Estimating Atmospheric Masses Using the Barometric Equation

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Homework Help Overview

The discussion revolves around estimating the mass of carbon dioxide in the atmospheres of Venus, Earth, and Mars using the barometric equation. Participants are exploring the relationship between pressure, gravity, and atmospheric composition, while grappling with the implications of the variables involved.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning, Assumption checking

Approaches and Questions Raised

  • The original poster attempts to apply the exponential atmosphere equation but expresses uncertainty about the lack of a specific pressure value. Participants discuss the fundamental relationship between pressure, force, and area, and question how to integrate these concepts with the barometric equation. There is also consideration of whether to account for atmospheric height in their calculations.

Discussion Status

Participants are actively engaging with the problem, offering insights and clarifications regarding the relationships between the variables. Some guidance has been provided on how to approach the calculations, but multiple interpretations and methods are still being explored.

Contextual Notes

There is an emphasis on estimating values and the discussion includes considerations about the height of the atmosphere and the definition of atmospheric mass. Participants are also reflecting on the assumptions related to the calculation of gravitational effects and the extent of the atmosphere.

Brewer
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I've been given some homework questions (about the solar system, but I'm sure that it fits in this section of the board) and its all fine until I get to the part asking about atmospheres. I have a feeling that I know what I'm supposed to do, but I feel that I'm missing something blindingly obvious, as I can't actually find an answer.

The question asks me to estimate the mass of carbon dioxide on Venus, Earth and Mars, given ground level pressure, surface temp, surface gravity and the fractional CO2 content.

My initial thought it to use the exponential atmosphere equation:

P(h) = P(0)*exp-(mgh/kT), and solve for m, and multiplying this by the fractional CO2 content. But I don't think that this is the way to go somehow, as I don't have a a value of P(h). And now I'm stumped. Can anyone help me at all (because my notes sure can't!)

Thanks guys
 
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Think about how you go about calculating the pressure of a mercury column.
 
You mean along the lines of pressure = force/unit area?
 
Yes. And --- force equals what?
 
f = ma. so in this case is a = g?

If that's right, do I then equate that with the equation I put down earlier? If i do that I can't see how to solve for m, if there's an m in the exponential as well as the LHS.
 
assuming unit area of course?
 
Brewer said:
f = ma. so in this case is a = g?

Yes.

If that's right, do I then equate that with the equation I put down earlier?

No.

If i do that I can't see how to solve for m, if there's an m in the exponential as well as the LHS.

You've been given P, g, and CO2 content. "You mean along the lines of pressure = force/unit area?" What does the force equal?
 
P=mg, therefore m=P/g right?
 
Correct. Now what're the total areas?
 
  • #10
4*pi*R^2??

Does it matter the height of the atmosphere, so that it would be radius of planet and height above planet, or is it best to keep it all at the surface? It makes more sense to me to keep it at the surface, but doesn't the atmosphere not start until you get a certain distance up?
 
  • #11
You're asked to "estimate." g depends upon distance from COM, but, just for example, the Earth's atmosphere extends how far above the surface? That's the barometric equation you were playing with --- integrate to get however many "nines" of the total mass you'd like to play with. Height matters for low mass systems. Planets are in general not low mass. The "atmosphere" includes all gas phase mass associated with the planet. You can look at that any way you like: include all pore space in soils, cavern volumes; exclude gases dissolved in liquid or solid phases in the planetary structure. The question isn't asking for that kind of detail, so you are calculating the mass above the surface.
 

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