... it would still constantly lose gases to space like every planet does but the half life of the atmosphere would be at least thousands of years...
Your air column would be much higher. Earth's thermosphere extends to 600 km. At 3,600 km the moon's gravity is significantly lower. Ions in the upper thermosphere would have a mean velocity over the orbital velocity. That should blow off quite rapidly.
Comets have a nucleus density less than that of water. This makes them hard to push around. (Earth's average density is about 10 times greater.)
90% of the Earth's atmosphere by mass is below 16 km and 99.99997% is below 100 km
Not to mention, only for the tiniest fraction of the atmosphere in the thermosphere or higher (>80 km on Earth) gravity matters at all, because molecules above that line follow mostly ballistic trajectories. Below that it's the thermal interaction between molecules that matters.
Quote from: pierre on 08/28/2017 11:21 pm90% of the Earth's atmosphere by mass is below 16 km and 99.99997% is below 100 km So ballpark one part in a million is flying away at any given time.
You can build vacuum safe domes with a small fraction of that mass.
If we solve potential health issues due to low gravity (or if they turn out not to be an issue at 1/6g), a billion people can comfortably live on the Moon. Might as well give them a great panorama.
That the Moon is able to hold an Earth-like atmosphere for at least thousands of years is a very commonly cited figure, see the old thread linked in the op and the Slate article. Admittedly I'd love to see a peer reviewed article on this.
In order to follow the water from the near field of the impact to the full planetary induced atmosphere, the 3D parallel DSMC code used a collision limiting scheme and an unsteady multi- domain approach. 3D results for the 45° oblique impact of a 2 km in diameter comet on the surface of the Moon at 30 km/s are presented. Most of the cometary water is lost due to escape just after impact and only 3% of the cometary water is initially retained on the Moon. Early downrange focusing of the water vapor plume is observed but the later material that is moving more slowly takes on a more symmetric shape with time. Several locations for the point of impact were investigated and final retention rates of 0.1% of the comet mass were observed.
Quote from: pierre on 08/30/2017 02:25 amThat the Moon is able to hold an Earth-like atmosphere for at least thousands of years is a very commonly cited figure, see the old thread linked in the op and the Slate article. Admittedly I'd love to see a peer reviewed article on this.I think this is the 'thousands of years' quoted sourceVondrak, R. R., "Creation of an Artificial Lunar Atmosphere," Nature 248, 657-659, 1974http://www.nature.com/nature/journal/v248/n5450/abs/248657a0.html?foxtrotcallback=trueHere are the referring workshttps://scholar.google.com/scholar?cites=16168342061603676328&as_sdt=2005&sciodt=0,5&hl=enMore recent take, 1992http://adsabs.harvard.edu/full/1992lbsa.conf..347B
EDIT: of course all analysis has been done on natural impacts, so these are rookie numbers, we gotta get those numbers up..Maybe with careful maneuvering or colliding objects on orbit or somehow slow boiling them on low or it it's could work a bit better.
The top of the mesosphere (i.e. the top of 99.99% of Earth's atmosphere) is as cold during the day as Antartica during the polar winter. At that temperature air molecules move at an average speed of 370 m/s. Even at room temperature they move at 464 m/s. The Moon's escape velocity is 4.5 times as high, even at hundreds of km from the surface.
The main way for a molecule to get to such anomalous speed is to acquire energy either via high-energy UV photons (which would be blocked by ozone at the very top of the atmosphere) or via the solar wind (which can be redirected with an artificial magnetosphere).
Said molecule would also need to be accelerated in the right direction and would need to avoid any further collision with other, slower, molecules. Even at the altitude of the ISS there's still enough air that molecules on average collide every km. Escaping this soup requires extraordinary luck. The thing would leak, just like the Earth leaks, but it would be slow.
I could not open the nature article without spending $$. The abstract says "hundreds of years". About the time scale of comet orbits.
One conclusion is that if the density of the lunar atmosphere is increased, a point can be reached where loss occurs so slowly that itis negligible over human time scales (that is, exponential decay lifetimes are greater than hundreds of years).
The problem with terraforming (and this applies to Mars) is that it's pretty much useless effort until it's close to finished. Indeed, it may make things more difficult for surface activity.Paraterraforming seems like a better option. You get maximum utility out of each section-area enclosed per unit of input.
Paraterraforming would be easier on the moon due to it's low gravity.But adding a thin atmosphere still might be desirable to allow spacecraft to aerocapture into orbit,help keep LLO clean though the mascons tend to deorbit things, and burn up smaller meteorites.
I've had a penchant for the scientific method lately. Yes, Halley's comet is only one of a handful of objects on a highly elliptical orbit in our solar system. However, there is very little proof that the Oort Cloud really exists. I am very proud to say that I reaally am one of those that deny the existence of the Oort Cloud. If the Oort Cloud really existed, then there would be some evidence by now using space telescopes.
Which brings the question. Given that the biggest problem with bringing comets to moon is the high energy of impacts and resulting minuscule retention rate of volatiles, is there some orbital momentum exchange dance that could be done to 'soften the blows' ?
Until then, a glass dome on the moon with some air at reasonable pressure sounds doable.