TOI-1846 b: A super-Earth in the radius valley orbiting a nearby M dwarf

  • Abderahmane Soubkiou
  • , Khalid Barkaoui
  • , Zouhair Benkhaldoun
  • , Mourad Ghachoui
  • , Jamila Chouqar
  • , Benjamin V. Rackham
  • , Adam Burgasser
  • , Emma Softich
  • , Enric Pallé
  • , Akihiko Fukui
  • , Norio Narita
  • , Felipe Murgas
  • , Steve B. Howell
  • , Catherine A. Clark
  • , Colin Littlefield
  • , Allyson Bieryla
  • , Andrew W. Boyle
  • , David Ciardi
  • , Karen Collins
  • , Kevin I. Collins
  • Jerome De Leon, Courtney D. Dressing, Jason Eastman, Emma Esparza-Borges, Steven Giacalone, Holden Gill, Michaël Gillon, Kai Ikuta, J. M. Jenkins, Taiki Kagetani, David W. Latham, Mayuko Mori, Hannu Parviainen, Emily Pass, G. Ricker, Boris S. Safonov, Arjun B. Savel, Richard P. Schwarz, Sara Seager, Ivan A. Strakhov, Gregor Srdoc, R. Vanderspek, Noriharu Watanabe, Cristilyn N. Watkins, J. Winn

Research output: Contribution to journalArticlepeer-review

Abstract

We present the discovery and validation of a super-Earth planet orbiting the M dwarf star TOI-1846 (TIC 198385543). The host star () is located 47 pc away and has a radius of, a mass of and an effective temperature of K. Our analyses are based on joint modelling of Transiting Exoplanet Survey Satellite (TESS) photometry and ground-based multicolour photometric data. We also use high-resolution imaging and archival images, as well as statistical validation techniques to support the planetary system nature. We find that TOI-1846 b is a super-Earth sized planet with radius of and a predicted mass of (from the Chen & Kipping relation) on a 3.9 d orbit, with an equilibrium temperature of (assuming a null Bond Albedo) and an incident flux of. Based on the two radial velocity (RV) measurements obtained with the Tillinghast Reflector Echelle Spectrograph and high-resolution imaging, a non-planetary transiting companion is excluded. With a radius of 1.8, TOI-1846 b is within the sparsely populated radius range around 2 known as the radius gap (or radius valley). This discovery can contribute to refining the precise location of the radius valley for small planets orbiting bright M dwarfs, thereby enhancing our understanding of planetary formation and evolution processes.

Original languageEnglish (US)
Pages (from-to)3249-3268
Number of pages20
JournalMonthly Notices of the Royal Astronomical Society
Volume541
Issue number4
DOIs
StatePublished - Aug 1 2025

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • planetary systems
  • planets and satellites
  • stars: individual: (TIC 198385543
  • TOI 1846)

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