2D projections of the UVW space velocities compared to well known moving groups, including TWA. The dashed grey box is taken from Zuckerman & Song (2004) and shows the region of UVW space typically occupied by nearby young stars. The UVW velocities of the young moving groups are taken from Malo et al. (2013), the 2σ uncertainties are plotted. HD 102077 is clearly not a member of any of these groups.