HIP 102408
HIP 102408 is a K-type (Orange) star.
At a distance of roughly 2,265 light-years, HIP 102408 is a distant star lying deep within the Milky Way galaxy.
HIP 102408 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102408 has an apparent magnitude of +8.56, 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 +1.442.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.442 |
Observation
| Apparent Magnitude | +8.56 |
| Absolute Magnitude | -0.65 |
| Distance | 2,265 ly |
Position
| Right Ascension | 20h 45.15m |
| Declination | -47° 16.99′ |
Frequently Asked Questions
What type of star is HIP 102408?
HIP 102408 is a Class K — K-type (Orange) star.
How far is HIP 102408 from Earth?
HIP 102408 is approximately 2,265.0 light-years from Earth.
Can you see HIP 102408 with the naked eye?
With an apparent magnitude of 8.56, HIP 102408 is not visible to the naked eye.