Epsilon Sagittarii

Epsilon Sagittarii
Observation data
Epoch J2000      Equinox J2000
Constellation Sagittarius
Right ascension 18h 24m 10.32s [1]
Declination –34° 23′ 04.6″ [1]
Apparent magnitude (V) 1.79
Characteristics
Spectral type B9.5 III
U−B color index -0.13
B−V color index -0.03
Variable type ?
Astrometry
Radial velocity (Rv) -15 km/s
Proper motion (μ) RA: -39.42 ± 0.22 [1] mas/yr
Dec.: -124.20 ± 0.14 [1] mas/yr
Parallax (π) 22.76 ± 0.24[1] mas
Distance 143 ± 2 ly
(43.9 ± 0.5 pc)
Absolute magnitude (MV) -1.45
Details
Mass 5 M
Radius 7 R
Luminosity 375 L
Temperature 9,200 K
Metallicity ?
Rotation 140 km/s.
Age ? years
Other designations
Kaus Australis, 20 Sagittarii, HR 6879, HD 169022, SAO 210091, FK5 689, CCDM 18242-3423, HIP 90185.

Epsilon Sagittarii (ε Sgr, ε Sagittarii) is a binary star that lies 144.64 light-years distant in the constellation Sagittarius. It has a faint, 14th magnitude, companion, Epsilon Sagittarii B, 32 arcseconds distant.

The star forms the base of the archer's "bow" in Sagittarius and also marks the base of the spout of the so-called "Teapot" asterism. Its traditional name is Kaus Australis, from Arabic قوس qaws 'bow' and Latin austrālis 'southern'.

Naming and etymology

Its traditional name is Kaus Australis, from Arabic قوس qaws 'bow' and Latin austrālis 'southern'.

The traditional Chinese name for this star is 箕宿三 (Mandarin: qí xìu sān), the Third Star of the Winnowing Basket.

Kaus Australis is listed in MUL.APIN as MA.GUR8, meaning "the Bark".[2].

References

  1. ^ a b c d e van Leeuwen, F. (2007). "HIP 90185". Hipparcos, the New Reduction. http://webviz.u-strasbg.fr/viz-bin/VizieR-5?-out.add=.&-source=I/311/hip2&recno=89886. Retrieved 2009-12-12. 
  2. ^ Rogers, J. H. (February 1998). "Origins of the ancient constellations: I. The Mesopotamian traditions". Journal of the British Astronomical Association, no.1 108: 9–28. Bibcode 1998JBAA..108....9R. 

External links