The equation is given by:
\[P = e \sigma A T^4\]
where:
- \(P\) is the power radiated,
- \(e\) is the emissivity of the surface,
- \(\sigma\) is the Stefan-Boltzmann constant (\(5.67 \times 10^{-8} \, \mathrm{W} \, \mathrm{m}^{-2} \, \mathrm{K}^{-4}\)),
- \(A\)
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