HIP 17772
HIP 17772 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 817.4 light-years from Earth, HIP 17772 resides within the broader disk of our Milky Way galaxy.
HIP 17772 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 17772 has an apparent magnitude of +6.18, 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 +0.028.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,028 |
Observation
| Magnitude Apparente | +6.18 |
| Magnitude Absolue | -0,82 |
| Distance | 817 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 48,30m |
| Déclinaison | 50° 44,21′ |
Questions fréquentes
What type of star is HIP 17772?
HIP 17772 is a Class B — B-type (Blue-White) star.
How far is HIP 17772 from Earth?
HIP 17772 is approximately 817.4 light-years from Earth.
Can you see HIP 17772 with the naked eye?
With an apparent magnitude of 6.18, HIP 17772 is not visible to the naked eye.
What constellation is HIP 17772 in?
HIP 17772 is located in the constellation Perseus.