Doeleman on how the Event Horizon Telescope team guarded against groupthink before releasing the first image of a black hole. Afterwards, they trained their algorithms on everything except rings, and the data kept coming back as a ring.
…a tie. And one of my postdocs is showing me the data for the first time. And there's a picture going, what am I looking at? And I came back to my office that night and I went through the calculations based on where these bounces were. And I realized it's exactly the size it's supposed to be.
Wow.
Right. So that was the first indication that we had something. And then we started imaging. So we had been perfecting these imaging algorithms on synthetic data. We'd fed these algorithms made-up data. So we would take a black hole image that we might be looking at, we'd corrupt it with noise, and we'd send it through these algorithms. We'd refine these to the point we were pretty confident in these algorithms. But before we set these loose on the data, we also realized that human error or human groupthink could be a really big problem. So we split our teams up into four groups. Each group had the data, but they could not talk to each other because we wanted to make sure that we all weren't in the same room thinking, like, I see a ring. Do You Take a ring? I see a ring. And it's not a ring, right? So we had four different geographically separated groups, and they all used different algorithms. And then we all came together to the building where I am sitting right now, the Black Hole? Initiative at Harvard, in July of 2018. And we were in the basement of this building, and the four teams put up their images, and they were all rings. That was a moment where there was a lot of crying and screaming. And then we all, and then we spent the next six…
Let's talk about the ring image again. You've alluded to why it looks this way. There's material splattered around the black hole that's orbiting outside of the event horizon, to be clear. But close, really close. You mentioned some observations of things in orbit around the black hole were…
Yeah, the way this works is that when you're so close to the black hole, the paths of light, which normally would travel in a straight line, is forced to travel along the curved space-time. And so it's really tracing the metric of space-time. It's tracing the gravitational well that it finds itself…
Yeah, there's nothing, there are no ingredients in there that aren't fundamental facts of nature except the mass of the black hole. And that's, I think people don't appreciate how black holes are fundamental in that way. All stars are kind of different, different colors, but black holes are…