HIP 10717
HIP 10717 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,353 light-years, HIP 10717 is a distant star lying deep within the Milky Way galaxy.
HIP 10717 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 10717 has an apparent magnitude of +7.94, 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 +0.016.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,016 |
Observation
| Magnitude Apparente | +7.94 |
| Magnitude Absolue | -0,15 |
| Distance | 1,353 ly |
| Constellation | Perseus |
Position
| Ascension droite | 2h 17,99m |
| Déclinaison | 51° 46,91′ |
Questions fréquentes
What type of star is HIP 10717?
HIP 10717 is a Class B — B-type (Blue-White) star.
How far is HIP 10717 from Earth?
HIP 10717 is approximately 1,353.3 light-years from Earth.
Can you see HIP 10717 with the naked eye?
With an apparent magnitude of 7.94, HIP 10717 is not visible to the naked eye.
What constellation is HIP 10717 in?
HIP 10717 is located in the constellation Perseus.