HIP 3869
HIP 3869 is a K-type (Orange) star.
At a distance of roughly 2,652 light-years, HIP 3869 is a distant star lying deep within the Milky Way galaxy.
HIP 3869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 3869 has an apparent magnitude of +7.51, 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 +1.428.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,428 |
Observation
| Magnitude Apparente | +7.51 |
| Magnitude Absolue | -2,04 |
| Distance | 2,652 ly |
Position
| Ascension droite | 0h 49,67m |
| Déclinaison | 6° 24,43′ |
Questions fréquentes
What type of star is HIP 3869?
HIP 3869 is a Class K — K-type (Orange) star.
How far is HIP 3869 from Earth?
HIP 3869 is approximately 2,651.7 light-years from Earth.
Can you see HIP 3869 with the naked eye?
With an apparent magnitude of 7.51, HIP 3869 is not visible to the naked eye.