Epoch J2000.0 Equinox J2000.0
|Right ascension||18h 27m 58.24072s|
|Declination||−25° 25′ 18.1146″|
|Apparent magnitude (V)||+2.82|
|Spectral type||K0 IV|
|U−B color index||+0.903|
|B−V color index||+1.045|
|Radial velocity (Rv)||−43.5 km/s|
|Proper motion (μ)||RA: −44.76 mas/yr
Dec.: −185.66 mas/yr
|Parallax (π)||41.72 ± 0.16 mas|
|Distance||78.2 ± 0.3 ly
(23.97 ± 0.09 pc)
|Surface gravity (log g)||2.90 cgs|
|Metallicity [Fe/H]||–0.20 dex|
|Rotational velocity (v sin i)||3.81 km/s|
With an apparent visual magnitude of +2.82, this is one of the brighter members of the constellation and, accordingly to the Bortle Dark-Sky Scale, it is readily visible to the naked eye. Based upon parallax measurements, it is located at a distance of 78.2 light-years (24.0 parsecs) from the Sun. Being near the ecliptic, Lambda Sgr is sometimes occulted by the Moon and, more rarely, by a planet. The last planet to pass in front of it was Venus, on 19 November 1984. The previous occasion was on 5 December 1865, when it was occulted by the planet Mercury.
Kaus Borealis is a subgiant star with a stellar classification of K0 IV. It has a mass 2.6 times that of the Sun. The interferometry-measured angular diameter of this star, after correction for limb darkening, is 4.24 ± 0.05 mas. At the estimated distance of Lambda Sagittarii, this yields a physical size of about 11 times the radius of the Sun. This expanded outer envelope is radiating energy at an effective temperature of 4,770 K, causing it to glow with the cool orange hue of a K-type star. It appears to be rotating at a leisurely rate, with a projected rotational velocity of 3.81 km s−1.
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) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Borealis for this star.
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.
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 (النعم الوارد), "The Going Ostriches" and Al Naʽām al Ṣādirah (النعم السادرة), "The Returning Ostriches".
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 known as 斗宿二 (Dǒu Sù èr, English: the Second Star of Dipper.)
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- (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日