Stephanie LaMassa did a double take. She was staring at two images on her computer screen, both of the same object — except they looked nothing alike.

The first image, captured in 2000 with the Sloan Digital Sky Survey, resembled a classic quasar: an extremely bright and distant object powered by a ravenous supermassive black hole in the center of a galaxy. It was blue, with broad peaks of light. But the second image, measured in 2010, was one-tenth its former brightness and did not exhibit those same peaks.

The quasar seemed to have vanished, leaving just another galaxy.

That had to be impossible, she thought. Although quasars turn off, transitioning into mere galaxies, the process should take 10,000 years or more. This quasar appeared to have shut down in less than 10 years — a cosmic eyeblink.

LaMassa, an astronomer now at the Space Telescope Science Institute, was mystified. Until that moment in 2014, she, like so many others, had expected quasars to be relatively stagnant. “Then you see these drastic changes within a human lifetime, and it’s pretty cool,” she said.

Confusion turned into excitement, and a hunt began to find more of these oddities. Although less luminous examples had already been seen, astronomers wanted to know if changes as dramatic as the one LaMassa discovered were common. It was no straightforward task, given that surveys tend not to go back and look at objects they have previously observed. But astronomers searched through archived data and discovered 50 to 100 more of what became known as “changing-look quasars.” Some of these have dimmed substantially more than LaMassa’s first example. Others have transitioned in the space of a month or two. And others, after disappearing, have reappeared again.

“It’s clear that the reason we weren’t finding these objects before is that we weren’t looking for them,” said Eric Morganson, an astronomer at the University of Illinois.

But how could such massive objects — superluminous beacons generated by solar-system-scale vortexes of gas and dust swirling into black holes with the mass of millions of suns — shut down so quickly? At first, astronomers refused to believe that they could, instead suggesting that these weren’t quasars at all, but rather supernovas and flaring stars masquerading as such. Or perhaps dust clouds were temporarily blocking our view.

But those ideas have largely failed to match what astronomers see. Within the past year a number of observations have peered more closely at these systems, providing details that suggest the accretion disk — that swirl of hot matter that encircles the black hole and gives these objects their dazzling luminosity — appears to flicker on and off. In parallel, theoretical astrophysicists have brainstormed how this change might happen. “It’s a little crazy that this whole system, which is just so enormous, is changing that quickly,” Morganson said.

Black Hole Doppelgängers

For the last four years, astronomers have attempted to understand changing-look quasars using the simplest theories possible. At first, that meant finding scenarios that did not require sweeping changes in the accretion disk.

To understand why, it helps to consider the size of these systems. If you could plop a quasar on top of the solar system, the supermassive black hole would swallow the sun, while the accretion disk would stretch out tens of thousands of times farther than Earth. To turn the quasar off, all of that material would have to swirl inward and fall onto the black hole — a process that calculations and even observations suggest should take tens to hundreds of thousands of years.