HIP 106890
HIP 106890 is a B-type (Blue-White) star.
At a distance of roughly 2,568 light-years, HIP 106890 is a distant star lying deep within the Milky Way galaxy.
HIP 106890 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 106890 has an apparent magnitude of +8.10, 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 +0.240.
Physical Properties
| Spectral Class | Class B — B-type (Blue-White) |
| Color Index (B−V) | 0.240 |
Observation
| Apparent Magnitude | +8.10 |
| Absolute Magnitude | -1.38 |
| Distance | 2,568 ly |
Position
| Right Ascension | 21h 38.98m |
| Declination | 57° 29.24′ |
Frequently Asked Questions
What type of star is HIP 106890?
HIP 106890 is a Class B — B-type (Blue-White) star.
How far is HIP 106890 from Earth?
HIP 106890 is approximately 2,568.2 light-years from Earth.
Can you see HIP 106890 with the naked eye?
With an apparent magnitude of 8.10, HIP 106890 is not visible to the naked eye.