HIP 16897
HIP 16897 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,337 light-years, HIP 16897 is a distant star lying deep within the Milky Way galaxy.
HIP 16897 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 16897 has an apparent magnitude of +7.01, 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 +0.052.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,052 |
Observation
| Magnitude Apparente | +7.01 |
| Magnitude Absolue | -1,05 |
| Distance | 1,337 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 37,39m |
| Déclinaison | 40° 5,38′ |
Questions fréquentes
What type of star is HIP 16897?
HIP 16897 is a Class B — B-type (Blue-White) star.
How far is HIP 16897 from Earth?
HIP 16897 is approximately 1,336.7 light-years from Earth.
Can you see HIP 16897 with the naked eye?
With an apparent magnitude of 7.01, HIP 16897 is not visible to the naked eye.
What constellation is HIP 16897 in?
HIP 16897 is located in the constellation Perseus.