HIP 16252
HIP 16252 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 637.0 light-years from Earth, HIP 16252 resides within the broader disk of our Milky Way galaxy.
HIP 16252 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 16252 has an apparent magnitude of +6.21, 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 +0.131.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,131 |
Observation
| Magnitude Apparente | +6.21 |
| Magnitude Absolue | -0,24 |
| Distance | 637 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 29,44m |
| Déclinaison | 46° 56,27′ |
Questions fréquentes
What type of star is HIP 16252?
HIP 16252 is a Class B — B-type (Blue-White) star.
How far is HIP 16252 from Earth?
HIP 16252 is approximately 637.0 light-years from Earth.
Can you see HIP 16252 with the naked eye?
With an apparent magnitude of 6.21, HIP 16252 is not visible to the naked eye.
What constellation is HIP 16252 in?
HIP 16252 is located in the constellation Perseus.