Thermo: Newtons law of cooling for radiation

AI Thread Summary
The discussion focuses on a problem involving a 4 kg copper cube cooling radiatively in a 100 °C environment. The net rate of heat transfer calculated using the Stefan-Boltzmann law is approximately 0.215 W, which is confirmed as correct by a participant. The user seeks clarification on the appropriate formula for Newton's law of cooling, indicating difficulty in finding it. The conversation emphasizes the importance of understanding radiative heat transfer and its calculations. Overall, the thread highlights the application of thermodynamic principles in practical scenarios.
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Homework Statement



A cube of copper of mass 4 kg and initial temperature of 110 oC is set to radiatively cool in an environment of 100 oC.
(Note: copper has an emissivity of about 0.05. Also, neglect conduction and convection as cooling agents in this problem.)

The surface area of the cube is .035 m^2



The Attempt at a Solution



Before the copper has had a chance to cool, find the net rate of heat transfer of the cube to the environment.

Using Pnet=Aes(to^4-ts^4), s=stefan boltzman constant, to= temp of object, ts= temp of surroundings, e=emissivity, a= surface area

(.035)(.05)(5.67*10^-8)(383.15^4-373.15^4)=.215 W

Is this correct?

The next part of the question asks for Newton's cooling approximation, which approximation is this I wasn't able to find a formula for it...


Thanks, and as always help is much appreciated!
 
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Numerical answer is correct.
 
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