Kappa Trianguli Australis

Variable star in the constellation Triangulum Australe From Wikipedia, the free encyclopedia

Kappa Trianguli Australis (κ Trianguli Australis) is a star in the constellation Triangulum Australe. It is a yellow G-type supergiant with an apparent magnitude of +5.08, making it visible to the naked eye under good observing conditions. It is around 1,200 light years from Earth.

A light curve for Kappa Trianguli Australis, plotted from Hipparcos data[12]
Quick facts Constellation, Right ascension ...
κ Trianguli Australis
Location of κ Trianguli Australis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Triangulum Australe
Right ascension 15h 55m 29.59831s[1]
Declination −68° 36 10.8101[1]
Apparent magnitude (V) +5.08[2]
Characteristics
Spectral type G3/5 Ib[3]
B−V color index +1.12[2]
Variable type suspected SRD[4]
Astrometry
Radial velocity (Rv)+3.9±0.3[5] km/s
Proper motion (μ) RA: −9.36[1] mas/yr
Dec.: −6.79[1] mas/yr
Parallax (π)2.70±0.26 mas[1]
Distance1,200 ± 100 ly
(370 ± 40 pc)
Absolute magnitude (MV)−2.71[6]
Details
Mass7.0[7] M
Luminosity1,761[8] L
Surface gravity (log g)1.90[9] cgs
Temperature4,658[10] K
Metallicity [Fe/H]+0.21[9] dex
Rotational velocity (v sin i)7.7±1.0[10] km/s
Age55.2[7] Myr
Other designations
κ TrA, CPD−68°2585, FK5 3253, HD 141767, HIP 77982, HR 5891, SAO 253342[11]
Database references
SIMBADdata
Close

It is not generally listed as a variable star but Hipparcos photometry showed small amplitude brightness changes. The dominant period was around 600 days and the amplitude less than a hundredth of a magnitude.[13]

References

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