HIP 4869
HIP 4869 is a K-type (Orange) star.
At a distance of roughly 1,250 light-years, HIP 4869 is a distant star lying deep within the Milky Way galaxy.
HIP 4869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4869 has an apparent magnitude of +7.24, 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 orange hue, which corresponds to a B-V color index of +1.390.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,390 |
Observation
| Magnitude Apparente | +7.24 |
| Magnitude Absolue | -0,68 |
| Distance | 1,250 ly |
Position
| Ascension droite | 1h 2,61m |
| Déclinaison | -77° 33,06′ |
Questions fréquentes
What type of star is HIP 4869?
HIP 4869 is a Class K — K-type (Orange) star.
How far is HIP 4869 from Earth?
HIP 4869 is approximately 1,249.6 light-years from Earth.
Can you see HIP 4869 with the naked eye?
With an apparent magnitude of 7.24, HIP 4869 is not visible to the naked eye.