Lambda Sagittarii
Observation data J2000.0
| ||
---|---|---|
Constellation | Sagittarius | |
Right ascension | 18h 27m 58.24072s[1] | |
Declination | −25° 25′ 18.1146″[1] | |
Apparent magnitude (V) | +2.82[2] | |
Characteristics | ||
Spectral type | K0 IV[3] | |
U−B color index | +0.903[4] | |
B−V color index | +1.045[4] | |
Absolute magnitude (MV) | 1.07±0.008[5] | |
Details Rotational velocity (v sin i)3.81 km/s | | |
PPM 268438 | ||
Database references | ||
SIMBAD | data |
Lambda Sagittarii (Latinized from λ Sagittarii), formally named Kaus Borealis /ˈkɔːs bɒriˈælɪs/,[8][9] is a star in the southern constellation of Sagittarius. The star marks the top of the Archer's bow.
Properties
With an
Being 2.1 degrees south of the ecliptic, Lambda Sgr is sometimes occulted by the Moon and, rarely, by a planet. The last planet to pass in front of it was Venus, on 19 November 1984. The previous occasion was 5 December 1865, when it was occulted by Mercury.[citation needed]
Kaus Borealis is a
Nomenclature
λ Sagittarii (Latinised to Lambda Sagittarii) is the star's Bayer designation.
It bore the traditional name Kaus Borealis, which derives from the Arabic قوس qaws 'bow' and Latin boreālis 'northern'. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[12] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[13] included a table of the first two batches of names approved by the WGSN; which included Kaus Borealis for this star.
This star, with Gamma Sagittarii, Delta Sagittarii, Epsilon Sagittarii, Zeta Sagittarii, Sigma Sagittarii, Tau Sagittarii and Phi Sagittarii comprises the Teapot asterism.[14]
In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Rai al Naaim, which was translated into Latin as Pastor Struthionum, meaning keeper of the ostriches.[15]
This star is Al Tizini's Rāʽi al Naʽāïm (ألراع ٱلنعم), the Keeper of the Naʽams (Ostrich), meaning the "keeper" the two asterisms al-Naʽām al-Wārid ( النعام الوارد ), "The Going Ostriches" and al-Naʽām al-Ṣādir (النعم الصادر), "The Returning Ostriches".[16]
In Chinese, 斗 (Dǒu), meaning Dipper, refers to an asterism consisting of Lambda Sagittarii, Phi Sagittarii, Mu Sagittarii, Sigma Sagittarii, Tau Sagittarii and Zeta Sagittarii. Consequently, Lambda Sagittarii itself is 斗宿二 (Dǒu Sù èr, English: the Second Star of Dipper.)[17]
References
- ^ S2CID 18759600.
- ^ Bibcode:1999VeARI..35....1W.
- ^ S2CID 119476992.
- ^ Bibcode:1966PDAUC...1....1G.
- S2CID 119187733.
- ^ S2CID 214802418
- ^ Bibcode:1988A&A...190..148E.
- ISBN 978-1-931559-44-7.
- ^ "IAU Catalog of Star Names". Retrieved 28 July 2016.
- ^ S2CID 10436552.
- Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the originalon March 18, 2012, retrieved 2012-01-16.
- ^ "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
- ^ "Bulletin of the IAU Working Group on Star Names, No. 1" (PDF). Retrieved 28 July 2016.
- ^ "Teapot". constellation-guide.com. Retrieved 2017-05-13.
- .
- ISBN 0-486-21079-0. Retrieved 2012-09-04.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日