Question #126517

The intensity distribution of solar radiation peaks at a wavelength of approximately 500 nm. Assuming the Sun radiates like a black body, calculate the flux of photons leaving the sun in W/m2.

Expert's answer

Re=σT4=5.67108(bλ)4=5.67108(0.002898500109)4=R_e=\sigma T^4=5.67\cdot 10^{-8}\cdot (\frac{b}{\lambda})^4=5.67\cdot 10^{-8}\cdot (\frac{0.002898}{500\cdot10^{-9}})^4=


64106\approx64\cdot10^6 W/m2W/m^2


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