TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley

TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley

Characterizing the bulk compositions of transiting exoplanets within the M dwarf radius valley offers a unique means to establish whether the radius valley emerges from an atmospheric mass-loss process or is imprinted by planet formation itself. We present the confirmation of such a planet orbiting...

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Hlavní autoři: Collin Cherubim, Ryan Cloutier, David Charbonneau, Chris Stockdale, Keivan G. Stassun, Richard P. Schwarz, Boris Safonov, Annelies Mortier, Pablo Lewin, David W. Latham, Keith Horne, Raphaëlle D. Haywood, Erica Gonzales, Maria V. Goliguzova, Karen A. Collins, David R. Ciardi, Allyson Bieryla, Alexandre A. Belinski, Bill Wohler, Christopher A. Watson, Roland Vanderspek, Stéphane Udry, Alessandro Sozzetti, Damien Ségransan, Dimitar Sasselov, George R. Ricker, Ken Rice, Ennio Poretti, Giampaolo Piotto, Francesco Pepe, Emilio Molinari, Giuseppina Micela, Michel Mayor, Christophe Lovis, Mercedes López-Morales, Jon M. Jenkins, Zahra Essack, Xavier Dumusque, John P. Doty, Knicole D. Colón, Andrew Collier Cameron, Lars A. Buchhave
Médium: Článek
Jazyk:English
Vydáno: IOP Publishing 2023-01-01
Edice:The Astronomical Journal
Témata:
Exoplanets
Exoplanet formation
Planet formation
Exoplanet evolution
M dwarf stars
Exoplanet atmospheric evolution
On-line přístup:https://doi.org/10.3847/1538-3881/acbdfd

Internet

https://doi.org/10.3847/1538-3881/acbdfd

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