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.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,233 |
Observação
| Magnitude Aparente | +6.00 |
| Magnitude Absoluta | 1,08 |
| Distância | 315 ly |
| Constelação | Aquila |
Posição
| Ascensão reta | 19h 49,04m |
| Declinação | -10° 52,25′ |
Perguntas frequentes
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.