HIP 105889
HIP 105889 is a K-type (Orange) star.
At a distance of roughly 1,000 light-years, HIP 105889 is a distant star lying deep within the Milky Way galaxy.
HIP 105889 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
At an apparent magnitude of +10.10, HIP 105889 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 red hue, which corresponds to a B-V color index of +1.545.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.545 |
Observation
| Apparent Magnitude | +10.10 |
| Absolute Magnitude | 2.67 |
| Distance | 1,000 ly |
Position
| Right Ascension | 21h 26.73m |
| Declination | 28° 22.86′ |
Frequently Asked Questions
What type of star is HIP 105889?
HIP 105889 is a Class K — K-type (Orange) star.
How far is HIP 105889 from Earth?
HIP 105889 is approximately 1,000.5 light-years from Earth.
Can you see HIP 105889 with the naked eye?
With an apparent magnitude of 10.10, HIP 105889 is not visible to the naked eye.