HIP 4167
HIP 4167 is a K-type (Orange) star.
At a distance of roughly 1,907 light-years, HIP 4167 is a distant star lying deep within the Milky Way galaxy.
HIP 4167 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4167 has an apparent magnitude of +8.54, 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 +1.537.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,537 |
Observation
| Magnitude Apparente | +8.54 |
| Magnitude Absolue | -0,30 |
| Distance | 1,907 ly |
Position
| Ascension droite | 0h 53,24m |
| Déclinaison | 9° 54,87′ |
Questions fréquentes
What type of star is HIP 4167?
HIP 4167 is a Class K — K-type (Orange) star.
How far is HIP 4167 from Earth?
HIP 4167 is approximately 1,907.3 light-years from Earth.
Can you see HIP 4167 with the naked eye?
With an apparent magnitude of 8.54, HIP 4167 is not visible to the naked eye.