HIP 20239
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 | 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′ |
Questions fréquentes
What type of star is HIP 20239?
HIP 20239 is a Class B — B-type (Blue-White) star.
How far is HIP 20239 from Earth?
HIP 20239 is approximately 1,568.1 light-years from Earth.
Can you see HIP 20239 with the naked eye?
With an apparent magnitude of 10.29, HIP 20239 is not visible to the naked eye.
What constellation is HIP 20239 in?
HIP 20239 is located in the constellation Perseus.