Calculate the blackbody temp of the sun from the following data .Stefan's constant=5.7×10^-8 wm^-2 k^-4.?
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calculation for the temperature on the surface of the Sun is as follows:
σ=5.67∗10−8Wm2K4 (Stefan-Boltzmann constant)
S=1367Wm2 (solar constant)
D=1.496∗10^11m (Earth-Sun average distance)
R=6.963∗10^8m (radius of the Sun)
T=(PσA)^1/4=(S4πD²÷σ4πR²)∧1/4=(SD²÷σR²)∧1/4=5775.8 K
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