HIP 3487
HIP 3487 is a B-type (Blue-White) star located in the constellation Cassiopeia.
At a distance of roughly 1,121 light-years, HIP 3487 is a distant star lying deep within the Milky Way galaxy.
HIP 3487 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 3487 has an apparent magnitude of +9.64, 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 +0.200.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | 0,200 |
Observación
| Magnitud Aparente | +9.64 |
| Magnitud Absoluta | 1,96 |
| Distancia | 1,121 ly |
| Constelación | Cassiopeia |
Posición
| Ascensión recta | 0h 44,51m |
| Declinación | 61° 46,83′ |
Preguntas frecuentes
What type of star is HIP 3487?
HIP 3487 is a Class B — B-type (Blue-White) star.
How far is HIP 3487 from Earth?
HIP 3487 is approximately 1,120.8 light-years from Earth.
Can you see HIP 3487 with the naked eye?
With an apparent magnitude of 9.64, HIP 3487 is not visible to the naked eye.
What constellation is HIP 3487 in?
HIP 3487 is located in the constellation Cassiopeia.