Issue |
A&A
Volume 664, August 2022
|
|
---|---|---|
Article Number | A199 | |
Number of page(s) | 23 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202243834 | |
Published online | 31 August 2022 |
The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
1
Instituto de Astrofisica de Andalucia (IAA-CSIC),
Glorieta de la Astronomia s/n,
18008
Granada, Spain
2
Department of Astronomy & Astrophysics, University of Chicago,
Chicago,
IL 60637
USA
e-mail: rluque@uchicago.edu
3
Division of Geological and Planetary Sciences, California Institute of Technology,
1200 East California Blvd,
Pasadena,
CA 91125
USA
4
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge,
MA 02139
USA
5
Institut für Astrophysik, Georg-August-Universität,
Friedrich-Hund-Platz 1,
37077
Göttingen, Germany
6
Astrophysics Group, Keele University,
Keele ST5 6BG,
UK
7
Center of Excellence in Information Systems, Tennessee State University,
Nashville,
TN 37209-1561
USA
8
Universitäts-Sternwarte, Ludwig-Maximilians-Universität München,
Scheinerstrasse 1,
81679
München, Germany
9
Exzellenzcluster Origins,
Boltzmannstraβe 2,
85748
Garching, Germany
10
Max-Planck-Institut für Astronomie,
Königstuhl 17,
69117
Heidelberg, Germany
11
Landessternwarte, Zentrum für Astronomie der Universität Heidelberg,
Königstuhl 12,
69117
Heidelberg, Germany
12
Instituto de Astrofisica de Canarias (IAC),
38205
La Laguna, Tenerife, Spain
13
Departamento de Astrofisica, Universidad de La Laguna (ULL),
38206
La Laguna, Tenerife, Spain
14
Space Sciences, Technologies and Astrophysics Research (STAR) Institute, Universitde Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
15
Astrobiology Research Unit, Université de Liège,
Allée du 6 Août 19C,
4000
Liège, Belgium
16
Center for Earth Evolution and Dynamics, Department of Geosciences, University of Oslo,
Sem Saelands vei 2b
0315
Oslo, Norway
17
Institut de Ciències de l’Espai (CSIC),
Campus UAB, c/de Can Magrans s/n,
08193
Bellaterra, Barcelona, Spain
18
Centro Astronómico Hispano Alemán, Observatorio de Calar Alto, Sierra de los Filabres,
04550
Gérgal, Almeria, Spain
19
NASA Exoplanet Science Institute, Caltech/IPAC,
Mail Code 100-22, 1200 E. California Blvd.,
Pasadena,
CA 91125
USA
20
Centro de Astrobiologia (INTA-CSIC), ESAC Campus,
Camino Bajo del Castillo s/n,
28692
Villanueva de la Cañada, Madrid, Spain
21
Center for Astrophysics I Harvard & Smithsonian,
60 Garden St,
Cambridge,
MA 02138,
USA
22
Vereniging Voor Sterrenkunde,
Oostmeers 122 C,
8000
Brugge, Belgium
23
Space Telescope Science Institute,
3700 San Martin Drive,
Baltimore,
MD 21218
USA
24
NSF’s Optical Infrared Astronomy Research Laboratory,
950 North Cherry Avenue Tucson,
AZ 85719
USA
25
Department of Astronomy, Yale University,
52 Hillhouse Avenue,
New Haven,
CT 06511
USA
26
Thüringer Landessternwarte Tautenburg,
Sternwarte 5,
07778
Tautenburg, Germany
27
Space Science & Astrobiology Division, NASA Ames Research Center,
Moffett Field,
CA 94035
USA
28
Department of Astronomy, The University of California,
Berkeley,
CA 94720
USA
29
Max Planck Institute for Solar System Research,
Justus-von-Liebig-Weg 3,
37077
Göttingen, Germany
30
Department of Earth and Planetary Sciences, University of California,
Riverside,
CA 92521
USA
31
Departamento de Física de la Tierra y Astrofísica & IPARCOSUCM (Instituto de Física de Particulas y del Cosmos de la UCM), Facultad de Ciencias Físicas, Universidad Complutense de Madrid,
28040
Madrid, Spain
32
Department of Physics, University of Warwick,
Gibbet Hill Road, Coventry CV4 7AL,
UK
33
Institut d’Estudis Espacials de Catalunya,
08034
Barcelona, Spain
34
Department of Astronomy/Steward Observatory, The University of Arizona,
933 North Cherry Avenue,
Tucson,
AZ 85721
USA
35
Hamburger Sternwarte, Universität Hamburg,
Gojenbergsweg 112,
21029
Hamburg, Germany
36
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology,
Cambridge,
MA 02139
USA
37
Department of Aeronautics and Astronautics, MIT,
77 Massachusetts Avenue,
Cambridge,
MA 02139
USA
38
Department of Physics and Astronomy, Vanderbilt University,
Nashville,
TN 37235
USA
39
Department of Physics, Ariel University,
Ariel
40700
Israel
40
Department of Astronomy, Sofia University “St Kliment Ohridski”,
5 James Bourchier Blvd,
1164
Sofia, Bulgaria
41
AstroLAB IRIS, Provinciaal Domein “De Palingbeek”,
Verbrandemolenstraat 5,
8902
Zillebeke, Ieper, Belgium
42
Department of Astrophysical Sciences, Princeton University,
4 Ivy Lane,
Princeton,
NJ 08544,
USA
43
Centro de Astrobiologia (CSIC-INTA),
Carretera de Ajalvir km 4,
28850
Torrejón de Ardoz, Madrid, Spain
Received:
21
April
2022
Accepted:
13
June
2022
We report the discovery of a multiplanetary system transiting the M0 V dwarf HD 260655 (GJ 239, TOI-4599). The system consists of at least two transiting planets, namely HD 260655 b, with a period of 2.77 d, a radius of Rb = 1.240 ± 0.023 R⊕, a mass of Mb = 2.14 ± 0.34 M⊕, and a bulk density of ρb = 6.2 ± 1.0 g cm−3, and HD 260655 c, with a period of 5.71 d, a radius of , a mass of Mc = 3.09 ± 0.48 M⊕, and a bulk density of g cm−3. The planets have been detected in transit by the Transiting Exoplanet Survey Satellite (TESS) mission and confirmed independently with archival and new precise radial velocities obtained with the HIRES and CARMENES instruments since 1998 and 2016, respectively. At a distance of 10 pc, HD 260655 has become the fourth closest known multitransiting planet system after HD 219134, LTT 1445 A, and AU Mic. Due to the apparent brightness of the host star (J = 6.7 mag), both planets are among the most suitable rocky worlds known today for atmospheric studies with the James Webb Space Telescope, both in transmission and emission.
Key words: planetary systems / techniques: photometric / techniques: radial velocities / stars: late-type / planets and satellites: individual: HD 260655
© R. Luque et al. 2022
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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