Stevenson, David J. (1992) Stalking the magma ocean. Nature, 355 . p. 301. ISSN 0028-0836. doi:10.1038/355301a0. https://resolver.caltech.edu/CaltechAUTHORS:20130702-095943237
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Abstract
Planets and smaller bodies are evidently differentiated, at least into a metallic core, silicate mantel and buoyant crust. Much of the differentiation occurred or began when the body was much hotter than now, back at the time of planetary formation around 4.5 thousand million years ago.
| Item Type: | Article | |||||||||
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| Additional Information: | © 1992 Nature Publishing Group. | |||||||||
| DOI: | 10.1038/355301a0 | |||||||||
| Record Number: | CaltechAUTHORS:20130702-095943237 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20130702-095943237 | |||||||||
| Official Citation: | Stevenson, D. J. (1992). "Stalking the magma ocean." Nature 355(6358): 301-301. | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 39182 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 02 Jul 2013 23:42 | |||||||||
| Last Modified: | 09 Nov 2021 23:43 |
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