HIP 56190
HIP 56190 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,359 light-years, HIP 56190 is a distant star lying deep within the Milky Way galaxy.
HIP 56190 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 56190 has an apparent magnitude of +7.64, 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 +1.378.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,378 |
Observation
| Magnitude Apparente | +7.64 |
| Magnitude Absolue | -0,46 |
| Distance | 1,359 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 11h 31,08m |
| Déclinaison | -43° 33,19′ |
Questions fréquentes
What type of star is HIP 56190?
HIP 56190 is a Class K — K-type (Orange) star.
How far is HIP 56190 from Earth?
HIP 56190 is approximately 1,359.0 light-years from Earth.
Can you see HIP 56190 with the naked eye?
With an apparent magnitude of 7.64, HIP 56190 is not visible to the naked eye.
What constellation is HIP 56190 in?
HIP 56190 is located in the constellation Centaurus.