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. 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 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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| Additional Information: | © 1984 Centre pour la communication scientifique directe. Contribution number 4143 of the Division of Geological and Planetary Sciences. | ||||||
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| Issue or Number: | 11 | ||||||
| DOI: | 10.1051/jphyscol:1984819 | ||||||
| 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: | 10 Nov 2021 16:25 |
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