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Hot Rocks Survey. IV. Emission from LTT 3780 b Is Consistent with a Bare Rock

It is an open question whether small planets around M dwarfs are able to maintain atmospheres. The Hot Rocks Survey aims to address this question by observing nine rocky exoplanets orbiting M dwarfs with MIRI emission photometry to constrain the onset of atmospheres. In this paper, we present two MI...

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Principais autores: Natalie H. Allen, Néstor Espinoza, Hannah Diamond-Lowe, João M. Mendonça, Brice-Olivier Demory, Amélie Gressier, Jegug Ih, Mark Fortune, Prune C. August, Måns Holmberg, Erik Meier Valdés, Merlin Zgraggen, Lars A. Buchhave, Adam J. Burgasser, Chloe Fisher, Neale P. Gibson, Kevin Heng, Jens Hoeijmakers, Daniel Kitzmann, Bibiana Prinoth, Alexander D. Rathcke, Brett M. Morris
Formato: Artigo
Idioma:Inglês
Publicado em: IOP Publishing 2025-01-01
coleção:The Astronomical Journal
Assuntos:
M dwarf stars
Exoplanet astronomy
Exoplanet atmospheres
Extrasolar rocky planets
Acesso em linha:https://doi.org/10.3847/1538-3881/adfc51
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