Star profile

Lambda Coronae Australis

3D likeness based on its real data · class A · ~8,500 K

What is Lambda Coronae Australis

Lambda Coronae Australis sits 205 light-years away within the small austral half-ring of the Crown, the southern echo of Corona Borealis. A white A-type star, young and hot, it belongs to the small handful of stars that trace a barely perceptible garland beside the body of Sagittarius. The region is rich in dark nebulae and pockets of recent star formation.

Where it is and when to see it

Lambda Coronae Australis lies in the southern celestial hemisphere. It is visible to the naked eye under a dark sky. Its best month of the year is July, when it culminates around midnight.

From London it culminates about 1° above the horizon.
From New York it culminates about 11° above the horizon.
From Sydney it culminates about 86° above the horizon.

It can be seen from anywhere south of 52° N.

It ranks no. 11 in brightness among the 29 stars of Corona Australis in our catalogue. To find it, start from Beta Coronae Australis, the brightest: it lies about 5° away (a fist at arm's length covers about 10°).

The light you see today left it about 210 years ago.

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Astronomical data for Lambda Coronae Australis

Constellation: Corona Australis
Apparent magnitude: 5.11
Distance: 205.3 light years
Coordinates (J2000): RA 280.946° · Dec -38.323°
Catalogue: HIP 91875 · HD 172777

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Other stars in Corona Australis

Corona Australis has 29 stars in Stelvia's catalogue. Here are a few of them.

See all 29 stars in Corona Australis