Distribution of dark matter in the Universe

In this illustration the NASA/ESA Hubble Space Telescope looks back in time to "map" evolving dark matter. The dataset is created by splitting the background source galaxy population into discrete epochs of time (like cutting through geological strata), looking back into the past. This is calibrated by measuring the cosmological redshift of the lensing galaxies used to map the dark matter distribution, and putting them into different time/distance "slices".

Background galaxies are lensed, or distorted, by all structures in their foreground. Thus, the more distant background galaxies are selected, the more structures can be detected. Here the respective strengths of the lensing effect depend on the distances involved.

The projected mass distributions inferred from the low, intermediate, and high redshift galaxies are shown in blue, green and red, respectively. Nearby structures may be detected by all subsets (as exemplified by the "blob" appearing on the top left of each panel), while very distant structures can only be detected by even more distant background galaxies, and thus appear in the red map only.

The new study presents the most comprehensive analysis of data from the COSMOS survey. These researchers have, for the first time ever, used Hubble and the natural "weak lenses" in space to characterise the accelerated expansion of the Universe.