HIP 1988
HIP 1988 is a K-type (Orange) star located in the constellation Cassiopeia.
Located approximately 997.4 light-years from Earth, HIP 1988 resides within the broader disk of our Milky Way galaxy.
HIP 1988 is classified as a spectral class K star (K-type (Orange)) on the Harvard spectral classification system.
HIP 1988 has an apparent magnitude of +8.34, 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 +1.597.
Propiedades físicas
| Clase Espectral | Class K — K-type (Orange) |
| Índice de color (B−V) | 1,597 |
Observación
| Magnitud Aparente | +8.34 |
| Magnitud Absoluta | 0,91 |
| Distancia | 997 ly |
| Constelación | Cassiopeia |
Posición
| Ascensión recta | 0h 25,17m |
| Declinación | 64° 38,32′ |
Preguntas frecuentes
What type of star is HIP 1988?
HIP 1988 is a Class K — K-type (Orange) star.
How far is HIP 1988 from Earth?
HIP 1988 is approximately 997.4 light-years from Earth.
Can you see HIP 1988 with the naked eye?
With an apparent magnitude of 8.34, HIP 1988 is not visible to the naked eye.
What constellation is HIP 1988 in?
HIP 1988 is located in the constellation Cassiopeia.