Could the secret to black hole formation be locked away in this record-breaking ancient quasar?

An artist's impression of a distant quasar with a flattened accretion disk.
A quasar that is the first in the early universe to be found by its flicker, more luminous than 2 trillion suns, could reveal how supermassive black holes grow. (Image credit: ESA/Hubble/NASA/M. Kornmesser.)

A faraway fluctuating quasar has been seen dimming and brightening by an extraordinary amount, changes in luminosity equivalent to 2 trillion times the brightness of the sun . It is the first time that a flickering quasar has been seen in the early universe, this one dating back 12.9 billion years – just around 900 million years after the Big Bang.

Quasars are the extremely active supermassive black holes at the heart of some galaxies, furiously feeding on gas that is being shoveled towards their maw, and growing as a result of this voracious feeding. As the gas circles the black hole's event horizon – the point beyond which nothing can escape the black hole – it grows hot as a result of friction, leading to the gas shining brightly. Additionally, magnetic fields can whip away some of the charged particles in the gas, blasting them away from the supermassive black hole in the form of powerful and bright jets. As such, quasars are some of the brightest objects in the universe.

More than a million quasars have been found across the universe, but only around 200 of these have been found existing in the first billion years after the Big Bang. While most quasars flicker, they usually do so by relatively modest amounts, and such flickering had not been seen in a quasar in the first billion years of cosmic history, until now.

"People have known that quasars in the nearby universe can flicker," Gene Leung of the Kavli Institute for Astrophysics and Space Research at the Massachusetts Institute of Technology (MIT) Kavli Institute for Astrophysics and Space Research, said in a statement. "The flickering comes from fluctuations in the way the gas is being fed into the black hole, and how the quasar flickers tells us something about the structure of a black hole's accretion disk and the kind of 'bites' that the black hole is eating."

The quasar in question is pumping out energy equivalent to the luminosity of 12 trillion suns, and its light fluctuates by about 20%, or 2 trillion times the luminosity of our sun, a quite remarkable amount indicative of how fast this black hole is growing.

Even so, the quasar is so distant that it is still extremely faint, so detecting these huge fluctuations wasn't easy. Not only has the light traveled a long way for a long time, but the expansion of the universe has also stretched the wavelength of that light to longer, redder wavelengths, a phenomenon called "redshift."

Distant quasar flickers like a cosmic candle

Leung and his MIT colleague Anna-Christina Eilers led a team that found the elusive flickering quasar after searching the archives of NASA's now-defunct NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) mission. NEOWISE scanned the whole sky for about 14 years, searching for hazardous asteroids, but also capturing a lot going on in the background sky.

The redshift of the quasar's light also lowered the frequency of the fluctuations. Flickering that might have taken place on timescales of days when the light left this quasar was redshifted to months by the time this light reached us. That is why NEOWISE's many years of data were invaluable.

"We saw the quasar flickering randomly over the 14-year period, much like a candle's flame flickers without a fixed pattern," said Leung.

The flickering of the quasar at different wavelengths is connected to variations in the temperature of the gas swirling around this black hole. The closer the gas is to the black hole, the hotter it is. From this, Leung's team could deduce that the gas had settled into a very flat, pancake-shaped accretion disk around the black hole.

Artist's conception of a black hole with an accretion disk, and jets of hot plasma.

An illustration of a supermassive black hole with an accretion disk, and blasting out jets of hot plasma. (Image credit: NASA/JPL-Caltech)

For an older quasar, this wouldn't be a surprise, but for such a young quasar, it is potentially revelatory. That's because supermassive black holes grow messily, and the cloud of infalling gas around a young quasar existing only 850 million years after the Big Bang should still be quite puffy, like a thick, chaotic donut-shaped torus. The gas should only flatten into a pancake shape once the quasar has matured. In other words, this quasar appears older than its years.

"I think that what this suggests is that all the messy, very rapid growth phases that we expect all black holes to go through at some point happen very, very early on, before we see them as these very bright luminous quasars," said Eilers. "That's the picture that's emerging."

Astronomers are already gaining evidence that supermassive black holes can form faster than we realized from directly collapsing clouds of gas, as evidenced by the 'little red dots' being discovered by the James Webb Space Telescope (JWST) in the early universe. The discovery of a mature quasar that existed 12.9 billion years ago bolsters the emerging theory that supermassive black holes formed early and developed fast.

"This means something happened even earlier on that led these systems to look so mature," said Leung.

Now, Leung and Eilers hope to search for even older quasars (the oldest ever seen existed 13.2 billion years ago), perhaps with the JWST, to try and capture whatever happened to cause them to grow up so quickly.

In the meantime, their findings can be read in a paper published on Monday (8th June) in Nature Astronomy.

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Keith Cooper
Contributing writer

Keith Cooper is a freelance science journalist and editor in the United Kingdom, and has a degree in physics and astrophysics from the University of Manchester. He's the author of "The Contact Paradox: Challenging Our Assumptions in the Search for Extraterrestrial Intelligence" (Bloomsbury Sigma, 2020) and has written articles on astronomy, space, physics and astrobiology for a multitude of magazines and websites.