HIP 90850
HIP 90850 is a M-type (Red) star located in the constellation Sagittarius.
At a distance of roughly 1,310 light-years, HIP 90850 is a distant star lying deep within the Milky Way galaxy.
HIP 90850 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
At an apparent magnitude of +10.91, HIP 90850 is a faint star that requires a telescope to observe. It is invisible to the naked eye and too dim for most binoculars. Observers will note its red hue, which corresponds to a B-V color index of +1.500.
Propiedades físicas
| Clase Espectral | M Class M — M-type (Red) |
| Índice de color (B−V) | 1,500 |
Observación
| Magnitud Aparente | +10.91 |
| Magnitud Absoluta | 2,89 |
| Distancia | 1,310 ly |
| Constelación | Sagittarius |
Posición
| Ascensión recta | 18h 32,02m |
| Declinación | -34° 42,37′ |
Frequently Asked Questions
What type of star is HIP 90850?
HIP 90850 is a Class M — M-type (Red) star.
How far is HIP 90850 from Earth?
HIP 90850 is approximately 1,309.9 light-years from Earth.
Can you see HIP 90850 with the naked eye?
With an apparent magnitude of 10.91, HIP 90850 is not visible to the naked eye.
What constellation is HIP 90850 in?
HIP 90850 is located in the constellation Sagittarius.