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Lacerta (Lizard)

COSMOS / CONSTELLATIONS / LAC

Lacerta (Lizard)

The Lizard. IAU abbreviation Lac. One of the seven constellations introduced by Johannes Hevelius and published in his star atlas of 1690.

STAR CHART

α Lac1 Lac5 Lacβ Lac11 LacHIP 109754↑ N ← E
Coloured dots are the stars of Lacerta 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
Lac
Latin name / genitive
Lacerta / Lacertae
Position
Right ascension ≈ 22 h 34 m; declination +36° to +57°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 84° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 27 October.
Number of stars
69 stars brighter than magnitude 6.5 in the catalogue; 13 brighter than 5 and 1 brighter than 4.

INTERACTIVE LAB

Where is Lacerta 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 27 October). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

A small zigzag constellation that Hevelius placed between Cygnus and Andromeda in 1687. BL Lacertae, once thought to be a variable star, turned out to be the brilliant nucleus of a distant galaxy and gave its name to the class of blazars.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
α Lac3.76103A1V
1 Lac4.14621K3III
5 Lac4.341,647M0II
β Lac4.42170G9III
HIP 1097544.50482K3III
11 Lac4.50333K3III
6 Lac4.521,717B2IV
2 Lac4.55555B6V

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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