HIP 97585
HIP 97585 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 3,020 light-years, HIP 97585 is a distant star lying deep within the Milky Way galaxy.
HIP 97585 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 97585 has an apparent magnitude of +8.77, 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 +1.658.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,658 |
Observation
| Magnitude Apparente | +8.77 |
| Magnitude Absolue | -1,06 |
| Distance | 3,020 ly |
| Constellation | Aquila |
Position
| Ascension droite | 19h 50,10m |
| Déclinaison | 0° 2,30′ |
Questions fréquentes
What type of star is HIP 97585?
HIP 97585 is a Class K — K-type (Orange) star.
How far is HIP 97585 from Earth?
HIP 97585 is approximately 3,020.0 light-years from Earth.
Can you see HIP 97585 with the naked eye?
With an apparent magnitude of 8.77, HIP 97585 is not visible to the naked eye.
What constellation is HIP 97585 in?
HIP 97585 is located in the constellation Aquila.