A high internal heat flux and large core in a warm neptune exoplanet.


Journal

Nature
ISSN: 1476-4687
Titre abrégé: Nature
Pays: England
ID NLM: 0410462

Informations de publication

Date de publication:
20 May 2024
Historique:
received: 15 01 2024
accepted: 02 05 2024
medline: 21 5 2024
pubmed: 21 5 2024
entrez: 20 5 2024
Statut: aheadofprint

Résumé

Interactions between exoplanetary atmospheres and internal properties have long been hypothesized to be drivers of the inflation mechanisms of gaseous planets and apparent atmospheric chemical disequilibrium conditions

Identifiants

pubmed: 38768634
doi: 10.1038/s41586-024-07514-w
pii: 10.1038/s41586-024-07514-w
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Informations de copyright

© 2024. The Author(s), under exclusive licence to Springer Nature Limited.

Auteurs

Luis Welbanks (L)

School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA. luis.welbanks@asu.edu.

Taylor J Bell (TJ)

Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA.
Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA.

Thomas G Beatty (TG)

Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA.

Michael R Line (MR)

School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA.

Kazumasa Ohno (K)

Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA.
Division of Science, National Astronomical Observatory of Japan, Tokyo, Japan.

Jonathan J Fortney (JJ)

Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA.

Everett Schlawin (E)

Steward Observatory, University of Arizona, Tucson, AZ, USA.

Thomas P Greene (TP)

Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA.

Emily Rauscher (E)

Department of Astronomy, University of Michigan, Ann Arbor, MI, USA.

Peter McGill (P)

Space Science Institute, Lawrence Livermore National Laboratory, Livermore, CA, USA.

Matthew Murphy (M)

Steward Observatory, University of Arizona, Tucson, AZ, USA.

Vivien Parmentier (V)

Laboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice, France.

Yao Tang (Y)

Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA.

Isaac Edelman (I)

Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA.

Sagnick Mukherjee (S)

Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA.

Lindsey S Wiser (LS)

School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA.

Pierre-Olivier Lagage (PO)

Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France.

Achrène Dyrek (A)

Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France.

Kenneth E Arnold (KE)

Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA.

Classifications MeSH