HIP 17456
HIP 17456 is a A-type (White) star located in the constellation Perseus.
At a distance of roughly 1,132 light-years, HIP 17456 is a distant star lying deep within the Milky Way galaxy.
HIP 17456 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 17456 has an apparent magnitude of +8.46, 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 +0.122.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,122 |
Observation
| Magnitude Apparente | +8.46 |
| Magnitude Absolue | 0,76 |
| Distance | 1,132 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 44,50m |
| Déclinaison | 47° 33,85′ |
Questions fréquentes
What type of star is HIP 17456?
HIP 17456 is a Class A — A-type (White) star.
How far is HIP 17456 from Earth?
HIP 17456 is approximately 1,132.5 light-years from Earth.
Can you see HIP 17456 with the naked eye?
With an apparent magnitude of 8.46, HIP 17456 is not visible to the naked eye.
What constellation is HIP 17456 in?
HIP 17456 is located in the constellation Perseus.