HIP 67251
HIP 67251 is a B-type (Blue-White) star located in the constellation Centaurus.
HIP 67251 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 67251 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 67251 has an apparent magnitude of +9.18, 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 +0.097.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,097 |
Observation
| Magnitude Apparente | +9.18 |
| Magnitude Absolue | -10,82 |
| Distance | 326,156 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 13h 47,05m |
| Déclinaison | -58° 4,27′ |
Questions fréquentes
What type of star is HIP 67251?
HIP 67251 is a Class B — B-type (Blue-White) star.
How far is HIP 67251 from Earth?
HIP 67251 is approximately 326,156.0 light-years from Earth.
Can you see HIP 67251 with the naked eye?
With an apparent magnitude of 9.18, HIP 67251 is not visible to the naked eye.
What constellation is HIP 67251 in?
HIP 67251 is located in the constellation Centaurus.