Can Jupiter’s Atmospheric Metallicity Be Different from the Deep Interior?

Updated formation and structure models of Jupiter predict a metal-poor envelope. This is at odds with the two to three times solar metallicity measured by the Galileo probe. Additionally, Juno data imply that water and ammonia are enriched. Here, we explore whether Jupiter could have a deep radiativ...

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Autors principals:	Simon Müller, Ravit Helled
Format:	Artigo
Idioma:	Inglês
Publicat:	IOP Publishing 2024-01-01
Col·lecció:	The Astrophysical Journal
Matèries:	Solar system gas giant planets Jupiter Planetary interior Planetary structure Planetary atmospheres Planetary science
Accés en línia:	https://doi.org/10.3847/1538-4357/ad3738
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