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Trio of supermassive black holes shake space-time26.06.2014 - (idw) Max-Planck-Institut für Radioastronomie
Astronomers have discovered three closely orbiting supermassive black holes in a galaxy more than 4 billion light years away. This is the tightest trio of black holes known to date. The discovery suggests that such closely packed supermassive black holes are far more common than previously thought. An international research team, including Hans-Rainer Klöckner from MPIfR, performed VLBI observations at a number of frequencies to discover the inner two black holes of the system. In this project the Effelsberg 100m radio telescope took part in European VLBI network (EVN) observations covering two radio frequencies.
Galaxies are believed to evolve through merging and that should lead to multiple supermassive black holes in some of those galaxies at a given time. The source under investigation was found in the Sloan Digital Sky Survey (SDSS) and has the catalog number SDSS J1502+1115. It is a quasar, the nucleus of an active galaxy at a redshift of z = 0.39, corresponding to a distance of more than four billion light years. A triple black hole system has been identified in that source, with two tight companions separated by less than 500 light years.
What remains extraordinary to me is that these black holes, which are at the very extreme of Einsteins Theory of General Relativity, are orbiting one another at 300 times the speed of sound on Earth, says Roger Deane from University of Cape Town/South Africa, the lead author of the paper. Not only that, but using the combined signals from radio telescopes on four continents we are able to observe this exotic system one third of the way across the Universe. It gives me great excitement as this is just scratching the surface of a long list of discoveries that will be made possible with the Square Kilometre Array.
Such systems are important to understand for several reasons; in terms of galaxy evolution it is known that black holes influence how galaxies evolve, and understanding how often black holes themselves merge is key to this work. Furthermore, closely orbiting systems such as this are sources of gravitational waves in the Universe, if General Relativity is correct. Future radio telescopes such as the Square Kilometre Array (SKA) will be able to measure the gravitational waves from such systems as their orbits decrease.
At this point, very little is actually known about black hole systems that are so close to one another that they emit detectable gravitational waves. This discovery not only suggests that close-pair black hole systems are much more common than previously expected, but also predicts that radio telescopes such as MeerKAT and African VLBI Network will directly assist in the detection and understanding of the gravitational wave signal, says Matt Jarvis from the Universities of Oxford and the Western Cape. Further in the future the SKA will allow us to find and study these systems in exquisite detail, and really allow us gain a much better understanding of how black holes shape galaxies over the history of the Universe.
While the VLBI technique was essential to discover the inner two black holes (which are in fact the second closest pair of supermassive black holes known), Deane and co-authors have also shown that the binary black hole presence can be revealed by much larger scale features. The orbital motion of the black hole is imprinted onto its large jets, twisting them into a helical or corkscrew-like shape. So even though black holes may be so close together that our telescopes cant tell them apart, their twisted jets may provide easy-to find pointers to them, much like using a flare to mark your location at sea. This may provide a way for sensitive future telescopes like MeerKAT and the SKA to find binary black holes with much greater efficiency.
We have found the first needle in the middle age Universe and I hope that we will find much more and even closer systems of this kind in the near future, concludes Hans-Rainer Klöckner from the Max Planck Institute for Radio Astronomy, a co-author of the paper. Such close-binaries will not only show us how supermassive black holes could grow or how they could alternate our space time, they will also help us to understand the inner workings and the interplay between jets and the accretion disc surrounding black holes. This discovery is a prime example of how radio astronomy is done nowadays; it is an international and close collaboration accessing data products from various facilities distributed all over the globe.
The future will be bright with the SKA, the biggest radio telescope ever built, enabling such discoveries in international collaborations and hopefully Germany will find a way to support this endeavor also in future and enable its scientists and engineers to participate in the SKA project.
A close-pair binary in a distant triple supermassive black-hole system, by R. P. Deane, Z. Paragi, M. J. Jarvis, M. Coriat, G. Bernardi, R. P. Fender, S. Frey, I. Heywood, H.-R. Klöckner, K. Grainge & C. Rumsey, Nature Online, June 25, 2014.
http://dx.doi.org/10.1038/nature13454 (after the embargo expires).
Dr. Hans-Rainer Klöckner
Max-Planck-Institut für Radioastronomie, Bonn.
Fon: +49 228-525-31
Dr. Norbert Junkes,
Press and Public Outreach,
Max-Planck-Institut für Radioastronomie.
Dr. Roger Deane
University of Cape Town, South Africa
Fon: +27 78 582-2308
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