War-Junkie
Nov 19 2007, 10:18 PM
I was just wondering where does the air go when there is rapid decompression or an air leak in space? Does it disassemble on a molecular level? or does it just disseapear?
Fluffybunny
Nov 19 2007, 10:27 PM
It would just spread out very thin, dispersing...there would still be oxygen molecules for example but just further apart. Imagine putting a drop of red food coloring into a bathtub full of water, it would still be there, but be spread so thin that you couldnt tell it was there...
atom286
Nov 19 2007, 10:38 PM
QUOTE (Fluffybunny @ Nov 19 2007, 10:27 PM)

It would just spread out very thin, dispersing...there would still be oxygen molecules for example but just further apart. Imagine putting a drop of red food coloring into a bathtub full of water, it would still be there, but be spread so thin that you couldnt tell it was there...
This is a good question. If you know about quantum mechanics you could argue that when the gas cloud has dispersed enough it does in fact cease to exist.
This is because quanrum effects caused by the uncertainty principle would come into play and your atoms would just merge into thew quanrum foam many scientists believe exist down at the atomic scale in space.
War-Junkie
Nov 19 2007, 10:46 PM
alright thanks for the reply i understand now.
magnetar
Nov 20 2007, 01:41 AM
I would add this. If you refer to a typical space orbit, and if it is exposed to sunlight, it would probably ionize after absorbing UV energy from the Sun. Then, I suppose, it may further gain altitude. At the region of the inner Van Allen belt, or else the magnetosphere, the charged nuclei would be attracted. The electrons would find a region, as well.
At some point, they may traverse the field lines back to the atmosphere, or they may just drift the magnetic pathways around Earth. I suspect some small amount is lost to space after a coronal mass discharge from the Sun stretches the field lines back until they 'short circuit' (reconnect), which may loosen some particles. Those would then likely get swept up in the solar wind, and head for the region beyond Jupiter.
There is an area there, that acts as a secondary line of defence against interstellar cosmic ray particles. The primary defense is the heliophere, a charged magnetic bubble surrounding the solar system that tends to block charged particles from outside (supernovae type ions). Even so, there are solar "pick-up ions" that ricochet and gain energy and might head back from the wall of the heliosphere. Most of those cosmic ray type ions are trapped and deflected somewhere beyond Jupiter, by the solar wind and solar magnetic field lines.
That is my "shoot-from-the-hip" opinion.