Find the mean number density of particles in the stellar atmosphere.

AI Thread Summary
To find the mean number density of particles in a star's atmosphere, the mean radiation pressure of 0.33 N m-2 and mean gas pressure of 8300 N m-2 are given. The radiation pressure equation leads to a calculated temperature of 6016K. The user expresses confusion about using the ideal gas law, pV=nRT, to find the number density, n/V. The discussion concludes with a clarification that the focus should be on determining the number density directly from the pressures provided. Understanding the relationship between pressure and density is crucial for solving the problem effectively.
Jon.G
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Homework Statement


The atmosphere of a star has a mean radiation pressure of 0.33 N m-2and a mean gas pressure of 8300 N m-2. Calculate:
a) the mean number density of particles in the stellar atmosphere, and
b) the radiation pressure in a stellar atmosphere with twice the effective temperature.

Homework Equations


Radiation pressure = \frac{4 \sigma T^{4}}{3c} where σ = 5.67*10-8


The Attempt at a Solution


a) From the radiation pressure equation, I get T=6016K
and I'm not sure where to go from here. I would have thought to have used pV=nRT, but then that bring volume into the equation. I know it's probably really simple and is just something I am forgetting, but I just can't figure it out :/


b) Multiply the given value (0.33) by 16, as it is T4
5.28Pa


Thanks
 
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Jon.G said:
I would have thought to have used pV=nRT, but then that bring volume into the equation.
You wish to find n/V, right?
 
:S
Yes I do.
... I don't even know what to say, how could I not see that?

Thanks
 
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