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Corona Australis (Southern Crown)

COSMOS / CONSTELLATIONS / CRA

Corona Australis (Southern Crown)

The Southern Crown. IAU abbreviation CrA. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

β CrAMeridianaγ CrAδ CrAθ CrAζ CrA↑ N ← E
Coloured dots are the stars of Corona Australis brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
CrA
Latin name / genitive
Corona Australis / Coronae Australis
Position
Right ascension ≈ 18 h 47 m; declination −45° to −37°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 9° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 30 August.
Number of stars
46 stars brighter than magnitude 6.5 in the catalogue; 9 brighter than 5 and 0 brighter than 4.

INTERACTIVE LAB

Where is Corona Australis tonight?

The lab opens for Ankara on today’s date. Drag the time slider through the night; the “Best night” button jumps to the date when the constellation is highest at 21:00 (around 30 August). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

A small arc of stars at the feet of Sagittarius, one of Ptolemy’s 48 constellations. The Corona Australis molecular cloud is one of the nearest star-forming regions to Earth. From Türkiye it appears just above the southern horizon on summer nights.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
β CrA4.10474K0II/IIICN
Meridiana4.11125A0/A1V
γ CrA4.2356F7IV-V
δ CrA4.57179K1III
θ CrA4.62558G5III
ζ CrA4.74193A0Vn
ε CrA4.8398F3IV/V
HIP 887264.92136A5V

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

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