Comparing Jupiter interior structure models to <i>Juno</i> gravity measurements and the role of a dilute core
S. M. Wahl(Planetary Science Institute), S. J. Bolton(Southwest Research Institute), Burkhard Militzer(Planetary Science Institute), D. R. Reese(Centre National de la Recherche Scientifique), S. Levin, Yohai Kaspi(Weizmann Institute of Science), T. Guillot(Centre National de la Recherche Scientifique), Eli Galanti(Weizmann Institute of Science), Yamila Miguel(Centre National de la Recherche Scientifique), J. E. P. Connerney(Goddard Space Flight Center), N. Movshovitz(Tel Aviv University), W. B. Hubbard(University of Arizona), Ravit Helled(Tel Aviv University)
Cited by 391
Related Papers
Cassini finds molecular hydrogen in the Enceladus plume: Evidence for hydrothermal processes
|Science|2017|556
Cassini Plasma Spectrometer Investigation
|Space Science Reviews|2004|514
Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
|Scientific Electronic Library Online (São Paulo Research Foundation, Latin American and Caribbean Center on Health Sciences Information, Conselho Nacional de Desenvolvimento Científico e Tecnológico)|2009|381
A New Model of Jupiter's Magnetic Field From Juno's First Nine Orbits
|Geophysical Research Letters|2018|365
The Juno Magnetic Field Investigation
|Space Science Reviews|2017|338