HIP 72985
HIP 72985 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,279 light-years, HIP 72985 is a distant star lying deep within the Milky Way galaxy.
HIP 72985 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 72985 has an apparent magnitude of +9.32, 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 +1.287.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,287 |
Observation
| Magnitude Apparente | +9.32 |
| Magnitude Absolue | 1,35 |
| Distance | 1,279 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 14h 54,92m |
| Déclinaison | -32° 48,79′ |
Frequently Asked Questions
What type of star is HIP 72985?
HIP 72985 is a Class K — K-type (Orange) star.
How far is HIP 72985 from Earth?
HIP 72985 is approximately 1,279.0 light-years from Earth.
Can you see HIP 72985 with the naked eye?
With an apparent magnitude of 9.32, HIP 72985 is not visible to the naked eye.
What constellation is HIP 72985 in?
HIP 72985 is located in the constellation Centaurus.