Blackbody radiation and stefans constant

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Homework Help Overview

The discussion revolves around the calculation of energy radiation per unit area of a blackbody at a specific temperature, specifically 260K, using Stefan-Boltzmann's law.

Discussion Character

  • Conceptual clarification, Assumption checking

Approaches and Questions Raised

  • Participants explore the application of Stefan-Boltzmann's law and question the interpretation of "per unit area" in the problem statement. Some express uncertainty about whether additional information is needed for the calculation.

Discussion Status

The discussion is active, with participants questioning the clarity of the problem and the implications of the term "per unit area." There is a mix of perspectives on the complexity of the problem, with some suggesting it may not be as tricky as it seems.

Contextual Notes

Participants are considering the definition of Stefan-Boltzmann's constant and its relevance to the problem, indicating a need for clarity on the fundamental concepts involved.

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What is the rate of energy radiation per unit area of a blackbody at a temperature of 260K ?

Where's the tricky part in this question?

Surely the answer to this question can't be just

stefans constant * T^4

ie. 5.67x10^-8 * 260^4 = 259.105 W/m^2
 
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Not every problem is tricky. The hard work was done to derive the constant. If you had been asked to that, it would be a whole different thing.
 
That's the question. Nothing else was asked.

What confuses me is how it says ...per unit area...in the question. So I'm thinking maybe they want some other number, I'm not sure
 
What's the definition of Stefan-Boltzmann's constant...?

Daniel.
 

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