HIP 39090
HIP 39090 is a M-type (Red) star.
At a distance of roughly 1,647 light-years, HIP 39090 is a distant star lying deep within the Milky Way galaxy.
HIP 39090 is classified as a spectral class M star (M-type (Red)) on the Harvard spectral classification system.
HIP 39090 has an apparent magnitude of +8.36, 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 +1.710.
Propiedades físicas
| Clase Espectral | Class M — M-type (Red) |
| Índice de color (B−V) | 1,710 |
Observación
| Magnitud Aparente | +8.36 |
| Magnitud Absoluta | -0,16 |
| Distancia | 1,647 ly |
Posición
| Ascensión recta | 7h 59,81m |
| Declinación | -20° 26,91′ |
Preguntas frecuentes
What type of star is HIP 39090?
HIP 39090 is a Class M — M-type (Red) star.
How far is HIP 39090 from Earth?
HIP 39090 is approximately 1,647.2 light-years from Earth.
Can you see HIP 39090 with the naked eye?
With an apparent magnitude of 8.36, HIP 39090 is not visible to the naked eye.