HIP 5225

HIP 5225 is a K-type (Orange) star.

At a distance of roughly 1,989 light-years, HIP 5225 is a distant star lying deep within the Milky Way galaxy.

HIP 5225 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.

HIP 5225 has an apparent magnitude of +8.83, placing it beyond naked-eye visibility. A good pair of binoculars or a small telescope is required to observe this star. Observers will note its orange hue, which corresponds to a B-V color index of +1.123.