With an apparent visual magnitude of 3.2, it is the fourth-brightest star in the constellation. The distance to this star has been measured using the parallax technique, yielding an estimate of roughly 900 light-years with a 15% margin of error.
With a visual magnitude of 3.2, it ranks as the fourth most luminous star within its constellation. The measurement of its distance was accomplished through the application of the parallax technique, yielding a calculated distance of roughly 900 light-years with an associated error margin of 15%.