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M92
Hubble · Messier 92 · ESA/Hubble & NASA; Acknowledgment: Gilles Chapdelaine

Messier 92

Star cluster in Hercules · 26,700 light-years

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TypeStar cluster
ConstellationHercules
Right ascension17h 17m 07s
Declination+43° 08′
Object distance26,700 light-years
Apparent magnitude6.5
Apparent size14.4′ (arc-minutes)
Approx. true diameter111.8 light-years across
Also known asM92 · NGC 6341
Messier 92 is a star cluster (also catalogued as NGC 6341) in Hercules — 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 14.4 arc-minutes on the sky. At about magnitude 6.5, it is an easy target for binoculars and small telescopes.

Although it appears about 14.4′ wide on the sky, its real span is roughly 111.8 light-years — the difference is a measure of how far away it lies.

Observing Messier 92

Messier 92 lies in the constellation Hercules 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 northern hemisphere, and sits low for those far south. It is a comfortable target for binoculars and small telescopes.

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