HD 185269 b

HD 185269 b is a hot Jupiter extrasolar planet approximately 170 light years away^[4] in the constellation of Cygnus. The minimum mass is slightly less than Jupiter and the orbital period is about one week. Most hot Jupiters are thought to have undergone tidal circularization, making the eccentricity of HD 185269 b (e=0.3) unusual. Despite having a large transit probability, none have yet been detected by various photometric monitoring campaigns.

HD 192699 b

Discovery[1][2]
Discovered by	Moutou et al. and Johnson et al.
Discovery site	Observatoire de Haute Provence and Lick Observatory
Discovery date	2006
Detection method	Doppler spectroscopy
Orbital characteristics[3]
Semi-major axis	0.0770±0.0034 AU
Eccentricity	0.229±0.014
Orbital period (sidereal)	6.83776±0.00027 d
Time of perihelion	2453154.25±0.11 JD
Argument of perihelion	176.2±3.5 º
Semi-amplitude	93.3±1.4 m/s
Star	HD 185269
Physical characteristics[3]
Mass	≥1.010±0.014 MJ

The planet was discovered nearly simultaneously by Johnson et al. as part of a search for planets around subgiants, and by Moutou et al. as part of a search for planets around metal-rich stars (the submission dates to the journals ApJ and Astronomy and Astrophysics were separated by only 9 days).^[1][2]