
\[
A_1 = 4\pi R^2,\quad T_1 = T
\]
\[
E_1 = \varepsilon \sigma (4\pi R^2)T^4 = E
\]
Step 3: Radiation from sphere $S_2$.
For $S_2$,
\[
A_2 = 4\pi (3R)^2 = 36\pi R^2,\quad T_2 = \frac{T}{\sqrt{3}}
\]
\[
E_2 = \varepsilon \sigma (36\pi R^2)\left(\frac{T}{\sqrt{3}}\right)^4
\]
\[
E_2 = \varepsilon \sigma (36\pi R^2)\frac{T^4}{9}
\]
Step 4: Comparing with $E_1$.
\[
E_2 = \frac{1}{9}\varepsilon \sigma (4\pi R^2)T^4 = \frac{E}{9}
\]
Step 5: Conclusion.
The rate of radiation of sphere $S_2$ is $\dfrac{E}{9}$.