Physics
Scientific paper
Oct 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002icar..159..518l&link_type=abstract
Icarus, Volume 159, Issue 2, p. 518-528.
Physics
21
Scientific paper
We performed high-pressure experiments on the crystallization of water ice I and III in the ammonia-water (NH3)x(H2O)(1-x) system, and apply the results to the interiors of icy bodies in the Solar System. Phase equilibrium lines between an entirely liquid solution and a liquid solution in which water ice forms (liquidus lines) were determined for ammonia concentration by mass X equal to 0.034, 0.0472, 0.111, 0.176, and 0.229. Growth-melting of ice I as well as ice III crystals were observed. Application of the results to icy satellites that are potential bearers of ammonia shows that ammonia admixture decreases the depth of the liquidus surface. A shift of the liquidus temperature within a satellite depends on three parameters: the ammonia concentration, X; the temperature gradient, α and the product of density and gravity, ρg.
Leliwa-Kopystyński Jacek
Maruyama Minoru
Nakajima Toshio
No associations
LandOfFree
The Water-Ammonia Phase Diagram up to 300 MPa: Application to Icy Satellites does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The Water-Ammonia Phase Diagram up to 300 MPa: Application to Icy Satellites, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Water-Ammonia Phase Diagram up to 300 MPa: Application to Icy Satellites will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1425181