Jupiter's inhomogeneous envelope

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 sta...

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Bibliographische Detailangaben

Veröffentlicht in:	arXiv.org 2022-03
Hauptverfasser:	Miguel, Y, Bazot, M, Guillot, T, Howard, S, Galanti, E, Kaspi, Y, Hubbard, W B, Militzer, B, Helled, R, Atreya, S K, Connerney, J E P, Durante, D, Kulowski, L, Lunine, J I, Stevenson, D, Bolton, S
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheric models Deposition Equations of state Heavy elements Jupiter Jupiter probes Physics - Earth and Planetary Astrophysics Physics - Solar and Stellar Astrophysics Planet formation Planetary interiors Planetary mass Solar system Space missions Statistical analysis Zonal flow (meteorology)
Online-Zugang:	Volltext
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