We are given that two black bodies radiate the same amount of heat per second. The amount of heat radiated by a body is given by the Stefan-Boltzmann law:
\[
P = \sigma A T^4
\]
where:
- \( P \) is the power radiated (amount of heat radiated per second),
- \( \sigma \) is the Stefan-Boltzmann constant,
- \( A \) is the surface area of the body,
- \( T \) is the temperature of the body.
For a spherical body, the surface area is:
\[
A = 4 \pi R^2
\]
Now, let the power radiated by the first body be \( P_1 \) and the second body be \( P_2 \). According to the problem, \( P_1 = P_2 \), so we have:
\[
\sigma 4 \pi R_1^2 T_1^4 = \sigma 4 \pi R_2^2 T_2^4
\]
Canceling common terms:
\[
R_1^2 T_1^4 = R_2^2 T_2^4
\]
Now, take the ratio of both sides:
\[
\left( \frac{R_1}{R_2} \right)^2 = \left( \frac{T_2}{T_1} \right)^4
\]
Taking the square root of both sides:
\[
\frac{R_1}{R_2} = \frac{T_2}{T_1}^2
\]
Finally, solving for \( T_1 \):
\[
T_1 = \sqrt{2} T_2
\]
Thus, the relation between the temperatures and radii is \( T_1 = \sqrt{2} T_2 \).