PPT-Stefan-Boltzmann law governs the radiation of energy by a black body: M = {emissivity}
Author : eve | Published Date : 2023-10-04
4 Emissivity is a constant so the energy radiated increases as the 4th power of temperature The sun T6000K emits vastly more energy than the earth at T300K The
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Stefan-Boltzmann law governs the radiation of energy by a black body: M = {emissivity}: Transcript
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