Based upon the position and movement of this star through space, it is a likely member of the Gould Belt. In particular, it belongs to the Lower Centaurus–Crux (LCC) group of the Scorpius–Centaurus association, which is the nearest OB association to the Sun.
Given the star's position and movement through space, it is likely that it is a member of the Gould Belt. More specifically, it belongs to the Lower Centaurus–Crux (LCC) subgroup within the Scorpius–Centaurus association, which is the nearest OB group to our Sun.