HIP 19659
HIP 19659 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,310 light-years, HIP 19659 is a distant star lying deep within the Milky Way galaxy.
HIP 19659 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 19659 has an apparent magnitude of +9.06, 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 +0.167.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,167 |
Observation
| Magnitude Apparente | +9.06 |
| Magnitude Absolue | 1,04 |
| Distance | 1,310 ly |
| Constellation | Perseus |
Position
| Ascension droite | 4h 12,75m |
| Déclinaison | 31° 47,68′ |
Questions fréquentes
What type of star is HIP 19659?
HIP 19659 is a Class B — B-type (Blue-White) star.
How far is HIP 19659 from Earth?
HIP 19659 is approximately 1,309.9 light-years from Earth.
Can you see HIP 19659 with the naked eye?
With an apparent magnitude of 9.06, HIP 19659 is not visible to the naked eye.
What constellation is HIP 19659 in?
HIP 19659 is located in the constellation Perseus.