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Saturn's Luminosity and Magnetism

Stevenson, D. J. (1980) Saturn's Luminosity and Magnetism. Science, 208 (4445). pp. 746-748. ISSN 0036-8075. https://resolver.caltech.edu/CaltechAUTHORS:20131114-143222111

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Abstract

The Pioneer 11 results for Saturn's large heat output, small magnetic field, and near-axisymmetry of the field may all be explained by an interior model in which the helium is undergoing phase separation and is nonuniformly distributed. Substantial depletion of helium from the atmosphere is predicted.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://www.jstor.org/stable/1683874JSTORArticle
http://dx.doi.org/10.1126/science.208.4445.746DOIArticle
http://www.sciencemag.org/content/208/4445/746PublisherArticle
ORCID:
AuthorORCID
Stevenson, D. J.0000-0001-9432-7159
Additional Information:© 1980 American Association for the Advancement of Science. Published May 16, 1980.
Issue or Number:4445
Record Number:CaltechAUTHORS:20131114-143222111
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20131114-143222111
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:42467
Collection:CaltechAUTHORS
Deposited By: John Wade
Deposited On:14 Nov 2013 23:31
Last Modified:03 Oct 2019 05:58

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