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2MASS near-infrared telescope survey centred on Messier 50
Messier 50 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 50

Star cluster in Monoceros · 3,200 light-years

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TypeStar cluster
ConstellationMonoceros
Right ascension7h 02m 40s
Declination−8° 22′
Object distance3,200 light-years
Apparent magnitude5.9
Apparent size14.1′ (arc-minutes)
Approx. true diameter13.1 light-years across
Also known asM50 · NGC 2323
Messier 50 is a star cluster (also catalogued as NGC 2323) in Monoceros — 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 14.1 arc-minutes on the sky. At about magnitude 5.9, it is an easy target for binoculars and small telescopes.

Although it appears about 14.1′ wide on the sky, its real span is roughly 13.1 light-years — the difference is a measure of how far away it lies.

Observing Messier 50

Messier 50 lies in the constellation Monoceros and is best placed in the evening sky around January. Its maximum altitude above the horizon depends on your latitude. Lying near the celestial equator, it can be seen from both hemispheres. It is a comfortable target for binoculars and small telescopes.

See Messier 50 in Universe Finder

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