Question 8 2 pts using the stefan boltzman law, what is the energy emitted by the sun in watts per meter squared (wm 2), assuming the sun has a temperature of 6000 k?

73,483,200 W/m^2

Explanation:

BY the stefan Boltzman law the energy radiated by a body is propotional to fourth power of its absolute temperature. Sun is considered to be black body,hence ts emisivity is one.

E= σT^4

σ= Boltsman constant = 5.67×10^(-8)

putting values we get

= 73,483,200 W/m^2

energy emitted by the sun = 73,483,200 W/m^2

thats correct, but whats the question

explanation: