Radiation energy Q emitted by an object in time t, object has surface area A, emissivity e and kelvin temperature T is:
Q=eσT4Atσ=5.87×10−8J/(s×m2×T4)Q=3.9×1026Wr=6.96×108mT=5800=5.8×103Kt=1s
The sun is an spherical shape object. The surface area of the sun is
A=4πr2=4π(6.96×108)2=6.087×1018m2e=σT4AtQ=5.87×10−8×(5.8×103)4×6.087×1018×13.9×1026=4.04×10263.9×1026=0.965≈1
e = 1 for black body
So, the sun radiates like a black body.
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