HIP 109979
HIP 109979 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 1,094 light-years, HIP 109979 is a distant star lying deep within the Milky Way galaxy.
HIP 109979 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 109979 has an apparent magnitude of +7.52, 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 +1.330.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,330 |
Observation
| Magnitude Apparente | +7.52 |
| Magnitude Absolue | -0,11 |
| Distance | 1,094 ly |
| Constellation | Pegasus |
Position
| Ascension droite | 22h 16,51m |
| Déclinaison | 32° 37,29′ |
Questions fréquentes
What type of star is HIP 109979?
HIP 109979 is a Class K — K-type (Orange) star.
How far is HIP 109979 from Earth?
HIP 109979 is approximately 1,094.5 light-years from Earth.
Can you see HIP 109979 with the naked eye?
With an apparent magnitude of 7.52, HIP 109979 is not visible to the naked eye.
What constellation is HIP 109979 in?
HIP 109979 is located in the constellation Pegasus.