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Corona Borealis

Corona Borealis
Constellation
Corona Borealis
Abbreviation CrB
Genitive Coronae Borealis
Pronunciation /kəˈrnə ˌbɔːriˈæls, -ˌb-, -ˈls/, genitive /kəˈrni/
Symbolism The Northern Crown
Right ascension 15h 16m 03.8205s–16h 25m 07.1526s
Declination 39.7117195°–25.5380573°
Family Ursa Major
Area 179 sq. deg. (73rd)
Main stars 8
Bayer/Flamsteed
stars
24
Stars with planets 5
Stars brighter than 3.00m 4
Stars within 10.00 pc (32.62 ly) 0
Brightest star α CrB (Alphecca or Gemma) (2.21m)
Nearest star HD 144579
(47.36 ly, 14.52 pc)
Messier objects 0
Meteor showers None
Bordering
constellations
Visible at latitudes between +90° and −50°.
Best visible at 21:00 (9 p.m.) during the month of July.

Corona Borealis is a small constellation in the Northern Celestial Hemisphere. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Its brightest stars form a semicircular arc. Its Latin name, inspired by its shape, means "northern crown". In classical mythology Corona Borealis generally represented the crown given by the god Dionysus to the Cretan princess Ariadne and set by him in the heavens. Other cultures likened the pattern to a circle of elders, an eagle's nest, a bear's den, or even a smokehole. Ptolemy also listed a southern counterpart, Corona Australis, with a similar pattern.

The brightest star is the magnitude 2.2 Alpha Coronae Borealis. The yellow supergiant R Coronae Borealis is the prototype of a rare class of giant stars—the R Coronae Borealis variables—that are extremely hydrogen deficient, and thought to result from the merger of two white dwarfs. T Coronae Borealis, also known as the Blaze Star, is another unusual type of variable star known as a recurrent nova. Normally of magnitude 10, it last flared up to magnitude 2 in 1946. ADS 9731 and Sigma Coronae Borealis are multiple star systems with six and five components respectively. Five star systems have been found to have Jupiter-sized exoplanets. Abell 2065 is a highly concentrated galaxy cluster one billion light-years from the Solar System containing more than 400 members, and is itself part of the larger Corona Borealis Supercluster.


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