HIP 102270
HIP 102270 is a K-type (Orange) star.
At a distance of roughly 1,812 light-years, HIP 102270 is a distant star lying deep within the Milky Way galaxy.
HIP 102270 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 102270 has an apparent magnitude of +8.21, 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 red hue, which corresponds to a B-V color index of +1.665.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,665 |
Observación
| Magnitud Aparente | +8.21 |
| Magnitud Absoluta | -0,51 |
| Distancia | 1,812 ly |
Posición
| Ascensión recta | 20h 43,33m |
| Declinación | 78° 48,93′ |
Frequently Asked Questions
What type of star is HIP 102270?
HIP 102270 is a Class K — K-type (Orange) star.
How far is HIP 102270 from Earth?
HIP 102270 is approximately 1,812.0 light-years from Earth.
Can you see HIP 102270 with the naked eye?
With an apparent magnitude of 8.21, HIP 102270 is not visible to the naked eye.