Globular cluster
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A globular cluster is a spheroidal conglomeration of stars that is bound together by gravity, with a higher concentration of stars towards its center. It can contain anywhere from tens of thousands to
Messier 2
NGC 7006 is a highly concentrated, Class I globular cluster.
The Messier 80 globular cluster in the constellation Scorpius is located about 30,000 light-years from the Sun and contains hundreds of thousands of stars.
NGC 2808 contains three distinct generations of stars. NASA image
Messier 62
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Messier 62 or M62, also known as NGC 6266 or the Flickering Globular Cluster, is a globular cluster of stars located in the south of the constellation of Ophiuchus. The cluster was discovered on 7 Jun
Messier 62 by the Hubble Space Telescope
Messier 62 by the Hubble Space Telescope; 1.65′ field of view
Globular Cluster M62 – wide field view