WASP-26b: a 1-Jupiter-mass planet around an early-G-type star

B. Smalley, D.~R. Anderson, A. Collier Cameron, M. Gillon, C. Hellier, T.~A. Lister, P.~F.~L. Maxted, D. Queloz, A.~H.~M.~J. Triaud, R.~G. West, S.~J. Bentley, B. Enoch, F. Pepe, D.~L. Pollacco, D. Segransan, A.~M.~S. Smith, J. Southworth, S. Udry, P.~J. Wheatley, P.~L. WoodJ. Bento

Research output: Contribution to journalArticlepeer-review

18 Citations (Scopus)

Abstract

We report the discovery of WASP-26b, a moderately over-sized Jupiter-mass exoplanet transiting its 11.3-mag early-G-type host star (1SWASP J001824.70-151602.3; TYC 5839-876-1) every 2.7566 days. A simultaneous fit to transit photometry and radial-velocity measurements yields a planetary mass of 1.02 plusmn 0.03 M$_Jup$ and radius of 1.32 plusmn 0.08 R$_Jup$. The host star, WASP-26, has a mass of 1.12 plusmn 0.03 M$_⊙$ and a radius of 1.34 plusmn 0.06 R$_⊙$ and is in a visual double with a fainter K-type star. The two stars are at least a common-proper motion pair with a common distance of around 250 plusmn 15 pc and an age of 6 plusmn 2 Gy. RV and photometric data are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/520/A56
Original languageEnglish
Pages (from-to)A56
JournalAstronomy and Astrophysics
Volume520
DOIs
Publication statusPublished - 1 Sept 2010

Keywords

  • planets and satellites: general, stars: individual: WASP-26, binaries: visual, techniques: photometric, techniques: spectroscopic, techniques: radial velocities

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