Q Centauri

Q Centauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
A
Right ascension 13h 41m 44.770s
Declination −54° 33′ 33.93″
Apparent magnitude (V) +5.22
B
Right ascension 13h 41m 44.956s
Declination −54° 33′ 39.21″
Apparent magnitude (V) +6.52
Characteristics
Spectral type B8Vn + A0V
U−B color index −0.23
B−V color index −0.05
Astrometry
A
Radial velocity (Rv)+14.49±0.74 km/s
Proper motion (μ) RA: −43.783 mas/yr
Dec.: −24.935 mas/yr
Parallax (π)11.2810±0.0956 mas
Distance289 ± 2 ly
(88.6 ± 0.8 pc)
B
Proper motion (μ) RA: −43.783 mas/yr
Dec.: −24.935 mas/yr
Parallax (π)11.3203±0.0329 mas
Distance288.1 ± 0.8 ly
(88.3 ± 0.3 pc)
Details
A
Mass2.8 M
Radius2.4 R
Luminosity70 L
Surface gravity (log g)4.12 cgs
Temperature10,740 K
B
Mass2.3 M
Radius1.6 R
Luminosity16 L
Surface gravity (log g)4.37 cgs
Temperature9,016 K
Other designations
HR 5141, HD 118991, CP−53°5725, HIP 66821, SAO 241076, GC 18495, CCDM J13417-5434
Database references
SIMBADdata
A
B

Q Centauri (Q Cen) is a binary star in the constellation Centaurus. It has a combined apparent magnitude of +4.99 and is approximately 288 light years from Earth.

The primary component, Q Centauri A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +5.2. Its companion, Q Centauri B, is a white A-type main sequence dwarf with an apparent magnitude of +6.5. The two stars are separated by 5.6 arcseconds on the sky.