HIP 3887
HIP 3887 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 2,509 light-years, HIP 3887 is a distant star lying deep within the Milky Way galaxy.
HIP 3887 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 3887 has an apparent magnitude of +8.51, 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 yellow-white hue, which corresponds to a B-V color index of +0.616.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,616 |
Observation
| Magnitude Apparente | +8.51 |
| Magnitude Absolue | -0,92 |
| Distance | 2,509 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 49,89m |
| Déclinaison | 64° 38,27′ |
Questions fréquentes
What type of star is HIP 3887?
HIP 3887 is a Class B — B-type (Blue-White) star.
How far is HIP 3887 from Earth?
HIP 3887 is approximately 2,508.9 light-years from Earth.
Can you see HIP 3887 with the naked eye?
With an apparent magnitude of 8.51, HIP 3887 is not visible to the naked eye.
What constellation is HIP 3887 in?
HIP 3887 is located in the constellation Cassiopeia.