HIP 51495
HIP 51495 is a K-type (Orange) star.
At a distance of roughly 1,032 light-years, HIP 51495 is a distant star lying deep within the Milky Way galaxy.
HIP 51495 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
With an apparent magnitude of +4.94, HIP 51495 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 +1.677.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.677 |
Observation
| Apparent Magnitude | +4.94 |
| Absolute Magnitude | -2.56 |
| Distance | 1,032 ly |
Position
| Right Ascension | 10h 31.03m |
| Declination | -73° 13.29′ |
Frequently Asked Questions
What type of star is HIP 51495?
HIP 51495 is a Class K — K-type (Orange) star.
How far is HIP 51495 from Earth?
HIP 51495 is approximately 1,032.1 light-years from Earth.
Can you see HIP 51495 with the naked eye?
With an apparent magnitude of 4.94, HIP 51495 is visible to the naked eye.