WASP-166b: a bloated super-Neptune transiting a V = 9 star

  • Coel Hellier
  • , D. R. Anderson
  • , A. H. M. J. Triaud
  • , F. Bouchy
  • , A. Burdanov
  • , A. Collier Cameron
  • , L. Delrez
  • , D. Ehrenreich
  • , M. Gillon
  • , E. Jehin
  • , M. Lendl
  • , E. Linder
  • , L. D. Nielsen
  • , P. F. L. Maxted
  • , F. Pepe
  • , D. Pollacco
  • , D. Queloz
  • , D. Segransan
  • , B. Smalley
  • , J. J. Spake
  • L. Y. Temple, S. Udry, R. G. West, A. Wyttenbach

Research output: Contribution to journalArticlepeer-review

7 Citations (Scopus)
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Abstract

We report the discovery of WASP-166b, a super-Neptune planet with a mass of 0.1 Mjup (1.9 Mnep) and a bloated radius of 0.63 Rjup. It transits a V = 9.36, F9V star in a 5.44-d orbit that is aligned with the stellar rotation axis (sky-projected obliquity angle lambda = 3 +/- 5 degrees). Variations in the radial-velocity measurements are likely the result of magnetic activity over a 12-d stellar rotation period. WASP-166b appears to be a rare object within the "Neptune desert".
Original languageEnglish
Pages (from-to)3067–3075
JournalMonthly Notices of the Royal Astronomical Society
Volume488
Issue number3
DOIs
Publication statusPublished - 10 Jul 2019

Keywords

  • astro-ph.EP
  • stars: individual: WASP-166

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