HIP 13319
HIP 13319 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,615 light-years, HIP 13319 is a distant star lying deep within the Milky Way galaxy.
HIP 13319 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 13319 has an apparent magnitude of +8.50, 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 orange hue, which corresponds to a B-V color index of +1.190.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,190 |
Observation
| Magnitude Apparente | +8.50 |
| Magnitude Absolue | 0,03 |
| Distance | 1,615 ly |
| Constellation | Perseus |
Position
| Ascension droite | 2h 51,40m |
| Déclinaison | 52° 25,29′ |
Questions fréquentes
What type of star is HIP 13319?
HIP 13319 is a Class K — K-type (Orange) star.
How far is HIP 13319 from Earth?
HIP 13319 is approximately 1,614.6 light-years from Earth.
Can you see HIP 13319 with the naked eye?
With an apparent magnitude of 8.50, HIP 13319 is not visible to the naked eye.
What constellation is HIP 13319 in?
HIP 13319 is located in the constellation Perseus.