HIP 94887
HIP 94887 is a K-type (Orange) star located in the constellation Cygnus.
At a distance of roughly 2,281 light-years, HIP 94887 is a distant star lying deep within the Milky Way galaxy.
HIP 94887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 94887 has an apparent magnitude of +8.37, 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 +1.403.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,403 |
Observation
| Magnitude Apparente | +8.37 |
| Magnitude Absolue | -0,85 |
| Distance | 2,281 ly |
| Constellation | Cygnus |
Position
| Ascension droite | 19h 18,57m |
| Déclinaison | 50° 52,45′ |
Questions fréquentes
What type of star is HIP 94887?
HIP 94887 is a Class K — K-type (Orange) star.
How far is HIP 94887 from Earth?
HIP 94887 is approximately 2,280.8 light-years from Earth.
Can you see HIP 94887 with the naked eye?
With an apparent magnitude of 8.37, HIP 94887 is not visible to the naked eye.
What constellation is HIP 94887 in?
HIP 94887 is located in the constellation Cygnus.