Sadr
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Radiating with an absolute magnitude of −6.52, the greatest intrinsic luminosity of any star treated here, Sadr appears at only apparent magnitude 2.23 because it lies extraordinarily far off — roughly 1,832 light-years, the most remote star in this group. It is a yellow-white F-type star and marks the Gamma position of Cygnus, at the very heart of the Swan where the constellation's cross-shaped figure intersects. Its colour index of 0.673 reflects the intermediate temperature of the F class. Embedded in one of the richest regions of the northern Milky Way, Sadr is a luminous supergiant whose faint appearance testifies chiefly to the immense distance across which its light reaches the Solar System.
الخصائص الفيزيائية
| النوع الطيفي | F Class F — F-type (Yellow-White) |
| مؤشر اللون (B−V) | 0,673 |
الرصد
| القدر الظاهري | +2.23 |
| القدر المطلق | -6,52 |
| المسافة | 1,832 ly |
| الكوكبة | Cygnus |
الموضع
| المطلع المستقيم | 20h 22,23m |
| الميل | 40° 15,40′ |