HIP 104387
HIP 104387 is a K-type (Orange) star.
At a distance of roughly 2,026 light-years, HIP 104387 is a distant star lying deep within the Milky Way galaxy.
HIP 104387 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104387 has an apparent magnitude of +8.14, 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 +1.401.
Physical Properties
| Spectral Class | K Class K — K-type (Orange) |
| Color Index (B−V) | 1.401 |
Observation
| Apparent Magnitude | +8.14 |
| Absolute Magnitude | -0.83 |
| Distance | 2,026 ly |
Position
| Right Ascension | 21h 8.83m |
| Declination | -18° 43.63′ |
Frequently Asked Questions
What type of star is HIP 104387?
HIP 104387 is a Class K — K-type (Orange) star.
How far is HIP 104387 from Earth?
HIP 104387 is approximately 2,025.8 light-years from Earth.
Can you see HIP 104387 with the naked eye?
With an apparent magnitude of 8.14, HIP 104387 is not visible to the naked eye.