Step 1:
The power of the radiation is given by the Stefan-Boltzmann equation, which is written as:
\[P = \sigma \cdot A \cdot e \cdot (T^4 - T_0^4)\]
where:
- \(P\) is the power,
- \(\sigma\) is the Stefan-Boltzmann constant,
- \(A\) is the surface area,
- \(e\) is
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