What is Stefan Boltzmann law?

1 Answer
May 9, 2018

The Stefan-Boltzmann law is #L=AsigmaT^4#, where:

  • #A# = surface area (#m^2#)
  • #sigma# = Stefan-Boltzmann (#~5.67*10^-8Wm^-2K^-4#)
  • #T# = surface temperature (#K#)

This law is used to find the luminosity (the rate of energy released), for an object given its surface temperature. This law assumes the body acts as a black-body radiator (an object that emits energy from the entire EM spectrum)

For a given object with a constant surface area, the Stefan-Boltzmann law says that luminosity is proportional to the temperature raised to the fourth power.