HIP 56125
HIP 56125 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 2,330 light-years, HIP 56125 is a distant star lying deep within the Milky Way galaxy.
HIP 56125 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 56125 has an apparent magnitude of +8.38, 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 +1.579.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,579 |
Beobachtung
| Scheinbare Helligkeit | +8.38 |
| Absolute Helligkeit | -0,89 |
| Entfernung | 2,330 ly |
| Sternbild | Centaurus |
Position
| Rektaszension | 11h 30,31m |
| Deklination | -42° 9,01′ |
Häufig gestellte Fragen
What type of star is HIP 56125?
HIP 56125 is a Class K — K-type (Orange) star.
How far is HIP 56125 from Earth?
HIP 56125 is approximately 2,329.7 light-years from Earth.
Can you see HIP 56125 with the naked eye?
With an apparent magnitude of 8.38, HIP 56125 is not visible to the naked eye.
What constellation is HIP 56125 in?
HIP 56125 is located in the constellation Centaurus.