Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Triangulum Australe |
Right ascension | 15h 19m 45.71231s[2] |
Declination | −66° 29′ 45.7417″[2] |
Apparent magnitude (V) | 6.73[3] (6.33 - 6.90)[4] |
Characteristics | |
Spectral type | F7 Ib/II[5] |
Variable type | δ Cep[6] |
Astrometry | |
Radial velocity (Rv) | −13.2±1.6[7] km/s |
Proper motion (μ) | RA: −5.113[2] mas/yr Dec.: −8.317[2] mas/yr |
Parallax (π) | 1.4754 ± 0.0371 mas[2] |
Distance | 2,210 ± 60 ly (680 ± 20 pc) |
Absolute magnitude (MV) | 2.69[8] |
Details | |
Mass | 5.42 or 5.66[9] M☉ |
Radius | 24.7±1.9[10] or 35.8±0.8[9] R☉ |
Surface gravity (log g) | 2.10[9] cgs |
Temperature | 5,852±21[9] K |
Metallicity [Fe/H] | +0.06±0.08[8] dex |
Rotational velocity (v sin i) | 16 km/s |
Other designations | |
Database references | |
SIMBAD | data |
R Trianguli Australis is a yellow-white hued variable star in the southern constellation Triangulum Australe. It is near the limit of visibility to the naked eye, having a typical apparent visual magnitude of 6.73.[3] Based upon an annual parallax shift of 1.48 mas,[2] it is located 2,210 light years away. R TrA is moving closer with a heliocentric radial velocity of −13 km/s.[7]
This is a Classical Cepheid variable with an apparent magnitude that ranges from 6.33 to 6.90 over 3.38926 days.[4] It is a bright giant/supergiant with a nominal stellar classification of F7 Ib/II,[5] but pulsates between spectral types F5Ib/II-G5.[4] Depending on the method employed, the estimated mass is 5.42 or 5.66 times the mass of the Sun and it has 24.7 or 35.8 times the Sun's radius.[9] R TrA has an infrared excess that is being emitted by circumstellar silicate dust heated to 150–200 K. It is losing mass at the rate of 4×10−9 M☉·y−1.[9]
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