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 ± 0.03 MJup and radius of 1.32 ± 0.08 R Jup. The host star, WASP-26, has a mass of 1.12 ± 0.03 M and a radius of 1.34 ± 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 ± 15 pc and an age of 6 ± 2 Gy.
Original language | English |
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Article number | A56 |
Pages (from-to) | 1-4 |
Number of pages | 4 |
Journal | Astronomy and Astrophysics |
Volume | 520 |
Issue number | 9 |
DOIs | |
Publication status | Published - 4 Oct 2010 |
Keywords
- binaries: visual
- planets and satellites: general
- stars: individual: WASP-26
- techniques: photometric
- techniques: radial velocities
- techniques: spectroscopic