Explanations & Calculations
- The equations involved here is R=ϵσAT4, in which R is the power of energy emission, ϵ=1 for a perfect black body and σ=5.67×10−8Wm−2K−4 .
- Then,
W=5.67×10−8×410m2×(155+273)4=7.8×105W
- To find any energy emitted, one needs to know the time for the emission did last.
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