Atmospheric Density Required for Mercury´s Polar Regions to be Warm?

In summary, the atmospheric density required for Mercury's polar regions to be warm involves understanding the unique conditions of the planet's thin atmosphere and its extreme temperature variations. Research indicates that even a minimal increase in atmospheric density could significantly enhance the retention of heat, particularly in the permanently shadowed craters near the poles. These findings suggest that atmospheric composition and dynamics play a crucial role in influencing thermal conditions on Mercury, potentially allowing for warmer polar regions despite the planet's proximity to the Sun.
  • #1
snorkack
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TL;DR Summary
At which atmospheric density would Mercury´s poles be neither hot nor cold?
Venus has a dense atmosphere (about 90 bar).
Although Venus has a low axial inclination and the poles of Venus are therefore always in twilight, the day side atmosphere heats to about +460 C and the heat transport at the 90 bar atmosphere is so efficient that the poles are no more than 10 C cooler than day side.
Mercury has a thin atmosphere.
Day side of Mercury heats to about +430 C; but the poles are only around -170 C because of thin atmosphere and weak atmospheric heat transport.
At which atmospheric density would Mercury have just enough heat transport to provide for +20 C at poles?
 
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  • #2
Interesting point, that with the right atmosphere the poles might be livable, but we know the atmosphere must be thinner than Earth because Earth is about the place where you get good (but not complete) sharing of heat. So if it was like Earth, and way closer to the Sun, it would be too hot. So if it's going to be thinner than Earth, it probably wouldn't be all that livable after all, but at least it could be temperature.

Note also that if you use a weak atmosphere to share the heat around, it might not be enough to raise the temperature of the ground. Let's say an atmosphere like Mars could warm it up to +20 C, but that would be the air, the ground would still be radiating away so could be much colder. In other words, there is a density where the T of the air is right, but if that density is too low to get the ground to come to that T, then the ground T could still be much lower. You probably wouldn't care what the T of the thin air was if you are walking around on -100 C ground.

But your question also points out something else that's interesting-- since the T of the actual Mercury goes from -170 to +430, there is a latitude where it already is +20 C. Since Mercury's axis isn't tilted, that place is always at +20 C, except for the darn eccentricity of the orbit. If it were a circular tidally locked orbit, there would be a curve on the surface of Mercury that was always +20 C, all the time, with a nice big Sun close to the horizon all the time. If not for the lack of air, that might be an interesting spot to hang out. Or, given how long Mercury's day is, maybe it would be possible to keep moving on its surface such that you always stay somewhere that is +20 C. It's not something you think to do on that supposedly hot planet!
 
  • #3
Ken G said:
But your question also points out something else that's interesting-- since the T of the actual Mercury goes from -170 to +430, there is a latitude where it already is +20 C. Since Mercury's axis isn't tilted, that place is always at +20 C, except for the darn eccentricity of the orbit.
No, there isn´t. Because of the 88 day nights. In the equatorial regions, the surface hears to +430C in the afternoon - and manages to cool to -160 Celsius by morning.
At high latitudes where the Sun is low, daytime may only warm to +20, but night is still 88 days, so necessarily even colder than at equator.
 

FAQ: Atmospheric Density Required for Mercury´s Polar Regions to be Warm?

What is atmospheric density?

Atmospheric density refers to the mass of air molecules per unit volume in the atmosphere. It typically decreases with altitude and varies depending on temperature, pressure, and composition of the atmosphere.

Why is atmospheric density important for warming Mercury's polar regions?

Atmospheric density is crucial for warming Mercury's polar regions because a denser atmosphere can better retain heat through the greenhouse effect. This would mitigate the extreme temperature fluctuations and potentially raise the average temperature in the polar regions.

What is the current atmospheric density on Mercury?

Mercury has an extremely thin atmosphere, known as an exosphere, with a density so low that it is almost negligible. The exosphere is composed mainly of oxygen, sodium, hydrogen, helium, and potassium, but it is not sufficient to retain significant heat.

How much would the atmospheric density need to increase to warm Mercury's polar regions?

To warm Mercury's polar regions significantly, the atmospheric density would need to increase by several orders of magnitude, potentially reaching levels comparable to Earth's lower atmosphere. This would involve creating an atmosphere dense enough to support a stable greenhouse effect.

Is it feasible to increase Mercury's atmospheric density artificially?

Currently, increasing Mercury's atmospheric density artificially is not feasible with existing technology. It would require the transportation and release of vast amounts of gases, which poses significant technical and economic challenges. Additionally, maintaining such an atmosphere would be difficult due to Mercury's low gravity and proximity to the Sun.

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