HIP 4167
HIP 4167 is a K-type (Orange) star.
At a distance of roughly 1,907 light-years, HIP 4167 is a distant star lying deep within the Milky Way galaxy.
HIP 4167 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 4167 has an apparent magnitude of +8.54, 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 +1.537.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.537 |
Observation
| Apparent Magnitude | +8.54 |
| Absolute Magnitude | -0.30 |
| Distance | 1,907 ly |
Position
| Right Ascension | 0h 53.24m |
| Declination | 9° 54.87′ |
Frequently Asked Questions
What type of star is HIP 4167?
HIP 4167 is a Class K — K-type (Orange) star.
How far is HIP 4167 from Earth?
HIP 4167 is approximately 1,907.3 light-years from Earth.
Can you see HIP 4167 with the naked eye?
With an apparent magnitude of 8.54, HIP 4167 is not visible to the naked eye.