HIP 1962
HIP 1962 is a K-type (Orange) star.
At a distance of roughly 1,161 light-years, HIP 1962 is a distant star lying deep within the Milky Way galaxy.
HIP 1962 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 1962 has an apparent magnitude of +6.90, 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 +1.426.
Propiedades físicas
| Clase Espectral | K Class K — K-type (Orange) |
| Índice de color (B−V) | 1,426 |
Observación
| Magnitud Aparente | +6.90 |
| Magnitud Absoluta | -0,86 |
| Distancia | 1,161 ly |
Posición
| Ascensión recta | 0h 24,83m |
| Declinación | -18° 28,31′ |
Frequently Asked Questions
What type of star is HIP 1962?
HIP 1962 is a Class K — K-type (Orange) star.
How far is HIP 1962 from Earth?
HIP 1962 is approximately 1,160.7 light-years from Earth.
Can you see HIP 1962 with the naked eye?
With an apparent magnitude of 6.90, HIP 1962 is not visible to the naked eye.