HIP 100917
HIP 100917 is a K-type (Orange) star.
At a distance of roughly 1,177 light-years, HIP 100917 is a distant star lying deep within the Milky Way galaxy.
HIP 100917 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 100917 has an apparent magnitude of +8.90, 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 +1.102.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.102 |
Observation
| Apparent Magnitude | +8.90 |
| Absolute Magnitude | 1.11 |
| Distance | 1,177 ly |
Position
| Right Ascension | 20h 27.68m |
| Declination | 21° 28.27′ |
Frequently Asked Questions
What type of star is HIP 100917?
HIP 100917 is a Class K — K-type (Orange) star.
How far is HIP 100917 from Earth?
HIP 100917 is approximately 1,177.5 light-years from Earth.
Can you see HIP 100917 with the naked eye?
With an apparent magnitude of 8.90, HIP 100917 is not visible to the naked eye.