HD 166066

Star in the constellation Octans From Wikipedia, the free encyclopedia

HD 166066 is a solitary star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 8.10,[3] making it readily visible in binoculars, but not to the naked eye. The object is located 223 light years away from the Solar System,[2] but is drifting away with a poorly constrained radial velocity of about 1.14 km/s.[2]

Right ascension18h 38m 51.0741s[2]
Declination−85° 42 32.2260[2]
Quick facts Constellation, Right ascension ...
HD 166066
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Octans[1]
Right ascension 18h 38m 51.0741s[2]
Declination −85° 42 32.2260[2]
Apparent magnitude (V) 8.10±0.01[3]
Characteristics
Spectral type G0 V[4]
B−V color index +0.59[3]
Astrometry
Radial velocity (Rv)1.14±2.01[2] km/s
Proper motion (μ) RA: +147.318 mas/yr[2]
Dec.: −43.097 mas/yr[2]
Parallax (π)14.5962±0.1186 mas[2]
Distance223 ± 2 ly
(68.5 ± 0.6 pc)
Absolute magnitude (MV)4.09[1]
Details
Mass1.13[5] M
Radius1.39+0.07
0.05
[6] R
Luminosity2.12[1] L
Surface gravity (log g)4.25[5] cgs
Temperature6,054±80[5] K
Metallicity [Fe/H]−0.03[5] dex
Rotational velocity (v sin i)5[7] km/s
Age7.0+2.5
1.2
[8] Gyr
Other designations
CD−85°150, CPD−85°478, HD 166066, HIP 91434, GSC 09527-01174[9]
Database references
SIMBADdata
Close

HD 166066 has a stellar classification of G0 V, indicating that it is a G-type main sequence star similar to the Sun.[4] However, the calcium H & K lines are narrow and weak for its class.[4] It has 113% the mass of the Sun[5] and 139% its radius, along with twice its luminosity.[1][6]

The iron abundance is 93% that of the Sun, and is slightly hotter, with an effective temperature of 6,054 K[5] compared to the Sun's 5,778 K. HD 166066 is significantly older, with an age of 7 billion years,[8] and rotates modestly with a projected rotational velocity of 5 km/s.[7]

References

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