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2MASS near-infrared telescope survey centred on Messier 39
Messier 39 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 39

Star cluster in Cygnus · 800 light-years

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TypeStar cluster
ConstellationCygnus
Right ascension21h 31m 48s
Declination+48° 26′
Object distance800 light-years
Apparent magnitude4.6
Apparent size19.5′ (arc-minutes)
Approx. true diameter4.5 light-years across
Also known asM39 · NGC 7092
Messier 39 is a star cluster (also catalogued as NGC 7092) in Cygnus — 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 19.5 arc-minutes on the sky. At about magnitude 4.6, it is bright enough to glimpse with the unaided eye under a dark sky.

Although it appears about 19.5′ wide on the sky, its real span is roughly 4.5 light-years — the difference is a measure of how far away it lies.

Observing Messier 39

Messier 39 lies in the constellation Cygnus and is best placed in the evening sky around August. 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. At its brightness it can be found with the unaided eye under a dark sky and is easy in binoculars.

See Messier 39 in Universe Finder

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