HIP 92125
HIP 92125 is a K-type (Orange) star located in the constellation Aquila.
At a distance of roughly 1,773 light-years, HIP 92125 is a distant star lying deep within the Milky Way galaxy.
HIP 92125 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 92125 has an apparent magnitude of +8.66, 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 +1.668.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,668 |
Observação
| Magnitude Aparente | +8.66 |
| Magnitude Absoluta | -0,02 |
| Distância | 1,773 ly |
| Constelação | Aquila |
Posição
| Ascensão reta | 18h 46,60m |
| Declinação | 12° 7,02′ |
Perguntas frequentes
What type of star is HIP 92125?
HIP 92125 is a Class K — K-type (Orange) star.
How far is HIP 92125 from Earth?
HIP 92125 is approximately 1,772.6 light-years from Earth.
Can you see HIP 92125 with the naked eye?
With an apparent magnitude of 8.66, HIP 92125 is not visible to the naked eye.
What constellation is HIP 92125 in?
HIP 92125 is located in the constellation Aquila.