HIP 18321
HIP 18321 is a F-type (Yellow-White) star located in the constellation Perseus.
HIP 18321 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 18321 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.07, HIP 18321 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 +0.513.
Propriétés physiques
| Classe Spectrale | Class F — F-type (Yellow-White) |
| Indice de couleur (B−V) | 0,513 |
Observation
| Magnitude Apparente | +10.07 |
| Magnitude Absolue | -9,93 |
| Distance | 326,156 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 55,00m |
| Déclinaison | 44° 16,87′ |
Questions fréquentes
What type of star is HIP 18321?
HIP 18321 is a Class F — F-type (Yellow-White) star.
How far is HIP 18321 from Earth?
HIP 18321 is approximately 326,156.0 light-years from Earth.
Can you see HIP 18321 with the naked eye?
With an apparent magnitude of 10.07, HIP 18321 is not visible to the naked eye.
What constellation is HIP 18321 in?
HIP 18321 is located in the constellation Perseus.