| | 22 Mar. 2010: As Figueira et al. (2010) find "a clear correlation between radial-velocities and bisector span", indicating that "this evidence points towards a stellar origin of the radial-velocity variations of the star instead of a barycentric movement of the star, and repudiates the reported detection of a hot-Jupiter", this planet is (provisionnally?) marked as "controversial".
17 Dec. 2009: Herman Obispo et al (2010) give also a slightly different oribit with Mpl = 6.15 ± 0.6 MJup and e = 0.14 ± 0.4 |