HIP 16430
HIP 16430 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 720.0 light-years from Earth, HIP 16430 resides within the broader disk of our Milky Way galaxy.
HIP 16430 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 16430 has an apparent magnitude of +6.77, 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 hue, which corresponds to a B-V color index of -0.027.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,027 |
Observation
| Magnitude Apparente | +6.77 |
| Magnitude Absolue | 0,05 |
| Distance | 720 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 31,55m |
| Déclinaison | 47° 51,74′ |
Questions fréquentes
What type of star is HIP 16430?
HIP 16430 is a Class B — B-type (Blue-White) star.
How far is HIP 16430 from Earth?
HIP 16430 is approximately 720.0 light-years from Earth.
Can you see HIP 16430 with the naked eye?
With an apparent magnitude of 6.77, HIP 16430 is not visible to the naked eye.
What constellation is HIP 16430 in?
HIP 16430 is located in the constellation Perseus.