A planetary system with a sub-Neptune planet in the habitable zone of TOI-2093

Aims . We aim to confirm and measure the mass of the transiting planet candidate around the K5 V star TOI-2093, previously announced by the Transiting Exoplanet Survey Satellite (TESS) project. Methods . We combined photometric data from 32 sectors between 2019 and 2024 with 86 radial velocity measurements obtained with the CARMENES spectrograph over a period of 2.4 years, along with a series of ground-based, broadband photometric monitoring campaigns to characterize the host star and the transiting planet candidate, as well as to search for additional planets in the system. Our data indicate that TOI-2093 is a main-sequence star located at a distance of 83 pc, with solar metallicity, and a rotation period of 43.8±1.8 d. Results . We have confirmed the planetary nature of the TESS transiting planet candidate, named TOI-2093 c, through the detection of its Keplerian signal in the spectroscopic data. We measured a planetary radius of 2.30±0.12 R ⊕ , a Neptune-like mass of 15.8 −3.8 +3.6 M ⊕ , and an orbital period of 53.81149±0.00017 d. This makes TOI-2093 c the smallest exoplanet known in the habitable zone of a main-sequence FGK star. Given its size and relatively high density, TOI-2093 c belongs to a class of planets with no analog in the Solar System. In addition, the CARMENES data revealed the presence of a second planet candidate with a minimum mass of 10.6±2.5 M ⊕ and an orbital period of 12.836±0.021 d. This inner planet, which we designated TOI-2093 b, shows no detectable photometric transit in the TESS light curves. The orbital planes of the two planets are misaligned by more than 1.6° despite the near 4:1 mean-motion resonance of their orbital periods.

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Journal
Astronomy and Astrophysics
Published
2025-09-30
DOI
https://doi.org/10.1051/0004-6361/202556361
Primary Topic
Stellar, planetary, and galactic studies
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article
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article

A planetary system with a sub-Neptune planet in the habitable zone of TOI-2093

A. Reiners, A. Schweitzer, M. Błażek, F. Murgas et al.
Astronomy and Astrophysics
Stellar, planetary, and galactic studies
article

A planetary system with a sub-Neptune planet in the habitable zone of TOI-2093

A. Reiners, A. Schweitzer, M. Błażek, F. Murgas, E. Nagel, S. Vanaverbeke, F. J. Pozuelos, D.W. Latham, Ε. Πάλλη, M. R. Zapatero Osorio, J. A. Caballero, P. J. Amado, C. López, E. Marfil, I. Carleo, K. R. Sreenivas, A. P. Hatzes, I. Ribas, V. J. S. Béjar, R.P. Schwarz, D. Montes, L. Tal-Or, K. Collins, David Rapetti, E. Herrero, G. Nowak, Juan Carlos Morales, David R. Ciardi, S. Reffert, E. González-Álvarez, C. Cifuentes, J. Lillo-Box, A. Quirrenbach, R. Luque, Th. Henning, J. Sanz‐Forcada
article en

Abstract

Aims . We aim to confirm and measure the mass of the transiting planet candidate around the K5 V star TOI-2093, previously announced by the Transiting Exoplanet Survey Satellite (TESS) project. Methods . We combined photometric data from 32 sectors between 2019 and 2024 with 86 radial velocity measurements obtained with the CARMENES spectrograph over a period of 2.4 years, along with a series of ground-based, broadband photometric monitoring campaigns to characterize the host star and the transiting planet candidate, as well as to search for additional planets in the system. Our data indicate that TOI-2093 is a main-sequence star located at a distance of 83 pc, with solar metallicity, and a rotation period of 43.8±1.8 d. Results . We have confirmed the planetary nature of the TESS transiting planet candidate, named TOI-2093 c, through the detection of its Keplerian signal in the spectroscopic data. We measured a planetary radius of 2.30±0.12 R ⊕ , a Neptune-like mass of 15.8 −3.8 +3.6 M ⊕ , and an orbital period of 53.81149±0.00017 d. This makes TOI-2093 c the smallest exoplanet known in the habitable zone of a main-sequence FGK star. Given its size and relatively high density, TOI-2093 c belongs to a class of planets with no analog in the Solar System. In addition, the CARMENES data revealed the presence of a second planet candidate with a minimum mass of 10.6±2.5 M ⊕ and an orbital period of 12.836±0.021 d. This inner planet, which we designated TOI-2093 b, shows no detectable photometric transit in the TESS light curves. The orbital planes of the two planets are misaligned by more than 1.6° despite the near 4:1 mean-motion resonance of their orbital periods.

Astronomy and AstrophysicsVol. 703
Universidad Complutense de Madrid (ES), Ames Research Center (US), The University of Sydney (AU), Universities Space Research Association (US), Universidad de La Laguna (ES), Heidelberg University (DE), NASA Exoplanet Science Institute (US), University of Chicago (US), Calar Alto Observatory (ES), Institute of Astrophysics and Space Sciences (PT), Institut d'Estudis Espacials de Catalunya (ES), Max Planck Institute for Astrophysics (DE), Osservatorio Astrofisico di Torino (IT), Max Planck Institute for Astronomy (DE), Institute of Space Sciences (ES), Institute of Astronomy (RU), Center for Astrophysics Harvard & Smithsonian (US), Centro de Astrobiología (ES), Instituto de Astrofísica de Canarias (ES), Nicolaus Copernicus Astronomical Center (PL), Research Institute of Geodesy, Topography and Cartography (CZ), Hamburger Fern-Hochschule (DE), Thüringer Landessternwarte Tautenburg (DE), Instituto de Astrofísica de Andalucía (ES), Stichting tot Steun VCVGZ (NL), Ariel University (IL), Netherlands Institute for Radio Astronomy (NL)
Openalex Percentile: Top 81%
Stellar, planetary, and galactic studies
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