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Hubble Offers Peek at Material
Swirling Close to a Black Hole
RA 10h 16m 53.632s Dec +73° 24' 02.34"
130 million light-years
October 2017 - March 2018
3.6 by 3.0 arcmin
Image is 2.2 arcmin across (about 83,000 light-years)
NASA/ESA, STScI, A. Riess et al.
July 11, 2019
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Astronomers are always tickled when they find something they didn't expect to be there. Peering deep into the heart of the majestic spiral galaxy NGC 3147, researchers uncovered a swirling gas disk precariously close to a black hole weighing about 250 million times the mass of our Sun. The surprise is that they thought the black hole was so malnourished, it shouldn't have such a structure around it. It's basically a "Mini-Me" version of more powerful disks seen in very active galaxies.
What's especially intriguing is that the disk is so deeply embedded in the black hole's intense gravitational field, its light is being stretched and intensified by the black hole's powerful grasp. It's a unique, real-world demonstration of Einstein's laws of relativity, formulated a century ago.
Hubble clocked material whirling around the black hole as moving at more than 10% of the speed of light. And, the gas astronomers measured is so entrenched in the gravitational well that light is struggling to climb out, and therefore appears stretched to redder wavelengths.
As if black holes weren't mysterious enough, astronomers using NASA's Hubble Space Telescope have found an unexpected thin disk of material furiously whirling around a supermassive black hole at the heart of the magnificent spiral galaxy NGC 3147, located 130 million light-years away. It was discovered by William Herschel on April 3, 1785
The conundrum is that the disk shouldn't be there, based on current astronomical theories. However, the unexpected presence of a disk so close to a black hole offers a unique opportunity to test Albert Einstein's theories of relativity. General relativity describes gravity as the curvature of space and special relativity describes the relationship between time and space.
"We've never seen the effects of both general and special relativity in visible light with this much clarity," said Marco Chiaberge of the European Space Agency, and the Space Telescope Science Institute and Johns Hopkins University, both in Baltimore, Maryland, a member of the team that conducted the Hubble study.
"This is an intriguing peek at a disk very close to a black hole, so close that the velocities and the intensity of the gravitational pull are affecting how the photons of light look," added the study's first author, Stefano Bianchi of Università degli Studi Roma Tre, in Rome, Italy. "We cannot understand the data unless we include the theories of relativity."
Black holes in certain types of galaxies like NGC 3147 are malnourished because there is not enough gravitationally captured material to feed them regularly. So, the thin haze of infalling material puffs up like a donut rather than flattening out in a pancake-shaped disk. Therefore, it is very puzzling why there is a thin disk encircling a starving black hole in NGC 3147 that mimics much more powerful disks found in extremely active galaxies with engorged, monster black holes.
"We thought this was the best candidate to confirm that below certain luminosities, the accretion disk doesn't exist anymore," explained Ari Laor of the Technion-Israel Institute of Technology located in Haifa, Israel. "What we saw was something completely unexpected. We found gas in motion producing features we can explain only as being produced by material rotating in a thin disk very close to the black hole."
The astronomers initially selected this galaxy to validate accepted models about lower-luminosity active galaxies-those with black holes that are on a meager diet of material. Models predict that an accretion disk forms when ample amounts of gas are trapped by a black hole's strong gravitational pull. This infalling matter emits lots of light, producing a brilliant beacon called a quasar, in the case of the most well-fed black holes. Once less material is pulled into the disk, it begins to break down, becomes fainter, and changes structure.
"The type of disk we see is a scaled-down quasar that we did not expect to exist," Bianchi said. "It's the same type of disk we see in objects that are 1,000 or even 100,000 times more luminous. The predictions of current models for gas dynamics in very faint active galaxies clearly failed."
The disk is so deeply embedded in the black hole's intense gravitational field that the light from the gas disk is modified, according to Einstein's theories of relativity, giving astronomers a unique look at the dynamic processes close to a black hole.
clocked material whirling around the black hole as moving at more than
10% of the speed of light. At those extreme velocities, the gas appears
to brighten as it travels toward Earth on one side, and dims as it speeds
away from our planet on the other side (an effect called relativistic
beaming). Hubble's observations also show that the gas is so entrenched
in the gravitational well the light is struggling to climb out, and therefore
appears stretched to redder wavelengths. The black hole's mass is around
250 million Suns.