Black holes are thought to dominate their surroundings by their extremely powerful gravitational pull.
However, other forces which are usually considered to be weaker are also at work near these objects. These include forces exerted by the pressure of the in-falling hot gas and magnetic forces.
In a surprising twist, a team of astronomers at the Max Planck Institute for Radio Astronomy (MPIfR) and Lawrence Berkeley National Laboratory (LBNL) has found that in fact magnetic forces can be as strong as gravity near supermassive black holes. These findings are published in this week's issue of Nature.
Some black holes that are voraciously consuming interstellar gas also expel some of it in twin narrow outflows, or jets. This study focused on those supermassive black holes at the centers of galaxies that have observed radio-emitting jets.
"We realized that the radio emission from a black hole's jets can be used to measure the magnetic field strength near the black hole itself", says the study's lead-author, Mohammad Zamaninasab (formerly at the MPIfR and supported by a grant from Deutsche Forschungsgemeinschaft, DFG). "Our real aha experience came when we compared our magnetic force measurements to the force of gravity near black holes, and found them to be comparable”, he continues.
On a purely theoretical level, the possibility that magnetic fields may be as strong as gravity near black holes has been studied by state-of-the-art computer simulations. “When the in-falling gas carries enough magnetic field in our simulations, then the magnetic field near the black hole gets stronger until it balances gravity”, explains Alexander Tchekhovskoy (LBNL), a co-author of the study. “This fundamentally changes the behavior of the gas near the black hole.”
Surprisingly, the magnetic field strength around these exotic objects is comparable to the magnetic field produced in something more familiar: a magnetic resonance imaging (MRI) machine that you can find in your local hospital. Both supermassive black holes and MRI machines produce magnetic fields that are roughly 10 000 times stronger than the Earth's surface magnetic field, which is what guides an ordinary compass.
The measurements of the magnetic field strength near the black hole were based on mapping what fraction of the radio emission is absorbed at different locations near the base of the jet. “Such observations existed for an order of hundred sources from earlier work of several international re-search teams using the Very Long Baseline Array, a network of radio telescopes spread across the United States”, says co-author Tuomas Savolainen from MPIfR. “A large fraction of these measurements had just relatively recently become available thanks to a large observing program called MOJAVE, which monitors several hundred jets launched by supermassive black holes.”
The strength of the magnetic field near the black hole horizon also controls how powerful its jets are and, therefore, how luminous they appear at radio wavelengths according to current theories that treat black holes as a sort of spinning magnet. Thus, it is possible that the bright radio jets emanate from those black hole systems that have magnetic fields as strong as gravity.
These results may lead to changes in how to interpret black hole observations. “If our ideas hold up to further scrutiny, then astronomers' expectations for how to measure black hole properties would need to be changed.” concludes Eric Clausen-Brown, also from MPIfR. “Our study also changes how powerful we expect black hole jets can be, and since these jets can impact their own galaxies and beyond, we may need to rethink how much of an environmental impact black holes can have.”
Dynamically-important magnetic fields near accreting supermassive black holes, by M. Zamaninasab, E. Clausen-Brown, T. Savolainen, A. Tchekhovskoy, published in: 2014, Nature. DOI: 10.1038/nature13399
(after the embargo expires).
Dr. Mohammad Zamaninasab
Fon: +49(0)176 64972814
Dr. Eric Clausen-Brown
Max-Planck-Institut für Radioastronomie.
Dr. Tuomas Savolainen
Max-Planck-Institut für Radioastronomie
Dr. Norbert Junkes,
Press and Public Outreach,
Max-Planck-Institut für Radioastronomie.
Norbert Junkes | Max-Planck-Institut
Astronomers discover dizzying spin of the Milky Way galaxy's 'halo'
26.07.2016 | NASA/Goddard Space Flight Center
Lonely Atoms, Happily Reunited
26.07.2016 | Technische Universität Wien
Transparent electronics devices are present in today’s thin film displays, solar cells, and touchscreens. The future will bring flexible versions of such devices. Their production requires printable materials that are transparent and remain highly conductive even when deformed. Researchers at INM – Leibniz Institute for New Materials have combined a new self-assembling nano ink with an imprint process to create flexible conductive grids with a resolution below one micrometer.
To print the grids, an ink of gold nanowires is applied to a substrate. A structured stamp is pressed on the substrate and forces the ink into a pattern. “The...
A new Fraunhofer MEVIS method conveys medical interrelationships quickly and intuitively with innovative visualization technology
On the monitor, a brain spins slowly and can be examined from every angle. Suddenly, some sections start glowing, first on the side and then the entire back of...
Researchers at the U.S. Department of Energy's (DOE) Ames Laboratory have discovered an unusual property of purple bronze that may point to new ways to achieve high temperature superconductivity.
While studying purple bronze, a molybdenum oxide, researchers discovered an unconventional charge density wave on its surface.
Munich Physicists have developed a novel electron microscope that can visualize electromagnetic fields oscillating at frequencies of billions of cycles per second.
Temporally varying electromagnetic fields are the driving force behind the whole of electronics. Their polarities can change at mind-bogglingly fast rates, and...
Breakup of continents with two speed: Continents initially stretch very slowly along the future splitting zone, but then move apart very quickly before the onset of rupture. The final speed can be up to 20 times faster than in the first, slow extension phase.phases
Present-day continents were shaped hundreds of millions of years ago as the supercontinent Pangaea broke apart. Derived from Pangaea’s main fragments Gondwana...
15.07.2016 | Event News
15.07.2016 | Event News
11.07.2016 | Event News
26.07.2016 | Information Technology
26.07.2016 | Health and Medicine
26.07.2016 | Physics and Astronomy