HIP 13007
HIP 13007 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 2,741 light-years, HIP 13007 is a distant star lying deep within the Milky Way galaxy.
HIP 13007 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 13007 has an apparent magnitude of +9.15, 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 +0.161.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,161 |
Observation
| Magnitude Apparente | +9.15 |
| Magnitude Absolue | -0,47 |
| Distance | 2,741 ly |
| Constellation | Perseus |
Position
| Ascension droite | 2h 47,18m |
| Déclinaison | 45° 55,00′ |
Questions fréquentes
What type of star is HIP 13007?
HIP 13007 is a Class B — B-type (Blue-White) star.
How far is HIP 13007 from Earth?
HIP 13007 is approximately 2,740.8 light-years from Earth.
Can you see HIP 13007 with the naked eye?
With an apparent magnitude of 9.15, HIP 13007 is not visible to the naked eye.
What constellation is HIP 13007 in?
HIP 13007 is located in the constellation Perseus.