Skip to main content
18 events
when toggle format what by license comment
Oct 24, 2015 at 3:01 review First posts
Oct 24, 2015 at 5:36
Oct 18, 2015 at 23:39 history tweeted twitter.com/StackChemistry/status/655890893359157248
Oct 17, 2015 at 9:08 history edited user21891 CC BY-SA 3.0
edited title; edited title
Oct 17, 2015 at 1:20 comment added Jason Patterson @chestermiller There are chunks of ice flying around the outer solar system that are fairly small (i.e. minimal gravitational attraction) that have been there for at least 4.5 billion years. At very low temperatures sublimation just about grinds to a halt in spite of the exceedingly low pressure.
Oct 16, 2015 at 20:44 history edited tschoppi CC BY-SA 3.0
fix grammar, add structure
Oct 16, 2015 at 17:01 answer added Newbie timeline score: 0
Oct 16, 2015 at 14:10 history edited user21891 CC BY-SA 3.0
added 619 characters in body
Oct 16, 2015 at 12:38 comment added tschoppi @user21891 Firstly, try to edit in this follow-up question into the question post itself. Secondly, please also show us your thoughts on the problem. This lets us know that we don't do your homework for you :)
Oct 16, 2015 at 10:36 comment added user21891 Nice answer @michael but can u explain why In lab vaccum conditions , why the water first boils and than condenses ? Whats the difference in a Adiabatic closed vaccum flask here on earth and interstellar space , Should'nt the results be all the same ??
Oct 16, 2015 at 10:33 vote accept user21891
Oct 16, 2015 at 9:30 answer added Gimelist timeline score: 6
Oct 15, 2015 at 15:11 comment added docscience *Interstellar *- significantly far away from any hot celestial bodies and the associated radiation - so ice! Any heat initially contained within the body of water you release will be radiated outward away from the water towards the background temperature of interstellar space - ~ 2 to 3 deg K.
Oct 15, 2015 at 14:48 comment added Chet Miller Any ice that forms will evaporate also.
Oct 15, 2015 at 12:18 comment added tschoppi From Wikipedia: "In cool, dense regions of the ISM [interstellar matter], matter is primarily in molecular form, and reaches number densities of 10⁶ molecules per cm³."
Oct 15, 2015 at 12:12 comment added Ivan Neretin Because such is the nature of things. Look at the phase diagram of water, to begin with. Now, the interstellar conditions imply extremely low pressure, far off the bottom edge of that plot. See, there is no liquid there, only vapours and ice.
Oct 15, 2015 at 11:44 comment added user21891 Why so @IvanNeretin ?
Oct 15, 2015 at 11:35 comment added Ivan Neretin Well, if you suddenly release some liquid water into the outer space, part of it will instantly evaporate and the rest will freeze.
Oct 15, 2015 at 11:24 history asked user21891 CC BY-SA 3.0