HIP 39080
HIP 39080 is a K-type (Orange) star.
At a distance of roughly 1,016 light-years, HIP 39080 is a distant star lying deep within the Milky Way galaxy.
HIP 39080 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 39080 has an apparent magnitude of +9.17, 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 +1.172.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,172 |
Observation
| Magnitude Apparente | +9.17 |
| Magnitude Absolue | 1,70 |
| Distance | 1,016 ly |
Position
| Ascension droite | 7h 59,75m |
| Déclinaison | -46° 54,18′ |
Frequently Asked Questions
What type of star is HIP 39080?
HIP 39080 is a Class K — K-type (Orange) star.
How far is HIP 39080 from Earth?
HIP 39080 is approximately 1,016.1 light-years from Earth.
Can you see HIP 39080 with the naked eye?
With an apparent magnitude of 9.17, HIP 39080 is not visible to the naked eye.