
science & techESA/Hubble
One cluster or two?
The galaxy cluster Abell 3192 was first catalogued as a single cluster, but measurements showed it is actually two separate clusters at different distances. The nearer group lies about 2.3 billion light-years away and the farther one about 5.4 billion light-years away. Both are enormous, with masses thought to be roughly 30 and 120 trillion times the Sun's. Their combined mass bends light from more distant galaxies, which is why background galaxies appear stretched into curved arcs. This acts as a natural gravitational lens.
Massive objects curve spacetime, so light from distant galaxies passing nearby is deflected, much like a lens bends light. The cluster's dark matter provides most of the mass, so the amount of distortion reveals how the mass is spread out. Two peaks in that distortion pointed to two clusters.
Clusters like this let astronomers measure dark matter indirectly, by how strongly they bend light, and they can be mistaken for single objects when seen only in projection. Telling them apart changes how mass is mapped across the universe.
Gravitational lensing has been used since the 1979 discovery of the first lensed quasar to map dark matter in clusters, and reclassifications of catalogued objects are common as surveys improve.
Gravitational lensing was predicted by Einstein's general relativity, and it is one of the main ways astronomers map dark matter.
