HIP 59475
HIP 59475 is a K-type (Orange) star located in the constellation Centaurus.
At a distance of roughly 1,094 light-years, HIP 59475 is a distant star lying deep within the Milky Way galaxy.
HIP 59475 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 59475 has an apparent magnitude of +8.55, 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 +1.100.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,100 |
Beobachtung
| Scheinbare Helligkeit | +8.55 |
| Absolute Helligkeit | 0,92 |
| Entfernung | 1,094 ly |
| Sternbild | Centaurus |
Position
| Rektaszension | 12h 11,93m |
| Deklination | -51° 24,79′ |
Häufig gestellte Fragen
What type of star is HIP 59475?
HIP 59475 is a Class K — K-type (Orange) star.
How far is HIP 59475 from Earth?
HIP 59475 is approximately 1,094.5 light-years from Earth.
Can you see HIP 59475 with the naked eye?
With an apparent magnitude of 8.55, HIP 59475 is not visible to the naked eye.
What constellation is HIP 59475 in?
HIP 59475 is located in the constellation Centaurus.