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Thousands of bright stars fill a spherically shaped globular cluster. In the center, most of the stars appear blue. The globular cluster’s bright blue-white core is surrounded by a thick shell of yellower stars, seen in differing sizes according to their position in the spherical star cluster. They spread out beyond the edges of the image, appearing smaller and sparser at the corners of the image. A distant spiral galaxy is also visible in the lower-left corner of the image.
Hubble · Messier 72 · ESA/Hubble & NASA, A. Sarajedini, G. Piotto, M. Libralato

Messier 72

Star cluster in Aquarius · 54,600 light-years

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TypeStar cluster
ConstellationAquarius
Right ascension20h 53m 28s
Declination−12° 32′
Object distance54,600 light-years
Apparent magnitude9
Apparent size4.5′ (arc-minutes)
Approx. true diameter71.5 light-years across
Also known asM72 · NGC 6981
Messier 72 is a star cluster (also catalogued as NGC 6981) in Aquarius — 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 9, it shows up well in a small backyard telescope.

Although it appears about 4.5′ wide on the sky, its real span is roughly 71.5 light-years — the difference is a measure of how far away it lies.

Observing Messier 72

Messier 72 lies in the constellation Aquarius and is best placed in the evening sky around August. Its maximum altitude above the horizon depends on your latitude. Lying near the celestial equator, it can be seen from both hemispheres. A small backyard telescope will show it; binoculars may hint at it under dark skies.

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