HIP 18415
HIP 18415 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,026 light-years, HIP 18415 is a distant star lying deep within the Milky Way galaxy.
HIP 18415 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 18415 has an apparent magnitude of +8.96, 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 +0.128.
Propriedades físicas
| Classe Espectral | Class B — B-type (Blue-White) |
| Índice de cor (B−V) | 0,128 |
Observação
| Magnitude Aparente | +8.96 |
| Magnitude Absoluta | 1,47 |
| Distância | 1,026 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 56,21m |
| Declinação | 46° 57,14′ |
Perguntas frequentes
What type of star is HIP 18415?
HIP 18415 is a Class B — B-type (Blue-White) star.
How far is HIP 18415 from Earth?
HIP 18415 is approximately 1,025.6 light-years from Earth.
Can you see HIP 18415 with the naked eye?
With an apparent magnitude of 8.96, HIP 18415 is not visible to the naked eye.
What constellation is HIP 18415 in?
HIP 18415 is located in the constellation Perseus.