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Zeta Trianguli Australis

Zeta Trianguli Australis
Observation data
Epoch J2000      Equinox J2000
Constellation Triangulum Australe
Right ascension 16h 28m 28.14362s
Declination −70° 05′ 03.8419″
Apparent magnitude (V) 4.90
Characteristics
Spectral type F9 V
U−B color index +0.02
B−V color index +0.55
Astrometry
Radial velocity (Rv) +8.3 km/s
Proper motion (μ) RA: 199.97 mas/yr
Dec.: 110.97 mas/yr
Parallax (π) 82.53 ± 0.52mas
Distance 39.5 ± 0.2 ly
(12.12 ± 0.08 pc)
Absolute magnitude (MV) 4.49
Orbit
Period (P) 12.97662 ± 0.00017 d
Eccentricity (e) 0.01442 ± 0.00021
Periastron epoch (T) JD 2452752.31955
Argument of periastron (ω)
(secondary)
252.98° ± 0.80°
Semi-amplitude (K1)
(primary)
7.4988 ± 0.0016 km/s
Details
ζ TrA A
Mass 1.12 M
Metallicity [Fe/H] –0.18 dex
Rotation 13 days
Rotational velocity (v sin i) 3.23 km/s
Age 600–900 Myr
ζ TrA B
Mass 0.40 M
Other designations
CD -69°2558, FK5 610, GCTP 3719.00, Gl 624, HD 147584, HIP 80686, HR 6098, LTT 6558, SAO 253554.
Database references
SIMBAD data
ARICNS data

Zeta Trianguli Australis (ζ TrA) is a spectroscopic binary in the constellation Triangulum Australe. It is approximately 39.5 light years from Earth.

The binary's composite spectral class is F9V and its combined apparent magnitude is +4.90. The pair orbit each other once every 13 days, and the orbital eccentricity is a low 0.014, making it nearly circular.

Somewhat surprisingly for a star located at 70° S, it is a candidate swarm member of the Ursa Major moving group. However, there is some evidence to the contrary.



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