Partial pressure and liquid water

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Discussion Overview

The discussion revolves around the conditions necessary for liquid water to exist on the surface of Mars, specifically focusing on the roles of temperature, atmospheric pressure, and the partial pressure of water vapor. Participants explore theoretical scenarios involving phase changes of ice under varying conditions.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Jack expresses confusion about whether liquid water can exist if temperature is above 273 K and atmospheric pressure is above 611 Pa, or if it is the partial pressure of water vapor that must exceed 611 Pa.
  • One participant asserts that the correct condition is that the partial pressure of water vapor must be above 611 Pa for liquid water to exist, explaining that condensed matter will sublimate or evaporate if the vapor pressure exceeds the partial pressure in the gas phase.
  • Jack presents a hypothetical scenario where ice on Mars at 270 K and 1000 Pa atmospheric pressure is questioned regarding whether it will turn to liquid or sublime to vapor, emphasizing the role of partial pressure.
  • Another participant confirms that the ice will sublimate into vapor, reiterating that the relevant pressure is that of the water vapor, not the total atmospheric pressure.
  • Jack proposes a further example involving a block of ice at 106 Pa atmospheric pressure and temperatures rising from 200 K to 350 K, questioning whether the ice would melt if the partial pressure of water vapor increases above 611 Pa as the temperature rises.
  • Jack also speculates that if the liquid water forms, it would be stable against freezing and boiling, but not necessarily against evaporation unless the air is fully saturated with water vapor.

Areas of Agreement / Disagreement

Participants express differing views on the conditions under which liquid water can exist, particularly regarding the importance of partial pressure versus total atmospheric pressure. The discussion remains unresolved as multiple competing views are presented.

Contextual Notes

The discussion includes assumptions about the behavior of water under Martian conditions, the definitions of pressure types, and the implications of saturation levels, which are not fully explored or agreed upon.

jf22901
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Hi everyone

I'm reading up on the possibility of liquid water existing on the surface of Mars, and have confused myself!

During my reading, I have come across various definitions that say liquid water can exist if the temperature is above 273 K and the atmospheric pressure is above 611 Pa, but others say it is the partial pressure of water vapour that needs to be above 611 Pa.

As an example, say there is an ice deposit on Mars in a region where the atmospheric pressure is 1000 Pa, and the temperature increases from 270 K to 280 K. What happens in this case? Does the ice turn to liquid or sublime to vapour? The temperature and atmospheric pressure are high enough for liquid water to exist, but how does the partial pressure of water vapour come into things in this situation?

I must be missing something blindingly obvious, but I can't see what it is!

Thanks,

Jack
 
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jf22901 said:
During my reading, I have come across various definitions that say liquid water can exist if the temperature is above 273 K and the atmospheric pressure is above 611 Pa, but others say it is the partial pressure of water vapour that needs to be above 611 Pa.

The second statement is correct. Condensed matter (solid or liquid) will sublimate or evaporate if the vapor pressure is higher than the partial pressure in the gas phase. The vapor pressure of water at 273 K is 611 Pa, so any liquid water would evaporate unless the partial pressure of water vapor in the gas phase were at least 611 Pa.

jf22901 said:
As an example, say there is an ice deposit on Mars in a region where the atmospheric pressure is 1000 Pa, and the temperature increases from 270 K to 280 K. What happens in this case? Does the ice turn to liquid or sublime to vapour? The temperature and atmospheric pressure are high enough for liquid water to exist, but how does the partial pressure of water vapour come into things in this situation?

The ice will sublimate into vapor. See the phase diagram http://www.colorado.edu/physics/phys4230/phys4230_sp03/images/phase.gif" , keeping in mind that the pressure is that of the water vapor, not the total pressure.

Also, if the original atmospheric pressure (at 270 K) did not include at least ~600 Pa of water vapor partial pressure, the ice would be sublimating already. Does this make sense?
 
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Mapes said:
The ice will sublimate into vapor. See the phase diagram http://www.colorado.edu/physics/phys4230/phys4230_sp03/images/phase.gif" , keeping in mind that the pressure is that of the water vapor, not the total pressure.

Also, if the original atmospheric pressure (at 270 K) did not include at least ~600 Pa of water vapor partial pressure, the ice would be sublimating already. Does this make sense?

Hi Mapes

Thanks for the reply. I think it makes sense now, but let me just try another example to make sure I have actually understood it! It's strange that I am comfortable with what what might be classed as 'difficult' physics topics (such as quantum mechanics, electromagnetism, calculus of variations etc.), but thermodynamics confuses the heck out of me! :blushing:

Right... let's say there is a block of ice on Mars, the pressure of the atmosphere is 106 Pa, and the temperature rises from 200 - 350 K (in no way realistic, but it'll do as an example, as it is easier to follow on the phase diagram!). Let's also assume the partial pressure due to water vapour in the atmosphere is less than 611 Pa. In this case, although the total atmospheric pressure falls above the triple point, because the partial pressure is below, the ice will sublime directly to vapour as the temperature increases.

But, as the vapour enters the atmosphere, the atmosphere (at least the thin layer close to the block of ice) will become more saturated with vapour, and in this small layer, the partial pressure of the water vapour may increase to above 611 Pa. In such a situation, with the temperature above 273 K (but below the boiling temperature), and the partial pressure due to vapour now above 611 Pa, would the ice begin to melt rather than sublime?

And if it did melt, the liquid would be stable against freezing and boiling, but not necessarily evaporation, unless the air was completely saturated with water vapour?

Thanks once again, :biggrin:

Jack
 
Last edited by a moderator:
Yes, this reasoning looks good.
 

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