HIP 105259

HIP 105259 is a B-type (Blue-White) star.

At a distance of roughly 1,930 light-years, HIP 105259 is a distant star lying deep within the Milky Way galaxy.

HIP 105259 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.

With an apparent magnitude of +5.51, HIP 105259 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 orange hue, which corresponds to a B-V color index of +1.114.