List of galaxies with richest globular cluster systems
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This is a list of galaxies with richest known globular cluster systems. As of 2019, the galaxy NGC 6166 has the richest globular cluster system, with 39 000 globular clusters.[1] Other galaxies with rich globular cluster systems are NGC 4874, NGC 4889, NGC 3311 and Messier 87. For comparison, the Milky Way has a poor globular cluster system, with only 150-180 globular clusters.
Galaxy | Image | Number of globular clusters | Notes |
---|---|---|---|
NGC 6166 | ![]() | 39 000 ± 2000[1] | Richest known globular cluster system |
NGC 4874 | ![]() | 18 700 ± 2260[2] | Richest globular cluster system in Coma cluster |
NGC 3311 | ![]() | 16 500 ± 2000[3] | Richest globular cluster system in southern part of the sky and in Hydra cluster |
Messier 87 | ![]() | 12 000 ± 800[4] | Richest globular cluster system in Virgo Supercluster and richest in Messier Catalog. Also richest within 100 million light-years. Data from 2006 survey |
NGC 4889 | ![]() | 11 000 ± 1340[5] | Largest galaxy in this list (diameter is about 1050 000 light-years) |
IC 4051 | ![]() | 6700 ± 530[5] | Richest globular cluster system in IC catalog |
NGC 1395 | ![]() | 6000 ± 1100 | Richest globular cluster system in Eridanus Cluster, divided into two populations (red and blue) |
NGC 1399 | ![]() | 6000 ± 600 | Richest globular cluster system in Fornax Cluster, most clusters are given |
Messier 49 | ![]() | 5900 | |
Messier 60 | ![]() | 5100[6] | |
Messier 86 | ![]() | 3800 | Richest globular cluster system in Markarian's Chain |
NGC 6861 | ![]() | 3000 ± 300[7] | |
NGC 1600 | ![]() | 2850 | |
Messier 59 | ![]() | 2200 | |
Messier 89 | ![]() | 2000 | Data from 2006 survey |
Messier 84 | ![]() | 1775 ± 150 | |
Sombrero Galaxy | ![]() | 1600 ± 400 | Richest globular cluster system around named galaxy |
Centaurus A | ![]() | 1450 ± 160[8] | |
NGC 4278 | ![]() | 1378+32 −194 | |
NGC 4926 | ![]() | 1300 ± 300[5] | |
Maffei 1 | ![]() | 1100 | Closest galaxy in this list (distance is about 11 000 000 light-years) |

References
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