Corona Borealis
Origin
Corona Borealis is a small constellation that was cataloged by the second-century astronomer Ptolemy. Corona Borealis is the Northern Crown and its brightest stars form a semicircle, similar to those of Corona Australis, the Southern Crown. Corona Borealis is a northern hemisphere constellation and is visible to anyone north of latitude 50 degrees south.
Bright Stars
The brightest star is Alpha Coronae Borealis, commonly known as Alphecca. Alphecca is a magnitude-2.2 blue-white star that lies about 75 light-years from Earth. Beta Coronae Borealis is a spectroscopic binary star that shines at about magnitude 3.7.
Photo of the constellation Corona Borealis produced by NOIRLab in collaboration with Eckhard Slawik, a German astrophotographer.
The annotations are from a standardized set of 88 western IAU constellations and stick figures from Sky & Telescope. Please find here a non-annotated version of the image.
Credit: E. Slawik/NOIRLab/NSF/AURA/M. Zamani
Credit: E. Slawik/NOIRLab/NSF/AURA/M. Zamani
Notable Objects
Corona Borealis contains many faint galaxies that typically require larger telescopes to observe.