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2MASS near-infrared telescope survey centred on Owl Cluster
Owl Cluster · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Owl Cluster

Star cluster in Cassiopeia · 7,900 light-years

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TypeStar cluster
ConstellationCassiopeia
Right ascension1h 19m 33s
Declination+58° 17′
Object distance7,900 light-years
Apparent magnitude6.4
Apparent size7.8′ (arc-minutes)
Approx. true diameter17.9 light-years across
Also known asC13 · NGC 457
Caldwell 13, popularly known as the Owl Cluster, is a star cluster (NGC 457) in Cassiopeia — a family of stars bound by gravity. It appears as number 13 in the Caldwell catalogue, Sir Patrick Moore's 1995 list of 109 bright deep-sky objects for amateur astronomers. It spans roughly 7.8 arc-minutes on the sky. At about magnitude 6.4, it is a rewarding binocular and small-telescope target.

Although it appears about 7.8′ wide on the sky, its real span is roughly 17.9 light-years — the difference is a measure of how far away it lies.

Observing Owl Cluster

Owl Cluster lies in the constellation Cassiopeia and is best placed in the evening sky around October. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the northern hemisphere, and sits low for those far south. It is a comfortable target for binoculars and small telescopes.

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