Calculating Cooling Rate for a Black Body in a Vacuum with a Radiation Screen

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SUMMARY

The discussion focuses on calculating the cooling rate of a spherical black body placed within a spherical thin shell, both of which are black and situated in a vacuum. The cooling rate is determined using the Stefan-Boltzmann law, expressed as dQ/dt = e*σ*4π*r²(T⁴_sphere - T⁴_vacuum). The user seeks clarification on whether the radiation screen can be neglected in the calculations, given its thin nature. The primary heat transfer mechanism in this scenario is black body radiation, as conduction and convection are absent in a vacuum.

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  • Knowledge of heat transfer concepts, specifically in vacuum conditions
  • Basic proficiency in calculus for differential equations
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Homework Statement


A spherical black body with a radius r and a temperature T is placed in a spherical thin shell (radiation screen) with a radius R. The shell is also absolutely black on both sides. The space between the shell and the sphere and the space outer of the shell contain vacuum, i.e., no gas.
Find the cooling rate


Homework Equations



R = dQ / dT = h*A*dT


The Attempt at a Solution


The black body radiates heat with
h - some heat transfer constant
A - area of the radiating body

\frac{dQ}{dT}_{bb} = h_{vacuum} * 4 \Pi *r^{2} (T_{sphere} - T_{vacuum})

the same works for the radiation screen

\frac{dQ}{dT}_{rs} = h_{gas} * 4 \Pi *R^{2} (T_{vacuum} - T_{environment})

The point is that I'm not sure how to find the overall cooling rate of the system. Thanks.
 
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In a vacuum, there will be no conduction or convection heat transfer (your equations are for convection). The only heat transfer mode will be black body radiation which is proportional to T^4.
 
Upps, I mixed up radiation, conductivity...

So

dQ/dt = e*\sigma*4\Pi*r^{2}(T^{4}_{sphere}-T^{4}_{vacuum})

but what about the radiation screen? It is a thin shell. Can I neglect it?
 

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