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HD 125628

Binary star system in the constellation Centaurus From Wikipedia, the free encyclopedia

HD 125628 is a binary star[3] system in the constellation Centaurus. It is faintly visible to the naked eye with a combined apparent visual magnitude of 4.76.[1] The distance to this system is approximately 380 light years based on parallax. It is drifting further away from the Sun with a radial velocity of +15 km/s.[1] The absolute magnitude is −0.55.[1]

Right ascension14h 22m 37.07301s[2]
Declination−58° 27 32.8193[2]
Apparentmagnitude(V)4.76[1] (5.09 + 6.94)[3]
Quick facts Constellation, Right ascension ...
HD 125628
Location of HD 125628 (circled in red)
Observation data
Epoch J2000      Equinox ICRS
Constellation Centaurus[1]
Right ascension 14h 22m 37.07301s[2]
Declination −58° 27 32.8193[2]
Apparent magnitude (V) 4.76[1] (5.09 + 6.94)[3]
Characteristics
A
Evolutionary stage giant[4]
Spectral type G9III[3]
B−V color index +0.795±0.003[1]
B
Evolutionary stage main sequence[5]
Spectral type F5V[3]
B−V color index +0.45[4]
Astrometry
A
Radial velocity (Rv)+14.6±2.8[1] km/s
B
Proper motion (μ) RA: −39.763 mas/yr[5]
Dec.: +24.058 mas/yr[5]
Parallax (π)13.0246±0.0192 mas[5]
Distance250.4 ± 0.4 ly
(76.8 ± 0.1 pc)
Details
A
Mass2.9[6] M
Radius12.3[6] R
Surface gravity (log g)2.73[6] cgs
Temperature5,370[6] K
Rotational velocity (v sin i)5.5[4] km/s
Age3.6[4] Gyr
B
Mass1.4[7] M
Radius2.1[7] R
Luminosity7.5[7] L
Surface gravity (log g)3.95[7] cgs
Temperature6,642[7] K
Rotational velocity (v sin i)6.3[4] km/s
Age2.7[4] Gyr
Other designations
CPD−57°6619, HD 125628, HIP 70264, HR 5371, SAO 241673[8]
Database references
SIMBADdata
Close

The primary component of this system, component A, is an aging giant star with a stellar classification of G9III[3] and a visual magnitude of 5.09.[3] The secondary companion, designated component B, is a magnitude 6.94[3] star located at an angular separation of 9.10 from the primary, along a position angle of 157°, as of 2016.[9] It is an F-type main-sequence star with a class of F5V.[3]

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