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Lyra (Lyre)

COSMOS / CONSTELLATIONS / LYR

Lyra (Lyre)

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

STAR CHART

VegaSulafatSheliak13 Lyrδ² Lyrκ Lyr↑ N ← E
Coloured dots are the stars of Lyra 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
Lyr
Latin name / genitive
Lyra / Lyrae
Position
Right ascension ≈ 18 h 54 m; declination +26° to +47°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 87° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 1 September.
Number of stars
71 stars brighter than magnitude 6.5 in the catalogue; 14 brighter than 5 and 3 brighter than 4.

INTERACTIVE LAB

Where is Lyra 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 1 September). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

The lyre of the poet Orpheus. Vega, the fifth-brightest star in the sky, was close to the pole about 14,000 years ago and will be again in roughly 12,000 years. The Ring Nebula (M57), the “Double Double” Epsilon Lyrae and the late-April Lyrid meteor shower are here.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Vega0.0325A0Vvar
Sulafat3.25620B9III
Sheliak3.52962A8:V
13 Lyr4.08298M5IIIvar
δ² Lyr4.22736M4IIvar
κ Lyr4.33252K2IIIvar
ζ¹ Lyr4.34156Am
θ Lyr4.35832K0II

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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