CAVALIÉ, Thibault; LUNINE, Jonathan; MOUSIS, Olivier; HUESO, Ricardo

doi:10.1007/s11214-024-01045-6

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CAVALIÉ, Thibault
ASP 2024

LUNINE, Jonathan
Cornell University [Ithaca] [CU]

MOUSIS, Olivier
Laboratoire d'Astrophysique de Marseille [LAM]

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Space Science Reviews. 2024, vol. 220, n° 1, p. 8

Springer Verlag

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Deep elemental composition is a challenging measurement to achieve in the giant planets of the solar system. Yet, knowledge of the deep composition offers important insights in the internal structure of these planets, their evolutionary history and their formation scenarios. A key element whose deep abundance is difficult to obtain is oxygen, because of its propensity for being in condensed phases such as rocks and ices. In the atmospheres of the giant planets, oxygen is largely stored in water molecules that condense below the observable levels. At atmospheric levels that can be investigated with remote sensing, water abundance can modify the observed meteorology, and meteorological phenomena can distribute water through the atmosphere in complex ways that are not well understood and that encompass deeper portions of the atmosphere. The deep oxygen abundance provides constraints on the connection between atmosphere and interior and on the processes by which other elements were trapped, making its determination an important element to understand giant planets. In this paper, we review the current constraints on the deep oxygen abundance of the giant planets, as derived from observations and thermochemical models.< Réduire

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Uranus

Neptune

Ice giants

Composition

Formation

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The Deep Oxygen Abundance in Solar System Giant Planets, with a New Derivation for Saturn

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