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2MASS near-infrared telescope survey centred on Messier 103
Messier 103 · Telescope survey view · 2MASS · University of Massachusetts and IPAC/Caltech; funded by NASA and NSF. Colour mosaic and cutout: CDS/Aladin.

Messier 103

Star cluster in Cassiopeia · 8,500 light-years

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TypeStar cluster
ConstellationCassiopeia
Right ascension1h 33m 22s
Declination+60° 39′
Object distance8,500 light-years
Apparent magnitude7.4
Apparent size4.5′ (arc-minutes)
Approx. true diameter11.1 light-years across
Also known asM103 · NGC 581
Messier 103 is a star cluster (also catalogued as NGC 581) in Cassiopeia — 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 4.5 arc-minutes on the sky. At about magnitude 7.4, it is an easy target for binoculars and small telescopes.

Although it appears about 4.5′ wide on the sky, its real span is roughly 11.1 light-years — the difference is a measure of how far away it lies.

Observing Messier 103

Messier 103 lies in the constellation Cassiopeia and is best placed in the evening sky around October. Its maximum altitude above the horizon depends on your latitude. It sits far enough north to be circumpolar from mid-northern latitudes, and never rises for most of the southern hemisphere. It is a comfortable target for binoculars and small telescopes.

See Messier 103 in Universe Finder

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