HIP 94090
HIP 94090 is a B-type (Blue-White) star located in the constellation Aquila.
At a distance of roughly 2,812 light-years, HIP 94090 is a distant star lying deep within the Milky Way galaxy.
HIP 94090 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 94090 has an apparent magnitude of +8.66, 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 +0.157.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.157 |
Observation
| Apparent Magnitude | +8.66 |
| Absolute Magnitude | -1.02 |
| Distance | 2,812 ly |
| Constellation | Aquila |
Position
| Right Ascension | 19h 9.25m |
| Declination | -10° 13.07′ |
Frequently Asked Questions
What type of star is HIP 94090?
HIP 94090 is a Class B — B-type (Blue-White) star.
How far is HIP 94090 from Earth?
HIP 94090 is approximately 2,811.7 light-years from Earth.
Can you see HIP 94090 with the naked eye?
With an apparent magnitude of 8.66, HIP 94090 is not visible to the naked eye.
What constellation is HIP 94090 in?
HIP 94090 is located in the constellation Aquila.