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Search: L773:0004 6256 OR L773:1538 3881 > Nowak G. > K2-155: A Bright Me...

K2-155: A Bright Metal-poor M Dwarf with Three Transiting Super-Earths

Hirano, T. (author)
Dai, Fei (author)
Massachusetts Institute of Technology (MIT),Princeton University
Livingston, J.H. (author)
University of Tokyo, Japan
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Fujii, Yuka (author)
Tokyo Institute of Technology
Cochran, William D. (author)
The University of Texas at Austin, USA
Endl, M. (author)
The University of Texas at Austin, USA
Gandolfi, D. (author)
Universita degli Studi di Torino,University of Turin
Redfield, S. (author)
Wesleyan University
Joshua, N. (author)
Princeton University
Guenther, E. W. (author)
Thüringer Landessternwarte Tautenburg
Prieto-Arranz, J. (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Albrecht, Simon (author)
Århus Universitet,Aarhus University
Barragán, O. (author)
Universita degli Studi di Torino,University of Turin
Cabrera, J. (author)
Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Cauley, P.W. (author)
Arizona State University
Csizmadia, Szilard (author)
Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Deeg, H. (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Eigmüller, P. (author)
Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Erikson, Anders (author)
Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Fridlund, Malcolm, 1952 (author)
Universiteit Leiden (UL),Leiden University (UL),Chalmers tekniska högskola,Chalmers University of Technology
Fukui, A. (author)
National Astronomical Observatory of Japan
Grziwa, S. (author)
Universität zu Köln,University of Cologne
Hatzes, A. (author)
Thüringer Landessternwarte Tautenburg
Korth, Judith (author)
Universität zu Köln,University of Cologne
Narita, Norio (author)
University of Tokyo, Japan,National Astronomical Observatory of Japan,National Institutes of Natural Sciences (NINS)
Nespral, David (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Niraula, Prajwal (author)
Wesleyan University
Nowak, G. (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Pätzold, Martin (author)
Universität zu Köln,University of Cologne
Palle, Enric (author)
Instituto de Astrofísica de Canarias,Universidad de la Laguna,University of La Laguna
Persson, Carina, 1964 (author)
Chalmers tekniska högskola,Chalmers University of Technology
Rauer, H. (author)
Technische Universität Berlin,Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Ribas, I. (author)
Institut de Ciències de l'Espai (ICE) - CSIC,Institute of Space Sciences (ICE) - CSIC
Smith, Alexis M. S. (author)
Deutsches Zentrums für Luft- und Raumfahrt (DLR),German Aerospace Center (DLR)
Van Eylen, V. (author)
Universiteit Leiden (UL),Leiden University (UL)
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 (creator_code:org_t)
2018-02-23
2018
English.
In: Astronomical Journal. - : American Astronomical Society. - 1538-3881 .- 0004-6256. ; 155:3
  • Journal article (peer-reviewed)
Abstract Subject headings
Close  
  • We report on the discovery of three transiting super-Earths around K2-155 (EPIC 210897587), a relatively bright early M dwarf (V = 12.81 mag) observed during Campaign 13 of the NASA K2 mission. To characterize the system and validate the planet candidates, we conducted speckle imaging and high-dispersion optical spectroscopy, including radial velocity measurements. Based on the K2 light curve and the spectroscopic characterization of the host star, the planet sizes and orbital periods are 1.55 -0.17 +0.20 R ⊕ and 6.34365 ±0.00028 days for the inner planet; 1.95 -0.22 +0.27 R ⊕ and 13.85402 ±0.00088 days for the middle planet; and 1.64 -0.17 +0.18 R ⊕ and 40.6835 ±0.0031 days for the outer planet. The outer planet (K2-155d) is near the habitable zone, with an insolation 1.67 ±0.38 times that of the Earth. The planet's radius falls within the range between that of smaller rocky planets and larger gas-rich planets. To assess the habitability of this planet, we present a series of three-dimensional global climate simulations, assuming that K2-155d is tidally locked and has an Earth-like composition and atmosphere. We find that the planet can maintain a moderate surface temperature if the insolation proves to be smaller than ∼1.5 times that of the Earth. Doppler mass measurements, transit spectroscopy, and other follow-up observations should be rewarding, as K2-155 is one of the optically brightest M dwarfs known to harbor transiting planets.

Subject headings

NATURVETENSKAP  -- Geovetenskap och miljövetenskap -- Meteorologi och atmosfärforskning (hsv//swe)
NATURAL SCIENCES  -- Earth and Related Environmental Sciences -- Meteorology and Atmospheric Sciences (hsv//eng)
NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)
NATURVETENSKAP  -- Fysik -- Atom- och molekylfysik och optik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Atom and Molecular Physics and Optics (hsv//eng)

Keyword

techniques: radial velocities
techniques: photometric
techniques: spectroscopic
stars: individual (K2-155 = EPIC 210897587)
planets and satellites: detection

Publication and Content Type

art (subject category)
ref (subject category)

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