HIP 19178
HIP 19178 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,035 light-years, HIP 19178 is a distant star lying deep within the Milky Way galaxy.
HIP 19178 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 19178 has an apparent magnitude of +7.05, 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 +0.035.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | 0,035 |
Observación
| Magnitud Aparente | +7.05 |
| Magnitud Absoluta | -0,46 |
| Distancia | 1,035 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 4h 6,65m |
| Declinación | 32° 23,10′ |
Preguntas frecuentes
What type of star is HIP 19178?
HIP 19178 is a Class B — B-type (Blue-White) star.
How far is HIP 19178 from Earth?
HIP 19178 is approximately 1,035.4 light-years from Earth.
Can you see HIP 19178 with the naked eye?
With an apparent magnitude of 7.05, HIP 19178 is not visible to the naked eye.
What constellation is HIP 19178 in?
HIP 19178 is located in the constellation Perseus.