HIP 11089
HIP 11089 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 2,013 light-years, HIP 11089 is a distant star lying deep within the Milky Way galaxy.
HIP 11089 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 11089 has an apparent magnitude of +9.61, 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 white hue, which corresponds to a B-V color index of +0.470.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,470 |
Observation
| Magnitude Apparente | +9.61 |
| Magnitude Absolue | 0,66 |
| Distance | 2,013 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 2h 22,83m |
| Déclinaison | 65° 48,24′ |
Questions fréquentes
What type of star is HIP 11089?
HIP 11089 is a Class B — B-type (Blue-White) star.
How far is HIP 11089 from Earth?
HIP 11089 is approximately 2,013.3 light-years from Earth.
Can you see HIP 11089 with the naked eye?
With an apparent magnitude of 9.61, HIP 11089 is not visible to the naked eye.
What constellation is HIP 11089 in?
HIP 11089 is located in the constellation Cassiopeia.