HIP 75758
HIP 75758 is a K-type (Orange) star.
At a distance of roughly 1,069 light-years, HIP 75758 is a distant star lying deep within the Milky Way galaxy.
HIP 75758 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 75758 has an apparent magnitude of +8.93, 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 +1.231.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,231 |
Observation
| Magnitude Apparente | +8.93 |
| Magnitude Absolue | 1,35 |
| Distance | 1,069 ly |
Position
| Ascension droite | 15h 28,61m |
| Déclinaison | 32° 21,75′ |
Frequently Asked Questions
What type of star is HIP 75758?
HIP 75758 is a Class K — K-type (Orange) star.
How far is HIP 75758 from Earth?
HIP 75758 is approximately 1,069.4 light-years from Earth.
Can you see HIP 75758 with the naked eye?
With an apparent magnitude of 8.93, HIP 75758 is not visible to the naked eye.