HIP 9168
HIP 9168 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 2,346 light-years, HIP 9168 is a distant star lying deep within the Milky Way galaxy.
HIP 9168 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 9168 has an apparent magnitude of +8.85, 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 +0.187.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.187 |
Observation
| Apparent Magnitude | +8.85 |
| Absolute Magnitude | -0.44 |
| Distance | 2,346 ly |
| Constellation | Perseus |
Position
| Right Ascension | 1h 58.05m |
| Declination | 57° 57.83′ |
Frequently Asked Questions
What type of star is HIP 9168?
HIP 9168 is a Class B — B-type (Blue-White) star.
How far is HIP 9168 from Earth?
HIP 9168 is approximately 2,346.4 light-years from Earth.
Can you see HIP 9168 with the naked eye?
With an apparent magnitude of 8.85, HIP 9168 is not visible to the naked eye.
What constellation is HIP 9168 in?
HIP 9168 is located in the constellation Perseus.