
science & techESA/Hubble
A galaxy cluster weighing 180 trillion suns bends light like a lens
Galaxy clusters are some of the most massive structures in the universe, groups of galaxies bound together by gravity. The cluster MACS J0454.1-0300 has a mass estimated at around 180 trillion times that of the Sun. Its gravity bends the path of light passing through it, so galaxies behind it appear stretched into sweeping arcs. This gravitational lensing acts as a natural magnifying glass, making objects too faint to detect otherwise visible. Astronomers use the effect to study the early universe, and Hubble's Frontier Fields programme was set up to exploit it.
Mass warps spacetime, as Einstein's general relativity describes, so light passing a massive object follows a curved path. A cluster this massive bends light from galaxies behind it, which can focus and stretch their images. The stretching forms arcs, while the amplification brightens distant galaxies enough for telescopes to detect them.
Lensing lets astronomers see galaxies from a much younger universe, which would be far too faint for current telescopes without the magnification. It also offers a way to weigh clusters directly, including their invisible dark matter.
Gravitational lensing was predicted by Einstein's general relativity and first confirmed in 1919, when starlight was observed bending around the Sun during a solar eclipse. Today lensing clusters are used to map dark matter, since the bending reveals mass whether or not it shines.
In 1936 Albert Einstein published a paper predicting that a star could be magnified by another star passing in front of it, an effect he thought too faint ever to observe.
