HIP 106718
HIP 106718 is a K-type (Orange) star.
At a distance of roughly 1,056 light-years, HIP 106718 is a distant star lying deep within the Milky Way galaxy.
HIP 106718 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 106718 has an apparent magnitude of +8.75, 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 +1.176.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,176 |
Observation
| Magnitude Apparente | +8.75 |
| Magnitude Absolue | 1,20 |
| Distance | 1,056 ly |
Position
| Ascension droite | 21h 37,00m |
| Déclinaison | -44° 53,51′ |
Frequently Asked Questions
What type of star is HIP 106718?
HIP 106718 is a Class K — K-type (Orange) star.
How far is HIP 106718 from Earth?
HIP 106718 is approximately 1,055.5 light-years from Earth.
Can you see HIP 106718 with the naked eye?
With an apparent magnitude of 8.75, HIP 106718 is not visible to the naked eye.