HIP 9122
HIP 9122 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,754 light-years, HIP 9122 is a distant star lying deep within the Milky Way galaxy.
HIP 9122 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9122 has an apparent magnitude of +8.23, 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 +1.465.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,465 |
Observation
| Magnitude Apparente | +8.23 |
| Magnitude Absolue | -0,42 |
| Distance | 1,754 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 1h 57,61m |
| Déclinaison | 64° 46,96′ |
Questions fréquentes
What type of star is HIP 9122?
HIP 9122 is a Class K — K-type (Orange) star.
How far is HIP 9122 from Earth?
HIP 9122 is approximately 1,753.5 light-years from Earth.
Can you see HIP 9122 with the naked eye?
With an apparent magnitude of 8.23, HIP 9122 is not visible to the naked eye.
What constellation is HIP 9122 in?
HIP 9122 is located in the constellation Cassiopeia.