HIP 115218
HIP 115218 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,059 light-years, HIP 115218 is a distant star lying deep within the Milky Way galaxy.
HIP 115218 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 115218 has an apparent magnitude of +6.39, 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 +1.678.
Propiedades físicas
| Clase Espectral | Class K — K-type (Orange) |
| Índice de color (B−V) | 1,678 |
Observación
| Magnitud Aparente | +6.39 |
| Magnitud Absoluta | -1,17 |
| Distancia | 1,059 ly |
| Constelación | Cassiopeia |
Posición
| Ascensión recta | 23h 20,24m |
| Declinación | 61° 58,21′ |
Preguntas frecuentes
What type of star is HIP 115218?
HIP 115218 is a Class K — K-type (Orange) star.
How far is HIP 115218 from Earth?
HIP 115218 is approximately 1,059.0 light-years from Earth.
Can you see HIP 115218 with the naked eye?
With an apparent magnitude of 6.39, HIP 115218 is not visible to the naked eye.
What constellation is HIP 115218 in?
HIP 115218 is located in the constellation Cassiopeia.