HIP 12012
HIP 12012 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,102 light-years, HIP 12012 is a distant star lying deep within the Milky Way galaxy.
HIP 12012 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 12012 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 red hue, which corresponds to a B-V color index of +1.468.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,468 |
Observation
| Magnitude Apparente | +9.15 |
| Magnitude Absolue | 1,51 |
| Distance | 1,102 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 2h 34,88m |
| Déclinaison | 67° 16,17′ |
Questions fréquentes
What type of star is HIP 12012?
HIP 12012 is a Class K — K-type (Orange) star.
How far is HIP 12012 from Earth?
HIP 12012 is approximately 1,101.9 light-years from Earth.
Can you see HIP 12012 with the naked eye?
With an apparent magnitude of 9.15, HIP 12012 is not visible to the naked eye.
What constellation is HIP 12012 in?
HIP 12012 is located in the constellation Cassiopeia.