HIP 10869
HIP 10869 is a K-type (Orange) star.
At a distance of roughly 1,279 light-years, HIP 10869 is a distant star lying deep within the Milky Way galaxy.
HIP 10869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10869 has an apparent magnitude of +8.96, 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 +1.075.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.075 |
Observation
| Apparent Magnitude | +8.96 |
| Absolute Magnitude | 0.99 |
| Distance | 1,279 ly |
Position
| Right Ascension | 2h 19.88m |
| Declination | -10° 23.15′ |
Frequently Asked Questions
What type of star is HIP 10869?
HIP 10869 is a Class K — K-type (Orange) star.
How far is HIP 10869 from Earth?
HIP 10869 is approximately 1,279.0 light-years from Earth.
Can you see HIP 10869 with the naked eye?
With an apparent magnitude of 8.96, HIP 10869 is not visible to the naked eye.