First Direct Images of ‘Cosmic Web’ That May Weave Entire Universe

A complex web of interconnected blue and red filaments resembling a cosmic or neural network pattern, with dense clusters and branching lines creating an intricate, abstract design.
This image is a simulation based on groundbreaking new images captured by an international team of astronomers. The team detected the very faint glow from the gas inside cosmic filaments, shown here in white. Where these filaments intersect, the gas inside galaxies, which helps create new stars, is shown in red/orange. | Credit: © Alejandro Benitez-Llambay/Universität Mailand-Bicocca/MPA

An international team of astronomers captured direct evidence of the filaments that weave an interconnected web throughout the cosmos.

Physicists have long theorized the existence of this cosmic web of matter, but it has proven exceptionally challenging to observe. As Earth reports, astronomers from the University of Milano-Bicocca and the Max Planck Institute for Astrophysics published new research that includes high-definition images of the filaments that connect a pair of quasar-host galaxies, providing the first direct images of the theorized cosmic web and lending credence to cold-dark-matter theories.

Many physicists believe that there is a hypothetical type of dark matter, cold dark matter, which underpins the Lambda-CDM mathematical model of the Big Bang. This is the current standard cosmological model, and despite its relatively high level of success under scientific scrutiny, the dark matter required for the model to function has been complicated to observe.

A black-and-white image of space shows two bright galaxy clusters, colored with red, orange, and purple contours, surrounded by scattered black dots representing distant stars and galaxies.
The scientists studied and observed the filament connecting two galaxies. The diffuse gas, depicted here as yellow to purple, travels along cosmic filaments. In this case, the cosmic filament is about three million light-years long. | Credit: © Davide Tornotti/University of Milano-Bicocca

Observation of dark matter and dark energy is a significant focus for modern physicists and astronomers. Scientists are using tools like the James Webb Space Telescope, the Euclid space telescope, and the groundbreaking LSST, the world’s largest digital camera, at the Vera C. Rubin Observatory to find evidence for the dark matter and dark energy scientists believe are coursing through the Universe. Current estimates suggest that only about 5% of the matter in the Universe is ordinary matter, the stuff that can be directly observed.

The new team of researchers who directly imaged cosmic filaments used the Multi-Unit Spectroscopic Explorer (MUSE) mounted on the Very Large Telescope (VLT) at the European Southern Observatory (ESO) in Chile. MUSE detects a wide range of spectra, which enables astronomers to see the very weak hydrogen emissions tied to the otherwise invisible filaments.

A bright, glowing network of purple and yellow filaments spreads across a dark background, resembling cosmic web structures or neural networks, with luminous clusters at several intersections.
During supercomputer simulations built using data observed by the MUSE instrument at the VLT in Chile, the researchers located a twin of the cosmic filament they observed in the real world. The gas that flows within the cosmic web, which feeds galaxy formation where filaments intersect, is shown here in purple. | Credit: Davide Tornotti/University of Milano-Bicocca/MPA

This very faint filament is, as Earth describes, a “gravitational highway” for cosmic gas, which includes the materials required to form new stars. The direct observation of this pathway through space provides significant evidence for cold dark matter theories, which suggest that galaxies grow by accumulating gas through a series of interconnected webs rather than through isolated clouds of matter in the interstellar medium.

“By capturing the faint light emitted by this filament, which traveled for just under 12 billion years to reach Earth, we were able to precisely characterize its shape,” says Ph.D student Davide Tornotti from the University of Milano-Bicocca. Tornotti is the lead author on the new study.

A complex web of interconnected, thin, light blue and orange lines on a dark blue background, resembling a network or cosmic web structure.

“For the first time, we could trace the boundary between the gas residing in galaxies and the material contained within the cosmic web through direct measurements,” Tornotti continues.

Tornotti and the team used MUSE’s sensitivity to capture the sharpest image ever of a cosmic filament, which spanned about three million light-years.


Image credits:High-definition imaging of a filamentary connection between a close quasar pair at z = 3‘ by Davide Tornotti et al. Additional image credit © Alejandro Benitez-Llambay/Universität Mailand-Bicocca/MPA

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