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Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization

文献类型:期刊论文

作者Luque, R.1,2; Palle, E.1,2; Kossakowski, D.3; Dreizler, S.4; Kemmer, J.5; Espinoza, N.3; Burt, J.6; Anglada-Escude, G.7,8; Bejar, V. J. S.1,2; Caballero, J. A.9
刊名ASTRONOMY & ASTROPHYSICS
出版日期2019-08-06
卷号628页码:18
ISSN号1432-0746
关键词planetary systems techniques: photometric techniques: radial velocities stars: individual: G1 357 stars: late-type
DOI10.1051/0004-6361/201935801
通讯作者Luque, R.(rluque@iac.es)
英文摘要We report the detection of a transiting Earth-size planet around GJ 357, a nearby M2.5 V star, using data from the Transiting Exoplanet Survey Satellite (TESS). GJ 357 b (TOI-562.01) is a transiting, hot, Earth-sized planet (T-eq = 525 +/- 11 K) with a radius of R-b = 1.217 +/- 0.084 R-circle plus and an orbital period of P-b = 3.93 d. Precise stellar radial velocities from CARMENES and PFS, as well as archival data from HIRES, UVES, and HARPS also display a 3.93-day periodicity, confirming the planetary nature and leading to a planetary mass of M-b = 1.84 +/- 0.31 M-circle plus. In addition to the radial velocity signal for GJ 357 b, more periodicities are present in the data indicating the presence of two further planets in the system: GJ 357 c, with a minimum mass of M-c = 3.40 +/- 0.46 M-circle plus in a 9.12 d orbit, and GJ 357 d, with a minimum mass of M-d = 6.1 +/- 1.0 M-circle plus in a 55.7 d orbit inside the habitable zone. The host is relatively inactive and exhibits a photometric rotation period of P-rot = 78 +/- 2 d. GJ 357 b is to date the second closest transiting planet to the Sun, making it a prime target for further investigations such as transmission spectroscopy. Therefore, GJ 357 b represents one of the best terrestrial planets suitable for atmospheric characterization with the upcoming JWST and ground-based ELTs.
WOS关键词ECHELLE SPECTROMETER ; BAYESIAN-INFERENCE ; ERROR-CORRECTION ; GIANT PLANETS ; MASS ; PRECISION ; EXOPLANET ; SKY ; SEARCH ; STARS
WOS研究方向Astronomy & Astrophysics
语种英语
出版者EDP SCIENCES S A
WOS记录号WOS:000479054700001
源URL[http://libir.pmo.ac.cn/handle/332002/28047]  
专题中国科学院紫金山天文台
通讯作者Luque, R.
作者单位1.Inst Astrofis Canarias, Tenerife 38205, Spain
2.Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain
3.Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany
4.Georg August Univ, Inst Astrophys, Friedrich Hund Pl 1, D-37077 Gottingen, Germany
5.Heidelberg Univ, Landessternwarte, Zentrum Astron, Konigstuhl 12, D-69117 Heidelberg, Germany
6.MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA
7.Queen Mary Univ London, Sch Phys & Astron, 327 Mile End Rd, London E1 4NS, England
8.CSIC, IAA, Glorieta Astron S-N, E-18008 Granada, Spain
9.ESAC, CSIC, Ctr Astrobiol, INTA, Camino Bajo Castillo S-N, Madrid 28692, Spain
10.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
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Luque, R.,Palle, E.,Kossakowski, D.,et al. Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization[J]. ASTRONOMY & ASTROPHYSICS,2019,628:18.
APA Luque, R..,Palle, E..,Kossakowski, D..,Dreizler, S..,Kemmer, J..,...&Wohler, B..(2019).Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization.ASTRONOMY & ASTROPHYSICS,628,18.
MLA Luque, R.,et al."Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization".ASTRONOMY & ASTROPHYSICS 628(2019):18.

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