Theta Circini

Theta Circini (θ Cir), is a binary star located in the southern constellation of Circinus, to the northwest of Alpha Circini. It is faintly visible to the naked eye with an apparent visual magnitude of 5.110. Based upon an annual parallax shift of 11.82 mas, it is located at a distance of about 276 light years from the Sun.

θ Circini

A light curve for Theta Circini, plotted from Hipparcos data
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Circinus
Right ascension 14h 56m 43.987s
Declination −62° 46 51.66
Apparent magnitude (V) 5.110 (5.90 + 5.90)
Characteristics
Spectral type B3 Ve (B2 + B2)
B−V color index +0.00
Variable type GCAS
Astrometry
Proper motion (μ) RA: +102.65 mas/yr
Dec.: +9.35 mas/yr
Parallax (π)11.82 ± 0.30 mas
Distance276 ± 7 ly
(85 ± 2 pc)
Absolute magnitude (MV)−2.43/−2.43
Orbit
Period (P)39.62±0.78 yr
Semi-major axis (a)0.08564±0.00056
Eccentricity (e)0.3014±0.0081
Inclination (i)153.3±2.0°
Longitude of the node (Ω)228.0±5.2°
Periastron epoch (T)1993.81±0.12
Argument of periastron (ω)
(secondary)
68.6±6.5°
Details
θ Cir A
Mass9.3±0.6 M
Surface gravity (log g)3.38 cgs
Temperature19,099 K
Rotational velocity (v sin i)195±13 km/s
Age27.1±6.1 Myr
Other designations
θ Cir, CD−62°891, HD 131492, HIP 73129, HR 5551, SAO 252965.
Database references
SIMBADdata

This is an astrometric binary star system with an orbital period of about 39.6 years, an eccentricity of 0.3, and a semimajor axis of 85.64 mas. The pair show a combined stellar classification of B3 Ve, which matches a B-type main sequence star. The 'e' suffix on the class indicates this is a Be star. Alternate classifications include B4 Vnp and B4npe, with the 'n' indicating broad ("nebulous") absorption lines due to rotation and the 'p' meaning a chemically peculiar star. The two components appear to have similar visual magnitude, mass, and classification. The system behaves as a Gamma Cassiopeiae variable showing occasional outbursts of up to 0.27 in magnitude.

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