HIP 89017
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HIP 89017 is a K-type (Orange) star.
At a distance of roughly 1,177 light-years, HIP 89017 is a distant star lying deep within the Milky Way galaxy.
HIP 89017 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 89017 has an apparent magnitude of +7.40, 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 +1.273.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,273 |
Observación
| Magnitud Aparente | +7.40 |
| Magnitud Absoluta | -0,39 |
| Distancia | 1,177 ly |
Posición
| Ascensión recta | 18h 10,06m |
| Declinación | 56° 16,01′ |
Frequently Asked Questions
What type of star is HIP 89017?
HIP 89017 is a Class K — K-type (Orange) star.
How far is HIP 89017 from Earth?
HIP 89017 is approximately 1,177.5 light-years from Earth.
Can you see HIP 89017 with the naked eye?
With an apparent magnitude of 7.40, HIP 89017 is not visible to the naked eye.