HIP 1811
HIP 1811 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,510 light-years, HIP 1811 is a distant star lying deep within the Milky Way galaxy.
HIP 1811 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 1811 has an apparent magnitude of +9.74, 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 hue, which corresponds to a B-V color index of -0.018.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,018 |
Observation
| Magnitude Apparente | +9.74 |
| Magnitude Absolue | 1,41 |
| Distance | 1,510 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 23,00m |
| Déclinaison | 55° 2,95′ |
Questions fréquentes
What type of star is HIP 1811?
HIP 1811 is a Class B — B-type (Blue-White) star.
How far is HIP 1811 from Earth?
HIP 1811 is approximately 1,510.0 light-years from Earth.
Can you see HIP 1811 with the naked eye?
With an apparent magnitude of 9.74, HIP 1811 is not visible to the naked eye.
What constellation is HIP 1811 in?
HIP 1811 is located in the constellation Cassiopeia.