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] |
Distance | 760 ± 30 ly (234 ± 9 pc) |
Absolute magnitude (MV) | −0.24 [6] |
Details | |
Mass | 3.49 [7] M☉ |
Radius | 24.38 [8] R☉ |
Luminosity | 300±5 [9] L☉ |
Surface gravity (log g) | 2.14±0.02 [1] cgs |
Temperature | 4953±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 | |
SIMBAD | data |
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]