HIP 7218
HIP 7218 is a K-type (Orange) star.
At a distance of roughly 1,631 light-years, HIP 7218 is a distant star lying deep within the Milky Way galaxy.
HIP 7218 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7218 has an apparent magnitude of +7.92, 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 +1.524.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,524 |
Observation
| Magnitude Apparente | +7.92 |
| Magnitude Absolue | -0,58 |
| Distance | 1,631 ly |
Position
| Ascension droite | 1h 32,98m |
| Déclinaison | 0° 7,62′ |
Questions fréquentes
What type of star is HIP 7218?
HIP 7218 is a Class K — K-type (Orange) star.
How far is HIP 7218 from Earth?
HIP 7218 is approximately 1,630.8 light-years from Earth.
Can you see HIP 7218 with the naked eye?
With an apparent magnitude of 7.92, HIP 7218 is not visible to the naked eye.