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Q Centauri
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Q Centauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus[1]
A
Right ascension 13h 41m 44.770s[2]
Declination −54° 33′ 33.93″[2]
Apparent magnitude (V) +5.22[3]
B
Right ascension 13h 41m 44.956s[4]
Declination −54° 33′ 39.21″[4]
Apparent magnitude (V) +6.52[3]
Characteristics
Spectral type B8Vn + A0V[5]
U−B color index −0.23[citation needed]
B−V color index −0.05[citation needed]
Astrometry
A
Radial velocity (Rv)+14.49±0.74[2] km/s
Proper motion (μ) RA: −43.783[2] mas/yr
Dec.: −24.935[2] mas/yr
Parallax (π)11.2810±0.0956 mas[2]
Distance289 ± 2 ly
(88.6 ± 0.8 pc)
B
Proper motion (μ) RA: −43.783[4] mas/yr
Dec.: −24.935[4] mas/yr
Parallax (π)11.3203±0.0329 mas[4]
Distance288.1 ± 0.8 ly
(88.3 ± 0.3 pc)
Details
A
Mass2.8[6] M
Radius2.4[6] R
Luminosity70[6] L
Surface gravity (log g)4.12[6] cgs
Temperature10,740[6] K
B
Mass2.3[6] M
Radius1.6[6] R
Luminosity16[6] L
Surface gravity (log g)4.37[6] cgs
Temperature9,016[6] 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[1] and is approximately 288 light years from Earth.[2][4]

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.[7]

References

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