HIP 92675
HIP 92675 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 2,104 light-years, HIP 92675 is a distant star lying deep within the Milky Way galaxy.
HIP 92675 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 92675 has an apparent magnitude of +8.15, 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 blue-white hue, which corresponds to a B-V color index of +0.111.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,111 |
Observation
| Magnitude Apparente | +8.15 |
| Magnitude Absolue | -0,90 |
| Distance | 2,104 ly |
| Constellation | Aquila |
Position
| Ascension droite | 18h 53,03m |
| Déclinaison | 8° 43,43′ |
Questions fréquentes
What type of star is HIP 92675?
HIP 92675 is a Class B — B-type (Blue-White) star.
How far is HIP 92675 from Earth?
HIP 92675 is approximately 2,104.2 light-years from Earth.
Can you see HIP 92675 with the naked eye?
With an apparent magnitude of 8.15, HIP 92675 is not visible to the naked eye.
What constellation is HIP 92675 in?
HIP 92675 is located in the constellation Aquila.