HIP 65851
HIP 65851 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,056 light-years, HIP 65851 is a distant star lying deep within the Milky Way galaxy.
HIP 65851 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 65851 has an apparent magnitude of +8.59, 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 +1.075.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,075 |
Observation
| Magnitude Apparente | +8.59 |
| Magnitude Absolue | 1,04 |
| Distance | 1,056 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 13h 29,93m |
| Déclinaison | -32° 51,35′ |
Questions fréquentes
What type of star is HIP 65851?
HIP 65851 is a Class K — K-type (Orange) star.
How far is HIP 65851 from Earth?
HIP 65851 is approximately 1,055.5 light-years from Earth.
Can you see HIP 65851 with the naked eye?
With an apparent magnitude of 8.59, HIP 65851 is not visible to the naked eye.
What constellation is HIP 65851 in?
HIP 65851 is located in the constellation Centaurus.