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Sagittarius (Archer)

COSMOS / CONSTELLATIONS / SGR

Sagittarius (Archer)

The Archer. IAU abbreviation Sgr. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

Kaus AustralisNunkiAscellaKaus MediaKaus BorealisAlbaldah↑ N ← E
Coloured dots are the stars of Sagittarius brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
Sgr
Latin name / genitive
Sagittarius / Sagittarii
Position
Right ascension ≈ 19 h 03 m; declination −45° to −12°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 21° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 3 September.
Number of stars
199 stars brighter than magnitude 6.5 in the catalogue; 41 brighter than 5 and 16 brighter than 4.

INTERACTIVE LAB

Where is Sagittarius tonight?

The lab opens for Ankara on today’s date. Drag the time slider through the night; the “Best night” button jumps to the date when the constellation is highest at 21:00 (around 3 September). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

A zodiac constellation drawn as a centaur drawing a bow; its bright stars form a distinctive “Teapot”. The centre of our Galaxy and its supermassive black hole, Sagittarius A*, lie in this direction. The Lagoon Nebula (M8), the Omega Nebula (M17) and the globular cluster M22 are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Kaus Australis1.79143B9.5III
Nunki2.05228B2.5V
Ascella2.6088A3IV
Kaus Media2.72348K3III
Kaus Borealis2.8278K1IIIb
Albaldah2.88510F2II/III
Alnasl2.9897K0III
η Sgr3.10146M2III

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

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