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M30 as observed by Hubble
Hubble · Messier 30 · NASA, ESA/Hubble

Messier 30

Star cluster in Capricornus · 27,100 light-years

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TypeStar cluster
ConstellationCapricornus
Right ascension21h 40m 22s
Declination−23° 11′
Object distance27,100 light-years
Apparent magnitude7.1
Apparent size9′ (arc-minutes)
Approx. true diameter70.9 light-years across
Also known asM30 · NGC 7099
Messier 30 is a star cluster (also catalogued as NGC 7099) in Capricornus — 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 9 arc-minutes on the sky. At about magnitude 7.1, it is an easy target for binoculars and small telescopes.

Although it appears about 9′ wide on the sky, its real span is roughly 70.9 light-years — the difference is a measure of how far away it lies.

Observing Messier 30

Messier 30 lies in the constellation Capricornus and is best placed in the evening sky around August. 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. It is a comfortable target for binoculars and small telescopes.

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Sources

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