K2-141 b: A 5- M super-Earth transiting a K7 v star every 6.7 h

  • O. Barragán
  • , D. Gandolfi
  • , F. Dai
  • , J. Livingston
  • , C. M. Persson
  • , T. Hirano
  • , N. Narita
  • , Sz Csizmadia
  • , J. N. Winn
  • , D. Nespral
  • , J. Prieto-Arranz
  • , A. M.S. Smith
  • , G. Nowak
  • , S. Albrecht
  • , G. Antoniciello
  • , A. Bo Justesen
  • , J. Cabrera
  • , W. D. Cochran
  • , H. Deeg
  • , Ph Eigmuller
  • M. Endl, A. Erikson, M. Fridlund, A. Fukui, S. Grziwa, E. Guenther, A. P. Hatzes, D. Hidalgo, M. C. Johnson, J. Korth, E. Palle, M. Patzold, H. Rauer, Y. Tanaka, V. Van Eylen

Research output: Contribution to journalArticlepeer-review

54 Scopus citations

Abstract

We report on the discovery of K2-141 b (EPIC 246393474 b), an ultra-short-period super-Earth on a 6.7 h orbit transiting an active K7 V star based on data from K2 campaign 12. We confirmed the planet's existence and measured its mass with a series of follow-up observations: seeing-limited Muscat imaging, NESSI high-resolution speckle observations, and FIES and HARPS high-precision radial-velocity monitoring. K2-141 b has a mass of 5.31 ± 0.46 M and radius of 1.54-0.09+0.10 R, yielding a mean density of 8.00-1.45+1.83 g cm-3 and suggesting a rocky-iron composition. Models indicate that iron cannot exceed ∼70% of the total mass. With an orbital period of only 6.7 h, K2-141 b is the shortest-period planet known to date with a precisely determined mass.

Original languageEnglish (US)
Article numberA95
JournalAstronomy and Astrophysics
Volume612
DOIs
StatePublished - Apr 1 2018

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics
  • Space and Planetary Science

Keywords

  • Planetary systems
  • Planets and satellites: individual: EPIC 246393474 b
  • Stars: fundamental parameters
  • Stars: individual: EPIC 246393474
  • Techniques: photometric
  • Techniques: radial velocities

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