Pan of Globular Cluster NGC 2005 in Dorado | Hubble

Pan of Globular Cluster NGC 2005 in Dorado | Hubble

The globular cluster NGC 2005 is not unusual in and of itself; but it is a peculiarity in relation to its surroundings. NGC 2005 is located about 750 light-years from the heart of the Large Magellanic Cloud (LMC). This is the Milky Way’s largest satellite galaxy. It lies about 162,000 light-years from Earth. Globular clusters are densely-packed clusters that can be made up of tens of thousands or millions of stars. Their density means that they are tightly gravitationally bound, and are therefore, very stable. This stability contributes to their longevity—globular clusters can be billions of years old, and often contain very old stars. Thus, studying globular clusters in space can be a little like studying fossils on Earth. Fossils give insights into the characteristics of ancient plants and animals, while globular clusters illuminate the characteristics of ancient stars.

Current theories of galaxy evolution predict that galaxies merge with one another. It is widely thought that the relatively large galaxies that we observe in the modern Universe were formed via the merging of smaller galaxies. If this is correct, then astronomers would expect to see evidence that the most ancient stars in nearby galaxies originated in unique galactic environments. As globular clusters are known to contain ancient stars, and because of their stability, they are an excellent laboratory to test this hypothesis. 

NGC 2005 is such a globular cluster, and its very existence has provided evidence to support the theory of galaxy evolution via mergers. Indeed, the stars in NGC 2005 have a chemical composition that is distinct from the stars in the LMC around it. This suggests that the LMC underwent a merger with another galaxy during its history. Although the other galaxy has long-since merged and otherwise dispersed, NGC 2005 remains behind as an ancient witness to the long-past merger. 

Credit: European Space Agency/Hubble & NASA, F. Niederhofer, L. Girardi, N. Bartmann (ESA/Hubble)

Duration: 30 seconds

Release Date: June 10, 2024

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