HIP 7218
HIP 7218 is a K-type (Orange) star.
At a distance of roughly 1,631 light-years, HIP 7218 is a distant star lying deep within the Milky Way galaxy.
HIP 7218 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7218 has an apparent magnitude of +7.92, 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 +1.524.
Propiedades físicas
| Clase Espectral | Class K — K-type (Orange) |
| Índice de color (B−V) | 1,524 |
Observación
| Magnitud Aparente | +7.92 |
| Magnitud Absoluta | -0,58 |
| Distancia | 1,631 ly |
Posición
| Ascensión recta | 1h 32,98m |
| Declinación | 0° 7,62′ |
Preguntas frecuentes
What type of star is HIP 7218?
HIP 7218 is a Class K — K-type (Orange) star.
How far is HIP 7218 from Earth?
HIP 7218 is approximately 1,630.8 light-years from Earth.
Can you see HIP 7218 with the naked eye?
With an apparent magnitude of 7.92, HIP 7218 is not visible to the naked eye.