Skip to main content

Record-breaking supermassive black hole is oldest even seen in X-rays

Astronomers recently discovered the most distant black hole ever observed in the X-ray wavelength, and it has some unusual properties that could help uncover the mysteries of how the largest black holes form.

Within the center of most galaxies lies a supermassive black hole, which is hundreds of thousands or even millions or billions of times the mass of our sun. These huge black holes are thought to be related to the way in which galaxies form, but this relationship isn’t clear — and how exactly supermassive black holes grow so massive is also an open question.

The recently discovered black hole, in the galaxy UHZ1 located an incredible 13.2 billion light-years away, is a young one and its mass is currently similar to that of the galaxy in which it resides. It is visible thanks to the gravitational lensing effect of the galaxy cluster Abell 2744, shown below, which has such huge mass that it bends spacetime and magnifies the distant galaxy to make it observable. It was located using the James Webb Space Telescope and then observed using then Chandra X-Ray Observatory.

Astronomers found the most distant black hole ever detected in X-rays (in a galaxy dubbed UHZ1) using the Chandra and Webb telescopes. X-ray emission is a telltale signature of a growing supermassive black hole. This result may explain how some of the first supermassive black holes in the universe formed. This composite image shows the galaxy cluster Abell 2744 that UHZ1 is located behind, in X-rays from Chandra (purple) and infrared data from Webb (red, green, blue).
Astronomers found the most distant black hole ever detected in X-rays, in a galaxy dubbed UHZ1, using the Chandra and Webb telescopes. This composite image shows the galaxy cluster Abell 2744 that UHZ1 is located behind, in X-rays from Chandra (purple) and infrared data from Webb (red, green, blue). Credits: X-ray: NASA/CXC/SAO/Ákos Bogdán; Infrared: NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare & K. Arcand

“We needed Webb to find this remarkably distant galaxy and Chandra to find its supermassive black hole,” said lead author of the research, Akos Bogdan of the Center for Astrophysics | Harvard & Smithsonian, in a statement. “We also took advantage of a cosmic magnifying glass that boosted the amount of light we detected.”

This black hole seems to have been born massive, which allowed it to reach a large mass even at a young age. “There are physical limits on how quickly black holes can grow once they’ve formed, but ones that are born more massive have a head start. It’s like planting a sapling, which takes less time to grow into a full-size tree than if you started with only a seed,” explained another of the researchers, Andy Goulding of Princeton University.

The black hole is located within a pocket of superheated gas that is giving off X-rays, suggesting that it could have formed from the collapse of a cloud of gas. “We think that this is the first detection of an ‘Outsize Black Hole’ and the best evidence yet obtained that some black holes form from massive clouds of gas,” said fellow researcher Priyamvada Natarajan of Yale University. “For the first time, we are seeing a brief stage where a supermassive black hole weighs about as much as the stars in its galaxy, before it falls behind.”

The research is published in the journal Nature Astronomy, with other results published in Astrophysical Journal Letters.

Editors' Recommendations

Georgina Torbet
Georgina is the Digital Trends space writer, covering human space exploration, planetary science, and cosmology. She…
Unique black hole is trailed by 200,000 light-year-long tail of stars
This is an artist's impression of a runaway supermassive black hole that was ejected from its host galaxy as a result of a tussle between it and two other black holes. As the black hole plows through intergalactic space it compresses tenuous gas in front to it. This precipitates the birth of hot blue stars. This illustration is based on Hubble Space Telescope observations of a 200,000-light-year-long contrail of stars behind an escaping black hole.

Black holes might have a reputation as terrifying monsters, devouring all they come into contact with -- but they can be a force of creation too, feeding the formation of new stars. Researchers using data from the Hubble Space Telescope recently spotted an unexpectedly huge trail of stars forming in the wake of a rogue black hole.

While most very large black holes, called supermassive black holes, sit at the center of galaxies, occasionally these enormous beasts can be found wandering alone in the depths of space. That's the case with the recently discovered black hole with the mass of 20 million suns, which is streaking through the sky at tremendous speed. This likely began with two galaxies merging, each with its own supermassive black hole, which formed a binary system. Then a third galaxy got too close, and in the chaos of a three-way merger one of the black holes was kicked out and sent zipping off into space -- so fast that if it were in our solar system, it would travel from the Earth to the moon in 14 minutes.

Read more
These supermassive black holes are cozying up close together
Scientists using the Atacama Large Millimeter/submillimeter Array (ALMA) to look deep into the heart of the pair of merging galaxies known as UGC 4211 discovered two black holes growing side by side, just 750 light-years apart. This artist’s conception shows the late-stage galaxy merger and its two central black holes. The binary black holes are the closest together ever observed in multiple wavelengths.

At the center of most galaxies lies a single monster: a supermassive black hole, with a mass millions or even billions of times that of the sun. These lonely beasts typically sit alone in the heart of galaxies, but recent research found two of these monsters nestled close together in the galaxy UGC4211.

The two supermassive black holes originated in two different galaxies which are now merging into one, located relatively close by at a distance of 500 million light-years from Earth. The pair is among the closest black hole binaries ever observed, sitting just 750 light-years apart, and was observed using the Atacama Large Millimeter/submillimeter Array (ALMA).

Read more
Listen to the spooky echoes of a black hole
The black hole in V404 Cygni is actively pulling material away from a companion star — with about half the mass of the Sun — into a disk around the invisible object. A burst of X-rays from the black hole detected in 2015 created the high-energy rings from a phenomenon known as light echoes, where light bounces off of dust clouds in between the system and Earth. In these images, X-rays from Chandra are shown, along with optical data from the Pan-STARRS telescope that depict the stars in the field of view.

As well as admiring beautiful pictures of space, you can also listen to those pictures via sonifications. These take images and translate them into eerie sounds to illustrate the wonderful and strange phenomena of our universe. NASA's latest sonification illustrates the rings of X-rays that have been observed echoing around a black hole in the V404 Cygni system.

Quick Look: 'Listen' to the Light Echoes From a Black Hole

Read more