calculate the temperature in K at which a perfect black body radiates energy 5.67 W/cm² Given that 5.567*10^-8 W^-2 k^-4
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For an ideal black body emissive power is
E=
A
P
=σεT
4
where A is area of black body, σ is Stefan-Boltzmann's constant, ε is emissivity and T is temperature
σ=5.67×10
−8
Wm
−2
K
−4
for an ideal black body ε=1
then
A
P
=σεT
4
⟹5.67×10
4
=5.67×10
−8
×T
4
T
4
=10
12
T=10
3
K
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