HIP 70911
HIP 70911 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,049 light-years, HIP 70911 is a distant star lying deep within the Milky Way galaxy.
HIP 70911 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 70911 has an apparent magnitude of +8.81, 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 +1.244.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,244 |
Observation
| Magnitude Apparente | +8.81 |
| Magnitude Absolue | 1,27 |
| Distance | 1,049 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 14h 30,06m |
| Déclinaison | -60° 50,98′ |
Frequently Asked Questions
What type of star is HIP 70911?
HIP 70911 is a Class K — K-type (Orange) star.
How far is HIP 70911 from Earth?
HIP 70911 is approximately 1,048.7 light-years from Earth.
Can you see HIP 70911 with the naked eye?
With an apparent magnitude of 8.81, HIP 70911 is not visible to the naked eye.
What constellation is HIP 70911 in?
HIP 70911 is located in the constellation Centaurus.