HIP 18111
HIP 18111 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 886.3 light-years from Earth, HIP 18111 resides within the broader disk of our Milky Way galaxy.
HIP 18111 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 18111 has an apparent magnitude of +7.43, 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 +0.044.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.044 |
Observation
| Apparent Magnitude | +7.43 |
| Absolute Magnitude | 0.26 |
| Distance | 886 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 52.32m |
| Declination | 34° 13.33′ |
Frequently Asked Questions
What type of star is HIP 18111?
HIP 18111 is a Class B — B-type (Blue-White) star.
How far is HIP 18111 from Earth?
HIP 18111 is approximately 886.3 light-years from Earth.
Can you see HIP 18111 with the naked eye?
With an apparent magnitude of 7.43, HIP 18111 is not visible to the naked eye.
What constellation is HIP 18111 in?
HIP 18111 is located in the constellation Perseus.