HIP 4590
HIP 4590 is a K-type (Orange) star.
At a distance of roughly 2,174 light-years, HIP 4590 is a distant star lying deep within the Milky Way galaxy.
HIP 4590 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4590 has an apparent magnitude of +8.26, 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 red hue, which corresponds to a B-V color index of +1.579.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,579 |
Observation
| Magnitude Apparente | +8.26 |
| Magnitude Absolue | -0,86 |
| Distance | 2,174 ly |
Position
| Ascension droite | 0h 58,75m |
| Déclinaison | -62° 27,11′ |
Questions fréquentes
What type of star is HIP 4590?
HIP 4590 is a Class K — K-type (Orange) star.
How far is HIP 4590 from Earth?
HIP 4590 is approximately 2,174.4 light-years from Earth.
Can you see HIP 4590 with the naked eye?
With an apparent magnitude of 8.26, HIP 4590 is not visible to the naked eye.