HIP 17869
HIP 17869 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 772.9 light-years from Earth, HIP 17869 resides within the broader disk of our Milky Way galaxy.
HIP 17869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17869 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 orange hue, which corresponds to a B-V color index of +1.032.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,032 |
Observation
| Magnitude Apparente | +8.26 |
| Magnitude Absolue | 1,39 |
| Distance | 773 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 49,41m |
| Déclinaison | 50° 56,19′ |
Questions fréquentes
What type of star is HIP 17869?
HIP 17869 is a Class K — K-type (Orange) star.
How far is HIP 17869 from Earth?
HIP 17869 is approximately 772.9 light-years from Earth.
Can you see HIP 17869 with the naked eye?
With an apparent magnitude of 8.26, HIP 17869 is not visible to the naked eye.
What constellation is HIP 17869 in?
HIP 17869 is located in the constellation Perseus.