If an hot object is radiating energy to its cooler surroundings the net radiation heat loss rate can be expressed as:
q = ε σ (Th4 - Tc4) Ah
where
Th = hot body absolute temperature (K)
Tc = cold surroundings absolute temperature (K)
Ah = area of the hot object (m2)
ε = emissivity coefficient of the object (one - 1 - for a black body)
σ = 5.6703 10-8 (W/m2K4) - The Stefan-Boltzmann Constant
Radiation heat transfer q = 37827 W
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