Discovery of quasar quartet may force cosmologists to rethink quasar models

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Quasars are hard to spot while in the act owing to their relatively shorter lifespans as compared to their host galaxy’s lifetime and spotting four at one time has odds of one in ten million; however, a group of astronomers led by Joseph Hennawi of the Max Planck Institute for Astronomy have managed to do just that – spotted the first ever quadruple quasar: four rare active black holes situated in close proximity to one another.

The astronomers used the W. M. Keck Observatory in Hawaii for their discovery of the quasar quartet and according to them it resides in one of the most massive structures ever discovered in the distant universe. The discovery of the quartet despite the unfavourable odds could mean that cosmologists may need to put a thought to their existing models of quasar evolution and the formation of the most massive cosmic structures.


Quasars are powered by in-fall of matter onto a supermassive black hole at the center of a galaxy and they constitute a brief phase in a galaxy’s evolution. When the in-fall of matter on the supermassive blackhole is at its peak, quasars are the most luminous objects in the universe, shining hundreds of times brighter than their host galaxies. But these hyper-luminous episodes are very short in galactic terms and one has to be very lucky to catch one in the act.

The Quarter

Clues come from peculiar properties of the quartet’s environment. The four quasars are surrounded by a giant nebula of cool dense hydrogen gas, which emits light because it is irradiated by the intense glare of the quasars. In addition, both the quartet and the surrounding nebula reside in a rare corner of the universe with a surprisingly large amount of matter. “There are several hundred times more galaxies in this region than you would expect to see at these distances,” said J. Xavier Prochaska, professor at the University of California Santa Cruz and the principal investigator of the Keck Observatory observations.

Given the exceptionally large number of galaxies, this system resembles the massive agglomerations of galaxies, known as galaxy clusters, that astronomers observe in the present-day universe. But because the light from this cosmic metropolis has been travelling for 10 billion years before reaching Earth, the images show the region as it was 10 billion years ago, less than 4 billion years after the big bang. It is thus an example of a progenitor or ancestor of a present-day galaxy cluster, or proto-cluster for short.

Piecing all of these anomalies together, the researchers tried to understand what appears to be their incredible stroke of luck. “If you discover something which, according to current scientific wisdom should be extremely improbable, you can come to one of two conclusions: either you just got very lucky, or you need to modify your theory,” Hennawi said.

The researchers speculate that some physical process might make quasar activity much more likely in specific environments. One possibility is that quasar episodes are triggered when galaxies collide or merge, because these violent interactions efficiently funnel gas onto the central black hole. Such encounters are much more likely to occur in a dense proto-cluster filled with galaxies, just as one is more likely to encounter traffic when driving through a big city.

“The giant emission nebula is an important piece of the puzzle since it signifies a tremendous amount of dense cool gas,” said Fabrizio Arrigoni-Battaia, a PhD student at the Max Planck Institute for Astronomy who was involved in the discovery.

Supermassive black holes can only shine as quasars if there is gas for them to swallow, and an environment that is gas rich could provide favorable conditions for fueling quasars.

On the other hand, given the current understanding of how massive structures in the universe form, the presence of the giant nebula in the proto-cluster is totally unexpected. “Our current models of cosmic structure formation based on supercomputer simulations predict that massive objects in the early universe should be filled with rarefied gas that is about ten million degrees, whereas this giant nebula requires gas thousands of times denser and colder,” said Sebastiano Cantalupo, currently at ETH Zurich, that led the imaging observations a the Keck Observatory during his previous research appointment at UCSC. “It is really amazing that this discovery was made the same night of the Slug Nebula while we were hunting for giant Lyman alpha nebulae illuminated by quasars — my first night at Keck Observatory and definitely the most exciting observing night I have ever had!”

“Extremely rare events have the power to overturn long-standing theories” Hennawi said.

As such, the discovery of the first quadruple quasar may force cosmologists to rethink their models of quasar evolution and the formation of the most massive structures in the universe.

The findings of the research have been published in journal Science.