HIP 102111
HIP 102111 is a A-type (White) star.
At a distance of roughly 1,080 light-years, HIP 102111 is a distant star lying deep within the Milky Way galaxy.
HIP 102111 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
At an apparent magnitude of +10.48, HIP 102111 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 white hue, which corresponds to a B-V color index of +0.489.
Propriétés physiques
| Classe Spectrale | Class A — A-type (White) |
| Indice de couleur (B−V) | 0,489 |
Observation
| Magnitude Apparente | +10.48 |
| Magnitude Absolue | 2,88 |
| Distance | 1,080 ly |
Position
| Ascension droite | 20h 41,58m |
| Déclinaison | 59° 59,20′ |
Questions fréquentes
What type of star is HIP 102111?
HIP 102111 is a Class A — A-type (White) star.
How far is HIP 102111 from Earth?
HIP 102111 is approximately 1,080.0 light-years from Earth.
Can you see HIP 102111 with the naked eye?
With an apparent magnitude of 10.48, HIP 102111 is not visible to the naked eye.