 This trajectory and the location of the system suggests that it may be a member of the TW Hydrae association of stars that share a common origin.A low-mass member of this association, identified as 2MASS J12354893−3950245, may be a tertiary component of the HR 4796 system.It has a proper motion matching HR 4796, suggesting it is gravitationally bound to the other two stars, and is separated from the pair by a distance of about 13,500 AU.