A question on heat transfer and blackbodys

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The discussion centers on the relationship between the Stefan-Boltzmann law, represented by the equation \(\frac{dQ}{dt} = \sigma A T^{4}\), and the specific heat equation \(Q = mc\Delta T\). The user inquires whether taking the time derivative of the second equation and equating it to the power emitted by a blackbody can yield a temperature function for a blackbody radiator cooling in a vacuum. The consensus is that these equations pertain to different heat transfer mechanisms, with the first addressing radiation and the second focusing on convective heat transfer, indicating that they cannot be directly equated.

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pastro
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Hello,

I was wondering:
\frac{dQ}{dt} = \sigma A T^{4}
for a perfect blackbody.

Also
Q = mc\DeltaT

If I take the time derivative of the above equation, set it equal to the power emitted by a blackbody, and solve the resulting differential equation for temperature, does that give me the temperature with which a blackbody radiator of a given mass and material cools in vacuum as a function of time?

Just curious...

Thanks!
 
Last edited:
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Ummm, I doubt it.

Equation 1 is for, well, radiation.

Equation 2, as I understand it, is for convective heat transfer.

The two are not really the same thing.
 

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