HIP 11189
HIP 11189 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,735 light-years, HIP 11189 is a distant star lying deep within the Milky Way galaxy.
HIP 11189 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 11189 has an apparent magnitude of +9.09, 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 blue-white hue, which corresponds to a B-V color index of +0.188.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,188 |
Observation
| Magnitude Apparente | +9.09 |
| Magnitude Absolue | 0,46 |
| Distance | 1,735 ly |
| Constellation | Perseus |
Position
| Ascension droite | 2h 24,10m |
| Déclinaison | 54° 11,89′ |
Questions fréquentes
What type of star is HIP 11189?
HIP 11189 is a Class B — B-type (Blue-White) star.
How far is HIP 11189 from Earth?
HIP 11189 is approximately 1,734.9 light-years from Earth.
Can you see HIP 11189 with the naked eye?
With an apparent magnitude of 9.09, HIP 11189 is not visible to the naked eye.
What constellation is HIP 11189 in?
HIP 11189 is located in the constellation Perseus.