For the first time, astronomers have spotted enormous, galaxy-scale shock waves rattling the "cosmic web" that connects nearly all known galaxies. These cosmic waves could reveal clues about how the largest objects in the universe were sculpted.
The discovery was made by stitching and stacking thousands of radio telescope images together, which revealed the soft "radio glow" produced by shock waves from colliding matter in our universe's biggest structures.
The cosmic web is a gigantic network of crisscrossing celestial superhighways paved with hydrogen gas and dark matter. Galaxies tend to form where multiple strands of the web intersect, often in clusters numbering in the hundreds of thousands. Now a new study, published Feb. 15 in the journal Science, could provide vital clues into the nature of the mysterious magnetic fields that stretch beside these tendrils.
"Magnetic fields pervade the universe — from planets and stars to the largest spaces in-between galaxies," lead author Tessa Vernstrom, an astronomer at the International Centre for Radio Astronomy Research in Crawley, Australia, said in a statement. "However, many aspects of cosmic magnetism are not yet fully understood, especially at the scales seen in the cosmic web."
Taking shape in the chaotic aftermath of the Big Bang, the cosmic web's tendrils formed as clumps of matter from the roiling particle-antiparticle broth of the young universe — whose rapid expansion pushed the filaments outwards to form an interconnected soap-sud structure of thin films surrounding countless, mostly empty voids.
Far from being completely frozen in place, the cosmic web's matter can sometimes violently collide. When matter in the web merges, enormous shock waves send charged particles ricocheting through the web's magnetic fields, causing the particles to emit a faint radio wave glow. These shock waves have been spotted around some of the universe's largest galaxy clusters, but until now they were never observed around the web itself.
"These shock waves give off radio emissions which should result in the cosmic web 'glowing' in the radio spectrum, but it had never really been conclusively detected due to how faint the signals are," Vernstrom said.
To search for the faint signals, the researchers used data from the Global Magneto-Ionic Medium Survey, the Planck Legacy Archive, the Owens Valley Long Wavelength Array and the Murchison Widefield Array to stack radio imaging from 612,025 galaxy cluster pairs, grouped together if they were close enough to be directly connected by cosmic web tendrils. This stacking helped boost the faint radio emissions from the shock waves beyond noisy background effects.
Then, by looking only for polarized radio waves — whose rays vibrate at the same angle as each other and were predicted in simulations to be emitted by the shock waves — the researchers found the signal.
"As very few sources emit polarised radio light, our search was less prone to contamination and we have been able to provide much stronger evidence that we are seeing emissions from the shock waves in the largest structures in the universe, which helps to confirm our models for the growth of this large-scale structure," Vernstrom said.
Now that the shock waves' existence has been confirmed, they could be used to probe the nature of the enormous magnetic fields that suffuse the web, which play an unknown role in shaping the universe.
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Ben Turner is a U.K. based staff writer at Live Science. He covers physics and astronomy, among other topics like tech and climate change. He graduated from University College London with a degree in particle physics before training as a journalist. When he's not writing, Ben enjoys reading literature, playing the guitar and embarrassing himself with chess.