Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...720..337s&link_type=abstract
The Astrophysical Journal, Volume 720, Issue 1, pp. 337-343 (2010).
Astronomy and Astrophysics
Astronomy
10
Planetary Systems
Scientific paper
We report the discovery of a new transiting close-in giant planet, WASP-24 b, in a 2.341 day orbit, 0.037 AU from its F8-9 type host star. By matching the star's spectrum with theoretical models, we infer an effective temperature T eff = 6075 ± 100 K and a surface gravity of log g = 4.15 ± 0.10. A comparison of these parameters with theoretical isochrones and evolutionary mass tracks places only weak constraints on the age of the host star, which we estimate to be 3.8+1.3 -1.2 Gyr. The planetary nature of the companion was confirmed by radial velocity measurements and additional photometric observations. These data were fit simultaneously in order to determine the most probable parameter set for the system, from which we infer a planetary mass of 1.071+0.036 -0.038 M Jup and radius 1.3+0.039 -0.037 R Jup.
Anderson David R.
Barros Susana C. C.
Bentley Sean J.
Bento Joao
Cathaway-Kjontvedt P.
No associations
LandOfFree
WASP-24 b: A New Transiting Close-in Hot Jupiter Orbiting a Late F-star does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with WASP-24 b: A New Transiting Close-in Hot Jupiter Orbiting a Late F-star, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and WASP-24 b: A New Transiting Close-in Hot Jupiter Orbiting a Late F-star will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1557441