
science & techESA/Hubble
A galaxy cluster 4.6 billion light-years away bends the light of galaxies behind it into arcs
Gravitational lensing happens when a massive object, here a galaxy cluster, bends the path of light from objects behind it. Because mass curves space, light from distant galaxies follows a curved route around the cluster and is magnified and stretched into arcs. The cluster SPT-CL J0019-2026 in Cetus lies about 4.6 billion light-years away, and the arcs around it are galaxies far beyond it. Lensing works like a natural telescope, letting astronomers see objects too faint and distant to observe directly. This image came from a project using Hubble's spare observing time to explore the most massive distant clusters, hoping to find promising targets for future study with Hubble and the James Webb Space Telescope.
Einstein's general relativity says mass curves spacetime, so light passing a massive object follows a bent path. A strong lens can produce multiple images and stretched arcs of a background galaxy. The magnification helps astronomers study galaxies that would otherwise be too dim to detect.
Lensing is a key tool for mapping how mass is distributed, including dark matter, which emits no light but still bends it. It also lets astronomers observe very early galaxies that would otherwise be out of reach.
The bending of starlight by the Sun was first measured during a 1919 solar eclipse, a key test of Einstein's general relativity.
