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What is the name of the largest cosmic superstructure ever detected, a chain of 68 galaxy clusters at least 1.4 billion light-years long, revealed by astronomers in early 2025?

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Quipu - current events illustration
Quipu — current events

Astronomers in early 2025 unveiled the largest cosmic superstructure ever reliably detected, a colossal chain of 68 galaxy clusters stretching at least 1.4 billion light-years across the universe. This monumental discovery was named Quipu, after the ancient Incan system of knotted cords used for record-keeping, a fitting moniker given its appearance as a long filament with numerous side branches of galaxy clusters. The sheer scale of Quipu, encompassing an astounding 200 quadrillion solar masses, makes it the most massive known structure in the local universe and a new benchmark for understanding the cosmos.

The identification of Quipu, made possible through the analysis of X-ray galaxy clusters detected by the ROSAT X-ray satellite, has profound implications for our understanding of cosmic evolution. This immense structure surpasses previous record holders, such as the Sloan Great Wall, challenging existing cosmological models and prompting scientists to refine their theories about how the universe's large-scale architecture formed and developed. Such superstructures are not merely passive collections of matter; their immense gravitational pull actively influences their surroundings, affecting phenomena like the cosmic microwave background and potentially distorting measurements of the universe's expansion rate.

Quipu is not alone in its grandeur; it is one of five prominent superstructures identified in the study, which collectively account for a significant portion of the observable universe's contents. These structures together contain about 45% of all galaxy clusters, 30% of galaxies, and 25% of the total matter, occupying 13% of the universe's volume. Studying these immense formations provides invaluable insights into galaxy evolution and allows astronomers to test and improve the accuracy of cosmological measurements, offering a clearer picture of the universe's intricate web-like structure.