HD 116029

HD 116029 is a binary star system about 400 light-years away.

HD 116029
Observation data
Epoch J2000      Equinox J2000
Constellation Coma Berenices
Right ascension 13h 20m 39.5422s
Declination +24° 38 55.3099
Apparent magnitude (V) 7.89
Characteristics
Evolutionary stage subgiant
Spectral type K1IV+M
B−V color index 1.009
Astrometry
Radial velocity (Rv)-6.42 km/s
Proper motion (μ) RA: -14.495 mas/yr
Dec.: -52.193 mas/yr
Parallax (π)8.0853 ± 0.0384 mas
Distance403 ± 2 ly
(123.7 ± 0.6 pc)
Orbit
PrimaryHD 116029 A
CompanionHD 116029 B
Semi-major axis (a)1.392"
(171 AU)
Details
HD 116029 A
Mass1.445±0.094 M
Radius4.6±0.1 R
Luminosity11.7 L
Surface gravity (log g)3.40±0.06 cgs
Temperature4894±36 K
Metallicity0.12 ± 0.02
Rotational velocity (v sin i)1.0±0.6 km/s
Age2.7±0.5 Gyr
HD 116029 B
Mass0.26 M
Surface gravity (log g)5.033±0.019 cgs
Other designations
BD+25 26232, Gaia DR2 1446584503287858560, HD 116029, HIP 65117, TYC 1994-2335-1, 2MASS J13203954+2438555
Database references
SIMBADdata

The primary subgiant star HD 116029 A belongs to the spectral class K1. Its age is younger than the Sun`s at 2.7±0.5 billion years. The primary star is slightly enriched by heavy elements, having 130% of solar abundance. The primary star does not have detectable flare activity.

In 2016 the co-moving binary stellar companion HD 116029 B was detected. It is a red dwarf star of visual magnitude 16. The companion was confirmed orbiting the primary at a projected separation of 171 AU in 2017.

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