Gamma Circini

γ Circini
Location of y Circini (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Circinus
Right ascension 15h 23m 22.64294s
Declination −59° 19 14.8131
Apparent magnitude (V) 4.51 (4.94 + 5.73)
Characteristics
Spectral type B5 IV + F8 V
Variable type Be
Astrometry
Radial velocity (Rv)16.90±1.78 km/s
Proper motion (μ) RA: −12.97 mas/yr
Dec.: −34.24 mas/yr
Parallax (π)7.27±0.81 mas
Distanceapprox. 450 ly
(approx. 140 pc)
Absolute magnitude (MV)−1.18
Orbit
Period (P)258 yr
Semi-major axis (a)2.576″
Eccentricity (e)0.931
Details
γ Cir A
Mass6.0±0.3 M
Temperature15,135 K
Age63.1±19.6 Myr
γ Cir B
Temperature4,786 K
Other designations
γ Cir, CPD−58°5908, HIP 75323, HR 5704, SAO 242463
γ Cir A: HD 136415
γ Cir B: HD 136416
Database references
SIMBADγ Cir AB
γ Cir A
γ Cir B

Gamma Circini, Latinized from γ Circini, is a star system in the constellation Circinus. It was noted as a double star by Herschel in 1835, who estimated the separation as 1 arc second. It is visible to the naked eye with an apparent visual magnitude of 4.51. Based upon an annual parallax shift of 7.27 mas, it is about 450 light-years away.

This is a wide binary star system and may even be a triple star. The two visible components orbit each other with a preliminary estimated period of 258 years and a large eccentricity of 0.931. As of 2014, the visible components have an angular separation of 0.80 arc seconds on a position angle of 359°.

The primary star, component A, is a B-type subgiant star with a stellar classification of B5 IV. Based upon isochrone curve fitting it is hypothesized to be a pair of matching B5 stars, and is a Be variable with an uncertain maximum. It has an effective temperature of 15,135 K and an estimated mass six times that of the Sun. The companion, component B, is an F-type main-sequence star with a stellar classification of F8 V. It has an effective temperature of 4,786 K.