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.
คุณสมบัติทางกายภาพ
| ประเภทสเปกตรัม | Class G — G-type (Yellow) |
| ดัชนีสี (B−V) | 0.694 |
การสังเกต
| โชติมาตรปรากฏ | +5.12 |
| โชติมาตรสัมบูรณ์ | 4.17 |
| ระยะทาง | 50.6 ly |
ตำแหน่ง
| ไรต์แอสเซนชัน | 17h 44.15m |
| เดคลิเนชัน | -51° 50.04′ |
คำถามที่พบบ่อย
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.