Post Stellar Civilizations - Life After The Last Star Fades (Narration Only)
Science & Futurism with Isaac Arthur
Isaac Arthur
4.9 • 781 Ratings
🗓️ 28 December 2025
⏱️ 40 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 add free, plus hours of bonus content, check out |
| 0:15.5 | go.nebola.tv slash Isaac Arthur and use my code, Isaac Arthur. |
| 0:21.5 | Many civilizations aspire to be eternal to outlive their rivers and mountains, and even the |
| 0:27.0 | stars themselves, but even they are thinking much too short term. |
| 0:33.5 | As we get ready to head in the new year and the future ahead of us, it doesn't hurt to reflect on what's come before, |
| 0:40.0 | and not much comes before the beginning of time. |
| 0:43.3 | It's strange to think, but back when the universe was hotter and denser, not long after the Big Bang, |
| 0:49.0 | more fusion took place in the first ten minutes than the next ten billion years. |
| 0:56.2 | All of our hydrogen and lithium, and most of our helium, dates from that period. Indeed, it will probably take the next |
| 1:00.7 | trillion years to surpass the amount of fusion that occurred in that window of time that's shorter |
| 1:05.9 | than this episode. Quite a lot of fusion occurred after that too, as the universe cooled down to something |
| 1:11.8 | more like normal stellar fusion rates, and eventually down to the temperatures we can see |
| 1:16.1 | at the surface of stars rather than their ultra-hot cores. |
| 1:20.8 | About the time that happened, things finally thinned and cooled enough to let atoms |
| 1:24.6 | with electrons form, and we stop seeing every single photon created |
| 1:28.9 | to get rapidly reabsorbed by its neighbors. Indeed, nowadays, most photons will never |
| 1:34.1 | get absorbed, and will meander off to the edge of eternity, so there will never will be a true |
| 1:39.4 | dark age in this universe, even when the last star burns out. It is that dark age we are going to discuss today, the one that comes after the stars go away, |
| 1:50.0 | and it is thousands of times further ahead in our future than the Big Bang is in our past, |
| 1:56.0 | but each epoch of our universe is longer than the last, with that brief ten-minute one where |
... |
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