HIP 10630
HIP 10630 is a K-type (Orange) star.
At a distance of roughly 2,398 light-years, HIP 10630 is a distant star lying deep within the Milky Way galaxy.
HIP 10630 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10630 has an apparent magnitude of +8.77, 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 +1.235.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.235 |
Observation
| Apparent Magnitude | +8.77 |
| Absolute Magnitude | -0.56 |
| Distance | 2,398 ly |
Position
| Right Ascension | 2h 16.83m |
| Declination | -2° 54.26′ |
Frequently Asked Questions
What type of star is HIP 10630?
HIP 10630 is a Class K — K-type (Orange) star.
How far is HIP 10630 from Earth?
HIP 10630 is approximately 2,398.2 light-years from Earth.
Can you see HIP 10630 with the naked eye?
With an apparent magnitude of 8.77, HIP 10630 is not visible to the naked eye.