Jupiter’s inhomogeneous envelope
Astronomy and Astrophysics, vol. 662, pp. A18
Abstract
Context.While Jupiter’s massive gas envelope consists mainly of hydrogen and helium, the key to understanding Jupiter’s formation and evolution lies in the distribution of the remaining (heavy) elements. Before the Juno mission, the lack of high-precision gravity harmonics precluded the use of statistical analyses in a robust determination of the heavy-element distribution in Jupiter’s envelope. Aims.In this paper, we assemble the most comprehensive and diverse collection of Jupiter interior models to date and use it to study the distribution of heavy elements in the planet’s envelope. Methods.We apply a Bayesian statistical approach to our interior model calculations, reproducing the Juno gravitational and atmospheric measurements and constraints from the deep zonal flows. Results.Our results show that the gravity constraints lead to a deep entropy of Jupiter corresponding to a 1 bar temperature that is 515 K higher than traditionally assumed. We also find that uncertainties in the equation of state are crucial when determining the amount of heavy elements in Jupiter’s interior. Our models put an upper limit to the inner compact core of Jupiter of 7MEarth, independently of the structure model (with or without a dilute core) and the equation of state considered. Furthermore, we robustly demonstrate that Jupiter’s envelope is inhomogeneous, with a heavy-element enrichment in the interior relative to the outer envelope. This implies that heavy-element enrichment continued through the gas accretion phase, with important implications for the formation of giant planets in our Solar System and beyond.
Authors 16
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Leiden University · Leiden Observatory · Space Research Organisation Netherlands
Affiliation as printed
Leiden Observatory, University of Leiden, Niels Bohrweg 2, 2333 CA Leiden, The Netherlands
SRON Netherlands Institute for Space Research, Niels Bohrweg 4, 2333 CA Leiden, The Netherlands
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New York University Abu Dhabi · Heidelberg Institute for Theoretical Studies
Affiliation as printed
CITIES, NYUAD Institute, New York University Abu Dhabi, PO Box 129188, Abu Dhabi, UAE
Heidelberg Institute for Theoretical Studies (HITS gGmbH), Schloss-Wolfsbrunnenweg 35, 69118 Heidelberg, Germany
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Centre National de la Recherche Scientifique · Université Côte d'Azur · Observatoire de la Côte d’Azur
Affiliation as printed
Université Côte d'Azur, OCA, Lagrange CNRS, 06304 Nice, France
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Centre National de la Recherche Scientifique · Université Côte d'Azur · Observatoire de la Côte d’Azur
Affiliation as printed
Université Côte d'Azur, OCA, Lagrange CNRS, 06304 Nice, France
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Affiliation as printed
Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel
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Department of Earth and Planetary Sciences, Weizmann Institute of Science, Rehovot 76100, Israel
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Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA
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University of California, Berkeley
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Department of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA
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Institute for Computational Science, University of Zurich, Winterthurerstr. 190, 8057 Zurich, Switzerland
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University of Michigan, Climate and Space Sciences and Engineering, Ann Arbor, MI 48109, USA
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NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
Space Research Corporation, Annapolis, MD 21403, USA
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Department of Mechanical and Aerospace Engineering, Sapienza University of Rome, Italy
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Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA
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Carl Sagan Institute, Cornell University, 122 Sciences Drive, Ithaca, NY 14853, USA
Department of Astronomy, Cornell University, 122 Sciences Drive, Ithaca, NY 14853, USA
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California Institute of Technology
Affiliation as printed
Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125 USA
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Affiliation as printed
Southwest Research Institute, San Antonio, TX 78238, USA
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