Scale & fate of the universe

The cosmic web

Galaxies strung along threads hundreds of millions of light-years long, around voids of nearly nothing

Artist's impression · drag to rotate
Parts filaments, walls, clusters and voids [2]
Filaments about 50% of the mass in 6% of the volume [3]
Voids about 77% of the volume with 15% of the mass [3]
Clusters 11% of the mass in less than 0.1% of the volume [3]
First great wall 1989 CfA2 Great Wall, about 500 million light-years long [4]
Sloan Great Wall 1.37 billion light-years long found 2003 [5]
Clearest image of a filament 2025 about 3 million light-years long, VLT [9]

About the image. Drawn as a cloud of points: dense knots where galaxy clusters sit, and threads of galaxies running between them. The pattern is generated, not a map of the real universe, and each point stands for many galaxies.

Galaxies are not scattered evenly through space. On the largest scales they gather into a vast, sponge-like pattern called the cosmic web. Long filaments of galaxies run between dense knots, flat walls of galaxies stretch between the filaments, and between them lie the voids: huge regions where almost nothing is found.

Who holds what

Gravity built the web from tiny ripples in the young universe. Denser regions pulled in more matter and grew denser still, while emptier regions emptied further. Today the contrast is extreme. A 2014 study by Marius Cautun and colleagues, using the Millennium simulation, found that filaments hold about half of all mass in only 6% of the volume. Galaxy clusters, where filaments meet, hold 11% of the mass in less than a tenth of a percent of space. The voids fill about 77% of the volume but hold only 15% of the mass.

Mapping it

The pattern began to emerge when astronomers measured distances to thousands of galaxies and plotted them in three dimensions. In 1986 Valérie de Lapparent, Margaret Geller and John Huchra published a slice of the sky that looked like a stick figure, with the Coma Cluster as its body. In 1989 Geller and Huchra described the CfA2 Great Wall, a sheet of galaxies about 500 million light-years long. In 2003 the Sloan Digital Sky Survey revealed the Sloan Great Wall, about 1.37 billion light-years long.

Larger structures have been claimed. The Hercules–Corona Borealis Great Wall, proposed in 2013 from the positions of gamma-ray bursts, would be about 10 billion light-years across, but its existence is disputed.

In 2005 the Millennium Run, a computer simulation following just over 10 billion particles, showed that the standard model of cosmology, with its dark matter, produces a web strikingly like the one observed.

Seeing the threads

Most of the web’s gas is too thin and faint to see. Filaments are traced by the galaxies along them, not seen directly. That began to change in 2019, when Hideki Umehata and colleagues detected glowing gas filaments more than a million light-years long in a young cluster of galaxies. In 2025 a team led by Davide Tornotti used the Very Large Telescope to capture what ESO called the clearest image yet of a single filament, about 3 million light-years long, stretching between two quasars. It took about 150 hours of observing.

The Milky Way itself sits in a modest part of the web, inside a supercluster whose galaxies are all drifting towards a region called the Great Attractor.

Gallery

A tangle of glowing violet and gold filaments with bright knots where they meet, an impression of the cosmic web. AI-generated painting.
A long, thin blue filament of light curving across black space, dotted with faint points, an impression of a strand of the cosmic web. AI-generated painting.
The cosmic web, 3D artist's impression, rendered from the interactive model.
The cosmic web, 3D artist's impression, from another angle, rendered from the interactive model.
The cosmic web, 3D artist's impression, close-up, rendered from the interactive model.

Timeline

  1. 1986 A slice of the universe shaped like a stick figure reveals large-scale structure.
  2. 1989 Geller and Huchra describe the CfA2 Great Wall.
  3. 2003 The Sloan Great Wall is found.
  4. 2005 The Millennium Run simulates the web with over 10 billion particles.
  5. 2019 Glowing gas filaments are detected in a young galaxy cluster.
  6. 2025 The clearest image yet of a single filament, about 3 million light-years long.

Questions people ask

What is the cosmic web?

The large-scale pattern of the universe: filaments and walls of galaxies meeting in clusters, around vast, nearly empty voids.

How much of the universe is empty?

In simulations, voids fill about 77% of the volume but hold only about 15% of the mass.

Can we see the cosmic web?

Mostly through the galaxies along it. Its thin gas has been imaged directly only in a few places, most clearly in 2025.

Sources

  1. Wikipedia: Galaxy filament
  2. Wikipedia: Void (astronomy)
  3. Cautun et al. (2014), Evolution of the cosmic web, MNRAS
  4. Wikipedia: CfA2 Great Wall (Geller & Huchra 1989)
  5. Wikipedia: Sloan Great Wall (Gott et al. 2003)
  6. Wikipedia: Hercules–Corona Borealis Great Wall
  7. Wikipedia: Millennium Run (Springel et al. 2005)
  8. Umehata et al. (2019), Gas filaments of the cosmic web located around active galaxies in a protocluster, Science
  9. ESO (2025): Clearest image yet of a cosmic web filament (Tornotti et al., Nature Astronomy)