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Introduction to Planetary Interiors

Stevenson, D. J. (2002) Introduction to Planetary Interiors. In: High Pressure Phenomena. IOS Press , Amsterdam, pp. 587-606. ISBN 9781586032692. https://resolver.caltech.edu/CaltechAUTHORS:20130814-102433603

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Abstract

In the context of this volume, planetary interiors provide a testing ground for fundamental physics (theory and laboratory) under "extreme" conditions. For example, much of the interest in metallic hydrogen stems from its inferred presence in Jupiter (and the implication that it is the most common metal in the Universe). The melting properties of iron at megabar pressures are likewise "tested" in the deepest Earth through their relevance to the presence of a solid inner core. There are also a small number of people who study planetary interiors for reasons that are not primarily motivated by the desire w understand materials under extreme conditions. They do so for three reasons: 1) An explanatory basis for many phenomena that arise within a planet (but have external manifestation). You cannot understand why certain planets have volcanoes, why some planets have magnetic fields (and others do not), and why Jupiter emits as much heat as it does without an understanding of the insides of these bodies. 2) An essential part of the understanding of phenomena and processes that are not intrinsically internal to the planet. For example, you cannot claim any understanding of the history of Mars' atmosphere if you are ignorant of likely outgassing rates or of how the sputtering of the atmosphere is affected by a magnetic field that varies through geologic time. 3) The search for a unifying story. If you want to build a story of how the planet formed and evolved to the present state, this will depend mainly on understanding the interior.


Item Type:Book Section
ORCID:
AuthorORCID
Stevenson, D. J.0000-0001-9432-7159
Additional Information:© 2002 Società Italiana di Fisica.
Record Number:CaltechAUTHORS:20130814-102433603
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130814-102433603
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:39910
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:19 Aug 2013 23:38
Last Modified:03 Oct 2019 05:11

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