HIP 15429
HIP 15429 is a B-type (Blue-White) star located in the constellation Perseus.
At a distance of roughly 1,843 light-years, HIP 15429 is a distant star lying deep within the Milky Way galaxy.
HIP 15429 is classified as a spectral class B star (B-type (Blue-White)) on the Harvard spectral classification system.
HIP 15429 has an apparent magnitude of +9.75, 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 +0.590.
Propiedades físicas
| Clase Espectral | Class B — B-type (Blue-White) |
| Índice de color (B−V) | 0,590 |
Observación
| Magnitud Aparente | +9.75 |
| Magnitud Absoluta | 0,99 |
| Distancia | 1,843 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 3h 18,87m |
| Declinación | 52° 1,80′ |
Preguntas frecuentes
What type of star is HIP 15429?
HIP 15429 is a Class B — B-type (Blue-White) star.
How far is HIP 15429 from Earth?
HIP 15429 is approximately 1,842.7 light-years from Earth.
Can you see HIP 15429 with the naked eye?
With an apparent magnitude of 9.75, HIP 15429 is not visible to the naked eye.
What constellation is HIP 15429 in?
HIP 15429 is located in the constellation Perseus.