The effect of differential rotation on Jupiter's low-degree even gravity moments
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Kaspi_et_al-2017-Geophysical_R ...
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FInal Published Version
Author
Kaspi, Y.Guillot, T.
Galanti, E.
Miguel, Y.
Helled, R.
Hubbard, W. B.
Militzer, B.
Wahl, S. M.
Levin, S.
Connerney, J. E. P.
Bolton, S. J.
Affiliation
Univ Arizona, Lunar & Planetary LabIssue Date
2017-06-28
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AMER GEOPHYSICAL UNIONCitation
The effect of differential rotation on Jupiter's low-degree even gravity moments 2017, 44 (12):5960 Geophysical Research LettersJournal
Geophysical Research LettersRights
© 2017. American Geophysical Union. All Rights Reserved.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The close-by orbits of the ongoing Juno mission allow measuring with unprecedented accuracy Jupiter's low-degree even gravity moments J(2), J(4), J(6), and J(8). These can be used to better determine Jupiter's internal density profile and constrain its core mass. Yet the largest unknown on these gravity moments comes from the effect of differential rotation, which gives a degree of freedom unaccounted for by internal structure models. Here considering a wide range of possible internal flow structures and dynamical considerations, we provide upper bounds to the effect of dynamics (differential rotation) on the low-degree gravity moments. In light of the recent Juno gravity measurements and their small uncertainties, this allows differentiating between the various models suggested for Jupiter's internal structure.Note
6 month embargo; Published Online: 19 June 2017ISSN
00948276Version
Final published versionSponsors
Israeli Ministry of Science; Minerva foundation; Federal German Ministry of Education and Research; Helen Kimmel Center for Planetary Science at the Weizmann Institute of Science; CNES; BSF; NSF; Juno projectAdditional Links
http://doi.wiley.com/10.1002/2017GL073629ae974a485f413a2113503eed53cd6c53
10.1002/2017GL073629
