HIP 4155
HIP 4155 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,240 light-years, HIP 4155 is a distant star lying deep within the Milky Way galaxy.
HIP 4155 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 4155 has an apparent magnitude of +7.26, 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 -0.026.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | -0,026 |
Observation
| Magnitude Apparente | +7.26 |
| Magnitude Absolue | -0,64 |
| Distance | 1,240 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 53,09m |
| Déclinaison | 57° 13,15′ |
Questions fréquentes
What type of star is HIP 4155?
HIP 4155 is a Class B — B-type (Blue-White) star.
How far is HIP 4155 from Earth?
HIP 4155 is approximately 1,240.1 light-years from Earth.
Can you see HIP 4155 with the naked eye?
With an apparent magnitude of 7.26, HIP 4155 is not visible to the naked eye.
What constellation is HIP 4155 in?
HIP 4155 is located in the constellation Cassiopeia.