HD 35843: A Sun-like Star Hosting a Long-period Sub-Neptune and Inner Super-Earth

  • Katharine Hesse
  • , Ismael Mireles
  • , François Bouchy
  • , Diana Dragomir
  • , Solène Ulmer-Moll
  • , Nora L. Eisner
  • , Keivan G. Stassun
  • , Samuel N. Quinn
  • , Hugh P. Osborn
  • , Sergio G. Sousa
  • , Cristilyn N. Watkins
  • , Karen A. Collins
  • , Edward M. Bryant
  • , Jonathan M. Irwin
  • , Coel Hellier
  • , Marshall C. Johnson
  • , Carl Ziegler
  • , Steve B. Howell
  • , David R. Anderson
  • , Daniel Bayliss
  • Allyson Bieryla, César Briceño, R. Paul Butler, David Charbonneau, Ryan Cloutier, Jeffrey Crane, Jason Dittmann, Jason D. Eastman, Sebastián A. Freigeiro, Benjamin J. Fulton, Samuel Gill, Maximilian Günther, Haedam Im, Jon M. Jenkins, Michelle Kunimoto, Baptiste Lavie, Monika Lendl, Michael B. Lund, Andrew W. Mann, Belinda Nicholson, David Osip, Martin Paegert, Nuno C. Santos, Richard P. Schwarz, Sara Seager, Stephen Shectman, Johanna Teske, Joseph D. Twicken, Stéphane Udry, Vincent Van Eylen, José Vinés, Sharon X. Wang, Peter J. Wheatley, Joshua N. Winn, Edward E. Zuidema

Research output: Contribution to journalArticlepeer-review

Abstract

We report the discovery and confirmation of two planets orbiting the metal-poor Sun-like star HD 35843 (TOI 4189). HD 35843 c is a temperate sub-Neptune transiting planet with an orbital period of 46.96 days that was first identified by Planet Hunters TESS. We combine data from TESS and follow-up observations to rule out false-positive scenarios and validate the planet. We then use ESPRESSO radial velocities (RVs) to confirm the planetary nature and characterize the planet’s mass and orbit. Further analysis of these RVs reveals the presence of an additional planet, HD 35843 b, with a period of 9.90 days and a minimum mass of 5.84 ± 0.84 M. For HD 35843 c, a joint photometric and spectroscopic analysis yields a radius of 2.54 ± 0.08 R, a mass of 11.32 ± 1.60 M, and an orbital eccentricity of e = 0.15 ± 0.07. With a bulk density of 3.80 ± 0.70 g cm−3, the planet might be rocky with a substantial H2 atmosphere or it might be a “water world.” With an equilibrium temperature of ∼480 K, HD 35843 c is among the coolest ∼5% of planets discovered by TESS. Combined with the host star’s relative brightness (V = 9.4), HD 35843 c is a promising target for atmospheric characterization that will probe this sparse population of temperate sub-Neptunes.

Original languageEnglish (US)
Article number108
JournalAstronomical Journal
Volume170
Issue number2
DOIs
StatePublished - Aug 4 2025

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

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