1 00:00:08,520 --> 00:00:11,920 Speaker 1: Hey, Katie, what's the biggest thing that you've ever seen 2 00:00:12,200 --> 00:00:12,760 Speaker 1: blow up? 3 00:00:12,920 --> 00:00:17,560 Speaker 2: Technically soup that I microwaved too high, But I've always 4 00:00:17,560 --> 00:00:19,800 Speaker 2: wanted to see one of those building demolitions. 5 00:00:20,079 --> 00:00:22,000 Speaker 1: Oh, that does sound fun. I'd love to see you 6 00:00:22,040 --> 00:00:24,840 Speaker 1: blow up soup or watch a building get exploded. I 7 00:00:24,880 --> 00:00:26,880 Speaker 1: wonder if they sell tickets to those events. 8 00:00:27,160 --> 00:00:29,000 Speaker 2: I hope they go on tour, and I hope they 9 00:00:29,000 --> 00:00:33,000 Speaker 2: come to my city. What about you, what is the 10 00:00:33,040 --> 00:00:35,120 Speaker 2: biggest explosion that you have seen? 11 00:00:35,680 --> 00:00:37,720 Speaker 1: Well, there was the time that I made a strawberry 12 00:00:37,720 --> 00:00:40,760 Speaker 1: smoothie without putting a lid on the blender and I'm 13 00:00:40,880 --> 00:00:44,680 Speaker 1: still cleaning up strawberry in the kitchen years later. But 14 00:00:44,960 --> 00:00:47,800 Speaker 1: I did once see a shoe store explode when an 15 00:00:47,800 --> 00:00:51,120 Speaker 1: air and firework hitted on New Year's Eve. It was crazy. 16 00:00:51,159 --> 00:00:53,080 Speaker 1: You could feel the heat from blocks away. 17 00:00:53,440 --> 00:00:57,200 Speaker 2: That's crazy, that's amazing. I'm sure you were going to 18 00:00:57,280 --> 00:00:59,360 Speaker 2: say something more dramatic, though. 19 00:00:59,320 --> 00:01:02,040 Speaker 1: More dramatic than a flaming shoes door, but. 20 00:01:02,080 --> 00:01:05,000 Speaker 2: I thought so you grew up in Los Alamos, Like, 21 00:01:05,319 --> 00:01:07,839 Speaker 2: isn't that the home of the atomic bomb? 22 00:01:08,160 --> 00:01:10,520 Speaker 1: It is, but we don't just like set them off 23 00:01:10,560 --> 00:01:11,960 Speaker 1: on holidays. 24 00:01:12,880 --> 00:01:13,880 Speaker 2: That seems like a shame. 25 00:01:14,400 --> 00:01:15,959 Speaker 1: I guess you could say we've kind of blown it. 26 00:01:18,240 --> 00:01:35,679 Speaker 2: You didn't blew it, and that's the problem. 27 00:01:35,840 --> 00:01:38,840 Speaker 1: Hi. I'm Daniel. I'm a particle physicist and a professor 28 00:01:38,920 --> 00:01:41,839 Speaker 1: at UC Irvine, and I hope to never be near 29 00:01:42,040 --> 00:01:43,280 Speaker 1: a nuclear explosion. 30 00:01:43,480 --> 00:01:47,520 Speaker 2: I am Katie Golden. I host the podcast Creature Feature, 31 00:01:47,840 --> 00:01:56,200 Speaker 2: and I hope there's never a nuclear explosion anywhere ever, space, Earth, 32 00:01:56,320 --> 00:01:58,760 Speaker 2: what have you? It seems like a bad sign of 33 00:01:58,840 --> 00:01:59,520 Speaker 2: things to come. 34 00:01:59,680 --> 00:02:02,560 Speaker 1: Are you saying that nukes can never be used for good? 35 00:02:02,880 --> 00:02:06,520 Speaker 1: You're not aware of the Peacetime nuclear weapons program or 36 00:02:06,560 --> 00:02:10,400 Speaker 1: the design of the Orion spaceship, which literally uses nuclear 37 00:02:10,440 --> 00:02:13,320 Speaker 1: weapons blowing up behind it in order to propel it forward. 38 00:02:13,680 --> 00:02:17,520 Speaker 2: I mean, if you're basically gonna do big space farts 39 00:02:17,760 --> 00:02:20,959 Speaker 2: with nukes to make your spaceship go, I'll make an exception. 40 00:02:22,120 --> 00:02:25,160 Speaker 1: All right. We have already broken down your barriers here 41 00:02:25,919 --> 00:02:29,120 Speaker 1: and so welcome to the podcast. Daniel and Jorge Explain 42 00:02:29,200 --> 00:02:32,600 Speaker 1: the Universe, a production of iHeartRadio in which we dive 43 00:02:32,760 --> 00:02:35,720 Speaker 1: deep into everything that happens in the universe, how it 44 00:02:35,760 --> 00:02:38,639 Speaker 1: all works, how it all began, how it all might end, 45 00:02:38,960 --> 00:02:42,079 Speaker 1: and how humans might bring about their own demise. 46 00:02:42,480 --> 00:02:46,480 Speaker 2: I'm a big fan of life on Earth. I love 47 00:02:46,639 --> 00:02:49,640 Speaker 2: all the animals on Earth, love all the plants, and 48 00:02:49,680 --> 00:02:52,600 Speaker 2: the humans, most of them, ninety nine percent of humans. 49 00:02:53,160 --> 00:02:56,960 Speaker 2: And you know, I have a lot of nuclear anxiety 50 00:02:57,520 --> 00:03:00,280 Speaker 2: when it comes to the planet Earth, because I don't 51 00:03:00,280 --> 00:03:04,240 Speaker 2: want one going off and you know, destroying a bunch 52 00:03:04,280 --> 00:03:08,480 Speaker 2: of stuff, radiating things, maybe causing a new ice age 53 00:03:09,000 --> 00:03:12,720 Speaker 2: with the clouds of debris. But I guess if it's 54 00:03:12,960 --> 00:03:16,160 Speaker 2: blown up in space, I'm a little less worried. 55 00:03:16,360 --> 00:03:19,280 Speaker 1: Well, this to me is a really interesting area because 56 00:03:19,400 --> 00:03:22,880 Speaker 1: it brings together the sort of fascinating progress we make 57 00:03:22,960 --> 00:03:25,400 Speaker 1: in physics as we start to understand the way the 58 00:03:25,520 --> 00:03:28,680 Speaker 1: universe works, what the forces are that underlie everything, how 59 00:03:28,720 --> 00:03:32,240 Speaker 1: they weave themselves together to make our reality. Understanding that 60 00:03:32,440 --> 00:03:35,040 Speaker 1: also gives us new power, the power to use that 61 00:03:35,120 --> 00:03:38,520 Speaker 1: knowledge to develop new technologies, which of course can be 62 00:03:38,600 --> 00:03:41,640 Speaker 1: good in peace time, like transistors and iPhones, but also 63 00:03:41,720 --> 00:03:44,680 Speaker 1: can be used to make weapons of mass destruction that 64 00:03:44,720 --> 00:03:48,400 Speaker 1: are pointed at civilian populations for political gain. And so, 65 00:03:48,600 --> 00:03:51,280 Speaker 1: while we like on this podcast to think about the 66 00:03:51,280 --> 00:03:54,640 Speaker 1: physics side of it, the scientific edge of knowledge, how 67 00:03:54,640 --> 00:03:57,480 Speaker 1: we can always push that forward, and we generally think 68 00:03:57,520 --> 00:04:01,520 Speaker 1: about that knowledge as purely good as sausfying our curiosity 69 00:04:01,560 --> 00:04:05,320 Speaker 1: is scratching our itch that wonders about how the universe works. 70 00:04:05,400 --> 00:04:08,080 Speaker 1: It's not possible to really live in a bubble and 71 00:04:08,120 --> 00:04:11,400 Speaker 1: pretend that that knowledge can't be used in all sorts 72 00:04:11,440 --> 00:04:13,800 Speaker 1: of ways that the original scientists who worked on it 73 00:04:13,840 --> 00:04:16,520 Speaker 1: aren't in control of. Personally, I did grow up in 74 00:04:16,560 --> 00:04:19,280 Speaker 1: Los Alamo's home in the Manhattan Project in Los Almos 75 00:04:19,400 --> 00:04:23,200 Speaker 1: National Laboratory, where weapons projects are ongoing to this day, 76 00:04:23,360 --> 00:04:25,440 Speaker 1: and both of my parents worked at the lab and 77 00:04:25,520 --> 00:04:28,919 Speaker 1: worked on weapons related projects. What exactly they did, I 78 00:04:28,960 --> 00:04:31,400 Speaker 1: don't know. I didn't know. I will never know, because 79 00:04:31,440 --> 00:04:35,000 Speaker 1: I don't have particular rants to know such secrets. But 80 00:04:35,160 --> 00:04:38,320 Speaker 1: such power over the universe comes with real responsibility. 81 00:04:38,520 --> 00:04:41,640 Speaker 2: Yeah, I think I remember that a lot of these 82 00:04:41,720 --> 00:04:45,760 Speaker 2: scientists who worked on the Manhattan Project became very anti 83 00:04:46,120 --> 00:04:49,760 Speaker 2: nuclear proliferation. You know. It's it's something that I think 84 00:04:49,800 --> 00:04:54,560 Speaker 2: people who really understand the devastating power of nukes also 85 00:04:54,720 --> 00:05:00,359 Speaker 2: are very much opposed to uncontrolled proliferation of dukes. I 86 00:05:00,360 --> 00:05:03,880 Speaker 2: don't think it's something where scientists are There's a bunch 87 00:05:03,880 --> 00:05:06,200 Speaker 2: of mad scientists who really just want to blow up 88 00:05:06,240 --> 00:05:08,360 Speaker 2: the planet. I think most of the scientists who really 89 00:05:08,440 --> 00:05:13,600 Speaker 2: understand this stuff are also probably pretty anxious and would 90 00:05:13,720 --> 00:05:15,320 Speaker 2: like a world with fewer nukes. 91 00:05:15,560 --> 00:05:18,159 Speaker 1: Yeah. Absolutely, I do know that my mother worked on 92 00:05:18,240 --> 00:05:22,360 Speaker 1: nuclear non proliferation programs, ways that you can detect nuclear 93 00:05:22,400 --> 00:05:25,120 Speaker 1: fuel and nuclear explosions, et cetera. But my father definitely 94 00:05:25,160 --> 00:05:27,120 Speaker 1: worked on the weapons side of it. And I asked 95 00:05:27,160 --> 00:05:29,920 Speaker 1: him once, not, of course, like tell me some nuclear secrets, 96 00:05:30,160 --> 00:05:33,600 Speaker 1: but how do you feel about working on the design 97 00:05:33,920 --> 00:05:36,760 Speaker 1: of huge weapons that are in the end pointed at 98 00:05:36,800 --> 00:05:40,960 Speaker 1: civilian populations. And you know, back in the eighties when 99 00:05:40,960 --> 00:05:43,000 Speaker 1: he started that job, it was a different era. We 100 00:05:43,000 --> 00:05:47,680 Speaker 1: were still in the Cold War and developing our nuclear capabilities. 101 00:05:47,760 --> 00:05:50,600 Speaker 1: Sort of felt patriotic. Back then, it felt like, Hey, 102 00:05:50,600 --> 00:05:53,600 Speaker 1: you're contributing to your country, you're protecting us, you're defending us. 103 00:05:53,640 --> 00:05:55,840 Speaker 1: I'm not saying that it's morally crisp and clean. I 104 00:05:55,839 --> 00:05:58,200 Speaker 1: certainly chose to do particle physics because it has no 105 00:05:58,320 --> 00:06:02,280 Speaker 1: weapons applications, and nobody's ever use my research to kill anybody. 106 00:06:02,440 --> 00:06:06,359 Speaker 2: Not yet, they haven't yet. Give me a pen and 107 00:06:06,400 --> 00:06:09,240 Speaker 2: a piece of paper, I'll come up with something that's. 108 00:06:09,080 --> 00:06:13,000 Speaker 1: Right, The Higgs Boson bomb by Katie goldd Well. Nuclear 109 00:06:13,040 --> 00:06:15,360 Speaker 1: weapons are very powerful and very dangerous, and they have 110 00:06:15,440 --> 00:06:18,360 Speaker 1: also captured the public imagination and I get a lot 111 00:06:18,400 --> 00:06:21,760 Speaker 1: of interest in our podcast email box about nuclear weapons. 112 00:06:21,800 --> 00:06:24,159 Speaker 1: People wonder what would happen if you dropped the nuclear 113 00:06:24,160 --> 00:06:26,640 Speaker 1: weapon into the Sun, or could we really use nuclear 114 00:06:26,680 --> 00:06:29,640 Speaker 1: weapons to blow up the polar ice caps on Mars 115 00:06:29,640 --> 00:06:32,680 Speaker 1: and to make more atmosphere? Or what exactly happens when 116 00:06:32,720 --> 00:06:35,560 Speaker 1: you drop a nuclear weapon in X? Basically I get 117 00:06:35,560 --> 00:06:38,920 Speaker 1: these questions where X is anything? And so we're starting 118 00:06:38,920 --> 00:06:42,000 Speaker 1: a new series of podcasts titled what Happens if You 119 00:06:42,040 --> 00:06:44,720 Speaker 1: Explode a Nuke in Blank? And we're going to explore 120 00:06:44,800 --> 00:06:47,400 Speaker 1: everywhere you can imagine putting a nuclear weapon. 121 00:06:47,680 --> 00:06:50,159 Speaker 2: So today, where are we exploding that nuke? 122 00:06:50,360 --> 00:06:52,120 Speaker 1: Well, we're not putting that nuke in any sort of 123 00:06:52,240 --> 00:06:56,160 Speaker 1: biological locations. We're mostly going to focus on the physics locations. 124 00:06:56,480 --> 00:06:58,800 Speaker 1: And today on the podcast, we'll be answering the question 125 00:07:03,920 --> 00:07:07,640 Speaker 1: what happens if you explode a nuke in space? 126 00:07:08,160 --> 00:07:12,240 Speaker 2: So we are definitely cordoning off any of the space whales, 127 00:07:12,320 --> 00:07:15,360 Speaker 2: any of the space jellyfish, any kind of free floating 128 00:07:15,480 --> 00:07:19,679 Speaker 2: space creatures that might be in the way of this nuke, 129 00:07:19,800 --> 00:07:23,800 Speaker 2: and presumably we're exploding it just in space space right 130 00:07:23,920 --> 00:07:28,080 Speaker 2: like where there's not too much around, just pure. 131 00:07:28,920 --> 00:07:33,239 Speaker 1: Space, just pure space exactly. And I think this question 132 00:07:33,320 --> 00:07:36,440 Speaker 1: is super fascinating from a scientific point of view, because 133 00:07:36,480 --> 00:07:38,920 Speaker 1: mostly what we know and what we imagine about nuclear 134 00:07:38,960 --> 00:07:41,560 Speaker 1: weapons comes from the interaction of the nuclear blast with 135 00:07:41,680 --> 00:07:45,400 Speaker 1: the atmosphere or with the Earth, those shockwaves, and that 136 00:07:45,440 --> 00:07:47,720 Speaker 1: doesn't happen in space. So we'll go in detail through 137 00:07:48,040 --> 00:07:50,880 Speaker 1: exactly what does happen in a nuclear explosion and how 138 00:07:50,920 --> 00:07:54,000 Speaker 1: that propagates through space when it's not surrounded by a 139 00:07:54,000 --> 00:07:57,640 Speaker 1: cocoon of air. This also the really fascinating political and 140 00:07:57,680 --> 00:08:00,000 Speaker 1: sort of militaristic side of it, as humanity tries to 141 00:08:00,200 --> 00:08:04,200 Speaker 1: build a space based civilization. Space war is a big question, 142 00:08:04,560 --> 00:08:07,120 Speaker 1: and so like understanding what happens when you blow up 143 00:08:07,120 --> 00:08:09,960 Speaker 1: a nuke in space from a sort of political or 144 00:08:10,080 --> 00:08:13,720 Speaker 1: military strategic point of view is also really interesting and important. 145 00:08:14,200 --> 00:08:18,440 Speaker 2: Could we go somewhere in the universe and not put 146 00:08:18,600 --> 00:08:19,760 Speaker 2: wars in there? 147 00:08:20,920 --> 00:08:22,960 Speaker 1: I think only if we don't bring the humans right, 148 00:08:22,960 --> 00:08:24,640 Speaker 1: the wars come with the humans. 149 00:08:25,800 --> 00:08:28,480 Speaker 2: I think only puppies should go to space so that 150 00:08:28,560 --> 00:08:29,640 Speaker 2: don't start any wars. 151 00:08:29,840 --> 00:08:32,160 Speaker 1: But that's also a really fascinating question. You see in 152 00:08:32,160 --> 00:08:34,839 Speaker 1: a lot of science fiction novels human civilization spread out 153 00:08:34,840 --> 00:08:37,120 Speaker 1: through the galaxy, or humans and aliens spread out through 154 00:08:37,120 --> 00:08:40,440 Speaker 1: the galaxy able to access all these vast resources, and 155 00:08:40,520 --> 00:08:44,320 Speaker 1: yet still fighting right, still having wars, and I wonder 156 00:08:44,360 --> 00:08:46,520 Speaker 1: if that's really true. I often pose that question to 157 00:08:46,559 --> 00:08:49,280 Speaker 1: our science fiction author guests, like, what are these people 158 00:08:49,320 --> 00:08:53,800 Speaker 1: fighting about? There's essentially limitless resources. Like you want water, 159 00:08:54,040 --> 00:08:57,400 Speaker 1: go to Neptune, it's basically a planet of water. You 160 00:08:57,440 --> 00:09:01,400 Speaker 1: want gold, there's like enormous blobs gold out there. Platinum 161 00:09:01,440 --> 00:09:04,080 Speaker 1: like this asteroid's made of platinum. If you need something, 162 00:09:04,200 --> 00:09:06,559 Speaker 1: don't come kill us for it, just go get it. 163 00:09:06,720 --> 00:09:08,760 Speaker 1: If you want energy, like the Sun is out there 164 00:09:08,880 --> 00:09:11,400 Speaker 1: dumping out energy, it seems to me that once you 165 00:09:11,520 --> 00:09:14,080 Speaker 1: make it to space, I don't know why people would 166 00:09:14,120 --> 00:09:16,840 Speaker 1: still be having wars unless they're just fundamentally grumpy. 167 00:09:18,440 --> 00:09:21,640 Speaker 2: That could be. I think that if you have resources 168 00:09:21,640 --> 00:09:25,760 Speaker 2: spread out relatively fairly, right, like you don't have a 169 00:09:25,880 --> 00:09:29,679 Speaker 2: space king that's hoarding all the Neptune water for himself, 170 00:09:30,200 --> 00:09:32,160 Speaker 2: that yeah, it would make sense that there would be 171 00:09:32,280 --> 00:09:35,680 Speaker 2: fewer wars because I think when people have a lot 172 00:09:35,679 --> 00:09:38,240 Speaker 2: of resources, they have a good quality of life, why 173 00:09:38,280 --> 00:09:39,920 Speaker 2: would they want to go to war? You know, what 174 00:09:40,000 --> 00:09:43,040 Speaker 2: would be the purpose for the everyday person to risk 175 00:09:43,120 --> 00:09:46,359 Speaker 2: it all for war? Again, if we have like space monarchies, 176 00:09:46,400 --> 00:09:47,840 Speaker 2: then yeah, there might be some wars. 177 00:09:48,000 --> 00:09:50,840 Speaker 1: Yeah. Well, there are some really interesting science fiction explorations 178 00:09:50,880 --> 00:09:53,320 Speaker 1: of this, like the Culture series and other like post 179 00:09:53,400 --> 00:09:57,160 Speaker 1: scarcity novels where basically everybody has everything they ever want. 180 00:09:57,240 --> 00:09:59,200 Speaker 1: You just ask for something and you get it, and 181 00:09:59,240 --> 00:10:02,240 Speaker 1: they explore like what would life be like in that situation. Anyway, 182 00:10:02,480 --> 00:10:04,920 Speaker 1: back to the topic of today's podcast, we are not 183 00:10:05,040 --> 00:10:07,840 Speaker 1: yet there. We are not yet in outer space living 184 00:10:07,880 --> 00:10:11,679 Speaker 1: among the riches where everybody gets their own platinum throne. Instead, 185 00:10:11,720 --> 00:10:13,760 Speaker 1: we're still down here on Earth and wondering what would 186 00:10:13,760 --> 00:10:16,640 Speaker 1: happen if you blew up a nuclear weapon in space? 187 00:10:16,960 --> 00:10:19,160 Speaker 1: And so, as usual, I pulled our listeners to hear 188 00:10:19,200 --> 00:10:22,520 Speaker 1: what they thought might happen in this scenario. If you 189 00:10:22,559 --> 00:10:25,400 Speaker 1: would like to participate in this segment of the podcast 190 00:10:25,440 --> 00:10:29,160 Speaker 1: giving your informed or uninformed answers for us to hear, 191 00:10:29,240 --> 00:10:31,679 Speaker 1: please don't be shy write to me two questions at 192 00:10:31,800 --> 00:10:35,120 Speaker 1: Danielandjorge dot com. So think about it for a minute. 193 00:10:35,120 --> 00:10:37,200 Speaker 1: Do you know what would happen if we blew up 194 00:10:37,240 --> 00:10:40,880 Speaker 1: a nuclear bomb in space? Here's what our listeners had 195 00:10:40,880 --> 00:10:42,520 Speaker 1: to say, probably. 196 00:10:42,120 --> 00:10:44,480 Speaker 3: Something very similar to what happens if you explode a 197 00:10:44,520 --> 00:10:47,440 Speaker 3: nuclear bomb not in space. A lot of energy is released. 198 00:10:47,880 --> 00:10:50,360 Speaker 3: Basically it's what the Sun is doing, so it's just 199 00:10:50,720 --> 00:10:52,960 Speaker 3: a bunch of energy pouring out into space. 200 00:10:53,160 --> 00:10:55,400 Speaker 4: I think that exploding a nucleipon in space would have 201 00:10:55,480 --> 00:10:58,400 Speaker 4: very little effect. It would be a pretty clean explosion. 202 00:10:58,840 --> 00:11:01,960 Speaker 4: If there're at some radio active particles, but there's loads 203 00:11:01,960 --> 00:11:05,280 Speaker 4: of them flying around in space anyway, so essentially I 204 00:11:05,320 --> 00:11:06,160 Speaker 4: have no concerns. 205 00:11:07,000 --> 00:11:07,480 Speaker 5: Go for it. 206 00:11:07,559 --> 00:11:10,640 Speaker 6: So if I understand right how a nuke works, it 207 00:11:10,800 --> 00:11:15,720 Speaker 6: requires a chain reaction between the atoms of our atmosphere, 208 00:11:15,960 --> 00:11:20,680 Speaker 6: So in deep space without atmosphere, it will have no effects. 209 00:11:21,080 --> 00:11:26,840 Speaker 7: You'd see a big, huge round flash, blinding flash of light, 210 00:11:26,920 --> 00:11:29,480 Speaker 7: and then you wouldn't hear anything, I guess because it's 211 00:11:29,520 --> 00:11:32,320 Speaker 7: the vacuum of space. And then as soon as all 212 00:11:32,360 --> 00:11:37,960 Speaker 7: the the fuel, the hydrogen was or uranium or plutonium 213 00:11:38,040 --> 00:11:41,959 Speaker 7: was gone, it should be done. And I don't think 214 00:11:41,960 --> 00:11:44,240 Speaker 7: it's any debris, because there's no like that start all 215 00:11:44,320 --> 00:11:44,800 Speaker 7: lighted up. 216 00:11:45,120 --> 00:11:48,480 Speaker 8: Is this an atomic bomb or a hydrogen bomb? I 217 00:11:48,520 --> 00:11:51,000 Speaker 8: think either way. I think you just make a tiny 218 00:11:51,000 --> 00:11:53,800 Speaker 8: little sun for a second, and then that much would happen, 219 00:11:53,800 --> 00:11:55,520 Speaker 8: except for some more radiation in space. 220 00:11:55,920 --> 00:11:59,440 Speaker 1: I assume it would just sort of do the same 221 00:11:59,480 --> 00:12:01,959 Speaker 1: thing it does here without a shock wave. 222 00:12:02,320 --> 00:12:05,040 Speaker 9: I believe that unless it's something close or it is 223 00:12:05,120 --> 00:12:08,480 Speaker 9: something to you know, to a planet, or maybe close 224 00:12:08,520 --> 00:12:11,680 Speaker 9: to I don't know, like a nebula, maybe it will 225 00:12:12,679 --> 00:12:15,600 Speaker 9: you know, push away that. But other than that, maybe 226 00:12:15,640 --> 00:12:18,080 Speaker 9: the only thing in space that will happen, if you know, 227 00:12:18,120 --> 00:12:20,880 Speaker 9: if it's in the vacuum space, it will create maybe 228 00:12:20,920 --> 00:12:24,320 Speaker 9: a little bit of a gravitational waves maybe, I don't know. 229 00:12:24,640 --> 00:12:27,520 Speaker 5: Well, you won't get a mushroom cloud, that's for sure, 230 00:12:27,520 --> 00:12:31,120 Speaker 5: because that only happens in the atmosphere. So when a 231 00:12:31,200 --> 00:12:36,439 Speaker 5: nuclear explosion happens, I believe that it releases basically lots 232 00:12:36,480 --> 00:12:38,719 Speaker 5: and lots of radiation in the form of photons and 233 00:12:40,120 --> 00:12:45,040 Speaker 5: the radioactive particles. So I imagine like a big bright 234 00:12:45,280 --> 00:12:49,920 Speaker 5: ball of light that will flash for a second and disappear. 235 00:12:50,360 --> 00:12:56,160 Speaker 10: I would suppose that the nuclear bomb would still explode, 236 00:12:56,440 --> 00:13:02,400 Speaker 10: and having nothing for the explosion too press back against. 237 00:13:02,440 --> 00:13:04,880 Speaker 10: I would expect that the explosion would be equal in 238 00:13:05,000 --> 00:13:09,679 Speaker 10: all directions, and that the residual matter would fly out 239 00:13:10,040 --> 00:13:11,160 Speaker 10: in all directions equally. 240 00:13:11,480 --> 00:13:16,080 Speaker 2: That's a lot of different answers, really interesting ideas. I 241 00:13:16,120 --> 00:13:18,200 Speaker 2: think the main thing people are thinking of, like it 242 00:13:18,280 --> 00:13:22,120 Speaker 2: in space, Right, you don't have atmosphere, you don't have air, 243 00:13:22,640 --> 00:13:24,680 Speaker 2: so you're not going to have the things that air 244 00:13:24,720 --> 00:13:29,720 Speaker 2: and atmosphere provides, like say a shock wave or sound. 245 00:13:30,080 --> 00:13:32,840 Speaker 1: Yeah, it's basically like a little sun in space. Is 246 00:13:32,880 --> 00:13:35,160 Speaker 1: a great little argument. There was somebody who said something 247 00:13:35,160 --> 00:13:38,600 Speaker 1: about how it requires a chain reaction in the atmosphere, 248 00:13:39,080 --> 00:13:41,320 Speaker 1: so in space it'll have no effect, which I think 249 00:13:41,440 --> 00:13:44,359 Speaker 1: might have some misunderstanding of how a nuclear weapon works. 250 00:13:44,600 --> 00:13:46,800 Speaker 1: But on the whole, yeah, these are great answers. 251 00:13:47,000 --> 00:13:51,200 Speaker 2: Well, how I think nuclear explosions work is you take 252 00:13:51,240 --> 00:13:54,080 Speaker 2: it at them and you get a little axe, very 253 00:13:54,080 --> 00:13:57,680 Speaker 2: sharp ax, and Y split it in half and that 254 00:13:58,160 --> 00:14:00,439 Speaker 2: releases a bunch of energy in floats. 255 00:14:00,720 --> 00:14:06,760 Speaker 1: Tell me I'm wrong, You're wrong, although you could be wronger, 256 00:14:07,000 --> 00:14:10,800 Speaker 1: I mean there is some elevation that is correct. Essentially, 257 00:14:10,800 --> 00:14:13,280 Speaker 1: there's two ways to make a nuclear explosion. One is 258 00:14:13,400 --> 00:14:17,160 Speaker 1: fission and one is fusion. Fission is when you're cracking 259 00:14:17,200 --> 00:14:20,080 Speaker 1: a big, heavy atom open. So you have like uranium 260 00:14:20,160 --> 00:14:23,240 Speaker 1: or something which already is on the verge of breaking apart, 261 00:14:23,320 --> 00:14:25,440 Speaker 1: and you take a little ax, which in this case 262 00:14:25,520 --> 00:14:28,120 Speaker 1: is a neutron, and you shoot it at the uranium 263 00:14:28,200 --> 00:14:30,960 Speaker 1: and it breaks open and it makes more neutrons, and 264 00:14:31,000 --> 00:14:34,680 Speaker 1: those neutrons fly out and hit other uranium atoms, which 265 00:14:34,760 --> 00:14:37,680 Speaker 1: then crack open and release energy and more neutrons, and 266 00:14:37,680 --> 00:14:40,440 Speaker 1: then you get this chain reaction. And so if your 267 00:14:40,520 --> 00:14:43,960 Speaker 1: axe is basically a tiny little neutron axe, then maybe 268 00:14:44,000 --> 00:14:46,600 Speaker 1: that works. And actually isn't. Thor's hammer supposed to be 269 00:14:46,600 --> 00:14:49,600 Speaker 1: made out of neutron star so there's already a precedent 270 00:14:49,640 --> 00:14:51,640 Speaker 1: there for like tools made of neutrons. 271 00:14:51,800 --> 00:14:56,160 Speaker 2: I knew Marvel was scientifically accurate in every way. That's 272 00:14:56,200 --> 00:14:59,920 Speaker 2: the fission part, where you have a bunch of un 273 00:15:00,080 --> 00:15:05,080 Speaker 2: stable large atoms being hacked apart by neutrons, and then 274 00:15:05,200 --> 00:15:08,000 Speaker 2: that interurn releases more neutrons than that hacks apart other 275 00:15:08,240 --> 00:15:13,000 Speaker 2: unstable atoms you've mentioned, though, there's a fusion one as well. 276 00:15:13,080 --> 00:15:16,080 Speaker 1: Yeah, exactly, so that's fission. And the design of a 277 00:15:16,080 --> 00:15:18,680 Speaker 1: fission bomb is actually quite interesting, like the way you 278 00:15:18,720 --> 00:15:20,520 Speaker 1: get that to blow up, because if you just have 279 00:15:20,600 --> 00:15:22,720 Speaker 1: a bunch of uraniums sitting around, it's not going to 280 00:15:22,760 --> 00:15:25,320 Speaker 1: have a chain reaction unless it has enough density, like 281 00:15:25,360 --> 00:15:27,560 Speaker 1: you pack those things dense enough, then it's going to 282 00:15:27,600 --> 00:15:29,840 Speaker 1: blow up. But what you want in a bomb is 283 00:15:29,840 --> 00:15:32,280 Speaker 1: something that blows up when you want it to, not 284 00:15:32,480 --> 00:15:34,840 Speaker 1: just like when you build it right. You want something 285 00:15:34,920 --> 00:15:38,200 Speaker 1: like a fuse, and so you need a controlled explosion. 286 00:15:38,440 --> 00:15:40,640 Speaker 1: And so what they do is they have two pieces 287 00:15:40,680 --> 00:15:43,920 Speaker 1: of uranium, both of which do not have enough mass 288 00:15:43,960 --> 00:15:47,280 Speaker 1: to blow they are subcritical masses. And then what happens 289 00:15:47,280 --> 00:15:49,640 Speaker 1: in the bomb is you basically smash those two together, 290 00:15:49,760 --> 00:15:52,840 Speaker 1: combine them together to make a super critical mass when 291 00:15:52,840 --> 00:15:56,359 Speaker 1: they can actually trigger this runaway effect and cause the explosion. 292 00:15:56,360 --> 00:15:58,400 Speaker 1: And sometimes they even have like a little trigger like 293 00:15:58,400 --> 00:16:01,640 Speaker 1: a pellet of polonium or rialium or something to get 294 00:16:01,680 --> 00:16:04,120 Speaker 1: the first neutrons going. But you're right, that's all fission. 295 00:16:04,280 --> 00:16:06,720 Speaker 1: And so the first bomb that was ever developed and 296 00:16:06,840 --> 00:16:10,360 Speaker 1: was blown up in Alamagordo, New Mexico, not too far 297 00:16:10,400 --> 00:16:12,760 Speaker 1: from where I grew up, was a fission bomb. But 298 00:16:12,760 --> 00:16:15,680 Speaker 1: there's another much more powerful nuclear process that we now 299 00:16:15,680 --> 00:16:18,240 Speaker 1: have a handle on, and that is fusion. Fusion is 300 00:16:18,240 --> 00:16:20,960 Speaker 1: the opposite. Instead of breaking up a big heavy atom 301 00:16:21,000 --> 00:16:24,440 Speaker 1: to release energy, you're sticking two light atoms together to 302 00:16:24,480 --> 00:16:27,520 Speaker 1: make a heavier one. So two protons, for example, come 303 00:16:27,560 --> 00:16:30,680 Speaker 1: together to make helium. It's actually a little bit more complicated. 304 00:16:30,840 --> 00:16:34,600 Speaker 1: You end up with like multiple protons making multiple helium nuclei. 305 00:16:34,920 --> 00:16:38,760 Speaker 1: But squeezing light atoms together to make heavier ones releases energy, 306 00:16:39,320 --> 00:16:42,400 Speaker 1: just like chopping up heavier atoms to make lighter ones 307 00:16:42,600 --> 00:16:43,480 Speaker 1: releases energy. 308 00:16:43,720 --> 00:16:46,680 Speaker 2: You mentioned that the fusion bombs are more powerful. Why 309 00:16:46,800 --> 00:16:47,040 Speaker 2: is that? 310 00:16:47,320 --> 00:16:50,280 Speaker 1: Yeah, that's a great question. And people also wonder like 311 00:16:50,440 --> 00:16:53,520 Speaker 1: why is it that when you stick light materials together 312 00:16:53,600 --> 00:16:56,520 Speaker 1: to make heavier ones you release energy, and if you 313 00:16:56,600 --> 00:16:59,800 Speaker 1: break up heavier ones to make lighter ones, you release energy. 314 00:17:00,040 --> 00:17:02,560 Speaker 1: And the answer to both questions just comes from the 315 00:17:02,560 --> 00:17:05,760 Speaker 1: sort of energy structure of the nucleus. So when you 316 00:17:05,880 --> 00:17:08,600 Speaker 1: squeeze two protons together to make helium, the way those 317 00:17:08,600 --> 00:17:12,120 Speaker 1: two protons are bound together by the strong force contains 318 00:17:12,160 --> 00:17:14,800 Speaker 1: like a deep potential well, sort of like the Earth 319 00:17:14,880 --> 00:17:17,680 Speaker 1: falling into a gravitational well being captured by the sun. 320 00:17:17,720 --> 00:17:20,399 Speaker 1: Those two protons capture each other, so you need a 321 00:17:20,440 --> 00:17:22,960 Speaker 1: lot of energy to break that up. Like if you 322 00:17:23,000 --> 00:17:25,440 Speaker 1: want it to take helium and break it up into hydrogen, 323 00:17:25,440 --> 00:17:27,840 Speaker 1: you'd have to zap it with a really powerful laser. 324 00:17:27,880 --> 00:17:30,439 Speaker 1: You have to add energy to that. So the energy 325 00:17:30,440 --> 00:17:33,359 Speaker 1: that's released from fusion has to do with the difference 326 00:17:33,720 --> 00:17:36,480 Speaker 1: between the sort of energy structure of two protons that 327 00:17:36,520 --> 00:17:38,520 Speaker 1: are far apart from each other and two protons that 328 00:17:38,560 --> 00:17:41,600 Speaker 1: are bound together in two helium. And why that number 329 00:17:41,760 --> 00:17:44,119 Speaker 1: is big. It just has to do with the strong 330 00:17:44,160 --> 00:17:46,760 Speaker 1: force and like how powerful it is. On the other 331 00:17:46,880 --> 00:17:49,639 Speaker 1: side of the spectrum. When you're breaking up uranium into 332 00:17:49,720 --> 00:17:52,119 Speaker 1: lighter stuff. That's a really big, heavy nucleus and it's 333 00:17:52,160 --> 00:17:55,800 Speaker 1: a little unstable already because of electromagnetism, which is pushing 334 00:17:55,800 --> 00:17:58,440 Speaker 1: all those protons apart, and the strong force isn't as 335 00:17:58,440 --> 00:18:00,920 Speaker 1: powerful because those protons are further or apart from each other, 336 00:18:00,960 --> 00:18:03,359 Speaker 1: just because the nucleus is like physically getting so big 337 00:18:03,400 --> 00:18:06,520 Speaker 1: that the strong force isn't as powerful over those distances, 338 00:18:06,720 --> 00:18:08,680 Speaker 1: So it's a little bit easier to break that up, 339 00:18:08,720 --> 00:18:12,040 Speaker 1: and the strong force bonds aren't as powerful because the 340 00:18:12,080 --> 00:18:14,040 Speaker 1: distance is a little bit greater there. So it all 341 00:18:14,040 --> 00:18:16,040 Speaker 1: has to do with like the structure of the energy 342 00:18:16,119 --> 00:18:19,560 Speaker 1: levels of the nuclear formation, which you're super complicated. 343 00:18:19,960 --> 00:18:24,280 Speaker 2: So when something heavy unstable atom, I thought that things 344 00:18:24,320 --> 00:18:28,680 Speaker 2: like uranium would sort of naturally decay because they are unstable. 345 00:18:29,080 --> 00:18:33,480 Speaker 2: Why don't they just spontaneously explode when they are decaying? 346 00:18:33,800 --> 00:18:36,800 Speaker 1: You mean, why don't you get runaway nuclear reactions in nature? 347 00:18:37,200 --> 00:18:37,760 Speaker 2: Exactly? 348 00:18:38,080 --> 00:18:41,360 Speaker 1: Actually you can. The crucial thing is just having enough uranium. 349 00:18:41,840 --> 00:18:44,639 Speaker 1: Uranium is typically dilute out in the world. It's in 350 00:18:44,720 --> 00:18:47,040 Speaker 1: oxides and it's not very pure. But if you do 351 00:18:47,119 --> 00:18:50,720 Speaker 1: happen to have a fairly pure uranium deposit, like sitting underground, 352 00:18:50,840 --> 00:18:54,040 Speaker 1: it will undergo a natural fission reaction. And there's a 353 00:18:54,080 --> 00:18:57,040 Speaker 1: spot in Africa where they're very certain that a couple 354 00:18:57,040 --> 00:19:00,359 Speaker 1: of billion years ago there was enough urinea and it 355 00:19:00,480 --> 00:19:03,000 Speaker 1: started a natural fission reaction and like cooked the rock 356 00:19:03,200 --> 00:19:05,320 Speaker 1: and like heated up the whole thing. We did a 357 00:19:05,320 --> 00:19:08,640 Speaker 1: whole podcast episode about it a year or so ago. Uranium, 358 00:19:08,680 --> 00:19:10,639 Speaker 1: of course, is unstable, and so it decays, and the 359 00:19:10,720 --> 00:19:13,600 Speaker 1: kind of uranium you need is getting more and more rare, 360 00:19:13,840 --> 00:19:15,679 Speaker 1: so it's not a likely thing to happen again, like 361 00:19:15,720 --> 00:19:19,679 Speaker 1: the conditions for natural fission reactions on Earth without human 362 00:19:19,720 --> 00:19:22,000 Speaker 1: intervention are no longer likely to exist. 363 00:19:22,240 --> 00:19:26,600 Speaker 2: Oh, that's really interesting. So back to the nuclear bombs, 364 00:19:26,640 --> 00:19:31,320 Speaker 2: Like what either for a fission bomb or a fusion bomb, 365 00:19:31,440 --> 00:19:35,040 Speaker 2: Like once you have set off that reaction, what happens 366 00:19:35,080 --> 00:19:38,920 Speaker 2: like on planet Earth exactly? Like what is the effect 367 00:19:39,040 --> 00:19:41,240 Speaker 2: the impact of a nuclear bomb? 368 00:19:41,400 --> 00:19:44,280 Speaker 1: So all bombs essentially are just a rapid release of 369 00:19:44,400 --> 00:19:47,879 Speaker 1: energy some process which is exothermic, maybe chemical for like 370 00:19:47,960 --> 00:19:52,040 Speaker 1: dynamite or nuclear for fusion fission bombs, but just a 371 00:19:52,200 --> 00:19:55,119 Speaker 1: very rapid release of energy. And the crucial things to 372 00:19:55,200 --> 00:19:57,280 Speaker 1: understand is how that energy is carried. In the case 373 00:19:57,280 --> 00:20:00,880 Speaker 1: of nuclear weapons, it's not just different carriers of energy 374 00:20:01,080 --> 00:20:04,879 Speaker 1: relative to chemical weapons, but it's also just much more dramatic. Right, 375 00:20:04,920 --> 00:20:09,000 Speaker 1: there's like so much more energy released per gram of 376 00:20:09,320 --> 00:20:12,640 Speaker 1: fuel because it's much more efficient at extracting energy from 377 00:20:12,680 --> 00:20:15,800 Speaker 1: those bonds. Chemical bonds and dynamite don't have nearly as 378 00:20:15,880 --> 00:20:19,200 Speaker 1: much energy as the nuclear bonds that we're releasing in 379 00:20:19,359 --> 00:20:22,679 Speaker 1: nuclear weapons, So you get different energy carriers flying out 380 00:20:22,840 --> 00:20:25,119 Speaker 1: and you just get a lot more So the energy 381 00:20:25,160 --> 00:20:29,200 Speaker 1: comes out in terms of photons, So like infrared photons, 382 00:20:29,320 --> 00:20:33,119 Speaker 1: visible light photons, UV photons, all of those things. You 383 00:20:33,200 --> 00:20:36,080 Speaker 1: also get a bunch of particles. You get neutrons, you 384 00:20:36,119 --> 00:20:39,639 Speaker 1: get electrons, you get protons, you get gamma rays, you 385 00:20:39,680 --> 00:20:43,159 Speaker 1: get all sorts of crazy things shooting out from the explosion. 386 00:20:43,320 --> 00:20:46,639 Speaker 2: When I've seen footage of test explosions of a nuclear 387 00:20:46,680 --> 00:20:49,880 Speaker 2: bomb on like an uninhabited house, it looks like this 388 00:20:50,080 --> 00:20:55,200 Speaker 2: huge wave of air almost just obliterating the house as 389 00:20:55,240 --> 00:20:59,400 Speaker 2: it passes through. What's causing that big shockwave a of air? 390 00:20:59,520 --> 00:21:03,080 Speaker 2: Is that just all these particles being released, this super 391 00:21:03,200 --> 00:21:05,760 Speaker 2: energy particles, or is there some kind of heat that's 392 00:21:05,800 --> 00:21:07,320 Speaker 2: also being released from the bomb. 393 00:21:07,400 --> 00:21:09,600 Speaker 1: So when you detonate a nuclear weapon, you produce all 394 00:21:09,640 --> 00:21:11,919 Speaker 1: of this energy in various forms, and then you have 395 00:21:11,960 --> 00:21:14,080 Speaker 1: to ask, like, Okay, the shell of stuff around the 396 00:21:14,160 --> 00:21:16,960 Speaker 1: nuclear weapon, the air or the water or whatever, is 397 00:21:16,960 --> 00:21:20,560 Speaker 1: that transparent to these energy carriers? Will it absorb that 398 00:21:20,760 --> 00:21:23,760 Speaker 1: energy or will it just pass through? And in some 399 00:21:23,840 --> 00:21:26,960 Speaker 1: cases it's transparent, in some cases it's not. So when 400 00:21:27,000 --> 00:21:29,080 Speaker 1: it's not transparent, when it's opaque, when it's going to 401 00:21:29,119 --> 00:21:32,280 Speaker 1: absorb that energy, then all that energy is getting dumped 402 00:21:32,320 --> 00:21:34,560 Speaker 1: into the air. So, for example, a lot of those 403 00:21:34,560 --> 00:21:38,080 Speaker 1: photons are absorbed by the air. The infrared, for example, 404 00:21:38,240 --> 00:21:41,400 Speaker 1: very efficiently absorbed by the air around the nuclear bomb, 405 00:21:41,520 --> 00:21:43,879 Speaker 1: and that heats up the air. So the energy has 406 00:21:43,920 --> 00:21:48,480 Speaker 1: been transformed from lower energy photons into temperature of the air. 407 00:21:48,640 --> 00:21:51,720 Speaker 1: So now that air is super duper hot. You've superheated 408 00:21:51,720 --> 00:21:54,600 Speaker 1: that air and it expands and then that heats the 409 00:21:54,680 --> 00:21:57,359 Speaker 1: air around it. And so that's where the shockwave comes from, 410 00:21:57,440 --> 00:22:00,600 Speaker 1: from the dumping of that energy from the particle that 411 00:22:00,680 --> 00:22:03,560 Speaker 1: come out of the nuclear weapons into the air itself, 412 00:22:03,600 --> 00:22:05,760 Speaker 1: and then the air becomes part of the explosion. 413 00:22:06,040 --> 00:22:08,720 Speaker 2: I see. And so you're saying, unless it's transparent, I 414 00:22:08,720 --> 00:22:13,520 Speaker 2: would assume that both air and water would absorb energy 415 00:22:13,760 --> 00:22:16,600 Speaker 2: from a nuke. So it doesn't seem like there'd be 416 00:22:17,000 --> 00:22:20,520 Speaker 2: anywhere on Earth where you wouldn't have an impact of 417 00:22:20,560 --> 00:22:22,520 Speaker 2: a nuclear explosion, right. 418 00:22:22,320 --> 00:22:24,560 Speaker 1: That's right. And so the breakdown is something like around 419 00:22:24,560 --> 00:22:26,240 Speaker 1: fifty percent of the energy in the air or in 420 00:22:26,240 --> 00:22:29,800 Speaker 1: the water goes into forming this shock wave. Basically it 421 00:22:29,840 --> 00:22:33,760 Speaker 1: gets turned into sound. Right, Sound is just matter pressing 422 00:22:33,800 --> 00:22:37,200 Speaker 1: on other matters compression waves. So like half the energy 423 00:22:37,200 --> 00:22:39,280 Speaker 1: of the nuclear bomb is absorbed by the matter that 424 00:22:39,280 --> 00:22:43,119 Speaker 1: surrounds it and then expands that something like forty percent 425 00:22:43,119 --> 00:22:45,639 Speaker 1: of it are photons to which the atmosphere or the 426 00:22:45,680 --> 00:22:49,760 Speaker 1: water are mostly transparent, so visible light UV light. Right, 427 00:22:49,800 --> 00:22:52,800 Speaker 1: the atmosphere is transparent to visible light. That's why we 428 00:22:52,840 --> 00:22:54,760 Speaker 1: can see each other and we can see the sun 429 00:22:55,200 --> 00:22:58,720 Speaker 1: because the atmosphere doesn't tend to absorb photons in this 430 00:22:58,920 --> 00:23:01,439 Speaker 1: range that we can see. And that's of course no accident. 431 00:23:01,520 --> 00:23:03,960 Speaker 1: That's why we can see these photons. We're evolved in 432 00:23:04,000 --> 00:23:07,480 Speaker 1: a situation to see these very useful photons. So fifty 433 00:23:07,520 --> 00:23:11,840 Speaker 1: percent into shock waves, forty percent into basically photons to 434 00:23:11,880 --> 00:23:14,360 Speaker 1: which the atmosphere of the water is transparent, and then 435 00:23:14,440 --> 00:23:17,360 Speaker 1: like ten percent of the energy in things like neutrons 436 00:23:17,400 --> 00:23:20,560 Speaker 1: and electrons, like other particles flying out like tiny bullets 437 00:23:20,600 --> 00:23:23,960 Speaker 1: with high energy, which can also pass right through the atmosphere. 438 00:23:24,240 --> 00:23:27,840 Speaker 2: So is it as hot as like having a little 439 00:23:27,960 --> 00:23:32,439 Speaker 2: sun in that area where the bomb went off? Like 440 00:23:32,480 --> 00:23:33,840 Speaker 2: how hot does that get? 441 00:23:34,119 --> 00:23:38,200 Speaker 1: Yeah, it gets to millions of degrees Calvin, It's really 442 00:23:38,280 --> 00:23:41,720 Speaker 1: incredibly hot. It's a huge amount of energy And that 443 00:23:41,840 --> 00:23:43,880 Speaker 1: sounds really hot, and it is really hot, and it's 444 00:23:43,920 --> 00:23:47,040 Speaker 1: actually hotter than the surface of the Sun, which is 445 00:23:47,119 --> 00:23:49,800 Speaker 1: just a few thousand degrees Calvin, and that's why it 446 00:23:49,840 --> 00:23:52,800 Speaker 1: can release energy like much much higher wavelengths. To remember 447 00:23:52,840 --> 00:23:56,359 Speaker 1: that the temperature of an object controls the energy spectrum 448 00:23:56,359 --> 00:23:59,560 Speaker 1: that's released. The hotter it is, the higher the frequency, 449 00:23:59,600 --> 00:24:02,840 Speaker 1: the higher energy the radiation, and so that's why nuclear 450 00:24:02,880 --> 00:24:05,320 Speaker 1: weapons release a lot of energy in the UV where 451 00:24:05,320 --> 00:24:08,800 Speaker 1: we can't even see it because they are so dang hot. 452 00:24:09,080 --> 00:24:12,400 Speaker 2: It is extremely bright as well, right, Like I think 453 00:24:12,400 --> 00:24:16,120 Speaker 2: that's something that everyone's kind of aware of, how incredibly 454 00:24:16,160 --> 00:24:19,600 Speaker 2: bright a nuclear explosion is, like you said, because the 455 00:24:19,720 --> 00:24:22,359 Speaker 2: light passes through the air and then we can see it. 456 00:24:22,400 --> 00:24:24,440 Speaker 2: Is it a white light or a yellow light? It'd 457 00:24:24,480 --> 00:24:26,000 Speaker 2: be probably a white light, right. 458 00:24:26,080 --> 00:24:28,520 Speaker 1: It's basically broad spectrum, And so if you're watching a 459 00:24:28,560 --> 00:24:31,719 Speaker 1: nuclear explosion, you actually see sort of two flashes. You 460 00:24:31,760 --> 00:24:34,680 Speaker 1: see an initial flash of light because it's very very 461 00:24:34,720 --> 00:24:37,160 Speaker 1: bright and it's very broad spectrum and it looks very white. 462 00:24:37,200 --> 00:24:40,680 Speaker 1: But then light that's released later is actually captured by 463 00:24:40,760 --> 00:24:42,920 Speaker 1: the shockwave. So you have the first flash which comes 464 00:24:42,960 --> 00:24:46,280 Speaker 1: out very quickly. Then the shockwave comes out and photons 465 00:24:46,280 --> 00:24:48,439 Speaker 1: which sort of bump up against the inner side of 466 00:24:48,480 --> 00:24:52,320 Speaker 1: that shockwave. Don't see it as transparent because the shockwave 467 00:24:52,320 --> 00:24:55,720 Speaker 1: has made that air denser and so it's no longer transparent. 468 00:24:55,840 --> 00:24:59,040 Speaker 1: And so until that shockwave dissipates, it's basically blocking the 469 00:24:59,119 --> 00:25:01,200 Speaker 1: light from the nuclear wave. And when it does, then 470 00:25:01,200 --> 00:25:03,560 Speaker 1: you see a second flash. You know, it's producing light 471 00:25:03,640 --> 00:25:06,440 Speaker 1: the whole time, but it's like momentarily blocked. So you 472 00:25:06,480 --> 00:25:09,919 Speaker 1: see this characteristic double peak of gamma radiation when you 473 00:25:09,920 --> 00:25:12,040 Speaker 1: blow up a nuclear bomb here on Earth, at least 474 00:25:12,080 --> 00:25:14,000 Speaker 1: underwater or in the air. 475 00:25:14,200 --> 00:25:16,800 Speaker 2: The other thing I think people think of when we 476 00:25:16,960 --> 00:25:23,520 Speaker 2: picture a nuclear explosion is that characteristic mushroom cloud. Why 477 00:25:23,760 --> 00:25:27,040 Speaker 2: does it have such a you know, specific shape, that 478 00:25:27,119 --> 00:25:30,080 Speaker 2: mushroom cloud shape. Is that just sort of basic physics 479 00:25:30,119 --> 00:25:32,680 Speaker 2: when it comes to an explosion that's large enough, or 480 00:25:32,800 --> 00:25:34,080 Speaker 2: is there something else going on. 481 00:25:34,160 --> 00:25:38,000 Speaker 1: That's basic physics from a really large explosion. It's typical 482 00:25:38,160 --> 00:25:42,159 Speaker 1: for nuclear explosions because they are so powerful. You know, 483 00:25:42,200 --> 00:25:45,040 Speaker 1: you have this sudden formation of a really large volume 484 00:25:45,080 --> 00:25:47,959 Speaker 1: of lower density gases, and then you get a buoyant 485 00:25:48,040 --> 00:25:51,480 Speaker 1: massive gas which rises rapidly, giving you all this turbulence 486 00:25:51,520 --> 00:25:54,200 Speaker 1: and curling down around the edges. But it can come 487 00:25:54,280 --> 00:25:57,080 Speaker 1: from chemical explosions also if they are big enough. 488 00:25:57,359 --> 00:26:00,800 Speaker 2: I see. Interesting. So when you have a nuclear explosion, 489 00:26:00,840 --> 00:26:03,800 Speaker 2: you have this huge amount of energy released. It superheats 490 00:26:03,840 --> 00:26:07,840 Speaker 2: the air, causes this shock wave, causes a massive amount 491 00:26:07,960 --> 00:26:13,119 Speaker 2: of energy to be released in heat in radiation, which 492 00:26:13,240 --> 00:26:16,440 Speaker 2: you know is a real sucker punch after the effects 493 00:26:16,480 --> 00:26:18,879 Speaker 2: of the bomb, right, Like, you have this radiation in 494 00:26:18,920 --> 00:26:22,360 Speaker 2: the area, and people can get radiation poisoning. But it dissipates, 495 00:26:22,560 --> 00:26:26,800 Speaker 2: it explodes, the energy dissipates, it reaks, whatever havoc it's 496 00:26:26,840 --> 00:26:29,399 Speaker 2: gonna reek and then it kind of it settles, the 497 00:26:29,560 --> 00:26:33,480 Speaker 2: dust cloud settles, the radiation settles, and then it's it's 498 00:26:33,520 --> 00:26:37,800 Speaker 2: a big explosion. And how long does it last? Typically 499 00:26:37,880 --> 00:26:41,280 Speaker 2: like the explosion part of a nuclear bomb. 500 00:26:41,520 --> 00:26:44,159 Speaker 1: So the actual reaction is very quick, but you know, 501 00:26:44,200 --> 00:26:46,639 Speaker 1: the shockwave travels at the speed of sound, which is 502 00:26:46,800 --> 00:26:49,800 Speaker 1: being like a thousand feet per second, and so depending 503 00:26:49,840 --> 00:26:51,520 Speaker 1: on the strength of the bomb, it can be like 504 00:26:51,600 --> 00:26:54,320 Speaker 1: thirty seconds to a minute or so before that shock 505 00:26:54,400 --> 00:26:57,199 Speaker 1: wave dissipates. And you're right that the initial danger is 506 00:26:57,280 --> 00:26:59,080 Speaker 1: very very strong. You have the shockwave, you have the 507 00:26:59,160 --> 00:27:01,720 Speaker 1: radiation exposure. Sure, but then this is the lasting effects 508 00:27:01,720 --> 00:27:04,159 Speaker 1: of the fallout. Right, you have released a bunch of 509 00:27:04,280 --> 00:27:07,600 Speaker 1: radioactive material, not all of it has fused or fizzed. 510 00:27:07,720 --> 00:27:11,320 Speaker 1: And also that radiation creates more radioactive material. All these 511 00:27:11,359 --> 00:27:14,480 Speaker 1: high energy neutrons can slam into other stuff, turning them 512 00:27:14,480 --> 00:27:18,159 Speaker 1: into radioactive elements, and so the whole area is radioactor 513 00:27:18,280 --> 00:27:20,480 Speaker 1: for a while, and in the cloud they are radioactive 514 00:27:20,480 --> 00:27:22,960 Speaker 1: elements produced. When you have a fission reaction, we know 515 00:27:23,320 --> 00:27:25,800 Speaker 1: that it produces very dangerous toxic waste. 516 00:27:25,880 --> 00:27:25,960 Speaker 5: Right. 517 00:27:26,000 --> 00:27:28,600 Speaker 1: That's why nuclear reactors have such a tricky problem to 518 00:27:28,640 --> 00:27:30,840 Speaker 1: deal with. And a nuclear bomb that's not contained at all, 519 00:27:30,840 --> 00:27:33,280 Speaker 1: it's just blown up into the atmosphere, and so the 520 00:27:33,320 --> 00:27:35,439 Speaker 1: fallout can be very dangerous and it can drift, right, 521 00:27:35,440 --> 00:27:37,920 Speaker 1: you have wind for example, so it can drift over 522 00:27:38,040 --> 00:27:38,920 Speaker 1: hundreds of miles. 523 00:27:39,080 --> 00:27:42,880 Speaker 2: Yeah, I mean that's one of the considerations that countries 524 00:27:42,920 --> 00:27:45,560 Speaker 2: have when they're thinking of using nukes. It's like, well, 525 00:27:45,560 --> 00:27:47,840 Speaker 2: if I use it on my neighbor, that might just 526 00:27:47,880 --> 00:27:51,520 Speaker 2: blow right back into my country, which I think is 527 00:27:51,880 --> 00:27:54,480 Speaker 2: in a way good, right, because you should think a 528 00:27:54,480 --> 00:27:58,359 Speaker 2: few times before you decide to ease a nuke. But 529 00:27:58,640 --> 00:28:01,800 Speaker 2: we should probably take a quick break practice our duck 530 00:28:01,840 --> 00:28:04,800 Speaker 2: and cover, and when we get back, talk about what 531 00:28:05,040 --> 00:28:09,440 Speaker 2: happens when you explode a nuke in space, not on Earth. 532 00:28:22,320 --> 00:28:24,960 Speaker 2: So I've practiced my duck and cover a few times, 533 00:28:24,960 --> 00:28:27,679 Speaker 2: which I'm sure would protect me really well if I 534 00:28:27,800 --> 00:28:31,320 Speaker 2: was in the heart of a nuclear explosion. My desk 535 00:28:31,560 --> 00:28:35,280 Speaker 2: is very sturdy. But we talked about what happens with 536 00:28:35,359 --> 00:28:39,600 Speaker 2: a nuclear explosion on Earth. Hopefully we'll never see one ourselves, 537 00:28:39,880 --> 00:28:44,520 Speaker 2: but what happens when you explode a nuke in space? 538 00:28:44,680 --> 00:28:48,400 Speaker 2: Because space is very different from our planet Earth. It's 539 00:28:48,960 --> 00:28:52,680 Speaker 2: missing a few things that we have that are nice 540 00:28:52,760 --> 00:28:55,680 Speaker 2: to have here on Earth that protects us in other life, 541 00:28:55,880 --> 00:29:00,000 Speaker 2: and so it seems like a nuclear bomb would react 542 00:29:00,240 --> 00:29:01,479 Speaker 2: differently in space. 543 00:29:01,960 --> 00:29:04,680 Speaker 1: Yeah, it's really different, and in a fascinating way. The 544 00:29:04,720 --> 00:29:07,720 Speaker 1: actual core reaction, of course, is the same. When the 545 00:29:07,720 --> 00:29:10,480 Speaker 1: bomb goes off, it doesn't need the atmosphere or water 546 00:29:10,640 --> 00:29:13,480 Speaker 1: or anything around it in order to actually detonate. It's 547 00:29:13,520 --> 00:29:16,240 Speaker 1: not like a fire where you're using the oxygen from 548 00:29:16,280 --> 00:29:19,560 Speaker 1: the atmosphere to burn. It can go all by itself, 549 00:29:19,600 --> 00:29:22,160 Speaker 1: so it's happy to blow up in space or underwater 550 00:29:22,400 --> 00:29:25,320 Speaker 1: or underground or in the air. So the core reaction 551 00:29:25,560 --> 00:29:27,880 Speaker 1: is no different, and the things that it produces are 552 00:29:27,920 --> 00:29:30,200 Speaker 1: the same. So a nuclear bomb in space blowing up 553 00:29:30,240 --> 00:29:34,560 Speaker 1: produces the same spectrum of photon energies and neutron energies 554 00:29:34,560 --> 00:29:37,280 Speaker 1: and electrons, et cetera as the nuclear bomb blowing up 555 00:29:37,280 --> 00:29:40,080 Speaker 1: anywhere else. But of course the immediate surroundings of the 556 00:29:40,160 --> 00:29:42,560 Speaker 1: bomb are very different. And so now instead of having 557 00:29:42,640 --> 00:29:45,840 Speaker 1: some of that radiation immediately absorbed basically by a pillow 558 00:29:45,880 --> 00:29:48,080 Speaker 1: that was surrounded the bomb, a pillow of air or 559 00:29:48,120 --> 00:29:52,120 Speaker 1: water or dirt, now there's nothing there, so everything is transparent. 560 00:29:52,360 --> 00:29:55,320 Speaker 1: So all that radiation instead of getting dumped into some 561 00:29:55,720 --> 00:29:59,440 Speaker 1: blanket or some pillow, just flies out, so it all 562 00:29:59,480 --> 00:30:02,920 Speaker 1: stays as radiation. It just flies out like a mini sun, 563 00:30:03,280 --> 00:30:07,640 Speaker 1: as our listeners describe, filling nearby space with very dangerous radiation. 564 00:30:08,000 --> 00:30:11,080 Speaker 2: So when I see things like in Star Trek or 565 00:30:11,920 --> 00:30:15,480 Speaker 2: Star Wars and they like fire some kind of missile 566 00:30:15,720 --> 00:30:18,600 Speaker 2: and then you see this like big explosion with like 567 00:30:18,640 --> 00:30:22,000 Speaker 2: a explodey cloud thing, if you're doing it just that 568 00:30:22,280 --> 00:30:25,760 Speaker 2: space right, like maybe I guess if you hit a spaceship, 569 00:30:25,800 --> 00:30:28,080 Speaker 2: you could get some debris that causes a bit of 570 00:30:28,080 --> 00:30:30,440 Speaker 2: a cloud. But if you're just firing out in space. 571 00:30:30,600 --> 00:30:34,160 Speaker 2: What exactly does an explosion look like when you're just 572 00:30:34,600 --> 00:30:36,360 Speaker 2: it's just happening in empty space? 573 00:30:36,640 --> 00:30:40,120 Speaker 1: Yeah, great question. Those science fiction explosions use cues from 574 00:30:40,200 --> 00:30:43,120 Speaker 1: our intuition. On Earth, you know, where things are loud 575 00:30:43,320 --> 00:30:46,600 Speaker 1: and they are hot, But in space things would be different. Right. 576 00:30:46,640 --> 00:30:48,680 Speaker 1: There's no sound. I mean, there are some particles out 577 00:30:48,680 --> 00:30:51,920 Speaker 1: in space. It's not totally empty, so technically speaking, there 578 00:30:51,920 --> 00:30:54,680 Speaker 1: there is the ability to propagate sound waves, but there's 579 00:30:54,680 --> 00:30:57,760 Speaker 1: no sound, and there's also no flames, right, so what 580 00:30:57,760 --> 00:31:00,800 Speaker 1: you would see instead is a very bright flash of 581 00:31:01,040 --> 00:31:03,880 Speaker 1: light because all those particles are just flying out. There's 582 00:31:03,920 --> 00:31:07,080 Speaker 1: nothing burning there. And you say, maybe the ship itself 583 00:31:07,080 --> 00:31:09,520 Speaker 1: would explode if there's like fuel on board or whatever, 584 00:31:09,640 --> 00:31:12,880 Speaker 1: but there's no flame, there's no oxidization effects, no chemical 585 00:31:12,920 --> 00:31:16,120 Speaker 1: burning there. So essentially it's just a very bright pinprick 586 00:31:16,200 --> 00:31:19,600 Speaker 1: of light, extremely bright, like something you should definitely not 587 00:31:19,760 --> 00:31:20,240 Speaker 1: look at. 588 00:31:20,560 --> 00:31:23,200 Speaker 2: So you don't get that double flash right like you 589 00:31:23,240 --> 00:31:25,800 Speaker 2: do with a nuke on Earth, because there's no shockwave 590 00:31:25,920 --> 00:31:28,680 Speaker 2: to absorb the light from and kind of prevent it 591 00:31:28,680 --> 00:31:31,360 Speaker 2: from reaching your eyes until the shockwave has moved on. 592 00:31:31,640 --> 00:31:34,520 Speaker 1: Exactly, that shockwave is purely a product of a race 593 00:31:34,600 --> 00:31:37,880 Speaker 1: between the photons and the sound wave that's propagetting out. 594 00:31:37,920 --> 00:31:41,320 Speaker 1: But because there is no soundwave, there's no shockwave, there's 595 00:31:41,320 --> 00:31:44,000 Speaker 1: nothing there to absorb that radiation. All the radiation just 596 00:31:44,040 --> 00:31:47,400 Speaker 1: flies out, and so it looks quite different. And what 597 00:31:47,440 --> 00:31:50,160 Speaker 1: that means is that nuclear weapons are dangerous over much 598 00:31:50,320 --> 00:31:54,200 Speaker 1: greater distances in space because the radiation is not absorbed, 599 00:31:54,200 --> 00:31:56,280 Speaker 1: and so if a nuclear bomb blows up in space, 600 00:31:56,440 --> 00:31:59,479 Speaker 1: you can get significant radiation damage from it, even if 601 00:31:59,480 --> 00:32:00,920 Speaker 1: you're much further away. 602 00:32:01,360 --> 00:32:06,240 Speaker 2: Say we exploded a nuke somewhere in our solar system, 603 00:32:06,760 --> 00:32:09,400 Speaker 2: would that radiation potentially hit. 604 00:32:09,280 --> 00:32:12,480 Speaker 1: Earth, you still are protected by physics is one over 605 00:32:12,600 --> 00:32:14,960 Speaker 1: distance squared law. The same with the Sun is like 606 00:32:14,960 --> 00:32:17,960 Speaker 1: one hundred times dimmer if you're ten times further away, 607 00:32:18,480 --> 00:32:20,880 Speaker 1: or electric fields go down by a factor of four 608 00:32:21,080 --> 00:32:23,360 Speaker 1: if you're twice as far from the charge as all 609 00:32:23,400 --> 00:32:26,480 Speaker 1: these one over distance squared law in physics, which actually 610 00:32:26,520 --> 00:32:29,280 Speaker 1: not hard to understand. Like from a geometrical point of view, 611 00:32:29,680 --> 00:32:32,440 Speaker 1: you imagine, like particles flying out from a nuclear bomb 612 00:32:32,560 --> 00:32:35,640 Speaker 1: or photons flying out from the Sun, the same certain 613 00:32:35,760 --> 00:32:39,520 Speaker 1: number are released, and then as the radius grows, those 614 00:32:39,800 --> 00:32:43,400 Speaker 1: particles are now spread out over a larger and larger sphere, 615 00:32:43,480 --> 00:32:45,760 Speaker 1: and the area of that sphere goes like four pi 616 00:32:46,000 --> 00:32:49,440 Speaker 1: are squared. So as that sphere gets larger, the same 617 00:32:49,520 --> 00:32:52,480 Speaker 1: number of photons or dangerous particles are spread out over 618 00:32:52,520 --> 00:32:54,760 Speaker 1: a larger area. So for any given area of the 619 00:32:54,840 --> 00:32:58,680 Speaker 1: radiation drops like one over the distance squared. And so 620 00:32:58,800 --> 00:33:01,360 Speaker 1: if you're far away from this thing, you'll be safe. Now, 621 00:33:01,360 --> 00:33:04,120 Speaker 1: on Earth, you can be just a couple of miles, two, three, 622 00:33:04,200 --> 00:33:08,120 Speaker 1: four miles from an explosion and be mostly safe from 623 00:33:08,120 --> 00:33:11,040 Speaker 1: the radiation because so much of it is absorbed into 624 00:33:11,080 --> 00:33:13,280 Speaker 1: the atmosphere. But in space you've got to be like 625 00:33:13,440 --> 00:33:17,040 Speaker 1: forty fifty sixty miles to be as safe as you 626 00:33:17,080 --> 00:33:20,440 Speaker 1: would be on Earth, because essentially there's no protection. Right 627 00:33:20,640 --> 00:33:23,200 Speaker 1: on Earth, you're kind of protected from this nuclear bomb 628 00:33:23,240 --> 00:33:25,920 Speaker 1: by the atmosphere or by the ground, or by the water, 629 00:33:26,000 --> 00:33:28,120 Speaker 1: but in space there's nothing there to shield you. 630 00:33:28,480 --> 00:33:32,800 Speaker 2: Right, So is this radiation constantly spreading out or does 631 00:33:32,840 --> 00:33:36,520 Speaker 2: it kind of stop dissipating after a while. Does it 632 00:33:36,600 --> 00:33:41,560 Speaker 2: keep dissipating forever until it just sort of has equalized somehow? 633 00:33:41,800 --> 00:33:44,880 Speaker 1: Yeah, great question. Well, the initial explosion again is very brief. 634 00:33:44,920 --> 00:33:47,640 Speaker 1: The actual nuclear detonation doesn't last very long, and so 635 00:33:47,640 --> 00:33:49,360 Speaker 1: what you're thinking about is sort of like a pulse, 636 00:33:49,800 --> 00:33:52,200 Speaker 1: like all this radiation in a sphere that's traveling out 637 00:33:52,320 --> 00:33:55,160 Speaker 1: very very fast, in many cases actually at the speed 638 00:33:55,160 --> 00:33:57,720 Speaker 1: of light, and then getting dimmer and dimmer as it goes. 639 00:33:58,000 --> 00:34:00,120 Speaker 1: And so it's really just like a pulse that travels 640 00:34:00,160 --> 00:34:02,960 Speaker 1: through space, washing over things and damaging them. 641 00:34:03,280 --> 00:34:06,080 Speaker 2: How long does that pulse last? Does it last like 642 00:34:06,640 --> 00:34:08,840 Speaker 2: seconds or hours or years? 643 00:34:09,040 --> 00:34:11,040 Speaker 1: Well, the pulse itself would last for less than a second. 644 00:34:11,080 --> 00:34:13,920 Speaker 1: The actual explosion itself doesn't take very long, so it's 645 00:34:13,920 --> 00:34:17,480 Speaker 1: not like sitting there stewing, continuing to produce pulses of energy. 646 00:34:17,520 --> 00:34:20,680 Speaker 1: It's one very high intensity pulse over a short time. 647 00:34:20,760 --> 00:34:24,160 Speaker 1: But it's various kinds of radiation. Also. There's photons, very 648 00:34:24,200 --> 00:34:26,960 Speaker 1: high energies, and then there's neutrons, of course, and there's 649 00:34:27,000 --> 00:34:30,719 Speaker 1: also electrons. And the electrons can be particularly damaging and 650 00:34:30,760 --> 00:34:33,640 Speaker 1: also kind of fascinating because the electrons are traveling at 651 00:34:33,719 --> 00:34:36,880 Speaker 1: very very high speeds and they tend to radiate. So electrons, 652 00:34:36,920 --> 00:34:38,799 Speaker 1: when they move to a magnetic field or anything they 653 00:34:38,880 --> 00:34:42,400 Speaker 1: change direction, they radiate photons, and so that creates this 654 00:34:42,520 --> 00:34:46,840 Speaker 1: electromagnetic pulse. So all these electrons create this electromagnetic pulse 655 00:34:46,840 --> 00:34:49,759 Speaker 1: which can disrupt the flow of electricity or damage any 656 00:34:49,800 --> 00:34:52,200 Speaker 1: sort of electronics. And you see this in science fiction 657 00:34:52,280 --> 00:34:54,640 Speaker 1: all the time, right, that like electronics are blacked out 658 00:34:54,680 --> 00:34:56,800 Speaker 1: when there's a nuclear bomb, And that's really true. It 659 00:34:56,800 --> 00:34:59,760 Speaker 1: will create like pulses of energy in electronics. 660 00:35:00,239 --> 00:35:03,080 Speaker 2: That's really interesting. So if you're a spaceship, right and 661 00:35:03,120 --> 00:35:05,960 Speaker 2: you're riding up and someone decides to blow up a 662 00:35:06,040 --> 00:35:08,799 Speaker 2: nuke in front of you, you're really screwed in many 663 00:35:08,840 --> 00:35:11,880 Speaker 2: ways because you've just got a huge dose of radiation 664 00:35:12,640 --> 00:35:15,480 Speaker 2: and then all of your electronics on your spaceship are 665 00:35:15,480 --> 00:35:17,960 Speaker 2: going to get messed up by that EMP pulse. Is 666 00:35:18,000 --> 00:35:20,239 Speaker 2: there anything else to look out for if you're on 667 00:35:20,280 --> 00:35:26,440 Speaker 2: that spaceship cruising and someone blows up a nuke, Miria, Well. 668 00:35:26,200 --> 00:35:27,960 Speaker 1: If you're on that spaceship, I really hope you have 669 00:35:28,000 --> 00:35:31,040 Speaker 1: a special leadlined room to protect yourself, like we do 670 00:35:31,160 --> 00:35:34,280 Speaker 1: actually on the space station. Because the Sun, of course, 671 00:35:34,360 --> 00:35:37,359 Speaker 1: is a huge source of radiation, and solar storms can 672 00:35:37,440 --> 00:35:40,759 Speaker 1: generate EMPs and also other kinds of radiation which can 673 00:35:40,800 --> 00:35:44,160 Speaker 1: damage satellites and people, and so they have a special 674 00:35:44,200 --> 00:35:46,319 Speaker 1: room on the space station where the astronauts can go 675 00:35:46,440 --> 00:35:48,520 Speaker 1: like a panic room when there's going to be like 676 00:35:48,560 --> 00:35:52,000 Speaker 1: a high radiation solar weather event. And so I hope 677 00:35:52,000 --> 00:35:53,960 Speaker 1: your spaceship is outfitted with one of those, because if 678 00:35:53,960 --> 00:35:55,880 Speaker 1: somebody blows up a nuclear bomb, it's going to damage 679 00:35:55,880 --> 00:35:58,520 Speaker 1: your ship and also damage you if you're within tens 680 00:35:58,520 --> 00:35:59,080 Speaker 1: of miles. 681 00:35:59,320 --> 00:36:02,919 Speaker 2: We know that for like when you explode a nuke 682 00:36:03,040 --> 00:36:08,320 Speaker 2: on Earth, long after the explosion, it's irradiated everything around, 683 00:36:08,320 --> 00:36:11,720 Speaker 2: and depending on how large the explosion is, the nature 684 00:36:11,760 --> 00:36:15,120 Speaker 2: of it, like with Chernobyl, the area in that exclusion 685 00:36:15,200 --> 00:36:19,279 Speaker 2: zone is still radioactive. Like it's still not necessarily a 686 00:36:19,320 --> 00:36:22,440 Speaker 2: safe place to be. It's not like you will immediately 687 00:36:22,920 --> 00:36:26,200 Speaker 2: get radiation poisoning and die if you step foot in 688 00:36:26,280 --> 00:36:29,640 Speaker 2: the exclusion zone, but you can get sick depending on 689 00:36:29,640 --> 00:36:32,040 Speaker 2: how long you're in there and how close you get 690 00:36:32,080 --> 00:36:36,520 Speaker 2: to the center where the explosion happened. But what happens, 691 00:36:36,680 --> 00:36:39,480 Speaker 2: like with this explosion in space, is there an area 692 00:36:39,680 --> 00:36:43,560 Speaker 2: like a sort of point in the middle that continues 693 00:36:43,600 --> 00:36:47,040 Speaker 2: to be sort of radioactive or does that without anything 694 00:36:47,080 --> 00:36:50,160 Speaker 2: to really absorb it, It just keeps moving until it 695 00:36:50,239 --> 00:36:53,960 Speaker 2: hits something that it can be absorbed by Yeah. 696 00:36:53,920 --> 00:36:56,440 Speaker 1: Great question. And remember, of course Schernobyl was a nuclear 697 00:36:56,480 --> 00:37:00,160 Speaker 1: meltdown of a reactor, not an actual nuclear explosion, so 698 00:37:00,200 --> 00:37:02,480 Speaker 1: nothing blew up, so you still have a lot of 699 00:37:02,480 --> 00:37:05,160 Speaker 1: the fuel and all that stuff there in that same location. 700 00:37:05,440 --> 00:37:07,560 Speaker 1: The larger exclusion zone is because of the weather and 701 00:37:07,600 --> 00:37:10,360 Speaker 1: the air that pulled the smoke and the radioactive particles 702 00:37:10,640 --> 00:37:13,239 Speaker 1: further away, so there was never actually a nuclear explosion there. 703 00:37:13,280 --> 00:37:15,520 Speaker 1: And in space, you blow this bomb up, there's not 704 00:37:15,560 --> 00:37:18,120 Speaker 1: going to be really anything left in the location of 705 00:37:18,120 --> 00:37:20,960 Speaker 1: your detonation to poison people. Everything is going to fly 706 00:37:21,080 --> 00:37:24,200 Speaker 1: out because there's nothing stopping it, right, There's nothing holding 707 00:37:24,239 --> 00:37:27,440 Speaker 1: it in place at all, So you haven't like poured 708 00:37:27,520 --> 00:37:30,880 Speaker 1: radiation into a bunch of nearby dirt or water. Everything 709 00:37:30,920 --> 00:37:33,240 Speaker 1: is just going to flow away. So you could probably 710 00:37:33,239 --> 00:37:36,000 Speaker 1: come back in, you know, a month or so after 711 00:37:36,000 --> 00:37:38,400 Speaker 1: the nuclear bomb, and the space would be no different 712 00:37:38,480 --> 00:37:41,200 Speaker 1: from when you started. All of the dangerous elements would 713 00:37:41,200 --> 00:37:44,719 Speaker 1: be flying out from the source in lots of directions, 714 00:37:44,840 --> 00:37:47,920 Speaker 1: poisoning people or causing damage as they hit them, But 715 00:37:48,000 --> 00:37:51,479 Speaker 1: the actual location of the nuclear explosion in space isn't 716 00:37:51,480 --> 00:37:53,640 Speaker 1: going to be like affected in any way, have we. 717 00:37:53,719 --> 00:37:56,000 Speaker 2: Ever thought to blow up a nuke? And I mean 718 00:37:56,040 --> 00:37:58,080 Speaker 2: I'm sure we've thought of it, but have we ever 719 00:37:58,280 --> 00:37:59,800 Speaker 2: actually done it before? 720 00:38:00,080 --> 00:38:03,239 Speaker 1: Oh? Yes, we have actually blown up nuclear weapons in 721 00:38:03,480 --> 00:38:06,440 Speaker 1: lots of places. We've blown them up in more Unfortunately, 722 00:38:06,520 --> 00:38:09,200 Speaker 1: we've blown them up above ground, we've blown them up underground, 723 00:38:09,239 --> 00:38:12,560 Speaker 1: and we have actually done a nuclear explosion in space. 724 00:38:13,000 --> 00:38:15,120 Speaker 1: So we don't even have to wonder about what this 725 00:38:15,160 --> 00:38:17,920 Speaker 1: looks like. We know we have pictures. 726 00:38:18,280 --> 00:38:23,200 Speaker 2: Well, that sounds terrifying. Let's take another quick break. I'm 727 00:38:23,239 --> 00:38:26,480 Speaker 2: gonna watch the little duck and cover turtle learn some 728 00:38:26,600 --> 00:38:29,440 Speaker 2: good lessons, and when we get back, I want you 729 00:38:29,480 --> 00:38:32,640 Speaker 2: to tell me about blowing up nukes and space, which 730 00:38:32,680 --> 00:38:48,200 Speaker 2: apparently we have already done. So we are back to 731 00:38:48,239 --> 00:38:51,759 Speaker 2: that little duck and cover turtle. He's got a turtle shell, 732 00:38:51,800 --> 00:38:56,040 Speaker 2: but he's also got a helmet redundant. Anyways, now we're 733 00:38:56,080 --> 00:38:59,919 Speaker 2: going to talk about how we actually have already blown 734 00:39:00,200 --> 00:39:03,160 Speaker 2: up a nuke in space. It terrifies me that we 735 00:39:03,200 --> 00:39:07,279 Speaker 2: may have pissed off some aliens and many generations from 736 00:39:07,280 --> 00:39:10,800 Speaker 2: now they'll finally reach us and give us a real scolding. 737 00:39:10,880 --> 00:39:14,280 Speaker 2: But Daniel, what happened? Why did we blow up space. 738 00:39:14,760 --> 00:39:17,680 Speaker 1: So nuclear testing started in nineteen forty five with the 739 00:39:17,680 --> 00:39:20,600 Speaker 1: Manhattan Project. The US, of course the first country to 740 00:39:20,640 --> 00:39:22,759 Speaker 1: develop these things and to test them and then to 741 00:39:22,840 --> 00:39:26,400 Speaker 1: use them in war, where thousands of people were killed horribly. 742 00:39:26,560 --> 00:39:30,600 Speaker 1: And since then there's been about two thousand nuclear explosions 743 00:39:30,640 --> 00:39:33,520 Speaker 1: conducted by humans. And in the early days it was 744 00:39:33,560 --> 00:39:35,600 Speaker 1: free for all, there were no laws. People were blowing 745 00:39:35,600 --> 00:39:39,360 Speaker 1: stuff underground, above ground, et cetera. But we pretty rapidly 746 00:39:39,400 --> 00:39:42,520 Speaker 1: realized that blowing up stuff in our atmosphere was a 747 00:39:42,560 --> 00:39:47,440 Speaker 1: bad idea, creating radioactive particles and fallout. They could drift anywhere. 748 00:39:47,640 --> 00:39:49,680 Speaker 1: We blew up a bunch of islands, which is terrible, 749 00:39:49,760 --> 00:39:52,400 Speaker 1: destroying people's homes. And so that was in the fifties, 750 00:39:52,440 --> 00:39:54,560 Speaker 1: and things were of course very tense between the US 751 00:39:54,600 --> 00:39:57,840 Speaker 1: and the USSR. The US had stopped atmospheric testing, but 752 00:39:57,880 --> 00:40:01,520 Speaker 1: in the early sixties the USSR started atmospheric testing again, 753 00:40:01,640 --> 00:40:04,480 Speaker 1: which was sort of part of a larger political struggle 754 00:40:04,480 --> 00:40:06,920 Speaker 1: within the USSR to like stand up to the US. 755 00:40:07,080 --> 00:40:09,400 Speaker 1: We really should have like a Russian political expert on 756 00:40:09,440 --> 00:40:11,600 Speaker 1: to tell us about why they started that up again. 757 00:40:11,760 --> 00:40:15,160 Speaker 1: But in nineteen sixty two, the US wanted to know, like, well, 758 00:40:15,200 --> 00:40:17,200 Speaker 1: what happens if you blow up a nuke in space? 759 00:40:17,239 --> 00:40:19,200 Speaker 1: They were basically curious, and they didn't want to do 760 00:40:19,200 --> 00:40:22,360 Speaker 1: any more atmospheric testing, and so they tested a nuke 761 00:40:22,760 --> 00:40:25,839 Speaker 1: over the Pacific in July of nineteen sixty two. 762 00:40:26,360 --> 00:40:29,600 Speaker 2: So I'm thinking, like, if we blow it up just 763 00:40:29,680 --> 00:40:32,480 Speaker 2: a little bit above our atmosphere, that's not going to 764 00:40:32,560 --> 00:40:35,800 Speaker 2: cut it. Like how far away did we go? Because 765 00:40:36,040 --> 00:40:39,080 Speaker 2: you know, it seems like if you're too close you 766 00:40:39,120 --> 00:40:42,239 Speaker 2: can still have an impact on the Earth that you're 767 00:40:42,239 --> 00:40:42,799 Speaker 2: not going to want. 768 00:40:43,400 --> 00:40:45,800 Speaker 1: Yeah, exactly, if it's too far away, you won't be 769 00:40:45,840 --> 00:40:47,760 Speaker 1: able to see it because we don't have great instruments 770 00:40:47,760 --> 00:40:50,040 Speaker 1: in space. If it's too close, then it's basically in 771 00:40:50,080 --> 00:40:53,120 Speaker 1: your atmosphere, and said they chose an altitude of two 772 00:40:53,200 --> 00:40:56,680 Speaker 1: hundred and forty miles above the Earth's surface, and they 773 00:40:56,760 --> 00:41:01,640 Speaker 1: launched a one point four mega ton nuke from Johnston Island, 774 00:41:01,680 --> 00:41:05,160 Speaker 1: which is like fifteen hundred kilometers southwest of Hawaii. And 775 00:41:05,200 --> 00:41:07,399 Speaker 1: the idea was like, well, if something bad happens, does 776 00:41:07,440 --> 00:41:10,520 Speaker 1: have it happen over less populated areas, I guess, And 777 00:41:10,560 --> 00:41:13,440 Speaker 1: people imagine like, oh, that's far enough away from Hawaii 778 00:41:13,480 --> 00:41:15,520 Speaker 1: to not be a big deal, right, And they check 779 00:41:15,560 --> 00:41:17,560 Speaker 1: with a scientist and the sounds just like yeah, right, 780 00:41:17,719 --> 00:41:22,480 Speaker 1: no problem. Turns out those scientists were wrong. Oh boy, yep. Scientists, 781 00:41:22,560 --> 00:41:24,480 Speaker 1: especially physicists, can be wrong. 782 00:41:25,160 --> 00:41:27,760 Speaker 2: Yeah, which is a big deal when you're talking about 783 00:41:27,800 --> 00:41:32,000 Speaker 2: a nuke and talking about people just trying to live 784 00:41:32,040 --> 00:41:35,040 Speaker 2: their lives. And then you're like, but we're curious to 785 00:41:35,080 --> 00:41:36,880 Speaker 2: see what this will do. Yikes. 786 00:41:37,040 --> 00:41:40,120 Speaker 1: You can google this thing. It's called starfish prime and 787 00:41:40,280 --> 00:41:43,719 Speaker 1: just as we expect, it makes a spherical explosion. So 788 00:41:43,760 --> 00:41:46,080 Speaker 1: you don't get like a mushroom cloud that's a product 789 00:41:46,080 --> 00:41:48,279 Speaker 1: of blowing up in an atmosphere. You just get this 790 00:41:48,400 --> 00:41:53,440 Speaker 1: spherical explosion. It's not completely perfectly spherical, because the nuclear 791 00:41:53,480 --> 00:41:56,800 Speaker 1: bomb is not perfectly symmetric. There's like some small differences 792 00:41:56,800 --> 00:41:59,400 Speaker 1: in how the explosion happens based on exactly how the 793 00:41:59,440 --> 00:42:02,760 Speaker 1: fuel is ranged. But it's almost completely spherical. 794 00:42:03,320 --> 00:42:07,640 Speaker 2: It kind of looks like a flower or like a 795 00:42:07,719 --> 00:42:09,600 Speaker 2: drawing of a sun where you kind of make the 796 00:42:09,640 --> 00:42:12,560 Speaker 2: outsides a little spiky, but yeah, it is pretty round, 797 00:42:12,640 --> 00:42:16,280 Speaker 2: and you've got like this bright white point in the middle, 798 00:42:16,480 --> 00:42:19,160 Speaker 2: and then you've got sort of a blue corona around it, 799 00:42:19,200 --> 00:42:22,560 Speaker 2: and then a larger white corona around the blue. What 800 00:42:22,719 --> 00:42:24,440 Speaker 2: is that sort of color difference. Why do you have 801 00:42:24,520 --> 00:42:27,319 Speaker 2: that like bright white light and then this blue and 802 00:42:27,360 --> 00:42:30,400 Speaker 2: then bright white light again on the outer edges. 803 00:42:30,680 --> 00:42:32,640 Speaker 1: Yeah. I think it's similar to the effects we were 804 00:42:32,680 --> 00:42:35,920 Speaker 1: talking about in the atmosphere, that there is some debris 805 00:42:35,920 --> 00:42:37,960 Speaker 1: that comes out of the explosion, and then the radiation 806 00:42:38,040 --> 00:42:40,880 Speaker 1: that's emitted after that is partially absorbed by some of 807 00:42:40,920 --> 00:42:43,680 Speaker 1: that debris, some of those heavier ions that are created 808 00:42:43,719 --> 00:42:46,600 Speaker 1: by the explosion, So you get this multiple effect with 809 00:42:46,760 --> 00:42:50,200 Speaker 1: the products of the explosion then absorb things that are 810 00:42:50,239 --> 00:42:53,200 Speaker 1: later produced in the latter stages of the explosion. And 811 00:42:53,239 --> 00:42:55,280 Speaker 1: it was a pretty dramatic event on Earth. 812 00:42:55,600 --> 00:42:58,280 Speaker 2: Yeah, I mean where people told this was going to happen. 813 00:42:58,440 --> 00:43:00,359 Speaker 1: People were told it was going to happen, and even 814 00:43:00,400 --> 00:43:02,600 Speaker 1: the newspapers were aware, and they kind of advertised it. 815 00:43:02,600 --> 00:43:06,280 Speaker 1: There's a headline in the Honolulu Advertiser, which is a newspaper, 816 00:43:06,280 --> 00:43:10,720 Speaker 1: which says, in blast night maybe dazzling, good view likely, 817 00:43:10,800 --> 00:43:13,400 Speaker 1: And a bunch of hotels in Hawaii had like rooftop 818 00:43:13,440 --> 00:43:16,360 Speaker 1: parties for people to watch this nuclear explosion happen. 819 00:43:16,680 --> 00:43:20,360 Speaker 2: I would be in a basement, but what would it 820 00:43:20,440 --> 00:43:24,160 Speaker 2: look like to someone on one of these rooftop parties. 821 00:43:24,400 --> 00:43:27,399 Speaker 1: So you can't see the actual explosion the same way 822 00:43:27,440 --> 00:43:30,000 Speaker 1: because of the atmosphere, but there aren't these great pictures 823 00:43:30,000 --> 00:43:32,799 Speaker 1: that people took from Hawaii. And you see all this 824 00:43:32,920 --> 00:43:35,719 Speaker 1: air glow. You see all this red light because the 825 00:43:35,800 --> 00:43:38,399 Speaker 1: radiation has hit the atmosphere and it's excited a bunch 826 00:43:38,400 --> 00:43:41,920 Speaker 1: of oxygen atoms which then glow. So it's basically like 827 00:43:42,160 --> 00:43:45,600 Speaker 1: heated up the atmosphere which then glows in this red light. 828 00:43:45,840 --> 00:43:49,080 Speaker 2: I mean that seems spectacular but also maybe kind of 829 00:43:49,080 --> 00:43:51,680 Speaker 2: apocalyptic looking. That would scare me. 830 00:43:52,040 --> 00:43:55,120 Speaker 1: Yeah, And then after the actual explosion there's a massive 831 00:43:55,160 --> 00:43:58,480 Speaker 1: aurora scene for like thousands of kilometers. You know, the 832 00:43:58,600 --> 00:44:02,040 Speaker 1: Northern Lights. These are high energy particles hitting the atmosphere. 833 00:44:02,120 --> 00:44:05,480 Speaker 1: They're mostly funneled up to the Northern and Southern poles 834 00:44:05,520 --> 00:44:07,960 Speaker 1: because of the magnetic field. But when a huge number 835 00:44:07,960 --> 00:44:10,840 Speaker 1: of high energy photons hit the atmosphere, they make the 836 00:44:10,840 --> 00:44:13,000 Speaker 1: atmosphere glow and you don't just get red, you get 837 00:44:13,040 --> 00:44:15,640 Speaker 1: greens and blues depending on exactly what it is that 838 00:44:15,680 --> 00:44:18,880 Speaker 1: has been like zapped and energized and then re emitted. 839 00:44:19,360 --> 00:44:23,400 Speaker 1: And so whereas you don't normally see auroras in Honolulu, 840 00:44:23,760 --> 00:44:26,520 Speaker 1: they had this massive aurora which stretched for thousands of 841 00:44:26,600 --> 00:44:28,040 Speaker 1: kilometers over the Pacific. 842 00:44:28,200 --> 00:44:31,360 Speaker 2: Well, maybe worth it to take a chance to accidentally 843 00:44:31,840 --> 00:44:34,640 Speaker 2: blow up a bunch of people, But you did mention 844 00:44:35,040 --> 00:44:40,080 Speaker 2: that the scientists had not quite calculated this right, So 845 00:44:40,400 --> 00:44:43,640 Speaker 2: were people actually in danger here? Like was there some 846 00:44:44,520 --> 00:44:45,960 Speaker 2: negative consequences to this? 847 00:44:46,320 --> 00:44:48,720 Speaker 1: Well, it like blew out street lights in Hawaii? 848 00:44:48,880 --> 00:44:49,560 Speaker 2: Oh wow, So this. 849 00:44:49,560 --> 00:44:52,680 Speaker 1: Electromagnetic pulse that was created went much further than the 850 00:44:52,719 --> 00:44:55,520 Speaker 1: scientists thought. I think they didn't realize how much of 851 00:44:55,560 --> 00:44:58,080 Speaker 1: that is absorbed by the atmosphere when you blow this 852 00:44:58,160 --> 00:45:00,680 Speaker 1: thing up on Earth, or when you blow it up underwater. 853 00:45:01,239 --> 00:45:03,840 Speaker 1: And so the radiation effects of this bomb in space 854 00:45:03,920 --> 00:45:07,120 Speaker 1: were much broader than they had anticipated. And so, yeah, 855 00:45:07,160 --> 00:45:09,480 Speaker 1: there were effects on Hawaii. They destroyed a bunch of 856 00:45:09,520 --> 00:45:12,200 Speaker 1: satellites that were up in space. Back then, there weren't 857 00:45:12,200 --> 00:45:14,680 Speaker 1: that many satellites. This is the beginning of the space era, 858 00:45:14,760 --> 00:45:18,360 Speaker 1: so only like six satellites were destroyed. These days, you 859 00:45:18,360 --> 00:45:20,200 Speaker 1: blew up a nuclear weapon and that kind of location, 860 00:45:20,400 --> 00:45:24,400 Speaker 1: you destroyed dozens of satellites, billions of dollars of damage, 861 00:45:24,440 --> 00:45:26,600 Speaker 1: and people were able to see this thing for like 862 00:45:26,719 --> 00:45:30,080 Speaker 1: thousands of miles away. People on Fiji described the light 863 00:45:30,120 --> 00:45:31,399 Speaker 1: show as breathtaking. 864 00:45:31,600 --> 00:45:34,840 Speaker 2: Wow. I mean, so you mentioned that the radiation spread 865 00:45:34,840 --> 00:45:38,160 Speaker 2: out much further than they had suspected. Did that negatively 866 00:45:38,200 --> 00:45:41,640 Speaker 2: impact Hawaiians? Did that hurt people on the island or 867 00:45:41,680 --> 00:45:44,960 Speaker 2: did it not actually have too much of a human impact. 868 00:45:45,120 --> 00:45:47,240 Speaker 1: It doesn't have very much of a human impact because 869 00:45:47,280 --> 00:45:49,840 Speaker 1: fortunately we are under the atmosphere, which is a really 870 00:45:49,840 --> 00:45:53,160 Speaker 1: thick blanket to protect ourselves from a lot of this radiation. 871 00:45:53,360 --> 00:45:55,920 Speaker 1: And so really the only impact in Hawaii was the 872 00:45:55,960 --> 00:45:59,319 Speaker 1: dramatic light show and the pulse from the EMP, which 873 00:45:59,400 --> 00:46:02,279 Speaker 1: damaged some electrical devices and blew out street lights and 874 00:46:02,600 --> 00:46:05,239 Speaker 1: dumped a bunch of energy basically in any conductor that 875 00:46:05,239 --> 00:46:09,120 Speaker 1: can absorb electromagnetic energy for hundreds of kilometers, and so 876 00:46:09,239 --> 00:46:12,719 Speaker 1: satellights and street lights are basically the only real damage. 877 00:46:12,760 --> 00:46:16,000 Speaker 1: There may also be some very small amounts of radioactive material, 878 00:46:16,200 --> 00:46:19,560 Speaker 1: but distributed over such a large area that doubt has 879 00:46:19,600 --> 00:46:21,680 Speaker 1: really any impact on it, like human life. 880 00:46:21,800 --> 00:46:25,719 Speaker 2: Well, it could have gone worse, it could have been. 881 00:46:25,640 --> 00:46:28,160 Speaker 1: Wronger, and actually some scientists were wondering if this was 882 00:46:28,200 --> 00:46:31,120 Speaker 1: going to have a long lasting effect on other features 883 00:46:31,160 --> 00:46:34,719 Speaker 1: of nearby space. Remember that near the Earth there are 884 00:46:34,760 --> 00:46:38,280 Speaker 1: these huge bands of radiation. They're called the Van Allen Belts, 885 00:46:38,719 --> 00:46:41,720 Speaker 1: and they're basically just particles like whizzing around the Earth 886 00:46:41,719 --> 00:46:44,600 Speaker 1: that were discovered in the fifties whence we sent up 887 00:46:44,600 --> 00:46:47,000 Speaker 1: our first space missions. That as you leave the Earth 888 00:46:47,000 --> 00:46:49,920 Speaker 1: you pass through these bands of massive radiation. There's an 889 00:46:49,920 --> 00:46:52,319 Speaker 1: inner belt and there's an outer belt. They're not very 890 00:46:52,320 --> 00:46:54,680 Speaker 1: well understood, and at the time they were seen as 891 00:46:54,719 --> 00:46:56,680 Speaker 1: like an impediment to space travel, that if you go 892 00:46:56,760 --> 00:46:59,480 Speaker 1: up into space, you have to survive passage through these 893 00:46:59,520 --> 00:47:03,640 Speaker 1: basically radiation guns. And some scientists were wondering, if we 894 00:47:03,719 --> 00:47:06,640 Speaker 1: blow up a nuclear weapon in these radiation belts, maybe 895 00:47:06,640 --> 00:47:09,320 Speaker 1: it would like disturb them or dissipate them, though some 896 00:47:09,360 --> 00:47:11,719 Speaker 1: people were sort of hopeful that it would blow up 897 00:47:11,719 --> 00:47:13,680 Speaker 1: the radiation belts, which to me is kind of crazy. 898 00:47:13,680 --> 00:47:16,080 Speaker 1: It's like, before you even really understand these things and 899 00:47:16,120 --> 00:47:18,759 Speaker 1: their purpose and their benefits and their detriments, you want 900 00:47:18,800 --> 00:47:20,880 Speaker 1: to just like blow them up and see what happens 901 00:47:20,920 --> 00:47:21,760 Speaker 1: to life on Earth. 902 00:47:22,080 --> 00:47:25,040 Speaker 2: Yeah, I mean, it's kind of looking forward and not 903 00:47:25,239 --> 00:47:28,960 Speaker 2: looking at the current situation right because you're thinking, like, 904 00:47:29,080 --> 00:47:33,319 Speaker 2: let's make space travel easier. But we have this functional 905 00:47:33,400 --> 00:47:36,480 Speaker 2: planet that we're pretty cozy on, so you might not 906 00:47:36,680 --> 00:47:39,520 Speaker 2: want to mess that up for some kind of future 907 00:47:39,600 --> 00:47:42,279 Speaker 2: space highway. I think that it is a lot of 908 00:47:42,440 --> 00:47:44,920 Speaker 2: decisions that we make we don't often think about, like, 909 00:47:45,000 --> 00:47:49,000 Speaker 2: but how will this impact the planet before we build 910 00:47:49,000 --> 00:47:53,640 Speaker 2: this space highway or regular highway? Did it impact these 911 00:47:53,840 --> 00:47:57,160 Speaker 2: radiation belts or did it not really have a permanent impact. 912 00:47:57,280 --> 00:47:59,680 Speaker 1: I had basically no impact on the radiation belts, which 913 00:47:59,719 --> 00:48:02,080 Speaker 1: contain an enormous amount of energy which could not be 914 00:48:02,120 --> 00:48:05,279 Speaker 1: affected by one nuclear bomb. But this nuclear explosion did 915 00:48:05,360 --> 00:48:08,840 Speaker 1: have sort of shockwaves through the political climate on Earth. 916 00:48:09,120 --> 00:48:11,560 Speaker 1: Things cooled down a little bit, and in nineteen sixty 917 00:48:11,600 --> 00:48:14,960 Speaker 1: three they passed a partial Test Ban treaty which prohibited 918 00:48:15,080 --> 00:48:19,160 Speaker 1: all nuclear testing except for underground testing, which was seen 919 00:48:19,280 --> 00:48:23,319 Speaker 1: as safer because it really is very well contained. And 920 00:48:23,400 --> 00:48:26,320 Speaker 1: so for about thirty years, the US and Soviet Union 921 00:48:26,360 --> 00:48:29,400 Speaker 1: did a bunch of underground tests until they were prohibited 922 00:48:29,440 --> 00:48:33,040 Speaker 1: in nineteen ninety six. I still remember my dad traveling 923 00:48:33,080 --> 00:48:35,960 Speaker 1: to the Nevada test site to participate in some of 924 00:48:36,000 --> 00:48:39,680 Speaker 1: those tests. So the US was still testing nuclear weapons 925 00:48:39,719 --> 00:48:42,319 Speaker 1: into the nineties. We have not blown one up since then. 926 00:48:42,360 --> 00:48:45,440 Speaker 1: The last nuclear test from the US was in the nineties. 927 00:48:45,800 --> 00:48:48,680 Speaker 2: It really feels like such a scary time though, during 928 00:48:48,719 --> 00:48:51,719 Speaker 2: the Cold War, when you're having all these tests going on, 929 00:48:51,800 --> 00:48:54,200 Speaker 2: you wonder about how many close calls we had in 930 00:48:54,280 --> 00:48:57,560 Speaker 2: terms of a test going wrong where it actually hurts people, 931 00:48:57,800 --> 00:49:02,879 Speaker 2: or a test that happens is misread by like say 932 00:49:02,920 --> 00:49:06,000 Speaker 2: that Russians are you know, by the US, and we think, well, 933 00:49:06,120 --> 00:49:10,080 Speaker 2: we're being attacked and that starts a whole cascade of nukes. 934 00:49:10,160 --> 00:49:13,080 Speaker 2: It feels like this wild West time where we were 935 00:49:13,120 --> 00:49:16,440 Speaker 2: just i mean, maybe not playing around with nukes, but 936 00:49:17,080 --> 00:49:19,640 Speaker 2: the fact we were doing so many of these tests, 937 00:49:19,680 --> 00:49:23,560 Speaker 2: and it feels like we just kind of escaped some 938 00:49:23,640 --> 00:49:26,120 Speaker 2: kind of horrible fate by the skin of our teeth. 939 00:49:26,480 --> 00:49:28,920 Speaker 1: We certainly did. If you dig too deep into his history, 940 00:49:28,960 --> 00:49:31,600 Speaker 1: it's terrifying. There were times when like a flock of 941 00:49:31,640 --> 00:49:34,520 Speaker 1: seagulls were mistaken for the launch of a nuclear weapon. 942 00:49:35,000 --> 00:49:38,600 Speaker 1: Another time when like a training tape was accidentally loaded 943 00:49:38,600 --> 00:49:41,279 Speaker 1: into a computer which became convinced that the Russians were 944 00:49:41,280 --> 00:49:44,759 Speaker 1: attacking us. It's really terrifying how close we came to 945 00:49:44,920 --> 00:49:47,799 Speaker 1: all out nuclear war several times. And you know, the 946 00:49:47,880 --> 00:49:51,160 Speaker 1: US and the USSR haven't tested nuclear weapons since the nineties, 947 00:49:51,360 --> 00:49:54,120 Speaker 1: but you know, India and Pakistan detonated nuclear weapons in 948 00:49:54,160 --> 00:49:56,840 Speaker 1: the very late nineties, and then of course North Korea 949 00:49:57,160 --> 00:50:00,879 Speaker 1: has done tests fairly recently of nuclear weapons. So it's 950 00:50:00,920 --> 00:50:02,719 Speaker 1: not like we're out of the woods in terms of 951 00:50:02,800 --> 00:50:08,200 Speaker 1: nuclear weapons. Nope, yeah, exactly. Israel actually is the only 952 00:50:08,239 --> 00:50:10,879 Speaker 1: country we think has nuclear weapons but has never done 953 00:50:10,920 --> 00:50:13,680 Speaker 1: a nuclear test that we know of, that we know of. 954 00:50:14,080 --> 00:50:17,920 Speaker 2: Yeah, I mean, it's interesting because at the start of 955 00:50:18,080 --> 00:50:21,799 Speaker 2: the Russian Ukraine War, I started following a bunch of 956 00:50:22,080 --> 00:50:28,759 Speaker 2: nuclear proliferation experts and sort of people who understood the politics, 957 00:50:28,760 --> 00:50:32,000 Speaker 2: who understood the science of nukes, because I was terrified, 958 00:50:32,280 --> 00:50:35,720 Speaker 2: and I'm not gonna say I got less terrified after 959 00:50:36,200 --> 00:50:38,960 Speaker 2: hearing what the experts had to say. I think the 960 00:50:39,200 --> 00:50:43,160 Speaker 2: knowledge of exactly the kind of circumstances that we were 961 00:50:43,200 --> 00:50:46,120 Speaker 2: in and stuff was helpful. Like, even though the Cold 962 00:50:46,160 --> 00:50:48,719 Speaker 2: War is over, the fact that there are so many 963 00:50:48,880 --> 00:50:52,200 Speaker 2: nukes out there, it's terrifying, so we should probably send 964 00:50:52,239 --> 00:50:54,920 Speaker 2: them all the space blaw them all up put them 965 00:50:54,960 --> 00:50:55,360 Speaker 2: in space. 966 00:50:55,719 --> 00:50:57,399 Speaker 1: I guess if I had to choose where to blow 967 00:50:57,440 --> 00:50:59,400 Speaker 1: up nuclear bombs, I probably choose to blow them up 968 00:50:59,440 --> 00:51:02,720 Speaker 1: in space, over the atmosphere or anywhere else on Earth. 969 00:51:02,760 --> 00:51:05,560 Speaker 1: But it is really interesting to understand what happens to 970 00:51:05,600 --> 00:51:07,239 Speaker 1: a nuclear bomb when you blow it up in space. 971 00:51:07,280 --> 00:51:09,720 Speaker 1: It turns out to be quite different from what happens 972 00:51:09,800 --> 00:51:13,000 Speaker 1: in our atmosphere. It doesn't dump that energy and create 973 00:51:13,080 --> 00:51:16,000 Speaker 1: a shock wave. It's basically like a little miniature sun, 974 00:51:16,080 --> 00:51:17,880 Speaker 1: and so there is no shockwave to hurt you, but 975 00:51:17,920 --> 00:51:21,560 Speaker 1: that radiation will travel much much further and damage things 976 00:51:21,600 --> 00:51:25,759 Speaker 1: that are much further away, especially electronics. So let's hope 977 00:51:25,760 --> 00:51:28,279 Speaker 1: that we don't end up in a nuclear space war 978 00:51:28,400 --> 00:51:29,239 Speaker 1: anytime soon. 979 00:51:29,480 --> 00:51:32,040 Speaker 2: And if you're flying your spaceship and you want to 980 00:51:32,440 --> 00:51:35,600 Speaker 2: fire some nukes, wear sunglasses. 981 00:51:35,080 --> 00:51:37,319 Speaker 1: And be careful microwaving your soup, and put a lid 982 00:51:37,320 --> 00:51:39,600 Speaker 1: on your blender when you make that strawberry smoothie. 983 00:51:39,640 --> 00:51:41,280 Speaker 2: All of this is practical advice. 984 00:51:42,239 --> 00:51:45,840 Speaker 1: Thanks Katie very much for joining us on this exclusive episode, 985 00:51:46,000 --> 00:51:48,320 Speaker 1: Thanks for having me, and thanks to all of our listeners. 986 00:51:48,600 --> 00:51:59,000 Speaker 1: Tune in next time. Thanks for listening, and remember that 987 00:51:59,160 --> 00:52:03,000 Speaker 1: Daniel and Jorge Explain the Universe is a production of iHeartRadio. 988 00:52:03,239 --> 00:52:08,400 Speaker 1: For more podcasts from iHeartRadio, visit the iHeartRadio app, Apple Podcasts, 989 00:52:08,520 --> 00:52:10,880 Speaker 1: or wherever you listen to your favorite shows.