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2MASS near-infrared telescope survey centred on Messier 52
Messier 52 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 52

Star cluster in Cassiopeia · 4,600 light-years

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TypeStar cluster
ConstellationCassiopeia
Right ascension23h 24m 48s
Declination+61° 36′
Object distance4,600 light-years
Apparent magnitude6.9
Apparent size9.9′ (arc-minutes)
Approx. true diameter13.2 light-years across
Also known asM52 · NGC 7654
Messier 52 is a star cluster (also catalogued as NGC 7654) in Cassiopeia — a gravitationally bound family of stars sharing a common origin. It was recorded by Charles Messier in his famous catalogue of 110 deep-sky objects. It spans roughly 9.9 arc-minutes on the sky. At about magnitude 6.9, it is an easy target for binoculars and small telescopes.

Although it appears about 9.9′ wide on the sky, its real span is roughly 13.2 light-years — the difference is a measure of how far away it lies.

Observing Messier 52

Messier 52 lies in the constellation Cassiopeia and is best placed in the evening sky around September. Its maximum altitude above the horizon depends on your latitude. It sits far enough north to be circumpolar from mid-northern latitudes, and never rises for most of the southern hemisphere. It is a comfortable target for binoculars and small telescopes.

See Messier 52 in Universe Finder

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