HIP 9089
HIP 9089 is a K-type (Orange) star located in the constellation Perseus.
Located approximately 521.9 light-years from Earth, HIP 9089 resides within the broader disk of our Milky Way galaxy.
HIP 9089 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9089 has an apparent magnitude of +9.21, 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 +1.252.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,252 |
Observação
| Magnitude Aparente | +9.21 |
| Magnitude Absoluta | 3,19 |
| Distância | 522 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 1h 57,08m |
| Declinação | 50° 56,97′ |
Perguntas frequentes
What type of star is HIP 9089?
HIP 9089 is a Class K — K-type (Orange) star.
How far is HIP 9089 from Earth?
HIP 9089 is approximately 521.8 light-years from Earth.
Can you see HIP 9089 with the naked eye?
With an apparent magnitude of 9.21, HIP 9089 is not visible to the naked eye.
What constellation is HIP 9089 in?
HIP 9089 is located in the constellation Perseus.