HIP 17450
HIP 17450 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,140 light-years, HIP 17450 is a distant star lying deep within the Milky Way galaxy.
HIP 17450 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 17450 has an apparent magnitude of +8.63, 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 +0.167.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | 0,167 |
Observação
| Magnitude Aparente | +8.63 |
| Magnitude Absoluta | 0,91 |
| Distância | 1,140 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 44,43m |
| Declinação | 44° 21,43′ |
Perguntas frequentes
What type of star is HIP 17450?
HIP 17450 is a Class B — B-type (Blue-White) star.
How far is HIP 17450 from Earth?
HIP 17450 is approximately 1,140.4 light-years from Earth.
Can you see HIP 17450 with the naked eye?
With an apparent magnitude of 8.63, HIP 17450 is not visible to the naked eye.
What constellation is HIP 17450 in?
HIP 17450 is located in the constellation Perseus.