HIP 18488
HIP 18488 is a K-type (Orange) star.
At a distance of roughly 1,463 light-years, HIP 18488 is a distant star lying deep within the Milky Way galaxy.
HIP 18488 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +4.99, HIP 18488 sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its red hue, which corresponds to a B-V color index of +1.435.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.435 |
Observation
| Apparent Magnitude | +4.99 |
| Absolute Magnitude | -3.27 |
| Distance | 1,463 ly |
Position
| Right Ascension | 3h 57.14m |
| Declination | 61° 6.53′ |
Frequently Asked Questions
What type of star is HIP 18488?
HIP 18488 is a Class K — K-type (Orange) star.
How far is HIP 18488 from Earth?
HIP 18488 is approximately 1,462.6 light-years from Earth.
Can you see HIP 18488 with the naked eye?
With an apparent magnitude of 4.99, HIP 18488 is visible to the naked eye.