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Cygnus (Swan)

COSMOS / CONSTELLATIONS / CYG

Cygnus (Swan)

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

STAR CHART

DenebSadrAljanahFawarisAlbireoζ Cyg↑ N ← E
Coloured dots are the stars of Cygnus 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
Cyg
Latin name / genitive
Cygnus / Cygni
Position
Right ascension ≈ 20 h 31 m; declination +28° to +60°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 86° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 26 September.
Number of stars
276 stars brighter than magnitude 6.5 in the catalogue; 46 brighter than 5 and 15 brighter than 4.

INTERACTIVE LAB

Where is Cygnus 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 26 September). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

The swan whose form Zeus took; it is drawn as a bird flying along the Milky Way and is also known as the Northern Cross. Deneb, the most distant star of the Summer Triangle, is tens of thousands of times more luminous than the Sun. 61 Cygni, whose parallax Bessel measured in 1838 for the first time for any star, and Cygnus X-1, one of the first black-hole candidates, are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Deneb1.251,412A2Ia
Sadr2.231,832F8Ib
Aljanah2.4873K0III
Fawaris2.86165B9.5III
Albireo3.05434K3II+
ζ Cyg3.21143G8II
ξ Cyg3.72843K5Ibv
τ Cyg3.7466F1IV

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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