HIP 6492
HIP 6492 is a K-type (Orange) star.
At a distance of roughly 1,000 light-years, HIP 6492 is a distant star lying deep within the Milky Way galaxy.
HIP 6492 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +5.97, HIP 6492 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 red hue, which corresponds to a B-V color index of +1.677.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.677 |
Observation
| Apparent Magnitude | +5.97 |
| Absolute Magnitude | -1.46 |
| Distance | 1,000 ly |
Position
| Right Ascension | 1h 23.42m |
| Declination | 20° 28.14′ |
Frequently Asked Questions
What type of star is HIP 6492?
HIP 6492 is a Class K — K-type (Orange) star.
How far is HIP 6492 from Earth?
HIP 6492 is approximately 1,000.5 light-years from Earth.
Can you see HIP 6492 with the naked eye?
With an apparent magnitude of 5.97, HIP 6492 is visible to the naked eye.