To find the temperature \( T_2 \) of the second black body, we use the Stefan-Boltzmann Law, which states that the power \( P \) radiated by a black body is given by \( P = \sigma A T^4 \), where \( \sigma \) is the Stefan-Boltzmann constant, \( A \) is the surface area, and \( T \) is the absolute temperature.
Given two black bodies radiating the same power:
\[P_1 = \sigma \times 4\pi R_1^2 \times T_1^4\]
\[P_2 = \sigma \times 4\pi R_2^2 \times T_2^4\]
Since \( P_1 = P_2 \):
\[\sigma \times 4\pi R_1^2 \times T_1^4 = \sigma \times 4\pi R_2^2 \times T_2^4\]
Canceling out the common terms, we have:
\[R_1^2 \times T_1^4 = R_2^2 \times T_2^4\]
Substitute the given values \( R_1 = 2 \), \( T_1 = 400 \), \( R_2 = 4 \):
\[(2)^2 \times (400)^4 = (4)^2 \times T_2^4\]
\[4 \times 256 \times 10^6 = 16 \times T_2^4\]
Simplifying:
\[256 \times 10^6 = 4 \times T_2^4\]
\[64 \times 10^6 = T_2^4\]
Taking the fourth root:
\[T_2 = 300 \, \text{K}\]
Thus, the temperature of the second black body is \(\boxed{300 \, \text{K}}\).