HIP 97499
HIP 97499 is a K-type (Orange) star located in the constellation Aquila.
Located approximately 314.5 light-years from Earth, HIP 97499 resides within the broader disk of our Milky Way galaxy.
HIP 97499 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 97499 has an apparent magnitude of +6.00, 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 +1.233.
Propriétés physiques
| Classe Spectrale | Class K — K-type (Orange) |
| Indice de couleur (B−V) | 1,233 |
Observation
| Magnitude Apparente | +6.00 |
| Magnitude Absolue | 1,08 |
| Distance | 315 ly |
| Constellation | Aquila |
Position
| Ascension droite | 19h 49,04m |
| Déclinaison | -10° 52,25′ |
Questions fréquentes
What type of star is HIP 97499?
HIP 97499 is a Class K — K-type (Orange) star.
How far is HIP 97499 from Earth?
HIP 97499 is approximately 314.5 light-years from Earth.
Can you see HIP 97499 with the naked eye?
With an apparent magnitude of 6.00, HIP 97499 is visible to the naked eye.
What constellation is HIP 97499 in?
HIP 97499 is located in the constellation Aquila.