Mostrar el registro sencillo del ítem

hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierLaboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA]
dc.contributor.authorCAVALIÉ, Thibault
hal.structure.identifierCornell University [New York]
dc.contributor.authorLUNINE, Jonathan
hal.structure.identifierLaboratoire d'Astrophysique de Marseille [LAM]
dc.contributor.authorMOUSIS, Olivier
hal.structure.identifierLaboratoire Interuniversitaire des Systèmes Atmosphériques [LISA (UMR_7583)]
dc.contributor.authorVENOT, Olivia
dc.date.issued2022
dc.date.conference2022
dc.description.abstractEnThe formation of giant planets can mainly be explained by two models: core accretion and gravitational collapse. Measurements of magnetic and gravity fields, as well as deep composition can help to constrain which scenario led to the formation of the Solar System Giant Planets. The deep composition also holds keys to understanding how primordial ices condensed and trapped the heavy elements, in the form of pure condensates, amorphous ices or clathrates. While the Galileo probe enabled measuring the abundances of noble gases and other heavy elements in Jupiter, the elemental composition of Saturn and the Ice Giants remains poorly constrained. Observations coupled with thermochemical modeling can help us to constrain the deep composition of giant planets and can also be used in synergy with mass spectrometry measurements of an in situ probe.In this paper, we will present recent results of thermochemical modeling of the Ice Giants and compare them with results obtained for Jupiter.
dc.language.isoen
dc.title.enObservations and thermochemical modeling of gas and ice giant planets
dc.typeCommunication dans un congrès
dc.identifier.doi10.5194/epsc2022-33
dc.subject.halPlanète et Univers [physics]
bordeaux.conference.title16th Europlanet Science Congress 2022
bordeaux.countryZZ
bordeaux.conference.cityà renseigner
bordeaux.peerReviewedoui
hal.identifierhal-03948220
hal.version1
hal.proceedingsoui
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-03948220v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2022&rft.au=CAVALI%C3%89,%20Thibault&LUNINE,%20Jonathan&MOUSIS,%20Olivier&VENOT,%20Olivia&rft.genre=unknown


Archivos en el ítem

ArchivosTamañoFormatoVer

No hay archivos asociados a este ítem.

Este ítem aparece en la(s) siguiente(s) colección(ones)

Mostrar el registro sencillo del ítem