HIP 92475
HIP 92475 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,259 light-years, HIP 92475 is a distant star lying deep within the Milky Way galaxy.
HIP 92475 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 92475 has an apparent magnitude of +6.37, 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 +1.443.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,443 |
Beobachtung
| Scheinbare Helligkeit | +6.37 |
| Absolute Helligkeit | -1,56 |
| Entfernung | 1,259 ly |
| Sternbild | Aquila |
Position
| Rektaszension | 18h 50,76m |
| Deklination | 10° 58,58′ |
Häufig gestellte Fragen
What type of star is HIP 92475?
HIP 92475 is a Class K — K-type (Orange) star.
How far is HIP 92475 from Earth?
HIP 92475 is approximately 1,259.3 light-years from Earth.
Can you see HIP 92475 with the naked eye?
With an apparent magnitude of 6.37, HIP 92475 is not visible to the naked eye.
What constellation is HIP 92475 in?
HIP 92475 is located in the constellation Aquila.