HIP 92409
HIP 92409 is a B-type (Blue-White) star located in the constellation Aquila.
HIP 92409 is an extraordinarily remote star, situated approximately 326,156 light-years from Earth.
HIP 92409 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 92409 has an apparent magnitude of +8.93, 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 +0.106.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,106 |
Observation
| Magnitude Apparente | +8.93 |
| Magnitude Absolue | -11,07 |
| Distance | 326,156 ly |
| Constellation | Aquila |
Position
| Ascension droite | 18h 49,91m |
| Déclinaison | 8° 31,18′ |
Questions fréquentes
What type of star is HIP 92409?
HIP 92409 is a Class B — B-type (Blue-White) star.
How far is HIP 92409 from Earth?
HIP 92409 is approximately 326,156.0 light-years from Earth.
Can you see HIP 92409 with the naked eye?
With an apparent magnitude of 8.93, HIP 92409 is not visible to the naked eye.
What constellation is HIP 92409 in?
HIP 92409 is located in the constellation Aquila.