HIP 17887
HIP 17887 is a G-type (Yellow) star.
Located approximately 223.6 light-years from Earth, HIP 17887 resides within the broader disk of our Milky Way galaxy.
HIP 17887 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 17887 has an apparent magnitude of +9.01, 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 white hue, which corresponds to a B-V color index of +0.582.
Propriétés physiques
| Classe Spectrale | G Class G — G-type (Yellow) |
| Indice de couleur (B−V) | 0,582 |
Observation
| Magnitude Apparente | +9.01 |
| Magnitude Absolue | 4,83 |
| Distance | 224 ly |
Position
| Ascension droite | 3h 49,58m |
| Déclinaison | 58° 46,09′ |
Frequently Asked Questions
What type of star is HIP 17887?
HIP 17887 is a Class G — G-type (Yellow) star.
How far is HIP 17887 from Earth?
HIP 17887 is approximately 223.6 light-years from Earth.
Can you see HIP 17887 with the naked eye?
With an apparent magnitude of 9.01, HIP 17887 is not visible to the naked eye.