New Study Finds Hercules-Corona Borealis Great Wall Bigger and Nearer Than Thought
Astronomers have revealed that the Hercules-Corona Borealis Great Wall, a massive network of galaxies, might be bigger than they realised. By mapping the cosmos with gamma-ray bursts (GRBs)—the brightest explosions in the universe—astronomers found that this structure is even bigger than previously estimated. Surprisingly, portions of it also lie significantly closer to Earth than previously believed, challenging fundamental assumptions about how the universe is structured and evolves.
This cosmic structure was first observed in 2014 — a dense galaxy forming a filament of a supercluster.
A new study now extends the researchers’ previous work, but with a wider GRB sample. Hakkila and Zsolt Bagoly, authors of the study, have refined the measurements. They detected a number of relatively nearby GRBs in their sample. The evidence also shows the Great Wall is larger and wider than previously predicted.
Gamma-Ray Bursts Expose Structure Too Large for Current Models
According to a Space.com report, the GRBs figure prominently in the early discovery and more recent growth of the Hercules–Corona Borealis Great Wall. These explosive outbursts — from either collapsing massive stars or colliding neutron stars — produce powerful jets that can be spotted over cosmological distances. Hakkila told the publication that GRBs act as another bright beacon for identifying galaxies, even those too faint to see directly. Because of their brightness, scientists can follow matter throughout the universe more distinctly than ever.
The Great Wall, over 10 billion light-years long, challenges the cosmological principle of uniform universe appearance. Its massive size indicates gaps in current theories and implies that the universe’s formation time was insufficient for such massive structures.
THESEUS May Reveal Full Scale of Cosmic Great Wall
NASA’s Fermi Gamma-ray Burst observations reveal 542 GRB events, but more data is needed to fully understand the Great Wall’s scope due to misidentified origins and sparse sampling. Hakkila points toward the upcoming ESA mission THESEUS — the Transient High Energy Sources and Early Universe Surveyor — as the next major leap.
The mission aims to dramatically expand the catalogue of known GRBs, particularly at extreme distances. “It could finally provide the observational leverage needed to map the Hercules–Corona Borealis Great Wall to its full extent,” Hakkila told Space.com, emphasising its role in refining our understanding of the universe’s large-scale structure.
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Water ice coats many outer solar system bodies – from Jupiter’s icy moon Ganymede (above) to interstellar dust. On Earth, ice freezes into a neat crystal lattice, but in the deep cold of space it was assumed to form a completely amorphous (glassy) solid. A new study by University College London and Cambridge scientists challenges this picture. Their computer simulations and X-ray tests on cosmic “low-density” ice suggest it actually contains tiny crystalline grains. In some models roughly 20–25% of the ice was in crystal form, overturning the long-held view that space ice is entirely structureless.
Simulations reveal hidden nanocrystals
According to the paper, computer simulations of space ice showed it contains nanocrystals. In one approach, researchers cooled virtual water to –120 °C at different rates to form model “ice cubes.” Depending on the cooling speed, the simulated ice ranged from fully amorphous to partly ordered. Structures with roughly 16–19% of the molecules in tiny crystal clusters best matched published X-ray data for low-density ice. In another simulation, thousands of nanometer-sized ice grains were packed together and then the remaining water molecules were randomized. This produced ice about 25% crystalline, yet still reproduced the known diffraction pattern.
In laboratory experiments the team also made actual low-density amorphous ice by vapor deposition and gentle compression. When these samples were slowly warmed to crystallize, the resulting ice showed a “memory” of its formation method.
Implications for planets and origins of life
The findings give “a good idea of what the most common form of ice in the Universe looks like at an atomic level,” which is important for models of planet and galaxy formation. They also bear on theories of life’s origins. Partly crystalline ice has less internal space to trap organic molecules, potentially making it a less efficient vehicle for amino acids or other prebiotic compounds. However, Dr. Davies notes that pockets of fully amorphous ice still exist, so cosmic dust grains and cometary ices could continue to harbor organic ingredients in those disordered regions.
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space ice, amorphous ice, crystalline ice, UCL, University of Cambridge, nanocrystals, planetary science, origins of life, X-ray diffraction, space research, Physical Review B
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