Delta Trianguli Australis

Luminous G-type star; Triangulum Australe From Wikipedia, the free encyclopedia

Delta Trianguli Australis

Delta Trianguli Australis (Delta TrA), Latinized from δ Trianguli Australis, is a solitary,[14] yellow-hued star in the constellation Triangulum Australe. It has an apparent magnitude of 3.84,[2] making it readily visible to the naked eye under ideal conditions, Parallax measurements place the object at a distance of 606 light years (182 parsecs).[1] It has a heliocentric radial velocity of −4.9 km/s,[5] indicating that it is drifting towards the Solar System.

Quick Facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
δ Trianguli Australis
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Location of δ TrA (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Triangulum Australe
Right ascension 16h 15m 26.26978s[1]
Declination −63° 41 08.4492[1]
Apparent magnitude (V) 3.84±0.01[2]
Characteristics
Spectral type G2 Ib-IIa[3]
U−B color index +0.87[4]
B−V color index +1.10[4]
Astrometry
Radial velocity (Rv)−4.9±0.7[5] km/s
Proper motion (μ) RA: +2.73 mas/yr[1]
Dec.: −12.92 mas/yr[1]
Parallax (π)5.37 ± 0.17 mas[1]
Distance610 ± 20 ly
(186 ± 6 pc)
Absolute magnitude (MV)−2.49[6]
Details
Mass6.51[7] M
Radius53.6[8] R
Luminosity1,210[9] L
Surface gravity (log g)1.54[10] cgs
Temperature4,705±122[8] K
Metallicity [Fe/H]−0.05[10] dex
Rotational velocity (v sin i)8.2±2[11] km/s
Other designations
δ TrA, 25 G. Trianguli Australis[12], CPD−63°3854, FK5 602, GC 21819, HD 145544, HIP 79664, HR 6030, SAO 253474, WDS J16154-6341A[13]
Database references
SIMBADdata
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Delta TrA has a stellar classification of G2 Ib-IIa[3] — an evolved G-type star with a luminosity class intermediate between a low luminosity supergiant and a bright giant. At present it has 6.5 times the mass of the Sun[7] and has an enlarged radius of 53.6 R.[8] It radiates at 1,210 times the luminosity of the Sun[9] from its photosphere at an effective temperature of 4,705 K.[8] Delta TrA has an iron abundance 89% that of the Sun,[10] placing it around solar metallicity. It spins modestly with a projected rotational velocity of 8.2 km/s, which is high for stars of this type.[11]

References

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