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Beta Sagittarii

β¹ Sagittarii
Diagram showing star positions and boundaries of the Sagittarius constellation and its surroundings
Cercle rouge 100%.svg

Location of Beta Sagittarii (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 19h 22m 38.3s
Declination −44° 27' 32"
Apparent magnitude (V) +3.96
Distance 378 ± 42 ly
(116 ± 13 pc)
Spectral type B9V
Other designations
Arkab Prior, CCDM J19226-4428A, CPD-40  8955, FK5 1502, GC 26703, HD 181454, HIP 95241, HR 7337, PPM 325041 , SAO 229646, WDS J19226-4428A
β² Sagittarii
Observation data
Epoch       Equinox
Constellation Sagittarius
Right ascension 19h 23m 13.2s
Declination -44° 47' 59"
Apparent magnitude (V) +4.27
Distance 139 ± 5 ly
(43 ± 2 pc)
Spectral type F2III
Other designations
Arkab Posterior, CPD-45  9701, GC 26718, HD 181623, HIP 95294, HR 7343, PPM 325051, SAO 229654,

Beta Sagittarii (β Sagittarii, abbreviated Beta Sgr, β Sgr) is the common designation shared by two star systems in the constellation of Sagittarius, themselves designated β¹ Sagittarii (itself a binary star) and β² Sagittarii. β¹ and β² Sagittarii are approximately 378 and 139 light years, respectively, from Earth. The two systems are separated by 0.36° in the sky.

β¹ Sagittarii's two components are designated β¹ Sagittarii A, also named Arkab Prior, and β¹ Sagittarii B (sometimes designated Arkab Prior A and B). β² Sagittarii is named Arkab Posterior. Beta Sagittarii is also referred to by the traditional name Arkab.

β Sagittarii (Latinised to Beta Sagittariii) is the system's Bayer designation; β¹ and β² Sagittarii, those of its two constituents. The designations of β¹'s components - β¹ Sagittarii A and B - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).

The system's traditional name Arkab derives from the Arabic عرقوب carqūb meaning Achilles Tendon. The two constituents bore the traditional names Arkab Prior and Arkab Posterior since β¹ leads β² (or β² follows β¹) across the sky. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalogue and standardize proper names for stars. The WGSN states that in the case of multiple stars the name should be understood to be attributed to the brightest component by visual brightness. The WGSN approved the names Arkab Prior and Arkab Posterior for β¹ Sagittarii A and β² Sagittarii on 5 October 2016 and they are now so entered in the IAU Catalog of Star Names.


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