HIP 105259
HIP 105259 is a B-type (Blue-White) star.
At a distance of roughly 1,930 light-years, HIP 105259 is a distant star lying deep within the Milky Way galaxy.
HIP 105259 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
With an apparent magnitude of +5.51, HIP 105259 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its orange hue, which corresponds to a B-V color index of +1.114.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 1,114 |
Observation
| Magnitude Apparente | +5.51 |
| Magnitude Absolue | -3,35 |
| Distance | 1,930 ly |
Position
| Ascension droite | 21h 19,26m |
| Déclinaison | 58° 37,41′ |
Questions fréquentes
What type of star is HIP 105259?
HIP 105259 is a Class B — B-type (Blue-White) star.
How far is HIP 105259 from Earth?
HIP 105259 is approximately 1,929.9 light-years from Earth.
Can you see HIP 105259 with the naked eye?
With an apparent magnitude of 5.51, HIP 105259 is visible to the naked eye.