HIP 45209
HIP 45209 is a K-type (Orange) star.
At a distance of roughly 1,843 light-years, HIP 45209 is a distant star lying deep within the Milky Way galaxy.
HIP 45209 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 45209 has an apparent magnitude of +8.17, 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 yellow hue, which corresponds to a B-V color index of +0.920.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 0,920 |
Observación
| Magnitud Aparente | +8.17 |
| Magnitud Absoluta | -0,59 |
| Distancia | 1,843 ly |
Posición
| Ascensión recta | 9h 12,79m |
| Declinación | 16° 37,82′ |
Frequently Asked Questions
What type of star is HIP 45209?
HIP 45209 is a Class K — K-type (Orange) star.
How far is HIP 45209 from Earth?
HIP 45209 is approximately 1,842.7 light-years from Earth.
Can you see HIP 45209 with the naked eye?
With an apparent magnitude of 8.17, HIP 45209 is not visible to the naked eye.