The distance to this star can be estimated through parallax measurements, which yield a separation of 165.6 light years from the Sun.
The photometric distance estimate for this object is 153 ± 31 ly (46.9 ± 9.5 pc), matching the primary within the margin of error.
[9] A Jovian planetary companion to this star was announced in 2005, based on radial velocity measurements indicating a periodic perturbation.
The inclination of the orbital plane remains unknown, so only a lower bound on the planet's mass can be determined.
[8] The orbital path of this object intersects the habitable zone of the star, which is likely to eject any Earth-like planet from that region.