Stevenson, D. J. (1980) The condensed matter physics of planetary interiors. In: Physique de la matière dense. Journal de physique - Colloque . No.C2. Société française de physique , pp. 53-59. ISBN 35350217. https://resolver.caltech.edu/CaltechAUTHORS:20130730-111127510
Full text is not posted in this repository.
Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20130730-111127510
Abstract
The deep interiors of Jupiter and Saturn consist of fluid, metallic hydrogen. In Jupiter the metallic hydrogen is uniformly mixed with helium. In Saturn, the incomplete solubility of helium may cause unmixing and energy release. In the interiors of Uranus and Neptune the fluid mixture (of hydrogen, helium, water, methane and ammonia) is metallic or ionic. The terrestral planetary cores are predominantly metallic iron.
| Item Type: | Book Section | ||||
|---|---|---|---|---|---|
| ORCID: |
| ||||
| Additional Information: | © 1980 Société française de physique. | ||||
| Series Name: | Journal de physique - Colloque | ||||
| Issue or Number: | C2 | ||||
| Record Number: | CaltechAUTHORS:20130730-111127510 | ||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20130730-111127510 | ||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||
| ID Code: | 39656 | ||||
| Collection: | CaltechAUTHORS | ||||
| Deposited By: | Tony Diaz | ||||
| Deposited On: | 20 Sep 2013 23:21 | ||||
| Last Modified: | 03 Oct 2019 05:09 |
Repository Staff Only: item control page
