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

Fuente: arXiv

Saved in:

Bibliographic Details
Main Authors:	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
Published:	2025
Subjects:	Earth and Planetary Astrophysics
Online Access:	Acceder al recurso
Tags:	Add Tag No Tags, Be the first to tag this record!

Internet

https://arxiv.org/abs/2510.07367