Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095
Journal article, 2023

The main scientific goal of TESS is to find planets smaller than Neptune around stars that are bright enough to allow for further characterization studies. Given our current instrumentation and detection biases, M dwarfs are prime targets in the search for small planets that are in (or near) the habitable zone of their host star. In this work, we use photometric observations and CARMENES radial velocity (RV) measurements to validate a pair of transiting planet candidates found by TESS. The data were fitted simultaneously, using a Bayesian Markov chain Monte Carlo (MCMC) procedure and taking into account the stellar variability present in the photometric and spectroscopic time series. We confirm the planetary origin of the two transiting candidates orbiting around TOI-2095 (LSPM J1902+7525). The star is a nearby M dwarf (d = 41.90 ± 0.03 pc, Teff = 3759 ± 87 K, V = 12.6 mag), with a stellar mass and radius of M∗ = 0.44 ± 0.02 M· and R∗ = 0.44 ± 0.02 R·, respectively. The planetary system is composed of two transiting planets: TOI-2095b, with an orbital period of Pb = 17.66484 ± (7 A - 10- 5) days, and TOI-2095c, with Pc = 28.17232 ± (14 A - 10- 5) days. Both planets have similar sizes with Rb = 1.25 ± 0.07 R· and Rc = 1.33 ± 0.08 R· for planet b and planet c, respectively. Although we did not detect the induced RV variations of any planet with significance, our CARMENES data allow us to set stringent upper limits on the masses of these objects. We find Mb < 4.1 M· for the inner and Mc < 7.4 M· for the outer planet (95% confidence level). These two planets present equilibrium temperatures in the range of 300 350 K and are close to the inner edge of the habitable zone of their star.

Techniques: photometric

Techniques: radial velocities

Planets and satellites: detection

Author

F. Murgas

Instituto de Astrofísica de Canarias

University of La Laguna

A. Castro-González

Centro de Astrobiologia (CAB)

Enric Palle

University of La Laguna

Instituto de Astrofísica de Canarias

Francisco J. Pozuelos

Institute of Astrophysics of Andalusia (IAA)

S. Millholland

Massachusetts Institute of Technology (MIT)

O. Foo

Massachusetts Institute of Technology (MIT)

Judith Korth

Lund University

E. Marfil

University of La Laguna

University of Hamburg

Instituto de Astrofísica de Canarias

P. J. Amado

Institute of Astrophysics of Andalusia (IAA)

J. A. Caballero

Centro de Astrobiologia (CAB)

Jessie L. Christiansen

National Aeronautics and Space Administration (NASA)

D. R. Ciardi

National Aeronautics and Space Administration (NASA)

Karen A. Collins

Harvard-Smithsonian Center for Astrophysics

M. Di Sora

Campo Catino Astronomical Observatory

A. Fukui

Instituto de Astrofísica de Canarias

University of Tokyo

Tianjun Gan

Tsinghua University

Erica J. Gonzales

University of California

T. Henning

Max Planck Society

Enrique Herrero

Institute of Space Studies of Catalonia (IEEC)

G. Isopi

Campo Catino Astronomical Observatory

Jon M. Jenkins

NASA Ames Research Center

J. Lillo-Box

Centro de Astrobiologia (CAB)

N. Lodieu

Instituto de Astrofísica de Canarias

University of La Laguna

R. Luque

University of Chicago

F. Mallia

Campo Catino Astronomical Observatory

Juan Carlos Morales

Institute of Space Studies of Catalonia (IEEC)

Institute of Space Sciences (ICE) - CSIC

Giuseppe Morello

Instituto de Astrofísica de Canarias

Chalmers, Space, Earth and Environment, Astronomy and Plasmaphysics

Norio Narita

Instituto de Astrofísica de Canarias

University of Tokyo

National Institutes of Natural Sciences

J. Orell-Miquel

Instituto de Astrofísica de Canarias

University of La Laguna

H. Parviainen

Instituto de Astrofísica de Canarias

University of La Laguna

M.A. Pérez-Torres

Institute of Astrophysics of Andalusia (IAA)

A. Quirrenbach

Heidelberg University

A. Reiners

University of Göttingen

I. Ribas

Institute of Space Studies of Catalonia (IEEC)

Institute of Space Sciences (ICE) - CSIC

B. S. Safonov

Moscow State University

S. Seager

Massachusetts Institute of Technology (MIT)

R. Schwarz

Harvard-Smithsonian Center for Astrophysics

A. Schweitzer

University of Hamburg

M. Schlecker

University of Arizona

I. A. Strakhov

Moscow State University

S. Vanaverbeke

Vereniging Voor Sterrenkunde (VVS)

KU Leuven

IRIS

Noriharu Watanabe

University of Tokyo

J. N. Winn

Princeton University

M. Zechmeister

University of Göttingen

Astronomy and Astrophysics

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

Vol. 677 A182

Subject Categories

Astronomy, Astrophysics and Cosmology

DOI

10.1051/0004-6361/202346692

More information

Latest update

11/2/2023