HIP 17490
HIP 17490 is a F-type (Yellow-White) star located in the constellation Perseus.
At a distance of roughly 1,195 light-years, HIP 17490 is a distant star lying deep within the Milky Way galaxy.
HIP 17490 is classified as a spectral class F star (F-type (Yellow-White)) on the Harvard spectral classification system.
HIP 17490 has an apparent magnitude of +8.33, 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 yellow-white hue, which corresponds to a B-V color index of +0.731.
Propriedades físicas
| Classe Espectral | Class F — F-type (Yellow-White) |
| Índice de cor (B−V) | 0,731 |
Observação
| Magnitude Aparente | +8.33 |
| Magnitude Absoluta | 0,51 |
| Distância | 1,195 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 44,80m |
| Declinação | 40° 56,32′ |
Perguntas frequentes
What type of star is HIP 17490?
HIP 17490 is a Class F — F-type (Yellow-White) star.
How far is HIP 17490 from Earth?
HIP 17490 is approximately 1,194.7 light-years from Earth.
Can you see HIP 17490 with the naked eye?
With an apparent magnitude of 8.33, HIP 17490 is not visible to the naked eye.
What constellation is HIP 17490 in?
HIP 17490 is located in the constellation Perseus.