Power radiated by a black body is given by the Stefan–Boltzmann law:
\[
P = \sigma A T^4 = \sigma (4\pi r^2) T^4
\]
Initial power:
\[
P_1 = \sigma (4\pi r^2) T^4
\]
New radius \(= 2r\), new temperature \(= \frac{T}{2}\)
New power:
\[
P_2 = \sigma (4\pi (2r)^2) \left(\frac{T}{2}\right)^4
= \sigma (4\pi \cdot 4r^2) \cdot \frac{T^4}{16}
= \sigma (4\pi r^2) T^4 \cdot \frac{4}{16} = \frac{1}{4} P_1
\]
\[
P_2 = \frac{1}{4} \times 400 = 100 \, \text{W}
\]