science & techESA/Hubble

A perfectly aligned galaxy and cluster bend light from behind into a bright Einstein ring

the gist

When a massive object sits almost exactly between us and a distant galaxy, its gravity bends the galaxy's light all the way around, forming a ring. Einstein predicted this effect in his general theory of relativity, and it is called an Einstein ring. Here the central galaxy of a cluster sits nearly in line with a background galaxy, and the background image is warped and magnified into an almost perfect circle. Other galaxies in the cluster add further distortions. Such rings are useful because they magnify galaxies too faint and distant to see otherwise.

how it works

Mass bends spacetime, so light from a background galaxy follows curved paths around a foreground mass. When the alignment is nearly perfect, the light is bent around all sides, forming a ring whose brightness is magnified.

so what

Einstein rings show general relativity working on cosmic scales and give astronomers a natural magnifying glass. Each one is a rare case where the alignment is precise enough to produce a near-perfect ring.

ESA/Hubble · CC BY 4.0

Image: ESA/Hubble & NASA, S. Jha Acknowledgement: L. Shatz