HIP 90979
HIP 90979 is a K-type (Orange) star.
Located approximately 89.0 light-years from Earth, HIP 90979 resides within the broader disk of our Milky Way galaxy.
HIP 90979 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
At an apparent magnitude of +10.03, HIP 90979 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its orange hue, which corresponds to a B-V color index of +1.263.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,263 |
Observation
| Magnitude Apparente | +10.03 |
| Magnitude Absolue | 7,85 |
| Distance | 89.0 ly |
Position
| Ascension droite | 18h 33,48m |
| Déclinaison | -11° 38,16′ |
Frequently Asked Questions
What type of star is HIP 90979?
HIP 90979 is a Class K — K-type (Orange) star.
How far is HIP 90979 from Earth?
HIP 90979 is approximately 89.0 light-years from Earth.
Can you see HIP 90979 with the naked eye?
With an apparent magnitude of 10.03, HIP 90979 is not visible to the naked eye.