Linked Life Data

11539120

Source:http://linkedlifedata.com/resource/pubmed/id/11539120

Statements in which the resource exists as a subject.
PredicateObject
rdf:type
lifeskim:mentions
pubmed:issue
2
pubmed:dateCreated
1997-1-29
pubmed:abstractText
In an extension of previously reported work on ices containing CO, CO2, H2O, CH3OH, NH3, and H2, measurements of the physical and infrared spectral properties of ices containing molecules relevant to Jupiter's moon Io are presented. These include studies on ice systems containing SO2, H2S, and CO2. The condensation and sublimation behaviors of each ice system and surface binding energies of their components are discussed. The surface binding energies can be used to calculate the residence times of the molecules on a surface as a function of temperature and thus represent important parameters for any calculation that attempts to model the transport of these molecules on Io's surface. The derived values indicate that SO2 frosts on Io are likely to anneal rapidly, resulting in less fluffy, "glassy" ices and that H2S can be trapped in the SO2 ices of Io during night-time hours provided that SO2 deposition rates are on the order of 5 micrometers/hr or larger.
pubmed:keyword
pubmed:language
eng
pubmed:journal
pubmed:citationSubset
S
pubmed:chemical
pubmed:status
MEDLINE
pubmed:month
Dec
pubmed:issn
0019-1035
pubmed:author
pubmed:issnType
Print
pubmed:volume
106
pubmed:owner
NASA
pubmed:authorsComplete
Y
pubmed:pagination
478-88
pubmed:dateRevised
2008-11-21
pubmed:meshHeading
pubmed:year
1993
pubmed:articleTitle
The condensation and vaporization behavior of ices containing SO2, H2S, and CO2: implications for Io.
pubmed:affiliation
NASA/Ames Research Center, Moffett Field, California 94035, USA.
pubmed:publicationType
Journal Article, Research Support, U.S. Gov't, Non-P.H.S.