Pressure and Volume of a Neutral Hydrogen Cloud

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SUMMARY

The discussion centers on calculating the pressure (P) and volume (V) of a neutral hydrogen cloud given its total mass (M), atomic weight of hydrogen (m), and temperature (T) of 50 K. The ideal gas equation PV = (M / m) * k * (50 K) is established, but the lack of a second equation complicates the determination of P and V. Participants highlight the necessity of additional information, such as the cloud's density, to solve for these variables effectively. The role of gravity and the variation of pressure and density with radial position are also emphasized as critical factors in understanding the cloud's behavior.

PREREQUISITES
  • Understanding of the Ideal Gas Law
  • Knowledge of atomic mass and its implications in calculations
  • Familiarity with differential equations and density gradients
  • Concept of gravitational effects on gaseous clouds
NEXT STEPS
  • Research the Ideal Gas Law and its applicability to astrophysical gases
  • Study differential equations related to density gradients in spherical systems
  • Explore gravitational effects on gaseous clouds and their implications for pressure and volume
  • Examine statistical definitions of volume in astrophysical contexts
USEFUL FOR

Astronomers, astrophysicists, and students studying gas dynamics in astrophysical contexts will benefit from this discussion, particularly those interested in the properties of neutral hydrogen clouds and their behavior under various physical conditions.

Parzeevahl
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Homework Statement
A diffuse cloud of neutral hydrogen atoms in space has a temperature of 50 K. Calculate the pressure (in Pa) and the volume (in cubic light-years) occupied by the cloud if its mass is 100 times the mass of the sun.
Relevant Equations
PV = NkT (k = Boltzmann constant)
Here's how I approached it. We know the total mass of the cloud, it is given. Let's call it 'M'. We can also find out the mass of a single hydrogen atom from its atomic weight. Let's call this 'm'. Then

N = M / m

is the total number of hydrogen atoms in the cloud. The temperature (T) is given - it is 50 K.

Then the gas equation becomes: PV = (M / m) * k * (50 K)

So, here are two unknown variables here that I have to find out - P and V. But I have only one equation (the gas equation above). How can I find out the other equation, since for two unknown variables we need two equations?
 
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I don't know how you can solve this without more information. Such as the density of the cloud. This may be given as a certain number of atoms per cubic centimeter. Did they tell you any information such as this?
I was doing some searching when reading this problem, because I did not know if these atoms obey the Ideal Gas Law.

I didn't really find a definite answer to that, but it seems that they may. I did find this following article interesting, though:

https://www.britannica.com/science/hydrogen-cloud
 
Yes, I also thought of the density and checked again, but the question didn't supply any such information.

Also, thanks for the article, I'll take a look :) !
 
I suppose gravity would be the force that keeps the volume finite? Then the temperature would have to be an average value, I guess?
 
DaveE said:
I suppose gravity would be the force that keeps the volume finite? Then the temperature would have to be an average value, I guess?
I agree that it makes sense to include gravity. But the temperature is given, so it doesn't need to be considered an average value. However, the pressure and density should vary with radial position.
 
Chestermiller said:
I agree that it makes sense to include gravity. But the temperature is given, so it doesn't need to be considered an average value. However, the pressure and density should vary with radial position.
I am not convinced that this is the intended interpretation. But...

Suppose that we arbitrarily fix the density at the center of the [spherically symmetric] cloud. Now we should be able to obtain a differential equation for the density gradient at radius r in terms of r and the cumulative mass at or beneath radius r.

We solve the differential equation. If the limit as ##r \to \infty## is finite, we re-scale the initial density to obtain the desired 100 solar mass total and hope that the resulting density still qualifies as "sparse".

Unfortunately, even if this approach succeeds, we will not have obtained a volume. We might, I suppose, consider the pressure at the center as the "pressure" part of the answer and the hypothetical volume that would be required for 100 solar masses at that uniform pressure as the "volume".
 
jbriggs444 said:
Unfortunately, even if this approach succeeds, we will not have obtained a volume.
Yes I find the volume issue problematic. I guess you have to pick a statistical definition, like "containing 99% of the atoms". For any volume chosen there could be an atom that has enough energy to leave that space.
 

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