HIP 10217
HIP 10217 is a K-type (Orange) star.
At a distance of roughly 1,087 light-years, HIP 10217 is a distant star lying deep within the Milky Way galaxy.
HIP 10217 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10217 has an apparent magnitude of +8.21, 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 yellow hue, which corresponds to a B-V color index of +0.938.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 0.938 |
Observation
| Apparent Magnitude | +8.21 |
| Absolute Magnitude | 0.60 |
| Distance | 1,087 ly |
Position
| Right Ascension | 2h 11.38m |
| Declination | 1° 40.96′ |
Frequently Asked Questions
What type of star is HIP 10217?
HIP 10217 is a Class K — K-type (Orange) star.
How far is HIP 10217 from Earth?
HIP 10217 is approximately 1,087.2 light-years from Earth.
Can you see HIP 10217 with the naked eye?
With an apparent magnitude of 8.21, HIP 10217 is not visible to the naked eye.