HIP 106625
HIP 106625 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 2,568 light-years, HIP 106625 is a distant star lying deep within the Milky Way galaxy.
HIP 106625 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 106625 has an apparent magnitude of +7.89, 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 +1.371.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,371 |
Observation
| Magnitude Apparente | +7.89 |
| Magnitude Absolue | -1,59 |
| Distance | 2,568 ly |
| Constellation | Pegasus |
Position
| Ascension droite | 21h 35,81m |
| Déclinaison | 17° 29,90′ |
Questions fréquentes
What type of star is HIP 106625?
HIP 106625 is a Class K — K-type (Orange) star.
How far is HIP 106625 from Earth?
HIP 106625 is approximately 2,568.2 light-years from Earth.
Can you see HIP 106625 with the naked eye?
With an apparent magnitude of 7.89, HIP 106625 is not visible to the naked eye.
What constellation is HIP 106625 in?
HIP 106625 is located in the constellation Pegasus.