HIP 109309
HIP 109309 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,212 light-years, HIP 109309 is a distant star lying deep within the Milky Way galaxy.
HIP 109309 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 109309 has an apparent magnitude of +8.68, 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 +1.114.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,114 |
Observation
| Magnitude Apparente | +8.68 |
| Magnitude Absolue | 0,83 |
| Distance | 1,212 ly |
| Constellation | Pegasus |
Position
| Ascension droite | 22h 8,76m |
| Déclinaison | 7° 19,90′ |
Questions fréquentes
What type of star is HIP 109309?
HIP 109309 is a Class K — K-type (Orange) star.
How far is HIP 109309 from Earth?
HIP 109309 is approximately 1,212.5 light-years from Earth.
Can you see HIP 109309 with the naked eye?
With an apparent magnitude of 8.68, HIP 109309 is not visible to the naked eye.
What constellation is HIP 109309 in?
HIP 109309 is located in the constellation Pegasus.