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Magma ocean interactions can explain JWST observations of the sub-Neptune TOI-270 d

Fuente: arXiv

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Détails bibliographiques
Auteurs principaux:	Nixon, Matthew C., Somers, R. Sander, Savel, Arjun B., Ih, Jegug, Kempton, Eliza M. -R., Young, Edward D., Schlichting, Hilke E., Lichtenberg, Tim, Welbanks, Luis, Misener, William, Piette, Anjali A. A., Wogan, Nicholas F.
Format:	Preprint
Publié:	2025
Sujets:	Earth and Planetary Astrophysics
Accès en ligne:	Acceder al recurso
Tags:	Ajouter un tag Pas de tags, Soyez le premier à ajouter un tag!

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