HIP 20908
HIP 20908 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 865.1 light-years from Earth, HIP 20908 resides within the broader disk of our Milky Way galaxy.
HIP 20908 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 20908 has an apparent magnitude of +7.80, 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 +0.105.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,105 |
Observation
| Magnitude Apparente | +7.80 |
| Magnitude Absolue | 0,68 |
| Distance | 865 ly |
| Constellation | Perseus |
Position
| Ascension droite | 4h 28,88m |
| Déclinaison | 52° 23,36′ |
Questions fréquentes
What type of star is HIP 20908?
HIP 20908 is a Class B — B-type (Blue-White) star.
How far is HIP 20908 from Earth?
HIP 20908 is approximately 865.1 light-years from Earth.
Can you see HIP 20908 with the naked eye?
With an apparent magnitude of 7.80, HIP 20908 is not visible to the naked eye.
What constellation is HIP 20908 in?
HIP 20908 is located in the constellation Perseus.