HD 120987

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Right ascension13h 53m 32.76039s[2]
Declination−35° 39 51.3200[2]
Apparentmagnitude(V)5.565[3] (6.27 / 6.38)[4]
HD 120987
Observation data
Epoch J2000      Equinox J2000
Constellation Centaurus[1]
Right ascension 13h 53m 32.76039s[2]
Declination −35° 39 51.3200[2]
Apparent magnitude (V) 5.565[3] (6.27 / 6.38)[4]
Characteristics
Spectral type F4V (F0V + F1V)[5]
U−B color index −0.03[6]
B−V color index +0.44[6]
Astrometry
Radial velocity (Rv)−8.00±7.40[7] km/s
Proper motion (μ) RA: −83.39[2] mas/yr
Dec.: −25.36[2] mas/yr
Parallax (π)19.13±0.93 mas[2]
Distance170 ± 8 ly
(52 ± 3 pc)
Absolute magnitude (MV)+1.84[1]
Orbit[4]
Period (P)373.0 yr
Semi-major axis (a)1.519″
Eccentricity (e)0.775
Inclination (i)74.2°
Longitude of the node (Ω)112.3°
Periastron epoch (T)B 1958.57
Argument of periastron (ω)
(secondary)
90.7°
Details
HD 120987 A
Mass1.56[8] M
HD 120987 B
Mass1.53[8] M
Other designations
CD−35°9090, HD 120987, HIP 67819, HR 5222, SAO 204955[3]
Database references
SIMBADdata

HD 120987 (y Centauri or y Cen) is a star system located in the constellation Centaurus. HD 120987 is a quintuple star system located 50 pc (163 light years) from the Sun. The system has an apparent magnitude of 5.565.[3] Based on the system's parallax, it is located some 172 light-years (52 parsecs) away.[2]

HD 120987 appears to be a single F-type star with the spectral classification F4V, but closer inspection reveals it to be two similar F-type main-sequence stars with spectral classifications of F0V and F1V, respectively.[5] The two orbit each other every 373 years, and are separated by 1.519 arcseconds while taking a very eccentric orbit.[4]

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