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Kepler-11 is a Solar Twin : Revising the Masses and Radii of Benchmark Planets via Precise Stellar Characterization

Bedell, Megan (author)
University of Chicago
Bean, Jacob L. (author)
University of Chicago
Meléndez, Jorge (author)
University of São Paulo
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Mills, Sean M. (author)
University of Chicago
Fabrycky, Daniel C. (author)
University of Chicago
Freitas, Fabrício C. (author)
University of São Paulo
Ramírez, Ivan (author)
University of Texas
Asplund, Martin (author)
Australian National University
Liu, Fan (author)
Lund University,Lunds universitet,Astronomi - Har omorganiserats,Institutionen för astronomi och teoretisk fysik - Har omorganiserats,Naturvetenskapliga fakulteten,Lund Observatory - Has been reorganised,Department of Astronomy and Theoretical Physics - Has been reorganised,Faculty of Science,Australian National University
Yong, David (author)
Australian National University
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 (creator_code:org_t)
2017-04-20
2017
English.
In: Astrophysical Journal. - : American Astronomical Society. - 0004-637X .- 1538-4357. ; 839:2
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The six planets of the Kepler-11 system are the archetypal example of a population of surprisingly low-density transiting planets revealed by the Kepler mission. We have determined the fundamental parameters and chemical composition of the Kepler-11 host star to unprecedented precision using an extremely high-quality spectrum from Keck-HIRES (R ≃ 67,000, S/N per pixel at 600 nm). Contrary to previously published results, our spectroscopic constraints indicate that Kepler-11 is a young main-sequence solar twin. The revised stellar parameters and new analysis raise the densities of the Kepler-11 planets by between 20% and 95% per planet, making them more typical of the emerging class of "puffy" close-in exoplanets. We obtain photospheric abundances of 22 elements and find that Kepler-11 has an abundance pattern similar to that of the Sun with a slightly higher overall metallicity. We additionally analyze the Kepler light curves using a photodynamical model and discuss the tension between spectroscopic and transit/TTV-based estimates of stellar density.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

planets and satellites: fundamental parameters
stars: abundances
stars: fundamental parameters
techniques: spectroscopic

Publication and Content Type

art (subject category)
ref (subject category)

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