[2] Based upon an annual parallax shift of 24.14 mas as seen from Earth, it is located 135 light-years from the Sun.

[6] Beta Pavonis is a member of the Ursa Major Moving Group, a set of stars that share a similar motion through space.

However, Houk (1979) listed a more evolved class of A7 III,[4] suggesting it is already a giant star.

At the estimated age of 305[8] million years, the star still has a relatively high rate of spin, having a projected rotational velocity of 75 km/s.

[3] Beta Pavonis is radiating 66[3] times the Sun's luminosity from its photosphere at an effective temperature of about 8,184 K.[8]