HIP 18090
HIP 18090 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 109.5 light-years from Earth, HIP 18090 resides within the broader disk of our Milky Way galaxy.
HIP 18090 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 18090 has an apparent magnitude of +9.47, 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 orange hue, which corresponds to a B-V color index of +1.070.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,070 |
Observação
| Magnitude Aparente | +9.47 |
| Magnitude Absoluta | 6,84 |
| Distância | 110 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 3h 52,00m |
| Declinação | 39° 47,74′ |
Perguntas frequentes
What type of star is HIP 18090?
HIP 18090 is a Class K — K-type (Orange) star.
How far is HIP 18090 from Earth?
HIP 18090 is approximately 109.5 light-years from Earth.
Can you see HIP 18090 with the naked eye?
With an apparent magnitude of 9.47, HIP 18090 is not visible to the naked eye.
What constellation is HIP 18090 in?
HIP 18090 is located in the constellation Perseus.