HIP 14350
HIP 14350 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 2,297 light-years, HIP 14350 is a distant star lying deep within the Milky Way galaxy.
HIP 14350 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 14350 has an apparent magnitude of +7.13, 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 +1.863.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,863 |
Observação
| Magnitude Aparente | +7.13 |
| Magnitude Absoluta | -2,11 |
| Distância | 2,297 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 5,06m |
| Declinação | 52° 37,70′ |
Perguntas frequentes
What type of star is HIP 14350?
HIP 14350 is a Class K — K-type (Orange) star.
How far is HIP 14350 from Earth?
HIP 14350 is approximately 2,296.9 light-years from Earth.
Can you see HIP 14350 with the naked eye?
With an apparent magnitude of 7.13, HIP 14350 is not visible to the naked eye.
What constellation is HIP 14350 in?
HIP 14350 is located in the constellation Perseus.