HIP 94299
HIP 94299 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 1,173 light-years, HIP 94299 is a distant star lying deep within the Milky Way galaxy.
HIP 94299 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 94299 has an apparent magnitude of +8.14, 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 +0.139.
Physikalische Eigenschaften
| Spektralklasse | Class B — B-type (Blue-White) |
| Farbindex (B−V) | 0,139 |
Beobachtung
| Scheinbare Helligkeit | +8.14 |
| Absolute Helligkeit | 0,36 |
| Entfernung | 1,173 ly |
| Sternbild | Aquila |
Position
| Rektaszension | 19h 11,65m |
| Deklination | 11° 59,92′ |
Häufig gestellte Fragen
What type of star is HIP 94299?
HIP 94299 is a Class B — B-type (Blue-White) star.
How far is HIP 94299 from Earth?
HIP 94299 is approximately 1,173.2 light-years from Earth.
Can you see HIP 94299 with the naked eye?
With an apparent magnitude of 8.14, HIP 94299 is not visible to the naked eye.
What constellation is HIP 94299 in?
HIP 94299 is located in the constellation Aquila.