Scientists using the W. M. Keck Observatory have discovered the first quadruple quasar: four rare active black holes situated in close proximity to one another. ADVERTISING Scientists using the W. M. Keck Observatory have discovered the first quadruple quasar: four
Scientists using the W. M. Keck Observatory have discovered the first quadruple quasar: four rare active black holes situated in close proximity to one another.
The quartet resides in one of the most massive structures ever discovered in the distant universe, and is surrounded by a giant nebula of cool dense gas, the observatory said Thursday. The quadruple quasar, which researchers estimate the odds of discovering at one in 10 million, may lead cosmologists to rethink their models of quasar evolution and the formation of the most massive cosmic structures.
The results of the discovery, led by Joseph Hennawi of the Max Planck Institute for Astronomy, will be published in the May 15 edition of the journal Science.
Quasars constitute a brief phase of galaxy evolution and are the most luminous objects in the universe, shining hundreds of times brighter than their host galaxies. However, such hyper-luminous episodes last only a tiny fraction of a galaxy’s lifetime, which is why astronomers need to be very lucky to catch any given galaxy in the act. As a result, quasars are exceedingly rare in the sky, and are typically separated by hundreds of millions of light years from one another.
Astronomers were able to cue in on the quadruple quasar with clues from 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.
Researchers said given the large number of galaxies, the system resembled 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 four billion years after the “big bang” providing an example of a progenitor or ancestor of a present-day galaxy cluster.
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 likely in specific environments. One possibility, they said, is that quasar episodes are triggered when galaxies collide or merge, because these violent interactions efficiently funnel gas onto the central black hole. These encounters are 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.
However, given the current understanding of how massive structures in the universe form, the presence of the giant nebula in the proto-cluster was 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 10 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.
