HIP 63050
HIP 63050 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,182 light-years, HIP 63050 is a distant star lying deep within the Milky Way galaxy.
HIP 63050 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 63050 has an apparent magnitude of +7.49, 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 red hue, which corresponds to a B-V color index of +1.518.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,518 |
Observation
| Magnitude Apparente | +7.49 |
| Magnitude Absolue | -0,30 |
| Distance | 1,182 ly |
| Constellation | Centaurus |
Position
| Ascension droite | 12h 55,14m |
| Déclinaison | -48° 5,50′ |
Frequently Asked Questions
What type of star is HIP 63050?
HIP 63050 is a Class K — K-type (Orange) star.
How far is HIP 63050 from Earth?
HIP 63050 is approximately 1,181.7 light-years from Earth.
Can you see HIP 63050 with the naked eye?
With an apparent magnitude of 7.49, HIP 63050 is not visible to the naked eye.
What constellation is HIP 63050 in?
HIP 63050 is located in the constellation Centaurus.