HIP 104895
HIP 104895 is a K-type (Orange) star.
At a distance of roughly 1,489 light-years, HIP 104895 is a distant star lying deep within the Milky Way galaxy.
HIP 104895 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 104895 has an apparent magnitude of +9.17, 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 orange hue, which corresponds to a B-V color index of +1.033.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,033 |
Beobachtung
| Scheinbare Helligkeit | +9.17 |
| Absolute Helligkeit | 0,87 |
| Entfernung | 1,489 ly |
Position
| Rektaszension | 21h 14,89m |
| Deklination | 8° 59,62′ |
Frequently Asked Questions
What type of star is HIP 104895?
HIP 104895 is a Class K — K-type (Orange) star.
How far is HIP 104895 from Earth?
HIP 104895 is approximately 1,489.3 light-years from Earth.
Can you see HIP 104895 with the naked eye?
With an apparent magnitude of 9.17, HIP 104895 is not visible to the naked eye.