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Thermal stability of water and hydroxyl on the surface of the Moon from temperature-programmed desorption measurements of lunar analog materials

Author
HIBBITTS, C. A1 ; GRIEVES, G. A2 ; POSTON, M. J2 ; DYAR, M. D3 ; ALEXANDROV, A. B2 ; JOHNSON, M. A2 ; ORLANDO, T. M2
[1] Johns Hopkins University Applied Physics Laboratory, 11100 Johns Hopkins Rd., Laurel, MD 20723, United States
[2] School of Chemistry and Biochemistry, Georgia Institute of Technology, Atlanta, GA 30332, United States
[3] Mount Holyoke College, Dept. of Astronomy, South Hadley, MA 01075, United States
Source

Icarus (New York, N.Y. 1962). 2011, Vol 213, Num 1, pp 64-72, 9 p ; ref : 3/4 p

CODEN
ICRSA5
ISSN
0019-1035
Scientific domain
Astronomy earth cosmic environment; Geology
Publisher
Elsevier, Amsterdam
Publication country
Netherlands
Document type
Article
Language
English
Author keyword
Ices Moon, Surfaces
Keyword (fr)
Adsorption Chimisorption Continuum Désorption Energie activation Evolution thermique Glace Modèle Régolithe Stabilité thermique Surface lunaire Système solaire
Keyword (en)
Adsorption Chemisorption Continuum Desorption Activation energy Thermal evolution Ice Models Regolith Thermal stability Lunar surface Solar system
Keyword (es)
Continuo Evolución térmica Modelo
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy / 001E03B Solar system

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
24135022

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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