Cervantes
Mu Ara
Cervantes is a G-type (Yellow) star. It carries the designation Mu Ara.
Located approximately 50.6 light-years from Earth, Cervantes resides within the broader disk of our Milky Way galaxy.
Cervantes is classified as a spectral class G star (G-type (Yellow)) on the Harvard spectral classification system.
With an apparent magnitude of +5.12, Cervantes sits near the limit of naked-eye visibility. It can be glimpsed without optical aid under dark skies, but binoculars will make observation much easier. Observers will note its yellow-white hue, which corresponds to a B-V color index of +0.694.
Propiedades físicas
| Clase Espectral | Class G — G-type (Yellow) |
| Índice de color (B−V) | 0,694 |
Observación
| Magnitud Aparente | +5.12 |
| Magnitud Absoluta | 4,17 |
| Distancia | 50.6 ly |
Posición
| Ascensión recta | 17h 44,15m |
| Declinación | -51° 50,04′ |
Preguntas frecuentes
What type of star is Cervantes?
Cervantes is a Class G — G-type (Yellow) star.
How far is Cervantes from Earth?
Cervantes is approximately 50.6 light-years from Earth.
Can you see Cervantes with the naked eye?
With an apparent magnitude of 5.12, Cervantes is visible to the naked eye.