HIP 17177
HIP 17177 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 2,051 light-years, HIP 17177 is a distant star lying deep within the Milky Way galaxy.
HIP 17177 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 17177 has an apparent magnitude of +8.68, 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 red hue, which corresponds to a B-V color index of +1.481.
Propiedades físicas
| Clase Espectral | Class K — K-type (Orange) |
| Índice de color (B−V) | 1,481 |
Observación
| Magnitud Aparente | +8.68 |
| Magnitud Absoluta | -0,31 |
| Distancia | 2,051 ly |
| Constelación | Perseus |
Posición
| Ascensión recta | 3h 40,75m |
| Declinación | 33° 38,08′ |
Preguntas frecuentes
What type of star is HIP 17177?
HIP 17177 is a Class K — K-type (Orange) star.
How far is HIP 17177 from Earth?
HIP 17177 is approximately 2,051.3 light-years from Earth.
Can you see HIP 17177 with the naked eye?
With an apparent magnitude of 8.68, HIP 17177 is not visible to the naked eye.
What constellation is HIP 17177 in?
HIP 17177 is located in the constellation Perseus.