HIP 101870
HIP 101870 is a K-type (Orange) star.
At a distance of roughly 2,038 light-years, HIP 101870 is a distant star lying deep within the Milky Way galaxy.
HIP 101870 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +5.91, HIP 101870 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its yellow hue, which corresponds to a B-V color index of +0.953.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 0.953 |
Observation
| Apparent Magnitude | +5.91 |
| Absolute Magnitude | -3.07 |
| Distance | 2,038 ly |
Position
| Right Ascension | 20h 38.58m |
| Declination | 23° 40.83′ |
Frequently Asked Questions
What type of star is HIP 101870?
HIP 101870 is a Class K — K-type (Orange) star.
How far is HIP 101870 from Earth?
HIP 101870 is approximately 2,038.5 light-years from Earth.
Can you see HIP 101870 with the naked eye?
With an apparent magnitude of 5.91, HIP 101870 is visible to the naked eye.