Step 1: Understanding the Concept:
For a black body, the power radiated is \(P = \sigma A T^4\), with \(A = 4\pi R^2\) for a sphere.
Step 2: Key Formula or Approach:
Equal powers: \(4\pi R_1^2\sigma T_1^4 = 4\pi R_2^2\sigma T_2^4\).
Step 3: Detailed Explanation:
\(R_1^2 T_1^4 = R_2^2 T_2^4\).
\(\frac{R_1^2}{R_2^2} = \frac{T_2^4}{T_1^4}\).
\[ \frac{R_1}{R_2} = \left(\frac{T_2}{T_1}\right)^2 \]
The hotter body must be smaller to radiate the same power. Options A and B have the temperatures in the wrong order, and option D has the wrong power.
Final Answer:
\(\frac{R_1}{R_2} = \left(\frac{T_2}{T_1}\right)^2\), option (C).
\[ \boxed{\left(\frac{T_2}{T_1}\right)^2} \]