(A) A dark matter map in our neighbourhood of the universe. The two large densities are dark matter halos of the Milky Way and Andromeda galaxy; (B) Zoomed-in on the dark matter map, showing a small dark matter clump ~700 million years after the Big Bang; (C-1 and C-2) stars and in the simulated ultra-faint dwarf galaxy, formed in the centre of the small dark matter halo in panel B. The two panels show two different radiation levels shortly after the Big Bang. It reveals how the ultra-faint dwarf galaxy changes its properties depending on which radiation is used. The scale on each image is in units of light years.Credit: J Sureda/A Fattahi/S Brown/S Avraham
Licence type: Attribution (CC BY 4.0)Ultra-faint dwarf galaxies – tiny satellite galaxies orbiting the Milky Way – have long been seen as cosmic fossils.
Now, a new study published today in Monthly Notices of the Royal Astronomical Society uses an unprecedented set of simulations to show just how powerfully
these faint systems can reflect the conditions of the early universe and tell us why some galaxies grew and others did not.
They could also reveal what the universe's earliest 'climate' was like – for example, the level of radiation and how this impacted whether and where stars formed.
Dwarf galaxies are often described as small cousins of the Milky Way. They form in small dark matter halos which are predicted by the standard model of cosmology. The faintest examples of such systems are extreme in both size and fragility, and lie on the boundary of our knowledge about galaxy formation and dark matter.
"In this work we presented a brand-new suite of cosmological simulations focused on the faintest galaxies in the universe, with an unprecedented resolution.
"These are by far the largest sample of such galaxies ever simulated at these resolutions," said Associate Professor Dr Azadeh Fattahi, of the Oskar Klein Centre (OKC) in Stockholm, which led the new study with the LYRA collaboration, in collaboration with Durham University and the University of Hawaii.
"The smallest galaxiesare called ultra-faint dwarf galaxies, which are a million times less massive than the Milky Way or even smaller.
They could also reveal what the universe's earliest 'climate' was like – for example, the level of radiation and how this impacted whether and where stars formed.
Dwarf galaxies are often described as small cousins of the Milky Way. They form in small dark matter halos which are predicted by the standard model of cosmology. The faintest examples of such systems are extreme in both size and fragility, and lie on the boundary of our knowledge about galaxy formation and dark matter.
"In this work we presented a brand-new suite of cosmological simulations focused on the faintest galaxies in the universe, with an unprecedented resolution.
"These are by far the largest sample of such galaxies ever simulated at these resolutions," said Associate Professor Dr Azadeh Fattahi, of the Oskar Klein Centre (OKC) in Stockholm, which led the new study with the LYRA collaboration, in collaboration with Durham University and the University of Hawaii.
"The smallest galaxiesare called ultra-faint dwarf galaxies, which are a million times less massive than the Milky Way or even smaller.
"Due to their small size these galaxies have proven very difficult to model and simulate."
This new simulation suite represents a major step forward, enabling a systematic view of how these galaxies form and evolve.
A down-to-earth analogy
"A useful analogy… is to plants and crops and how the way they grow is sensitive to the weather conditions," said Shaun Brown, who led the study while working at OKC and Durham University.
"In the same way that the yield of a crop in summer can indirectly tell you a lot about what the weather in spring must have been like, the properties of faint dwarf galaxies today can tell us a lot about the conditions, or weather, of the universe at a much earlier time."
What makes the results especially timely is that the simulations do more than reproduce faint dwarf galaxies – they suggest that these local objects can act as a probe of the universe's earliest 'climate'. The team explored how different assumptions about the early radiation environment influence which small dark matter haloes manage to form stars at all.
"In the paper we studied two different assumptions about the properties of the early universe when it was less than 500 million years old, to understand the effect on the properties of these small galaxies today when the universe is 13 billion years old," Brown explained.
"We found that these small ultra-faint galaxies are very sensitive to these changes, while more massive galaxies, like our Milky Way, don't really care," he added
"For the smallest galaxies, early conditions can decide whether they become visible galaxies – or remain starless dark matter halos."
"In the same way that the yield of a crop in summer can indirectly tell you a lot about what the weather in spring must have been like, the properties of faint dwarf galaxies today can tell us a lot about the conditions, or weather, of the universe at a much earlier time."
What makes the results especially timely is that the simulations do more than reproduce faint dwarf galaxies – they suggest that these local objects can act as a probe of the universe's earliest 'climate'. The team explored how different assumptions about the early radiation environment influence which small dark matter haloes manage to form stars at all.
"In the paper we studied two different assumptions about the properties of the early universe when it was less than 500 million years old, to understand the effect on the properties of these small galaxies today when the universe is 13 billion years old," Brown explained.
"We found that these small ultra-faint galaxies are very sensitive to these changes, while more massive galaxies, like our Milky Way, don't really care," he added
"For the smallest galaxies, early conditions can decide whether they become visible galaxies – or remain starless dark matter halos."
Future research
That sensitivity opens a clear path to testing early-universe physics with upcoming observations.
"Excitingly, in the near future we will have data from the Vera C. Rubin Observatory which will be able to find many more of these ultra faint dwarfs around the Milky Way," Dr Fattahi said.
Many astronomers hope Rubin can deliver a near-complete census of Milky Way satellite galaxies – and these simulations hint that this census may carry information far beyond our local neighbourhood.
"Our work suggests that these upcoming observations of the very local universe will be able to constrain what the universe at its infancy looked like, something we currently cannot directly access with other observations," Dr Fattahi added.
The result is particularly relevant in the light of recent discoveries, by the James Webb Space Telescope (JWST), of galaxies in the early universe, some of which are unexpectedly massive and bright.
If the early universe is producing surprises at large distances, then local relics from the same epoch – ultra-faint dwarfs – may provide an additional route to understanding what happened, according to Dr Fattahi.
Many astronomers hope Rubin can deliver a near-complete census of Milky Way satellite galaxies – and these simulations hint that this census may carry information far beyond our local neighbourhood.
"Our work suggests that these upcoming observations of the very local universe will be able to constrain what the universe at its infancy looked like, something we currently cannot directly access with other observations," Dr Fattahi added.
The result is particularly relevant in the light of recent discoveries, by the James Webb Space Telescope (JWST), of galaxies in the early universe, some of which are unexpectedly massive and bright.
If the early universe is producing surprises at large distances, then local relics from the same epoch – ultra-faint dwarfs – may provide an additional route to understanding what happened, according to Dr Fattahi.
But with research such as this there are still major practical challenges to overcome.
"Running these simulations is challenging, and extremely expensive in both time and computational resources. In total it took more than 6 months to run all of the simulations," Dr Fattahi added.
"The simulation also produces very large amounts of data (in total ~ 300 terabytes). Thismeant many of the old algorithms designed for smaller amounts of data needed updating and improving to effectively handle this new large amount of data."
Most of the work was carried out on the COSMA 8 supercomputer, which is designed for simulation-driven research. Durham University’s Institute for Computational Cosmology hosts COSMA 8 on behalf of the UK’s DiRAC High Performance Computing Facility.
Looking ahead, Dr Fattahi’s team plans to use the new suite to tackle questions that are still open in modern galaxy and structure formation, such as where can we find the very first generation of stars formed in the universe? Or what do the properties of ultra-faint dwarf galaxies tell us about the nature of dark matter?
"The simulation also produces very large amounts of data (in total ~ 300 terabytes). Thismeant many of the old algorithms designed for smaller amounts of data needed updating and improving to effectively handle this new large amount of data."
Most of the work was carried out on the COSMA 8 supercomputer, which is designed for simulation-driven research. Durham University’s Institute for Computational Cosmology hosts COSMA 8 on behalf of the UK’s DiRAC High Performance Computing Facility.
Looking ahead, Dr Fattahi’s team plans to use the new suite to tackle questions that are still open in modern galaxy and structure formation, such as where can we find the very first generation of stars formed in the universe? Or what do the properties of ultra-faint dwarf galaxies tell us about the nature of dark matter?
Media contacts:
Sam Tonkin
Royal Astronomical Society
Mob: +44 (0)7802 877 700
press@ras.ac.uk
Science contacts:
Dr Azadeh Fattahi
Oskar Klein Centre
azadeh.fattahi@fysik.su.se
Images & captions
Dwarf galaxies
Caption: (A) A dark matter map in our neighbourhood of the universe. The two large densities are dark matter halos of the Milky Way and Andromeda galaxy; (B) Zoomed-in on the dark matter map, showing a small darkmatter clump ~700 million years after the Big Bang; (C-1 and C-2) stars and gas in the simulated ultra-faint dwarf galaxy, formed in the centre of the small dark matter halo in panel B. The two panels show twodifferent radiation levels shortly after the Big Bang. It reveals how the ultra-faint dwarf galaxy changes its properties depending on which radiation is used. The scale on each image is in units of light years.
Credit: J Sureda/A Fattahi/S Brown/S Avraham
Further information
The paper ‘LYRA ultra-faints: The emergence of faint dwarf galaxies in the presence of an early Lyman-Werner background’ by Brown et al. has been published in Monthly Notices of the Royal Astronomical Society. DOI: 10.1093/mnras/stag439.
Notes for editors
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The RAS organises scientific meetings, publishes international research journals, recognises outstanding achievements by the award of medals and prizes, maintains an extensive library, supports education through grants and outreach activities and represents UK astronomy nationally and internationally. Its more than 4,000 members (Fellows), a third based overseas, include scientific researchers in universities, observatories and laboratories as well as historians of astronomy and others.
The RAS accepts papers for its journals based on the principle of successful peer review, following which experts on the Editorial Boards accept the papers for publication. The Society issues press releases based on a similar principle, but the organisations and scientists concerned have overall responsibility for their content.
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Submitted by Sam Tonkin on Fri, 24/04/2026 - 00:01
