HIP 18108
HIP 18108 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,019 light-years, HIP 18108 is a distant star lying deep within the Milky Way galaxy.
HIP 18108 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 18108 has an apparent magnitude of +8.95, 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 +0.490.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.490 |
Observation
| Apparent Magnitude | +8.95 |
| Absolute Magnitude | 1.48 |
| Distance | 1,019 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 52.27m |
| Declination | 33° 24.37′ |
Frequently Asked Questions
What type of star is HIP 18108?
HIP 18108 is a Class B — B-type (Blue-White) star.
How far is HIP 18108 from Earth?
HIP 18108 is approximately 1,019.2 light-years from Earth.
Can you see HIP 18108 with the naked eye?
With an apparent magnitude of 8.95, HIP 18108 is not visible to the naked eye.
What constellation is HIP 18108 in?
HIP 18108 is located in the constellation Perseus.