HIP 106869
HIP 106869 is a K-type (Orange) star.
At a distance of roughly 1,406 light-years, HIP 106869 is a distant star lying deep within the Milky Way galaxy.
HIP 106869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 106869 has an apparent magnitude of +7.23, 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 +1.646.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.646 |
Observation
| Apparent Magnitude | +7.23 |
| Absolute Magnitude | -0.94 |
| Distance | 1,406 ly |
Position
| Right Ascension | 21h 38.69m |
| Declination | 64° 23.14′ |
Frequently Asked Questions
What type of star is HIP 106869?
HIP 106869 is a Class K — K-type (Orange) star.
How far is HIP 106869 from Earth?
HIP 106869 is approximately 1,405.8 light-years from Earth.
Can you see HIP 106869 with the naked eye?
With an apparent magnitude of 7.23, HIP 106869 is not visible to the naked eye.