Discovery of TOI-1260d and the characterization of the multiplanet system
Journal article, 2023

We report the discovery of a third planet transiting the star TOI-1260, previously known to host two transiting sub-Neptune planets with orbital periods of 3.127 and 7.493 d, respectively. The nature of the third transiting planet with a 16.6-d orbit is supported by ground-based follow-up observations, including time-series photometry, high-angular resolution images, spectroscopy, and archival imagery. Precise photometric monitoring with CHEOPS allows to improve the constraints on the parameters of the system, improving our knowledge on their composition. The improved radii of TOI-1260b and TOI-1260c are 2.36 +/- 0.06R(circle plus), 2.82 +/- 0.08R(circle plus), respectively while the newly discovered third planet has a radius of 3.09 +/- 0.09R(circle plus). The radius uncertainties are in the range of 3 per cent, allowing a precise interpretation of the interior structure of the three planets. Our planet interior composition model suggests that all three planets in the TOI-1260 system contains some fraction of gas. The innermost planet TOI-1260b has most likely lost all of its primordial hydrogen-dominated envelope. Planets c and d were also likely to have experienced significant loss of atmospheric through escape, but to a lesser extent compared to planet b.

stars: individual: TOI-1260

techniques: radial velocities

planets and satellites: individual: TOI-1260b, c, d

planets and satellites: detection

techniques: photometric

planets and satellites: composition

Author

K. W. F. Lam

German Aerospace Center (DLR)

J. Cabrera

German Aerospace Center (DLR)

M. J. Hooton

University of Bern

University of Cambridge

Y. Alibert

University of Bern

A. Bonfanti

Austrian Academy of Sciences

M. Beck

University of Geneva

A. Deline

University of Geneva

H-G Floren

Stockholm University

A. E. Simon

University of Bern

L. Fossati

Austrian Academy of Sciences

Carina Persson

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Malcolm Fridlund

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

S. Salmon

University of Geneva

S. Hoyer

Aix Marseille University

H. P. Osborn

Massachusetts Institute of Technology (MIT)

University of Bern

T.G. Wilson

University of St Andrews

Iskra Georgieva

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Gr Nowak

Instituto de Astrofísica de Canarias

University of La Laguna

R. Luque

University of Chicago

J. A. Egger

University of Bern

V Adibekyan

University of Porto

R. Alonso

Instituto de Astrofísica de Canarias

University of La Laguna

G. A. Escude

Spanish National Research Council (CSIC)

Institute of Space Studies of Catalonia (IEEC)

T. Barczy

Admatis

D. Barrado

Spanish Astrobiology Center (INTA-CSIC)

S. C. C. Barros

University of Porto

W. Baumjohann

Austrian Academy of Sciences

T. Beck

University of Bern

A. Bekkelien

University of Geneva

W. Benz

University of Bern

N. Billot

University of Geneva

X. Bonfils

Grenoble Alpes University

A. Brandeker

Stockholm University

C. Broeg

University of Bern

S. Charnoz

Paris Descartes University

A. Collier Cameron

University of St Andrews

Sz Csizmadia

German Aerospace Center (DLR)

M. B. Davies

Lund University

M. Deleuil

Aix Marseille University

L. Delrez

University of Liège

O. D. S. Demangeon

University of Porto

B-O Demory

University of Bern

D. Ehrenreich

University of Geneva

A. Erikson

German Aerospace Center (DLR)

A. Fortier

University of Bern

D. Futyan

University of Geneva

D. Gandolfi

University of Turin

M. Gillon

University of Liège

M. Guedel

University of Vienna

P. Guterman

Aix Marseille University

Institut National des Sciences de l'Univers

J. Laskar

Sorbonne University

D. W. Latham

Harvard-Smithsonian Center for Astrophysics

A. Lecavelier des Etangs

Pierre and Marie Curie University (UPMC)

M. Lendl

University of Geneva

C. Lovis

Austrian Academy of Sciences

K. Heng

The University of Warwick

University of Bern

K. G. Isaak

European Space Research and Technology Centre (ESA ESTEC)

L. Kiss

The University of Sydney

Eötvös Loránd University (ELTE)

Hungarian Academy of Sciences

D. Magrin

Istituto nazionale di astrofisica (INAF)

P. F. L. Maxted

Keele University

V Nascimbeni

Istituto nazionale di astrofisica (INAF)

G. Olofsson

Stockholm University

R. Ottensamer

University of Vienna

I Pagano

Istituto nazionale di astrofisica (INAF)

E. Palle

University of La Laguna

Instituto de Astrofísica de Canarias

G. Peter

German Aerospace Center (DLR)

G. Piotto

Istituto nazionale di astrofisica (INAF)

D. Pollacco

The University of Warwick

D. Queloz

Swiss Federal Institute of Technology in Zürich (ETH)

University of Cambridge

I Ribas

Institute of Space Studies of Catalonia (IEEC)

Spanish National Research Council (CSIC)

R. Ragazzoni

Istituto nazionale di astrofisica (INAF)

University of Padua

N. Rando

European Space Agency (ESA)

H. Rauer

German Aerospace Center (DLR)

Technische Universität Berlin

Freie Universität Berlin

N. C. Santos

University of Porto

G. Scandariato

Istituto nazionale di astrofisica (INAF)

S. Seager

Massachusetts Institute of Technology (MIT)

D. Segransan

University of Geneva

L. M. Serrano

University of Turin

A. M. S. Smith

German Aerospace Center (DLR)

S. G. Sousa

University of Porto

M. Steller

Austrian Academy of Sciences

Gy M. Szabo

Eötvös Loránd University (ELTE)

N. Thomas

University of Bern

S. Udry

University of Geneva

V. Van Grootel

University of Liège

N. A. Walton

University of Cambridge

J. N. Winn

Princeton University

Monthly Notices of the Royal Astronomical Society

0035-8711 (ISSN) 1365-2966 (eISSN)

Vol. 519 1 1437-1451

Subject Categories

Astronomy, Astrophysics and Cosmology

Other Physics Topics

DOI

10.1093/mnras/stac3639

More information

Latest update

9/15/2023