Ever dreamt of being present during the birth of the first galaxies? Perhaps being able to fast-forward through billions of years of cosmic evolution to watch those galaxies grow and shape the universe we know today? Of course, that sadly isn’t possible. But thanks to a revolutionary new and unique audiovisual simulation of “virtual universes,” scientists have developed the best picture of cosmic evolution to date, and you too can see and hear it!

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A blue and purple web in the background. Two insets show galaxies. The first one shows a spiral from above and the other one shows a galaxy edge-on. The latter looks more like a line.

(Left) The so-called cosmic web, where the color encodes the projected density of gas and stars. (Right) Two of the many galaxies formed in the simulations seen face-on (top) and edge-on (right). (Image credit: Schaye et al. (2026))

“It is exhilarating to see ‘galaxies’ come out of our computer that look indistinguishable from the real thing and share many of the properties that astronomers measure in real data, such as their number, luminosities, colors and sizes,” COLIBRE team member Carlos Frenk said in a statement. “I like to tease my observer colleagues by asking, ‘Which galaxy catalogue do you think these images came from?’ What is most remarkable is that we are able to produce this synthetic universe purely by solving the relevant equations of physics in the expanding universe.”

black hole seeds.

Though most of the simulations were completed in 2025, some are still running, and the data they have already delivered will take years to analyze.

“We’re excited not just about the science, but also about creating new ways to explore it,” James Trayford, of the University of Portsmouth, U.K., who led the development of COLIBRE’s dust model and the sonification of its visualizations, said in the statement. “These tools could provide new insights, make our field more accessible, and help us build intuition for how galaxies grow and evolve.”

The COLIBRE research was published on Monday (April 13) in the journal Monthly Notices of the Royal Astronomical Society.