HD 193721

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Right ascension20h 33m 17.6366s[1]
Declination−80° 57 53.5944[1]
HD 193721
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Octans
Right ascension 20h 33m 17.6366s[1]
Declination −80° 57 53.5944[1]
Apparent magnitude (V) 5.77±0.01[2]
Characteristics
Spectral type G6/8 II[3]
U−B color index +0.85[4]
B−V color index +1.14[4]
Astrometry
Radial velocity (Rv)8.6±0.7[5] km/s
Proper motion (μ) RA: +9.794 mas/yr[1]
Dec.: −16.081 mas/yr[1]
Parallax (π)4.2823±0.165 mas[1]
Distance760 ± 30 ly
(234 ± 9 pc)
Absolute magnitude (MV)−0.24[6]
Details
Mass3.49[7] M
Radius24.38[8] R
Luminosity300±5[9] L
Surface gravity (log g)2.14±0.02[1] cgs
Temperature4953±122[8] K
Metallicity [Fe/H]−0.15[10] dex
Rotational velocity (v sin i)2.7±1.1[11] km/s
Other designations
47 G. Octantis[12], CPD−81°901, FK5 3994, GC 28453, HD 193721, HIP 101427, HR 7785, SAO 258861, WDS J20333-8058A[13]
Database references
SIMBADdata

HD 193721 (HR 7785) is an astrometric binary[14] in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.77,[2] allowing it to be faintly seen with the naked eye. Parallax measurements place the system 760 light years[1] away from the Solar System and it is currently receding with a heliocentric radial velocity 8.6 km/s.[5]

HD 193721 has a stellar classification of G6/8 II[3] — intermediate between a G6 and 8 bright giant. At present it has 3.49 times the mass of the Sun,[7] but has expanded to 24.4 times its girth.[8] It shines with a luminosity of 300 L[9] from its enlarged photosphere at an effective temperature of 4,953 K,[8] giving a yellow hue. HD 193721 is metal deficient with an iron abundance 71% that of the Sun[10] and spins leisurely with a projected rotational velocity of 2.7 km/s.[11]

The system has a companion designated CPD −81°900. The object has a spectral classification of F8[15] and is located 25.5 along a position angle of 0° (as of 1998).[16] CPD −81°900 is a foreground object, having a higher parallax[17] and different proper motion.[16]

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