Step 1: Understand the change.
A black surface emits energy $E$ per second at $27^\circ$C. Its length and breadth each shrink to one third, and its temperature rises to $327^\circ$C. We find the new emission rate.
Step 2: Recall Stefan's law.
A black body radiates at a rate $E=\sigma A T^4$, so $E$ depends on the area $A$ and the fourth power of the absolute temperature $T$.
Step 3: Change the temperatures to kelvin.
Always use absolute temperature. \[ T_1=27+273=300\ \text{K},\qquad T_2=327+273=600\ \text{K}. \]
Step 4: Find the new area.
Area is length times breadth. Each shrinks to one third, so \[ A_2=\frac{L}{3}\times\frac{B}{3}=\frac{LB}{9}=\frac{A}{9}. \]
Step 5: Set up the ratio.
\[ \frac{E_2}{E_1}=\frac{A_2}{A_1}\left(\frac{T_2}{T_1}\right)^4. \]
Step 6: Put in the numbers.
\[ \frac{E_2}{E}=\frac{1}{9}\times\left(\frac{600}{300}\right)^4=\frac{1}{9}\times2^4=\frac{16}{9}. \]
Step 7: State the result.
\[ E_2=\frac{16E}{9}, \] which is option (4).
\[ \boxed{\dfrac{16E}{9}} \]