HIP 43887
HIP 43887 is a K-type (Orange) star.
At a distance of roughly 1,045 light-years, HIP 43887 is a distant star lying deep within the Milky Way galaxy.
HIP 43887 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 43887 has an apparent magnitude of +8.23, 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 +1.264.
Physikalische Eigenschaften
| Spektralklasse | K Class K — K-type (Orange) |
| Farbindex (B−V) | 1,264 |
Beobachtung
| Scheinbare Helligkeit | +8.23 |
| Absolute Helligkeit | 0,70 |
| Entfernung | 1,045 ly |
Position
| Rektaszension | 8h 56,42m |
| Deklination | -61° 52,69′ |
Frequently Asked Questions
What type of star is HIP 43887?
HIP 43887 is a Class K — K-type (Orange) star.
How far is HIP 43887 from Earth?
HIP 43887 is approximately 1,045.4 light-years from Earth.
Can you see HIP 43887 with the naked eye?
With an apparent magnitude of 8.23, HIP 43887 is not visible to the naked eye.