Steffan-Boltzmann's Equation: Epsilon Sigma T^4

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The discussion centers on the Stefan-Boltzmann equation, represented as R=εσT^4, where ε is emissivity, σ is Stefan's constant, and T is temperature in Kelvin. Participants confirm that this equation is indeed the Stefan-Boltzmann law and suggest starting from it for clarity. There is a mention of checking derivations on Wikipedia for accuracy. The conversation reflects a common experience of feeling overwhelmed when the answer seems obvious. Overall, the exchange highlights the importance of understanding foundational equations in thermodynamics.
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R=\epsilon\sigmaT^{4}

\epsilon --> emmisivity
\sigma --> Steffan's constant
T[ --> Temp (in Kelvin)

should i start with steffan-boltzmann's equation (since its the nearest formula)?

thanks... ^_^
 
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Actually, I think that already is the Stefan-Boltzmann law; if you start from it you're done.

There is a derivation here, though generally I always check derivations on Wikipedia before I trust them :smile:
 
oh... I am sorry. i feel noobish! haha!
 
Sucks when the answer was staring you right in the face huh?
Don't worry, happens to me all the time :smile:
 
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