HIP 16887
HIP 16887 is a K-type (Orange) star located in the constellation Cassiopeia.
Located approximately 192.2 light-years from Earth, HIP 16887 resides within the broader disk of our Milky Way galaxy.
HIP 16887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 16887 has an apparent magnitude of +9.29, 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 +0.824.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 0,824 |
Observation
| Magnitude Apparente | +9.29 |
| Magnitude Absolue | 5,44 |
| Distance | 192 ly |
| Constellation | Cassiopeia |
Position
| Ascension droite | 3h 37,31m |
| Déclinaison | 73° 5,01′ |
Questions fréquentes
What type of star is HIP 16887?
HIP 16887 is a Class K — K-type (Orange) star.
How far is HIP 16887 from Earth?
HIP 16887 is approximately 192.2 light-years from Earth.
Can you see HIP 16887 with the naked eye?
With an apparent magnitude of 9.29, HIP 16887 is not visible to the naked eye.
What constellation is HIP 16887 in?
HIP 16887 is located in the constellation Cassiopeia.