HIP 8630
HIP 8630 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,382 light-years, HIP 8630 is a distant star lying deep within the Milky Way galaxy.
HIP 8630 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 8630 has an apparent magnitude of +9.77, 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 +0.541.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | 0,541 |
Observação
| Magnitude Aparente | +9.77 |
| Magnitude Absoluta | 1,64 |
| Distância | 1,382 ly |
| Constelação | Cassiopeia |
Posição
| Ascensão reta | 1h 51,32m |
| Declinação | 67° 37,89′ |
Perguntas frequentes
What type of star is HIP 8630?
HIP 8630 is a Class B — B-type (Blue-White) star.
How far is HIP 8630 from Earth?
HIP 8630 is approximately 1,382.0 light-years from Earth.
Can you see HIP 8630 with the naked eye?
With an apparent magnitude of 9.77, HIP 8630 is not visible to the naked eye.
What constellation is HIP 8630 in?
HIP 8630 is located in the constellation Cassiopeia.