TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley
Artikel i vetenskaplig tidskrift, 2022

We report the discovery and characterization of two small transiting planets orbiting the bright M3.0V star TOI-1468 (LSPM J0106+1913), whose transit signals were detected in the photometric time series in three sectors of the TESS mission. We confirm the planetary nature of both of them using precise radial velocity measurements from the CARMENES and MAROON-X spectrographs, and supplement them with ground-based transit photometry. A joint analysis of all these data reveals that the shorter-period planet, TOI-1468 b (P-b = 1.88 d), has a planetary mass of M-b = 3.21 +/- 0.24M(circle plus) and a radius of R-b = 1.280(-0.039)(+0.038) R-circle plus, resulting in a density of rho(b) = 8.39(-0.92)(+1.05) g cm(-3), which is consistent with a mostly rocky composition. For the outer planet, TOI-1468 c (P-c = 15.53 d), we derive a mass of M-c = 6.64(-0.68)(+0.67) M-circle plus,aradius of R-c = 2.06 +/- 0.04 R-circle plus, and a bulk density of rho(c) = 2.00(-0.19)(+0.21) g cm(-3), which corresponds to a rocky core composition with a H/He gas envelope. These planets are located on opposite sides of the radius valley, making our system an interesting discovery as there are only a handful of other systems with the same properties. This discovery can further help determine a more precise location of the radius valley for small planets around M dwarfs and, therefore, shed more light on planet formation and evolution scenarios.

techniques: radial velocities

stars: late-type

techniques: photometric

stars: individual: TOI-1468

Författare

P. Chaturvedi

Thüringer Landessternwarte Tautenburg

P. Bluhm

Universität Heidelberg

E. Nagel

Universität Hamburg

Thüringer Landessternwarte Tautenburg

A. P. Hatzes

Thüringer Landessternwarte Tautenburg

Giuseppe Morello

Instituto de Astrofísica de Canarias

Universidad de la Laguna

M. Brady

University of Chicago

Judith Korth

Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik

K. Molaverdikhani

Exzellenzcluster Origins

Ludwig-Maximilians-Universität München (LMU)

Universität Heidelberg

D. Kossakowski

Max-Planck-Gesellschaft

J. A. Caballero

European Space Astronomy Centre (ESAC)

E. W. Guenther

Thüringer Landessternwarte Tautenburg

E. Palle

Universidad de la Laguna

Instituto de Astrofísica de Canarias

N. Espinoza

Space Telescope Science Institute (STScI)

A. Seifahrt

University of Chicago

N. Lodieu

Universidad de la Laguna

Instituto de Astrofísica de Canarias

C. Cifuentes

European Space Astronomy Centre (ESAC)

E. Furlan

California Institute of Technology (Caltech)

P. J. Amado

Consejo Superior de Investigaciones Científicas (CSIC)

T. Barclay

University of Maryland

National Aeronautics and Space Administration (NASA)

J. Bean

University of Chicago

V. J. S. Bejar

Instituto de Astrofísica de Canarias

Universidad de la Laguna

G. Bergond

CAHA - Centro Astronómico hispano Alemán, A.I.E.

A. W. Boyle

California Institute of Technology (Caltech)

D. Ciardi

California Institute of Technology (Caltech)

K. A. Collins

Harvard-Smithsonian Center for Astrophysics

Collins

George Mason University

E. Esparza-Borges

Instituto de Astrofísica de Canarias

Universidad de la Laguna

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

C. L. Gnilka

National Aeronautics and Space Administration (NASA)

R. Goeke

Massachusetts Institute of Technology (MIT)

P. Guerra

Observatori Astronòmic Albanya

Th Henning

Max-Planck-Gesellschaft

E. Herrero

Consejo Superior de Investigaciones Científicas (CSIC)

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

S. B. Howell

National Aeronautics and Space Administration (NASA)

Jeffers

Max-Planck-Gesellschaft

J. M. Jenkins

National Aeronautics and Space Administration (NASA)

E. L. N. Jensen

Swarthmore College

D. Kasper

University of Chicago

T. Kodama

University of Tokyo

D. W. Latham

Harvard-Smithsonian Center for Astrophysics

M. J. Lopez-Gonzalez

Consejo Superior de Investigaciones Científicas (CSIC)

R. Luque

University of Chicago

D. Montes

Universidad Complutense de Madrid

J. C. Morales

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

Consejo Superior de Investigaciones Científicas (CSIC)

M. Mori

University of Tokyo

F. Murgas

Instituto de Astrofísica de Canarias

N. Narita

Astrobiology Center, Japan

University of Tokyo

Instituto de Astrofísica de Canarias

G. Nowak

Instituto de Astrofísica de Canarias

Universidad de la Laguna

H. Parviainen

Instituto de Astrofísica de Canarias

Universidad de la Laguna

V. M. Passegger

University of Oklahoma

Universität Hamburg

A. Quirrenbach

Universität Heidelberg

S. Reffert

Universität Heidelberg

A. Reiners

Georg-August-Universität Göttingen

I Ribas

Consejo Superior de Investigaciones Científicas (CSIC)

Centre Tecnològic de Telecomunicacions de Catalunya (CTTC)

G. R. Ricker

Massachusetts Institute of Technology (MIT)

E. Rodriguez

Consejo Superior de Investigaciones Científicas (CSIC)

C. Rodriguez-Lopez

Consejo Superior de Investigaciones Científicas (CSIC)

M. Schlecker

Max-Planck-Gesellschaft

University of Arizona

R. P. Schwarz

Patashnick Voorheesville Observatory

A. Schweitzer

Universität Hamburg

S. Seager

Massachusetts Institute of Technology (MIT)

G. Stefansson

Princeton University

C. Stockdale

Hazelwood Observatory

L. Tal-Or

Ariel University

Georg-August-Universität Göttingen

J. D. Twicken

SETI Institute

National Aeronautics and Space Administration (NASA)

S. Vanaverbeke

KU Leuven

Vereniging vor Sterrenkunde

AstroLAB IRIS

G. Wang

Tsinghua International School

D. Watanabe

Planetary Discoveries

J. N. Winn

Princeton University

M. Zechmeister

Georg-August-Universität Göttingen

Astronomy and Astrophysics

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

Vol. 666 A155

Ämneskategorier (SSIF 2011)

Astronomi, astrofysik och kosmologi

Atom- och molekylfysik och optik

Annan fysik

DOI

10.1051/0004-6361/202244056

Mer information

Senast uppdaterat

2025-03-18