What is the Ideal Gas Law in Space?

In summary: It's not in my chem book either. I'm wondering how to figure out what R we're supposed to use for a problem like this.In summary, a nebula contains a tenuous gas that is heated by ultraviolet radiation from nearby stars. To determine the pressure in atmospheres, we use the gas constant R=0.0821 L*atm*K^-1*mol^-1 and the ideal gas law pV=nRT. After solving for n and plugging in the given values, we get a pressure of 1.02*10^-16 atm. It is important to use the correct units and gas constant when solving these types of problems.
  • #1
kikko
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Homework Statement



A nebula-a region of the galaxy where new stars are forming-contains a very tenuous gas with 100 atoms/cm^3. This gas is heated to 7500 K by ultraviolet radiation from nearby stars. Put the answer in atmospheres.

Homework Equations



pV=nRT
R=8.31
n=N/NA
NA = 6.02*10^23
N/V = number density


The Attempt at a Solution



100 = N/V
100V=N
100V=nNA
100V/NA = n
p=nRT/V
P= 100V/NART
P=(((100(1*10^-6))/(6.02*10^23))(8.31)(7500))/(1*10^-6)

P=1*10^-17 Pascals = 1*10^-22 atm


Not where where I went wrong.
 
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  • #2
Why are you dividing by 1*10^-6?

N/v = 100 atoms/cm^3 = 0.0001 atoms/m^3
n/v = (.0001 atoms/m^3)*(1/(6.022*10^23 atoms/mol))=1.66*10^-28 mol/m^3
p=(n/v)rt=(1.66*10^-28 mol/m^3)(8.314 J/mol*K)(7500 K)=1.04*10^-23 Pa = 1.03*10^-28 atm.
 
  • #3
Actually 1.03*10^-28 atm was the first answer I used in mastering physics and got it wrong.

I was going along the lines pV=nRT so p=(nRT)/V = ((100V/NA)RT)/V, and V=1*10^-6 m^3
 
  • #4
Oops. We're both using the wrong gas constant. The units don't work out.
 
  • #5
Isn't there just Boltzmann's Constant which equals the gas constant R divided by Avogrado's number, which we divided the gas constant by avogrado's number in the problem when multiply n and R.
 
  • #6
I'm losing it. :cry:

The answer wants atmospheres so just use a gas constant with atmospheres. R=0.0821 L*atm*K^-1*mol^-1.

n=1.66*10^-22 mol/cm^3 = 1.66*10^-19 mol/L.
p=(1.66*10^-19 mol/L)(0.0821 L*atm*K^-1*mol^-1)(7500 K)

Moles cancel, liters cancel, Kelvin cancel, and you get atmospheres.

p = 1.02*10^-16 atm.

I hate these types of problems. More on getting caught up in unit analysis than actually solving a problem.
 
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  • #7
That works out pretty straightforward with the R=0.0821 L*atm*K^-1*mol^-1. Thanks a ton. I'm wondering how we get that number for R. Is it just a given, like 8.31 we're supposed to just know when we do problems? My physics text doesn't mention any other values for R, and I can't remember the professor mentioning it either.
 

FAQ: What is the Ideal Gas Law in Space?

What is the Ideal Gas Law?

The Ideal Gas Law is a mathematical equation that describes the relationship between the pressure, volume, temperature, and number of gas particles in a closed system.

Does the Ideal Gas Law apply in space?

Yes, the Ideal Gas Law still applies in space as long as the gas is contained in a closed system and there is no significant gravitational pull or magnetic field present.

How is the Ideal Gas Law affected by low temperatures in space?

The Ideal Gas Law states that as temperature decreases, the volume of the gas also decreases, and the pressure increases. This is because the gas particles have less kinetic energy at lower temperatures, causing them to move slower and collide more frequently with each other and the walls of the container.

Can the Ideal Gas Law be used to predict the behavior of gases in space?

Yes, the Ideal Gas Law can be used to predict the behavior of gases in space as long as the conditions of the gas are known and the gas is in a closed system. However, it may not accurately predict the behavior of gases in extreme conditions, such as very low or high temperatures or pressures.

How does the Ideal Gas Law relate to the ideal gas state?

The Ideal Gas Law is based on the ideal gas state, which assumes that the gas particles have no volume and do not interact with each other. This state is an approximation and is only valid for gases at low pressures and high temperatures. In real gases, there are intermolecular forces and the volume of the gas particles is not negligible, so the Ideal Gas Law may not be completely accurate in predicting their behavior.

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