HD 129357

G-type star in the constellation Boötes From Wikipedia, the free encyclopedia

HD 129357 is a G-type main-sequence star in the constellation Boötes that is located about 154 light years from the Sun. The measured properties of this star are very similar to those of the Sun, making it a candidate solar twin. However, it has a lower abundance of lithium than the Sun and appears to be over 3 billion years older, so it may instead be a solar analog.[8][6]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HD 129357
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes[1]
Right ascension 14h 41m 22.401s[2]
Declination +29° 03 31.70[2]
Apparent magnitude (V) 7.823[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type G2V[1]
U−B color index +0.115[4]
B−V color index +0.635[4]
Astrometry
Radial velocity (Rv)−33.2[3] km/s
Proper motion (μ) RA: +12.418[2] mas/yr
Dec.: −159.824[2] mas/yr
Parallax (π)21.0587±0.0264 mas[2]
Distance154.9 ± 0.2 ly
(47.49 ± 0.06 pc)
Absolute magnitude (MV)+4.49[1]
Details
Mass1.00±0.06[5] M
Radius1.3[2] R
Luminosity1.5[2] L
Surface gravity (log g)4.16±0.13[5] cgs
Temperature5,749±47[5] K
Metallicity [Fe/H]−0.02±0.04[5] dex
Rotational velocity (v sin i)2[6] km/s
Age8.1[3] Gyr
Other designations
BD+29 2568, HIP 71813, PPM 103504, SAO 83469[7]
Database references
SIMBADdata
Close

It was suggested by astronomer Olin Eggen that HD 129357 is a member of the Wolf 630 moving group of stars that share a common motion through space. The space velocity components of HD 129357 are (U, V, W) = (+21.3, −36.3, −32.0).[5]

References

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