Accretion disc

Weird Ancient Black Hole Has Extra Suck.

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Astronomers observing distant quasars have discovered something puzzling about a very rare class of these enigmatic objects — some appear to be sucking material inwards at relativistic speeds, whereas the vast majority of quasars do exactly the opposite.

Quasars dominated the early Cosmos, generating vast quantities of radiation that can be observed today right at the edge of our observable Universe. Consisting of an active supermassive black hole and a searing disk of plasma in the cores of young galaxies, the vast majority of quasars eject material from their energetic environments at high speed.

This may sound counter-intuitive; black holes consume matter after all, they don’t eject it. But in a quasar’s hot accretion disk — composed of a superheated soup of blended stars, gas and dust that strayed too close to the supermassive black hole’s gravitational wrath — the intense radiation blasts the surrounding material away from the black hole. Although some material inevitably gets fed from the accretion disk into the black hole, vast quantities are ejected at up to a significant fraction of the speed of light.

However, by taking a Doppler speed check of the motion of gas around known quasars, a team of researchers analyzing data from the Sloan Digital Sky Survey (SDSS-III) have discovered a very rare subset of quasars that don’t fit the norm.

“The gas in this new type of quasar is moving in two directions: some is moving toward Earth but most of it is moving at high velocities away from us, possibly toward the quasar’s black hole,” said Niel Brandt, study co-author and Distinguished Professor of Astronomy and Astrophysics at Penn State University. “Just as you can use the Doppler shift for sound to tell if an airplane is moving away from you or toward you, we used the Doppler shift for light to tell whether the gas in these quasars is moving away from Earth or toward these distant black holes, which have a mass from millions to billions of times that of the sun.”

“Matter falling into black holes may not sound surprising,” added team leader Patrick Hall of York University in Toronto, “but what we found is, in fact, quite mysterious and was not predicted by current theories.

“The gas in the disc must eventually fall into the black hole to power the quasar, but what is often seen instead is gas blown away from the black hole by the heat and light of the quasar, heading toward us at velocities up to 20 percent of the speed of light,” he said. “If the gas is falling into the black hole, then we don’t understand why it’s so rare to see infalling gas. There’s nothing else unusual about these quasars. If gas can be seen falling into them, why not in other quasars?”

So how rare are these objects? 1-in-10,000 rare. Of the tens of thousands of quasars known, only 17 such objects have been discovered so far.

For now, the researchers are baffled as to why these few distant supermassive black holes, which have masses millions to billions of times of the mass of our sun, appear to have more suck than the rest of their quasar cousins. Their work has been published in the journal Monthly Notices of the Royal Astronomical Society (doi: 10.1093/mnras/stt1012).

One explanation, says Hall, is that in actuality, the majority of gas is being ejected from the quasar, but it is moving in a peculiar fashion. Perhaps gas is rapidly orbiting around the black hole’s superheated accretion disk, sometimes traveling toward, sometimes away from us, but the Doppler measurements appear to show a bias toward the gas that is moving away. This may give the impression that the gas is being sucked into the black hole, when, in fact, it’s being ejected.

Regardless, these are strange objects that don’t appear to fit with current quasar theory, something astrophysicists will have to work on for a while yet.

Source: Physorg.com

How to Escape from a Black Hole.

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There are ways out of the gravitational death grip of a black hole — but it’s not easy

 

Black holes have a bit of an image problem. That’s to be expected from an immense remnant of a stellar explosion with billions of times the mass of the sun and a gravitational pull so powerful, not even light can escape. Anything that ventures too close gets swallowed whole, never to be seen again. Or so the popular thinking goes. But there’s a dramatic exception to that ironclad rule: all over the cosmos, galaxies with black holes at their center produce powerful energy jets, or blasts of superheated gas and dust that erupt from the very matter swirling down into the hole and travel outward for hundreds of thousands of light-years.

Astronomers have cataloged thousands of such energy jets over the decades, but what they’ve never been able to figure out is what powers them. How can material that effectively circles the galactic drain suddenly wrest itself free, and with such titanic force? Now, thanks to a study by an international team of astrophysicists that was published in the journal Science, there appears to be an answer — one that helps explain not only how the galactic pyrotechnics are produced but also how galaxies themselves grow and expand.

What astronomers — with a little help from Albert Einstein — already understand is that every black hole is surrounded by what’s called an event horizon, a threshold at which matter reaches a point of no return. It may be impossible to see the black hole itself, but with the right instruments you can detect the matter at the last moment before it disappears and, in effect, measure and mark the presence of the hole by the very absence it produces. Material at the event horizon forms a so-called accretion disk, a concentrated swirl of dust and gas that orbits the hole at nearly the speed of light, gradually feeding itself inward. It’s at that point that, well, something happens to produce the jets. But what?

To find out, a team led by Sheperd Doeleman, an astrophysicist at MIT’s Haystack Observatory, focused on a jet bursting from a black hole at the center of the M87 elliptical galaxy, 54 million light-years from the Milky Way. That jet, studied since the early 1900s and among the closest within viewing range, also happens to emanate from a black hole with a highly visible event horizon — mostly because M87 ranks among the sky’s brightest deep-space objects, meaning there are plenty of light emissions reflecting off the debris in the accretion disk.

That doesn’t mean the disk can be studied with any detail, however. Black holes are very small objects on a cosmic scale, and 58 million light-years is still 58 million light-years. To sharpen their resolution, Doeleman and his team thus used a method known as Very Long Baseline Interferometry (VLBI), in which multiple radio telescope dishes collect wave emissions from different perspectives and later align them into measurement data, much as the mirror and lens on a standard telescope aligns light waves into an image. “It’s a specialized thoroughbred technique which gives us the highest amount of detail of anything available to astronomers,” says Doeleman. For their study, they used data from radio dishes in Arizona, California and Hawaii, combining them in such a way that the observatories acted as a single, massive instrument with a resolution 2,000 times that of the Hubble Space Telescope. That revealed a lot.

M87′s event horizon, the researchers learned, is about the size of our solar system. The matter that produces the jets appears to come from an orbital position near the innermost edge of the accretion disk, about 5.5 times as distant as the horizon itself. That seems remote, but according to Einstein’s gravitational theories, it’s the last possible point at which matter can move in a stable orbit, because space time is distorted near a black hole. It’s also the birthing ground for the jets, possibly because magnetic fields embedded in the material that’s circling near the hole become twisted, carrying energy away in the form of an electromagnetic blast that is filled with charged particles — the very charged particles that emit the radio waves the scientists collected from Earth for their study.

The M87 jet’s tight orbit fits only one theoretical model of black-hole dynamics, one that suggests that gravity from the swirling accretion disk can rotate a black hole over time, causing both to spin in the same direction and drawing the innermost orbit into the range where the astronomers found the M87 jet. That supports years of conjecture that black holes are anything but motionless. Says Doeleman: “The black hole has to be spinning to explain those measurements.”

Although the study centers on a single jet, the ramifications extend across the galaxy, since the energy blasts broadly distribute matter and energy, feeding and disrupting star formation. Astronomers therefore hope their next look at the jets’ launch pad will be even more detailed. They plan on expanding their telescope array to include radio dishes worldwide, increasing the sensitivity of their virtual telescope by a factor of 10 and possibly leading to images rather than just measurements. As good as the high-speed energy jets are at escaping black holes, avoiding astronomers’ prying eyes will — with luck — prove much more difficult.

Source: http://science.time.com/