HIP 17409
HIP 17409 is a G-type (Yellow) star located in the constellation Perseus.
Located approximately 141.3 light-years from Earth, HIP 17409 resides within the broader disk of our Milky Way galaxy.
HIP 17409 is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
HIP 17409 has an apparent magnitude of +7.48, 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 white hue, which corresponds to a B-V color index of +0.583.
Propriedades físicas
| Classe Espectral | Class G — G-type (Yellow) |
| Índice de cor (B−V) | 0,583 |
Observação
| Magnitude Aparente | +7.48 |
| Magnitude Absoluta | 4,30 |
| Distância | 141 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 43,79m |
| Declinação | 42° 36,20′ |
Perguntas frequentes
What type of star is HIP 17409?
HIP 17409 is a Class G — G-type (Yellow) star.
How far is HIP 17409 from Earth?
HIP 17409 is approximately 141.3 light-years from Earth.
Can you see HIP 17409 with the naked eye?
With an apparent magnitude of 7.48, HIP 17409 is not visible to the naked eye.
What constellation is HIP 17409 in?
HIP 17409 is located in the constellation Perseus.