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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. doi:10.1051/jphyscol:1984819.

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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 H₂, H-He, H₂-H₂O, H₂-CH₄, NH₃, and CH₄.5.75H₂O. Present and future theory and experiment are of great benefit t o planetary science.

Item Type:Article
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URLURL TypeDescription DOIArticle
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.
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Caltech Division of Geological and Planetary Sciences 4143
Issue or Number:11
Record Number:CaltechAUTHORS:20131120-113714678
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Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:42595
Deposited By: Ruth Sustaita
Deposited On:24 Nov 2013 00:45
Last Modified:10 Nov 2021 16:25

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