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A black body is at a temperature $300 \mathrm{~K}$. It emits energy at a rate, which is proportional to
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$(300)^4$.
Temperature of a black body $(T)=300 \mathrm{~K}$. Stefan's law of radiation states that energy emitted by the black body $(E) \propto T^4 \propto(300)^4$.
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