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Tech & Science A Cool, Gassy Ring Has Been Detected Around Our Galaxy's Gigantic Black Hole

03:40  06 june  2019
03:40  06 june  2019 Source:   gizmodo.com.au

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The immediate area surrounding the supermassive black hole is kind of intense. Called Sagittarius A*, this behemoth has a mass around 4 million times This donut-like ring extends from the black hole ’ s event horizon to a few tenths of a light-year away. Astronomers had previously detected a blazingly

Our galaxy , the Milky Way, is no exception; it boasts a supermassive black hole at its heart called Sagittarius A*, often shortened to Sgr A*. Supermassive “But the contribution of cool gas on a black hole has never been studied.” Murchikova and her colleagues suggest with their study that the cold

A Cool, Gassy Ring Has Been Detected Around Our Galaxy's Gigantic Black Hole© Image: NRAO/AUI/NSF; S. Dagnello Artist’s impression of the accretion disk surrounding the supermassive black hole at the center of the Milky Way galaxy. (Image: NRAO/AUI/NSF; S. Dagnello) Using the ALMA observatory, scientists have detected a previously undocumented band of cool gas wrapped around the black hole at the core of our galaxy.

The immediate area surrounding the supermassive black hole is kind of intense. Called Sagittarius A*, this behemoth has a mass around 4 million times that of our Sun. As befits a supermassive black hole of that size, it has managed, through its intense gravitational influence, to collect an assortment of cosmological wonders, including wayward stars, troves of interstellar dust, and various gases.

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The cool hydrogen ring is currently around one hundredth of a light-year away from the black hole ' s event horizon. Moreover, it boasts an amount of hydrogen the equivalent to one tenth ALMA image of the disk of cool hydrogen gas flowing around the supermassive black hole at the center of our galaxy .

A supermassive black hole named Sagittarius A-Star resides there, drawing material in with its Since the environment around a black hole is so chaotic, it takes a lot of work to understand everything This is important because this is our closest supermassive black hole . Even so, we still have no

A Cool, Gassy Ring Has Been Detected Around Our Galaxy's Gigantic Black Hole
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Much of the gas collected by Sagittarius A* orbits the black hole in an accretion disk. This doughnut-like ring extends from the black hole’s event horizon to a few tenths of a light-year away. Astronomers had previously detected a blazingly hot band of gas within this accretion disk, which—weirdly—didn’t show any signs of rotation around the black hole. New research published today in Nature now describes a disk of cool interstellar gas, along with evidence of movement within the accretion disk.

“We were the first to image this elusive disk and study its rotation,” Elena Murchikova, the lead author of the new paper and an astrophysicist at the Institute for Advanced Study in Princeton, said in a release from the National Radio Astronomy Observatory.

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At the center of our galaxy lies the supermassive black hole Sagittarius A*, often abbreviated Sgr A "But the contribution of cool gas on a black hole has never been studied." Now Murchikova and her colleagues suggest that they may have imaged the cool accretion disk around Sgr A* for the first time.

Using the ALMA observatory, scientists have detected a previously undocumented band of cool gas wrapped around the black hole at the core of our galaxy .

As noted, astronomers had previously captured evidence of the hot portion of the gaseous ring. And by hot, we’re not kidding. Its temperature is around 10 million degrees Celsius (18 million degrees Fahrenheit), which is two-thirds the temperature found at the core of the Sun. When gas gets this hot, it emits X-ray light that can be detected from Earth. Astronomers had also previously detected cooler gas near the black hole, but nowhere near the accretion disk.

To be clear, the “cooler gas” is just cool by comparison; it’s still around 10,000 degrees Celsius. The relationship, if any, between this cool gas and the hot gas within the nebulous disk is not known.

But as the new research shows, cooler gas also exists in close proximity to the supermassive black hole. Using the ALMA telescope in Chile’s Atacama desert, the astronomers detected the faint millimetre-wavelength signals emanating from a cool ring of gas. These signals—the result of radiation on hydrogen atoms—travelled 26,000 light-years to Earth with barely any degradation along the way. The result is the first-ever image of the cooler gas disk. Incredibly, it’s located one hundredth of a light-year away from Sagittarius A* and is roughly 20,000 times the diameter of the black hole.

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Scientists have spotted six galaxies that appear trapped in orbit around a supermassive black hole that astronomers are seeing as it was when the universe was less Supermassive black holes are also relatively common; they lurk at the hearts of most, if not all, galaxies , including our own Milky Way.

These intermediate-mass black holes black holes were believed to exist but none had ever actually been identified - until now. Recent research has shown supermassive black holes are essential to the creation of galaxies , stars - and even life itself. Each one is about half a per cent of the host galaxy ' s

A Cool, Gassy Ring Has Been Detected Around Our Galaxy's Gigantic Black Hole© Image: ALMA (ESO/NAOJ/NRAO), E.M. Murchikova; NRAO/AUI/NSF, S. Dagnello ALMA image of the cool gas within the accretion disk. Areas in blue are moving toward us, while the regions in blue are moving away—evidence that the accretion disk is spinning around the black hole, which is shown by the crosshair. (Image: ALMA (ESO/NAOJ/NRAO), E.M. Murchikova; NRAO/AUI/NSF, S. Dagnello)

The ALMA data also allowed Murchikova and her colleagues to track the location and motion of the gas within the accretion disk. Owing to the radio light doppler effect, which produces shifts of blue (moving away from us) and red (moving toward us), the astronomers were able to see that the gas was slowly rotating around the black hole. The amount of hydrogen within the cool area of the disk was estimated at around one-tenth the total mass of Jupiter.

Importantly, these observations provide new insights into how the supermassive black hole at the center of the Milky Way collects and devours surrounding matter. In the new study, the researchers estimate that Sagittarius A* gobbles up a relatively tiny amount of matter—less than half a per cent of the mass of the Moon per year.

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Our galaxy ' s supermassive black hole is not as active as those in most galaxies . Like many galaxies , our Milky Way harbours a supermassive black hole at its centre, one which researchers have The grains also emit polarised, far-infrared light, which scientists detected using the new

Supermassive black holes are incredibly dense areas in the centre of galaxies with masses that can be billions of times that of the sun. The light blue ring on the back of the torus is due to the fluorescence of iron atoms excited by X-rays from the hot gas disk. This is what the astronomers used

These new observations are exciting, but Murchikova said “we still have no good understanding of how” the accretion process actually works at Sagittarius A*. A deeper dive into the new ALMA data, plus observations by other observatories, will hopefully reveal more about the monster parked at the core of our galaxy.

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A Cool, Gassy Ring Has Been Detected Around Our Galaxy's Gigantic Black Hole
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