HIP 13252
HIP 13252 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 1,699 light-years, HIP 13252 is a distant star lying deep within the Milky Way galaxy.
HIP 13252 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 13252 has an apparent magnitude of +8.41, 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 +1.652.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.652 |
Observation
| Apparent Magnitude | +8.41 |
| Absolute Magnitude | -0.17 |
| Distance | 1,699 ly |
| Constellation | Perseus |
Position
| Right Ascension | 2h 50.56m |
| Declination | 36° 17.81′ |
Frequently Asked Questions
What type of star is HIP 13252?
HIP 13252 is a Class K — K-type (Orange) star.
How far is HIP 13252 from Earth?
HIP 13252 is approximately 1,698.7 light-years from Earth.
Can you see HIP 13252 with the naked eye?
With an apparent magnitude of 8.41, HIP 13252 is not visible to the naked eye.
What constellation is HIP 13252 in?
HIP 13252 is located in the constellation Perseus.