HIP 96400
HIP 96400 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 1,294 light-years, HIP 96400 is a distant star lying deep within the Milky Way galaxy.
HIP 96400 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 96400 has an apparent magnitude of +8.70, 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 white hue, which corresponds to a B-V color index of +0.310.
Propriétés physiques
| Classe Spectrale | Class B — B-type (Blue-White) |
| Indice de couleur (B−V) | 0,310 |
Observation
| Magnitude Apparente | +8.70 |
| Magnitude Absolue | 0,71 |
| Distance | 1,294 ly |
| Constellation | Aquila |
Position
| Ascension droite | 19h 35,97m |
| Déclinaison | 14° 49,47′ |
Questions fréquentes
What type of star is HIP 96400?
HIP 96400 is a Class B — B-type (Blue-White) star.
How far is HIP 96400 from Earth?
HIP 96400 is approximately 1,294.3 light-years from Earth.
Can you see HIP 96400 with the naked eye?
With an apparent magnitude of 8.70, HIP 96400 is not visible to the naked eye.
What constellation is HIP 96400 in?
HIP 96400 is located in the constellation Aquila.