Chi Lupi

χ Lupi
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lupus
Right ascension 15h 50m 57.5376s
Declination −33° 37 37.796
Apparent magnitude (V) 3.957
Characteristics
Spectral type B9.5V + A2Vm
U−B color index −0.13
B−V color index −0.04
R−I color index −0.07
Astrometry
Radial velocity (Rv)5 ± 20 km/s
Proper motion (μ) RA: −5.92 mas/yr
Dec.: −24.91 mas/yr
Parallax (π)15.86±0.84 mas
Distance210 ± 10 ly
(63 ± 3 pc)
Details
χ Lup A
Mass2.84±0.12 M
Radius2.85±0.15 R
Luminosity63 L
Surface gravity (log g)4.08 cgs
Temperature10,200 K
Rotational velocity (v sin i)0 km/s
Age280±30 Myr
χ Lup B
Mass1.94±0.09 M
Radius1.75±0.18 R
Surface gravity (log g)4.2 cgs
Temperature9,200 K
Other designations
χ Lup, Chi Lupi, Chi Lup, 5 Lupi, 5 Lup, CD−33 10754, CPD−33 3933, FK5 586, GC 21281, HD 141556, HIP 77634, HR 5883, PPM 294334, SAO 207040
Database references
SIMBADdata

Chi Lupi (Chi Lup, χ Lupi, χ Lup) is a spectroscopic binary star in the constellation of Lupus. It has an apparent visual magnitude of approximately 3.957. The primary star in the binary is a mercury-manganese star of spectral type B9.5V; the secondary is a metallic-lined star of type A2Vm.

This system is a proper motion member of the Upper Scorpius sub-group in the Scorpius–Centaurus OB association, the nearest such co-moving association of massive stars to the Sun. The Upper Scorpius subgroup contains thousands of stars with an average age of 11 million years old at mean distances of 145 parsecs (470 light years).