Everything Everywhere Daily: History, Science, Geography & More - Cosmic Rays

Episode Date: September 16, 2021

Who matter where you are right now, no matter what time you are listening to this, there is one thing that I can safely say about you right now. Your body is being bombarded with cosmic rays. In fac...t, pretty much every moment of your life since you’ve been born, you’ve been hit by cosmic rays. Learn more about cosmic rays, what they are and where they come from, on this episode of Everything Everywhere Daily. Learn more about your ad choices. Visit megaphone.fm/adchoices

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Starting point is 00:00:00 No matter where you are right now, no matter what time you're listening to this, there is one thing I can safely say about you right now. Your body is being bombarded with cosmic rays. In fact, pretty much every moment of your life since you've been born, you've been hit with cosmic rays. Learn more about cosmic rays, what they are and where they come from, on this episode of Everything Everywhere Daily. Do you ever climb into bed ready to sleep,
Starting point is 00:00:34 only to have your mind start racing the moment your head hits the pillow? Thoughts bouncing around, replaying the day, or jumping ahead to tomorrow? That is exactly why Catherine Nikolai created Nothing Much Happens. Each episode is a gentle, cozy bedtime story where, well, nothing much happens. No drama, no tension, nothing you need to follow closely. Just soft narration, calming repetition, and soothing sensory details designed to help your mind slow down and your body relax. It's not about entertainment, it's about rest. And millions of listeners around the world use it every night to quiet their thoughts and finally fall asleep.
Starting point is 00:01:08 If you've ever struggled to shut your brain off at night, this might be exactly what you've been missing. You can listen to Nothing Much Happens wherever you get your podcasts. Episodes are every Monday and Thursday. This episode is sponsored by CuriosityStream. I've talked many times before about CuriosityStream, but if you still haven't gotten a subscription, you really need to consider doing it. CuriosityStream has thousands of educational and documentary programs covering a wide range of subjects. I personally watch Curiosity Stream several times a week, and I've used their programs to get ideas for this podcast, as well as doing show research. You can get an entire year of CuriosityStream for less than $20.
Starting point is 00:01:49 It's so cheap that you almost can't afford to not get it. If you're even remotely curious about the world you live in, and let's face it, you are because you listen to this podcast, go to everything-everywhere.com slash curiosity stream to start your subscription. Once again, that's everything-everywhere.com slash curiosity stream. The discovery of cosmic rays coincided with the discovery of radiation. Radiation was first discovered in 1896 by French physicist Henri Baccaro when he famously put photographic plates in a drawer with uranium. Subsequent experiments done by the likes of Marie Curie and others showed that radiation was a property that came from certain substances.
Starting point is 00:02:32 Rocks with radioactive elements were thought to be where radiation came from. In 1909, German physicist and Jesuit priest, Theodore Wolfe, created an electromagnet which was sealed in an airtight container. An electrometer is a simple device with two gold foil leaves. In the presence of ionizing radiation, the gold leaves would separate, and the further they would separate, the more radiation would be present. He took his electromagnet to the top of the Eiffel Tower, and, surprisingly, found out there was more radiation at the top than there was at the bottom.
Starting point is 00:03:02 Based on the current theory of radiation at the time, this observation made absolutely no sense. If radiation came from rocks, then there should be less radiation the further you got away from the ground, not more. Most of the physics community dismissed Wolf's findings. However, one Austrian physicist named Victor Hess wanted to verify Wolf's finding himself. He made three more advanced electrometers and took them with him in a hot air balloon. He went up to 5,300 meters or 17,000 feet and found that the radiation was four times higher than it was on the ground. At first he thought that it must have been something coming from the sun, so he did another balloon flight at night and another during a solar eclipse and found the exact same thing. He concluded that high-powered radiation was entering our atmosphere from space. Hess was awarded the Nobel Prize in Physics in 1936 for his discoveries.
Starting point is 00:03:55 The term cosmic ray was coined by American physicist Robert Milliken, who ran tests to measure the amount of ionization at very high elevations, with automated electromagners and balloons, as well as testing it far below sea level. The term cosmic ray is actually a misnomer, as I'll explain in a bit, as the term ray implied light. At first, it was thought that cosmic rays were high-energy photons like gamma rays. More discoveries were soon made about this mysterious radiation from the heavens. In 1927, it was found that cosmic radiation was lower at lower latitudes and higher at higher latitudes. This indicated that it wasn't photons at all, but rather charged particles that were being deflected by the Earth's magnetic field. In 1929, it was found that cosmic rays could penetrate 4.1 centimeters of gold.
Starting point is 00:04:44 Gold is very dense and good at blocking most radiation. If something could get through that much gold, it had to have a lot of energy behind it. In 1930, an Italian physicist named Bruno Rossi predicted that if the particles were charged, then we should see a difference in the intensity of cosmic rays based on the direction they came from. Sure enough, it was found that cosmic rays coming from the west were stronger than those coming from the east, again, due to the polarity of the Earth's magnetic field. So, if the cosmic rays aren't photons as originally thought, then what are they? What we know is that 99% of cosmic rays are atomic nuclei.
Starting point is 00:05:24 90% are protons, which are nuclei from hydrogen atoms, and 9% are the nuclei of helium atoms. If you remember back to my episode on Radiation 101, helium nuclei are known as alpha radiation. The remaining 1% are electrons, which is also known as beta radiation, as well as the small number of antimatter particles that hit the atmosphere, as well as the nuclei of heavier elements. The other thing we know is that they have a lot of energy. The highest energies ever observed in a cosmic ray particle have been 3.2 times 10 to the 20 electron volts. An electron volt is a unit of energy used for subatomic particles, so it isn't something that you can relate to in everyday life. So to put that into perspective, the most powerful cosmic rays are 40 times more powerful than the particles in the large Hadron Collider in Switzerland. or to put it into an even better real-world example,
Starting point is 00:06:20 a single subatomic particle can have the same energy as a baseball being thrown at 56 miles per hour. You might be wondering why you never feel like you're getting hit by a 56-mile-per-hour baseball all the time. First, most particles don't make it to the surface of the earth. They will hit air molecules in the atmosphere and start a cascade of other particles which rain down on the surface. Second, if one did hit you, you really wouldn't notice because it would just go right through you. In fact, there's a good chance that some cosmic particles went through your body since this episode started. And I'm not even talking about neutrinos, which is a whole other episode, and trillions of them have passed through you in that same amount of time. You might now be wondering, is this dangerous?
Starting point is 00:07:03 Well, as I mentioned in my previous episode on radiation, this is radiation. cosmic rays are probably the single biggest source of radiation that most people experience in their lifetime. If you live at a higher altitude, let's say Denver or Keto Ecuador, you'll have more radiation exposure than someone who lives at sea level. Likewise, flying in airplanes will increase your radiation exposure due to cosmic rays. Your level of exposure will primarily depend on how much you fly and at what altitude you fly. For the most part, cosmic rays pose no real health threat. All life forms throughout the history of life have been exposed to cosmic rays, and we evolve for our DNA to repair low-level radiation damage. One thing that can be damaged by cosmic rays is computers.
Starting point is 00:07:49 If a particle hits the right part of a processor or a memory chip, it can flip a bit causing an error. In 2003, there was an election in Belgium that was conducted electronically. The results were more than the number of votes cast. In an audit, checking the paper ballots also cast, found that the error perfectly, corresponded to a single bit in a single computer, which could only have been caused by a stray cosmic ray particle. This is why computers on spacecraft have to have so much redundancy. The space shuttles had to have triple redundancy for exactly this reason. The issue of cosmic rays is also a huge consideration for long-term spaceflight. The only time humans have ever been outside of
Starting point is 00:08:29 Earth's magnetic field was during the Apollo missions, and that was only briefly. The issue of cosmic rays is a considerable one that needs to be considered for any mission to Mars. One proposal would be to surround a ship with water, which would stop most of the cosmic rays. The problem is that water is heavy, and either we would need to get it from the moon, or we would need to get it from Earth. There is one thing, one big thing I haven't yet mentioned. Where do cosmic rays come from? Sure, they come from space, but where in space exactly?
Starting point is 00:09:00 The truth is, no one really knows. You can't just detect the direction a particle is coming from because they're so easily influenced by magnetic or gravitational fields. Not just the gravity and magnetism of Earth, but also that of the sun, or even possibly the galactic center. The particles which are flying around space may come from other stars, the center of our galaxy, or even other galaxies. Once a particle is jettisoned, it can basically travel forever until it runs into something. The smallest change in its trajectory will render its origin. impossible to determine. There are actually many theories about where they come from, but it's very difficult to actually prove anything. Cosmic rays are all around us, all the time,
Starting point is 00:09:42 and always have been. There really isn't anything you can do about them, and so long as you remain on Earth, it also really isn't anything to worry about. However, if you're traveling in interplanetary space, it probably is something you might want to consider. The associate producers of Everything Everywhere Daily are Peter Bennett and Thor Thompson. If you'd like to support the show, join the list of patrons over at patreon.com. And also remember, if you leave a review or send me a question, you too can have it read on the show.

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