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2MASS near-infrared telescope survey centred on Messier 36
Messier 36 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 36

Star cluster in Auriga · 4,100 light-years

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TypeStar cluster
ConstellationAuriga
Right ascension5h 36m 18s
Declination+34° 08′
Object distance4,100 light-years
Apparent magnitude6
Apparent size7.2′ (arc-minutes)
Approx. true diameter8.6 light-years across
Also known asM36 · NGC 1960
Messier 36 is a star cluster (also catalogued as NGC 1960) 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 7.2 arc-minutes on the sky. At about magnitude 6, it is an easy target for binoculars and small telescopes.

Although it appears about 7.2′ wide on the sky, its real span is roughly 8.6 light-years — the difference is a measure of how far away it lies.

Observing Messier 36

Messier 36 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 36 in Universe Finder

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