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...

Fuld beskrivelse

Bibliografiske detaljer

Principais autores:	Simon Müller, Ravit Helled
Format:	Artigo
Sprog:	Inglês
Udgivet:	IOP Publishing 2024-01-01
Serier:	The Astrophysical Journal
Fag:	Solar system gas giant planets Jupiter Planetary interior Planetary structure Planetary atmospheres Planetary science
Online adgang:	https://doi.org/10.3847/1538-4357/ad3738
Tags:	Tilføj Tag Ingen Tags, Vær først til at tagge denne postø!