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.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 1,114 |
Beobachtung
| Scheinbare Helligkeit | +5.51 |
| Absolute Helligkeit | -3,35 |
| Entfernung | 1,930 ly |
Position
| Rektaszension | 21h 19,26m |
| Deklination | 58° 37,41′ |
Häufig gestellte Fragen
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.