HIP 16209

HIP 16209 is a K-type (Orange) star located in the constellation Perseus.

Located approximately 83.0 light-years from Earth, HIP 16209 resides within the broader disk of our Milky Way galaxy.

HIP 16209 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.

At an apparent magnitude of +11.10, HIP 16209 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 orange hue, which corresponds to a B-V color index of +1.314.