Step 1: Pick a convenient starting temperature.
Since only the ratio matters, take a sample value \(T_1 = 300 \text{ K}\). Doubling the surface temperature gives \(T_2 = 600 \text{ K}\). By the Stefan-Boltzmann law, emissive power scales as \(E \propto T^4\).
Step 2: Compute both fourth powers directly.
\[
T_1^4 = 300^4 = 8.1 \times 10^{9}
\]
\[
T_2^4 = 600^4 = 1.296 \times 10^{11}
\]
Step 3: Take the ratio of emitted energy.
\[
\frac{E_2}{E_1} = \frac{T_2^4}{T_1^4} = \frac{1.296 \times 10^{11}}{8.1 \times 10^{9}} = 16
\]
\[
\boxed{E_2 = 16 \, E_1}
\]
Since any starting temperature would give the same ratio, the emitted radiation rises by a factor of 16 whenever the absolute temperature is doubled, matching option 3.