HIP 18900
HIP 18900 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,735 light-years, HIP 18900 is a distant star lying deep within the Milky Way galaxy.
HIP 18900 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 18900 has an apparent magnitude of +8.84, 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 blue-white hue, which corresponds to a B-V color index of +0.170.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,170 |
Observation
| Magnitude Apparente | +8.84 |
| Magnitude Absolue | 0,21 |
| Distance | 1,735 ly |
| Constellation | Perseus |
Position
| Ascension droite | 4h 3,08m |
| Déclinaison | 52° 37,74′ |
Questions fréquentes
What type of star is HIP 18900?
HIP 18900 is a Class B — B-type (Blue-White) star.
How far is HIP 18900 from Earth?
HIP 18900 is approximately 1,734.9 light-years from Earth.
Can you see HIP 18900 with the naked eye?
With an apparent magnitude of 8.84, HIP 18900 is not visible to the naked eye.
What constellation is HIP 18900 in?
HIP 18900 is located in the constellation Perseus.