Issue |
A&A
Volume 642, October 2020
|
|
---|---|---|
Article Number | A236 | |
Number of page(s) | 20 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/202038967 | |
Published online | 23 October 2020 |
Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)★
1
Landessternwarte, Zentrum für Astronomie der Universität Heidelberg,
Königstuhl 12,
69117
Heidelberg,
Germany
e-mail: j.kemmer@lsw.uni-heidelberg.de
2
Max-Planck-Institut für Astronomie, Königstuhl 17,
69117
Heidelberg,
Germany
3
Centro de Astrobiología (CSIC-INTA), ESAC, Camino bajo del castillo s/n,
28692
Villanueva de la Cañada,
Madrid, Spain
4
Instituto de Astrofísica de Andalucía (IAA-CSIC), Glorieta de la Astronomía s/n,
18008
Granada, Spain
5
Departamento de Matemática y Físíca Aplicadas, Universidad Católica de la Santísima Concepción, Alonso de Rivera 2850,
Concepción, Chile
6
Univ. Grenoble Alpes, CNRS, IPAG,
38000
Grenoble, France
7
Caltech/IPAC-NASA Exoplanet Science Institute, 770 S. Wilson Avenue,
Pasadena,
CA
91106, USA
8
Center for Astrophysics | Harvard & Smithsonian, 60 Garden Street,
Cambridge,
MA
02138, USA
9
Space Telescope Science Institute, 3700 San Martin Drive,
Baltimore,
MD
21218, USA
10
Department of Earth and Planetary Science, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
11
Departamento de Astrofísica, Universidad de La Laguna,
38206
La Laguna,
Tenerife,
Spain
12
Department of Earth and Planetary Sciences, Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro-ku,
Tokyo
152-8551, Japan
13
NASA Ames Research Center,
Moffett Field,
CA
94035, USA
14
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139, USA
15
Komaba Institute for Science, The University of Tokyo, 3-8-1 Komaba, Meguro,
Tokyo
153-8902, Japan
16
JST, PRESTO, 3-8-1 Komaba, Meguro,
Tokyo
153-8902, Japan
17
Astrobiology Center, 2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
18
Instituto de Astrofísica de Canarias (IAC),
38205
La Laguna,
Tenerife, Spain
19
Institut für Astrophysik, Georg-August-Universität, Friedrich-Hund-Platz 1,
37077
Göttingen, Germany
20
Institut de Ciències de l’Espai (ICE, CSIC), Campus UAB, Can Magrans s/n,
08193
Bellaterra, Spain
21
Institut d’Estudis Espacials de Catalunya (IEEC),
08034
Barcelona, Spain
22
NASA Goddard Space Flight Center, 8800 Greenbelt Road,
Greenbelt,
MD
20771, USA
23
Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology,
Cambridge,
MA
02139, USA
24
Department of Aeronautics and Astronautics, MIT, 77 Massachusetts Avenue,
Cambridge,
MA
02139, USA
25
Department of Astrophysical Sciences, Princeton University, 4 Ivy Lane,
Princeton,
NJ
08544, USA
26
Observatoire de Genève, Université de Genève, 51 Ch. des Maillettes,
1290
Sauverny,
Switzerland
27
George Mason University, 4400 University Drive,
Fairfax, VA, 22030 USA
28
European Space Agency, ESTEC, Keplerlaan 1, 2201 AZ Noordwijk, The Netherlands
29
Department of Astronomy, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku,
Tokyo
113-0033, Japan
30
Department of Physics, United States Air Force Academy,
Colorado, CO
80840, USA
31
European Southern Observatory, Alonso de Córdova 3107,
Vitacura,
Región Metropolitana, Chile
32
Instituto de Astrofísica e Ciências do Espaço, Universidade do Porto, CAUP, Rua das Estrelas, 4150-762
Porto, Portugal
33
Centro Astronómico Hispano-Alemán, Observatorio de Calar Alto, Sierra de los Filabres,
04550
Gérgal, Spain
34
Department of Astronomy, Tsinghua University,
Beijing
100084, PR China
35
Department of Astronomy and Astrophysics, University of California, Santa Cruz, 1156 High St.
Santa Cruz, CA 95064, USA
36
Observatori Astronómic Albanyá, Camí de Bassegoda s/n,
Albanyá
17733, Girona, Spain
37
Subaru Telescope, 650 N. Aohoku Place,
Hilo, HI 96720, USA
38
Thüringer Landessternwarte Tautenburg, Sternwarte 5,
07778 Tautenburg, Germany
39
University of Hawaii, Institute for Astronomy, 640 N. Aohoku Place,
Hilo,
HI
96720, USA
40
National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka,
Tokyo
181-8588, Japan
41
Okayama Observatory, Kyoto University, 3037-5 Honjo, Kamogatacho, Asakuchi,
Okayama
719-0232, Japan
42
Deutsches Zentrum für Luft und Raumfahrt, Institut für Planetenforschung Rutherfordstrasse 2, 12489
Berlin, Germany
43
Department of Astronomical Science, The Graduated University for Advanced Studies, SOKENDAI, 2-21-1, Osawa, Mitaka, Tokyo 181-8588 Japan
44
Tokyo University of Agriculture and Technology, 3-8-1, Saiwai-cho, Fuchu,
Tokyo
183-0054, Japan
45
U.S. Naval Observatory, 3450 Massachusetts Avenue NW,
Washington, D.C.
20392, USA
46
Department of Astronomy, Institute for Astrophysical Research, Boston University, 725 Commonwealth Ave. Room 514, Boston, MA
02215, USA
47
Departamento de Física e Astronomia, Faculdade de Ciências, Universidade do Porto, Rua do Campo Alegre, 4169-007
Porto, Portugal
48
Patashnick Voorheesville Observatory,
Voorheesville,
NY
12186, USA
49
SETI Institute,
Mountain View, CA 94043, USA
Received:
18
July
2020
Accepted:
10
September
2020
We present the confirmation and characterisation of GJ 3473 b (G 50–16, TOI-488.01), a hot Earth-sized planet orbiting an M4 dwarf star, whose transiting signal (P = 1.1980035 ± 0.0000018 d) was first detected by the Transiting Exoplanet Survey Satellite (TESS). Through a joint modelling of follow-up radial velocity observations with CARMENES, IRD, and HARPS together with extensive ground-based photometric follow-up observations with LCOGT, MuSCAT, and MuSCAT2, we determined a precise planetary mass, Mb = 1.86 ± 0.30 M⊕, and radius, Rb = 1.264 ± 0.050 R⊕. Additionally, we report the discovery of a second, temperate, non-transiting planet in the system, GJ 3473 c, which has a minimum mass, Mc sin i = 7.41 ± 0.91 M⊕, and orbital period, Pc = 15.509 ± 0.033 d. The inner planet of the system, GJ 3473 b, is one of the hottest transiting Earth-sized planets known thus far, accompanied by a dynamical mass measurement, which makes it a particularly attractive target for thermal emission spectroscopy.
Key words: planetary systems / planets and satellites: detection / techniques: radial velocities / techniques: photometric / stars: late-type / stars: individual: G 50-16
RV data are only available at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/cat/J/A+A/642/A236
© ESO 2020
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