CrA · Coronae Australis
Corona Australis Constellation
IAU constellation mapCrACorona Australis (CrA) is one of the 88 constellations recognised by the International Astronomical Union. It covers 128 square degrees of the southern sky in quadrant SQ4. Its brightest star is Alfecca Meridiana. The Latin genitive of the name is Coronae Australis, used to form star names within the constellation. The IAU standardised all constellation boundaries in 1930.
Quick facts
- IAU name
- Corona Australis
- Abbreviation
- CrA
- Latin genitive
- Coronae Australis
- Hemisphere
- southern
- Area
- 128 sq deg
- Brightest star
- Alfecca Meridiana
- Quadrant
- SQ4
- Family
- Hercules
- Discovery era
- Ptolemy's 48 (Almagest, c. 150 CE)
Overview
Corona Australis is one of the 88 constellations formally recognised by the International Astronomical Union (IAU). It occupies 128 square degrees of sky in the southern hemisphere sky, best visible at latitudes between +45 and -90 degrees in September. The constellation belongs to the Hercules family of constellations. Its Latin genitive is Coronae Australis, the form used when naming stars within the constellation — for example, the brightest star Alfecca Meridiana may appear in catalogues as Alpha Coronae Australis or similar. The IAU standardised the boundaries of all 88 constellations in 1930 under the direction of Eugène Delporte, using straight lines of right ascension and declination to eliminate the ambiguities of earlier variable-boundary systems.
Notable stars
The brightest star in Corona Australis is Alfecca Meridiana. Individual stars within Corona Australis are conventionally named using Bayer designation — Greek letters followed by the Latin genitive of the constellation name (Coronae Australis) — introduced by Johann Bayer in his 1603 star atlas Uranometria. Flamsteed numbers (numeric designators followed by Corona Australis) were added by John Flamsteed in his 1712 catalogue. Variable stars, double stars, and deep-sky objects within the Corona Australis boundary are catalogued by the IAU with the abbreviation CrA.
History and catalogue
Corona Australis was introduced or documented by Ptolemy's 48 (Almagest, c. 150 CE). The modern IAU constellation boundaries were formally established in 1930. The designation CrA is the official three-letter IAU abbreviation used in star catalogues, variable star designations, and positional references. The family classification 'Hercules' groups this constellation with others sharing a region of sky or a common historical source in astronomical literature.
Sources & further reading (2)
- official-iau — accessed 2026-05-06
- encyclopedia — accessed 2026-05-06
Frequently asked questions
What does the name Corona Australis mean?
Corona Australis is the Latin name used by the IAU to designate this constellation. The name comes from classical Latin and Greek astronomical tradition. In star catalogues, stars within Corona Australis are designated using the genitive form of the name (e.g. Alpha Corona Australis or similar Latin genitive forms) — a naming convention introduced by Johann Bayer in his 1603 atlas Uranometria and still in use today.
How large is Corona Australis compared to other constellations?
Corona Australis covers 128 square degrees of sky. The full sphere of the sky contains 41,253 square degrees, so Corona Australis occupies about 0.3% of the total sky. For comparison, the largest constellation is Hydra at 1303 square degrees; the smallest is Crux at 68 square degrees.
When and where is Corona Australis visible?
Corona Australis is primarily a southern hemisphere constellation. Observers at high northern latitudes cannot see it; it is best appreciated from the southern tropics or high southern latitudes. The brightest star, Alfecca Meridiana, serves as the main visual anchor for locating the constellation. As with all constellations, the best viewing conditions are a dark sky away from artificial light pollution, with the constellation high enough above the horizon to minimise atmospheric absorption.
