Podcast Summary: "Are You REALLY Made Of Stars?"
The Rest Is Science
Hosts: Professor Hannah Fry & Michael Stevens (Vsauce)
Date: December 16, 2025
Overview: Main Theme & Purpose
This episode tackles the oft-quoted phrase, "We are made of stars," scrutinizing its accuracy through the lens of physics, chemistry, and cosmic events. Hosts Hannah Fry and Michael Stevens unpack what humans are truly made of—from the origins of our atoms to the surprising influence of cosmic rays—challenging the popular science narrative and exploring how star matter and cosmic events literally and figuratively permeate our existence.
Key Discussion Points & Insights
1. Are We Made of Stars or Made by Stars? (02:34–08:20)
-
Introduction to the Question
- Hannah asks, "What are we made of?" and Michael immediately references stars, but with skepticism toward the romanticized phrase.
- Michael objects to the simplistic idea, explaining, "We're made of matter...that matter wasn't created by our mothers in the womb ex nihilo. It was already there, and it was rearranged into us. And before we were here, it was something else." (03:08)
-
Breakdown of Element Origins
- Hydrogen: Most of our body’s hydrogen wasn’t made in stars but in the very early universe before stars existed. (05:03)
- Boron and Beryllium: These elements in our bodies aren't formed in stars but come instead from cosmic ray spallation—high-energy space particles smashing into atoms. (06:06)
- "My knockdown point is boron and beryllium...they are made by cosmic ray spallation." —Michael (05:42)
-
Semantics & Pedantry
- A playful debate: are we made "of" stars or "by" stars? Michael insists, "We're made by stars of stuff," emphasizing the role of cosmic rays.
-
Trace Elements
- Beryllium and boron exist in minuscule amounts in the human body, leading Hannah to joke about Michael’s ‘pedantry’. (07:13–08:17)
2. Cosmic Rays: What Are They? (08:33–13:25)
-
Violent Universe
- Hannah summarises space as “extremely violent”, with cosmic rays being a product of explosions and collisions across galaxies.
-
Nature of Cosmic Rays
- Not actual “rays”, but particle bullets (protons, helium nuclei) flooding the universe—about 10,000 hit every square meter per second at sea level. (09:40–10:28)
- Michael: "These things are not just like rare, they are flooding the universe." (10:11)
- Not actual “rays”, but particle bullets (protons, helium nuclei) flooding the universe—about 10,000 hit every square meter per second at sea level. (09:40–10:28)
-
Earth’s Protection
- Our atmosphere and magnetic field shield us from most, but not all, cosmic rays.
-
Cosmic Ray Interactions
- When cosmic rays hit atmospheric particles, they create a cascade of subatomic shrapnel, notably muons, which should decay before reaching the ground but survive due to relativistic time dilation, confirming Einstein's theories. (12:00–13:08)
- "These particles were decaying exactly when they should. It's just that time was running so slowly for them compared to our time, that their brief lives allowed them to travel all the way to Earth's surface." —Michael (12:02)
- When cosmic rays hit atmospheric particles, they create a cascade of subatomic shrapnel, notably muons, which should decay before reaching the ground but survive due to relativistic time dilation, confirming Einstein's theories. (12:00–13:08)
3. Detecting Cosmic Rays & Childhood Anecdotes (13:25–15:44)
-
Detection Methods
- Cloud chambers and bubble chambers reveal cosmic particles as visible trails.
- Michael shares a childhood story about ordering a radioactive needle for his chamber—despite his mother’s strictness!
-
DIY Science
- Hannah and Michael describe the process of building a cloud chamber and explain its function in visualizing incoming particles.
4. Impact of Cosmic Rays on Technology & Life (15:44–24:20)
-
Energy Spectrum
- Cosmic ray particles range from "slow" (10–80% light speed) to ultra-high energy, like the legendary “Oh-My-God Particle”, traveling at more than 99.999...% of light speed. (17:27–18:48)
- “At the speed it was traveling, if it entered a race with a beam of light after a quarter million years, the light would only be 1cm ahead of it.” —Michael (18:14)
- Cosmic ray particles range from "slow" (10–80% light speed) to ultra-high energy, like the legendary “Oh-My-God Particle”, traveling at more than 99.999...% of light speed. (17:27–18:48)
-
Mystery Particles
- Introduction of the "Amaterasu Particle," detected from a nearby cosmic void—evidence that space itself may produce these particles. (20:08)
-
Cosmic Rays & Technology Anomalies
- Cosmic rays can flip bits in computer memory, causing malfunctions:
- Pacemaker Incident: Mary Mo’s pacemaker entered backup mode mid-flight, likely because a cosmic ray altered its computer memory. (21:07–22:44)
- Qantas Flight: In 2008, a plane twice nose-dived after its computer received erroneous data, likely from a bit flip due to a cosmic ray. (22:58–24:20)
- Cosmic rays can flip bits in computer memory, causing malfunctions:
5. Historical Experiments—Proof of Cosmic Rays (27:20–29:32)
- Victor Hess’ Experiment (1912)
- Ascended in a hydrogen balloon during a solar eclipse to test whether radiation came from the sun.
- Discovered radiation increased with altitude and was unaffected by the eclipse, proving an extra-solar cosmic origin.
6. Cosmic Rays and Video Games—Mario’s Once-in-a-Lifetime Glitch (29:38–32:18)
- Speedrunning and the Super Mario 64 Anomaly
- In 2013, speedrunner "Dotateabag" achieved a teleport in-game never replicated since. Investigation revealed the leap was due to a cosmic ray flipping a single bit in the hardware. (31:05–32:12)
- “The only explanation is that a cosmic ray, or some spallation from a cosmic ray collision in the atmosphere, hit his machine, flipped a bit...Once in a lifetime. Once in a species existence phenomenon happened.” —Michael (32:12)
- In 2013, speedrunner "Dotateabag" achieved a teleport in-game never replicated since. Investigation revealed the leap was due to a cosmic ray flipping a single bit in the hardware. (31:05–32:12)
7. Cosmic Rays’ Role in Human Evolution and Death (32:36–35:17)
-
Potential Effects on Evolution
- Because they're ionizing, cosmic rays can cause random DNA mutations—possibly contributing to evolution.
-
Carbon Dating and the Death Connection
- Cosmic rays convert atmospheric nitrogen to radioactive carbon-14, which enters living organisms.
- After death, new carbon-14 is no longer absorbed; scientists can calculate time since death by measuring its remaining amount. (33:21–35:17)
- "When you die, you stop communing with the universe. You stop taking in new carbon 14. And the carbon 14 that's in you continues to decay." —Michael (34:36)
8. Wrapping Up: What Are We Really Made Of? (35:38–36:12)
- From Stardust to "Star Puke"
- The hosts agree the best answer is we are made by cosmic rays and star "puke"—star debris released by cosmic violence. (36:04)
- Hannah: “So can we say we're star puke?” (36:04)
- Michael: "We can and should." (36:06)
- The hosts agree the best answer is we are made by cosmic rays and star "puke"—star debris released by cosmic violence. (36:04)
Notable Quotes & Memorable Moments
-
On the Romanticism of Star Origins
"I'm not a big fan of that phrase. It gets spoken a lot. But today, I want us to really answer the question. What are we made of?" —Michael (02:42) -
Cosmic Abundance
"Every square meter at sea level gets 10,000 of these space bullets every second." —Hannah (10:28) -
Einstein's Relativity in Action
"These particles were decaying exactly when they should. It’s just that time was running so slowly for them." —Michael (12:02) -
Cosmic Rays in Everyday Life
"A charged particle...can interfere with these bits and flip them...That might have been enough to cause the pacemaker to go problem." —Michael (22:09) -
Mario’s Glitch: Once-in-a-Species Event
"Once in a lifetime. Once in a species existence phenomenon happened." —Michael (32:18) -
On What We’re Made Of
"We can and should [say we're star puke]." —Michael (36:06)
Timestamps for Important Segments
- What Are We Made Of? – 02:34
- Hydrogen’s Origin – 05:03
- Boron and Beryllium: Not Star-Made – 06:06
- Cosmic Rays: The Universe’s Bullets – 08:40–10:28
- Muons Confirm Relativity – 12:00
- Detecting Cosmic Rays: Cloud Chambers – 13:25
- Ultra-High Energy Particles: "Oh-My-God Particle" – 17:27
- Cosmic Rays Disrupt Tech – 21:07 (Pacemaker), 22:58 (Qantas Flight)
- Victor Hess Proves Cosmic Rays – 27:20
- Cosmic Rays & Gaming: Super Mario Bit Flip – 31:05
- Cosmic Rays and Evolution – 32:36
- Carbon Dating Explained – 33:21
- Concluding: Star Puke – 36:04
Final Thoughts
This episode masterfully deconstructs a catchy popular science claim, blending hard science with lively banter and real-world examples—from cosmic origins to death, gaming mishaps, and evolution. Michael's playful literalism and Hannah's curiosity make the show both accessible and precise. The final consensus: we are “star puke”—an ever-shifting residue of cosmic processes, and reality is stranger (and more wonderfully messy) than any inspirational quote suggests.
