Galaxy with strangely-spinning clouds could unlock a cosmic mystery
Astronomers have discovered a galaxy with some strange clouds orbiting the supermassive black hole in the center. Rather than all circling in the same direction as is usually expected, the galaxy NGC 1068 has two rings that orbit in opposite directions. This phenomenon might go a long way towards explaining another long-standing cosmic puzzle.
When water is sucked down a drain, the liquid swirls around in one direction. Black holes generally work the same way, pulling dust and gas and anything else that gets too close, into a spiral that usually moves in one direction.
But that’s not the case for the galaxy NGC 1068. Located about 47 million light-years from Earth, it’s hard to get a good look at the galaxy thanks to a large cloud of dust and gas in the center, obscuring its supermassive black hole. But now astronomers from the National Radio Astronomy Observatory (NRAO) have peered closer using the ALMA telescope, and found a strange circulation pattern at the heart of the galaxy.
“Thanks to the spectacular resolution of ALMA, we measured the movement of gas in the inner orbits around the black hole,” says Violette Impellizzeri, lead author of the study. “Surprisingly, we found two disks of gas rotating in opposite directions.”
The inner gas disk stretches between two and four light-years from the black hole, and is spinning in the same direction as the rotation of the galaxy itself. But a little further out – between four and 22 light-years from the black hole – is a second disk that’s spinning in the opposite direction. And the find surprised the astronomers.
“We did not expect to see this, because gas falling into a black hole would normally spin around it in only one direction,” says Impellizzeri. “Something must have disturbed the flow, because it is impossible for a part of the disk to start rotating backward all on its own.”
This kind of counter-rotation is not completely unheard of in galaxies, but it’s never been seen on this scale before. Normally, if it is spotted it’s happening to stars and other matter on the fringes of a galaxy, thousands of light-years from the center, which is moving in the opposite direction.
In those cases, the cause is usually a collision with another galaxy that was spinning in the opposite direction. The researchers believe something similar may be at play in NGC 1068 – the backwards rotation may be the remnants of a smaller captured galaxy, or gas clouds that fell out of the host galaxy.
Perhaps most interestingly, this two-faced galaxy could go a long way towards explaining a different mystery. Astronomers have spotted plenty of supermassive black holes at huge distances from Earth – meaning we’re seeing them as they appeared in the very early years of the universe. According to current models, it should take several billion years for black holes to grow to this mass, so a persistent puzzle has been how they get so big so quickly.
“Counter-rotating gas streams are unstable, which means that clouds fall into the black hole faster than they do in a disk with a single rotation direction,” says Impellizzeri. “This could be a way in which a black hole can grow rapidly.”
The research was published in the Astrophysical Journal.
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Yes, there is the implication of an annular orifice, but no certainty of the orientation; let alone the dynamics of the expelled material. Again, disregarding that conventional science tells us that once material is delivered into the "supermassive black hole" at the centre of such a galaxy, it cannot escape; where here we can see illustrated by the astronomers, "expelled material".
So, where/what has the material been expelled from? No answer given. . .
First of all the external event horizon of the Galactic Core Object at the centre of the galaxy must be a very substantial distance from the outer surface of the GCO, which in turn, must be another "supermassive black hole". So what we can observe must be mass and gas orbiting outside of the event horizon. Now again, with the other rotational dynamics, we may be observing the dynamics of the ejection of mass from an annular orifice; is it at all possible that the rotational dynamics are all relative to the internal structure of the "supermassive black hole" at the centre of the galaxy?