HIP 9077
HIP 9077 is a K-type (Orange) star located in the constellation Perseus.
At a distance of roughly 2,938 light-years, HIP 9077 is a distant star lying deep within the Milky Way galaxy.
HIP 9077 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 9077 has an apparent magnitude of +7.10, 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 +1.477.
Propriedades físicas
| Classe Espectral | Class K — K-type (Orange) |
| Índice de cor (B−V) | 1,477 |
Observação
| Magnitude Aparente | +7.10 |
| Magnitude Absoluta | -2,67 |
| Distância | 2,938 ly |
| Constelação | Perseus |
Posição
| Ascensão reta | 1h 56,87m |
| Declinação | 52° 29,37′ |
Perguntas frequentes
What type of star is HIP 9077?
HIP 9077 is a Class K — K-type (Orange) star.
How far is HIP 9077 from Earth?
HIP 9077 is approximately 2,938.3 light-years from Earth.
Can you see HIP 9077 with the naked eye?
With an apparent magnitude of 7.10, HIP 9077 is not visible to the naked eye.
What constellation is HIP 9077 in?
HIP 9077 is located in the constellation Perseus.