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2MASS near-infrared telescope survey centred on Messier 37
Messier 37 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 37

Star cluster in Auriga · 4,500 light-years

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TypeStar cluster
ConstellationAuriga
Right ascension5h 52m 18s
Declination+32° 33′
Object distance4,500 light-years
Apparent magnitude5.6
Apparent size11.4′ (arc-minutes)
Approx. true diameter14.9 light-years across
Also known asM37 · NGC 2099
Messier 37 is a star cluster (also catalogued as NGC 2099) in Auriga — 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 11.4 arc-minutes on the sky. At about magnitude 5.6, it is an easy target for binoculars and small telescopes.

Although it appears about 11.4′ wide on the sky, its real span is roughly 14.9 light-years — the difference is a measure of how far away it lies.

Observing Messier 37

Messier 37 lies in the constellation Auriga and is best placed in the evening sky around December. 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.

See Messier 37 in Universe Finder

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