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

Butterfly Cluster

Star cluster in Scorpius · 1,600 light-years

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TypeStar cluster
ConstellationScorpius
Right ascension17h 40m 21s
Declination−32° 15′
Object distance1,600 light-years
Apparent magnitude4.2
Apparent size15.6′ (arc-minutes)
Approx. true diameter7.3 light-years across
Also known asM6 · NGC 6405
Messier 6, popularly known as the Butterfly Cluster, is a star cluster (also catalogued as NGC 6405) in Scorpius — 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 15.6 arc-minutes on the sky. At about magnitude 4.2, it is bright enough to glimpse with the unaided eye under a dark sky.

Although it appears about 15.6′ wide on the sky, its real span is roughly 7.3 light-years — the difference is a measure of how far away it lies.

Observing Butterfly Cluster

Butterfly Cluster lies in the constellation Scorpius and is best placed in the evening sky around June. Its maximum altitude above the horizon depends on your latitude. It is best placed for observers in the southern hemisphere, and sits low for those far north. At its brightness it can be found with the unaided eye under a dark sky and is easy in binoculars.

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