HIP 10982
HIP 10982 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,274 light-years, HIP 10982 is a distant star lying deep within the Milky Way galaxy.
HIP 10982 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10982 has an apparent magnitude of +9.41, 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 +1.613.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.613 |
Observation
| Apparent Magnitude | +9.41 |
| Absolute Magnitude | 1.45 |
| Distance | 1,274 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 21.51m |
| Declination | 56° 11.01′ |
Frequently Asked Questions
What type of star is HIP 10982?
HIP 10982 is a Class K — K-type (Orange) star.
How far is HIP 10982 from Earth?
HIP 10982 is approximately 1,274.0 light-years from Earth.
Can you see HIP 10982 with the naked eye?
With an apparent magnitude of 9.41, HIP 10982 is not visible to the naked eye.
What constellation is HIP 10982 in?
HIP 10982 is located in the constellation Perseus.