Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Apus |
Right ascension | 18h 11m 15.80732s[1] |
Declination | −75° 53′ 29.4836″[1] |
Apparent magnitude (V) | 5.86[2] |
Characteristics | |
Evolutionary stage | red giant branch[3] |
Spectral type | K2 III[4] |
U−B color index | +1.43[5] |
B−V color index | +1.24[5] |
Astrometry | |
Radial velocity (Rv) | 14.8±3.2[6] km/s |
Proper motion (μ) | RA: +16.16 mas/yr[1] Dec.: -296.819 mas/yr[1] |
Parallax (π) | 14.2681 ± 0.0440 mas[1] |
Distance | 228.6 ± 0.7 ly (70.1 ± 0.2 pc) |
Absolute magnitude (MV) | +1.48[2] |
Details | |
Mass | 1.15[7] M☉ |
Radius | 9.09[8] R☉ |
Luminosity | 33.1+1.6 −1.5[9] L☉ |
Surface gravity (log g) | 2.55[7] cgs |
Temperature | 4,360±90[9] K |
Metallicity [Fe/H] | +0.24[10] dex |
Rotational velocity (v sin i) | <1.5[11] km/s |
Age | 4.54+0.46 −0.56[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
HD 164712, also known as HR 6731 is an orange hued star located in the southern constellation of Apus. It has an apparent magnitude of 5.86,[2] making it faintly visible to the naked eye if viewed under ideal conditions. Parallax measurements place the object at a distance of 229 light-years (70 pc),[1] and it is currently receding with a heliocentric radial velocity of 14.8 km/s.[6]
HD 164712 has a stellar classification of K2 III, indicating that it is a red giant. David Stanley Evans gave it a slightly cooler class of K3 III.[14] Gaia Data Release 3 models place it on the bump of red giant branch, a period of temporary contraction.[3] At present it has 1.15 times the mass of the Sun[7] but at an age of 4.54 billion years,[3] it has expanded to 9.09 times its girth.[8] It shines with a luminosity of 33.1 L☉ from its enlarged photosphere at an effective temperature of 4,360 K.[9] HD 164712 is a thick disk star with an iron abundance 73% above solar level.[10] This makes it metal enriched. Like most giants, it spins slowly, with its projected rotational velocity being lower than 1.5 km/s.[11]
HR 6731 has two faint companions. Component B is a 13th magnitude object separated 24.6″ away along a position angle of 299°.[15] Component C is a 14th magnitude star 18.1″ away along a position angle of 109°.[15] The first one is a background object while the other one appears to be physically related.[15] As for HD 164712, it shows indications of an infrared excess, suggesting there may be a dusty disk in orbit around the star.[16][17]
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