HD 197027

HD 197027

HIP 102152
Credit: ESO/Digitized Sky Survey 2
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Capricornus
Right ascension 20h 41m 54.6336s
Declination −27° 12 57.4154
Apparent magnitude (V) 9.15±0.02
Characteristics
Spectral type G3 V
U−B color index +0.30
B−V color index +0.65
Astrometry
Radial velocity (Rv)−43.9±0.3 km/s
Proper motion (μ) RA: +175.628 mas/yr
Dec.: −15.593 mas/yr
Parallax (π)12.7715±0.0164 mas
Distance255.4 ± 0.3 ly
(78.3 ± 0.1 pc)
Absolute magnitude (MV)4.74
Details
Mass0.97 M
Radius1.08+0.07
0.05
 R
Luminosity1.19 L
Surface gravity (log g)4.40±0.02 cgs
Temperature5718±5 K
Metallicity [Fe/H]−0.020±0.005 dex
Rotational velocity (v sin i)1.78±0.12 km/s
Age6.92±0.69 Gyr
Other designations
CD−27°14976, CPD−27°7079, HD 197027, HIP 102152, SAO 189585
Database references
SIMBADdata

HD 197027 (HIP 102152) is a star in the constellation Capricornus. It has an apparent magnitude of 9.15, making it readily visible through a telescope but not to the naked eye. The object is located at a distance of 255 light years but is approaching the Solar System with a heliocentric radial velocity of −44 km/s.

HD 197027 has a stellar classification of G3 V, indicating that it is an ordinary G-type main-sequence star like the Sun. It has only 97% the mass of the Sun but 108% of its radius. It shines at 119% the luminosity of the Sun from its photosphere at an effective temperature of 5,718 K, similar to the Sun's 5,778 K. HD 197027's metallicity – elements heavier than helium – is similar to the Sun. At an older age of 6.92 billion years, it spins with a projected rotational velocity of about 2 km/s.

Since its measured properties of this star are very similar to those of the Sun, it has been considered a candidate older solar twin. The abundances of 21 elements overall are more similar to the Sun than any other known solar twin. Its Iron Abundance is −0.03 with an error value of 0.02 Fe/H. (The value comes from the Hipparcos Extended Catalog.)