Wasp-7: A Bright Transiting-Exoplanet System in the Southern Hemisphere
Abstract
We report that a Jupiter-mass planet, WASP-7b, transits the V = 9.5 star HD 197286 every 4.95 d. This is the brightest discovery from the WASP-South transit survey so far and is currently the brightest transiting-exoplanet system in the southern hemisphere. WASP-7b is among the densest of the known Jupiter-mass planets, suggesting that it has a massive core. The planet mass is 0.96+0.12 -0.18 M Jup, the radius is 0.915+0.046 -0.040 R Jup, and the density is 1.26+0.25 -0.21 ρJup (1.67+0.33 -0.28 g cm-3).
- Publication:
-
The Astrophysical Journal
- Pub Date:
- January 2009
- DOI:
- 10.1088/0004-637X/690/1/L89
- arXiv:
- arXiv:0805.2600
- Bibcode:
- 2009ApJ...690L..89H
- Keywords:
-
- stars: individual: WASP-7 HD 197286;
- planetary systems;
- Astrophysics
- E-Print:
- Astrophys.J.Lett.690:L89-L91,2009