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Giant Arc

Large-scale structure in the observable universe seen in 2021

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Through Light-year, Galaxy and Homogeneity and heterogeneity

The Giant Arc was discovered using a new method for finding large-scale structure by looking for intervening Mg II absorption lines in background quasars. It consists of two parts, GA-main (larger) and GA-sub (smaller), which appear visually linked but become distinct under algorithmic analysis.

It and the Big Ring, also discovered by Lopez, may be part of the same large-scale structure, with a galaxy filament potentially connecting the two structures.

In February 2025, a team led by Dr. Till Sawala from the University of Helsinki claimed to show that the existence of the Giant Arc does not contradict the cosmological principle, because similarly-sized structures were predicted in their cosmological simulations, as well as in random patterns.

If the Giant Arc were visible in the night sky it would form an arc occupying as much space as 20 full moons, or 10 degrees on the sky.

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