HIP 5225
HIP 5225 is a K-type (Orange) star.
At a distance of roughly 1,989 light-years, HIP 5225 is a distant star lying deep within the Milky Way galaxy.
HIP 5225 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 5225 has an apparent magnitude of +8.83, 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 +1.123.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.123 |
Observation
| Apparent Magnitude | +8.83 |
| Absolute Magnitude | -0.10 |
| Distance | 1,989 ly |
Position
| Right Ascension | 1h 6.79m |
| Declination | 0° 56.26′ |
Frequently Asked Questions
What type of star is HIP 5225?
HIP 5225 is a Class K — K-type (Orange) star.
How far is HIP 5225 from Earth?
HIP 5225 is approximately 1,988.8 light-years from Earth.
Can you see HIP 5225 with the naked eye?
With an apparent magnitude of 8.83, HIP 5225 is not visible to the naked eye.