Astronomers have created a simulation of the universe with more realistic galaxies that are similar in mass, size and age to real ones.
The simulation provides a glimpse of how cosmos evolved into its current state over the past 14 billion years.
The simulations developed by an international team of astronomers, based at the Universities of Leiden in the Netherlands and Durham in the UK, took several months to run at the "Cosmology Machine" in Durham and at "Curie" in Paris, among the largest computers used for scientific research in the UK and France, respectively.
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For years, astronomers have studied the formation of galaxies using computer simulations, but with limited success. The galaxies that formed in previous simulations were often too massive, too small, too old and too spherical.
The galaxies formed in the EAGLE-simulation (Evolution and Assembly of GaLaxies and their Environments) are a much closer reflection of real galaxies thanks to the strong galactic winds, which blow away the gas supply needed for the formation of stars, researchers said.
EAGLE's galaxies are lighter and younger because fewer stars form and they form later.
In the EAGLE simulation these galactic winds - which are powered by stars, supernova explosions and supermassive black holes - are stronger than in earlier simulations.
The sizes and shapes of the thousands of galaxies that form in the EAGLE simulation are also similar to those of galaxies that astronomers observe in the universe.
"The universe generated by the computer is just like the real thing. There are galaxies everywhere, with all the shapes, sizes and colours I've seen with the world's largest telescopes. It is incredible. In the EAGLE universe I can even press a button to make time run backwards," said coauthor Richard Bower from Durham University.
Having developed a simulation which produces galaxies with characteristics similar to observed galaxies, astronomers led by professor Joop Schaye of Leiden University, can now study the evolution of individual galaxies in detail.
The study appears in journal Monthly Notices of the Royal Astronomical Society.