HIP 105890
HIP 105890 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 2,077 light-years, HIP 105890 is a distant star lying deep within the Milky Way galaxy.
HIP 105890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 105890 has an apparent magnitude of +8.97, 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 +1.156.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,156 |
Observation
| Magnitude Apparente | +8.97 |
| Magnitude Absolue | -0,05 |
| Distance | 2,077 ly |
| Constellation | Pegasus |
Position
| Ascension droite | 21h 26,73m |
| Déclinaison | 3° 35,18′ |
Questions fréquentes
What type of star is HIP 105890?
HIP 105890 is a Class K — K-type (Orange) star.
How far is HIP 105890 from Earth?
HIP 105890 is approximately 2,077.4 light-years from Earth.
Can you see HIP 105890 with the naked eye?
With an apparent magnitude of 8.97, HIP 105890 is not visible to the naked eye.
What constellation is HIP 105890 in?
HIP 105890 is located in the constellation Pegasus.