Supermassive Gone Rogue
The Supermassive Podcast
Izzie Clarke
4.6 • 556 Ratings
🗓️ 14 November 2025
⏱️ 22 minutes
🧾️ Download transcript
Summary
Can JWST detect exomoons? How can black holes keep absorbing more mass? How big is our cosmic neighbourhood? And what is a rogue black hole?! Izzie, Dr Becky and Robert answer YOUR questions.
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Transcript
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| 0:00.0 | Hello and welcome to another bonus episode of the Supermassive podcast from the Royal Astronomical Society. |
| 0:08.6 | With me, science journalist Izzy Clark, astrophysicist Dr. Becky Smethers and the Society's deputy |
| 0:13.8 | director, Dr. Robert Massey. We've had a lot of questions and I've always enjoyed them. |
| 0:19.8 | I feel like it's been a while since we've all been on this call. So Becky, Sean O'Rourke has a question about rogue black holes. So before we dive into that, can you actually explain what is a rogue black hole? Yeah, rogue basically means it's wandering interstellar or intergalactic space. So in between stars or in between |
| 0:39.2 | galaxies, it's not bound in orbit to anything else, whether that's another star that it might be |
| 0:44.7 | orbiting round or a star cluster or even the center of the galaxy. It is just freely roaming. And that |
| 0:51.5 | feels like we should do a whole episode on them. |
| 1:00.5 | Rogue anything is we should go Rogue one. Supermassive gone rogue. Rogue stars, rogue planets, |
| 1:04.0 | rogue black colors. We'll do all them all. Okay. Right. So on to Sean's question, |
| 1:09.6 | who says, hey gang, greetings from New Hampshire, USA. Thanks for the engaging content and continued success with the podcast. Well, thank you. |
| 1:12.3 | Very nice. Nice part of the world as well, especially at this time of year. |
| 1:14.4 | Yeah, definitely. He says, been reading more about rogue black holes. So Sean has sent in a few |
| 1:19.9 | questions here, Becky. First one. Is Beetlejuice large enough to produce a black hole when it goes |
| 1:25.0 | supernova? Or will its remnant be something of an other type of |
| 1:29.2 | byproduct? Unknown really. It's right on the boundary, Beetlejuice, of around about 15 times |
| 1:36.1 | heavier than the sun, which is kind of like the boundary of where things lighten that tend to |
| 1:41.0 | become neutron stars and things heavier than that tend to become black holes. |
| 1:44.9 | So it all sort of depends what happens when Beetlejuice goes supernova and what its exact matters |
| 1:49.7 | because we also, we can't measure it that precisely either to know exactly which side of the |
| 1:54.0 | boundary it will fall on. And it also depends how heavy its core is as well. And that's really |
| 1:58.5 | the crucial thing because if the supernova is very |
| 2:01.2 | energetic, so the actual part where the supernova is, it happens because there's no process in the |
... |
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