James Webb Telescope Maps 164,000 Galaxies to Reveal the Cosmic Web Across 13.7 Billion Years of History

Astronomers using NASA's James Webb Space Telescope have produced the most detailed map ever made of the universe's cosmic web — the vast, invisible scaffolding of dark matter filaments and gas sheets that organises matter on the largest scales in existence.¹² Led by researchers at the University of California, Riverside, the team catalogued 164,000 galaxies to trace the three-dimensional structure of the cosmos from the present day all the way back to a time when the universe was barely one billion years old — less than a tenth of its current age.²⁶

The research, published in The Astrophysical Journal, drew on COSMOS-Web, the largest survey yet carried out with the James Webb Space Telescope.²³ The jump in resolution and depth compared to previous cosmic web maps is substantial: structures that appeared as single undifferentiated blobs in earlier observations now resolve into distinct, complex networks of filaments, nodes, and voids, visible at epochs that were essentially unreachable before Webb came online.¹⁵

What the cosmic web is

The cosmic web is the largest-scale structure in the observable universe. It consists of enormous filaments — threads of dark matter and gas hundreds of millions of light-years long — that intersect at dense nodes where galaxy clusters form, surrounding gigantic empty regions called voids where almost no matter exists.³⁷ The web is not a static object: it has been growing and evolving since the earliest moments after the Big Bang, with galaxies forming preferentially along filaments where gas flows inward and collapses under gravity.

Understanding how the cosmic web evolved over time is a central challenge in cosmology, because its structure encodes information about the nature of dark matter, the history of galaxy formation, and the geometry of the universe itself.⁶⁸ Mapping it accurately across billions of years requires a telescope sensitive enough to detect faint, distant galaxies in the deep universe — which is precisely what Webb was designed to do.¹²

What the new map reveals

The 164,000-galaxy catalogue allows researchers to trace how the cosmic web's structure changed over 13.7 billion years of cosmic history — from a time when the universe was densely packed and rapidly evolving, through the long middle period of accelerating expansion driven by dark energy, to the present-day web of filaments visible in our cosmic neighbourhood.²⁴ The researchers can now see the web during epochs when the universe was only a few hundred million years old, an era previously inaccessible to direct observation.¹

The new data also reveals significant structural complexity that earlier surveys could not resolve. "What used to look like a single structure now resolves into many," the UC Riverside team noted in their analysis, "and details that were smoothed away before are now clearly visible."¹ This level of detail is critical for testing theoretical models of how dark matter behaves and whether the standard model of cosmology, known as Lambda-CDM, accurately describes the universe's large-scale evolution.⁶⁹

Implications for dark matter research

The cosmic web is essentially a map of dark matter — the invisible substance that makes up around 27% of the universe's total mass-energy content but interacts with ordinary matter only through gravity.⁷⁸ Because dark matter dominates the gravitational scaffolding that organises galaxies, the shape and evolution of the cosmic web is one of the most powerful tests available for dark matter models. James Webb's observations complement separate dark matter research recently published by UC Riverside and NASA's Jet Propulsion Laboratory, which revealed new details about how dark matter influences the distribution of galaxies across cosmic scales.⁹¹⁰

The COSMOS-Web catalogue represents a significant resource for the broader astronomy community: 164,000 galaxies with precise positions, distances, and physical properties, spanning nearly the full history of the universe, now publicly available for analysis by researchers worldwide.²³ Follow-up studies are expected to use the catalogue to investigate galaxy formation, the growth of supermassive black holes, and the statistical properties of the dark matter distribution in unprecedented detail.⁵⁶