WASP-26b: A 1-Jupiter-mass planet around an early-G-type star
arXiv:1004.1542 · doi:10.1051/0004-6361/201014705
Abstract
We report the discovery of WASP-26b, a moderately over-sized Jupiter-mass exoplanet transiting its 11.3-magnitude 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 M_Jup and radius of 1.32 +/- 0.08 R_Jup. The host star, WASP-26, has a mass of 1.12 +/- 0.03 M_sun and a radius of 1.34 +/- 0.06 R_sun 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.
4 pages, 5 figure, submitted to A&A
References in corpus (12)
- Accurate masses and radii of normal stars: modern results and applications
- Detection of Thermal Emission from an Extrasolar Planet
- Efficient identification of exoplanetary transit candidates from SuperWASP light curves
- The Third US Naval Observatory CCD Astrograph Catalog (UCAC3)
- WASP-3b: a strongly-irradiated transiting gas-giant planet
- A fast hybrid algorithm for exoplanetary transit searches
- Properties of planets in binary systems. The role of binary separation
- Improved parameters for the transiting hot Jupiters WASP-4b and WASP-5b
- Homogeneous studies of transiting extrasolar planets. II. Physical properties
- An Improved Method for Estimating the Masses of Stars with Transiting Planets
- HAT-P-5b: A Jupiter-like hot Jupiter Transiting a Bright Star
- HAT-P-6b: A Hot Jupiter transiting a bright F star
Cited by in corpus (23)
- Obliquities of Hot Jupiter host stars: Evidence for tidal interactions and primordial misalignments
- The Mass of KOI-94d and a Relation for Planet Radius, Mass, and Incident Flux
- Determining stellar macroturbulence using asteroseismic rotational velocities from Kepler
- Evidence of an Upper Bound on the Masses of Planets and its Implications for Giant Planet Formation
- New and updated stellar parameters for 90 transit hosts. The effect of the surface gravity
- Constraining Tidal Dissipation in Stars from The Destruction Rates of Exoplanets
- TESS Transit Timing of Hundreds of Hot Jupiters
- Tidal Dissipation and Obliquity Evolution in Hot Jupiter Systems
- ExoClock Project III: 450 new exoplanet ephemerides from ground and space observations
- A simple model of the reflection effect for the interacting binaries and extrasolar planets
- High-precision photometry by telescope defocussing. VI. WASP-24, WASP-25 and WASP-26
- HAT-P-65b and HAT-P-66b: Two Transiting Inflated Hot Jupiters and Observational Evidence for the Re-Inflation of Close-In Giant Planets
- ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides
- Obliquities of Exoplanet Host Stars: 19 New and Updated Measurements, and Trends in the Sample of 205 Measurements
- ExoClock Project: An open platform for monitoring the ephemerides of Ariel targets with contributions from the public
- Colour-magnitude diagrams of transiting Exoplanets - II. A larger sample from photometric distances
- Tidally Distorted Exoplanets: Density Corrections for Short-Period Hot-Jupiters based solely on Observable Parameters
- Spin-orbit measurements and refined parameters for the exoplanet systems WASP-22 and WASP-26
- WASP-32b: A transiting hot Jupiter planet orbiting a lithium-poor, solar-type star
- High-resolution Imaging of Transiting Extrasolar Planetary systems (HITEP). II. Lucky Imaging results from 2015 and 2016
- UBV(RI)_C photometry of transiting planet host stars
- Warm Spitzer Occultation Photometry of WASP-26b at 3.6μm and 4.5μm
- Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities