HIP 14890
HIP 14890 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,294 light-years, HIP 14890 is a distant star lying deep within the Milky Way galaxy.
HIP 14890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 14890 has an apparent magnitude of +8.26, 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 +1.303.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,303 |
Observation
| Magnitude Apparente | +8.26 |
| Magnitude Absolue | 0,27 |
| Distance | 1,294 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 12,18m |
| Déclinaison | 53° 14,29′ |
Questions fréquentes
What type of star is HIP 14890?
HIP 14890 is a Class K — K-type (Orange) star.
How far is HIP 14890 from Earth?
HIP 14890 is approximately 1,294.3 light-years from Earth.
Can you see HIP 14890 with the naked eye?
With an apparent magnitude of 8.26, HIP 14890 is not visible to the naked eye.
What constellation is HIP 14890 in?
HIP 14890 is located in the constellation Perseus.