HIP 17424
HIP 17424 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,463 light-years, HIP 17424 is a distant star lying deep within the Milky Way galaxy.
HIP 17424 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17424 has an apparent magnitude of +7.66, 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 red hue, which corresponds to a B-V color index of +1.641.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,641 |
Observation
| Magnitude Apparente | +7.66 |
| Magnitude Absolue | -0,60 |
| Distance | 1,463 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 43,98m |
| Déclinaison | 38° 22,43′ |
Questions fréquentes
What type of star is HIP 17424?
HIP 17424 is a Class K — K-type (Orange) star.
How far is HIP 17424 from Earth?
HIP 17424 is approximately 1,462.6 light-years from Earth.
Can you see HIP 17424 with the naked eye?
With an apparent magnitude of 7.66, HIP 17424 is not visible to the naked eye.
What constellation is HIP 17424 in?
HIP 17424 is located in the constellation Perseus.