To determine the energy radiated by two spherical bodies, we utilize the Stefan-Boltzmann law, which states that the energy radiated per unit time is \(P = \sigma A T^4\), where \(\sigma\) is the Stefan-Boltzmann constant, \(A\) is the surface area, and \(T\) is the temperature. For a sphere, the surface area is given by \(A = 4\pi r^2\).
First, we calculate the energy radiated by the smaller body:
- Radius \(r_1 = 0.2\ m\)
- Temperature \(T_1 = 800\ K\)
- Surface area \(A_1 = 4\pi (0.2)^2 = 0.16\pi\ m^2\)
- Power \(P_1 = \sigma A_1 T_1^4 = \sigma \times 0.16\pi \times 800^4\). This power is denoted as \(E\).
Next, we calculate the energy radiated by the larger body:
- Radius \(r_2 = 0.8\ m\)
- Temperature \(T_2 = 400\ K\)
- Surface area \(A_2 = 4\pi (0.8)^2 = 2.56\pi\ m^2\)
- Power \(P_2 = \sigma A_2 T_2^4 = \sigma \times 2.56\pi \times 400^4\)
To find the relationship between \(P_1\) and \(P_2\), we compare the two powers: \(\frac{P_2}{P_1}=\frac{\sigma \times 2.56\pi \times 400^4}{\sigma \times 0.16\pi \times 800^4}=\frac{2.56}{0.16}\times \left(\frac{400}{800}\right)^4\)
This simplifies to:
- \(\frac{P_2}{P_1}=\frac{2.56}{0.16}\times \left(\frac{1}{2}\right)^4 = 16 \times \frac{1}{16} = 1\)
Therefore, \(P_2 = P_1\). This indicates that the energy radiated from the larger body is equal to \(E\).
The final answer is \(E\).