Coronet Cluster
The Coronet Cluster, also known as the R CrA cluster after its best-known member, is a small open cluster located about 170 parsecs away in the southern constellation Corona Australis, isolated at the edge of the Gould Belt. The Coronet Cluster is 3.5 times closer to the Earth than the Orion Nebula Cluster. The cluster center is composed of mostly young stars. The variable T Coronae Australis is also a member, only one arc minute from R CrA.
| Coronet Cluster | |
|---|---|
The Coronet Cluster, R CrA is the central dominantly bright star, with reflection nebulae NGC 6726/NGC 6727 lit by TY CrA and HD 176386 to upper right and parts of IC 4812 at the lower right. | |
| Observation data (J2000.0 epoch) | |
| Right ascension | 19h 1m 54s |
| Declination | −36° 57.2′ |
| Distance | 420–550 ly (130–170 pc) |
| Apparent magnitude (V) | 8 |
| Apparent dimensions (V) | 26 arcmin |
| Physical characteristics | |
| Mass | unknown M☉ |
| Radius | 2.1 light years |
| Estimated age | 0.5–2 million years |
| relative scarcity of circumstellar discs | |
| Other designations | R CRA, G359.93-17.85 by BDB2003 catalog |
| Associations | |
| Constellation | Corona Australis |
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