Primordial Planets
Science & Futurism with Isaac Arthur
Isaac Arthur
4.9 • 781 Ratings
🗓️ 3 March 2024
⏱️ 37 minutes
🧾️ Download transcript
Summary
Our world is ancient, but the Universe is far older. What were those first planets like, and how soon can life emerge on new ones?
Watch my exclusive video Crystal Aliens hhttps://nebula.tv/videos/isaacarthur-primordial-planets
Get Nebula using my link for 40% off an annual subscription: https://go.nebula.tv/isaacarthur
Visit our Website: http://www.isaacarthur.net
Join Nebula: https://go.nebula.tv/isaacarthur
Support us on Patreon: https://www.patreon.com/IsaacArthur
Support us on Subscribestar: https://www.subscribestar.com/isaac-arthur
Facebook Group: https://www.facebook.com/groups/1583992725237264/
Reddit: https://www.reddit.com/r/IsaacArthur/
Twitter: https://twitter.com/Isaac_A_Arthur on Twitter and RT our future content.
SFIA Discord Server: https://discord.gg/53GAShE
Credits:
Primordial Planets
Episode 436b; March 3, 2024
Produced, Written & Narrated by: Isaac Arthur
Editors: Konstantin Sokerin
Music Courtesy of:
Epidemic Sound http://epidemicsound.com/creator
Stellardrone, "Red Giant", "Ultra Deep Field", "Cosmic Sunrise"
Sergey Cheremisinov, "Labyrinth", "Forgotten Stars"
Lombus, "Cosmic Soup", "Hydrogen Sonata"
See Privacy Policy at https://art19.com/privacy and California Privacy Notice at https://art19.com/privacy#do-not-sell-my-info.
Transcript
Click on a timestamp to play from that location
| 0:00.0 | Hello, SFIA audio listeners. |
| 0:02.5 | In this month's Nebula exclusive, big alien theory, |
| 0:05.2 | we're asking 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, |
| 0:15.1 | check out go.nebler.tv slash Isaac Arthur and use my code, Isaac Arthur. |
| 0:20.7 | Our world is ancient, but the universe is far older. |
| 0:25.5 | What were those hot and dense, |
| 0:45.3 | they surpassed a supernova, and in under a minute, virtually every particle of hydrogen, |
| 0:50.8 | helium, deuterium, and lithium that now exists was formed. |
| 0:56.2 | Things grew less dense and cooler after that, and by 400,000 years after the Big Bang, |
| 1:01.5 | conditions since settled down to what the surface of a dim or star would be like. |
| 1:06.0 | It's ironic that folks think we have problems recreating fusion in the lab because we're |
| 1:10.3 | trying to replicate |
| 1:11.2 | the innards of stars, but we are not. Fusion of any given particle in the core of a typical |
| 1:16.7 | star is the sort of thing that happens less often than once in a billion years. People might |
| 1:22.2 | envision a house-sized fusion reactor replicating our sun's interior with 100 tons of stellar core matter inside |
| 1:28.9 | as some powerful joker not, but only be able to run a few light bulbs off the fusion |
| 1:33.5 | energy it was producing, albeit it would run them for billions of years. |
| 1:38.7 | No, to generate useful power from fusion, you need to replicate the conditions inside a dying |
| 1:43.9 | star, and those are the conditions that replicate the conditions inside a dying star, and those |
| 1:45.2 | are the conditions that forge the matter planets are made of, and those conditions lasted |
| 1:49.5 | only a few brief moments after the beginning of time. |
... |
Please login to see the full transcript.
Disclaimer: The podcast and artwork embedded on this page are from Isaac Arthur, and are the property of its owner and not affiliated with or endorsed by Tapesearch.
Generated transcripts are the property of Isaac Arthur and are distributed freely under the Fair Use doctrine. Transcripts generated by Tapesearch are not guaranteed to be accurate.
Copyright © Tapesearch 2026.

