HIP 52102
HIP 52102 is a K-type (Orange) star.
At a distance of roughly 2,346 light-years, HIP 52102 is a distant star lying deep within the Milky Way galaxy.
HIP 52102 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +4.69, HIP 52102 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 +1.562.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.562 |
Observation
| Apparent Magnitude | +4.69 |
| Absolute Magnitude | -4.60 |
| Distance | 2,346 ly |
Position
| Right Ascension | 10h 38.75m |
| Declination | -59° 10.98′ |
Frequently Asked Questions
What type of star is HIP 52102?
HIP 52102 is a Class K — K-type (Orange) star.
How far is HIP 52102 from Earth?
HIP 52102 is approximately 2,346.4 light-years from Earth.
Can you see HIP 52102 with the naked eye?
With an apparent magnitude of 4.69, HIP 52102 is visible to the naked eye.