HIP 31992

HIP 31992 is a B-type (Blue-White) star.

At a distance of roughly 1,254 light-years, HIP 31992 is a distant star lying deep within the Milky Way galaxy.

HIP 31992 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

With an apparent magnitude of +5.79, HIP 31992 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its blue hue, which corresponds to a B-V color index of -0.094.