HIP 2418
HIP 2418 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,337 light-years, HIP 2418 is a distant star lying deep within the Milky Way galaxy.
HIP 2418 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 2418 has an apparent magnitude of +9.95, 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 white hue, which corresponds to a B-V color index of +0.349.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,349 |
Observation
| Magnitude Apparente | +9.95 |
| Magnitude Absolue | 1,89 |
| Distance | 1,337 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 0h 30,82m |
| Déclinaison | 66° 7,86′ |
Questions fréquentes
What type of star is HIP 2418?
HIP 2418 is a Class B — B-type (Blue-White) star.
How far is HIP 2418 from Earth?
HIP 2418 is approximately 1,336.7 light-years from Earth.
Can you see HIP 2418 with the naked eye?
With an apparent magnitude of 9.95, HIP 2418 is not visible to the naked eye.
What constellation is HIP 2418 in?
HIP 2418 is located in the constellation Cassiopeia.