The sub-Jupiter mass transiting exoplanet WASP-11b
Abstract
We report the discovery of a sub-Jupiter mass exoplanet transiting a magnitude {V} = 11.6 host star 1SWASP J030928.54+304024.7. A simultaneous fit to the transit photometry and radial-velocity measurements yield a planet mass Mp = 0.53 ± 0.07 {M_J}, radius Rp = 0.91+0.06-0.03 {R_J} and an orbital period of 3.722465^+0.000006-0.000008 days. The host star is an early to mid-K dwarf, with a spectral analysis yielding an effective temperature of 4800 ± 100 K and log g = 4.45 ± 0.2. It is amongst the smallest, least massive and lowest luminosity stars known to harbour a transiting exoplanet. WASP-11b is the third least strongly irradiated transiting exoplanet discovered to date, experiencing an incident flux Fp = 1.9×108 erg s-1 cm-2 and having an equilibrium temperature T_eql = 960 ± 70 K.
Photometric measurements and Table 2 are available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/502/395- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- July 2009
- DOI:
- 10.1051/0004-6361/200810973
- arXiv:
- arXiv:0809.4597
- Bibcode:
- 2009A&A...502..395W
- Keywords:
-
- stars: individual: WASP-11;
- planetary systems;
- techniques: photometric;
- techniques: radial velocities;
- techniques: spectroscopic;
- Astrophysics
- E-Print:
- Submitted to A&