HIP 7418
HIP 7418 is a K-type (Orange) star located in the constellation Cassiopeia.
At a distance of roughly 1,125 light-years, HIP 7418 is a distant star lying deep within the Milky Way galaxy.
HIP 7418 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 7418 has an apparent magnitude of +8.57, 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 +1.560.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,560 |
Observação
| Magnitude Aparente | +8.57 |
| Magnitude Absoluta | 0,88 |
| Distância | 1,125 ly |
| Constelação | Cassiopeia |
Posição
| Ascensão reta | 1h 35,61m |
| Declinação | 61° 28,59′ |
Perguntas frequentes
What type of star is HIP 7418?
HIP 7418 is a Class K — K-type (Orange) star.
How far is HIP 7418 from Earth?
HIP 7418 is approximately 1,124.7 light-years from Earth.
Can you see HIP 7418 with the naked eye?
With an apparent magnitude of 8.57, HIP 7418 is not visible to the naked eye.
What constellation is HIP 7418 in?
HIP 7418 is located in the constellation Cassiopeia.