HIP 8125
HIP 8125 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 3,077 light-years, HIP 8125 is a distant star lying deep within the Milky Way galaxy.
HIP 8125 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.66, HIP 8125 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its white hue, which corresponds to a B-V color index of +0.505.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,505 |
Observation
| Magnitude Apparente | +10.66 |
| Magnitude Absolue | 0,79 |
| Distance | 3,077 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 1h 44,42m |
| Déclinaison | 60° 37,24′ |
Questions fréquentes
What type of star is HIP 8125?
HIP 8125 is a Class B — B-type (Blue-White) star.
How far is HIP 8125 from Earth?
HIP 8125 is approximately 3,076.9 light-years from Earth.
Can you see HIP 8125 with the naked eye?
With an apparent magnitude of 10.66, HIP 8125 is not visible to the naked eye.
What constellation is HIP 8125 in?
HIP 8125 is located in the constellation Cassiopeia.