HIP 14887
HIP 14887 is a B-type (Blue-White) star located in the constellation Perseus.
Located approximately 653.6 light-years from Earth, HIP 14887 resides within the broader disk of our Milky Way galaxy.
HIP 14887 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 14887 has an apparent magnitude of +6.15, 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 hue, which corresponds to a B-V color index of -0.099.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.099 |
Observation
| Apparent Magnitude | +6.15 |
| Absolute Magnitude | -0.36 |
| Distance | 654 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 12.16m |
| Declination | 42° 22.55′ |
Frequently Asked Questions
What type of star is HIP 14887?
HIP 14887 is a Class B — B-type (Blue-White) star.
How far is HIP 14887 from Earth?
HIP 14887 is approximately 653.6 light-years from Earth.
Can you see HIP 14887 with the naked eye?
With an apparent magnitude of 6.15, HIP 14887 is not visible to the naked eye.
What constellation is HIP 14887 in?
HIP 14887 is located in the constellation Perseus.