HIP 20239
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HIP 20239 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,568 light-years, HIP 20239 is a distant star lying deep within the Milky Way galaxy.
HIP 20239 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.29, HIP 20239 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its white hue, which corresponds to a B-V color index of +0.364.
Propriétés physiques
| Classe Spectrale | B Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,364 |
Observation
| Magnitude Apparente | +10.29 |
| Magnitude Absolue | 1,88 |
| Distance | 1,568 ly |
| Constellation | Perseus |
Position
| Ascension droite | 4h 20,22m |
| Déclinaison | 50° 16,49′ |