HIP 102185
HIP 102185 is a B-type (Blue-White) star.
At a distance of roughly 1,517 light-years, HIP 102185 is a distant star lying deep within the Milky Way galaxy.
HIP 102185 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 102185 has an apparent magnitude of +9.20, 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 -0.016.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | -0.016 |
Observation
| Apparent Magnitude | +9.20 |
| Absolute Magnitude | 0.86 |
| Distance | 1,517 ly |
Position
| Right Ascension | 20h 42.29m |
| Declination | 25° 17.92′ |
Frequently Asked Questions
What type of star is HIP 102185?
HIP 102185 is a Class B — B-type (Blue-White) star.
How far is HIP 102185 from Earth?
HIP 102185 is approximately 1,517.0 light-years from Earth.
Can you see HIP 102185 with the naked eye?
With an apparent magnitude of 9.20, HIP 102185 is not visible to the naked eye.