HIP 4677
HIP 4677 is a K-type (Orange) star.
At a distance of roughly 1,773 light-years, HIP 4677 is a distant star lying deep within the Milky Way galaxy.
HIP 4677 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4677 has an apparent magnitude of +7.62, 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 +1.503.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.503 |
Observation
| Apparent Magnitude | +7.62 |
| Absolute Magnitude | -1.06 |
| Distance | 1,773 ly |
Position
| Right Ascension | 1h 0.09m |
| Declination | 2° 37.98′ |
Frequently Asked Questions
What type of star is HIP 4677?
HIP 4677 is a Class K — K-type (Orange) star.
How far is HIP 4677 from Earth?
HIP 4677 is approximately 1,772.6 light-years from Earth.
Can you see HIP 4677 with the naked eye?
With an apparent magnitude of 7.62, HIP 4677 is not visible to the naked eye.