HIP 9317
HIP 9317 is a K-type (Orange) star.
At a distance of roughly 1,069 light-years, HIP 9317 is a distant star lying deep within the Milky Way galaxy.
HIP 9317 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9317 has an apparent magnitude of +9.20, 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 +1.517.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.517 |
Observation
| Apparent Magnitude | +9.20 |
| Absolute Magnitude | 1.62 |
| Distance | 1,069 ly |
Position
| Right Ascension | 1h 59.68m |
| Declination | -34° 45.55′ |
Frequently Asked Questions
What type of star is HIP 9317?
HIP 9317 is a Class K — K-type (Orange) star.
How far is HIP 9317 from Earth?
HIP 9317 is approximately 1,069.4 light-years from Earth.
Can you see HIP 9317 with the naked eye?
With an apparent magnitude of 9.20, HIP 9317 is not visible to the naked eye.