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Globular clusters

Globular clusters are densely packed groups of thousands to millions of stars, bound together by gravity. They are typically found in the halos of galaxies, including our Milky Way. These clusters are ancient, often containing some of the oldest stars in the universe, which have formed around 10 to 13 billion years ago. Globular clusters are spherical in shape and can provide valuable insights into the early stages of galaxy formation and the evolution of stars. Their beauty and density make them fascinating objects for astronomers and stargazers alike.

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    Globular clusters are large groups of tightly packed stars, often containing thousands to millions of them, all orbiting a central point in space. They are typically spherical in shape and are found in the halo of galaxies, including our Milky Way. These clusters are among the oldest objects in the universe, with ages often exceeding 10 billion years. They provide valuable insights into the early history of stars and galaxies. Studying globular clusters helps astronomers understand stellar evolution and the formation of galaxies over cosmic time.