TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
Journal article, 2023

Context. The current architecture of a given multi-planetary system is a key fingerprint of its past formation and dynamical evolution history. Long-term follow-up observations are key to complete their picture. Aims. In this paper, we focus on the confirmation and characterization of the components of the TOI-969 planetary system, where TESS detected a Neptune-size planet candidate in a very close-in orbit around a late K-dwarf star. Methods. We use a set of precise radial velocity observations from HARPS, PFS, and CORALIE instruments covering more than two years in combination with the TESS photometric light curve and other ground-based follow-up observations to confirm and characterize the components of this planetary system. Results. We find that TOI-969 b is a transiting close-in (Pb ∼ 1.82 days) mini-Neptune planet (Formula Presented), placing it on the lower boundary of the hot-Neptune desert (Teq,b = 941 ± 31 K). The analysis of its internal structure shows that TOI-969 b is a volatile-rich planet, suggesting it underwent an inward migration. The radial velocity model also favors the presence of a second massive body in the system, TOI-969 c, with a long period of (Formula Presented) days, a minimum mass of (Formula Presented), and a highly eccentric orbit of (Formula Presented). Conclusions. The TOI-969 planetary system is one of the few around K-dwarfs known to have this extended configuration going from a very close-in planet to a wide-separation gaseous giant. TOI-969 b has a transmission spectroscopy metric of 93 and orbits a moderately bright (G = 11.3 mag) star, making it an excellent target for atmospheric studies. The architecture of this planetary system can also provide valuable information about migration and formation of planetary systems.

planets and satellites: fundamental parameters

planets and satellites: composition

techniques: photometric

planets and satellites: detection

stars: individual: TOI-969

techniques: radial velocities

Author

J. Lillo-Box

European Space Astronomy Centre (ESAC)

D. Gandolfi

University of Turin

D. J. Armstrong

The University of Warwick

K. A. Collins

Harvard-Smithsonian Center for Astrophysics

L. D. Nielsen

University of Geneva

European Southern Observatory (ESO)

R. Luque

Institute of Astrophysics of Andalusia (IAA)

Judith Korth

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

S. G. Sousa

University of Porto

S. N. Quinn

Harvard-Smithsonian Center for Astrophysics

L. Acuña

Laboratoire d'Astrophysique de Marseille

S. B. Howell

NASA Ames Research Center

Giuseppe Morello

University of La Laguna

Instituto de Astrofísica de Canarias

Coel Hellier

Keele University

S. Giacalone

University of California

S. Hoyer

Laboratoire d'Astrophysique de Marseille

K. Stassun

Vanderbilt University

E. Palle

Instituto de Astrofísica de Canarias

University of La Laguna

A. Aguichine

Laboratoire d'Astrophysique de Marseille

O. Mousis

Laboratoire d'Astrophysique de Marseille

V. Adibekyan

University of Porto

T. Azevedo Silva

University of Porto

D. Barrado

European Space Astronomy Centre (ESAC)

M. Deleuil

Laboratoire d'Astrophysique de Marseille

J. D. Eastman

Harvard-Smithsonian Center for Astrophysics

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

F. Hawthorn

The University of Warwick

J. M. Irwin

University of Cambridge

Jon M. Jenkins

NASA Ames Research Center

D. W. Latham

Harvard-Smithsonian Center for Astrophysics

Alexandra Muresan

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

N. Narita

Instituto de Astrofísica de Canarias

National Institutes of Natural Sciences

University of Tokyo

Carina Persson

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

A. Santerne

Laboratoire d'Astrophysique de Marseille

N. C. Santos

University of Porto

A. B. Savel

University of Maryland

H. P. Osborn

University of Bern

J. K. Teske

Carnegie Observatories

P. J. Wheatley

The University of Warwick

J. N. Winn

Princeton University

S. C.C. Barros

University of Porto

R. P. Butler

Carnegie Observatories

D. A. Caldwell

NASA Ames Research Center

D. Charbonneau

Harvard-Smithsonian Center for Astrophysics

R. Cloutier

Harvard-Smithsonian Center for Astrophysics

J. D. Crane

Carnegie Observatories

O. Demangeon

University of Porto

R. F. Díaz

Consejo Nacional de Investigaciones Cientificas y Tecnicas

X. Dumusque

University of Geneva

M. Esposito

Thüringer Landessternwarte Tautenburg

B. Falk

Space Telescope Science Institute (STScI)

H. Gill

University of California

S. Hojjatpanah

Laboratoire d'Astrophysique de Marseille

L. Kreidberg

Max Planck Society

Ismael Mireles

University of New Mexico

A. Osborn

The University of Warwick

G. R. Ricker

Massachusetts Institute of Technology (MIT)

J. E. Rodriguez

Michigan State University

R. P. Schwarz

Harvard-Smithsonian Center for Astrophysics

S. Seager

Massachusetts Institute of Technology (MIT)

J. Serrano Bell

National University of La Plata

S.A. Shectman

Carnegie Observatories

Avi Shporer

Massachusetts Institute of Technology (MIT)

Michael L. Vezie

Massachusetts Institute of Technology (MIT)

S. X. Wang

Tsinghua University

G. Zhou

University of Southern Queensland

Astronomy and Astrophysics

0004-6361 (ISSN) 1432-0746 (eISSN)

Vol. 669 A109

Subject Categories

Astronomy, Astrophysics and Cosmology

Embedded Systems

Computer Science

DOI

10.1051/0004-6361/202243879

More information

Latest update

2/17/2023