HIP 13275

HIP 13275 is a K-type (Orange) star located in the constellation Perseus.

Located approximately 736.2 light-years from Earth, HIP 13275 resides within the broader disk of our Milky Way galaxy.

HIP 13275 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.

HIP 13275 has an apparent magnitude of +6.51, 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 red hue, which corresponds to a B-V color index of +1.476.