Skip to main content

Machine learning used to sharpen the first image of a black hole

The world watched in delight when scientists revealed the first-ever image of a black hole in 2019, showing the huge black hole at the center of galaxy Messier 87. Now, that image has been refined and sharpened using machine learning techniques. The approach, called PRIMO or principal-component interferometric modeling, was developed by some of the same researchers that worked on the original Event Horizon Telescope project that took the photo of the black hole.

That image combined data from seven radio telescopes around the globe which worked together to form a virtual Earth-sized array. While that approach was amazingly effective at seeing such a distant object located 55 million light-years away, it did mean that there were some gaps in the original data. The new machine learning approach has been used to fill in those gaps, which allows for a more sharp and more precise final image.

A team of researchers, including an astronomer with NSF’s NOIRLab, has developed a new machine-learning technique to enhance the fidelity and sharpness of radio interferometry images. To demonstrate the power of their new approach, which is called PRIMO, the team created a new, high-fidelity version of the iconic Event Horizon Telescope's image of the supermassive black hole at the center of Messier 87, a giant elliptical galaxy located 55 million light-years from Earth. The image of the M87 supermassive black hole originally published by the EHT collaboration in 2019 (left); and a new image generated by the PRIMO algorithm using the same data set (right).
The image of the M87 supermassive black hole originally published by the Event Horizon Telescope collaboration in 2019 (left); and a new image generated by the PRIMO algorithm using the same data set (right). L. Medeiros (Institute for Advanced Study), D. Psaltis (Georgia Tech), T. Lauer (NSF’s NOIRLab), and F. Ozel (Georgia Tech)

“With our new machine-learning technique, PRIMO, we were able to achieve the maximum resolution of the current array,” said lead author of the research, Lia Medeiros of the Institute for Advanced Study, in a statement. “Since we cannot study black holes up close, the detail in an image plays a critical role in our ability to understand its behavior. The width of the ring in the image is now smaller by about a factor of two, which will be a powerful constraint for our theoretical models and tests of gravity.”

PRIMO was trained using tens of thousands of example images which were created from simulations of gas accreting onto a black hole. By analyzing the pictures that resulted from these simulations for patterns, PRIMO was able to refine the data for the EHT image. The plan is that the same technique can be used for future observations from the EHT collaboration as well.

“PRIMO is a new approach to the difficult task of constructing images from EHT observations,” said another of the researchers, Tod Lauer of NSF’s NOIRLab. “It provides a way to compensate for the missing information about the object being observed, which is required to generate the image that would have been seen using a single gigantic radio telescope the size of the Earth.”

In 2022, the EHT collaboration followed up its image of the black hole in M87 with a stunning image of the black hole at the heart of the Milky Way, so that image could be the next target for sharpening using this technique.

“The 2019 image was just the beginning,” said Medeiros. “If a picture is worth a thousand words, the data underlying that image have many more stories to tell. PRIMO will continue to be a critical tool in extracting such insights.”

The research is published in The Astrophysical Journal Letters.

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Swift Observatory spots a black hole snacking on a nearby star
Swift J0230 occurred over 500 million light-years away in a galaxy named 2MASX J02301709+2836050, captured here by the Pan-STARRS telescope in Hawaii.

Black holes can be hungry beasts, devouring anything that comes to close to them, including clouds of gas, rogue planets, and even stars. When stars get too close to a black hole, they can be pulled apart by gravity in a process called tidal disruption that breaks up the star into streams of gas. But a recent discovery shows a different phenomenon: a black hole that is "snacking" on a star. It's not totally destroying the star, but pulling off material and nibbling at it on a regular basis.

Black Hole Snack Attack

Read more
See the stunning image James Webb took to celebrate its first birthday
The first anniversary image from the NASA/ESA/CSA James Webb Space Telescope displays star birth like it’s never been seen before, full of detailed, impressionistic texture. The subject is the Rho Ophiuchi cloud complex, the closest star-forming region to Earth. It is a relatively small, quiet stellar nursery, but you’d never know it from Webb’s chaotic close-up. Jets bursting from young stars crisscross the image, impacting the surrounding interstellar gas and lighting up molecular hydrogen, shown in red. Some stars display the telltale shadow of a circumstellar disc, the makings of future planetary systems.

Today marks the one-year anniversary of the first images shared from the James Webb Space Telescope, and to celebrate this milestone NASA has shared yet another gorgeous image of space captured by Webb.

The new image shows a star system called Rho Ophiuchi; a busy region where new stars are being born amide swirls of dust and gas. Located just 390 light-years away, Webb was able to capture the region in stunning detail using its NIRCam instrument.

Read more
Researchers want to use gravitational waves to learn about dark matter
Artist's conception shows two merging black holes similar to those detected by LIGO.

When two sufficiently massive objects collide -- such as when two black holes merge -- the forces can actually bend space-time, creating ripples called gravitational waves. These gravitational waves can be detected even from millions of light-years away, making them a way to learn about distant, dramatic events in far-off parts of the universe. And now, a team of astronomers has come up with a method for using gravitational waves to study the mysterious phenomenon of dark matter.

The idea of the research was to create different computer models of what gravitational waves from black hole mergers would look like in universes with different types of dark matter. By comparing the models to what is seen in the real world, we can learn more about what type of dark matter is most likely.

Read more