A visual band light curve for S Coronae Australis, adapted from Mundt (1979).[1] The error bar shown on the left-most point applies to all points. | |
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Australis |
Right ascension | 19h 01m 08.59709s[2] |
Declination | −36° 57′ 19.8950″[2] |
Apparent magnitude (V) | 10.91[2] |
Characteristics | |
Spectral type | G0Ve + K0Ve[3] |
Variable type | T Tau[3] |
Astrometry | |
Radial velocity (Rv) | −33 ± 5[4] km/s |
Proper motion (μ) | RA: −2.6 ± 5.8[2] mas/yr Dec.: −9.8 ± 2.3[2] mas/yr |
Distance | 460 ly (140[3] pc) |
Details | |
Other designations | |
S CrA, S Coronae Australis, HH 82 | |
Database references | |
SIMBAD | data |
S Coronae Australis (S CrA), is a young binary star system estimated to be around 2 million years old located in the constellation Corona Australis. It is composed of a G-type main sequence star that is about as luminous as and just over twice as massive as the Sun, and a smaller K-type main sequence star that has around 50-60% of the Sun's luminosity and 1.3 times its mass. Both stars are T Tauri stars and both show evidence of having circumstellar disks. The system is around 140 parsecs distant.[3]
Mundt
was invoked but never defined (see the help page).