HIP 12587
HIP 12587 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,109 light-years, HIP 12587 is a distant star lying deep within the Milky Way galaxy.
HIP 12587 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 12587 has an apparent magnitude of +7.69, 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 +1.660.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.660 |
Observation
| Apparent Magnitude | +7.69 |
| Absolute Magnitude | 0.03 |
| Distance | 1,109 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 41.88m |
| Declination | 45° 0.11′ |
Frequently Asked Questions
What type of star is HIP 12587?
HIP 12587 is a Class K — K-type (Orange) star.
How far is HIP 12587 from Earth?
HIP 12587 is approximately 1,109.4 light-years from Earth.
Can you see HIP 12587 with the naked eye?
With an apparent magnitude of 7.69, HIP 12587 is not visible to the naked eye.
What constellation is HIP 12587 in?
HIP 12587 is located in the constellation Perseus.