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Sculptor

COSMOS / CONSTELLATIONS / SCL

Sculptor

IAU abbreviation Scl. One of the 14 southern constellations that Nicolas-Louis de Lacaille introduced after observing from the Cape of Good Hope in 1751–1752.

STAR CHART

α Sclβ Sclγ Sclδ Sclη Sclζ Scl↑ N ← E
Coloured dots are the stars of Sculptor 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
Scl
Latin name / genitive
Sculptor / Sculptoris
Position
Right ascension ≈ 0 h 28 m; declination −39° to −25°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 18° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 25 November.
Number of stars
56 stars brighter than magnitude 6.5 in the catalogue; 5 brighter than 5 and 0 brighter than 4.

INTERACTIVE LAB

Where is Sculptor 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 25 November). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

A faint constellation that Lacaille introduced in 1756 as the “sculptor’s studio”. The south galactic pole lies here; the bright Sculptor Galaxy (NGC 253) can be seen even in binoculars. From Türkiye it is followed low in the south on autumn evenings.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
α Scl4.30777B7IIIp
β Scl4.38174B9.5IVMNpe
γ Scl4.41182K1III
δ Scl4.59137A0V
η Scl4.86452M2/M3III
ζ Scl5.04503B4V
ι Scl5.18330K0III
θ Scl5.2469F3/F5V

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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