HIP 52900
HIP 52900 is a K-type (Orange) star.
At a distance of roughly 1,763 light-years, HIP 52900 is a distant star lying deep within the Milky Way galaxy.
HIP 52900 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 52900 has an apparent magnitude of +9.20, 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 +1.573.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.573 |
Observation
| Apparent Magnitude | +9.20 |
| Absolute Magnitude | 0.54 |
| Distance | 1,763 ly |
Position
| Right Ascension | 10h 49.17m |
| Declination | -35° 56.67′ |
Frequently Asked Questions
What type of star is HIP 52900?
HIP 52900 is a Class K — K-type (Orange) star.
How far is HIP 52900 from Earth?
HIP 52900 is approximately 1,763.0 light-years from Earth.
Can you see HIP 52900 with the naked eye?
With an apparent magnitude of 9.20, HIP 52900 is not visible to the naked eye.