HIP 104677
HIP 104677 is a K-type (Orange) star.
At a distance of roughly 1,503 light-years, HIP 104677 is a distant star lying deep within the Milky Way galaxy.
HIP 104677 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104677 has an apparent magnitude of +6.96, 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 +1.627.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.627 |
Observation
| Apparent Magnitude | +6.96 |
| Absolute Magnitude | -1.36 |
| Distance | 1,503 ly |
Position
| Right Ascension | 21h 12.20m |
| Declination | 11° 46.89′ |
Frequently Asked Questions
What type of star is HIP 104677?
HIP 104677 is a Class K — K-type (Orange) star.
How far is HIP 104677 from Earth?
HIP 104677 is approximately 1,503.0 light-years from Earth.
Can you see HIP 104677 with the naked eye?
With an apparent magnitude of 6.96, HIP 104677 is not visible to the naked eye.