WASP-4b: A 12th Magnitude Transiting Hot Jupiter in the Southern Hemisphere
Abstract
We report the discovery of WASP-4b, a large transiting gas-giant planet with an orbital period of 1.34 days. This is the first planet to be discovered by the SuperWASP-South observatory and CORALIE collaboration and the first planet orbiting a star brighter than 16th magnitude to be discovered in the southern hemisphere. A simultaneous fit to high-quality light curves and precision radial velocity measurements leads to a planetary mass of 1.22+ 0.09-0.08 MJup and a planetary radius of 1.42+ 0.07-0.04 RJup. The host star is USNO-B1.0 0479-0948995, a G7 V star of visual magnitude 12.5. As a result of the short orbital period, the predicted surface temperature of the planet is 1761 K, making it an ideal candidate for detections of the secondary eclipse at infrared wavelengths.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- March 2008
- DOI:
- 10.1086/586735
- arXiv:
- arXiv:0801.1509
- Bibcode:
- 2008ApJ...675L.113W
- Keywords:
-
- planetary systems;
- stars: individual: WASP-4;
- Astrophysics
- E-Print:
- Added 3 new RV measurements and resultant fit parameters updated. Minor revisions to text. 7 pages incl. 4 figures. Accepted for publication in ApJL