10亿光年外的某超重黑洞正在吞噬寒冷气体

At the center of a galaxy¹ cluster, 1 billion light years from Earth, a voracious², supermassive black hole is preparing for a chilly³ feast. For the first time, astronomers⁵ have detected billowy clouds of cold, clumpy gas streaming toward a black hole, at the center of a massive galaxy cluster. The clouds are traveling at speeds of up to 355 kilometers per second -- that's almost 800,000 miles per hour -- and may be only 150 light years away from its edge, almost certain to fall into the black hole, feeding its bottomless well. The observations, which will be published in the journal Nature, represent the first direct evidence to support the hypothesis that black holes feed on clouds of cold gas.

 

The results also suggest that fueling a black hole -- a process known as accretion⁶ -- is a whole lot messier than scientists had once thought. 

 

"The simple model of black hole accretion consists of a black hole surrounded by a sphere of hot gas, and that gas accretes⁷ smoothly⁸ onto the black hole, and everything's simple, mathematically," says Michael McDonald, assistant professor of physics in MIT's Kavli Institute for Astrophysics and Space Research. "But this is the most compelling evidence that this process is not smooth, simple, and clean, but actually quite chaotic⁹ and clumpy." 

 

Given the new observations, McDonald says black holes probably have two ways of feeding: For most of the time, they may slowly graze on a steady diet of diffuse¹⁰ hot gas. Once in a while, they may quickly gobble up clumps¹¹ of cold gas as it comes nearby. 

 

"This diffuse, hot gas is available to the black hole at a low level all the time, and you can have a steady trickle¹² of it going in," McDonald says. "Every now and then, you can have a rainstorm with all these droplets¹³ of cold gas, and for a short amount of time, the black hole's eating very quickly. So the idea that there are these two dinner modes for black holes is a pretty nice result."

 

McDonald is a co-author on the paper, which was led by Grant Tremblay, an astronomer⁴ at Yale University.

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