It is located at a distance of approximately 380 light years from the Sun based on parallax, and has an absolute magnitude of −0.53. The system is a probable member of the Sco OB2 association of co-moving stars. The visible component is a B-type main-sequence star with a stellar classification of B9V.
This celestial body is situated at a distance of around 380 light years from the Sun based on parallax, and it has an absolute magnitude of −0.53. It is part of the Sco OB2 group of stars moving together. The visible component is a B-type main-sequence star with a stellar classification of B9V.