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See att dot com, slash Samsung or visit 36 00:01:53,400 --> 00:01:56,960 Speaker 2: an AT and T store for details. 37 00:02:06,520 --> 00:02:09,480 Speaker 5: Hey Daniel, would you risk your life for science? 38 00:02:10,040 --> 00:02:12,920 Speaker 1: It might depend on the science we're talking about. 39 00:02:13,400 --> 00:02:16,280 Speaker 5: Would you risk getting eaten if you got to meet adiens? 40 00:02:16,320 --> 00:02:16,840 Speaker 5: For example? 41 00:02:17,040 --> 00:02:18,600 Speaker 1: Tempting, but I'll pass. 42 00:02:18,720 --> 00:02:21,919 Speaker 5: How about would you risk spec getification if you got 43 00:02:21,919 --> 00:02:23,880 Speaker 5: to see the inside of a black hole. 44 00:02:24,200 --> 00:02:26,239 Speaker 1: You know, I might actually take that trip? 45 00:02:26,480 --> 00:02:29,720 Speaker 5: Or would you risk deadly radiation to understand the nature 46 00:02:29,800 --> 00:02:30,280 Speaker 5: of matter? 47 00:02:30,639 --> 00:02:32,679 Speaker 1: Actually, I've kind of already done that one. 48 00:02:32,720 --> 00:02:36,440 Speaker 5: Oh, really, does it a large hadron collider generate deadly radiation? 49 00:02:36,919 --> 00:02:39,079 Speaker 1: It does, But that's not how I've been exposed. 50 00:02:39,160 --> 00:02:41,160 Speaker 5: Oh how have you been exposed to radiation? 51 00:02:41,280 --> 00:02:44,440 Speaker 1: Well, flying the Switzerland and back like a thousand times, 52 00:02:44,560 --> 00:02:47,480 Speaker 1: you get a lot more radiation at high altitude. Really, yep, 53 00:02:47,600 --> 00:02:50,239 Speaker 1: every transatlantic trip is like a chest X ray. 54 00:02:50,480 --> 00:02:52,680 Speaker 5: I thought you said you've been been by a radioactive 55 00:02:52,760 --> 00:02:53,840 Speaker 5: Swiss spider. 56 00:02:54,840 --> 00:02:58,240 Speaker 1: And I gained that spider's proportional physics, smarts. 57 00:02:58,000 --> 00:03:17,560 Speaker 5: And chocolate making ability. I am Horhem, a cartoonist and 58 00:03:17,600 --> 00:03:19,160 Speaker 5: the creator of PhD comics. 59 00:03:19,240 --> 00:03:22,280 Speaker 1: Hi, I'm Daniel. I'm a particle physicist, and I like 60 00:03:22,320 --> 00:03:24,120 Speaker 1: to think of myself as radioactive. 61 00:03:24,639 --> 00:03:28,680 Speaker 5: Are you technically radioactive? Are most people radioactive at some level? 62 00:03:28,800 --> 00:03:30,080 Speaker 5: Like bananas are radioactive? 63 00:03:30,240 --> 00:03:32,880 Speaker 1: Yeah, so you're probably more radioactive than most people. But 64 00:03:33,080 --> 00:03:35,240 Speaker 1: I grew up in Los Alamos, New Mexico, where we 65 00:03:35,360 --> 00:03:39,120 Speaker 1: like to say we all glow in the dark. Really, uh, 66 00:03:41,000 --> 00:03:42,640 Speaker 1: I did grow up in Los Alamos, but we don't 67 00:03:42,640 --> 00:03:43,480 Speaker 1: actually like to say that. 68 00:03:43,920 --> 00:03:45,600 Speaker 5: Well, I do eat a lot of bananas, and I 69 00:03:45,640 --> 00:03:47,640 Speaker 5: do have a certain glow about me, I like to think, 70 00:03:48,040 --> 00:03:50,680 Speaker 5: but yeah, Welcome to our podcast. Daniel and Jorge explain 71 00:03:50,760 --> 00:03:53,520 Speaker 5: the university production of iHeartRadio. 72 00:03:52,920 --> 00:03:55,680 Speaker 1: In which we shine a radioactive glow into all the 73 00:03:55,720 --> 00:03:59,120 Speaker 1: mysteries of the universe, the big, crazy things that are 74 00:03:59,160 --> 00:04:02,360 Speaker 1: out there tearing universe apart, the powerful forces that are 75 00:04:02,360 --> 00:04:04,880 Speaker 1: holding it together, the things far from home, and the 76 00:04:04,960 --> 00:04:08,320 Speaker 1: things right here in our backyard. All the mysteries of 77 00:04:08,320 --> 00:04:10,520 Speaker 1: physics revealed and explained to you. 78 00:04:10,640 --> 00:04:13,720 Speaker 5: That's right, we radiate knowledge and give you an X 79 00:04:13,840 --> 00:04:16,960 Speaker 5: ray view of all of the amazing secrets that are 80 00:04:17,040 --> 00:04:19,800 Speaker 5: out there to discover in the universe, and all of 81 00:04:19,839 --> 00:04:21,440 Speaker 5: the secrets that are yet to be discovered. 82 00:04:21,480 --> 00:04:23,599 Speaker 1: And all the while you can stay home and safe, 83 00:04:23,920 --> 00:04:26,320 Speaker 1: tucked into your couch, sipping that mug of tea and 84 00:04:26,440 --> 00:04:27,760 Speaker 1: learning about the universe. 85 00:04:27,880 --> 00:04:31,480 Speaker 5: No tinfoil hat needed or leadline hats. 86 00:04:32,120 --> 00:04:34,680 Speaker 1: That's right. This counts exactly zero as part of your 87 00:04:34,680 --> 00:04:37,960 Speaker 1: annual dose of radiation, even though you'll be learning all 88 00:04:38,000 --> 00:04:38,400 Speaker 1: about it. 89 00:04:38,400 --> 00:04:41,960 Speaker 5: That's right. Well, we're technically getting to people through sound waves, 90 00:04:42,160 --> 00:04:44,200 Speaker 5: not lightweights or radiation. 91 00:04:43,960 --> 00:04:46,680 Speaker 1: That's right. But actually radiation is sort of any sort 92 00:04:46,720 --> 00:04:51,320 Speaker 1: of energetic particle or wave. So sound is technically speaking 93 00:04:51,600 --> 00:04:55,279 Speaker 1: a kind of radiation. So we are irradiating your ears 94 00:04:55,360 --> 00:04:56,159 Speaker 1: with our voices. 95 00:04:56,360 --> 00:04:59,719 Speaker 5: What no, you get to say a limit? Can't you like, 96 00:04:59,760 --> 00:05:02,080 Speaker 5: if I throw a baseball, I'm radiating a baseball. 97 00:05:02,520 --> 00:05:06,800 Speaker 1: Baseballs are radiation? Yes, absolutely, Now, the technical definition of 98 00:05:06,880 --> 00:05:10,360 Speaker 1: radiation is sort of weirdly broad. Any kind of light, 99 00:05:10,400 --> 00:05:12,800 Speaker 1: any kind of particle, any kind of way that transmits 100 00:05:12,920 --> 00:05:17,600 Speaker 1: energy is radiation. But practically speaking, when we talk about radiation, 101 00:05:17,720 --> 00:05:21,400 Speaker 1: we mean very high energy particles or higher energy waves 102 00:05:21,440 --> 00:05:24,120 Speaker 1: that are going to deposit a significant amount of energy. 103 00:05:24,440 --> 00:05:27,440 Speaker 1: And so a flashlight or this podcast are not typically 104 00:05:27,520 --> 00:05:31,760 Speaker 1: categorized as radiation, even though technically, according to physicists it is. 105 00:05:32,680 --> 00:05:35,240 Speaker 5: Well, it's a very loaded word, isn't it. I mean, 106 00:05:36,160 --> 00:05:38,400 Speaker 5: especially like in the eighties. I feel in the nineties, 107 00:05:38,720 --> 00:05:41,240 Speaker 5: you know, radiation was such a negative thing, and know 108 00:05:41,279 --> 00:05:43,839 Speaker 5: what they wanted, radiation and the thing that made you sick. 109 00:05:44,000 --> 00:05:47,360 Speaker 1: Yeah, exactly. Radiation can be pretty dangerous. They are basically 110 00:05:47,360 --> 00:05:50,560 Speaker 1: these little invisible bullets flying through the universe, and they 111 00:05:50,560 --> 00:05:52,840 Speaker 1: can do real damage. They can fly through your cells, 112 00:05:52,839 --> 00:05:56,040 Speaker 1: they can bust up your DNA, they can cause you cancer. 113 00:05:56,480 --> 00:05:58,880 Speaker 1: And so radiation definitely is something to think about and 114 00:05:58,920 --> 00:06:02,320 Speaker 1: worry about. These things in the world that's not visible 115 00:06:02,360 --> 00:06:05,920 Speaker 1: to our naked eye yet turns out to be pretty important. 116 00:06:06,279 --> 00:06:07,919 Speaker 1: So it's a key that tells us that there's a 117 00:06:07,960 --> 00:06:10,960 Speaker 1: lot going on in the universe that we can't directly see. 118 00:06:11,040 --> 00:06:13,320 Speaker 5: Yeah, so a big question is how do we even 119 00:06:13,400 --> 00:06:17,600 Speaker 5: discover radiation or even come to believe it exists if 120 00:06:17,600 --> 00:06:20,080 Speaker 5: it is in fact the invisible. 121 00:06:19,720 --> 00:06:22,039 Speaker 1: Yeah, it's part of this story of peeling back the 122 00:06:22,160 --> 00:06:24,640 Speaker 1: nature of reality and figuring out that the universe has 123 00:06:24,720 --> 00:06:27,240 Speaker 1: a lot of stuff going on. But to me, it's 124 00:06:27,240 --> 00:06:29,960 Speaker 1: always fascinating to figure out how that came to be, 125 00:06:30,040 --> 00:06:33,480 Speaker 1: how that understanding sort of filtered into human minds, because 126 00:06:33,680 --> 00:06:36,440 Speaker 1: here we are standing on the shoulders of giants, understanding 127 00:06:36,480 --> 00:06:39,080 Speaker 1: all these things about the way the world works. But 128 00:06:39,160 --> 00:06:42,320 Speaker 1: this required a real shift in people's understanding of the 129 00:06:42,440 --> 00:06:45,360 Speaker 1: nature of the universe. So I'm always super interested in 130 00:06:45,360 --> 00:06:48,120 Speaker 1: those moments, like what was it that convinced people? What 131 00:06:48,160 --> 00:06:51,440 Speaker 1: experiments did people do that revealed that, because I hope 132 00:06:51,440 --> 00:06:53,919 Speaker 1: that will help us understand what experiments in the future 133 00:06:54,279 --> 00:06:56,919 Speaker 1: might again change the way we think about the universe. 134 00:06:57,000 --> 00:07:01,960 Speaker 5: Yeah. So usually people assign the discovered to Madame Cirie 135 00:07:02,240 --> 00:07:05,880 Speaker 5: and her experiments, But there's actually more to the story. 136 00:07:05,640 --> 00:07:09,000 Speaker 1: Right there is she did not, in fact discover radiation. 137 00:07:09,360 --> 00:07:11,520 Speaker 1: She won a couple of Nobel prizes. She was quite 138 00:07:11,520 --> 00:07:13,880 Speaker 1: a genius. She discovered a lot of stuff, but you 139 00:07:13,960 --> 00:07:17,880 Speaker 1: can't give her credit for discovering radiation. It's a fascinating story. 140 00:07:17,920 --> 00:07:21,280 Speaker 5: Well you can't even define it. I mean, sure, then 141 00:07:21,360 --> 00:07:24,880 Speaker 5: nobody discovered her radiation or everyone discovered radiation. 142 00:07:24,640 --> 00:07:27,320 Speaker 1: That's right. The first little swimming organism that developed an eyeball, 143 00:07:27,360 --> 00:07:30,880 Speaker 1: I suppose discovered radiation when it used photons to guide 144 00:07:30,920 --> 00:07:33,160 Speaker 1: itself around the primordial soup on Earth. 145 00:07:33,160 --> 00:07:36,360 Speaker 5: I suppose, yeah, right, like the first organism to use 146 00:07:36,520 --> 00:07:37,960 Speaker 5: or detect light. 147 00:07:38,560 --> 00:07:41,559 Speaker 1: Right, that definitely predates humanity. But I think we should 148 00:07:41,560 --> 00:07:44,280 Speaker 1: focus on the kind of radiation we're talking about, which is, 149 00:07:44,560 --> 00:07:47,320 Speaker 1: you know, high energy particles or waves that come from 150 00:07:47,320 --> 00:07:50,520 Speaker 1: like radioactive decay, things that are different from the normal 151 00:07:50,600 --> 00:07:52,920 Speaker 1: kinds of radiation we used to live our lives. We're 152 00:07:52,920 --> 00:07:55,800 Speaker 1: talking about a change in how we've understood the universe. 153 00:07:56,120 --> 00:08:02,720 Speaker 5: Okay, so it's invisible, potentially dangerous, and obviously very scientifically significant. 154 00:08:03,080 --> 00:08:06,680 Speaker 5: But how was radiation discovered? That's a big question, and 155 00:08:06,720 --> 00:08:09,120 Speaker 5: that's the question we're exploring today. So to the end 156 00:08:09,120 --> 00:08:18,360 Speaker 5: of the program, we'll be talking about how was radiation discovered? So, 157 00:08:18,400 --> 00:08:20,640 Speaker 5: as usually, we were wondering how many people out there 158 00:08:20,760 --> 00:08:22,840 Speaker 5: knew how radiation was discovered? 159 00:08:22,880 --> 00:08:25,520 Speaker 1: So thank you to everybody who volunteered their answers to 160 00:08:25,560 --> 00:08:29,520 Speaker 1: these tricky physics questions without referring to any reference materials, 161 00:08:29,560 --> 00:08:32,800 Speaker 1: Google or bing or ask Jeeves. And if you would 162 00:08:32,800 --> 00:08:36,280 Speaker 1: like to participate in future Baseless Speculations for the podcast, 163 00:08:36,360 --> 00:08:39,280 Speaker 1: please write to us to questions at Daniel and Jorge 164 00:08:39,440 --> 00:08:40,000 Speaker 1: dot com. 165 00:08:40,040 --> 00:08:42,160 Speaker 5: Maybe that should be the name of that website, Daniel 166 00:08:42,200 --> 00:08:45,480 Speaker 5: Baseless Speculation dot com. You might get a lot of hits. 167 00:08:46,120 --> 00:08:48,840 Speaker 1: Yeah exactly. We just pointed to our book every single time. 168 00:08:48,880 --> 00:08:51,240 Speaker 1: We have no idea dot com is the answer to 169 00:08:51,280 --> 00:08:52,319 Speaker 1: all these questions. 170 00:08:52,679 --> 00:08:58,160 Speaker 5: Oh interesting, interesting marketing technique. Lure people in with a 171 00:08:58,240 --> 00:09:00,680 Speaker 5: juicy website and then sell them a book. 172 00:09:00,880 --> 00:09:03,040 Speaker 1: Yeah exactly. I think they call that clickbait. 173 00:09:03,160 --> 00:09:05,280 Speaker 5: So think about it for a second. If someone approached 174 00:09:05,280 --> 00:09:08,199 Speaker 5: you and asks you if you knew how radiation was discovered. 175 00:09:08,440 --> 00:09:10,800 Speaker 5: What would you say here? What people had to say? 176 00:09:11,160 --> 00:09:13,000 Speaker 5: I have no idea, but I think it has something 177 00:09:13,000 --> 00:09:15,400 Speaker 5: to do with Marie Currey playing around with some kind 178 00:09:15,400 --> 00:09:18,160 Speaker 5: of radioactive substance and like X raying her hand or 179 00:09:18,200 --> 00:09:18,920 Speaker 5: something like that. 180 00:09:19,040 --> 00:09:21,680 Speaker 6: Radiation was discovered by Madame Curie. 181 00:09:22,160 --> 00:09:25,760 Speaker 1: I just know that was discovered by Marie Currey. 182 00:09:26,120 --> 00:09:29,560 Speaker 7: I believe radiation was discovered by Marie Cury. I don't 183 00:09:29,600 --> 00:09:32,720 Speaker 7: know how she did it. She was probably experimenting with 184 00:09:34,280 --> 00:09:37,560 Speaker 7: what became known as radium and saw it glowing. 185 00:09:37,960 --> 00:09:42,160 Speaker 6: I think radiation was discovered in the eighteen hundreds when 186 00:09:42,240 --> 00:09:47,160 Speaker 6: some radioactive material uranium was glowing in the dark or 187 00:09:47,400 --> 00:09:48,400 Speaker 6: was unusually hot. 188 00:09:48,440 --> 00:09:51,080 Speaker 5: All right, it looks like Marie curriy and the Curris 189 00:09:51,120 --> 00:09:54,760 Speaker 5: have a pretty good policies because most people went to 190 00:09:54,880 --> 00:09:56,959 Speaker 5: them as the discoverers of radiation. 191 00:09:57,280 --> 00:10:00,679 Speaker 1: Yeah, she is definitely ensconced in popular colu cure as 192 00:10:00,720 --> 00:10:04,040 Speaker 1: somebody deeply associated with radiation. And you know, she actually 193 00:10:04,040 --> 00:10:06,640 Speaker 1: did have a good publicist late in her career. She 194 00:10:06,679 --> 00:10:09,400 Speaker 1: did a whole tour of the United States giving talks 195 00:10:09,400 --> 00:10:12,360 Speaker 1: all about radiation stuff. So she became quite famous and 196 00:10:12,440 --> 00:10:16,120 Speaker 1: associated with radiation. So that has lasted up till the 197 00:10:16,160 --> 00:10:18,000 Speaker 1: present day, almost one hundred years later. 198 00:10:18,160 --> 00:10:20,760 Speaker 5: Right, Well, we don't want to take away anything that 199 00:10:20,840 --> 00:10:24,319 Speaker 5: she did or the decrease did. It's really more about definition. 200 00:10:24,400 --> 00:10:26,760 Speaker 5: I think I think she discovered a particular type of 201 00:10:26,880 --> 00:10:31,199 Speaker 5: radiation or I guess we'll get into that. But generally speaking, 202 00:10:31,240 --> 00:10:34,600 Speaker 5: it kind of seems like radiation maybe is a broader 203 00:10:34,679 --> 00:10:36,520 Speaker 5: concept than most people assume it is. 204 00:10:36,640 --> 00:10:40,040 Speaker 1: There's definitely that, and she made important contributions and discovered 205 00:10:40,040 --> 00:10:43,400 Speaker 1: particular kinds of radioactive elopments. We'll dig into that. But 206 00:10:43,440 --> 00:10:46,040 Speaker 1: you're right, radiation is sort of a broader set of things. 207 00:10:46,280 --> 00:10:51,040 Speaker 1: Radiation is not just uranium decays and shoots out deadly particles. 208 00:10:51,240 --> 00:10:54,480 Speaker 1: There's a broader set of things. We consider radiation not 209 00:10:54,559 --> 00:10:58,280 Speaker 1: just ordinary light. But it starts, for example, with X rays. 210 00:10:58,520 --> 00:11:01,840 Speaker 1: Like X rays are just hot energy photons, but we 211 00:11:01,920 --> 00:11:03,080 Speaker 1: consider them radiation. 212 00:11:03,800 --> 00:11:06,800 Speaker 5: Yeah. I guess you were saying earlier that any light 213 00:11:07,000 --> 00:11:10,480 Speaker 5: is considered radiation. Even sound is considered radiation. Yeah, even 214 00:11:10,520 --> 00:11:12,160 Speaker 5: like heat, I guess heat is radiation. 215 00:11:12,280 --> 00:11:14,840 Speaker 1: Yeah, exactly, you radiate heat. You go run a lap 216 00:11:14,840 --> 00:11:17,040 Speaker 1: and you get really hot, you are radiating heat out 217 00:11:17,040 --> 00:11:20,000 Speaker 1: into the universe, and everything in the universe that has 218 00:11:20,040 --> 00:11:23,120 Speaker 1: a temperature gives off heat, and so everything in the 219 00:11:23,200 --> 00:11:27,120 Speaker 1: universe is radiating constantly. Radiation is everywhere. But that's sort 220 00:11:27,120 --> 00:11:29,640 Speaker 1: of again the sort of technical physical term for it. 221 00:11:29,880 --> 00:11:32,199 Speaker 1: When we talk about radiation, we think about sort of 222 00:11:32,280 --> 00:11:35,640 Speaker 1: damaging radiation, radiation that's long been invisible to us and 223 00:11:35,679 --> 00:11:38,600 Speaker 1: reveals something different about how the world works. And it 224 00:11:38,640 --> 00:11:41,160 Speaker 1: was really crucial in understanding things like the nature of 225 00:11:41,200 --> 00:11:43,480 Speaker 1: the atom and the deep structure of matter. 226 00:11:43,600 --> 00:11:45,960 Speaker 5: Right, Well, we knew about light for a long time. 227 00:11:46,200 --> 00:11:48,400 Speaker 5: I mean it's kind of in the Bible, Daniel, let 228 00:11:48,400 --> 00:11:50,880 Speaker 5: there be Light. It was like the first thing. 229 00:11:51,480 --> 00:11:54,360 Speaker 1: Is that a reference book? I wasn't familiar with that, Yeah, 230 00:11:54,400 --> 00:11:58,559 Speaker 1: got it all. I think there's some rata for that one. 231 00:11:58,559 --> 00:12:02,960 Speaker 5: It's probably the most impact factor of all publications in 232 00:12:03,000 --> 00:12:03,640 Speaker 5: the history of man. 233 00:12:03,800 --> 00:12:03,959 Speaker 7: Yeah. 234 00:12:04,000 --> 00:12:06,199 Speaker 1: I submitted something, but it got rejected by the referees. 235 00:12:06,880 --> 00:12:09,839 Speaker 5: So, I mean, of course we've known about light for 236 00:12:09,920 --> 00:12:12,720 Speaker 5: a long time. So I guess when do you draw 237 00:12:12,760 --> 00:12:16,320 Speaker 5: the line as us having discovered radiation, Like, is it 238 00:12:16,559 --> 00:12:18,960 Speaker 5: X rays? Is that the first kind of you know, 239 00:12:19,440 --> 00:12:22,600 Speaker 5: powerful kind of radiation invisible that we've discovered. 240 00:12:22,679 --> 00:12:24,880 Speaker 1: Yeah, I think the discovery of X rays really marked 241 00:12:24,880 --> 00:12:27,400 Speaker 1: the turning point. It's the time we discover that there 242 00:12:27,400 --> 00:12:31,080 Speaker 1: are ways to transmit energy or other kinds of light 243 00:12:31,520 --> 00:12:33,640 Speaker 1: that are different from the kind of visible light we 244 00:12:33,640 --> 00:12:36,360 Speaker 1: were familiar with. And this specifically was the kind of 245 00:12:36,400 --> 00:12:39,240 Speaker 1: light that we saw could sort of pass through walls 246 00:12:39,280 --> 00:12:42,040 Speaker 1: and pass through barriers, and so it really was doing 247 00:12:42,120 --> 00:12:44,600 Speaker 1: something different from the kind of visible light we were 248 00:12:44,600 --> 00:12:47,440 Speaker 1: familiar with. And that's exactly how it was discovered. 249 00:12:47,559 --> 00:12:49,600 Speaker 5: I see, like, if you shine a flashlight, it gets 250 00:12:49,640 --> 00:12:52,040 Speaker 5: blocked by the wall, but if you shine an X 251 00:12:52,160 --> 00:12:54,559 Speaker 5: ray tube at a wall, it will go right through. 252 00:12:54,720 --> 00:12:56,800 Speaker 1: It'll go through most of it. Yeah, exactly. And that's 253 00:12:56,840 --> 00:12:59,480 Speaker 1: why we call it, you know, X raying something because 254 00:12:59,600 --> 00:13:02,040 Speaker 1: X rays pass through the soft tissue of your body, 255 00:13:02,080 --> 00:13:04,760 Speaker 1: but not your bones, and so they reveal what's going 256 00:13:04,800 --> 00:13:08,280 Speaker 1: on inside. And so radiation is interesting because they can 257 00:13:08,360 --> 00:13:10,920 Speaker 1: do these things that visible like can't do, but also 258 00:13:10,960 --> 00:13:13,559 Speaker 1: because it has this power it penetrates and so what 259 00:13:13,640 --> 00:13:14,880 Speaker 1: reveals what's inside? 260 00:13:15,200 --> 00:13:17,280 Speaker 5: All right, So then how do we discover X rays? 261 00:13:17,320 --> 00:13:20,040 Speaker 1: So X ray's discovered in eighteen ninety five by this 262 00:13:20,080 --> 00:13:22,920 Speaker 1: guy Runken, and this guy was a character. I think 263 00:13:22,920 --> 00:13:25,360 Speaker 1: you'd like this. He actually was kicked out of high 264 00:13:25,400 --> 00:13:28,520 Speaker 1: school as a student because he drew a caricature of 265 00:13:28,559 --> 00:13:31,480 Speaker 1: one of his teachers, which is not very flattering, and 266 00:13:31,520 --> 00:13:34,240 Speaker 1: so he's sort of a physicist and a cartoonist. 267 00:13:34,400 --> 00:13:36,440 Speaker 5: Oh, I almost got exposed from high school for the 268 00:13:36,440 --> 00:13:40,200 Speaker 5: exact same reason, actually, except I didn't just caricature one teacher. 269 00:13:40,960 --> 00:13:41,920 Speaker 5: I did all of them. 270 00:13:42,120 --> 00:13:44,240 Speaker 1: Well, then maybe there's a Nobel prize in your future. 271 00:13:44,360 --> 00:13:45,440 Speaker 5: Yeah, stay tuned. 272 00:13:46,160 --> 00:13:48,360 Speaker 1: But he was doing experiments at the time with these 273 00:13:48,360 --> 00:13:51,480 Speaker 1: things called Crooks tubes. We've talked about these before because 274 00:13:51,480 --> 00:13:54,600 Speaker 1: they were how electrons were discovered. They're basically just these 275 00:13:54,640 --> 00:13:57,679 Speaker 1: glass tubes that are mostly have vacuum in them, and 276 00:13:57,760 --> 00:14:00,000 Speaker 1: then you have an anode and a cathode with voltage 277 00:14:00,120 --> 00:14:02,800 Speaker 1: across them, and so you pull electrons off. People had 278 00:14:02,800 --> 00:14:05,480 Speaker 1: seen these things before, and you get these beams, these 279 00:14:05,480 --> 00:14:09,400 Speaker 1: glowing beams inside that look really cool because the electrons 280 00:14:09,400 --> 00:14:12,439 Speaker 1: were like knocking off atoms and ionizing them, and people 281 00:14:12,440 --> 00:14:14,559 Speaker 1: were doing lots of experiments with them trying to understand 282 00:14:14,600 --> 00:14:17,160 Speaker 1: what they were. And again JJ Thompson used them to 283 00:14:17,160 --> 00:14:21,120 Speaker 1: discover the electrons. But runkit was really interested in whether 284 00:14:21,240 --> 00:14:24,600 Speaker 1: or not the rays that were being produced inside these 285 00:14:24,600 --> 00:14:27,360 Speaker 1: tubes could pass through the glass. He was curious to 286 00:14:27,400 --> 00:14:28,720 Speaker 1: see what they could get through. 287 00:14:29,320 --> 00:14:33,120 Speaker 5: But these rays were originally electrons, like a stream of 288 00:14:33,160 --> 00:14:35,160 Speaker 5: electrons or were they light? 289 00:14:35,400 --> 00:14:37,600 Speaker 1: These were a stream of electrons and that's what JJ 290 00:14:37,640 --> 00:14:40,640 Speaker 1: Thompson discovered. But the glow that you saw that was 291 00:14:40,720 --> 00:14:43,560 Speaker 1: visible light. And so the electrons would knock into a 292 00:14:43,600 --> 00:14:47,040 Speaker 1: few atoms inside the tube, ionize them, they would give 293 00:14:47,040 --> 00:14:48,800 Speaker 1: off some light, and then they would decay back to 294 00:14:48,840 --> 00:14:51,760 Speaker 1: their ground state. So what people were sort of oohing 295 00:14:51,800 --> 00:14:55,520 Speaker 1: and aweing over were seeing a beam of electrons exciting 296 00:14:55,520 --> 00:14:57,040 Speaker 1: the gas inside the tube. 297 00:14:57,120 --> 00:14:59,240 Speaker 5: Okay, but just to be clear that the X ray 298 00:14:59,280 --> 00:15:02,480 Speaker 5: is not the electrons and X rays is a light beam, right. 299 00:15:02,440 --> 00:15:02,840 Speaker 7: That's right. 300 00:15:02,840 --> 00:15:05,040 Speaker 1: The X ray is not an electron. Electron is a particle. 301 00:15:05,120 --> 00:15:07,360 Speaker 1: An X ray is a piece of light. Right, It's 302 00:15:07,360 --> 00:15:10,080 Speaker 1: a photon of a specific energy. But this is what 303 00:15:10,160 --> 00:15:12,760 Speaker 1: Runkin started with. He started with these tubes and he 304 00:15:12,800 --> 00:15:15,920 Speaker 1: was playing around with them, and he accidentally discovered that 305 00:15:15,960 --> 00:15:17,880 Speaker 1: they also generate X rays. 306 00:15:17,680 --> 00:15:21,200 Speaker 5: Mmm, like along with the electrons or when the electrons 307 00:15:21,240 --> 00:15:21,760 Speaker 5: hit stuff. 308 00:15:21,840 --> 00:15:23,800 Speaker 1: Yes, so the electrons one of the things they do 309 00:15:23,880 --> 00:15:26,440 Speaker 1: is they generated glow you can see with your naked eye. 310 00:15:26,560 --> 00:15:29,600 Speaker 1: But they also sometimes generate X rays, and we can 311 00:15:29,600 --> 00:15:31,640 Speaker 1: get into the whole details of exactly how that happens, 312 00:15:31,720 --> 00:15:35,480 Speaker 1: how they're accelerated and radiated. But sometimes they generate visible 313 00:15:35,560 --> 00:15:38,360 Speaker 1: light in our spectrum, and sometimes they generate photons that 314 00:15:38,400 --> 00:15:41,240 Speaker 1: are higher energy than these are X rays. So he 315 00:15:41,320 --> 00:15:44,320 Speaker 1: was interested in understanding, like, what is this thing generating? 316 00:15:44,400 --> 00:15:47,200 Speaker 1: Can it pass through the glass walls of the tube. 317 00:15:47,400 --> 00:15:49,720 Speaker 1: So what he did was he built a big black box, 318 00:15:49,880 --> 00:15:53,320 Speaker 1: like a light proof box, and his idea was, I'm 319 00:15:53,320 --> 00:15:56,240 Speaker 1: going to put this box around my tube. I'm going 320 00:15:56,280 --> 00:15:59,080 Speaker 1: to see what light is shined on the inside of 321 00:15:59,120 --> 00:16:01,880 Speaker 1: the box from this tube, so I can see sort 322 00:16:01,880 --> 00:16:04,040 Speaker 1: of like you know, what light comes out of the 323 00:16:04,040 --> 00:16:06,000 Speaker 1: tube and hits the side of the box. 324 00:16:06,120 --> 00:16:06,400 Speaker 7: Mmm. 325 00:16:07,240 --> 00:16:09,720 Speaker 5: So I guess he wanted to know. He thought he 326 00:16:09,800 --> 00:16:12,600 Speaker 5: was trapping the light that was coming from the tube, 327 00:16:13,120 --> 00:16:15,360 Speaker 5: but actually he saw that the light kind of leaked 328 00:16:15,400 --> 00:16:15,960 Speaker 5: outside of it. 329 00:16:16,040 --> 00:16:18,960 Speaker 1: Yeah, exactly. He turned off the lights in his laboratory 330 00:16:19,080 --> 00:16:21,080 Speaker 1: just to sort of like get things warmed up, and 331 00:16:21,120 --> 00:16:23,160 Speaker 1: he was going to look inside the box to see 332 00:16:23,160 --> 00:16:25,680 Speaker 1: if he could see like light on the inside walls 333 00:16:25,680 --> 00:16:28,480 Speaker 1: of the box. But before he did that, he noticed 334 00:16:28,640 --> 00:16:31,840 Speaker 1: that he saw this weird light outside the box on 335 00:16:31,880 --> 00:16:34,480 Speaker 1: the wall of his laboratory, and he was like, what's 336 00:16:34,520 --> 00:16:36,600 Speaker 1: that over there? And it turns out he had a 337 00:16:36,600 --> 00:16:39,360 Speaker 1: special sort of screen over there just happened to be 338 00:16:39,400 --> 00:16:42,520 Speaker 1: in the right location that can receive X rays and 339 00:16:42,640 --> 00:16:46,000 Speaker 1: glows when it hits X rays. And so he discovered 340 00:16:46,200 --> 00:16:48,360 Speaker 1: that the light doesn't just go through the glass. It 341 00:16:48,440 --> 00:16:51,360 Speaker 1: also went through his box all the way out to 342 00:16:51,400 --> 00:16:53,520 Speaker 1: the side of his lab and hit this special screen. 343 00:16:53,600 --> 00:16:55,960 Speaker 1: So it was quite by accident that he discovered these 344 00:16:56,080 --> 00:16:58,040 Speaker 1: X rays. WHOA, what was. 345 00:16:58,000 --> 00:17:00,680 Speaker 5: This special screen that he just had that it seems 346 00:17:00,720 --> 00:17:02,240 Speaker 5: like such an accidental discovery. 347 00:17:02,320 --> 00:17:05,640 Speaker 1: It's totally an accidental discovery. And it's a special screen 348 00:17:05,640 --> 00:17:09,440 Speaker 1: covered with a material that phosphoress, so it absorbs photons 349 00:17:09,440 --> 00:17:11,959 Speaker 1: at one wavelength and then it gives off photons at 350 00:17:11,960 --> 00:17:15,760 Speaker 1: a different wavelength, so it's a wavelength shifting effect. And 351 00:17:15,840 --> 00:17:17,000 Speaker 1: this is the kind of thing we do all the 352 00:17:17,000 --> 00:17:19,640 Speaker 1: time in physics these days. We absorb photons of one 353 00:17:19,680 --> 00:17:22,720 Speaker 1: thing and give off photons of another color. So we 354 00:17:22,760 --> 00:17:25,399 Speaker 1: happen to have a screen covered in this material. It 355 00:17:25,480 --> 00:17:28,919 Speaker 1: was a barrio phosphorescent material that could absorb X rays 356 00:17:28,960 --> 00:17:31,359 Speaker 1: and glow in the visible light. And he was like, 357 00:17:31,400 --> 00:17:34,480 Speaker 1: what's that over there? And did a bunch of experiments 358 00:17:34,520 --> 00:17:37,199 Speaker 1: and he discovered that it could pass through his box, 359 00:17:37,440 --> 00:17:39,359 Speaker 1: and it could pass through lots of other things, but 360 00:17:39,440 --> 00:17:41,920 Speaker 1: that it wouldn't pass through metal, for example. 361 00:17:42,000 --> 00:17:44,399 Speaker 5: Wow, Now, was this the first time that you know, 362 00:17:44,520 --> 00:17:48,159 Speaker 5: humans kind of got the idea that light can go 363 00:17:48,400 --> 00:17:51,000 Speaker 5: through things? Or did we already kind of know that 364 00:17:51,040 --> 00:17:53,560 Speaker 5: there are things in nature that can go through things? 365 00:17:53,640 --> 00:17:55,600 Speaker 1: Now, this is the first time we understood that light 366 00:17:55,640 --> 00:17:58,800 Speaker 1: could pass through something that we thought was otherwise solid. 367 00:17:59,240 --> 00:18:01,840 Speaker 1: And famously, the first X ray picture he ever took 368 00:18:02,160 --> 00:18:04,720 Speaker 1: was of his wife's hand, and you could see her 369 00:18:04,800 --> 00:18:07,400 Speaker 1: hand with its wedding ring on it, and he showed 370 00:18:07,440 --> 00:18:08,800 Speaker 1: it to her and he thought, this is gonna be 371 00:18:08,880 --> 00:18:11,399 Speaker 1: so romantic and awesome, but she was actually really creeped 372 00:18:11,400 --> 00:18:13,320 Speaker 1: out and she thought, oh my gosh, I've seen my 373 00:18:13,359 --> 00:18:16,560 Speaker 1: own death, because she'd seemed like her own skeleton inside 374 00:18:16,560 --> 00:18:19,160 Speaker 1: her hand. And I think it really changed the way 375 00:18:19,160 --> 00:18:23,280 Speaker 1: people felt about like the solidity of stuff. Right, you 376 00:18:23,320 --> 00:18:25,959 Speaker 1: think of yourself as solid and opaque but you're not. 377 00:18:26,280 --> 00:18:30,000 Speaker 1: You're transparent in some wavelengths of light and you're opaque 378 00:18:30,000 --> 00:18:31,400 Speaker 1: in other wavelengths of light. 379 00:18:31,560 --> 00:18:34,520 Speaker 5: Oh. So then from that day they invented X rays, 380 00:18:34,560 --> 00:18:35,840 Speaker 5: you know, for medical purposes. 381 00:18:35,920 --> 00:18:39,399 Speaker 1: Yeah. Things happened really fast because people very quickly understood 382 00:18:39,520 --> 00:18:41,840 Speaker 1: how powerful this was. Like you could see broken bones 383 00:18:41,880 --> 00:18:44,119 Speaker 1: inside the body, or you could see if your child 384 00:18:44,119 --> 00:18:47,520 Speaker 1: had swallowed something metal, and so just seeing inside the 385 00:18:47,520 --> 00:18:50,639 Speaker 1: body without having it cut it open was immediately and 386 00:18:50,840 --> 00:18:53,879 Speaker 1: enormously powerful. And within a year people were using it 387 00:18:53,920 --> 00:18:56,840 Speaker 1: in hospitals. And it wasn't hard to make X rays 388 00:18:56,920 --> 00:18:59,399 Speaker 1: Like Crook's tubes were a thing that already existed, and 389 00:18:59,440 --> 00:19:02,000 Speaker 1: so the technology sort of was all around. It just 390 00:19:02,040 --> 00:19:04,520 Speaker 1: took the right combination of knowing what to do and 391 00:19:04,560 --> 00:19:07,440 Speaker 1: how to do it. And he went on to win 392 00:19:07,520 --> 00:19:10,440 Speaker 1: the first Nobel Prize in physics just a few years later. 393 00:19:10,600 --> 00:19:13,720 Speaker 5: Really, the first one, Wow, the first one. 394 00:19:13,680 --> 00:19:16,280 Speaker 1: Yeah, exactly. And you know, it sort of satisfies all 395 00:19:16,280 --> 00:19:18,920 Speaker 1: the requirements. It teaches you something deep about the universe. 396 00:19:19,040 --> 00:19:21,959 Speaker 1: It also made a very big impact on humanity. 397 00:19:22,080 --> 00:19:24,800 Speaker 5: Wow. And it sounds like it was really more about 398 00:19:24,880 --> 00:19:26,159 Speaker 5: discovering the screen. 399 00:19:27,240 --> 00:19:29,720 Speaker 1: Yeah, it's a combination. You have to have the radiation 400 00:19:29,880 --> 00:19:32,640 Speaker 1: and you have to have a screen that can receive it. Right, 401 00:19:33,040 --> 00:19:35,439 Speaker 1: X rays are invisible to us, and so if they 402 00:19:35,480 --> 00:19:37,359 Speaker 1: can just fly through the universe and fly through a 403 00:19:37,400 --> 00:19:39,520 Speaker 1: wall to see them, you have to put something in 404 00:19:39,600 --> 00:19:43,280 Speaker 1: their path that they will interact with and transform that 405 00:19:43,359 --> 00:19:45,920 Speaker 1: information into something your eyeballs can see. 406 00:19:46,400 --> 00:19:50,080 Speaker 5: All right, Well, that's X ray radiation, which is light radiation. 407 00:19:50,280 --> 00:19:53,040 Speaker 5: But I guess the more popular kind of radiation, or 408 00:19:53,040 --> 00:19:56,480 Speaker 5: at least in people's consciousness, is particle radiation. And that's 409 00:19:56,480 --> 00:19:59,560 Speaker 5: where the curers come in. And so let's get into 410 00:19:59,640 --> 00:20:02,560 Speaker 5: that kin radiation. 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Would that helped Daniel 463 00:22:55,600 --> 00:23:01,040 Speaker 5: and near physicist, probably because they're so shiny and beaming. 464 00:23:01,240 --> 00:23:03,440 Speaker 1: Yeah, well, they just had to do these crazy experiments 465 00:23:03,480 --> 00:23:06,240 Speaker 1: which sometimes you know, do damage their own help. 466 00:23:06,920 --> 00:23:09,479 Speaker 5: All right, Well, I guess we talked about X ray radiation, 467 00:23:09,680 --> 00:23:13,240 Speaker 5: which is really just light at higher frequencies that can 468 00:23:13,280 --> 00:23:16,560 Speaker 5: pass through things, and some people associate that with radiation, 469 00:23:17,320 --> 00:23:20,720 Speaker 5: but maybe the more common type of radiation that people 470 00:23:20,760 --> 00:23:23,040 Speaker 5: think of is kind of the dangerous kind, I guess, 471 00:23:23,119 --> 00:23:26,399 Speaker 5: the nuclear kind, and that's more like particle radiation. 472 00:23:26,560 --> 00:23:29,000 Speaker 1: Yeah, and X rays, of course also dangerous. They can 473 00:23:29,080 --> 00:23:31,800 Speaker 1: deposit a lot of energy in your skin, and they 474 00:23:31,800 --> 00:23:34,679 Speaker 1: can cause cancer and UV radiation all that stuff, So 475 00:23:34,680 --> 00:23:38,280 Speaker 1: it's definitely dangerous. But particle radiation also very dangerous and 476 00:23:38,320 --> 00:23:41,479 Speaker 1: more famous because I think of the radioactive decays involved 477 00:23:41,520 --> 00:23:46,359 Speaker 1: in nuclear physics, for example. But particle radiation was discovered 478 00:23:46,400 --> 00:23:50,280 Speaker 1: pretty soon after particles were discovered. Remember, the whole idea 479 00:23:50,320 --> 00:23:54,160 Speaker 1: of a particle didn't really exist until JJ Thompson discovered 480 00:23:54,200 --> 00:23:57,000 Speaker 1: the electron in the late eighteen hundreds. You know, this 481 00:23:57,160 --> 00:24:00,000 Speaker 1: notion that everything was made out of tiny little bits, 482 00:24:00,040 --> 00:24:02,440 Speaker 1: and we could find those things and we could associate 483 00:24:02,720 --> 00:24:05,440 Speaker 1: like a tiny dot in space with mass and with 484 00:24:05,480 --> 00:24:08,920 Speaker 1: other quantities. This is a whole new idea in physics 485 00:24:09,160 --> 00:24:11,280 Speaker 1: at the time. It's not something which had existed for 486 00:24:11,320 --> 00:24:12,120 Speaker 1: a long time. 487 00:24:12,080 --> 00:24:14,480 Speaker 5: Right before, Like light was just like a beam, right, 488 00:24:14,840 --> 00:24:16,359 Speaker 5: like pure energy kind of. 489 00:24:16,520 --> 00:24:19,000 Speaker 1: Yeah, the wave properties of light were dominant, and people 490 00:24:19,119 --> 00:24:21,960 Speaker 1: thought about light as a wave. They thought about matter 491 00:24:22,040 --> 00:24:24,719 Speaker 1: and waves existing. But the whole idea that things were 492 00:24:24,720 --> 00:24:27,000 Speaker 1: made out of tiny particles, or that these tiny particles 493 00:24:27,040 --> 00:24:30,840 Speaker 1: could fly through space invisibly and hurt you, for example, 494 00:24:31,080 --> 00:24:33,960 Speaker 1: this was brand new. But it was discovered pretty soon 495 00:24:34,160 --> 00:24:38,400 Speaker 1: after the electron was discovered again in the late eighteen hundreds, yeah, 496 00:24:38,440 --> 00:24:40,400 Speaker 1: like the next year. Yeah, And it was spurred by 497 00:24:40,400 --> 00:24:43,359 Speaker 1: the discovery of X rays. Like everybody in the world 498 00:24:43,440 --> 00:24:45,320 Speaker 1: was very excited about the X ray discovery made a 499 00:24:45,440 --> 00:24:48,200 Speaker 1: huge wave in the world of physics. No pun intended, 500 00:24:48,240 --> 00:24:50,199 Speaker 1: pun definitely intended. 501 00:24:49,840 --> 00:24:53,159 Speaker 5: Oh intended, all right, sorry and pause for it. So 502 00:24:53,800 --> 00:24:55,280 Speaker 5: I thought me it was unintentional. 503 00:24:55,800 --> 00:24:58,320 Speaker 1: No, And this bit about the screen that you latched onto, 504 00:24:58,680 --> 00:25:01,719 Speaker 1: this guy deckrel He also was really excited about that. 505 00:25:01,960 --> 00:25:05,280 Speaker 1: He thought it's really cool for something to absorb energy 506 00:25:05,320 --> 00:25:08,480 Speaker 1: in one wavelength and emit in another. To absorb one 507 00:25:08,600 --> 00:25:11,160 Speaker 1: kind of energy and emit another kind of thing. It's 508 00:25:11,200 --> 00:25:14,480 Speaker 1: called luminescence, and he thought it was really exciting and 509 00:25:14,560 --> 00:25:17,000 Speaker 1: he wanted to follow up in this and make also 510 00:25:17,080 --> 00:25:20,119 Speaker 1: some kind of crazy discovery. And he came from a 511 00:25:20,160 --> 00:25:23,160 Speaker 1: long line of physicists people have been studying this sort 512 00:25:23,200 --> 00:25:26,240 Speaker 1: of kind of thing of generation of heat and energy. 513 00:25:26,760 --> 00:25:29,320 Speaker 1: So he did a series of experiments with uranium crystals 514 00:25:29,440 --> 00:25:32,240 Speaker 1: and he was the first to discover particle radiation. So 515 00:25:32,280 --> 00:25:34,480 Speaker 1: he actually came well before the curies. 516 00:25:34,680 --> 00:25:38,080 Speaker 5: Oh interesting, Well, apparently his father was also a physicist 517 00:25:38,280 --> 00:25:39,880 Speaker 5: and a radiation physicist too. 518 00:25:39,960 --> 00:25:43,240 Speaker 1: That's right. He actually came from several generations of physicists 519 00:25:43,280 --> 00:25:45,080 Speaker 1: and they all had the same job. They all had 520 00:25:45,119 --> 00:25:47,600 Speaker 1: like the same chair in the head of the natural 521 00:25:47,640 --> 00:25:50,320 Speaker 1: science department in Paris, and so it was sort of 522 00:25:50,400 --> 00:25:54,600 Speaker 1: like a hereditary position almost. He's like a legacy physicist 523 00:25:54,640 --> 00:25:55,080 Speaker 1: in France. 524 00:25:55,160 --> 00:25:57,680 Speaker 5: So his father looked into radiation, but he didn't discovery. 525 00:25:57,800 --> 00:26:00,960 Speaker 1: Yeah, his father also had been studying uranium crests and 526 00:26:01,160 --> 00:26:04,479 Speaker 1: after Becherel discovered radiation, people went back and looked at 527 00:26:04,520 --> 00:26:06,919 Speaker 1: his father's notebooks, and there was plenty of evidence in 528 00:26:06,960 --> 00:26:10,960 Speaker 1: his father's notebooks to document evidence of radiation, but his 529 00:26:11,000 --> 00:26:14,560 Speaker 1: father just sort of didn't put it together. And this 530 00:26:14,600 --> 00:26:16,520 Speaker 1: is something you can do in physics. When people make 531 00:26:16,520 --> 00:26:18,760 Speaker 1: a big discovery, you can look back at people who 532 00:26:19,000 --> 00:26:21,520 Speaker 1: might have discovered it if they had only believed their 533 00:26:21,560 --> 00:26:24,639 Speaker 1: results or followed up on something they didn't understand. It 534 00:26:24,760 --> 00:26:27,120 Speaker 1: sort of missed opportunities in physics. 535 00:26:27,240 --> 00:26:29,320 Speaker 5: So I wonder if you want people to see that 536 00:26:30,880 --> 00:26:33,160 Speaker 5: or if that's just kind of a little bit embarrassing 537 00:26:33,240 --> 00:26:34,320 Speaker 5: from a physics point of view. 538 00:26:34,600 --> 00:26:37,280 Speaker 1: I think it's super fascinating from a sort of history 539 00:26:37,320 --> 00:26:39,480 Speaker 1: of science point of view. You get a result that 540 00:26:39,520 --> 00:26:42,000 Speaker 1: you don't understand or doesn't make sense, do you always 541 00:26:42,000 --> 00:26:43,920 Speaker 1: follow up on it or do you sort of leave 542 00:26:43,960 --> 00:26:47,120 Speaker 1: it behind? And those missed opportunities, you know, those times 543 00:26:47,160 --> 00:26:50,119 Speaker 1: when science could have gone differently if somebody had taken 544 00:26:50,160 --> 00:26:52,880 Speaker 1: a different path and thought about something different or had 545 00:26:52,880 --> 00:26:55,679 Speaker 1: a different conversation at a conference. It's fascinating to me 546 00:26:55,760 --> 00:26:58,800 Speaker 1: to imagine the sort of alternate universes in which we 547 00:26:58,840 --> 00:27:00,720 Speaker 1: discovered things in different words. 548 00:27:00,840 --> 00:27:03,000 Speaker 5: Because that's what everyone wants in their tombstone, you know, 549 00:27:03,520 --> 00:27:04,960 Speaker 5: could have won a Nobel prize. 550 00:27:05,359 --> 00:27:09,280 Speaker 1: Yeah, But they did these experiments with uranium crystals. So 551 00:27:09,440 --> 00:27:11,440 Speaker 1: uranium was a thing, it was a known, it wasn't 552 00:27:11,520 --> 00:27:14,280 Speaker 1: understood what it was doing, but they were doing early 553 00:27:14,320 --> 00:27:16,680 Speaker 1: studies with it. And essentially what they did basically is 554 00:27:16,720 --> 00:27:19,840 Speaker 1: they just put it next to photographic plates, like photographs 555 00:27:19,840 --> 00:27:22,280 Speaker 1: were a thing back then, So they just wrapped them 556 00:27:22,280 --> 00:27:24,520 Speaker 1: in paper and put them next to photographic plates and 557 00:27:24,520 --> 00:27:26,080 Speaker 1: they wanted to see what would happen. 558 00:27:26,359 --> 00:27:30,120 Speaker 5: Oh, right, because they had photographs at that time. And 559 00:27:30,320 --> 00:27:32,440 Speaker 5: that is also kind of like magic, like light hits 560 00:27:32,480 --> 00:27:34,560 Speaker 5: it or not hits it, and it changes color. 561 00:27:34,640 --> 00:27:37,960 Speaker 1: Yeah, exactly. It's a special process that absorbs photons and 562 00:27:38,240 --> 00:27:40,679 Speaker 1: develops in a different way based on, you know, the 563 00:27:40,720 --> 00:27:42,879 Speaker 1: amount of photons that hit it. To really sort of 564 00:27:42,920 --> 00:27:47,119 Speaker 1: awesome chemical process for absorbing things and taking data. And 565 00:27:47,160 --> 00:27:49,720 Speaker 1: back before we had computers and digital cameras and stuff, 566 00:27:49,760 --> 00:27:52,639 Speaker 1: everything was analog. This was a powerful way to do 567 00:27:52,720 --> 00:27:56,119 Speaker 1: science experiments. But Beckerel sort of started off on the 568 00:27:56,119 --> 00:27:59,160 Speaker 1: wrong track. Remember, he was interested in luminescence. He thought, 569 00:27:59,320 --> 00:28:01,800 Speaker 1: if you took these uranium crystals and you left them 570 00:28:01,800 --> 00:28:04,240 Speaker 1: in the sun, that they would absorb a bunch of 571 00:28:04,359 --> 00:28:06,919 Speaker 1: energy from the sun and then they might glow in 572 00:28:06,960 --> 00:28:10,000 Speaker 1: some new invisible way. So he put these uranium crystals 573 00:28:10,000 --> 00:28:12,320 Speaker 1: in the sun, then he wrapped them in paper to 574 00:28:12,359 --> 00:28:14,560 Speaker 1: block in the invisible light, and he put them next 575 00:28:14,600 --> 00:28:17,119 Speaker 1: to these photographic plates. So he was hoping maybe he 576 00:28:17,119 --> 00:28:19,439 Speaker 1: would like spind a new way to make X rays, 577 00:28:19,520 --> 00:28:21,320 Speaker 1: or that they would admit in the X ray because 578 00:28:21,440 --> 00:28:23,440 Speaker 1: X rays had just been discovered. 579 00:28:22,920 --> 00:28:26,840 Speaker 5: All right, So he saw radiation and X rays and 580 00:28:26,880 --> 00:28:28,640 Speaker 5: he thought, hey, I wonder if that works for everything. 581 00:28:28,880 --> 00:28:31,200 Speaker 5: So do you think he tried a bunch of different materials, 582 00:28:31,240 --> 00:28:32,800 Speaker 5: not just these uranium crystals. 583 00:28:32,960 --> 00:28:35,200 Speaker 1: Yeah, he tried a bunch of different materials wondering what 584 00:28:35,240 --> 00:28:38,800 Speaker 1: would glow. But these uranium salts, these uranium crystals were 585 00:28:38,840 --> 00:28:41,560 Speaker 1: the things that gave him the best results. But that's 586 00:28:41,600 --> 00:28:44,560 Speaker 1: not actually the most interesting part of his discovery. I mean, 587 00:28:44,600 --> 00:28:46,560 Speaker 1: first he did that, he said, I'm gonna put these 588 00:28:46,560 --> 00:28:48,800 Speaker 1: things out in the sun. Then I'm going to wrap 589 00:28:48,840 --> 00:28:50,920 Speaker 1: them in paper to block in the invisible light and 590 00:28:51,040 --> 00:28:53,600 Speaker 1: see if they make an impact on the photographic plates. 591 00:28:53,720 --> 00:28:56,520 Speaker 1: And they did, so he thought, ooh, that's cool. But 592 00:28:56,600 --> 00:29:00,680 Speaker 1: then he accidentally left a bunch of them a drawer 593 00:29:01,320 --> 00:29:05,040 Speaker 1: next to these photographic plates without shining them in the sun. Mmm, 594 00:29:05,520 --> 00:29:07,520 Speaker 1: so he sort of messed up his experiment. He thought 595 00:29:07,560 --> 00:29:08,960 Speaker 1: it was necessary to leave it in the sun to 596 00:29:09,000 --> 00:29:11,560 Speaker 1: absorb energy and then it would give off this radiation. 597 00:29:12,040 --> 00:29:14,880 Speaker 1: But he accidentally left over the weekend a bunch of 598 00:29:15,000 --> 00:29:18,320 Speaker 1: uranium crystals next to one of these photographic plates and 599 00:29:18,440 --> 00:29:21,480 Speaker 1: came back the next week and said, hmm, oops, for guys, 600 00:29:21,520 --> 00:29:23,400 Speaker 1: will leave this stuff in the sun. But let's just 601 00:29:23,480 --> 00:29:25,440 Speaker 1: develop this film and see what it says. 602 00:29:25,760 --> 00:29:30,120 Speaker 5: Woad seriously, total accident. 603 00:29:29,800 --> 00:29:32,120 Speaker 1: Total accident. And he thought, well, you know, I guess 604 00:29:32,120 --> 00:29:34,360 Speaker 1: I did this weird experiment where I skipped the step 605 00:29:34,360 --> 00:29:37,040 Speaker 1: with the sun. Let's see what happens. And he developed 606 00:29:37,080 --> 00:29:39,920 Speaker 1: it and the picture looked exactly the same, which tells 607 00:29:39,960 --> 00:29:42,680 Speaker 1: him that it didn't need to absorb energy from the sun. 608 00:29:42,800 --> 00:29:46,160 Speaker 1: It wasn't luminescence where it was slurping in energy from 609 00:29:46,200 --> 00:29:48,800 Speaker 1: the sun and then changing it into X rays or something. 610 00:29:49,000 --> 00:29:51,960 Speaker 1: It was different. The uranium crystals were just giving off 611 00:29:52,120 --> 00:29:54,760 Speaker 1: energy on their own. They were just like a source 612 00:29:54,800 --> 00:29:55,960 Speaker 1: of some new kind of. 613 00:29:56,000 --> 00:30:00,400 Speaker 5: Radiation, some new kind of invisible ray. Right, really what 614 00:30:00,440 --> 00:30:02,920 Speaker 5: he thought, right, something invisible was coming out of this 615 00:30:03,080 --> 00:30:05,400 Speaker 5: and this invisible thing somehow had energy. 616 00:30:05,600 --> 00:30:08,760 Speaker 1: Yeah, and you didn't have to put in energy. It's 617 00:30:08,760 --> 00:30:10,120 Speaker 1: not like with the Crooks too, where you had to 618 00:30:10,120 --> 00:30:13,720 Speaker 1: apply electricity and it generated energy for the electrons which 619 00:30:13,720 --> 00:30:16,880 Speaker 1: generated the X rays. And it wasn't like phosphorescence where 620 00:30:16,920 --> 00:30:18,560 Speaker 1: you had to sit out in the sun and absorb 621 00:30:18,640 --> 00:30:20,560 Speaker 1: the energy and then give it off. It was just 622 00:30:20,600 --> 00:30:24,080 Speaker 1: like pumping out this invisible energy. And now we know 623 00:30:24,240 --> 00:30:27,160 Speaker 1: that it was alpha radiation and beta radiation, but he 624 00:30:27,200 --> 00:30:28,960 Speaker 1: didn't know that at the time. He just knew he 625 00:30:29,000 --> 00:30:30,840 Speaker 1: was emitting some crazy new rays. 626 00:30:31,320 --> 00:30:33,360 Speaker 5: And then he also won a Nobel Prize for it, right, 627 00:30:33,440 --> 00:30:34,960 Speaker 5: he won like the third one. 628 00:30:35,040 --> 00:30:37,560 Speaker 1: He did, He won the third one, but just barely. 629 00:30:37,920 --> 00:30:41,520 Speaker 1: He discovered this. And the day after he made this discovery, 630 00:30:41,840 --> 00:30:45,280 Speaker 1: he gave a presentation at like the local Scientific society, 631 00:30:45,640 --> 00:30:48,120 Speaker 1: and he beat out some English physicists who made the 632 00:30:48,160 --> 00:30:49,960 Speaker 1: discovery like later that week. 633 00:30:50,200 --> 00:30:53,240 Speaker 5: What but if he gave the presentation, then the other 634 00:30:53,280 --> 00:30:57,320 Speaker 5: one technically didn't discovery or I guess he wasn't at 635 00:30:57,360 --> 00:30:57,920 Speaker 5: the presentation. 636 00:30:58,040 --> 00:30:59,720 Speaker 1: He wasn't there yet, because you know, the world was 637 00:30:59,840 --> 00:31:02,560 Speaker 1: much smaller, so you could give a whole presentation and 638 00:31:02,600 --> 00:31:04,800 Speaker 1: a society in France and nobody would hear about it 639 00:31:04,800 --> 00:31:08,400 Speaker 1: in England until weeks later or so. And so Sylvanis 640 00:31:08,440 --> 00:31:12,200 Speaker 1: Thompson made very very similar experiments, very similar discoveries just 641 00:31:12,240 --> 00:31:14,760 Speaker 1: a few days later and lost out on the Nobel 642 00:31:14,840 --> 00:31:18,240 Speaker 1: Prize because Beckerell made this discovery and was very quick 643 00:31:18,280 --> 00:31:18,880 Speaker 1: to report it. 644 00:31:19,160 --> 00:31:21,040 Speaker 5: Oh, I see Bekerel was in another country. 645 00:31:21,120 --> 00:31:22,080 Speaker 1: Yes, this is in France. 646 00:31:22,240 --> 00:31:26,760 Speaker 5: Oh interesting, Wow, that's crazy. Two people in two different 647 00:31:26,800 --> 00:31:31,520 Speaker 5: countries make the same fundamental discovery almost a week apart. Yeah, 648 00:31:31,520 --> 00:31:32,480 Speaker 5: and there was no internet. 649 00:31:32,960 --> 00:31:35,560 Speaker 1: There was no internet. But this is all spurred by 650 00:31:35,680 --> 00:31:38,760 Speaker 1: Runkid's discovery of X rays and like cracked open whole 651 00:31:38,800 --> 00:31:41,600 Speaker 1: new area of research. People looking for these invisible rays? 652 00:31:41,600 --> 00:31:43,680 Speaker 1: How can we find them? What's making them? What kinds 653 00:31:43,720 --> 00:31:46,160 Speaker 1: are out there? And it really did sparkle, you know, 654 00:31:46,200 --> 00:31:47,560 Speaker 1: a whole new field of research. 655 00:31:48,120 --> 00:31:51,120 Speaker 5: All right. So then that's where we get to Madame 656 00:31:51,360 --> 00:31:54,760 Speaker 5: Currie and Pierre Currie, and that this is kind of 657 00:31:54,760 --> 00:31:57,280 Speaker 5: where their story starts, right like the year after. 658 00:31:57,280 --> 00:31:59,520 Speaker 1: Yeah, exactly, this is where their story starts. So they 659 00:31:59,560 --> 00:32:03,360 Speaker 1: came in after Becharel had already discovered radiation and Runken 660 00:32:03,400 --> 00:32:06,280 Speaker 1: had discovered X rays, and they were really interested in this. 661 00:32:06,800 --> 00:32:10,600 Speaker 1: And Curie herself has a really fascinating backstory. Remember, it's 662 00:32:10,680 --> 00:32:14,880 Speaker 1: very difficult for women in science to have any position 663 00:32:15,160 --> 00:32:17,760 Speaker 1: and to have any engagement. To even get an education. 664 00:32:18,360 --> 00:32:20,680 Speaker 1: She and her sister, for example, had to take turns 665 00:32:20,960 --> 00:32:23,560 Speaker 1: working and going to school. They had this deal where 666 00:32:23,560 --> 00:32:24,960 Speaker 1: one of them would work and the other one would 667 00:32:24,960 --> 00:32:27,120 Speaker 1: go to school, and then they took turns. Wow, and 668 00:32:27,160 --> 00:32:30,080 Speaker 1: you had to be really dedicated and sort of fend 669 00:32:30,160 --> 00:32:32,360 Speaker 1: off a lot of societal pressure even to get to 670 00:32:32,360 --> 00:32:34,880 Speaker 1: have an education, not to mention be a scientist at 671 00:32:34,920 --> 00:32:36,400 Speaker 1: the leading edge of physics knowledge. 672 00:32:36,440 --> 00:32:39,880 Speaker 5: Oh yeah, it's amazing, a pretty powerful story. So she 673 00:32:39,960 --> 00:32:42,200 Speaker 5: was in France and she I guess she knew about 674 00:32:42,240 --> 00:32:43,400 Speaker 5: Bequerel's discovery. 675 00:32:43,480 --> 00:32:46,160 Speaker 1: She knew about Beckerreil's discovery, but most of the world 676 00:32:46,240 --> 00:32:48,840 Speaker 1: was more excited about the X rays, like these new 677 00:32:48,960 --> 00:32:52,200 Speaker 1: uranium rays that they called them U rays. People are like, Okay, 678 00:32:52,200 --> 00:32:54,720 Speaker 1: that's cool, but X rays are better because they're easier 679 00:32:54,760 --> 00:32:57,760 Speaker 1: to use, they're faster, they're cheaper, they make sharper images. 680 00:32:58,160 --> 00:33:00,720 Speaker 1: But she was really interested in these us She was like, 681 00:33:00,760 --> 00:33:03,400 Speaker 1: what are these what's making them? What does it tell 682 00:33:03,480 --> 00:33:06,720 Speaker 1: us about the atom that these things are just being 683 00:33:06,840 --> 00:33:10,520 Speaker 1: created out of there. And she was working with her husband, Pierre, 684 00:33:10,840 --> 00:33:13,080 Speaker 1: and they had this really cool device, this thing called 685 00:33:13,120 --> 00:33:17,280 Speaker 1: an electrometer, and it could basically measure very sensitively how 686 00:33:17,320 --> 00:33:20,440 Speaker 1: well things could conduct electricity. And Pierre had developed this 687 00:33:20,480 --> 00:33:24,200 Speaker 1: technology from his earlier research which was into piezo electronics, 688 00:33:24,480 --> 00:33:27,680 Speaker 1: these little devices which create electricity if you squeeze them 689 00:33:27,800 --> 00:33:30,719 Speaker 1: or move if you apply electrical voltage across them. So 690 00:33:30,760 --> 00:33:33,360 Speaker 1: we had this technology and they applied it to the 691 00:33:33,400 --> 00:33:36,400 Speaker 1: study of these urrays and they found something pretty cool, 692 00:33:36,600 --> 00:33:38,480 Speaker 1: which is that if you have a bunch of uranium, 693 00:33:38,760 --> 00:33:42,360 Speaker 1: the air around the uranium tends to get ionized. They 694 00:33:42,400 --> 00:33:45,800 Speaker 1: can conduct electricity more easily than if you don't have 695 00:33:46,000 --> 00:33:46,760 Speaker 1: uranium around. 696 00:33:46,880 --> 00:33:49,239 Speaker 5: Oh I see. And that was a big clue that 697 00:33:49,320 --> 00:33:51,280 Speaker 5: it was maybe giving off some kind of energy. 698 00:33:51,400 --> 00:33:53,640 Speaker 1: Yeah, that was a big clue that it was shooting 699 00:33:53,640 --> 00:33:56,360 Speaker 1: out something because it was like changing the air, right, 700 00:33:56,400 --> 00:33:58,680 Speaker 1: This energy was coming out, It was changing the air 701 00:33:58,880 --> 00:34:02,239 Speaker 1: around the uranium. And Pierre and Marie they took like 702 00:34:02,480 --> 00:34:05,760 Speaker 1: no safety precautions. They got to read it so much 703 00:34:05,840 --> 00:34:08,239 Speaker 1: in their research. There are all these moments you can 704 00:34:08,280 --> 00:34:10,560 Speaker 1: read about in their lab notebooks where they're like, Pierre 705 00:34:10,560 --> 00:34:13,280 Speaker 1: has been sick every single day for the last three months. 706 00:34:13,440 --> 00:34:15,839 Speaker 1: I wonder if it's coinciding with all these experiments we've 707 00:34:15,880 --> 00:34:20,120 Speaker 1: done whatever, my goodness, and they just kept going. It 708 00:34:20,200 --> 00:34:23,200 Speaker 1: was pretty incredible. They were really pretty sick during this 709 00:34:23,239 --> 00:34:26,040 Speaker 1: whole period, like nineteen hundred to nineteen ten, which is 710 00:34:26,040 --> 00:34:28,640 Speaker 1: a very intense period of their research and discoveries. They're 711 00:34:28,680 --> 00:34:32,120 Speaker 1: basically sick the whole time, and they never really associated 712 00:34:32,200 --> 00:34:35,439 Speaker 1: like all this illness with the research they were doing. 713 00:34:35,680 --> 00:34:38,080 Speaker 1: I'm not sure if that was like a cognitive choice, 714 00:34:38,160 --> 00:34:41,880 Speaker 1: like let's not influence our research with these petty details 715 00:34:41,880 --> 00:34:44,359 Speaker 1: of life, or if they knew and they just sort 716 00:34:44,360 --> 00:34:46,920 Speaker 1: of didn't care because they just were so hungry to 717 00:34:46,960 --> 00:34:47,840 Speaker 1: reveal the knowledge. 718 00:34:48,239 --> 00:34:50,080 Speaker 5: Well, technically, we don't know. I mean, they could have 719 00:34:50,200 --> 00:34:52,560 Speaker 5: just been, you know, on a rash of eating bad 720 00:34:53,400 --> 00:34:54,320 Speaker 5: s cargoers. 721 00:34:54,440 --> 00:34:56,600 Speaker 1: I suppose so. But you know, you look at the 722 00:34:56,640 --> 00:34:59,759 Speaker 1: pattern of damage to their bodies, like their fingertips had 723 00:34:59,760 --> 00:35:02,720 Speaker 1: the really terrible damage to them, you know. Murray Curie. 724 00:35:02,840 --> 00:35:05,399 Speaker 1: She's now like a hero in France. Of course, they 725 00:35:05,480 --> 00:35:08,520 Speaker 1: moved her ashes from wherever they had been born just 726 00:35:08,520 --> 00:35:10,880 Speaker 1: about twenty years ago. They moved them to the Pantheon 727 00:35:10,960 --> 00:35:13,480 Speaker 1: in Paris, which is where you know, France ters the 728 00:35:13,520 --> 00:35:16,560 Speaker 1: ashes and the remains of its most highly revered citizens. 729 00:35:16,880 --> 00:35:20,680 Speaker 1: And those ashes were still radioactive. This is like, you know, 730 00:35:20,880 --> 00:35:26,440 Speaker 1: seventy years later what, yeah, exactly. She definitely hurt herself 731 00:35:26,600 --> 00:35:31,080 Speaker 1: for science, he lives. She was really fascinated with this 732 00:35:31,239 --> 00:35:34,520 Speaker 1: fact that the uranium, the U rays could change the 733 00:35:34,560 --> 00:35:36,920 Speaker 1: air around them, and this is what led her to 734 00:35:36,960 --> 00:35:39,880 Speaker 1: this hypothesis that it wasn't like chemical, It's not like 735 00:35:40,120 --> 00:35:42,920 Speaker 1: the electron is giving off some energy that it's absorbed 736 00:35:43,080 --> 00:35:45,280 Speaker 1: from some other way. She thought it was something deep 737 00:35:45,400 --> 00:35:48,760 Speaker 1: in the atom, that the atoms themselves are maybe not stable, 738 00:35:49,080 --> 00:35:51,640 Speaker 1: that there was something changing internally and it was giving 739 00:35:51,680 --> 00:35:54,160 Speaker 1: off this energy. And of course now we know she's right, 740 00:35:54,520 --> 00:35:57,640 Speaker 1: it was radioactive decay. But this was a really big 741 00:35:57,680 --> 00:35:59,560 Speaker 1: and sort of bold idea at the time. 742 00:36:00,239 --> 00:36:02,800 Speaker 5: Well, at this point in our history, we knew about 743 00:36:02,840 --> 00:36:04,719 Speaker 5: the atom, and we knew about the kind of the 744 00:36:04,760 --> 00:36:05,680 Speaker 5: structure of it. 745 00:36:05,840 --> 00:36:08,399 Speaker 1: We knew about the electron, but we hadn't yet even 746 00:36:08,440 --> 00:36:11,480 Speaker 1: discovered the nucleus of the atom. It wasn't until Rutherford 747 00:36:11,760 --> 00:36:15,719 Speaker 1: bombarded gold foil with radiation later that we understood that 748 00:36:15,760 --> 00:36:17,759 Speaker 1: there was like a hard center to the atom that 749 00:36:17,840 --> 00:36:20,800 Speaker 1: had a nucleus. God forbid, you know, understanding the proton 750 00:36:20,840 --> 00:36:23,359 Speaker 1: and the neutron inside of it. At the time, after 751 00:36:23,440 --> 00:36:26,560 Speaker 1: JJ Thompson discovered the electron, he thought that matter was 752 00:36:26,640 --> 00:36:29,200 Speaker 1: like a bunch of electrons sort of floating in a 753 00:36:29,440 --> 00:36:33,360 Speaker 1: positively charged jelly. And so we didn't really even understand 754 00:36:33,360 --> 00:36:35,360 Speaker 1: the structure of the atom. So this is a really 755 00:36:35,400 --> 00:36:36,879 Speaker 1: big leap for anybody to make. 756 00:36:36,960 --> 00:36:38,799 Speaker 5: Yeah, I mean, she's saying that it comes from deep 757 00:36:38,840 --> 00:36:40,520 Speaker 5: within the atom, but we didn't even know there was 758 00:36:40,520 --> 00:36:40,920 Speaker 5: an atom. 759 00:36:41,000 --> 00:36:42,719 Speaker 1: Well, we knew there were atoms, we just didn't really 760 00:36:42,760 --> 00:36:45,120 Speaker 1: know like what was going on inside there. We didn't 761 00:36:45,200 --> 00:36:48,120 Speaker 1: really understand there was a hard nucleus that was made 762 00:36:48,120 --> 00:36:51,040 Speaker 1: out of these smaller particles. So yeah, it's a pretty 763 00:36:51,040 --> 00:36:51,520 Speaker 1: big leap. 764 00:36:51,800 --> 00:36:54,680 Speaker 5: All right, Let's get into her actual experiment in which 765 00:36:54,719 --> 00:36:58,120 Speaker 5: she discovered this nuclear radiation and what that means and 766 00:36:58,120 --> 00:37:01,480 Speaker 5: what other types of radiation were surrounded. But first let's 767 00:37:01,520 --> 00:37:02,719 Speaker 5: take another quick break. 768 00:37:06,719 --> 00:37:08,520 Speaker 1: When you pop a piece of cheese into your mouth 769 00:37:08,640 --> 00:37:11,760 Speaker 1: or enjoy a rich spoonful of Greek yogurt, you're probably 770 00:37:11,840 --> 00:37:15,880 Speaker 1: not thinking about the environmental impact of each and every bite, 771 00:37:15,920 --> 00:37:18,520 Speaker 1: But the people in the dairy industry are. US Dairy 772 00:37:18,560 --> 00:37:22,839 Speaker 1: has set themselves some ambitious sustainability goals, including being greenhouse 773 00:37:22,880 --> 00:37:25,480 Speaker 1: gas neutral by twenty to fifty. That's why they're working 774 00:37:25,480 --> 00:37:27,799 Speaker 1: hard every day to find new ways to reduce waste, 775 00:37:27,880 --> 00:37:32,120 Speaker 1: conserve natural resources, and drive down greenhouse gas emissions. Take water, 776 00:37:32,160 --> 00:37:35,239 Speaker 1: for example, most dairy farms reuse water up to four 777 00:37:35,320 --> 00:37:38,759 Speaker 1: times the same water cools the milk, cleans equipment, washes 778 00:37:38,800 --> 00:37:41,600 Speaker 1: the barn, and irrigates the crops. How is US dairy 779 00:37:41,640 --> 00:37:45,399 Speaker 1: tackling greenhouse gases? Many farms use anaerobic digestors that turn 780 00:37:45,440 --> 00:37:49,360 Speaker 1: the methane from maneuver into renewable energy that can power farms, towns, 781 00:37:49,360 --> 00:37:51,440 Speaker 1: and electric cars. So the next time you grab a 782 00:37:51,480 --> 00:37:53,480 Speaker 1: slice of pizza or lick an ice cream cone, know 783 00:37:53,560 --> 00:37:56,239 Speaker 1: that dairy farmers and processors around the country are using 784 00:37:56,280 --> 00:37:59,719 Speaker 1: the latest practices and innovations to provide the nutrient dense 785 00:37:59,800 --> 00:38:02,240 Speaker 1: days every products we love with less of an impact. 786 00:38:02,360 --> 00:38:05,479 Speaker 1: Visit US dairy dot com slash sustainability to learn more. 787 00:38:06,520 --> 00:38:10,000 Speaker 9: There are children, friends and families walking, riding on paths 788 00:38:10,000 --> 00:38:12,160 Speaker 9: and the roads every day. Remember they're real people with 789 00:38:12,239 --> 00:38:14,600 Speaker 9: loved ones who need them to get home safely. Protect 790 00:38:14,600 --> 00:38:17,640 Speaker 9: our cyclists and pedestrians because they're people too, Go safely, 791 00:38:17,680 --> 00:38:21,160 Speaker 9: California from the California Office of Traffic Safety and caltrans Uh. 792 00:38:21,239 --> 00:38:23,800 Speaker 4: Why does this room look amazing? What'd you change? 793 00:38:23,920 --> 00:38:24,120 Speaker 5: Oh? 794 00:38:24,400 --> 00:38:26,720 Speaker 10: I just got these customs shades from Blinds dot Com. 795 00:38:26,800 --> 00:38:29,839 Speaker 10: It's all online, so it's really easy. Great price too. 796 00:38:30,239 --> 00:38:30,359 Speaker 6: Ugh. 797 00:38:30,760 --> 00:38:35,200 Speaker 4: I remember shopping for Blinds. I waited around all day 798 00:38:35,560 --> 00:38:36,400 Speaker 4: just to get a quote. 799 00:38:36,920 --> 00:38:37,080 Speaker 10: Hi. 800 00:38:37,200 --> 00:38:39,200 Speaker 5: Sorry, I'm Lee. I know you said just the bedroom, 801 00:38:39,200 --> 00:38:40,200 Speaker 5: but what do you feel about it? 802 00:38:40,200 --> 00:38:41,960 Speaker 4: I feel like I had to say yes just to 803 00:38:41,960 --> 00:38:42,560 Speaker 4: get rid of her. 804 00:38:42,640 --> 00:38:44,200 Speaker 5: All right, just go ahead and sign here and we'll 805 00:38:44,200 --> 00:38:44,680 Speaker 5: get everything. 806 00:38:44,680 --> 00:38:47,720 Speaker 4: It took forever and the worst part for them hidden fees. 807 00:38:48,960 --> 00:38:49,520 Speaker 4: How about you. 808 00:38:50,120 --> 00:38:52,719 Speaker 10: I chatted with my Blinds dot Com design consultant on 809 00:38:52,800 --> 00:38:55,399 Speaker 10: my time, got free samples and it was all super 810 00:38:55,480 --> 00:38:58,080 Speaker 10: high quality at a great price. Plus they make it 811 00:38:58,120 --> 00:39:00,960 Speaker 10: easy to diy or at in like I did. 812 00:39:01,080 --> 00:39:03,480 Speaker 4: Blinds dot Com sounds way better. 813 00:39:03,640 --> 00:39:06,719 Speaker 10: Way better and everything comes with there one hundred percent 814 00:39:06,760 --> 00:39:08,800 Speaker 10: satisfaction guarantee plus. 815 00:39:08,920 --> 00:39:09,719 Speaker 5: Check this out. 816 00:39:09,880 --> 00:39:11,520 Speaker 10: I can control them from my phone. 817 00:39:11,760 --> 00:39:14,160 Speaker 4: Whoa Magic, There's a better way. 818 00:39:14,400 --> 00:39:17,040 Speaker 9: Shop blinds dot com for up to forty five percent 819 00:39:17,120 --> 00:39:18,360 Speaker 9: off Blinds dot Com. 820 00:39:18,480 --> 00:39:19,880 Speaker 1: Rules and restrictions may apply. 821 00:39:28,920 --> 00:39:32,399 Speaker 5: All right, we're talking about the discovery of radiation, and 822 00:39:32,600 --> 00:39:35,840 Speaker 5: we're up to Marie Crie and her discovery that the 823 00:39:36,000 --> 00:39:41,800 Speaker 5: nuclei of atoms also radiate things. Because we knew about 824 00:39:42,040 --> 00:39:44,960 Speaker 5: X ray radiation, but we didn't know about this particular 825 00:39:45,040 --> 00:39:47,040 Speaker 5: kind which is coming from the nucleus. 826 00:39:47,120 --> 00:39:49,319 Speaker 1: Yeah, and we didn't even really know about the nucleus yet. 827 00:39:49,400 --> 00:39:51,880 Speaker 1: So this is giving us an insight that there's something 828 00:39:51,960 --> 00:39:55,200 Speaker 1: inside the atom, some mechanism which is capable of generating 829 00:39:55,360 --> 00:40:00,000 Speaker 1: powerful particle radiation. And so this is discovered originally in urine. 830 00:40:00,640 --> 00:40:03,359 Speaker 1: Beccarell saw that it happened, but what the curis did 831 00:40:03,440 --> 00:40:06,279 Speaker 1: was that they sort of refined it. They discovered that 832 00:40:06,480 --> 00:40:10,359 Speaker 1: uranium itself was radioactive, but that there were variations of 833 00:40:10,520 --> 00:40:15,200 Speaker 1: uranium or that was even more radioactive than pure uranium itself, 834 00:40:15,400 --> 00:40:17,919 Speaker 1: which suggested that there might be something else in there, 835 00:40:18,080 --> 00:40:19,399 Speaker 1: even more radioactive. 836 00:40:19,560 --> 00:40:22,600 Speaker 5: Oh, I see interesting, like it's possible to make an 837 00:40:22,600 --> 00:40:25,480 Speaker 5: element like an atom the extra radioactive. 838 00:40:25,719 --> 00:40:28,800 Speaker 1: Yeah, exactly. They were working with this material called pitch blend, 839 00:40:29,080 --> 00:40:32,240 Speaker 1: which is a version of uranium ore, and they discovered 840 00:40:32,239 --> 00:40:34,920 Speaker 1: that before you purified it, before you purified it to 841 00:40:35,000 --> 00:40:38,960 Speaker 1: make just pure uranium, it was actually more radioactive. So 842 00:40:39,000 --> 00:40:41,960 Speaker 1: they had this hypothesis that there was something else in there, 843 00:40:42,000 --> 00:40:45,840 Speaker 1: a new element that was even more radioactive than uranium. 844 00:40:46,080 --> 00:40:49,239 Speaker 1: So they developed this technique to purify it, and a 845 00:40:49,280 --> 00:40:51,319 Speaker 1: lot of the time they spent, a lot of their 846 00:40:51,360 --> 00:40:55,399 Speaker 1: actual science was in this process of isolating this bit. 847 00:40:55,719 --> 00:40:58,759 Speaker 1: It took them, for example, three years of work on 848 00:40:58,840 --> 00:41:02,040 Speaker 1: pitch blend just isolate a tenth of a gram of 849 00:41:02,080 --> 00:41:03,320 Speaker 1: this new substance. 850 00:41:04,560 --> 00:41:07,239 Speaker 5: That's crazy. I imagine most people think of radioactive things 851 00:41:07,280 --> 00:41:09,400 Speaker 5: as like rocks or something, but for them, this is 852 00:41:09,400 --> 00:41:10,879 Speaker 5: probably like a powder or something. 853 00:41:11,000 --> 00:41:12,640 Speaker 1: Right, Yeah, these are like salts. 854 00:41:12,760 --> 00:41:12,920 Speaker 7: Right. 855 00:41:12,920 --> 00:41:15,480 Speaker 1: They're grinding them up, they're purifying it, they're doing chemistry 856 00:41:15,480 --> 00:41:17,719 Speaker 1: to try to separate the bits from the other, like 857 00:41:17,719 --> 00:41:19,960 Speaker 1: does this dissolve in that? How do we pull this 858 00:41:20,000 --> 00:41:23,040 Speaker 1: thing apart? So it really is sort of chemical, and 859 00:41:23,239 --> 00:41:25,719 Speaker 1: what they discovered is that there really is something in 860 00:41:25,760 --> 00:41:29,200 Speaker 1: there that's more radioactive than uranium. Yeah, and so their 861 00:41:29,200 --> 00:41:31,959 Speaker 1: big discovery was the discovery of a new element, which 862 00:41:32,040 --> 00:41:35,400 Speaker 1: Marie called polonium after her native poland mm. 863 00:41:36,520 --> 00:41:38,760 Speaker 5: I see, because like if you take a uranium atom 864 00:41:38,800 --> 00:41:42,520 Speaker 5: and you give it extra protons and neutrons, then it 865 00:41:42,560 --> 00:41:43,520 Speaker 5: becomes a different element. 866 00:41:43,600 --> 00:41:43,799 Speaker 7: Yeah. 867 00:41:43,800 --> 00:41:47,799 Speaker 1: Actually, uranium breaks down, right, it splits open, it's unstable, 868 00:41:47,960 --> 00:41:51,400 Speaker 1: and it turns into other stuff now we know, into thorium, 869 00:41:51,600 --> 00:41:55,520 Speaker 1: and into radium and eventually into polonium and all sorts 870 00:41:55,520 --> 00:41:57,560 Speaker 1: of stuff. So if you have a bunch of uranium, 871 00:41:57,560 --> 00:42:01,440 Speaker 1: it eventually turns into this combination of elements. It breaks 872 00:42:01,480 --> 00:42:04,799 Speaker 1: open and turns into smaller, lighter elements, some of which 873 00:42:04,840 --> 00:42:07,320 Speaker 1: are more radioactive than uranium itself. 874 00:42:08,200 --> 00:42:10,560 Speaker 5: So I guess you could say her discovery was kind 875 00:42:10,560 --> 00:42:13,360 Speaker 5: of about nuclear physics, right, even before we knew there 876 00:42:13,440 --> 00:42:16,719 Speaker 5: was a nucleus, she sort of maybe intuited that, you know, 877 00:42:16,719 --> 00:42:20,040 Speaker 5: there's something going on here inside of matter and atoms 878 00:42:20,040 --> 00:42:24,160 Speaker 5: that can somehow, you know, give off energy and change 879 00:42:24,239 --> 00:42:27,440 Speaker 5: into different elements. Right, that's maybe it was sort of 880 00:42:27,440 --> 00:42:30,320 Speaker 5: a big contribution. And yeah, not so much about the radiation, 881 00:42:30,480 --> 00:42:33,839 Speaker 5: but just kind of about the nature of the insides 882 00:42:33,920 --> 00:42:34,360 Speaker 5: of atoms. 883 00:42:34,480 --> 00:42:37,360 Speaker 1: Yeah, exactly what the radiation reveals about the structure of 884 00:42:37,400 --> 00:42:40,440 Speaker 1: atoms and the structure of matter itself. And you're right, 885 00:42:40,440 --> 00:42:44,120 Speaker 1: it's totally fascinating to see one element turn into another element. 886 00:42:44,560 --> 00:42:46,920 Speaker 1: And if it does that by giving off a particle, 887 00:42:47,280 --> 00:42:50,080 Speaker 1: that tells you that what defines an element must be 888 00:42:50,120 --> 00:42:54,040 Speaker 1: something related to its particle content. Right, you're giving off 889 00:42:54,040 --> 00:42:56,160 Speaker 1: a piece and you turn into something else. That tells 890 00:42:56,200 --> 00:42:58,960 Speaker 1: you that piece was essential for you to be uranium 891 00:42:59,040 --> 00:43:01,680 Speaker 1: or for you to be re So that was pretty 892 00:43:01,680 --> 00:43:04,360 Speaker 1: fascinating clue into the structure of the atom itself. He 893 00:43:04,400 --> 00:43:07,600 Speaker 1: had early nuclear physics. And so she went on to 894 00:43:08,000 --> 00:43:10,919 Speaker 1: win the Nobel Prize in nineteen oh three, same year 895 00:43:11,280 --> 00:43:12,680 Speaker 1: she got her pH d thesis. 896 00:43:12,719 --> 00:43:13,480 Speaker 5: Oh my goodness. 897 00:43:13,800 --> 00:43:16,600 Speaker 1: Yeah, pretty awesome. Not only the first woman to win 898 00:43:16,600 --> 00:43:19,279 Speaker 1: a Nobel Prize in physics, but the first woman in 899 00:43:19,360 --> 00:43:21,000 Speaker 1: France to receive a PhD. 900 00:43:21,160 --> 00:43:24,760 Speaker 5: Wow. I wonder which one's more significant in a way. 901 00:43:25,560 --> 00:43:28,239 Speaker 5: So she was also in on the third Nobel Prize ever. 902 00:43:28,440 --> 00:43:32,080 Speaker 1: Yeah, she and her husband Pierre and Becquerel all won 903 00:43:32,120 --> 00:43:34,560 Speaker 1: the Nobel Prize in nineteen oh three. But you know, 904 00:43:34,600 --> 00:43:38,040 Speaker 1: obviously she was very deserving, but the initial nomination was 905 00:43:38,120 --> 00:43:41,680 Speaker 1: only for Pierre and Becquerel. They excluded her, probably because 906 00:43:41,719 --> 00:43:44,839 Speaker 1: she was a woman, but Pierre insisted that, hey, look, 907 00:43:44,880 --> 00:43:47,120 Speaker 1: Marie has done at least as much work as anybody else. 908 00:43:47,160 --> 00:43:49,520 Speaker 1: She's very deserving. So she ended up being included in 909 00:43:49,560 --> 00:43:50,280 Speaker 1: the Nobel Prize. 910 00:43:50,280 --> 00:43:52,200 Speaker 5: Wow, that's a great great husband there. 911 00:43:52,120 --> 00:43:56,200 Speaker 1: Yeah, exactly. Unfortunately he died tragically. He was hit by 912 00:43:56,200 --> 00:43:59,400 Speaker 1: a horse cart filled with heavy equipment and was crushed 913 00:43:59,440 --> 00:43:59,839 Speaker 1: one day. 914 00:44:00,160 --> 00:44:03,200 Speaker 5: No way, after all this, so he was killed by 915 00:44:03,280 --> 00:44:04,319 Speaker 5: horse radiation. 916 00:44:04,120 --> 00:44:09,520 Speaker 1: Anyway, exactly. Horses are an energetic particle. I suppose. No, 917 00:44:09,680 --> 00:44:11,960 Speaker 1: we shouldn't laugh over anybody's death. It was tragic and 918 00:44:12,000 --> 00:44:15,080 Speaker 1: it was very difficult for Marie, but she persevered and 919 00:44:15,160 --> 00:44:18,800 Speaker 1: she did a bunch more chemistry and isolated another element, radium, 920 00:44:19,160 --> 00:44:21,719 Speaker 1: for which she won the nineteen eleven Nobel Prize, this 921 00:44:21,840 --> 00:44:23,000 Speaker 1: time in chemistry. 922 00:44:23,920 --> 00:44:26,080 Speaker 5: Also, it's rare. How many people get a Nobel Prize 923 00:44:26,080 --> 00:44:29,080 Speaker 5: for their PhD work? Almost nobody, right. 924 00:44:29,000 --> 00:44:31,080 Speaker 1: Not very many. There was the guy who got the 925 00:44:31,120 --> 00:44:36,000 Speaker 1: Nobel Prize for his PhD work. He discovered the binary pulsars, 926 00:44:36,000 --> 00:44:39,640 Speaker 1: which were an excellent test of general relativity. A fascinating 927 00:44:39,680 --> 00:44:41,680 Speaker 1: story there is that he did this work as a 928 00:44:41,719 --> 00:44:45,360 Speaker 1: PhD student. It wasn't really understood or appreciated at the time, 929 00:44:45,680 --> 00:44:48,280 Speaker 1: so he actually left the field, then won the Nobel 930 00:44:48,320 --> 00:44:50,480 Speaker 1: Prize and ended up coming back and getting to do 931 00:44:50,520 --> 00:44:52,080 Speaker 1: more research. So that's pretty fun. 932 00:44:52,360 --> 00:44:54,520 Speaker 5: He was like selling cars and then he suddenly gets 933 00:44:54,520 --> 00:44:55,000 Speaker 5: a call. 934 00:44:56,040 --> 00:44:58,400 Speaker 1: Not quite that far. He was working in the computing division, 935 00:44:58,400 --> 00:45:00,640 Speaker 1: I think at Princeton, and then he won the Nobel 936 00:45:00,680 --> 00:45:02,400 Speaker 1: Prize and they called them up and they were like, so, 937 00:45:02,760 --> 00:45:04,120 Speaker 1: how big an office would you like? 938 00:45:04,920 --> 00:45:07,359 Speaker 5: Yeah, it's weird to kind of peak that early in 939 00:45:07,440 --> 00:45:11,279 Speaker 5: your career, right, Although Marie kept going. She won a 940 00:45:11,320 --> 00:45:14,239 Speaker 5: second Nobel Prize, and even her daughter won one too. 941 00:45:14,480 --> 00:45:17,680 Speaker 1: Yes, her daughter and her daughter's husband worked together again 942 00:45:17,800 --> 00:45:22,000 Speaker 1: on radiation and they induced artificial radioactivity. They took an 943 00:45:22,040 --> 00:45:25,480 Speaker 1: element which was not radioactive, a lunum, and then bombarded 944 00:45:25,520 --> 00:45:29,520 Speaker 1: it with radiation and they made it radioactive. And so 945 00:45:29,600 --> 00:45:31,640 Speaker 1: that was a pretty interesting discovery and they won the 946 00:45:31,640 --> 00:45:34,640 Speaker 1: Nobel Prize in nineteen thirty five. So there's a lot 947 00:45:34,680 --> 00:45:37,440 Speaker 1: of Nobel Prizes in the Curee family, all right. 948 00:45:37,480 --> 00:45:40,879 Speaker 5: Well, then at this point, I guess radiation is pretty 949 00:45:40,960 --> 00:45:43,799 Speaker 5: much discovered. I mean we sort of that point. They 950 00:45:43,840 --> 00:45:46,880 Speaker 5: knew about X rays and then also about kind of 951 00:45:47,000 --> 00:45:49,960 Speaker 5: particle radiation coming from the nucleus. 952 00:45:50,000 --> 00:45:52,920 Speaker 1: Yeah, and everybody thought that radiation came from stuff, right. 953 00:45:52,960 --> 00:45:56,160 Speaker 1: We had found it in ores from metals deep within 954 00:45:56,160 --> 00:45:58,880 Speaker 1: the earth, and so people thought, well, if there's radiation 955 00:45:59,120 --> 00:46:02,719 Speaker 1: around from the ground beneath us. So people thought if 956 00:46:02,719 --> 00:46:06,280 Speaker 1: you went higher up, like higher altitude, the radiation should decrease, 957 00:46:06,360 --> 00:46:08,319 Speaker 1: right because you're further away from the Earth and all 958 00:46:08,400 --> 00:46:11,960 Speaker 1: these sources of radiation. But people who did measurements found 959 00:46:11,960 --> 00:46:14,480 Speaker 1: something really strange. They found that as you went up 960 00:46:14,520 --> 00:46:17,600 Speaker 1: to the tops of mountains, the amount of radiation seemed 961 00:46:17,640 --> 00:46:20,960 Speaker 1: to be increasing, and that was weird and surprising to people. 962 00:46:20,800 --> 00:46:23,360 Speaker 5: Right, Yeah, that's when we discovered cosmic radiation. 963 00:46:23,560 --> 00:46:28,040 Speaker 1: Yeah, exactly. So there's this wonderfully hilarious pioneering physicist named 964 00:46:28,120 --> 00:46:31,160 Speaker 1: Victor Hess. This guy was born in a castle and 965 00:46:31,200 --> 00:46:34,560 Speaker 1: his father was a royal forester to a prince, and 966 00:46:34,680 --> 00:46:37,799 Speaker 1: he did these amazing experiments where he went up on 967 00:46:37,880 --> 00:46:42,040 Speaker 1: a balloon with his equipment. He improved on Pierre's electroscope 968 00:46:42,160 --> 00:46:45,000 Speaker 1: to measure like ionization due to radiation, and he went 969 00:46:45,080 --> 00:46:46,920 Speaker 1: up on balloons. But you couldn't just like send up 970 00:46:46,920 --> 00:46:49,000 Speaker 1: the balloon and then get the data later right like 971 00:46:49,040 --> 00:46:50,680 Speaker 1: the way we do now, because there's no way to 972 00:46:50,760 --> 00:46:53,720 Speaker 1: record this information. So he actually went on these balloon 973 00:46:53,719 --> 00:46:56,920 Speaker 1: ships himself, like sometimes up at night, really high in 974 00:46:56,920 --> 00:47:01,080 Speaker 1: the atmosphere, a great personal risk. But he discovered that 975 00:47:01,200 --> 00:47:03,960 Speaker 1: as you went up higher and higher, even above mountaintops, 976 00:47:04,120 --> 00:47:07,600 Speaker 1: the amount of radiation increased dramatically. So this point is 977 00:47:07,640 --> 00:47:10,360 Speaker 1: something really new and interesting that most of the radiation 978 00:47:10,480 --> 00:47:13,200 Speaker 1: that we were feeling around us wasn't coming from the 979 00:47:13,239 --> 00:47:16,240 Speaker 1: earth beneath us, but from the skies above us. Wow. 980 00:47:16,360 --> 00:47:18,759 Speaker 5: I guess once you sort of understand that there are 981 00:47:18,800 --> 00:47:22,760 Speaker 5: invisible you know, things flying around you coming from the earth, 982 00:47:22,880 --> 00:47:24,839 Speaker 5: and kind of makes you wonder where else are these 983 00:47:24,840 --> 00:47:27,400 Speaker 5: things coming from? Or where else can you find them exactly? 984 00:47:27,440 --> 00:47:29,680 Speaker 1: And every time you discover a new way to look 985 00:47:29,719 --> 00:47:32,880 Speaker 1: at the universe, you are bound to find something surprising. 986 00:47:33,239 --> 00:47:35,759 Speaker 1: So discovery of radiation not just showed us what was 987 00:47:35,840 --> 00:47:38,400 Speaker 1: inside the atom and helped us see inside our bodies, 988 00:47:38,520 --> 00:47:40,799 Speaker 1: it also helped us see the universe in a new 989 00:47:40,800 --> 00:47:43,759 Speaker 1: way and to see really really bright sources of this 990 00:47:43,960 --> 00:47:46,920 Speaker 1: new kind of information, and most of it was coming 991 00:47:46,920 --> 00:47:49,640 Speaker 1: from space, and so that was a big question mark 992 00:47:49,719 --> 00:47:53,320 Speaker 1: for decades, like what is making radiation out in space 993 00:47:53,400 --> 00:47:55,840 Speaker 1: and shooting it at us? And that's an area of 994 00:47:55,880 --> 00:47:58,160 Speaker 1: research still today, Like we understand a lot of the 995 00:47:58,200 --> 00:48:00,680 Speaker 1: source of that cosmic radiation now, but not all of it. 996 00:48:00,760 --> 00:48:02,839 Speaker 5: Right, Yeah, it's a big mystery. It's like it could 997 00:48:02,880 --> 00:48:03,440 Speaker 5: be anything. 998 00:48:03,680 --> 00:48:06,160 Speaker 1: Yeah, at the time, people really didn't understand. Now we 999 00:48:06,239 --> 00:48:08,239 Speaker 1: know that a lot of that radiation comes from the Sun, 1000 00:48:08,320 --> 00:48:10,760 Speaker 1: it's the solar wind, and it also comes from outside 1001 00:48:10,760 --> 00:48:13,400 Speaker 1: our solar system, from the galaxy, from the black hole 1002 00:48:13,480 --> 00:48:15,480 Speaker 1: at the center of the Milky Wave, for example, emits 1003 00:48:15,480 --> 00:48:17,520 Speaker 1: a lot of radiation, and other crazy stuff out there 1004 00:48:17,560 --> 00:48:20,440 Speaker 1: emits radiation. But there's still a lots of this radiation 1005 00:48:20,520 --> 00:48:22,919 Speaker 1: from space that we do not understand. The very very 1006 00:48:23,239 --> 00:48:26,680 Speaker 1: high energy particles very tip of that spectrum are higher 1007 00:48:26,760 --> 00:48:30,359 Speaker 1: energy than anything we understand can make. So radiation is 1008 00:48:30,440 --> 00:48:33,280 Speaker 1: still telling us about the universe and giving us clues 1009 00:48:33,320 --> 00:48:35,160 Speaker 1: about things out there that we don't know about. 1010 00:48:35,760 --> 00:48:38,000 Speaker 5: I'm guessing the scientist just wanted a better view out 1011 00:48:38,040 --> 00:48:39,560 Speaker 5: of his lab, so he's like, I'm gonna put it 1012 00:48:39,560 --> 00:48:40,080 Speaker 5: out a balloon. 1013 00:48:41,200 --> 00:48:43,239 Speaker 1: Yeah, I don't know. Or maybe he needed a break 1014 00:48:43,239 --> 00:48:45,200 Speaker 1: from whatever was going on in his life and he 1015 00:48:45,360 --> 00:48:47,000 Speaker 1: just needed an excuse to take a flight. 1016 00:48:47,440 --> 00:48:50,960 Speaker 5: In this castle. Too much castle drama. It's I'm hoping 1017 00:48:50,960 --> 00:48:52,520 Speaker 5: on my balloon to do signs. 1018 00:48:52,239 --> 00:48:54,160 Speaker 1: As we all do. If they ad made a reality 1019 00:48:54,160 --> 00:48:56,200 Speaker 1: show about it, that would have been the dramatic ending 1020 00:48:56,239 --> 00:48:58,360 Speaker 1: to an episode as he floats away in his balloon. 1021 00:48:59,040 --> 00:49:01,600 Speaker 5: All right. Well, I think it's just a really interesting 1022 00:49:02,239 --> 00:49:05,799 Speaker 5: kind of view into how we came to see that 1023 00:49:05,840 --> 00:49:08,160 Speaker 5: there are a lot of things that we can see, right, 1024 00:49:08,560 --> 00:49:10,680 Speaker 5: because how else would you know that there's things there 1025 00:49:10,680 --> 00:49:12,399 Speaker 5: if you can't see them or hear them. 1026 00:49:12,520 --> 00:49:14,319 Speaker 1: Yeah, And this is a pattern in physics that we 1027 00:49:14,520 --> 00:49:18,279 Speaker 1: keep discovering that their entire segments of the universe we 1028 00:49:18,320 --> 00:49:21,120 Speaker 1: didn't know anything about because for a long time they 1029 00:49:21,120 --> 00:49:24,640 Speaker 1: were invisible to us. The discovery of dark matter, for example, 1030 00:49:24,880 --> 00:49:26,719 Speaker 1: we know that dark matter is out there, it's all 1031 00:49:26,760 --> 00:49:30,000 Speaker 1: around us, it's streaming everywhere. It contains vast amounts of 1032 00:49:30,000 --> 00:49:32,960 Speaker 1: information about what's going on in the universe and how 1033 00:49:32,960 --> 00:49:34,840 Speaker 1: it was born and how it came to be, and 1034 00:49:34,880 --> 00:49:38,000 Speaker 1: we only recently discovered it exists and that tells us 1035 00:49:38,000 --> 00:49:41,040 Speaker 1: that there's almost certainly more stuff going on that we 1036 00:49:41,120 --> 00:49:44,080 Speaker 1: haven't yet cracked open and we haven't discovered that will 1037 00:49:44,080 --> 00:49:47,359 Speaker 1: tell future physicists crazy things about the universe that we 1038 00:49:47,400 --> 00:49:48,759 Speaker 1: cannot yet even anticipate. 1039 00:49:48,960 --> 00:49:51,680 Speaker 5: Yeah, and it kind of also reminds you that physics 1040 00:49:51,719 --> 00:49:54,720 Speaker 5: can be dangerous, you know, like you're probing the unknown, 1041 00:49:54,800 --> 00:49:58,520 Speaker 5: you're exposing yourself to things yet you don't know whether 1042 00:49:58,640 --> 00:50:00,600 Speaker 5: or not they exist or not or what through drink 1043 00:50:00,680 --> 00:50:01,560 Speaker 5: your body. 1044 00:50:01,320 --> 00:50:03,760 Speaker 1: Right, that's right. I've eaten a lot of very dangerous 1045 00:50:03,800 --> 00:50:05,680 Speaker 1: airline food and all of my trips to the Large 1046 00:50:05,719 --> 00:50:06,440 Speaker 1: Hadron Collider. 1047 00:50:06,520 --> 00:50:10,480 Speaker 5: So yeah, your ashes were probably glow too, Daniel. All 1048 00:50:10,520 --> 00:50:13,440 Speaker 5: that Swiss teas that you're eating, it's probably redoactive. 1049 00:50:13,680 --> 00:50:16,440 Speaker 1: Yes, fondue is probably not good for you, Yeah, but 1050 00:50:16,480 --> 00:50:17,479 Speaker 1: it's delicious. Yeah. 1051 00:50:17,520 --> 00:50:20,880 Speaker 5: All right. Well, that's a pretty fascinating trip down science 1052 00:50:20,960 --> 00:50:21,920 Speaker 5: history lane. 1053 00:50:21,640 --> 00:50:23,480 Speaker 1: And I hope it encourages all of you who are 1054 00:50:23,520 --> 00:50:26,360 Speaker 1: curious about things we don't understand, things we have not 1055 00:50:26,440 --> 00:50:29,560 Speaker 1: yet unraveled, to follow up those threads. If you see 1056 00:50:29,560 --> 00:50:32,239 Speaker 1: something you don't understand, try to figure it out. Something 1057 00:50:32,280 --> 00:50:35,640 Speaker 1: doesn't make sense to you, ask yourself questions until it does. 1058 00:50:35,680 --> 00:50:38,920 Speaker 1: Because remember that the history of science is just people 1059 00:50:38,960 --> 00:50:42,120 Speaker 1: being curious, trying to figure stuff out, and pushing forward 1060 00:50:42,160 --> 00:50:43,720 Speaker 1: on the envelope of human knowledge. 1061 00:50:43,840 --> 00:50:46,399 Speaker 5: Right, yeah, you too can win a Nobel Prize even 1062 00:50:46,440 --> 00:50:49,040 Speaker 5: if you get kicked out of high school for drawing cartoons. 1063 00:50:50,760 --> 00:50:52,040 Speaker 1: That's not an exaggeration. 1064 00:50:52,200 --> 00:50:54,279 Speaker 5: All right, Well, we hope you enjoyed that. Thanks for 1065 00:50:54,360 --> 00:50:56,160 Speaker 5: joining us, See you next time. 1066 00:51:03,960 --> 00:51:06,760 Speaker 1: Thanks for listening, and remember that Daniel and Jorge Explain 1067 00:51:06,800 --> 00:51:10,799 Speaker 1: the Universe is a production of iHeartRadio. For more podcasts 1068 00:51:10,800 --> 00:51:15,480 Speaker 1: from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, or wherever 1069 00:51:15,520 --> 00:51:29,840 Speaker 1: you listen to your favorite shows. When you pop a 1070 00:51:29,840 --> 00:51:32,160 Speaker 1: piece of cheese into your mouth, you're probably not thinking 1071 00:51:32,160 --> 00:51:35,080 Speaker 1: about the environmental impact. But the people in the dairy 1072 00:51:35,080 --> 00:51:38,239 Speaker 1: industry are. That's why they're working hard every day to 1073 00:51:38,280 --> 00:51:41,319 Speaker 1: find new ways to reduce waste, conserve natural resources, and 1074 00:51:41,440 --> 00:51:46,240 Speaker 1: drive down greenhouse gas emissions. House US dairy tackling greenhouse gases. 1075 00:51:46,560 --> 00:51:49,640 Speaker 1: Many farms use anaerobic digestors to turn the methane from 1076 00:51:49,680 --> 00:51:53,640 Speaker 1: manure into renewable energy that can power farms, towns, and 1077 00:51:53,800 --> 00:51:57,680 Speaker 1: electric cars. Visit you as dairy dot COM's last sustainability 1078 00:51:57,719 --> 00:51:58,520 Speaker 1: to learn more. 1079 00:52:00,080 --> 00:52:03,439 Speaker 9: There are children, friends, and families walking, riding on paths 1080 00:52:03,480 --> 00:52:05,960 Speaker 9: and roads every day. Remember they're real people with loved 1081 00:52:06,000 --> 00:52:08,160 Speaker 9: ones who need them to get home safely. Protect our 1082 00:52:08,200 --> 00:52:11,719 Speaker 9: cyclists and pedestrians because they're people too, Go safely California 1083 00:52:11,760 --> 00:52:14,080 Speaker 9: from the California Office of Traffic Safety and Caltrans. 1084 00:52:14,239 --> 00:52:17,440 Speaker 3: Hey, their fellow globetrotters and destination dreamers. If you're anything 1085 00:52:17,520 --> 00:52:19,720 Speaker 3: like us, you'd note that life's too short for boring 1086 00:52:19,760 --> 00:52:20,800 Speaker 3: toasters and towels. 1087 00:52:20,880 --> 00:52:23,800 Speaker 2: That's why we decided to ditch the traditional wedding registry 1088 00:52:23,840 --> 00:52:26,600 Speaker 2: and went with honeyfund dot com. 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