HIP 102187
HIP 102187 is a K-type (Orange) star.
At a distance of roughly 1,102 light-years, HIP 102187 is a distant star lying deep within the Milky Way galaxy.
HIP 102187 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102187 has an apparent magnitude of +8.12, 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 yellow hue, which corresponds to a B-V color index of +0.971.
Propriétés physiques
| Classe Spectrale | K Class K — K-type (Orange) |
| Indice de couleur (B−V) | 0,971 |
Observation
| Magnitude Apparente | +8.12 |
| Magnitude Absolue | 0,48 |
| Distance | 1,102 ly |
Position
| Ascension droite | 20h 42,32m |
| Déclinaison | 57° 45,47′ |
Frequently Asked Questions
What type of star is HIP 102187?
HIP 102187 is a Class K — K-type (Orange) star.
How far is HIP 102187 from Earth?
HIP 102187 is approximately 1,101.9 light-years from Earth.
Can you see HIP 102187 with the naked eye?
With an apparent magnitude of 8.12, HIP 102187 is not visible to the naked eye.