HIP 5451
HIP 5451 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,812 light-years, HIP 5451 is a distant star lying deep within the Milky Way galaxy.
HIP 5451 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 5451 has an apparent magnitude of +8.05, 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 orange hue, which corresponds to a B-V color index of +1.179.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,179 |
Observation
| Magnitude Apparente | +8.05 |
| Magnitude Absolue | -0,67 |
| Distance | 1,812 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 1h 9,76m |
| Déclinaison | 52° 51,27′ |
Questions fréquentes
What type of star is HIP 5451?
HIP 5451 is a Class K — K-type (Orange) star.
How far is HIP 5451 from Earth?
HIP 5451 is approximately 1,812.0 light-years from Earth.
Can you see HIP 5451 with the naked eye?
With an apparent magnitude of 8.05, HIP 5451 is not visible to the naked eye.
What constellation is HIP 5451 in?
HIP 5451 is located in the constellation Cassiopeia.