HD 126129 and HD 126128

Triple star system in the constellation of Boötes From Wikipedia, the free encyclopedia

HD 126129 and HD 126128 form a triple star in the northern constellation of Boötes. HD 126128 is a very close pair which lies at an angular separation of 6.250 from the brightest member of the trio, HD 126129.[7]

Quick facts Observation data Epoch J2000 Equinox J2000, Apparent magnitude (V) ...
HD 126129 and HD 126128
Observation data
Epoch J2000      Equinox J2000
Constellation Boötes[1]
HD 126129
Right ascension 14h 23m 22.69548s[2]
Declination +08° 26 47.8266[2]
Apparent magnitude (V) 5.04[3]
HD 126128
Right ascension 14h 23m 22.59914s[4]
Declination +08° 26 41.6666[4]
Apparent magnitude (V) 6.74[3] (7.50 + 7.70)[5]
Characteristics
HD 126129
Evolutionary stage main sequence[6]
Spectral type A0V[7]
U−B color index −0.08[8]
B−V color index −0.02[8]
HD 126128
Spectral type F0V + F2V[7]
U−B color index −0.01[8]
B−V color index +0.43[8]
Astrometry
HD 126129
Radial velocity (Rv)−22.6[9] km/s
Proper motion (μ) RA: −75.188[2] mas/yr
Dec.: −9.265[2] mas/yr
Parallax (π)14.3216±0.1123 mas[2]
Distance228 ± 2 ly
(69.8 ± 0.5 pc)
HD 126128
Radial velocity (Rv)−17.6[9] km/s
Proper motion (μ) RA: −83.783[4] mas/yr
Dec.: −4.601[4] mas/yr
Parallax (π)9.7572±0.7363 mas[10]
Distance330 ± 30 ly
(102 ± 8 pc)
Orbit[11]
PrimaryB
NameC
Period (P)40.0 yr
Semi-major axis (a)0.24″
Eccentricity (e)0.25
Inclination (i)42°
Details
HD 126129
Mass2.4[2] M
Radius2.4[2] R
Luminosity47[2] L
Surface gravity (log g)3.95[2] cgs
Temperature9,729[2] K
Rotational velocity (v sin i)133[6] km/s
Age381[2] Myr
B
Mass1.37 M
Rotational velocity (v sin i)133[12] km/s
C
Mass1.31 M
Other designations
BD+09°2882, HIP 70327, ADS 9247, WDS J14234+0827[13]
HD 126129: HD 126129, HR 5386, SAO 120426
HD 126128: HD 126128, HR 5385
Database references
SIMBADdata
HD 126129
HD 126128
Close

The Hipparcos parallax for the combined triple is 15.17±0.42 mas, suggesting a distance around 215 light years.[14] The Gaia DR3 parallax for HD 126129 (component A) indicates a distance close to 228 light years. Gaia DR3 does not contain a parallax for the BC pair HD 126128, but Gaia DR2 indicates an approximate distance of 330 light years. However, the stars are treated as being related and both are considered members of the IC 2391 supercluster.[15]

References

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