Gigantic clusters of galaxies pose a new dark-matter puzzle

Yellow, white and blue galaxies against a black background.

Among the galactic clusters examined by researchers seeking to understand the distribution of dark matter is MACSJ1206 (spread across centre of image), which distorts other galaxies’ light into smears and arcs. Credit: ESA/Hubble & NASA (CC BY 4.0)


The Hubble Space Telescope shows that galactic ‘lenses’ of the invisible material are more common than computer models of galaxy clumping predict.

Examination of huge clusters of galaxies has revealed that dark matter — the invisible stuff that constitutes most of the Universe’s mass — forms more galactic-scale lumps than expected.

Massimo Meneghetti at the National Institute for Astrophysics in Bologna, Italy, and his colleagues surveyed 11 clusters that each contain around 1,000 galaxies and are massive enough to curve the light of more distant galaxies as it travels past them, making the distant galaxies look like long arcs when viewed from Earth. These ‘strong gravitational lenses’ had been imaged by the Hubble Space Telescope.

As expected, most of the lensing power was centred around the clusters’ middle regions, where dark matter forms a dense ‘halo’. But Hubble’s images also enabled a finer mapping, revealing dozens of smaller lenses — like “additional bubbles of little lenses”, says co-author Priyamvada Natarajan at Yale University in New Haven, Connecticut. These ‘subhaloes’ were more numerous, and their lensing was on average ten times stronger, than predicted by computer simulations of clusters formed according to existing theories of dark matter, the authors write.

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