HIP 30475
HIP 30475 is a K-type (Orange) star.
At a distance of roughly 2,219 light-years, HIP 30475 is a distant star lying deep within the Milky Way galaxy.
HIP 30475 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 30475 has an apparent magnitude of +9.10, 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 orange hue, which corresponds to a B-V color index of +1.254.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,254 |
Observación
| Magnitud Aparente | +9.10 |
| Magnitud Absoluta | -0,06 |
| Distancia | 2,219 ly |
Posición
| Ascensión recta | 6h 24,40m |
| Declinación | -37° 32,03′ |
Frequently Asked Questions
What type of star is HIP 30475?
HIP 30475 is a Class K — K-type (Orange) star.
How far is HIP 30475 from Earth?
HIP 30475 is approximately 2,218.8 light-years from Earth.
Can you see HIP 30475 with the naked eye?
With an apparent magnitude of 9.10, HIP 30475 is not visible to the naked eye.