A massive gravitationally bound system typically refers to a structure in the universe where a significant amount of mass, such as galaxies or galaxy clusters, is held together by gravitational forces. This binding occurs when the gravitational attraction between the constituent objects is strong enough to overcome their kinetic energy, preventing them from drifting apart. Such systems can include galaxies, star clusters, or even larger structures like superclusters, which play a crucial role in the large-scale structure of the universe.
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