Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Australis |
Right ascension | 19h 08m 20.96980s[1] |
Declination | −40° 29′ 48.1155″[1] |
Apparent magnitude (V) | 4.57[2] |
Characteristics | |
Evolutionary stage | horizontal branch[3] |
Spectral type | K1III[4] |
B−V color index | +1.070±0.052[2] |
Astrometry | |
Radial velocity (Rv) | +21.24±0.19[1] km/s |
Proper motion (μ) | RA: +47.344[1] mas/yr Dec.: −27.047[1] mas/yr |
Parallax (π) | 18.6963 ± 0.3123 mas[1] |
Distance | 174 ± 3 ly (53.5 ± 0.9 pc) |
Absolute magnitude (MV) | 0.93[5] |
Details[3] | |
Mass | 1.50±0.01 M☉ |
Radius | 11.25±0.11 R☉ |
Luminosity | 53±1 L☉ |
Surface gravity (log g) | 2.59±0.10 cgs |
Temperature | 4,645±14 K |
Metallicity [Fe/H] | +0.01±0.10 dex |
Age | 2.80±0.13 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Delta Coronae Australis is a single[7] star located in the southern constellation of Corona Australis. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.57.[2] The star is located about 174 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +21 km/s.[1]
This object is an evolved giant star with a stellar classification of K1III.[4] After exhausting the supply of hydrogen at its core, the star expanded off the main sequence and now has 11[1] times the radius of the Sun. It is a red clump giant,[3][5] which indicates it is on the horizontal branch and is generating energy through core helium fusion. The star is 2.8[3] billion years old with 1.5[3] times the mass of the Sun. It is radiating 55[1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,654 K.[1]
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