# Difference between revisions of "Dictionary:Stefan-Boltzmann’s law"

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(shte’ fan bōltz’ monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin. | (shte’ fan bōltz’ monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin. | ||

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## Revision as of 15:36, 18 October 2017

(shte’ fan bōltz’ monz) The amount of energy radiated by a blackbody per unit time per unit area is proportional to the fourth power of the temperature in kelvin.