HIP 18270
HIP 18270 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,000 light-years, HIP 18270 is a distant star lying deep within the Milky Way galaxy.
HIP 18270 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 18270 has an apparent magnitude of +8.29, 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 hue, which corresponds to a B-V color index of -0.400.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | -0,400 |
Observación
| Magnitud Aparente | +8.29 |
| Magnitud Absoluta | 0,86 |
| Distancia | 1,000 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 3h 54,49m |
| Declinación | 45° 46,89′ |
Preguntas frecuentes
What type of star is HIP 18270?
HIP 18270 is a Class B — B-type (Blue-White) star.
How far is HIP 18270 from Earth?
HIP 18270 is approximately 1,000.5 light-years from Earth.
Can you see HIP 18270 with the naked eye?
With an apparent magnitude of 8.29, HIP 18270 is not visible to the naked eye.
What constellation is HIP 18270 in?
HIP 18270 is located in the constellation Perseus.