Giant Planets Tristan Guillot, Daniel Gautier
To cite this version:
Tristan Guillot, Daniel Gautier. Giant Planets. G. Schubert, T. Spohn. Treatise on Geophysics, 2nd edition, Elsevier, 2015, 10.1016/B978-0-444-53802-4.00176-7. hal-00991246v2
HAL Id: hal-00991246 https://hal.archives-ouvertes.fr/hal-00991246v2 Submitted on 20 Jan 2015
HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Treatise on Geophysics, 2nd Edition 00 (2015) 1–42
To appear in Treatise on Geophysics, 2nd Edition, Eds. T. Spohn & G. Schubert
Giant Planets
Tristan Guillota,∗, Daniel Gautierb
aLaboratoire Lagrange, Universit´ede Nice-Sophia Antipolis, Observatoire de la Cˆote d’Azur, CNRS, CP 34229, 06304 NICE Cedex 04, France bLESIA, Observatoire de Paris, CNRS FRE 2461, 5 pl. J. Janssen, 92195 Meudon Cedex, France
Abstract We review the interior structure and evolution of Jupiter, Saturn, Uranus and Neptune, and giant exoplanets with particular em- phasis on constraining their global composition. Compared to the first edition of this review, we provide a new discussion of the atmospheric compositions of the solar system giant planets, we discuss the discovery of oscillations of Jupiter and Saturn, the significant improvements in our understanding of the behavior of material at high pressures and the consequences for interior and evolution models. We place the giant planets in our Solar System in context with the trends seen for exoplanets.