HIP 18167
HIP 18167 is a G-type (Yellow) star located in the constellation Perseus.
Located approximately 662.9 light-years from Earth, HIP 18167 resides within the broader disk of our Milky Way galaxy.
HIP 18167 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 18167 has an apparent magnitude of +8.39, 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 +1.120.
Propriétés physiques
| Classe Spectrale | Class G — G-type (Yellow) |
| Indice de couleur (B−V) | 1,120 |
Observation
| Magnitude Apparente | +8.39 |
| Magnitude Absolue | 1,85 |
| Distance | 663 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 53,04m |
| Déclinaison | 52° 15,30′ |
Questions fréquentes
What type of star is HIP 18167?
HIP 18167 is a Class G — G-type (Yellow) star.
How far is HIP 18167 from Earth?
HIP 18167 is approximately 662.9 light-years from Earth.
Can you see HIP 18167 with the naked eye?
With an apparent magnitude of 8.39, HIP 18167 is not visible to the naked eye.
What constellation is HIP 18167 in?
HIP 18167 is located in the constellation Perseus.