HIP 12492
HIP 12492 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,773 light-years, HIP 12492 is a distant star lying deep within the Milky Way galaxy.
HIP 12492 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 12492 has an apparent magnitude of +9.41, 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 blue-white hue, which corresponds to a B-V color index of +0.020.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | 0,020 |
Observação
| Magnitude Aparente | +9.41 |
| Magnitude Absoluta | 0,73 |
| Distância | 1,773 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 2h 40,71m |
| Declinação | 47° 13,08′ |
Perguntas frequentes
What type of star is HIP 12492?
HIP 12492 is a Class B — B-type (Blue-White) star.
How far is HIP 12492 from Earth?
HIP 12492 is approximately 1,772.6 light-years from Earth.
Can you see HIP 12492 with the naked eye?
With an apparent magnitude of 9.41, HIP 12492 is not visible to the naked eye.
What constellation is HIP 12492 in?
HIP 12492 is located in the constellation Perseus.