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High pressure physics and chemistry in giant planets and their satellites

Stevenson, D. J. (1984) High pressure physics and chemistry in giant planets and their satellites. Journal de Physique Colloques, 45 (11). pp. 97-103. ISSN 0449-1947. https://resolver.caltech.edu/CaltechAUTHORS:20131120-113714678

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Abstract

The deep interiors of Jupiter, Saturn, Uranus, Neptune, and their satellites are discussed. The important issues relevant to the physics of condensed matter are identified. The discussion emphasizes H_2, H-He, H_2- H_2O, H_2-CH_4, NH_3, and CH_4·5.75H_2O. Present and future theory and experiment are of great benefit to planetary science.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1051/jphyscol:1984819 DOIArticle
http://hal.archives-ouvertes.fr/jpa-00224317PublisherArticle
ORCID:
AuthorORCID
Stevenson, D. J.0000-0001-9432-7159
Additional Information:© 1984 Centre pour la communication scientifique directe. Contribution number 4143 of the Division of Geological and Planetary Sciences.
Other Numbering System:
Other Numbering System NameOther Numbering System ID
Caltech Division of Geological and Planetary Sciences 4143
Issue or Number:11
Record Number:CaltechAUTHORS:20131120-113714678
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20131120-113714678
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:42595
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:24 Nov 2013 00:45
Last Modified:03 Oct 2019 06:00

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