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korth

Judith Korth

Postdoc

korth

K2-139 b : A low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star

Author

  • O. Barragán
  • D. Gandolfi
  • A. M.S. Smith
  • H. J. Deeg
  • M. C.V. Fridlund
  • C. M. Persson
  • P. Donati
  • M. Endl
  • Sz Csizmadia
  • S. Grziwa
  • D. Nespral
  • A. P. Hatzes
  • W. D. Cochran
  • L. Fossati
  • S. S. Brems
  • J. Cabrera
  • F. Cusano
  • Ph Eigmüller
  • C. Eiroa
  • A. Erikson
  • E. Guenther
  • J. Korth
  • D. Lorenzo-Oliveira
  • L. Mancini
  • M. Pätzold
  • J. Prieto-Arranz
  • H. Rauer
  • I. Rebollido
  • J. Saario
  • O. V. Zakhozhay

Summary, in English

We announce the discovery of K2-139 b (EPIC 218916923 b), a transiting warm-Jupiter (Teq = 547± 25 K) on a 29-d orbit around an active (logR' HK =-4.46±0.06) K0V star in K2 Campaign 7.We derive the system's parameters by combining the K2 photometry with groundbased follow-up observations. With a mass of 0.387 -0.033+0.075 MJ and radius of 0.808 -0.033+0.034 RJ, K2-139 b is one of the transiting warm Jupiters with the lowest mass known to date. The planetary mean density of 0.91 -0.20+0.24 g cm-3can be explained with a core of ~50M. Given the brightness of the host star (V=11.653 mag), the relatively short transit duration (~5 h), and the expected amplitude of the Rossiter-McLaughlin effect (~25m s-1), K2-139 is an ideal target to measure the spin-orbit angle of a planetary system hosting a warm Jupiter.

Publishing year

2018-04-01

Language

English

Pages

1765-1776

Publication/Series

Monthly Notices of the Royal Astronomical Society

Volume

475

Issue

2

Document type

Journal article

Publisher

Oxford University Press

Keywords

  • Planetary systems
  • Planets and satellites: detection
  • Planets and satellites: individual: K2-139 b (EPIC 218916923b)
  • Stars: fundamental parameters

Status

Published

ISBN/ISSN/Other

  • ISSN: 0035-8711