HIP 890
HIP 890 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,152 light-years, HIP 890 is a distant star lying deep within the Milky Way galaxy.
HIP 890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 890 has an apparent magnitude of +9.64, 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 +0.560.
Propriétés physiques
| Classe Spectrale | B Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,560 |
Observation
| Magnitude Apparente | +9.64 |
| Magnitude Absolue | 1,90 |
| Distance | 1,152 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 10,93m |
| Déclinaison | 64° 57,79′ |
Frequently Asked Questions
What type of star is HIP 890?
HIP 890 is a Class B — B-type (Blue-White) star.
How far is HIP 890 from Earth?
HIP 890 is approximately 1,152.5 light-years from Earth.
Can you see HIP 890 with the naked eye?
With an apparent magnitude of 9.64, HIP 890 is not visible to the naked eye.
What constellation is HIP 890 in?
HIP 890 is located in the constellation Cassiopeia.