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3 Centauri








3 Centauri


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3 Centauri

Observation data
Epoch J2000.0      Equinox J2000.0

Constellation

Centaurus

Right ascension
13h 51m 49.60s[1]

Declination
−32° 59′ 38.7″[1]

Apparent magnitude (V)
+4.56/+6.06
Characteristics

Spectral type
B5IIIp/B8V
U−B color index
−0.60
B−V color index
−0.13

Variable type

eclipsing binary?
Astrometry
Radial velocity (Rv) +10 km/s
Proper motion (μ) RA: -34.54 ± 0.78[1] mas/yr
Dec.: -28.21 ± 0.62[1] mas/yr
Parallax (π) 9.49 ± 0.89[1] mas
Distance 340 ± 30 ly
(105 ± 10 pc)
Absolute magnitude (MV) −0.23/+1.27
Other designations
k Centauri, V983 Centauri, HR 5210/5211, HD 120709/120710, CD−32°9676, HIP 67669, SAO 204916/204917, GC 18724/18725, CCDM J13518-3300
Database references
SIMBAD data

3 Centauri is a binary star in the constellation Centaurus. It is approximately 340 light years from Earth.


The primary component, 3 Centauri A, is a blue-white B-type giant with a mean apparent magnitude of +4.56. It is a variable star, and its brightness varies from magnitude +4.27 to +4.32 It is suspected the variations in luminosity are a result of the primary being an eclipsing binary, which would mean the system would consist of at least three objects. Its more distant companion, 3 Centauri B, is located 7.9 arcseconds away. It is a blue-white B-type main sequence dwarf and has an apparent magnitude of +6.06.



References[edit]





  1. ^ abcde van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357..mw-parser-output cite.citation{font-style:inherit}.mw-parser-output q{quotes:"""""""'""'"}.mw-parser-output code.cs1-code{color:inherit;background:inherit;border:inherit;padding:inherit}.mw-parser-output .cs1-lock-free a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-limited a,.mw-parser-output .cs1-lock-registration a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-lock-subscription a{background:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration{color:#555}.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration span{border-bottom:1px dotted;cursor:help}.mw-parser-output .cs1-hidden-error{display:none;font-size:100%}.mw-parser-output .cs1-visible-error{font-size:100%}.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-format{font-size:95%}.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-left{padding-left:0.2em}.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-right{padding-right:0.2em}
    Vizier catalog entry



















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