NASA researchers recently unveiled a new animation that explains the intertwining relationship between two black holes, specifically pinpointing on how the binary system is able to distort and redirect light that surrounds an accretion disk.
The animation was published on April 15 and is the work of a team of researchers led by Jeremy Schnittman, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. It shows two black holes, one of which is colored in red and is about 200 million times the mass of the sun. The second black hole, which is illustrated in blue, weighs about half of that mass.
Video shows that as one black hole passes in front of the other, gravitational forces distort the paths of light that are emanating from parts of the disk, giving off a similar impression seen in circus funhouse mirrors. The goal of the animation was to demonstrate how light coming off a black hole’s accretion disk shifts and moves around a companion black hole.
It’s worth noting that the distortions detected in the animations are not seen when the viewer is examining the binary system from above, a development that serves as an example of a subtle phenomenon known as relativistic aberration. The animation shifts between an orbital plane view and an overview shot.
“We’re seeing two supermassive black holes, a larger one with 200 million solar masses and a smaller companion weighing half as much,” Schnittman said in a statement released by the US space agency. “These are the kinds of black hole binary systems where we think both members could maintain accretion disks lasting millions of years.”
“A striking aspect of this new visualization is the self-similar nature of the images produced by gravitational lensing,” Schnittman explained. “Zooming into each black hole reveals multiple, increasingly distorted images of its partner.”
In order to create the animation, Schnittman calculated the movements by tapping the capabilities of the Discover supercomputing at the NASA Center for Climate Simulation.
