Issue |
A&A
Volume 636, April 2020
|
|
---|---|---|
Article Number | A89 | |
Number of page(s) | 13 | |
Section | Planets and planetary systems | |
DOI | https://doi.org/10.1051/0004-6361/201937080 | |
Published online | 24 April 2020 |
Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M⊕ super-Earth and two warm 14.7 and 10.2-M⊕ sub-Neptunes★,★★
1
Instituto de Astrofisica de Canarias,
Tenerife,
Spain
e-mail: dhidalgo@iac.es
2
Departamento de Astrofísica Universidad de La Laguna,
Tenerife,
Spain
3
Dipartimento di Fisica, Università degli Studi di Torino,
Torino,
Italy
4
Department of Space, Earth and Environment, Chalmers University of Technology, Onsala Space Observatory,
439 92
Onsala,
Sweden
5
Leiden Observatory, University of Leiden,
Leiden,
The Netherlands
6
Department of Earth and Planetary Sciences, Tokyo Institute of Technology,
2-12-1 Ookayama, Meguro-ku,
Tokyo
152-8551,
Japan
7
Department of Astronomy, Graduate School of Science, The University of Tokyo,
Hongo 7-3-1,
Bunkyo-ku,
Tokyo
113-0033,
Japan
8
JST, PRESTO,
2-21-1 Osawa,
Mitaka,
Tokyo
181-8588,
Japan
9
Astrobiology Center, NINS,
2-21-1 Osawa,
Mitaka,
Tokyo
181-8588,
Japan
10
National Astronomical Observatory of Japan, NINS,
2-21-1 Osawa,
Mitaka,
Tokyo
181-8588,
Japan
11
Stellar Astrophysics Centre, Deparment of Physics and Astronomy, Aarhus University,
Ny Munkegrade 120,
8000
Aarhus C,
Denmark
12
Department of Astronomy and McDonald Observatory, University of Texas at Austin,
2515 Speedway, Stop C1400,
Austin,
TX
78712,
USA
13
Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology,
Cambridge,
MA,
02139,
USA
14
Department of Astrophysical Sciences, Princeton University,
4 Ivy Lane,
Princeton,
NJ,
08544,
USA
15
Astronomy Department and Van Vleck Observatory, Wesleyan University,
Middletown,
CT
06459,
USA
16
Institute of Planetary Research, German Aerospace Center,
Rutherfordstrasse 2,
12489
Berlin,
Germany
17
Center for Astronomy and Astrophysics, TU Berlin,
Hardenbergstr. 36,
10623
Berlin,
Germany
18
Thüringer Landessternwarte Tautenburg,
Sternwarte 5,
07778
Tautenburg,
Germany
19
Rheinisches Institut für Umweltforschung, Abteilung Planetenforschung an der Universität zu Köln,
Aachener Strasse 209,
50931
Köln,
Germany
20
Institute of Geological Sciences, Freie Universität Berlin,
Malteserstr. 74-100,
12249
Berlin,
Germany
21
Hamburger Sternwarte,
Gojenbergsweg 112,
21029
Hamburg,
Germany
22
Institut de Ciències de l’Espai (ICE, CSIC),
Campus UAB, C/ de Can Magrans s/n,
08193
Bellaterra,
Spain
23
Institut d’Estudis Espacials de Catalunya (IEEC),
C/ Gran Capità 2-4,
08034
Barcelona,
Spain
24
Monash Centre for Astrophysics, School of Physics and Astronomy, Monash University,
VIC
3800,
Australia
25
European Southern Observatory (ESO),
Alonso de Córdova 3107, Vitacura,
Casilla
19001,
Santiago de Chile,
Chile
26
Mullard Space Science Laboratory, University College London,
Holmbury St Mary,
Dorking,
Surrey
RH5 6NT,
UK
27
Sub-department of Astrophysics, Department of Physics, University of Oxford,
Oxford
OX1 3RH,
UK
28
Astronomical Institute of the Czech Academy of Sciences,
Fričova 298,
25165
Ondřejov,
Czech Republic
29
Astronomical Institute of Charles University,
V Holešovičkách 2,
180 00
Praha,
Czech Republic
30
Centro de Astrobiología (CSIC-INTA), ESAC,
camino bajo del castillo s/n,
28692
Villanueva de la Cañada,
Madrid Spain
31
Institut für Astrophysik, Georg-August-Universität,
Friedrich-Hund-Platz 1,
37077
Göttingen,
Germany
32
Zentrum für Astronomie der Universtät Heidelberg,
Landessternwarte, Königstuhl 12,
69117
Heidelberg,
Germany
33
Instituto de Astrofísica de Andalucía (IAA-CSIC),
Glorieta de la Astronomía s/n,
18008
Granada,
Spain
34
Centre for Exoplanets and Habitability, University of Warwick,
Gibbet Hill Road,
Coventry,
CV4 7AL,
UK
35
Department of Physics, University of Warwick,
Gibbet Hill Road,
Coventry,
CV4 7AL,
UK
36
European Southern Observatory,
Alonso de Córdova 3107,
Vitacura,
Casilla 19001,
Santiago 19,
Chile
37
Instituto de Astrofísica e Ciências do Espaço, CAUP, Universidade do Porto, Rua das Estrelas,
4150-762
Porto,
Portugal
38
Departamento de Física, Universidade Federal do Rio Grande do Norte,
59078-970
Natal,
RN,
Brazil
39
Geneva Observatory, University of Geneva,
Chemin des Mailettes 51,
1290
Versoix,
Switzerland
40
Center for Space and Habitability, Universität Bern,
Gesellschaftsstrasse 6,
3012
Bern,
Switzerland
Received:
7
November
2019
Accepted:
29
January
2020
We report the discovery of a new planetary system with three transiting planets, one super-Earth and two sub-Neptunes, that orbit EPIC 249893012, a G8 IV-V evolved star (M⋆ = 1.05 ± 0.05 M⊙, R⋆ = 1.71 ± 0.04 R⊙, Teff = 5430 ± 85 K). The star is just leaving the main sequence. We combined K2 photometry with IRCS adaptive-optics imaging and HARPS, HARPS-N, and CARMENES high-precision radial velocity measurements to confirm the planetary system, determine the stellar parameters, and measure radii, masses, and densities of the three planets. With an orbital period of 3.5949−0.0007+0.0007 days, a mass of 8.75−1.08+1.09 M⊕, and a radius of 1.95−0.08+0.09 R⊕, the inner planet b is compatible with nickel-iron core and a silicate mantle (ρb = 6.39−1.04+1.19 g cm−3). Planets c and d with orbital periods of 15.624−0.001+0.001 and 35.747−0.005+0.005 days, respectively, have masses and radii of 14.67−1.89+1,84 M⊕ and 3.67−0.14+0.17 R⊕ and 10.18−2.42+2.46 M⊕ and 3.94−0.12+0.13 R⊕, respectively, yielding a mean density of 1.62−0.29+0.30 and 0.91−0.23+0.25 g cm−3, respectively. The radius of planet b lies in the transition region between rocky and gaseous planets, but its density is consistent with a rocky composition. Its semimajor axis and the corresponding photoevaporation levels to which the planet has been exposed might explain its measured density today. In contrast, the densities and semimajor axes of planets c and d suggest a very thick atmosphere. The singularity of this system, which orbits a slightly evolved star that is just leaving the main sequence, makes it a good candidate for a deeper study from a dynamical point of view.
Key words: planetary systems / planets and satellites: detection / techniques: photometric / techniques: radial velocities / planets and satellites: fundamental parameters
Based on observations made with the ESO-3.6m telescope at La Silla Observatory (Chile) under programs 0101.C-0829, 1102.C-0923, and 60.A-9700.
Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Istituto Nazionale di Astrofisica) at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias, under programs CAT18A_130, CAT18B_93, and A37TAC_37.
© ESO 2020
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