HIP 3869
HIP 3869 is a K-type (Orange) star.
At a distance of roughly 2,652 light-years, HIP 3869 is a distant star lying deep within the Milky Way galaxy.
HIP 3869 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 3869 has an apparent magnitude of +7.51, 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 +1.428.
Physical Properties
| Spectral Class | Class K — K-type (Orange) |
| Color Index (B−V) | 1.428 |
Observation
| Apparent Magnitude | +7.51 |
| Absolute Magnitude | -2.04 |
| Distance | 2,652 ly |
Position
| Right Ascension | 0h 49.67m |
| Declination | 6° 24.43′ |
Frequently Asked Questions
What type of star is HIP 3869?
HIP 3869 is a Class K — K-type (Orange) star.
How far is HIP 3869 from Earth?
HIP 3869 is approximately 2,651.7 light-years from Earth.
Can you see HIP 3869 with the naked eye?
With an apparent magnitude of 7.51, HIP 3869 is not visible to the naked eye.