HIP 10808
HIP 10808 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,812 light-years, HIP 10808 is a distant star lying deep within the Milky Way galaxy.
HIP 10808 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 10808 has an apparent magnitude of +9.19, 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 +1.300.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,300 |
Beobachtung
| Scheinbare Helligkeit | +9.19 |
| Absolute Helligkeit | 0,47 |
| Entfernung | 1,812 ly |
| Sternbild | Cassiopeia |
Position
| Rektaszension | 2h 19,14m |
| Deklination | 59° 44,87′ |
Häufig gestellte Fragen
What type of star is HIP 10808?
HIP 10808 is a Class K — K-type (Orange) star.
How far is HIP 10808 from Earth?
HIP 10808 is approximately 1,812.0 light-years from Earth.
Can you see HIP 10808 with the naked eye?
With an apparent magnitude of 9.19, HIP 10808 is not visible to the naked eye.
What constellation is HIP 10808 in?
HIP 10808 is located in the constellation Cassiopeia.