HIP 57867
HIP 57867 is a B-type (Blue-White) star located in the constellation Centaurus.
At a distance of roughly 3,020 light-years, HIP 57867 is a distant star lying deep within the Milky Way galaxy.
HIP 57867 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 57867 has an apparent magnitude of +9.53, 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 +0.059.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,059 |
Observation
| Magnitude Apparente | +9.53 |
| Magnitude Absolue | -0,30 |
| Distance | 3,020 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 11h 52,15m |
| Déclinaison | -53° 46,30′ |
Questions fréquentes
What type of star is HIP 57867?
HIP 57867 is a Class B — B-type (Blue-White) star.
How far is HIP 57867 from Earth?
HIP 57867 is approximately 3,020.0 light-years from Earth.
Can you see HIP 57867 with the naked eye?
With an apparent magnitude of 9.53, HIP 57867 is not visible to the naked eye.
What constellation is HIP 57867 in?
HIP 57867 is located in the constellation Centaurus.