TOI-4438 b: a transiting mini-Neptune amenable to atmospheric characterization
Elisa Goffo, P. Chaturvedi, F. Murgas, Giuseppe Morello, J. Orell-Miquel, L. Acuña, L. Peña-Moñino, Ε. Πάλλη, A. P. Hatzes, S. Geraldía-González, F. J. Pozuelos, A. F. Lanza, D. Gandolfi, J. A. Caballero, Martin Schlecker, M. Á. Pérez-Torres, N. Lodieu, A. Schweitzer, C. Hellier, S. V. Jeffers, C. Duque-Arribas, C. Cifuentes, V. J. S. Béjar, Mangesh Daspute, Franky Dubois, Sjoerd Dufoer, E. Esparza-Borges, Akihiko Fukui, Yuya Hayashi, E. Herrero, M. Mori, Norio Narita, H. Parviainen, L. Tal-Or, S. Vanaverbeke, I. Hermelo, P. J. Amado, S. Dreizler, Th. Henning, J. Lillo-Box, R. Luque, M. Mallorquín, E. Nagel, A. Quirrenbach, S. Reffert, A. Reiners, I. Ribas, P. Schöfer, H. M. Tabernero, M. Zechmeister
Abstract
We report the confirmation and mass determination of a mini-Neptune transiting the M3.5 V star TOI-4438 (G 182-34) every 7.44 days. A transit signal was detected with NASA’s TESS space mission in the sectors 40, 52, and 53. In order to validate the planet TOI-4438 b and to determine the system properties, we combined TESS data with high-precision radial velocity measurements from the CARMENES spectrograph, spanning almost one year, and ground-based transit photometry. We found that TOI-4438 b has a radius of R b = 2.52 ± 0.13 R ⊕ (5% precision), which together with a mass of M b = 5.4 ± 1.1 M ⊕ (20% precision), results in a bulk density of ρ b = 1.85 −0.44 +0.51 g cm −3 (~28% precision), aligning the discovery with a volatile-rich planet. Our interior structure retrieval with a pure water envelope yields aminimum water mass fraction of 46% (1 σ ). TOI-4438 b is a volatile-rich mini-Neptune with likely H/He mixed with molecules, such as water, CO 2 , and CH 4 . The primary star has a J -band magnitude of 9.7, and the planet has a high transmission spectroscopy metric (TSM) of 136 ± 13. Taking into account the relatively warm equilibrium temperature of T eq = 435 ± 15 K, and the low activity level of its host star, TOI-4438 b is one of the most promising mini-Neptunes around an M dwarf for transmission spectroscopy studies.