HIP 109025
HIP 109025 is a K-type (Orange) star located in the constellation Pegasus.
At a distance of roughly 2,416 light-years, HIP 109025 is a distant star lying deep within the Milky Way galaxy.
HIP 109025 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 109025 has an apparent magnitude of +8.39, 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 +1.347.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,347 |
Beobachtung
| Scheinbare Helligkeit | +8.39 |
| Absolute Helligkeit | -0,96 |
| Entfernung | 2,416 ly |
| Sternbild | Pegasus |
Position
| Rektaszension | 22h 5,22m |
| Deklination | 9° 11,06′ |
Häufig gestellte Fragen
What type of star is HIP 109025?
HIP 109025 is a Class K — K-type (Orange) star.
How far is HIP 109025 from Earth?
HIP 109025 is approximately 2,416.0 light-years from Earth.
Can you see HIP 109025 with the naked eye?
With an apparent magnitude of 8.39, HIP 109025 is not visible to the naked eye.
What constellation is HIP 109025 in?
HIP 109025 is located in the constellation Pegasus.