Post Stellar Civilizations - Life After The Last Star Fades
Science & Futurism with Isaac Arthur
Isaac Arthur
4.9 • 782 Ratings
🗓️ 28 December 2025
⏱️ 41 minutes
🧾️ Download transcript
Summary
Stars won’t last forever, but civilizations might. Join us as we journey into the post-stellar future, where Dyson remnants, black holes, and exotic physics could sustain life long after the galaxies fade.
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Credits:
Post-Stellar Civilizations [Extended Edition]
Episode 475a; December 1, 2024
Produced, Narrated & Written: Isaac Arthur
Editor: Jonathan Maltz
Graphics: Jeremy Jozwik, Ken York YD Visual, Steve Bowers, Udo Schroeter
Select imagery/video supplied by Getty Images
Music Courtesy of Epidemic Sound http://epidemicsound.com/creator
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Transcript
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| 0:00.0 | Hello, SFIA audio listeners. In this month's Nebula exclusive, big alien theory, |
| 0:05.2 | we're asked at the reason alien civilizations might be rare is because most aliens are huge. |
| 0:10.5 | To hear it and every episode early and ad-free, plus hours of bonus content, check out |
| 0:15.5 | go.nebola.tv slash Isaac Arthur and use my code, Isaac Arthur. |
| 0:21.1 | Many civilizations aspire to be eternal to outlive their rivers and mountains, and even the stars themselves, |
| 0:28.6 | but even they are thinking much too short term. |
| 0:35.8 | As we get ready to head in the new year and the future ahead of us, it doesn't hurt |
| 0:40.4 | to reflect on what's come before, and not much comes before the beginning of time. |
| 0:45.3 | It's strange to think, but back when the universe was hotter and denser, not long after |
| 0:49.7 | the Big Bang, more fusion took place in the first 10 minutes than in the next 10 billion years. |
| 0:56.7 | All of our hydrogen and lithium and most of our helium dates from that period. |
| 1:01.2 | Indeed, it'll probably take the next 10 trillion years to surpass the amount of fusion that |
| 1:05.7 | occurred in that window of time that's shorter than this episode. |
| 1:10.7 | Quite a lot of fusion occurred after that too, as the universe cooled down to something |
| 1:14.5 | more like normal stellar fusion rates and eventually down to the temperature as we can see |
| 1:18.8 | at the surface of stars rather than their ultra-hot cores. |
| 1:23.2 | About the time that happened, things finally thinned and cooled enough to let atoms |
| 1:27.3 | with electrons form, and we stopped seeing every single photon created About the time that happened, things finally thinned and cooled enough to let atoms with |
| 1:27.5 | electrons form, and we stopped seeing every single photon created to get rapidly reabsorbed |
| 1:33.0 | by its neighbors. Indeed nowadays, most photons will never get absorbed, and will meander |
| 1:38.5 | off to the edge of eternity, so there will never will be a true dark age in this universe, |
| 1:44.1 | even when the last star burns out. |
... |
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