HIP 14578
HIP 14578 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,843 light-years, HIP 14578 is a distant star lying deep within the Milky Way galaxy.
HIP 14578 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 14578 has an apparent magnitude of +7.91, 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 +0.016.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,016 |
Observation
| Magnitude Apparente | +7.91 |
| Magnitude Absolue | -0,85 |
| Distance | 1,843 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 8,18m |
| Déclinaison | 41° 35,12′ |
Questions fréquentes
What type of star is HIP 14578?
HIP 14578 is a Class B — B-type (Blue-White) star.
How far is HIP 14578 from Earth?
HIP 14578 is approximately 1,842.7 light-years from Earth.
Can you see HIP 14578 with the naked eye?
With an apparent magnitude of 7.91, HIP 14578 is not visible to the naked eye.
What constellation is HIP 14578 in?
HIP 14578 is located in the constellation Perseus.