HIP 17308
HIP 17308 is a A-type (White) star located in the constellation Perseus.
At a distance of roughly 1,259 light-years, HIP 17308 is a distant star lying deep within the Milky Way galaxy.
HIP 17308 is classified as a spectral class A star (A-type (White)) on the Harvard spectral classification system.
HIP 17308 has an apparent magnitude of +9.24, 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 yellow-white hue, which corresponds to a B-V color index of +0.660.
Propiedades físicas
| Clase Espectral | Class A — A-type (White) |
| Índice de color (B−V) | 0,660 |
Observación
| Magnitud Aparente | +9.24 |
| Magnitud Absoluta | 1,31 |
| Distancia | 1,259 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 3h 42,30m |
| Declinación | 37° 16,04′ |
Preguntas frecuentes
What type of star is HIP 17308?
HIP 17308 is a Class A — A-type (White) star.
How far is HIP 17308 from Earth?
HIP 17308 is approximately 1,259.3 light-years from Earth.
Can you see HIP 17308 with the naked eye?
With an apparent magnitude of 9.24, HIP 17308 is not visible to the naked eye.
What constellation is HIP 17308 in?
HIP 17308 is located in the constellation Perseus.