| |
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | 19h23m 13.13745s[1] |
| Declination | −44° 47′ 59.2051″[1] |
| Apparent magnitude (V) | +4.29[2] |
| Characteristics | |
| Spectral type | F2/3 V[3] or F2 III[4] |
| U−B color index | +0.07[2] |
| B−V color index | +0.34[2] |
| Astrometry | |
| Radial velocity (Rv) | +19.0[5] km/s |
| Proper motion (μ) | RA: +93.45[1] mas/yr Dec.: −54.09[1] mas/yr |
| Parallax (π) | 24.31 ± 0.19 mas[1] |
| Distance | 134 ± 1 ly (41.1 ± 0.3 pc) |
| Absolute magnitude (MV) | +1.20[6] |
| Details | |
| Mass | 1.43[7] M☉ |
| Luminosity | 20[8] L☉ |
| Surface gravity (log g) | 3.57[7] cgs |
| Temperature | 7,035±239[7] K |
| Metallicity [Fe/H] | −0.54[5] dex |
| Rotational velocity (v sin i) | 155[9] km/s |
| Age | 933[7] Myr |
| Other designations | |
Arkab Posterior, β2 Sgr, CD−45° 13171, HD 181623, HIP 95294, HR 7343, SAO 229654[10] | |
| Database references | |
| SIMBAD | data |
Beta2 Sagittarii (β2 Sagittarii, abbreviated Beta2 Sgr, β2 Sgr) is a star in the zodiac constellationofSagittarius. It is visible to the naked eye, having an apparent visual magnitude of +4.29.[2] Based upon an annual parallax shift of 24.31 mas as seen from Earth,[1] it is located 134 light-years from the Sun.
Based upon variations in its proper motion, this is a probable astrometric binary system.[11] As such, its two components would be designated Beta2 Sagittarii A (officially named Arkab Posterior /ˈɑːrkæb pɒˈstɪəriər/, the traditional name of the system)[12][13] and B.
β2 Sagittarii (LatinisedtoBeta2 Sagittarii) is the system's Bayer designation. The designations of the two components as Beta2 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).[14]
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[15] to catalog and standardize proper names for stars. The WGSN approved the name Arkab Posterior for Beta2 Sagittarii on 5 October 2016 and it is now so included in the List of IAU-approved Star Names.[13] For such names relating to members of multiple star systems, and where a component letter (from e.g. Washington Double Star Catalog) is not explicitly listed, the WGSN says that the name should be understood to be attributed to the brightest component by visual brightness.[16]
InChinese, 天淵 (Tiān Yuān), meaning Celestial Spring, refers to an asterism consisting of Beta2 Sagittarii, Beta1 Sagittarii and Alpha Sagittarii. Consequently, the Chinese name for Beta2 Sagittarii itself is 天淵一 (Tiān Yuān yī, English: the First Star of Celestial Spring.)[17]
Houk (1978) categorizes the visible component (Beta2 Sagittarii A) as an F-type main-sequence star with a stellar classification of F2/3 V.[3] However, Malaroda (1975) lists it as an F-type giant star.[4] It is spinning rapidly with a projected rotational velocity of 155 km/s. This is giving it an oblate shape with an equatorial bulge that is 22% larger than the polar radius.[9] Beta2 Sagittarii has an estimated 1.4[7] times the mass of the Sun and is around 933[7] million years old.
