HIP 80890
HIP 80890 is a K-type (Orange) star.
At a distance of roughly 1,717 light-years, HIP 80890 is a distant star lying deep within the Milky Way galaxy.
HIP 80890 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 80890 has an apparent magnitude of +8.48, 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 +1.573.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,573 |
Observation
| Magnitude Apparente | +8.48 |
| Magnitude Absolue | -0,13 |
| Distance | 1,717 ly |
Position
| Ascension droite | 16h 31,07m |
| Déclinaison | -49° 58,87′ |
Frequently Asked Questions
What type of star is HIP 80890?
HIP 80890 is a Class K — K-type (Orange) star.
How far is HIP 80890 from Earth?
HIP 80890 is approximately 1,716.6 light-years from Earth.
Can you see HIP 80890 with the naked eye?
With an apparent magnitude of 8.48, HIP 80890 is not visible to the naked eye.