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Stefan-Boltzmann Constan |
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Stefan-Boltzmann Constan
(σ), a physical constant appearing in the Stefan-Boltzmann law, which states that the energy radiated by a blackbody is proportional to the fourth power of the body’s absolute temperature: σ = (5.67032 ± 0.00071) × 10–8 watt/(m2.°K4) = (5.67032 ± 0.00071) × 10–5 erg/(sec-cm2.°K4). Want to thank TFD for its existence? Tell a friend about us, add a link to this page, add the site to iGoogle, or visit the webmaster's page for free fun content. |
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