When scientists unveiled humanity’s historic first image of a black hole in 2019 – depicting a dark core encircled by a fiery aura of material falling toward it – they believed even richer imagery and insights were waiting to be teased out of the data.

Simulations predicted that, hidden behind the glare of the diffuse orange glow, there should be a thin, bright ring of light created by photons flung around the back of the black hole by its intense gravity.

A team of researchers led by astrophysicist Avery Broderick used sophisticated imaging algorithms to essentially “remaster” the original imagery of the supermassive black hole at the centre of the M87 galaxy.

“We turned off the searchlight to see the fireflies,” explains Broderick, an associate faculty member at Perimeter Institute and the University of Waterloo. “We have been able to do something profound – to resolve a fundamental signature of gravity around a black hole.”

By essentially “peeling off” elements of the imagery, says co-author Hung-Yi Pu, an assistant professor at National Taiwan Normal University, “the environment around the black hole can then be clearly revealed.”

To accomplish this, the team employed a new imaging algorithm within the EHT analysis framework THEMIS to isolate and extract the distinct ring feature from the original observations of the M87 black hole – as well as detect the telltale footprint of a powerful jet blasting outward from the black hole.

The researchers’ findings both confirm theoretical predictions and offer new ways to explore these mysterious objects, which are believed to reside at the heart of most galaxies.

Black holes were long considered unseeable until scientists coaxed them out of hiding with a globe-spanning network of telescopes, the Event Horizon Telescope (EHT). Using eight observatories on four continents, all pointed at the same spot in the sky and linked together with nanosecond timing; the EHT researchers observed two black holes in 2017.

The EHT collaboration first unveiled the supermassive black hole in M87 in 2019, and then in 2022, the comparatively small but tumultuous black hole at the heart of our own Milky Way galaxy, called Sagittarius A* (or Sgr A*). Supermassive black holes occupy the centre of most galaxies, packing an incredible amount of mass and energy into a small space. The M87 black hole, for example, is two quadrillion (that’s a two followed by 15 zeros) times more massive than Earth.

The M87 image scientists unveiled in 2019 was a landmark, but the researchers felt they could sharpen the image and glean new insights by working smarter, not harder. They applied new software techniques to reconstruct the original 2017 data in search of phenomena that theories and models predicted were lurking beneath the surface. The new, resulting image depicts the photon ring, comprised of a series of increasingly sharp sub-rings, which the team then stacked to get the full image.

“The approach we took involved leveraging our theoretical understanding of how these black holes look to build a customized model for the EHT data,” says Dominic Pesce, a team member based at the Center for Astrophysics | Harvard & Smithsonian. “This model decomposes the reconstructed image into the two pieces that we care most about, so we can study both pieces individually rather than blended together.”

The result was possible because the EHT is a “computational instrument at its heart,” says Broderick. “It is as dependent on algorithms as it is upon steel. Cutting-edge algorithmic developments have allowed us to probe key features of the image while rendering the remainder in the EHT's native resolution.”

The researchers’ findings were published on August 16 in The Astrophysical Journal.

Avery Broderick holds the Delaney Family John Archibald Wheeler Chair at Perimeter Institute. "We believe in their strategy and mission of bringing the brightest minds in physics together and letting them pursue their most ambitious ideas," say Kiki and Ian Delaney. "We are excited to see what Avery does next."