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A Hubble image of the globular cluster Omega Centauri, a collection of myriad stars colored red, white, and blue on the black background of space.
Hubble · Caldwell 80 · ESA/Hubble, NASA, Maximilian Häberle (MPIA)

Omega Centauri

Star cluster in Centaurus · 17,000 light-years

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TypeStar cluster
ConstellationCentaurus
Right ascension13h 26m 46s
Declination−47° 29′
Object distance17,000 light-years
Apparent magnitude5.3
Apparent size27′ (arc-minutes)
Approx. true diameter133.5 light-years across
Also known asC80 · NGC 5139
Caldwell 80, popularly known as the Omega Centauri, is a star cluster (NGC 5139) in Centaurus — a family of stars bound by gravity. It appears as number 80 in the Caldwell catalogue, Sir Patrick Moore's 1995 list of 109 bright deep-sky objects for amateur astronomers. It spans roughly 27 arc-minutes on the sky. At about magnitude 5.3, it can be glimpsed with the unaided eye under dark skies.

Although it appears about 27′ wide on the sky, its real span is roughly 133.5 light-years — the difference is a measure of how far away it lies.

Observing Omega Centauri

Omega Centauri lies in the constellation Centaurus and is best placed in the evening sky around April. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the southern hemisphere, and sits low for those far north. At its brightness it can be found with the unaided eye under a dark sky and is easy in binoculars.

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