HIP 15087
HIP 15087 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 93.4 light-years from Earth, HIP 15087 resides within the broader disk of our Milky Way galaxy.
HIP 15087 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
At an apparent magnitude of +10.30, HIP 15087 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its red hue, which corresponds to a B-V color index of +1.589.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,589 |
Observation
| Magnitude Apparente | +10.30 |
| Magnitude Absolue | 8,02 |
| Distance | 93.4 ly |
| Constellation | Perseus |
Position
| Ascension droite | 3h 14,57m |
| Déclinaison | 52° 20,90′ |
Questions fréquentes
What type of star is HIP 15087?
HIP 15087 is a Class K — K-type (Orange) star.
How far is HIP 15087 from Earth?
HIP 15087 is approximately 93.4 light-years from Earth.
Can you see HIP 15087 with the naked eye?
With an apparent magnitude of 10.30, HIP 15087 is not visible to the naked eye.
What constellation is HIP 15087 in?
HIP 15087 is located in the constellation Perseus.