HIP 97979
HIP 97979 is a K-type (Orange) star.
At a distance of roughly 1,152 light-years, HIP 97979 is a distant star lying deep within the Milky Way galaxy.
HIP 97979 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 97979 has an apparent magnitude of +6.73, 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 +1.508.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,508 |
Observation
| Magnitude Apparente | +6.73 |
| Magnitude Absolue | -1,01 |
| Distance | 1,152 ly |
Position
| Ascension droite | 19h 54,74m |
| Déclinaison | 22° 25,75′ |
Frequently Asked Questions
What type of star is HIP 97979?
HIP 97979 is a Class K — K-type (Orange) star.
How far is HIP 97979 from Earth?
HIP 97979 is approximately 1,152.5 light-years from Earth.
Can you see HIP 97979 with the naked eye?
With an apparent magnitude of 6.73, HIP 97979 is not visible to the naked eye.