HIP 18636
HIP 18636 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,084 light-years, HIP 18636 is a distant star lying deep within the Milky Way galaxy.
HIP 18636 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 18636 has an apparent magnitude of +8.46, 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 orange hue, which corresponds to a B-V color index of +1.052.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.052 |
Observation
| Apparent Magnitude | +8.46 |
| Absolute Magnitude | 0.85 |
| Distance | 1,084 ly |
| Constellation | Perseus |
Position
| Right Ascension | 3h 59.35m |
| Declination | 43° 21.65′ |
Frequently Asked Questions
What type of star is HIP 18636?
HIP 18636 is a Class K — K-type (Orange) star.
How far is HIP 18636 from Earth?
HIP 18636 is approximately 1,083.6 light-years from Earth.
Can you see HIP 18636 with the naked eye?
With an apparent magnitude of 8.46, HIP 18636 is not visible to the naked eye.
What constellation is HIP 18636 in?
HIP 18636 is located in the constellation Perseus.