The star centred in this image is actually a system with three components: a close binary designated 'A' and a third star in a wider orbit designated 'B'. Sigma Coronae Borealis C is also a binary, much more widely separated from the triple system, and is visible among the fainter stars to the southwest (lower right) of this image. It follows a distant orbit around the AB system that takes nearly nine hundred thousand years to complete. Imagery provided by Aladin sky atlas