HIP 97458
HIP 97458 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,294 light-years, HIP 97458 is a distant star lying deep within the Milky Way galaxy.
HIP 97458 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 97458 has an apparent magnitude of +9.18, 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 +1.295.
Physikalische Eigenschaften
| Spektralklasse | Class K — K-type (Orange) |
| Farbindex (B−V) | 1,295 |
Beobachtung
| Scheinbare Helligkeit | +9.18 |
| Absolute Helligkeit | 1,19 |
| Entfernung | 1,294 ly |
| Sternbild | Aquila |
Position
| Rektaszension | 19h 48,55m |
| Deklination | 13° 36,84′ |
Häufig gestellte Fragen
What type of star is HIP 97458?
HIP 97458 is a Class K — K-type (Orange) star.
How far is HIP 97458 from Earth?
HIP 97458 is approximately 1,294.3 light-years from Earth.
Can you see HIP 97458 with the naked eye?
With an apparent magnitude of 9.18, HIP 97458 is not visible to the naked eye.
What constellation is HIP 97458 in?
HIP 97458 is located in the constellation Aquila.