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The Interior of Saturn

Fortney, Jonathan J. and Helled, Ravit and Nettelmann, Nadine and Stevenson, David J. and Marley, Mark S. and Hubbard, William B. and Iess, Luciano (2016) The Interior of Saturn. . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190402-104303791

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Abstract

We review our current understanding of the interior structure and thermal evolution of Saturn, with a focus on recent results in the Cassini era. There has been important progress in understanding physical inputs, including equations of state of planetary materials and their mixtures, physical parameters like the gravity field and rotation rate, and constraints on Saturnian free oscillations. At the same time, new methods of calculation, including work on the gravity field of rotating fluid bodies, and the role of interior composition gradients, should help to better constrain the state of Saturn's interior, now and earlier in its history. However, a better appreciation of modeling uncertainties and degeneracies, along with a greater exploration of modeling phase space, still leave great uncertainties in our understanding of Saturn's interior. Further analysis of Cassini data sets, as well as precise gravity field measurements from the Cassini Grand Finale orbits, will further revolutionize our understanding of Saturn's interior over the next few years.


Item Type:Report or Paper (Discussion Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1609.06324arXivDiscussion Paper
ORCID:
AuthorORCID
Fortney, Jonathan J.0000-0002-9843-4354
Stevenson, David J.0000-0001-9432-7159
Marley, Mark S.0000-0002-5251-2943
Record Number:CaltechAUTHORS:20190402-104303791
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190402-104303791
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:94363
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:02 Apr 2019 18:19
Last Modified:02 Apr 2019 18:19

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