Stevenson, David J. (1988) The role of high pressure experiment and theory in our understanding of gaseous and icy planets. In: Shock waves in condensed matter. Elsevier , Amsterdam, pp. 51-54. ISBN 9780444870971. https://resolver.caltech.edu/CaltechAUTHORS:20130628-141445107
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Abstract
High pressure experiments provide essential data for modeling planetary structure. Shock wave experiments are often especially suitable because they sample the same region of pressure-temperature space that is achieved naturally within the planet during its evolution. A very brief overview of planetary properties is given, followed by a summary of the issues of current interest: the behavior of hydrogen and hydrogen-rich mixtures; C, N, and O at high pressure, and rock-ice mixtures.
| Item Type: | Book Section | ||||
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| Additional Information: | © 1988 Elsevier Science Publishers B.V. | ||||
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| Record Number: | CaltechAUTHORS:20130628-141445107 | ||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20130628-141445107 | ||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||
| ID Code: | 39151 | ||||
| Collection: | CaltechAUTHORS | ||||
| Deposited By: | Tony Diaz | ||||
| Deposited On: | 09 Jul 2013 19:03 | ||||
| Last Modified: | 03 Oct 2019 05:04 |
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