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2MASS near-infrared telescope survey centred on Messier 34
Messier 34 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 34

Star cluster in Perseus · 1,500 light-years

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TypeStar cluster
ConstellationPerseus
Right ascension2h 42m 07s
Declination+42° 45′
Object distance1,500 light-years
Apparent magnitude5.2
Apparent size22.5′ (arc-minutes)
Approx. true diameter9.8 light-years across
Also known asM34 · NGC 1039
Messier 34 is a star cluster (also catalogued as NGC 1039) in Perseus — 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 22.5 arc-minutes on the sky. At about magnitude 5.2, it is bright enough to glimpse with the unaided eye under a dark sky.

Although it appears about 22.5′ wide on the sky, its real span is roughly 9.8 light-years — the difference is a measure of how far away it lies.

Observing Messier 34

Messier 34 lies in the constellation Perseus 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. At its brightness it can be found with the unaided eye under a dark sky and is easy in binoculars.

See Messier 34 in Universe Finder

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