Radio telescope reveals secrets of massive black hole
April 23, 2008
Artist's conception of region near supermassive black hole where twisted magnetic fields propel and shape jet of particles. Credit: Marscher et al., Wolfgang Steffen, Cosmovision, NRAO/AUI/NSF
At the cores of many galaxies, supermassive black holes expel powerful jets of particles at nearly the speed of light. Just how they perform this feat has long been one of the mysteries of astrophysics.
The leading theory says the particles are accelerated by tightly-twisted magnetic fields close to the black hole, but confirming that idea required an elusive close-up view of the jet's inner throat. Now, using the unrivaled resolution of the National Radio Astronomy Observatory's Very Long Baseline Array (VLBA), astronomers have watched material winding a corkscrew outward path and behaving exactly as predicted by the theory. The astronomers reported their findings in the April 24 issue of the journal Nature.
"We have gotten the clearest look yet at the innermost portion of the jet, where the particles actually are accelerated, and everything we see supports the idea that twisted, coiled magnetic fields are propelling the material outward," said Alan Marscher, of Boston University, leader of an international research team. "This is a major advance in our understanding of a remarkable process that occurs throughout the Universe," he added.
Marscher's team studied a galaxy called BL Lacertae (BL Lac), some 950 million light-years from Earth. BL Lac is a blazar, the most energetic type of black-hole-powered galactic core. A black hole is a concentration of mass so dense that not even light can escape its gravitational pull. Supermassive black holes in galaxies' cores power jets of particles and intense radiation in similar objects including quasars and Seyfert galaxies.
Material pulled inward toward the black hole forms a flattened, rotating disk, called an accretion disk. As the material moves from the outer edge of the disk inward, magnetic field lines perpendicular to the disk are twisted, forming a tightly-coiled bundle that, astronomers believe, propels and confines the ejected particles. Closer to the black hole, space itself, including the magnetic fields, is twisted by the strong gravitational pull and rotation of the black hole.
Theorists predicted that material moving outward in this close-in acceleration region would follow a corkscrew-shaped path inside the bundle of twisted magnetic fields. They also predicted that light and other radiation emitted by the moving material would brighten when its rotating path was aimed most directly toward Earth.
Marscher and his colleagues predicted there would also be a flare later when the material hits a stationary shock wave called the "core" some time after it has emerged from the acceleration region.
"That behavior is exactly what we saw," Marscher said, when his team followed an outburst from BL Lac. In late 2005 and early 2006, the astronomers watched BL Lac with an international collection of telescopes as a knot of material was ejected outward through the jet. As the material sped out from the neighborhood of the black hole, the VLBA could pinpoint its location, while other telescopes measured the properties of the radiation emitted from the knot.
Bright bursts of light, X-rays, and gamma rays came when the knot was precisely at locations where the theories said such bursts would be seen. In addition, the alignment of the radio and light waves -- a property called polarization -- rotated as the knot wound its corkscrew path inside the tight throat of twisted magnetic fields.
"We got an unprecedented view of the inner portion of one of these jets and gained information that's very important to understanding how these tremendous particle accelerators work," Marscher said.
Source: National Radio Astronomy Observatory
Nov 17, 2009 |
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Something just doesn't add up.
"Theorists predicted that material moving outward in this close-in acceleration region would follow a corkscrew-shaped path inside the bundle of twisted magnetic fields. They also predicted that light and other radiation emitted by the moving material would brighten when its rotating path was aimed most directly toward Earth."
What a load of baloney. What a non prediction.
How about predicting where the energy comes from.
How about predicting the Right Hand Rule when dealing with magnetic fields and electric currents.
That means if you have a jet shaped twisted magnetic field, there is a electrical current flowing in that jet.
Gravitational force, like the other forces can be overcome at certain energy levels. Maybe the incoming baryonic matter is accelerated to such an extent that as it collides with the core of the black hole you have huge amounts of energy released, enough to overcome the gravitational force. Maybe some smart cosmologist could even calculate this value someday.
And btw, I don't buy that the graviton doesn't have mass. It might be a fraction of the mass of other carriers, but it must have some mass, right?
I'm also inclined to think there's no "black hole" or central "body of mass" also... And it's just an empty "focal point" that the surrounding matter revolves around.
Take out the central super-masses out of the galaxy rotation equation and see what comes up... Wish I could.