HIP 20239

HIP 20239 is a B-type (Blue-White) star located in the constellation Perseus.

At a distance of roughly 1,568 light-years, HIP 20239 is a distant star lying deep within the Milky Way galaxy.

HIP 20239 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

At an apparent magnitude of +10.29, HIP 20239 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its white hue, which corresponds to a B-V color index of +0.364.