HIP 9886
HIP 9886 is a M-type (Red) star located in the constellation Perseus.
At a distance of roughly 1,864 light-years, HIP 9886 is a distant star lying deep within the Milky Way galaxy.
HIP 9886 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 9886 has an apparent magnitude of +8.61, 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 red hue, which corresponds to a B-V color index of +2.157.
Physical Properties
| Spectral Class | Class M — M-type (Red) |
| Color Index (B−V) | 2.157 |
Observation
| Apparent Magnitude | +8.61 |
| Absolute Magnitude | -0.18 |
| Distance | 1,864 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 7.20m |
| Declination | 58° 47.26′ |
Frequently Asked Questions
What type of star is HIP 9886?
HIP 9886 is a Class M — M-type (Red) star.
How far is HIP 9886 from Earth?
HIP 9886 is approximately 1,863.8 light-years from Earth.
Can you see HIP 9886 with the naked eye?
With an apparent magnitude of 8.61, HIP 9886 is not visible to the naked eye.
What constellation is HIP 9886 in?
HIP 9886 is located in the constellation Perseus.