PPT-Stefan-Boltzmann law governs the radiation of energy by a black body: M = {emissivity} PowerPoint Presentation

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

Upload by eve
Published on 2023-10-04

Presentation Embed Code

<iframe width="560" height="315" src="https://www.docslides.com/embed/1023044" frameborder="0" allowfullscreen></iframe>

Download Presentation

Download Presentation The PPT/PDF document "Stefan-Boltzmann law governs the radiat..." is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.