Author
Listed:
- T. Guillot
(Université Côte d’Azur, OCA, Lagrange CNRS)
- Y. Miguel
(Université Côte d’Azur, OCA, Lagrange CNRS
Leiden Observatory, University of Leiden)
- B. Militzer
(University of California)
- W. B. Hubbard
(Lunar and Planetary Laboratory, University of Arizona)
- Y. Kaspi
(Weizmann Institute of Science)
- E. Galanti
(Weizmann Institute of Science)
- H. Cao
(California Institute of Technology
Harvard University)
- R. Helled
(University of Zurich)
- S. M. Wahl
(University of California)
- L. Iess
(Sapienza Università di Roma)
- W. M. Folkner
(Jet Propulsion Laboratory, California Institute of Technology)
- D. J. Stevenson
(California Institute of Technology)
- J. I. Lunine
(Cornell University)
- D. R. Reese
(LESIA, Observatoire de Paris, PSL Research University, CNRS, Sorbonne Universités, UPMC Université Paris 06, Université Paris Diderot, Sorbonne Paris Cité)
- A. Biekman
(Université Côte d’Azur, OCA, Lagrange CNRS)
- M. Parisi
(Jet Propulsion Laboratory, California Institute of Technology)
- D. Durante
(Sapienza Università di Roma)
- J. E. P. Connerney
(NASA/GSFC)
- S. M. Levin
(Jet Propulsion Laboratory, California Institute of Technology)
- S. J. Bolton
(Southwest Research Institute)
Abstract
The determination of Jupiter’s even gravitational moments by the Juno spacecraft reveals that more than three thousand kilometres below the cloud tops, differential rotation is suppressed and the gas giant’s interior rotates as a solid body.
Suggested Citation
T. Guillot & Y. Miguel & B. Militzer & W. B. Hubbard & Y. Kaspi & E. Galanti & H. Cao & R. Helled & S. M. Wahl & L. Iess & W. M. Folkner & D. J. Stevenson & J. I. Lunine & D. R. Reese & A. Biekman & M, 2018.
"A suppression of differential rotation in Jupiter’s deep interior,"
Nature, Nature, vol. 555(7695), pages 227-230, March.
Handle:
RePEc:nat:nature:v:555:y:2018:i:7695:d:10.1038_nature25775
DOI: 10.1038/nature25775
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