2020 Kavli Prize in Astrophysics

The Norwegian Academy of Science and Letters has decided to award the Kavli Prize in Astrophysics for 2020 to

Andrew Fabian
University of Cambridge, UK

“For his groundbreaking research in the field of observational X-ray astronomy, covering a wide range of topics from gas flows in clusters of galaxies to supermassive black holes at the heart of galaxies.”

X-ray astronomy has opened up access to the extremely hot and energetic components of the Universe. In the current cosmological paradigm, the universe is a living ecosystem, in which flows of gas into galaxies and black holes at their centers, and the subsequent release of energy back into the galaxies and their surroundings all play vital roles. X-ray observations have provided stunning evidence for these processes at work, unveiling how the major constituents of such an ecosystem can profoundly influence their overall evolution.

Andrew Fabian, one of the most prolific and influential astronomers of our time, has been a leading figure in several major research areas in X-ray astronomy. On large scales, he played a vital role in revealing the mystery of and solution to the prodigious heating and cooling mechanisms operating on inter-galactic gas in clusters of galaxies. On small scales, he predicted and co-discovered high velocity X-ray spectral emission from around black holes, which allowed Fabian and his collaborators to develop a powerful method for measuring black-hole spins. These very spinning black holes may provide the energy to heat the inter-galactic gas and affect the evolution of the constituent galaxies. Fabian’s breadth of knowledge and insights on vastly different scales have provided key physical understanding of how those disparate phenomena are interconnected.

Committee Members 

Kavli Prize Committee in Astrophysics

  • Viggo Hansteen (Chair), University of Oslo, Norway
  • Alessandra Buonanno, Max Planck Institute for Gravitational Physics, Germany
  • Andrea Ghez, UCLA, US
  • Robert C. Kennicutt, Jr, University of Arizona, US
  • Irwin I. Shapiro, Harvard University, US


Andrew Fabian

University of Cambridge


Andrew Fabian is one of the world’s leading X-ray astronomers, having made major contributions to observational and theoretical astrophysics. Read Full Bio
Explanatory Notes 

Black holes as galactic engines

Black holes are among the most enigmatic objects in the universe. Created by imploding massive stars, they are so dense that the gravitational field around them completely warps space-time and prevents even light from escaping their clutches. Anything that passes their event horizon is lost from view forever. And yet we know that black holes exist. That’s because the vast amounts of energy given off in their vicinity generate signals that we can intercept, even if those signals take millions of years to reach us.

Andrew Fabian, an astronomer at Cambridge University in the UK, has spent his life studying the signals that arrive in the form of X-rays. In particular, he has scrutinised the X-rays emitted by supermassive black holes at the centre of very bright galaxies, revealing that those black holes play an intimate role in the life of galaxies and clusters of galaxies.

A supermassive black hole can be up to billions of times more massive than the Sun, its immense gravity sucking in vast amounts of gas from surrounding space. Because most of that gas arrives off-target having travelled a long way, it overshoots the black hole slightly and then gets pulled back – putting it on a spiral trajectory. The result is a thin “accretion disk” surrounding the black hole within which particles collide and give off energy, much of it at X-ray frequencies.

 An X-ray image from NASA’s Chandra satellite showing heated gas surrounding the centre of the vast Perseus galaxy cluster. Photo: © NASA/CXC/IoA/A.Fabian et al
An X-ray image from NASA’s Chandra satellite showing heated gas surrounding the centre of the vast Perseus galaxy cluster. Photo: © NASA/CXC/IoA/A.Fabian et al

These cosmic X-rays can’t be seen on Earth because they are blocked by the atmosphere. So scientists instead observe them from space. Having first measured the emission from a black-hole-like source known as Cygnus X-1 in the early 1970s, researchers have since launched a series of ever more sophisticated X-ray satellites.

In 1995, Fabian and colleagues reported having found tell-tale signs of a black-hole powered accretion disk in X-rays gathered by a Japanese-American mission known as the Advanced Satellite for Cosmology and Astrophysics. They discovered that a peak in the energy spectrum due to the emission of X-rays by iron within several very bright galaxies was broader and at slightly lower frequencies than expected. They interpreted this as an effect of Einstein’s general theory of relativity, an effect that had been predicted by Fabian and other researchers a few years earlier – that time close to a powerful source of gravity slows down when measured from outside.

Building on that research, Fabian found it was possible to measure two distinct sets of X-rays emitted close to a black hole – those generated by the accretion disk directly as well as others produced by very hot electrons close to the black hole that bounce off the disk before travelling out across space. By measuring the short time delays between the two emissions he and his collaborators were able to map the accreting gas and measure the black hole’s rate of spin.

 The active galaxy NGC 1275 is a well-known radio source (Perseus A) and a strong emitter of X-rays due to the presence of a black hole in the center of the galaxy.
The active galaxy NGC 1275 is a well-known radio source (Perseus A) and a strong emitter of X-rays due to the presence of a black hole in the center of the galaxy. Credit: X-ray: NASA/CXC/IoA/A.Fabian et al.; Radio: NRAO/VLA/G. Taylor; Optical: NASA/ESA/Hubble Heritage (STScI/AURA) & Univ. of Cambridge/IoA/A. Fabian 

But Fabian has also used X-ray data to study the effect of black holes over much greater distances. Indeed, he posed and then found a solution to a problem that has kept astronomers busy for decades – where does intergalactic gas in clusters of galaxies get its energy from? The gas between galaxies in certain bright clusters should be cool enough that it clumps together to form new stars. But astronomers observe no such star formation and measure the gas to be millions of degrees hotter than it ought to be without an extra source of energy.

Fabian and co-workers found clues to help solve the mystery in several X-ray images of the Perseus cluster taken by NASA’s Chandra satellite in the first few years of this century. These images showed a range of features within the cluster, including dark patches and ripples of brightness, spaced 30,000 light-years apart, emanating from a central dark region.

Andrew Fabian and colleagues have used NASA’s Chandra observatory, seen here in an artist’s impression, to make detailed studies of the Perseus galaxy cluster
Andrew Fabian and colleagues have used NASA’s Chandra observatory, seen here in an artist’s impression, to make detailed studies of the Perseus galaxy clusterCredits: NASA/CXC & J.Vaugha

Fabian reckoned that these features were created as a result of energy being transferred mechanically from a central black hole to the surrounding gas. The idea was that the dark regions are bubbles formed when jets of material shooting out from the black hole at right angles to the accretion disk push against the gas. The huge pressure generated then propagates outwards as a series of sound waves that heat up the gas.

That work earned Fabian a place in the Guinness Book of Records for having discovered “the deepest note in the universe” – a B-flat, 57 octaves below middle C (a sound, it was pointed out, that no-one would be able to hear). But the research also underlined the central role that black holes play in the lives of galaxies, in this case by generating negative feedback that limits both their own growth and that of surrounding stars. It might also explain why the mass of supermassive black holes is tied to the mass of their host galaxies, as has been observed.

This idea of black-hole feedback is now widely accepted. What’s more, Fabian has found that black holes in less massive galaxies than those at the centres of clusters also transfer energy, but do so more directly. In this case, their intense X-rays and ultraviolet radiation simply push dusty gas out of the host galaxy.

A number of details about these processes still remain to be filled in, including the extent to which the spin of a black hole contributes to the heating. But these details aside, says Kavli astrophysics committee chair Viggo Hansteen of the University of Oslo, there is now no doubt that black holes are the central engines heating intergalactic gas. “Every time you solve a problem others emerge,” he says. “But the central problem of ‘what is heating the gas?’ is solved.”

By Edwin Cartlidge



I was hooked on astronomy by the age of about seven, having read in a children’s encyclopedia that astronomers could work out the composition of a star from the light it emits. That seemed wonderful. I recall seeing Comet Arend-Roland when I was nine and as a teenager I followed the emerging Space Progammes and spent time studying the night sky with a one inch refractor from our back garden. Continue (pdf)

Interviews & Video 

Science in Focus - The Kavli Prize 2020 - Astrophysics:

2020 Kavli Prize Laureate Andrew Fabian:

Watch more videos of the 2020 The Kavli Prize laureate on our YouTube Channel