1 00:00:09,000 --> 00:00:11,080 Speaker 1: Hey, Daniel, what do you think will happen the day 2 00:00:11,200 --> 00:00:15,000 Speaker 1: we discover alien life? Oh? I'm imagining like a huge 3 00:00:15,240 --> 00:00:18,800 Speaker 1: worldwide celebration. Oh yeah, and you think it'll be good news. Yeah, 4 00:00:18,920 --> 00:00:22,280 Speaker 1: I think we'll learn something very deep and important about 5 00:00:22,320 --> 00:00:25,319 Speaker 1: the nature of life and the universe and everything. But 6 00:00:25,400 --> 00:00:27,400 Speaker 1: what if it's not good news? What do you considered 7 00:00:27,800 --> 00:00:31,840 Speaker 1: darker possibilities about alien life? Like if they're not friendly 8 00:00:31,840 --> 00:00:34,479 Speaker 1: to humans they show up in space and zappaus, Well, 9 00:00:34,479 --> 00:00:36,639 Speaker 1: they could be friendly to humans. You know, they might 10 00:00:36,640 --> 00:00:38,839 Speaker 1: find us delicious. I guess that depends on which kind 11 00:00:38,840 --> 00:00:41,760 Speaker 1: of humans they find delicious. We probably all taste the same, 12 00:00:41,880 --> 00:00:47,000 Speaker 1: you know, like chicken. Maybe chickens taste like humans. I'm 13 00:00:47,040 --> 00:00:49,239 Speaker 1: sure there are people in this world who know the 14 00:00:49,360 --> 00:00:52,040 Speaker 1: answer to that question. What if we find out about 15 00:00:52,080 --> 00:00:55,480 Speaker 1: aliens because of some giant space battle they're having with themselves. 16 00:00:55,640 --> 00:00:58,080 Speaker 1: Oh well, that sounds pretty exciting. In that case, I'd 17 00:00:58,160 --> 00:01:01,480 Speaker 1: like to reserve a front row seat. Well really, Oh 18 00:01:01,640 --> 00:01:04,160 Speaker 1: you do that, I'll be running away in the other direction, 19 00:01:05,160 --> 00:01:22,920 Speaker 1: and I'll be popping the popcorn. Hi, am Orham and 20 00:01:23,000 --> 00:01:26,160 Speaker 1: cartoonists and the creator of PhD comments. Hi, I'm Daniel 21 00:01:26,200 --> 00:01:29,360 Speaker 1: I'm a particle physicist and a professor at UC Irvine, 22 00:01:29,560 --> 00:01:32,520 Speaker 1: and I don't wish any aliens to die, but I 23 00:01:32,600 --> 00:01:35,600 Speaker 1: do want to see a giant alien space battle. Wait, 24 00:01:35,640 --> 00:01:37,679 Speaker 1: so how would they have a battle but without any 25 00:01:37,680 --> 00:01:41,119 Speaker 1: even dying. Isn't just like a virtual battle or they're 26 00:01:41,160 --> 00:01:43,600 Speaker 1: like plane laser tag? What are you talking about here? 27 00:01:43,959 --> 00:01:45,880 Speaker 1: I mean it's like a wortal battle. Are they having 28 00:01:45,920 --> 00:01:48,919 Speaker 1: a wortal battle? Maybe they've evolved to a higher plane 29 00:01:48,920 --> 00:01:51,880 Speaker 1: of combat exactly. No, it's tension within me. As much 30 00:01:51,920 --> 00:01:54,240 Speaker 1: as I would like to see alien space battles, I 31 00:01:54,280 --> 00:01:56,760 Speaker 1: also don't want any aliens out there to die. But 32 00:01:56,800 --> 00:01:59,280 Speaker 1: you know some of our favorite stories are about alien 33 00:01:59,320 --> 00:02:01,600 Speaker 1: space battles. Isn't that what Star Wars is all about. 34 00:02:02,280 --> 00:02:04,920 Speaker 1: Star Wars is about aliens. That's what you told me. 35 00:02:04,920 --> 00:02:08,079 Speaker 1: It's in another galaxy, far far away, right, they're all aliens. 36 00:02:08,480 --> 00:02:12,120 Speaker 1: Maybe we're the aliens in the Star Wars universe. Well, 37 00:02:12,120 --> 00:02:15,000 Speaker 1: we're not capable of putting on giant space battles yet. Also, 38 00:02:15,040 --> 00:02:17,040 Speaker 1: people don't die in Star Wars. They just come back 39 00:02:17,080 --> 00:02:21,359 Speaker 1: as ghosts, Jedi ghosts more powerful than you could even imagine, 40 00:02:21,480 --> 00:02:23,000 Speaker 1: Or do you the Emperor did they just keep bringing 41 00:02:23,000 --> 00:02:25,639 Speaker 1: you back for all the movies. Don't the Stormtrooper die though, 42 00:02:25,720 --> 00:02:28,160 Speaker 1: or do they also come back as Jedi ghosts. I 43 00:02:28,200 --> 00:02:30,440 Speaker 1: guess it's not clear. You know, they get zapped with 44 00:02:30,480 --> 00:02:32,519 Speaker 1: their little armor and they just fall down. Maybe they're 45 00:02:32,560 --> 00:02:34,280 Speaker 1: just taking a nap. There you go. I'd like a 46 00:02:34,320 --> 00:02:37,680 Speaker 1: giant alien space battle where the losers just take a nap. Yeah, 47 00:02:37,760 --> 00:02:41,359 Speaker 1: I want to see that movie. Star naps were Welcome 48 00:02:41,360 --> 00:02:43,920 Speaker 1: to our podcast Daniel and Jorge Explain the Universe, a 49 00:02:44,000 --> 00:02:47,079 Speaker 1: production of iHeartRadio, in which we try to zap your 50 00:02:47,160 --> 00:02:50,960 Speaker 1: brain with all sorts of incredible information about the universe. 51 00:02:51,120 --> 00:02:54,600 Speaker 1: We know that everything out there is amazing and mysterious 52 00:02:54,760 --> 00:02:58,760 Speaker 1: and confusing, but we hope to help you understand what 53 00:02:58,960 --> 00:03:02,400 Speaker 1: little of it human entity has managed to decode. And 54 00:03:02,440 --> 00:03:04,960 Speaker 1: we hope that one day aliens come and give us 55 00:03:05,000 --> 00:03:07,440 Speaker 1: a little bit more information about what's going on out 56 00:03:07,440 --> 00:03:10,960 Speaker 1: there in the universe, if indeed they do exist. That's right, 57 00:03:11,000 --> 00:03:14,160 Speaker 1: because it is a pretty incredible universe, and we do 58 00:03:14,240 --> 00:03:17,800 Speaker 1: battle every day here with the mysteries of it, and 59 00:03:17,840 --> 00:03:20,440 Speaker 1: we go to war with our ignorance about how it 60 00:03:20,440 --> 00:03:23,000 Speaker 1: works and what's going on in the universe. We're trying 61 00:03:23,000 --> 00:03:25,920 Speaker 1: to drop a knowledge bomb on everybody's ignorance. That's right. 62 00:03:26,200 --> 00:03:28,320 Speaker 1: You can think of us as a laser gun of 63 00:03:28,360 --> 00:03:33,680 Speaker 1: amazing facts zapping people's brains. There's that warm, fuzzy feeling 64 00:03:33,720 --> 00:03:36,840 Speaker 1: you get when you understand something about the universe. But 65 00:03:36,880 --> 00:03:39,560 Speaker 1: there's also lots of things that we still don't understand 66 00:03:39,560 --> 00:03:43,040 Speaker 1: about the universe, things that give you that gnawing feeling 67 00:03:43,080 --> 00:03:47,000 Speaker 1: of desperate curiosity, that desire to just know what's going 68 00:03:47,120 --> 00:03:49,720 Speaker 1: on out there. There's some of the deepest questions in 69 00:03:49,840 --> 00:03:53,920 Speaker 1: human existence which have answers, which are facts about the 70 00:03:54,000 --> 00:03:57,920 Speaker 1: universe which maybe one day people will know. How frustrating 71 00:03:58,000 --> 00:04:00,360 Speaker 1: is it to live in the era of dark to 72 00:04:00,520 --> 00:04:03,240 Speaker 1: not know the answers to basic questions like are we 73 00:04:03,320 --> 00:04:06,839 Speaker 1: alone in the universe? Yeah? What bigger question can there 74 00:04:06,880 --> 00:04:10,240 Speaker 1: be about the existence of humans than the question of 75 00:04:10,280 --> 00:04:14,720 Speaker 1: whether we are the only living thing or intelligent thing 76 00:04:14,920 --> 00:04:18,320 Speaker 1: living and existing in this universe? And we wonder about it, 77 00:04:18,400 --> 00:04:21,120 Speaker 1: we speculate about it, but we have a very very 78 00:04:21,240 --> 00:04:25,320 Speaker 1: deep lack of information about it. The universe is vast, 79 00:04:25,480 --> 00:04:27,800 Speaker 1: and from our tiny little rock we have done a 80 00:04:27,839 --> 00:04:31,600 Speaker 1: pretty good job of exploring a tiny, little corner of it. 81 00:04:31,680 --> 00:04:34,520 Speaker 1: We have telescopes to tell us about nearby star systems 82 00:04:34,520 --> 00:04:37,800 Speaker 1: and compeer further and deeper into the universe, but we've 83 00:04:37,839 --> 00:04:42,120 Speaker 1: only begun recently to identify other planets and other places 84 00:04:42,120 --> 00:04:46,760 Speaker 1: in the universe where life might spring independently from Earth. Yeah, 85 00:04:46,839 --> 00:04:48,680 Speaker 1: we know that here in our Solar systems there aren't 86 00:04:48,680 --> 00:04:50,839 Speaker 1: on at the signs of life, and so we know 87 00:04:50,920 --> 00:04:52,960 Speaker 1: that if there is alien life out there, it has 88 00:04:53,000 --> 00:04:55,560 Speaker 1: to be kind of far away. Right, how close is 89 00:04:55,600 --> 00:04:58,200 Speaker 1: the nearest planet to us light years away? The nearest 90 00:04:58,200 --> 00:05:00,800 Speaker 1: planet to me is about zero meters away. It's right 91 00:05:00,839 --> 00:05:03,200 Speaker 1: here under my feet. There are other places in the 92 00:05:03,240 --> 00:05:06,480 Speaker 1: Solar System people think there might be life, like under 93 00:05:06,520 --> 00:05:09,760 Speaker 1: the frozen crust of Europa. So there are still exciting 94 00:05:09,800 --> 00:05:13,080 Speaker 1: places in our backyard. But you're right, other Solar systems 95 00:05:13,120 --> 00:05:17,720 Speaker 1: are frustratingly far away, several light years. The closest identified 96 00:05:17,760 --> 00:05:21,800 Speaker 1: exoplanets around Proxima Centauri, which happens to be their closest star, 97 00:05:22,200 --> 00:05:24,919 Speaker 1: just under four light years away. And what that tells 98 00:05:24,960 --> 00:05:28,000 Speaker 1: us is that there are planets everywhere in the galaxy 99 00:05:28,120 --> 00:05:31,239 Speaker 1: and in the universe. We now think that almost every 100 00:05:31,279 --> 00:05:33,799 Speaker 1: star out there has planets around it, and a huge 101 00:05:33,839 --> 00:05:37,960 Speaker 1: fraction of them have even earthlike planets, maybe around this size, 102 00:05:38,040 --> 00:05:41,160 Speaker 1: maybe around this kind of surface temperature, maybe even with 103 00:05:41,279 --> 00:05:44,320 Speaker 1: liquid water on their surface. And so with so many 104 00:05:44,400 --> 00:05:46,960 Speaker 1: places that life could be out there in the universe, 105 00:05:47,279 --> 00:05:51,520 Speaker 1: sometimes we wonder, why haven't we found it already. Yeah, 106 00:05:51,560 --> 00:05:54,479 Speaker 1: it's a very big question, one that would kind of 107 00:05:54,480 --> 00:05:57,720 Speaker 1: determine our place in the universe. Because if the answer 108 00:05:57,839 --> 00:06:00,200 Speaker 1: is that there isn't life out there, that is that 109 00:06:00,520 --> 00:06:04,000 Speaker 1: humans are pretty special right in the entire universe. Imagine 110 00:06:04,000 --> 00:06:05,919 Speaker 1: what it'd be like to know that we're the only 111 00:06:05,920 --> 00:06:08,680 Speaker 1: intelligence species in such a big place. Yeah, it would 112 00:06:08,680 --> 00:06:11,000 Speaker 1: make you feel special. It'll also make you feel kind 113 00:06:11,040 --> 00:06:14,760 Speaker 1: of lonely being the only intelligent life in the entire universe. 114 00:06:14,760 --> 00:06:17,880 Speaker 1: It's kind of a lot of responsibility also, like we're 115 00:06:17,920 --> 00:06:20,240 Speaker 1: the only ones out there doing anythinking. We're the only 116 00:06:20,240 --> 00:06:22,600 Speaker 1: ones trying to figure out this huge puzzle about the 117 00:06:22,680 --> 00:06:25,239 Speaker 1: nature of the universe, trying to crack the cosmic mystery 118 00:06:25,360 --> 00:06:28,880 Speaker 1: of how all these quantum particles weave themselves together into 119 00:06:29,000 --> 00:06:32,080 Speaker 1: this experience. I prefer to imagine that there's lots of 120 00:06:32,080 --> 00:06:34,760 Speaker 1: other civilizations out there, and maybe they've even solved some 121 00:06:34,800 --> 00:06:38,120 Speaker 1: of these questions and have the answers waiting for us. 122 00:06:38,560 --> 00:06:41,000 Speaker 1: But we don't know. And we've been looking out in 123 00:06:41,080 --> 00:06:45,359 Speaker 1: the cosmos and listening for signals from aliens, hoping that 124 00:06:45,400 --> 00:06:48,320 Speaker 1: they are as excited as we are to meet their neighbors, 125 00:06:48,320 --> 00:06:51,480 Speaker 1: and sending us messages which we might capture in radio 126 00:06:51,520 --> 00:06:55,520 Speaker 1: waves or other electromagnetic signals. Of course, so far we've 127 00:06:55,560 --> 00:06:58,640 Speaker 1: heard nothing conclusive. Wait, so you want aliens to exist 128 00:06:58,800 --> 00:07:01,039 Speaker 1: just to take some of the pressure off of your job. 129 00:07:01,240 --> 00:07:05,000 Speaker 1: Is that kind of what you're you're talking about? You know, 130 00:07:05,040 --> 00:07:08,920 Speaker 1: I'm very strongly believe in funding basic research and expanding science, 131 00:07:09,000 --> 00:07:11,840 Speaker 1: and that goes beyond the limits of our species. I 132 00:07:11,880 --> 00:07:15,280 Speaker 1: think science should be funded here on Earth and everywhere 133 00:07:15,400 --> 00:07:18,960 Speaker 1: in the universe, and I hope that budget aliens out 134 00:07:18,960 --> 00:07:22,239 Speaker 1: there are, you know, giving a healthy dose of funding 135 00:07:22,320 --> 00:07:26,200 Speaker 1: to those science aliens out there struggling to understand the 136 00:07:26,320 --> 00:07:29,080 Speaker 1: nature of the universe, burned by the same curiosity that 137 00:07:29,120 --> 00:07:31,680 Speaker 1: we have. Or maybe they don't. Maybe they just don't 138 00:07:31,680 --> 00:07:33,320 Speaker 1: care about the nature of the universe and they're not 139 00:07:33,360 --> 00:07:36,080 Speaker 1: even doing science. I feel like you're like little kid 140 00:07:36,120 --> 00:07:38,520 Speaker 1: in class who's looking at his test or her tests 141 00:07:38,520 --> 00:07:40,360 Speaker 1: and going like, I have no idea what's going on, 142 00:07:40,840 --> 00:07:43,480 Speaker 1: and you're sort of like looking around to see if 143 00:07:43,480 --> 00:07:46,400 Speaker 1: anyone else knows the answers. Yes, I definitely want to 144 00:07:46,480 --> 00:07:49,560 Speaker 1: cheat off of alien physicists. I would love to get 145 00:07:49,640 --> 00:07:52,080 Speaker 1: like an alien physics textbook and then win like a 146 00:07:52,080 --> 00:07:55,600 Speaker 1: whole string of Nobel prizes here on Earth just by 147 00:07:55,680 --> 00:07:58,960 Speaker 1: copying their ideas. Yes, I will completely admit that is 148 00:07:59,000 --> 00:08:02,240 Speaker 1: my fantasy. Really, So wait, you would get the secrets 149 00:08:02,240 --> 00:08:04,080 Speaker 1: from the alien I'm just trying to figure this scenario. 150 00:08:04,360 --> 00:08:06,560 Speaker 1: Let's work through it. You would get the secrets from 151 00:08:06,560 --> 00:08:08,920 Speaker 1: the aliens, but you wouldn't tell anyone that aliens exist, 152 00:08:09,400 --> 00:08:11,800 Speaker 1: and you would use that knowledge for your own personal game. 153 00:08:12,080 --> 00:08:17,320 Speaker 1: That sounds fantastic. Yes, remind me not to tell you 154 00:08:17,360 --> 00:08:20,320 Speaker 1: any secrets. Then, If you are holding a Nobel prize 155 00:08:20,320 --> 00:08:23,280 Speaker 1: winning secret, please do share it with me. I would 156 00:08:23,320 --> 00:08:25,040 Speaker 1: love to hear it. You would be the last person 157 00:08:25,080 --> 00:08:28,560 Speaker 1: I would share with, obviously. I hope you would share 158 00:08:28,560 --> 00:08:30,800 Speaker 1: it with all of humanity, Like if somebody gave me 159 00:08:30,920 --> 00:08:32,719 Speaker 1: secrets from aliens, I would share it with all of 160 00:08:32,800 --> 00:08:36,360 Speaker 1: humanity absolutely, But the aliens themselves would be the biggest secrets. 161 00:08:36,400 --> 00:08:39,440 Speaker 1: I just said it's the biggest question in human existence. No, 162 00:08:39,520 --> 00:08:41,560 Speaker 1: you're right, And of course, if aliens do come or 163 00:08:41,559 --> 00:08:44,920 Speaker 1: communicate with us, probably physicists wouldn't be at the front 164 00:08:44,920 --> 00:08:47,439 Speaker 1: of the line of people who get to chat with them, right, 165 00:08:47,480 --> 00:08:51,240 Speaker 1: probably would send like engineers or doctors, or politicians or 166 00:08:51,320 --> 00:08:55,400 Speaker 1: linguists or mathematicians or philosophers before the physicists even get 167 00:08:55,440 --> 00:08:57,720 Speaker 1: their shot. I think I would send the physicists first 168 00:08:57,840 --> 00:09:00,960 Speaker 1: for sure. Yeah, because you know what, if they're hungry, 169 00:09:02,760 --> 00:09:04,960 Speaker 1: we got to test the waters here. So you don't 170 00:09:04,960 --> 00:09:06,720 Speaker 1: want me to learn the secrets from the aliens, but 171 00:09:06,760 --> 00:09:08,880 Speaker 1: you do want me to be there first. I mean, 172 00:09:09,160 --> 00:09:11,560 Speaker 1: there's two sides to that coin. Well, I want you 173 00:09:11,600 --> 00:09:13,360 Speaker 1: to learn the secrets, but I want you to share 174 00:09:13,400 --> 00:09:17,280 Speaker 1: the secrets verybody. I will share the secrets with you 175 00:09:17,559 --> 00:09:20,360 Speaker 1: and the Nobel Committee. And if their secret is what 176 00:09:20,400 --> 00:09:23,360 Speaker 1: their stomachs look like, well, you know you can't share it, 177 00:09:23,400 --> 00:09:26,640 Speaker 1: but at least we would know. Just like going inside 178 00:09:26,640 --> 00:09:29,240 Speaker 1: a black hole, you learn some deep secrets about the universe, 179 00:09:29,320 --> 00:09:31,680 Speaker 1: but only you can know them. But it's interesting you 180 00:09:31,720 --> 00:09:34,400 Speaker 1: talk about some of the ways that people usually think 181 00:09:34,440 --> 00:09:37,480 Speaker 1: that we're gonna meet aliens or know about aliens, which 182 00:09:37,520 --> 00:09:39,520 Speaker 1: is getting signals from them. I mean that's sort of 183 00:09:39,520 --> 00:09:42,240 Speaker 1: like one way we can learn about them. I guess 184 00:09:42,280 --> 00:09:44,600 Speaker 1: another way is to go to another planet and see 185 00:09:44,600 --> 00:09:47,200 Speaker 1: them too, right, Yeah, And this is a really common 186 00:09:47,240 --> 00:09:50,040 Speaker 1: thing in science. When you have no idea how hard 187 00:09:50,200 --> 00:09:53,600 Speaker 1: a problem is, you start with the easiest things, like 188 00:09:53,840 --> 00:09:56,719 Speaker 1: maybe the universe is filled with aliens and they're all 189 00:09:56,720 --> 00:09:59,200 Speaker 1: sending messages and we just haven't been listening, and as 190 00:09:59,200 --> 00:10:03,280 Speaker 1: soon as we turn on our electronic ears and use 191 00:10:03,400 --> 00:10:06,640 Speaker 1: our radio satellites to tune in, maybe we could instantly 192 00:10:06,679 --> 00:10:10,120 Speaker 1: tap into the galactic internet and hear all those conversations. 193 00:10:10,200 --> 00:10:12,480 Speaker 1: There's some scenario in which it would have been easy, 194 00:10:12,720 --> 00:10:14,880 Speaker 1: and as soon as we started listening, we discovered it. 195 00:10:15,120 --> 00:10:17,600 Speaker 1: So it makes sense to first do the easy thing 196 00:10:17,679 --> 00:10:20,680 Speaker 1: and see if alien messages our feeling space. Of course, 197 00:10:20,720 --> 00:10:23,320 Speaker 1: we've been listening and we haven't heard anything, and so 198 00:10:23,440 --> 00:10:26,160 Speaker 1: people are starting to try to be creative and think about, like, well, 199 00:10:26,160 --> 00:10:28,800 Speaker 1: what are other ways we could hear from aliens, or 200 00:10:28,960 --> 00:10:31,480 Speaker 1: what are other ways we could detect their existence? As 201 00:10:31,480 --> 00:10:34,199 Speaker 1: you say, maybe we could go to those planets and 202 00:10:34,320 --> 00:10:37,560 Speaker 1: discover them. Right. That's limited, of course, by our ability 203 00:10:37,600 --> 00:10:40,560 Speaker 1: to travel from star to star. These stars are so 204 00:10:40,760 --> 00:10:43,560 Speaker 1: far away and the speed of light is such a 205 00:10:43,559 --> 00:10:46,760 Speaker 1: stubborn limitation. But until we develop a warp drives or 206 00:10:46,840 --> 00:10:50,240 Speaker 1: practical wormholes, it's not realistic to think that we could 207 00:10:50,240 --> 00:10:54,160 Speaker 1: explore a significant fraction of the galaxy. Yeah, Like, what 208 00:10:54,200 --> 00:10:56,120 Speaker 1: would it take, I guess to send a probe to 209 00:10:56,400 --> 00:10:59,600 Speaker 1: Alpha Centauri? Right, it's four light years away. That's like 210 00:11:00,040 --> 00:11:02,280 Speaker 1: zillions of miles away. Right now, it seems kind of 211 00:11:02,320 --> 00:11:05,480 Speaker 1: impossible because I think the furthest we've send a probe 212 00:11:05,559 --> 00:11:08,679 Speaker 1: right now is just barely outside this Solar system, right, 213 00:11:08,679 --> 00:11:11,319 Speaker 1: and it took like thirty years, yes, exactly, the most 214 00:11:11,360 --> 00:11:15,160 Speaker 1: distant object send by humanity. Some of these old Voyager 215 00:11:15,200 --> 00:11:18,520 Speaker 1: and Pioneer probes are not very far outside the Solar system, 216 00:11:18,800 --> 00:11:21,160 Speaker 1: so it would take a long time for anything to 217 00:11:21,200 --> 00:11:23,280 Speaker 1: get anywhere. But you know, if you were thinking about 218 00:11:23,320 --> 00:11:25,760 Speaker 1: it on long time scales, it's not going to take 219 00:11:25,800 --> 00:11:28,920 Speaker 1: like millions of years. We're talking like thousands or tens 220 00:11:28,920 --> 00:11:30,920 Speaker 1: of thousands of years. And if you send a few 221 00:11:31,000 --> 00:11:35,080 Speaker 1: probes to other planets, and if those probes are very clever, 222 00:11:35,280 --> 00:11:39,280 Speaker 1: they're like AI driven self replicating probes, so they can 223 00:11:39,640 --> 00:11:42,560 Speaker 1: land on some distant moon, they can find materials on 224 00:11:42,600 --> 00:11:45,400 Speaker 1: those moons to make more of themselves, and then they 225 00:11:45,400 --> 00:11:48,320 Speaker 1: can send those probes out, and those probes make more 226 00:11:48,360 --> 00:11:51,040 Speaker 1: of themselves, and those make more of themselves. It's not 227 00:11:51,120 --> 00:11:56,080 Speaker 1: impossible to imagine rapidly exploring the entire galaxy, where by 228 00:11:56,160 --> 00:11:58,360 Speaker 1: rapid we mean on the time scale of like fifty 229 00:11:58,400 --> 00:12:01,199 Speaker 1: to one hundred thousand years. So that's a really interesting 230 00:12:01,280 --> 00:12:04,800 Speaker 1: argument because it suggests that with technology not super far 231 00:12:04,840 --> 00:12:08,960 Speaker 1: in our future, some other civilization could have explored the 232 00:12:08,960 --> 00:12:12,160 Speaker 1: whole galaxy with self replicating probes. And then you have 233 00:12:12,200 --> 00:12:15,199 Speaker 1: to ask, like, well, why haven't we been visited by 234 00:12:15,240 --> 00:12:18,120 Speaker 1: such a probe yet? Are there no other advanced civilizations 235 00:12:18,160 --> 00:12:20,840 Speaker 1: out there who have this idea? Yeah, we address this 236 00:12:20,960 --> 00:12:23,520 Speaker 1: question and this whole scenario in our book. Frequently asked 237 00:12:23,559 --> 00:12:25,680 Speaker 1: questions about the universe. That was one of the chapters, 238 00:12:25,760 --> 00:12:29,400 Speaker 1: right like why haven't we seen aliens? And maybe we 239 00:12:29,440 --> 00:12:33,040 Speaker 1: can do that with these self repulating robots, which would 240 00:12:33,080 --> 00:12:37,160 Speaker 1: litter the universe in no time exactly. And one basic 241 00:12:37,200 --> 00:12:40,760 Speaker 1: assumptions a lot of these scenarios make is that aliens 242 00:12:41,000 --> 00:12:43,640 Speaker 1: want us to find them, or that they are trying 243 00:12:43,679 --> 00:12:46,120 Speaker 1: to talk to us, or they are curious about the 244 00:12:46,160 --> 00:12:49,000 Speaker 1: rest of the universe as well, so they're sending messages 245 00:12:49,000 --> 00:12:52,679 Speaker 1: out or they're sending probes out there explorational the same 246 00:12:52,720 --> 00:12:54,920 Speaker 1: way that we are. But of course we don't know 247 00:12:55,000 --> 00:12:58,280 Speaker 1: what alien psychology is like, and what does aliens want, 248 00:12:58,400 --> 00:13:01,160 Speaker 1: or even what it means to want something as an alien. 249 00:13:01,320 --> 00:13:03,559 Speaker 1: So these days a lot of people are imagining other 250 00:13:03,640 --> 00:13:08,000 Speaker 1: ways to detect aliens when they're not trying to be detected. 251 00:13:08,360 --> 00:13:11,200 Speaker 1: Are there things the aliens can do imprints they leave 252 00:13:11,280 --> 00:13:14,640 Speaker 1: on the universe that aren't intended for us to discover them, 253 00:13:14,679 --> 00:13:17,679 Speaker 1: but might allow us to spot them anyway. So today 254 00:13:17,679 --> 00:13:25,079 Speaker 1: on the program, we'll be asking the question could we 255 00:13:25,200 --> 00:13:30,079 Speaker 1: detect alien nuclear explosions? I imagine you're saying these are 256 00:13:30,120 --> 00:13:35,959 Speaker 1: like accidental nuclear explosions or on purpose nuclear explosions, either one, right, 257 00:13:36,040 --> 00:13:38,680 Speaker 1: we don't discriminate. We just like to know the aliens 258 00:13:38,720 --> 00:13:44,160 Speaker 1: are there, and whatever they do in their normal civilization extrapolasition, 259 00:13:44,600 --> 00:13:47,440 Speaker 1: we'd like to see if we could detect it. Maybe 260 00:13:47,480 --> 00:13:49,840 Speaker 1: they're just doing testing like we're doing, or maybe they 261 00:13:49,960 --> 00:13:55,160 Speaker 1: have some globe spanning nuclear annihilation. The question is, could 262 00:13:55,240 --> 00:13:58,600 Speaker 1: we see it right, If aliens are blowing up nuclear bombs, 263 00:13:58,720 --> 00:14:01,240 Speaker 1: is it possible for us to spot that? Yeah, because 264 00:14:01,280 --> 00:14:03,400 Speaker 1: as you mentioned, you know, one scenario is that they're 265 00:14:03,559 --> 00:14:07,679 Speaker 1: sending out signals on purpose, either to talk to us 266 00:14:07,679 --> 00:14:11,600 Speaker 1: directly or just like that's their TV, maybe their broadcast TV. 267 00:14:11,920 --> 00:14:14,200 Speaker 1: But I think we talked in an earlier episode about 268 00:14:14,280 --> 00:14:17,040 Speaker 1: how like for us to detect the signal from an alien, 269 00:14:17,120 --> 00:14:20,320 Speaker 1: it would have to be like a pretty focus beam, right, 270 00:14:20,320 --> 00:14:22,240 Speaker 1: like the like the club we're just listening to their 271 00:14:22,280 --> 00:14:24,880 Speaker 1: TV broadcast is pretty low, that's right. If you're just 272 00:14:24,960 --> 00:14:28,240 Speaker 1: sending signals in every direction, then you pay a really 273 00:14:28,360 --> 00:14:32,000 Speaker 1: big price because those signals get weaker with distance, and 274 00:14:32,000 --> 00:14:35,280 Speaker 1: they get weaker with distance squared. So when signals go 275 00:14:35,640 --> 00:14:38,480 Speaker 1: twice as far, they're four times as week, When they 276 00:14:38,520 --> 00:14:41,080 Speaker 1: go ten times as far, they're one hundred times as week. 277 00:14:41,440 --> 00:14:45,680 Speaker 1: That makes it really really hard to detect non focus signals. 278 00:14:46,280 --> 00:14:49,000 Speaker 1: And if we wanted to detect signals that we could 279 00:14:49,040 --> 00:14:52,400 Speaker 1: generate using technology that we have, we would not be 280 00:14:52,520 --> 00:14:55,400 Speaker 1: able to spot signals of the kinds we can generate 281 00:14:55,520 --> 00:14:58,320 Speaker 1: using our own technology from planets that are more than 282 00:14:58,400 --> 00:15:01,920 Speaker 1: like one light year away. If however, they're like beaming 283 00:15:02,000 --> 00:15:05,280 Speaker 1: us messages, they're shooting laser beams in our direction. Then 284 00:15:05,280 --> 00:15:07,680 Speaker 1: the math works differently and we could get messages from 285 00:15:07,720 --> 00:15:10,000 Speaker 1: further away, But then they'd have to know we were 286 00:15:10,120 --> 00:15:13,320 Speaker 1: here and try to send us messages on purpose, which 287 00:15:13,320 --> 00:15:16,360 Speaker 1: seems less likely. I think here today we're exploring a 288 00:15:16,400 --> 00:15:18,880 Speaker 1: different scenario, which is like, what if they're doing something 289 00:15:19,320 --> 00:15:23,360 Speaker 1: without trying by accident maybe or through some sort of event, 290 00:15:23,640 --> 00:15:26,360 Speaker 1: and then that's what we see, and that's how we 291 00:15:26,400 --> 00:15:28,440 Speaker 1: know that there are aliens exactly. And people have been 292 00:15:28,480 --> 00:15:30,560 Speaker 1: thinking about this and wondering like, well, what's the most 293 00:15:30,720 --> 00:15:34,480 Speaker 1: visible thing that you can do, not just broadcasting Rick 294 00:15:34,480 --> 00:15:37,920 Speaker 1: and Morty episodes into the cosmos? All right, Sometimes our 295 00:15:37,960 --> 00:15:42,480 Speaker 1: civilization does things which generate very bright flashes of radiation, 296 00:15:42,520 --> 00:15:45,680 Speaker 1: and hey, what's brighter than a nuclear explosion? But what 297 00:15:45,720 --> 00:15:47,800 Speaker 1: if there's a kid in that alien planet pointing a 298 00:15:47,880 --> 00:15:55,120 Speaker 1: laser partner directly Ow my eye? Ow alien burnt my eye? Yeah, 299 00:15:55,120 --> 00:15:56,960 Speaker 1: I know, that's why you should be careful you knock 300 00:15:57,000 --> 00:15:59,320 Speaker 1: about this guy. So then the scenario here is that 301 00:15:59,480 --> 00:16:03,200 Speaker 1: somehow this alien civilization out there is exploding nuclear their 302 00:16:03,200 --> 00:16:08,080 Speaker 1: own nuclear bombs, either by accident, or some testing or something. 303 00:16:08,160 --> 00:16:10,080 Speaker 1: Maybe they have their own nuclear war, and so the 304 00:16:10,160 --> 00:16:14,440 Speaker 1: question is like, could we see those nuclear explosions exactly? 305 00:16:14,600 --> 00:16:16,680 Speaker 1: All right? Well, as usual, we were wondering how many 306 00:16:16,680 --> 00:16:21,200 Speaker 1: people out there had the interesting curiosity to ask this 307 00:16:21,320 --> 00:16:24,120 Speaker 1: question about alien life and how we could detect them. So, 308 00:16:24,120 --> 00:16:26,120 Speaker 1: as usual, Daniel went out there. Did you go to 309 00:16:26,200 --> 00:16:28,360 Speaker 1: the internet or are you? Are you going on campus? 310 00:16:28,360 --> 00:16:31,720 Speaker 1: Now these are still Internet based questions. I felt a 311 00:16:31,760 --> 00:16:34,800 Speaker 1: little bit weird walking around campus asking people about aliens 312 00:16:34,840 --> 00:16:38,240 Speaker 1: and nuclear bombs. That's never stopped you before. I thought 313 00:16:38,240 --> 00:16:42,000 Speaker 1: it might get reported to the UCI police. Yeah, you 314 00:16:42,040 --> 00:16:45,200 Speaker 1: have tenure. They're not gonna fire you. Anyways, usually have 315 00:16:45,280 --> 00:16:48,680 Speaker 1: to do worst things. So thanks very much to our 316 00:16:48,760 --> 00:16:52,640 Speaker 1: internet volunteers who responded with enthusiasm to this question. If 317 00:16:52,680 --> 00:16:54,800 Speaker 1: you would like to play this part in future episodes, 318 00:16:54,840 --> 00:16:57,760 Speaker 1: please write to me to questions at Daniel and Jorge 319 00:16:57,760 --> 00:17:00,400 Speaker 1: dot com. We can do it all over email. It's fast, 320 00:17:00,520 --> 00:17:03,320 Speaker 1: it's easy, it's fun to think about it for a second. 321 00:17:03,320 --> 00:17:08,240 Speaker 1: Do you think we could detect alien nuclear explosions? Here's 322 00:17:08,280 --> 00:17:10,720 Speaker 1: what people have to say. Yes, So it depends whether 323 00:17:10,760 --> 00:17:14,679 Speaker 1: the detonation happened on Earth or a planet from Solar 324 00:17:14,680 --> 00:17:18,040 Speaker 1: System or somewhere far away. In any of these cases, 325 00:17:18,080 --> 00:17:20,800 Speaker 1: I think we might be able to detect. Considering that 326 00:17:21,240 --> 00:17:23,920 Speaker 1: why decaying of the matter and the amount of radiation 327 00:17:23,960 --> 00:17:26,600 Speaker 1: that is being exposed out of that location on Earth, 328 00:17:26,800 --> 00:17:29,760 Speaker 1: we might be able to analyze whether it's man made 329 00:17:30,280 --> 00:17:33,960 Speaker 1: or alien, and if it is happening on some other planet. 330 00:17:34,160 --> 00:17:38,280 Speaker 1: Considering the amount of information that we have already gained 331 00:17:38,280 --> 00:17:41,679 Speaker 1: with the telescopes in place, we will be able to 332 00:17:41,720 --> 00:17:44,080 Speaker 1: do it. That's what I believe. By now, we have 333 00:17:44,119 --> 00:17:47,639 Speaker 1: satellites now that can detect detonations on Earth. I don't 334 00:17:47,640 --> 00:17:51,800 Speaker 1: think it would work at interstellar distances, especially considering that 335 00:17:51,800 --> 00:17:55,359 Speaker 1: there's so many sources of radiation in space, you know, 336 00:17:55,440 --> 00:17:59,000 Speaker 1: from stars to gamma ray burst everything in between. So no, 337 00:17:59,440 --> 00:18:02,320 Speaker 1: I don't think we could. Well, I guess so. I 338 00:18:02,359 --> 00:18:05,439 Speaker 1: guess it would depend on how good the detector was 339 00:18:05,480 --> 00:18:08,520 Speaker 1: and how far away it was away from you. If 340 00:18:08,560 --> 00:18:11,159 Speaker 1: there was set off over your head, you might be 341 00:18:11,200 --> 00:18:14,399 Speaker 1: able to detect it pretty soon. I feel like we 342 00:18:14,560 --> 00:18:19,000 Speaker 1: probably could detect alien nuclear detonations if there was like 343 00:18:19,160 --> 00:18:24,080 Speaker 1: enough radiation to reach far enough, But other than that, 344 00:18:24,480 --> 00:18:27,240 Speaker 1: I don't really think we could all right. Some people 345 00:18:27,280 --> 00:18:30,560 Speaker 1: said yes, some people said no, some people said maybe yeah. 346 00:18:30,560 --> 00:18:32,760 Speaker 1: I think they really put their finger on the issue, 347 00:18:32,880 --> 00:18:36,320 Speaker 1: which is that nobody knows, not even us. It's all 348 00:18:36,359 --> 00:18:40,240 Speaker 1: about brightness and distance. You know, what's the faintest radiation 349 00:18:40,359 --> 00:18:42,439 Speaker 1: we could pick up? And how close would these bombs 350 00:18:42,480 --> 00:18:44,640 Speaker 1: have to be for us to spot them. I feel 351 00:18:44,680 --> 00:18:48,160 Speaker 1: like you're missing one important factor, which is how big 352 00:18:48,200 --> 00:18:50,280 Speaker 1: are these bombs? That's a huge unknown. You're right, and 353 00:18:50,320 --> 00:18:52,040 Speaker 1: we'll get into it in a minute. And the only 354 00:18:52,080 --> 00:18:55,000 Speaker 1: standard we have is like how big are our bombs? 355 00:18:55,400 --> 00:18:59,360 Speaker 1: So we can imagine whether we could detect nuclear explosions 356 00:18:59,400 --> 00:19:03,040 Speaker 1: of the size we could make if aliens also did them. 357 00:19:03,040 --> 00:19:04,880 Speaker 1: All right, we'll dig into it, but I guess first 358 00:19:04,920 --> 00:19:07,640 Speaker 1: let's start with the basics, Like Daniel, what happens during 359 00:19:07,680 --> 00:19:10,760 Speaker 1: a nuclear explosion? Besides the explosion part of it. Yeah, 360 00:19:10,800 --> 00:19:13,600 Speaker 1: to understand whether we could see a nuclear explosion on 361 00:19:13,640 --> 00:19:16,520 Speaker 1: another planet, you have to think about what the signals are, 362 00:19:16,880 --> 00:19:19,800 Speaker 1: like what signals does a nuclear explosion generate? And we 363 00:19:19,840 --> 00:19:22,480 Speaker 1: had a whole episode about how nuclear bombs work where 364 00:19:22,680 --> 00:19:24,840 Speaker 1: we went to a lot of detail, but not enough 365 00:19:24,920 --> 00:19:28,639 Speaker 1: detail for you to build a nuclear bomb. Hopefully but 366 00:19:28,960 --> 00:19:32,679 Speaker 1: human nuclear weapons at least are either fission weapons or 367 00:19:32,840 --> 00:19:36,720 Speaker 1: fusion weapons triggered by fission. And remember that the basic 368 00:19:36,800 --> 00:19:41,080 Speaker 1: processes here fission involved breaking up of a heavy nucleus 369 00:19:41,080 --> 00:19:44,480 Speaker 1: like plutonium or uranium, which then shoots off a bunch 370 00:19:44,480 --> 00:19:48,040 Speaker 1: of neutrons and rams into other nuclei, which breaks them 371 00:19:48,040 --> 00:19:50,720 Speaker 1: apart and sets off a chain reaction where you very 372 00:19:50,880 --> 00:19:54,440 Speaker 1: rapidly are releasing energy. And the fusion bomb is similar 373 00:19:54,640 --> 00:19:58,080 Speaker 1: except it uses a fission bomb to compress a bunch 374 00:19:58,080 --> 00:20:02,360 Speaker 1: of fusion fuel that it fuses, and in both scenarios 375 00:20:02,400 --> 00:20:05,240 Speaker 1: the key thing is releasing a huge amount of energy 376 00:20:05,520 --> 00:20:08,840 Speaker 1: very very quickly, but not just energy, right, You're releasing 377 00:20:08,920 --> 00:20:12,040 Speaker 1: energy but also a lot of radiation. Yeah, maybe step 378 00:20:12,080 --> 00:20:15,000 Speaker 1: us through like what's actually being released, Like when you 379 00:20:15,080 --> 00:20:19,159 Speaker 1: fuse things together they click together, to nuclear click together, 380 00:20:19,280 --> 00:20:25,200 Speaker 1: and then what actually gets released like light or particles 381 00:20:25,440 --> 00:20:29,399 Speaker 1: or Yeah, so fusion produces high energy photons. It also 382 00:20:29,520 --> 00:20:35,200 Speaker 1: produces neutrons and electrons and neutrinos. Right, so all these 383 00:20:35,280 --> 00:20:37,959 Speaker 1: kinds of things are produced and then much just produced, 384 00:20:38,000 --> 00:20:42,160 Speaker 1: but they're like they're produced, but then they're flying really fast. Yes, 385 00:20:42,359 --> 00:20:44,879 Speaker 1: they're produced, and they're carrying a lot of energy is 386 00:20:45,000 --> 00:20:47,359 Speaker 1: what you actually see from the bomb from like a 387 00:20:47,400 --> 00:20:50,720 Speaker 1: certain distance. Depends on how that energy is absorbed or 388 00:20:50,840 --> 00:20:53,320 Speaker 1: not absorbed. So, for example, a lot of the energy 389 00:20:53,600 --> 00:20:57,399 Speaker 1: gets dumped into the matters immediately surrounding the bomb, right, 390 00:20:57,440 --> 00:20:59,800 Speaker 1: and so it's absorbed very very rapidly by the st 391 00:21:00,119 --> 00:21:03,280 Speaker 1: around the bomb, which expands that matter and creates a 392 00:21:03,280 --> 00:21:06,680 Speaker 1: shock wave. I mean like the bomb casing or like whatever, 393 00:21:07,520 --> 00:21:09,080 Speaker 1: if it's on the ground, that that's what it's going 394 00:21:09,160 --> 00:21:12,199 Speaker 1: to push out. Yeah, I mean whatever material is around 395 00:21:12,200 --> 00:21:14,760 Speaker 1: the bomb, like the air or the water or the ground, 396 00:21:15,320 --> 00:21:18,000 Speaker 1: and you get very different scenarios if you have an 397 00:21:18,000 --> 00:21:22,320 Speaker 1: in air explosion or underground explosion or just above the water. 398 00:21:22,520 --> 00:21:25,480 Speaker 1: But the material that surrounds the bomb is inundated with 399 00:21:25,560 --> 00:21:27,480 Speaker 1: a huge amount of energy, a lot of it from 400 00:21:27,520 --> 00:21:30,240 Speaker 1: gamma rays, and a lot of that gets rapidly absorbed 401 00:21:30,280 --> 00:21:32,639 Speaker 1: and that material gets heated up to like tens of 402 00:21:32,760 --> 00:21:36,400 Speaker 1: millions of degrees and then you get this shockwave. So 403 00:21:36,480 --> 00:21:38,880 Speaker 1: in the end, on average, and it depends on exactly 404 00:21:38,920 --> 00:21:41,600 Speaker 1: what you've surrounded the bomb with, about half of the 405 00:21:41,720 --> 00:21:45,720 Speaker 1: energy of a nuclear bomb go these shockwaves, these expanding 406 00:21:45,840 --> 00:21:50,040 Speaker 1: waves of matter basically sound waves through matter that carry 407 00:21:50,040 --> 00:21:52,479 Speaker 1: away a lot of this energy, doesn't It depend on 408 00:21:52,520 --> 00:21:55,200 Speaker 1: what's around the bomb. Like if you explode it in water, 409 00:21:55,560 --> 00:21:57,359 Speaker 1: all of it's going to go into the water, But 410 00:21:57,400 --> 00:21:59,480 Speaker 1: if you put it in air, you know there's maybe 411 00:21:59,480 --> 00:22:02,320 Speaker 1: a chance for that energy to go out further. Even 412 00:22:02,320 --> 00:22:04,400 Speaker 1: in air, a lot of that energy is absorbed by 413 00:22:04,480 --> 00:22:06,919 Speaker 1: the air and you get shock waves. So yes, it 414 00:22:06,960 --> 00:22:10,560 Speaker 1: definitely does depend on the kind of material surrounded. Like 415 00:22:10,600 --> 00:22:13,320 Speaker 1: if you blow it up underground, it's absorbed differently than 416 00:22:13,359 --> 00:22:15,320 Speaker 1: if you blow it up in the air. But you know, 417 00:22:15,440 --> 00:22:18,600 Speaker 1: since we're just dealing with like approximate numbers here, roughly 418 00:22:18,640 --> 00:22:21,600 Speaker 1: on average, over all those circumstances, about half of the 419 00:22:21,680 --> 00:22:24,919 Speaker 1: energy gets dumped into shock waves and then like another 420 00:22:25,080 --> 00:22:28,000 Speaker 1: forty percent of the energy comes out in what we 421 00:22:28,040 --> 00:22:32,080 Speaker 1: call thermal radiation, basically photons to which the atmosphere is 422 00:22:32,119 --> 00:22:36,639 Speaker 1: transparent visible light, infrared light, UV light, things that are 423 00:22:36,680 --> 00:22:39,800 Speaker 1: not immediately absorbed by the surrounding material which conduct fly 424 00:22:39,960 --> 00:22:44,000 Speaker 1: out through that material because that material is transparent to 425 00:22:44,080 --> 00:22:47,440 Speaker 1: this kind of radiation. Why is it transparent. Is it 426 00:22:47,480 --> 00:22:50,760 Speaker 1: because it just doesn't absorb because of quantum effects, or 427 00:22:50,880 --> 00:22:53,040 Speaker 1: is it just that it's so like air is so 428 00:22:53,119 --> 00:22:55,840 Speaker 1: thin that it just doesn't hit enough air molecules. Yeah, 429 00:22:55,880 --> 00:22:58,320 Speaker 1: air is transparent to visible light, right, we know that 430 00:22:58,359 --> 00:23:01,040 Speaker 1: because we can see the sun through the air. Why 431 00:23:01,160 --> 00:23:03,320 Speaker 1: is the air transparent to visible light, You're right, is 432 00:23:03,400 --> 00:23:07,320 Speaker 1: quantum effects. You have certain gases under certain conditions, and 433 00:23:07,400 --> 00:23:10,520 Speaker 1: they either like to absorb photons of various frequencies or 434 00:23:10,560 --> 00:23:13,680 Speaker 1: they don't. These air molecules can't just absorb a photon 435 00:23:13,720 --> 00:23:16,480 Speaker 1: of an arbitrary frequency. They have to have like a 436 00:23:16,600 --> 00:23:20,399 Speaker 1: quantum state that their electron can jump up into, or 437 00:23:20,400 --> 00:23:22,880 Speaker 1: like a new rotation that they can do. So atoms 438 00:23:22,880 --> 00:23:26,280 Speaker 1: can only absorb certain frequencies of light, and the other 439 00:23:26,320 --> 00:23:29,840 Speaker 1: frequencies pass right through. So air is mostly transparent to 440 00:23:30,040 --> 00:23:33,679 Speaker 1: visible light and also infrared light. It's less transparent in 441 00:23:33,720 --> 00:23:35,800 Speaker 1: the UV, which is one reason why we have like 442 00:23:36,280 --> 00:23:39,879 Speaker 1: UV space telescopes above the atmosphere. But you know a 443 00:23:39,960 --> 00:23:42,439 Speaker 1: lot of energy is dumped out and so some of 444 00:23:42,440 --> 00:23:47,080 Speaker 1: these very high energy UV light does survive passing through 445 00:23:47,080 --> 00:23:49,560 Speaker 1: the atmosphere. If you're near a nuclear bomb, so you 446 00:23:49,560 --> 00:23:52,359 Speaker 1: have like fifty percent of it roughly in the shock wave, 447 00:23:52,520 --> 00:23:56,960 Speaker 1: like another forty percent in thermal radiation these photons that 448 00:23:57,040 --> 00:24:00,440 Speaker 1: don't get absorbed, and then another ten percent in other 449 00:24:00,480 --> 00:24:04,000 Speaker 1: particles like neutrons or very high energy photons we call 450 00:24:04,080 --> 00:24:07,800 Speaker 1: gamma rays or electrons. Is it sort of like lightning 451 00:24:07,800 --> 00:24:09,960 Speaker 1: and thunder? Like you will see the flash of a 452 00:24:10,080 --> 00:24:14,560 Speaker 1: nuclear bomb before you actually get hit by the shockwave. Yeah, 453 00:24:14,600 --> 00:24:17,399 Speaker 1: it's really cool. You actually see two flashes of a 454 00:24:17,480 --> 00:24:21,359 Speaker 1: nuclear bomb. You see the first flash because the visible 455 00:24:21,440 --> 00:24:23,960 Speaker 1: light reaches you before the shockwave. But at some point 456 00:24:23,960 --> 00:24:27,320 Speaker 1: the shock wave passes the fireball because the shockwave is 457 00:24:27,520 --> 00:24:31,800 Speaker 1: making the material more dense, which acts to obscure the fireball. 458 00:24:32,280 --> 00:24:35,800 Speaker 1: So the shockwave itself is opaque to the kind of 459 00:24:35,880 --> 00:24:38,840 Speaker 1: light being generated by the nuclear bomb. So then for 460 00:24:38,880 --> 00:24:41,000 Speaker 1: a moment you can't see the fireball, but then it 461 00:24:41,040 --> 00:24:43,560 Speaker 1: dissipates and you can see it again. So it's like 462 00:24:43,600 --> 00:24:45,960 Speaker 1: you see fireball and then you see the shock wave, 463 00:24:46,000 --> 00:24:47,639 Speaker 1: and then you see the fireball. So it's sort of 464 00:24:47,680 --> 00:24:50,680 Speaker 1: like lightning and then thunder and then a second flash 465 00:24:50,720 --> 00:24:53,840 Speaker 1: of lightning. Whoa, I mean, assuming you survived the first 466 00:24:54,600 --> 00:24:57,720 Speaker 1: event to get to see the other two. Yeah, So 467 00:24:57,800 --> 00:25:00,679 Speaker 1: this is a very characteristic signature of nuclear bombs. This 468 00:25:00,920 --> 00:25:05,200 Speaker 1: double peak of gamma radiation over several milliseconds. Well, it's 469 00:25:05,200 --> 00:25:08,560 Speaker 1: definitely an event and nuclear explosion. And so the question 470 00:25:08,680 --> 00:25:12,960 Speaker 1: is if aliens exploded nuclear bombs in their planets, could 471 00:25:13,040 --> 00:25:16,639 Speaker 1: we see them from here. Let's dig into that question 472 00:25:16,840 --> 00:25:18,800 Speaker 1: and what we should be looking for if we're looking 473 00:25:18,840 --> 00:25:23,240 Speaker 1: for those kinds of signals. First, let's take a quick break. 474 00:25:36,040 --> 00:25:40,959 Speaker 1: All right, we are spending today imagining aliens blowing themselves up. 475 00:25:41,000 --> 00:25:44,080 Speaker 1: We're not hoping they blow themselves up, but if they do, 476 00:25:44,400 --> 00:25:47,280 Speaker 1: we hope to see it. We're not hoping they blow 477 00:25:47,320 --> 00:25:49,640 Speaker 1: themselves up, but if they do, it would be nice. 478 00:25:49,880 --> 00:25:52,080 Speaker 1: Is that what you say? Is that? What are you saying? 479 00:25:52,359 --> 00:25:56,840 Speaker 1: I mean, I don't aliens living in obscurity forever, or 480 00:25:56,920 --> 00:26:00,000 Speaker 1: aliens killing themselves about then we find out about them. 481 00:26:00,000 --> 00:26:01,760 Speaker 1: I mean, it would also be kind of sad to 482 00:26:01,840 --> 00:26:05,119 Speaker 1: discover aliens only to discover they had all killed themselves, 483 00:26:06,240 --> 00:26:08,439 Speaker 1: that they were the last ones. Yeah, that would be 484 00:26:08,600 --> 00:26:11,119 Speaker 1: that would be pretty tragic. Yeah, that would be a bummer. Well, 485 00:26:11,160 --> 00:26:14,119 Speaker 1: we've talked about what a nuclear explosion is and what 486 00:26:14,200 --> 00:26:16,320 Speaker 1: happens to it. So you said about half of the 487 00:26:16,520 --> 00:26:19,840 Speaker 1: energy is really just pushing the stuff around it so 488 00:26:19,920 --> 00:26:22,639 Speaker 1: I imagine that won't get very far. Maybe forty percent 489 00:26:22,680 --> 00:26:26,639 Speaker 1: of it goes into just light, basically invisible light or 490 00:26:26,760 --> 00:26:29,640 Speaker 1: light you'd be light, And about ten percent of it 491 00:26:29,680 --> 00:26:35,120 Speaker 1: goes into shooting out basically radiation, right, like charged particles. Yeah, 492 00:26:35,160 --> 00:26:39,800 Speaker 1: not just charged particles, but neutrons, gamma rays, and also electrons. Well, 493 00:26:39,800 --> 00:26:42,280 Speaker 1: gamma rays are light, right, Gamma rays are very high 494 00:26:42,400 --> 00:26:45,400 Speaker 1: energy photons, Yeah, even more high energy than X rays 495 00:26:45,560 --> 00:26:48,480 Speaker 1: or UV. These are all ionizing radiation. They all have 496 00:26:48,480 --> 00:26:52,600 Speaker 1: the capacity to knock electrons off of materials. And because 497 00:26:52,600 --> 00:26:56,200 Speaker 1: they're ionizing and electrons themselves have charge, they can also 498 00:26:56,280 --> 00:26:59,640 Speaker 1: generate an electro magnetic pulse. This is a common feature 499 00:27:00,080 --> 00:27:04,000 Speaker 1: a lot of movies nuclear weapons knocking out electronics because 500 00:27:04,040 --> 00:27:08,800 Speaker 1: of a very high energy pulse of electromagnetic radiation. Oh interesting, 501 00:27:08,920 --> 00:27:11,680 Speaker 1: it's not just that it's like a giant magnet. It's 502 00:27:11,720 --> 00:27:15,159 Speaker 1: like it's actually shooting out little magnets. Yeah, exactly. And 503 00:27:15,200 --> 00:27:17,760 Speaker 1: so all those gamma rays and all those electrons can 504 00:27:17,840 --> 00:27:20,520 Speaker 1: damage a lot of electronics. So if you have electronics 505 00:27:20,600 --> 00:27:23,280 Speaker 1: near a nuclear weapons blast, then you will feel it. 506 00:27:23,280 --> 00:27:26,640 Speaker 1: They could get knocked offline. They don't shoot protons explosions 507 00:27:26,760 --> 00:27:29,520 Speaker 1: or neutrinos. They do generate a lot of neutrinos. He 508 00:27:29,560 --> 00:27:33,080 Speaker 1: has absolutely fusion and fission both generate neutrinos, but not 509 00:27:33,119 --> 00:27:36,800 Speaker 1: so many protons. Mostly neutrons and neutrinos and electrons. What 510 00:27:36,880 --> 00:27:40,720 Speaker 1: about later rays and sound effects like in Star Wars? 511 00:27:40,960 --> 00:27:43,280 Speaker 1: They don't go pupupu as far as I've seen. It's 512 00:27:43,320 --> 00:27:46,000 Speaker 1: not in the literature. But the sounds of thousands of 513 00:27:47,200 --> 00:27:50,919 Speaker 1: souls being snuffed at the same time, Oh, that's sad. 514 00:27:51,040 --> 00:27:52,800 Speaker 1: I don't know if they create a great disturbance in 515 00:27:52,840 --> 00:27:54,960 Speaker 1: the force. We don't have detectors that can measure the 516 00:27:55,000 --> 00:27:57,840 Speaker 1: force yet, so I'm not sure about that, not yet 517 00:27:57,880 --> 00:28:00,000 Speaker 1: at least, although I have a good acronym for them. 518 00:28:00,080 --> 00:28:05,159 Speaker 1: They should be a named Jedi, right, And how does 519 00:28:05,200 --> 00:28:11,360 Speaker 1: that work? Just the Electron Detection Institute sounds good? Are 520 00:28:11,359 --> 00:28:13,199 Speaker 1: you setting that up with some funding? Are you going 521 00:28:13,240 --> 00:28:16,200 Speaker 1: to endow the Jedi Institute? Maybe I have already, I'm 522 00:28:16,200 --> 00:28:20,800 Speaker 1: just not telling you. No. That's extra frustrating. But you know, 523 00:28:20,880 --> 00:28:23,359 Speaker 1: there are a lot of scientists here on Earth that 524 00:28:23,400 --> 00:28:26,760 Speaker 1: are developed very sensitive technology for a studying nuclear weapons, 525 00:28:27,160 --> 00:28:30,280 Speaker 1: both because we want to understand what happens when they 526 00:28:30,320 --> 00:28:32,160 Speaker 1: blow up, because we have done tests and we want 527 00:28:32,200 --> 00:28:35,120 Speaker 1: to understand whether our nuclear weapons are working and are 528 00:28:35,160 --> 00:28:38,280 Speaker 1: still working and are surviving the test of time as 529 00:28:38,280 --> 00:28:41,040 Speaker 1: they sit in our stockpiles. But also because we wanted 530 00:28:41,040 --> 00:28:45,000 Speaker 1: to detect if other countries are blowing up their nuclear bombs. 531 00:28:45,040 --> 00:28:48,320 Speaker 1: So there's been a lot of investment in detection of 532 00:28:48,520 --> 00:28:51,400 Speaker 1: nuclear weapons activity, you mean, like here on Earth. Like 533 00:28:51,520 --> 00:28:54,480 Speaker 1: if you wanted to detect whether a nuclear bomb exploded 534 00:28:54,600 --> 00:28:57,040 Speaker 1: here on Earth, not in an alien planet, we have 535 00:28:57,200 --> 00:28:59,000 Speaker 1: techniques here on Earth to do that because I guess 536 00:28:59,080 --> 00:29:02,000 Speaker 1: if someone explodes a nuther bomb on the other side 537 00:29:02,000 --> 00:29:03,760 Speaker 1: of the world, in the middle of the ocean, you 538 00:29:03,800 --> 00:29:06,840 Speaker 1: may not necessarily know what happened, right, And if you're 539 00:29:07,440 --> 00:29:10,800 Speaker 1: a big country in a cold war or not, you 540 00:29:10,840 --> 00:29:13,560 Speaker 1: might want to know if your enemies are exploding bombs 541 00:29:13,680 --> 00:29:15,520 Speaker 1: or testing them, that's right, and you might not want 542 00:29:15,600 --> 00:29:17,560 Speaker 1: the other country to know that you're doing it. So, 543 00:29:17,640 --> 00:29:20,880 Speaker 1: like secret testing of nuclear weapons was a big industry 544 00:29:20,880 --> 00:29:23,240 Speaker 1: and a sort of an arms race of hiding nuclear 545 00:29:23,280 --> 00:29:27,080 Speaker 1: bomb detonations and nuclear weapons detections. I grew up in 546 00:29:27,120 --> 00:29:29,480 Speaker 1: Los Almos, which was certainly a nerve center for this 547 00:29:29,560 --> 00:29:32,400 Speaker 1: kind of stuff. My mom actually worked on a nuclear 548 00:29:32,480 --> 00:29:35,680 Speaker 1: non proliferation technology when she was at Los Almos, trying 549 00:29:35,680 --> 00:29:38,360 Speaker 1: to detect if people are blowing up nuclear bombs and 550 00:29:38,400 --> 00:29:40,080 Speaker 1: all this kind of stuff. So we have a lot 551 00:29:40,080 --> 00:29:42,080 Speaker 1: of ways to try to figure out if someone has 552 00:29:42,120 --> 00:29:44,480 Speaker 1: blown up a nuclear bomb here on Earth. Yeah, it 553 00:29:44,480 --> 00:29:46,760 Speaker 1: sounds like you would want to know. And it's kind 554 00:29:46,760 --> 00:29:49,840 Speaker 1: of interesting that we test nuclear bombs right Like, first 555 00:29:49,880 --> 00:29:51,400 Speaker 1: of all, I guess you have to test them right 556 00:29:51,400 --> 00:29:52,880 Speaker 1: now or the wise do not even know they work. 557 00:29:52,960 --> 00:29:55,440 Speaker 1: But it's amazing to me that we have tested nuclear 558 00:29:55,480 --> 00:29:57,640 Speaker 1: bombs here in the US, right in the desert back 559 00:29:57,640 --> 00:30:00,240 Speaker 1: in the fifties and sixties that there was all they did. Yeah, 560 00:30:00,280 --> 00:30:02,600 Speaker 1: they have done above ground tests here in the US. 561 00:30:02,720 --> 00:30:05,200 Speaker 1: You know, Alamagordo was the first site in New Mexico 562 00:30:05,320 --> 00:30:07,280 Speaker 1: and they tested them on a bunch of islands, which 563 00:30:07,320 --> 00:30:10,360 Speaker 1: was terrible and like totally obliterated them. And then there 564 00:30:10,400 --> 00:30:13,600 Speaker 1: was an atmosphereic test ban treaty, so you couldn't test 565 00:30:13,600 --> 00:30:16,640 Speaker 1: the nuclear weapons in the atmosphere anymore, which is good, 566 00:30:16,680 --> 00:30:19,560 Speaker 1: and they moved the testing underground. So in the United States, 567 00:30:19,560 --> 00:30:22,320 Speaker 1: for example, there's the Nevada underground test site where they 568 00:30:22,360 --> 00:30:24,680 Speaker 1: blow these weapons up underground. But there hasn't been any 569 00:30:24,760 --> 00:30:28,600 Speaker 1: recent testing. There's a Comprehensive Test Band treaty now and 570 00:30:28,680 --> 00:30:31,800 Speaker 1: so instead people now do simulations. They try to understand 571 00:30:32,200 --> 00:30:35,120 Speaker 1: what would happen in the event of a nuclear explosion, 572 00:30:35,320 --> 00:30:38,120 Speaker 1: or try to model what's happening to the nuclear weapons 573 00:30:38,200 --> 00:30:40,720 Speaker 1: we have now, are they going to survive? The whole 574 00:30:40,720 --> 00:30:43,960 Speaker 1: big industry called stockpile stewardship to try to make sure 575 00:30:43,960 --> 00:30:47,640 Speaker 1: that our nuclear weapons would still work if we fired them. Interesting, 576 00:30:47,680 --> 00:30:50,480 Speaker 1: So it's a treaty. So like with Russian other countries, 577 00:30:50,520 --> 00:30:53,520 Speaker 1: we have a handshake agreement that you can't test. Basically, 578 00:30:53,800 --> 00:30:56,720 Speaker 1: you can't test nuclear weapons anymore. Yeah, there's a Comprehensive 579 00:30:56,800 --> 00:31:00,280 Speaker 1: Nuclear Test Band Treaty signed in nineteen ninety six. And 580 00:31:00,320 --> 00:31:03,360 Speaker 1: you know, these treatings are always complicated because some nations 581 00:31:03,400 --> 00:31:05,960 Speaker 1: don't ratify them. They're signed by presidents and then their 582 00:31:06,320 --> 00:31:08,560 Speaker 1: local parliaments don't agree to them. But yeah, it's been 583 00:31:08,560 --> 00:31:10,800 Speaker 1: a long time since there was sort of a public 584 00:31:10,840 --> 00:31:13,720 Speaker 1: test of a nuclear weapon out in the open, all right. 585 00:31:13,720 --> 00:31:16,560 Speaker 1: So if someone did test the weapon or use one 586 00:31:16,640 --> 00:31:18,480 Speaker 1: here on earth, how can we detect them? So we 587 00:31:18,520 --> 00:31:20,680 Speaker 1: have a few ways to try to spot this. Number 588 00:31:20,680 --> 00:31:23,480 Speaker 1: one is seismic. If you do test underground, then it's 589 00:31:23,480 --> 00:31:26,200 Speaker 1: going to shake the earth and the earth will ring 590 00:31:26,320 --> 00:31:28,960 Speaker 1: like a bell. Shock waves will pass all the way 591 00:31:28,960 --> 00:31:31,080 Speaker 1: around the Earth, and you can detect them in other 592 00:31:31,120 --> 00:31:34,720 Speaker 1: places the same way we can put detectors in California 593 00:31:34,800 --> 00:31:37,600 Speaker 1: that can spot earthquakes in Japan or in other parts 594 00:31:37,640 --> 00:31:41,320 Speaker 1: of the world. You can detect large seismic events all 595 00:31:41,360 --> 00:31:43,920 Speaker 1: over the world. Right because I guess the shock waves 596 00:31:44,080 --> 00:31:46,800 Speaker 1: of these earthquakes or nuclear explosions, they kind of go 597 00:31:46,920 --> 00:31:49,080 Speaker 1: through the rock of the Earth, right, even though it's 598 00:31:49,120 --> 00:31:52,600 Speaker 1: like lava and molten it'll still kind of propagate sound 599 00:31:52,600 --> 00:31:56,240 Speaker 1: waves lava sound waves. Imagine the Earth is just like 600 00:31:56,240 --> 00:31:58,320 Speaker 1: a ball of metal and you ring it with a hammer, 601 00:31:58,360 --> 00:32:00,480 Speaker 1: then those sound chock waves are going to bounce all 602 00:32:00,480 --> 00:32:03,560 Speaker 1: around inside it. And this is actually really cool for 603 00:32:03,760 --> 00:32:07,200 Speaker 1: studying the interior of the Earth. You ring the earth 604 00:32:07,240 --> 00:32:09,520 Speaker 1: and how those shockwaves move through the earth tells you 605 00:32:09,560 --> 00:32:12,040 Speaker 1: about what's inside of it. And like the boundary layers, 606 00:32:12,160 --> 00:32:14,120 Speaker 1: that's actually given us a lot of clues about what's 607 00:32:14,160 --> 00:32:18,040 Speaker 1: inside the earth. Is watching the impact of earthquakes sending 608 00:32:18,080 --> 00:32:21,320 Speaker 1: shockwaves through the earth. It can be hard, however, to 609 00:32:21,320 --> 00:32:24,640 Speaker 1: tell the difference between an earthquake and a smaller nuclear 610 00:32:24,680 --> 00:32:27,200 Speaker 1: weapons explosion, and they try to do a lot these 611 00:32:27,240 --> 00:32:29,800 Speaker 1: days to hide the nuclear weapons explosions by having like 612 00:32:29,920 --> 00:32:33,040 Speaker 1: dampers materials which will absorb a lot of this energy 613 00:32:33,080 --> 00:32:35,520 Speaker 1: instead of properly getting it into the earth. And one 614 00:32:35,560 --> 00:32:38,320 Speaker 1: thing that they've done to try to distinguish between earthquakes 615 00:32:38,320 --> 00:32:41,640 Speaker 1: and nuclear bombs is to listen to it, to take 616 00:32:41,680 --> 00:32:44,520 Speaker 1: the data and translate it into an audio file. And 617 00:32:44,560 --> 00:32:47,440 Speaker 1: it turns out the human brains are pretty good at 618 00:32:47,480 --> 00:32:51,720 Speaker 1: distinguishing the sound of an earthquake versus the sound of 619 00:32:51,760 --> 00:32:55,840 Speaker 1: a nuclear bomb going off. Okay, so sound waves through 620 00:32:55,840 --> 00:32:57,720 Speaker 1: the earth is one way we can detect them here 621 00:32:57,720 --> 00:32:59,760 Speaker 1: on Earth. What are some of the other ways? Other 622 00:32:59,760 --> 00:33:02,680 Speaker 1: ways are through the air and through the water. So 623 00:33:02,880 --> 00:33:06,320 Speaker 1: if you, for example, blowing up underwater, then you create 624 00:33:06,520 --> 00:33:10,560 Speaker 1: hydroacoustic signals. It's just like shock waves through the earth, 625 00:33:10,600 --> 00:33:12,400 Speaker 1: but instead now you're make sways through the water, and 626 00:33:12,440 --> 00:33:15,560 Speaker 1: water is very good at transmitting sound. Right. The speed 627 00:33:15,600 --> 00:33:17,920 Speaker 1: of sound through water is faster than it is through air, 628 00:33:18,160 --> 00:33:20,880 Speaker 1: and so sound travels pretty far. All the way across 629 00:33:20,920 --> 00:33:23,120 Speaker 1: the globe, which is one reason why they think that 630 00:33:23,160 --> 00:33:25,920 Speaker 1: like whales can talk to each other from different parts 631 00:33:25,920 --> 00:33:28,520 Speaker 1: of the planet. You know, they think whales in Japan 632 00:33:28,680 --> 00:33:30,880 Speaker 1: might be able to hear the songs of whales off 633 00:33:30,920 --> 00:33:33,560 Speaker 1: of Alaska, this kind of stuff. And so in the 634 00:33:33,600 --> 00:33:35,680 Speaker 1: same way, if you blow up a nuclear bomb anywhere 635 00:33:35,680 --> 00:33:37,720 Speaker 1: neither its not even just in the water, then the 636 00:33:37,760 --> 00:33:40,120 Speaker 1: seismic waves will propagate through the ocean. And we have 637 00:33:40,120 --> 00:33:43,240 Speaker 1: a lot of listening stations underwater to try to listen 638 00:33:43,360 --> 00:33:47,200 Speaker 1: for all sorts of activity, but including nuclear explosions. Is 639 00:33:47,200 --> 00:33:49,840 Speaker 1: that allowed? Can you test nuclear weapons in the water? 640 00:33:50,160 --> 00:33:53,760 Speaker 1: Definitely not allowed, but has been done in the past, right, 641 00:33:54,040 --> 00:33:56,320 Speaker 1: all right, how else you can also look more directly 642 00:33:56,320 --> 00:33:58,960 Speaker 1: for the radioactivity, right if you do blow up a 643 00:33:59,040 --> 00:34:01,720 Speaker 1: nuclear bomb, and there's a lot of radiation emitted and 644 00:34:01,920 --> 00:34:04,400 Speaker 1: radioactive elements. So one thing we do is we try 645 00:34:04,440 --> 00:34:07,280 Speaker 1: to sample by airplane. You know, you have airplanes flying 646 00:34:07,280 --> 00:34:11,600 Speaker 1: all around the world, and they're sampling for unusual radioactive isotopes, 647 00:34:11,640 --> 00:34:15,000 Speaker 1: some of which are indicative of nuclear explosions. Even if 648 00:34:15,040 --> 00:34:17,719 Speaker 1: you like test it underground, a little bit of these 649 00:34:17,800 --> 00:34:21,319 Speaker 1: radioactive isotopes will eventually leak. It's not always easy to 650 00:34:21,320 --> 00:34:25,000 Speaker 1: tell where the nuclear bomb explosion happened using these techniques, 651 00:34:25,040 --> 00:34:27,720 Speaker 1: because it depends on how it's carried by the wind 652 00:34:27,840 --> 00:34:30,759 Speaker 1: and the weather and how recently it happened. But you 653 00:34:30,800 --> 00:34:33,160 Speaker 1: can sort of tell that one maybe did happen if 654 00:34:33,160 --> 00:34:35,880 Speaker 1: you pick up a signal of these particular fingerprints of 655 00:34:35,880 --> 00:34:39,760 Speaker 1: a nuclear bomb through their radioactive isotopes. So that's happening 656 00:34:39,880 --> 00:34:42,640 Speaker 1: right now. Like there are aeroplanes out there up there 657 00:34:43,480 --> 00:34:47,279 Speaker 1: basically sweeping the earth like a like a roombay. Exactly. 658 00:34:47,680 --> 00:34:49,720 Speaker 1: I don't know the details because they're not public because 659 00:34:49,760 --> 00:34:52,160 Speaker 1: like the US doesn't want Russia, for example, to know 660 00:34:52,280 --> 00:34:55,040 Speaker 1: exactly how it's monitoring it, because then Russia will know 661 00:34:55,320 --> 00:34:57,799 Speaker 1: how best to evade it. So it's a whole game 662 00:34:57,840 --> 00:35:01,000 Speaker 1: of secrecy. But absolutely I'm sure that the Russians and 663 00:35:01,040 --> 00:35:04,920 Speaker 1: the Americans are both monitoring the atmosphere in high altitude 664 00:35:04,920 --> 00:35:07,360 Speaker 1: planes to try to detect whether the other side is 665 00:35:07,400 --> 00:35:10,200 Speaker 1: cheating on the Test band treaty. We're also basically looking 666 00:35:10,200 --> 00:35:12,640 Speaker 1: for these explosions, right like if you can have satellites 667 00:35:12,680 --> 00:35:15,560 Speaker 1: maybe with camera strain at the Earth looking waiting for 668 00:35:15,600 --> 00:35:17,880 Speaker 1: these flashes of light, absolutely, and that's one of the 669 00:35:17,880 --> 00:35:20,200 Speaker 1: most powerful ways we can see these and one of 670 00:35:20,200 --> 00:35:23,040 Speaker 1: the ways that might apply to alien detonations, which is 671 00:35:23,440 --> 00:35:26,360 Speaker 1: just look with satellites, right, we have pictures basically the 672 00:35:26,480 --> 00:35:28,600 Speaker 1: entire surface of the Earth, and we can look for 673 00:35:28,840 --> 00:35:31,719 Speaker 1: high energy sources of gamma rays and X rays, which 674 00:35:31,719 --> 00:35:34,640 Speaker 1: are unusual and you don't expect to produce these things 675 00:35:34,680 --> 00:35:36,680 Speaker 1: in lots of different ways. And so if you see 676 00:35:36,760 --> 00:35:39,759 Speaker 1: one of these signals, flashes of gamma rays, especially the 677 00:35:39,800 --> 00:35:42,520 Speaker 1: double peak signature, then you have a very strong smoking 678 00:35:42,560 --> 00:35:45,120 Speaker 1: gun signature of a nuclear detonation. But what if you 679 00:35:45,280 --> 00:35:48,239 Speaker 1: detonated underground, like deep underground would be with the X 680 00:35:48,360 --> 00:35:50,719 Speaker 1: rays and gamma rays still make it through all those 681 00:35:50,800 --> 00:35:53,520 Speaker 1: layers of rock. It depends a lot on the shielding, right, 682 00:35:53,560 --> 00:35:55,800 Speaker 1: and sometimes they try to shield it with heavier metals 683 00:35:55,880 --> 00:35:58,840 Speaker 1: or they go deep deep underground. X rays can penetrate 684 00:35:58,880 --> 00:36:01,600 Speaker 1: a lot of material. Rays tend to be more ionizing, 685 00:36:01,680 --> 00:36:04,040 Speaker 1: so they do end up getting absorbed, but it depends 686 00:36:04,080 --> 00:36:06,160 Speaker 1: a lot on the depth. All right, Well, that's how 687 00:36:06,239 --> 00:36:09,000 Speaker 1: you can tell if someone exploded something here on Earth. 688 00:36:09,320 --> 00:36:12,680 Speaker 1: But what about the question of aliens exploding things in 689 00:36:12,719 --> 00:36:17,200 Speaker 1: their planets? Could we detect alien explosions or an alien 690 00:36:17,239 --> 00:36:20,040 Speaker 1: nuclear war. So if aliens have the same kind of 691 00:36:20,040 --> 00:36:23,240 Speaker 1: technology that we have, meaning they're blowing up bombs similar 692 00:36:23,239 --> 00:36:24,840 Speaker 1: to the ones we have, then we can look for 693 00:36:24,840 --> 00:36:27,520 Speaker 1: the same signatures from their planets that we would look 694 00:36:27,560 --> 00:36:31,520 Speaker 1: for on Earth. Obviously, we can't look for seismic activity 695 00:36:31,680 --> 00:36:35,920 Speaker 1: or hydroacoustic activity, and we can't sample their atmosphere directly. 696 00:36:36,160 --> 00:36:37,799 Speaker 1: The best way to do it would be to look 697 00:36:37,840 --> 00:36:41,160 Speaker 1: for these gamma ray flashes. And of course we already 698 00:36:41,280 --> 00:36:44,600 Speaker 1: have telescopes that are scanning the sky looking for gamma 699 00:36:44,680 --> 00:36:48,239 Speaker 1: rays because lots of non alien sources of gamma rays 700 00:36:48,320 --> 00:36:51,360 Speaker 1: are very interesting to us, and there's even a huge 701 00:36:51,480 --> 00:36:55,040 Speaker 1: fun physics mystery about gamma ray flashes. These things are 702 00:36:55,040 --> 00:36:58,800 Speaker 1: called gamma ray bursts that come from all over the sky. 703 00:36:59,120 --> 00:37:01,800 Speaker 1: We don't really understand them. They last for like sometimes 704 00:37:01,800 --> 00:37:05,080 Speaker 1: a few seconds, sometimes like thirty seconds. We think they 705 00:37:05,200 --> 00:37:08,960 Speaker 1: might be due to the collapse of supermassive stars, but 706 00:37:09,000 --> 00:37:12,560 Speaker 1: they generate very bright flashes of gamma rays that are 707 00:37:12,600 --> 00:37:15,520 Speaker 1: sort of similar to what you might expect from a 708 00:37:15,640 --> 00:37:19,200 Speaker 1: nuclear detonation. M I think you're sort of painting the 709 00:37:19,320 --> 00:37:23,359 Speaker 1: scenario where We're basically looking at the sky right with 710 00:37:23,520 --> 00:37:26,920 Speaker 1: giant antennas that can detect gamma rays. And if we 711 00:37:27,040 --> 00:37:29,600 Speaker 1: somehow are pointing to a particular planet or star and 712 00:37:29,640 --> 00:37:32,120 Speaker 1: we see a big flash or a signal, then that 713 00:37:32,160 --> 00:37:34,480 Speaker 1: could be the sign that the amiens blew themselves up. 714 00:37:34,560 --> 00:37:36,400 Speaker 1: It could be the sign. As one of the members 715 00:37:36,400 --> 00:37:40,040 Speaker 1: of Listener Panel pointed out, it might be hard to distinguish. Right. 716 00:37:40,360 --> 00:37:43,719 Speaker 1: On one hand, it's cool that supermassive stars collapse and 717 00:37:43,760 --> 00:37:46,120 Speaker 1: give off gamma ray bursts. On the other hand, it's 718 00:37:46,160 --> 00:37:48,480 Speaker 1: a bit of a bomber because it makes it harder 719 00:37:48,480 --> 00:37:52,279 Speaker 1: to distinguish between alien nuclear bomb gamma ray bursts and 720 00:37:52,440 --> 00:37:55,760 Speaker 1: just natural sources of gamma ray bursts. But I guess 721 00:37:55,760 --> 00:37:59,080 Speaker 1: if it was a super massive star collapsing, wouldn't we 722 00:37:59,160 --> 00:38:01,600 Speaker 1: also see other signs that go along with it that 723 00:38:01,680 --> 00:38:04,799 Speaker 1: wouldn't go along with a nuclear explosion. It could be, 724 00:38:05,000 --> 00:38:07,400 Speaker 1: And one thing we're doing is to try to study 725 00:38:07,480 --> 00:38:10,040 Speaker 1: these gamma ray bursts in more detail and see whether 726 00:38:10,080 --> 00:38:13,279 Speaker 1: they come along with other signs like flashes of neutrinos 727 00:38:13,400 --> 00:38:16,279 Speaker 1: or other things we can see in the optical To 728 00:38:16,320 --> 00:38:18,520 Speaker 1: try to figure these things out. We don't always have 729 00:38:18,560 --> 00:38:20,080 Speaker 1: a lot of warning, right, We don't know when it's 730 00:38:20,120 --> 00:38:21,719 Speaker 1: going to happen. We just see like, oh wow, that 731 00:38:21,840 --> 00:38:24,120 Speaker 1: was a big flash of gamma rays from this spot 732 00:38:24,200 --> 00:38:26,640 Speaker 1: in the sky. You don't always have time to train 733 00:38:26,800 --> 00:38:29,680 Speaker 1: other telescopes on that spot to get sort of multi 734 00:38:29,880 --> 00:38:32,840 Speaker 1: channel data, and they do look kind of similar. In fact, 735 00:38:33,080 --> 00:38:36,799 Speaker 1: when we first discovered gamma ray bursts, scientists thought that 736 00:38:36,880 --> 00:38:40,839 Speaker 1: what they were seeing were gamma rays from earthbound detonations 737 00:38:40,840 --> 00:38:43,640 Speaker 1: of nuclear weapons. They thought they had just picked up 738 00:38:43,840 --> 00:38:48,480 Speaker 1: the Russian explosions because I would explain the signal too, Yeah, 739 00:38:48,600 --> 00:38:51,239 Speaker 1: because that would have explained the signal. Now, gamma ray 740 00:38:51,280 --> 00:38:55,520 Speaker 1: bursts come from really really incredibly powerful events. These things 741 00:38:55,520 --> 00:38:58,480 Speaker 1: release enormous amounts of energy, so we can see gamma 742 00:38:58,520 --> 00:39:01,560 Speaker 1: ray bursts from all across the universe. We've seen them 743 00:39:01,600 --> 00:39:04,600 Speaker 1: from really really far away, like millions and millions, almost 744 00:39:04,600 --> 00:39:08,120 Speaker 1: a billion light years away, because they are so powerful. 745 00:39:08,280 --> 00:39:11,120 Speaker 1: Some of these things released like ten to the forty 746 00:39:11,200 --> 00:39:15,799 Speaker 1: four jewels of energy just in the gamma rays, and 747 00:39:15,880 --> 00:39:18,399 Speaker 1: so they're very bright, very powerful. We can see these 748 00:39:18,440 --> 00:39:21,600 Speaker 1: things from very very far away. Our nuclear bombs are 749 00:39:21,640 --> 00:39:24,759 Speaker 1: not nearly as powerful as these other natural sources of 750 00:39:24,880 --> 00:39:28,200 Speaker 1: gamma rays, so they would be relatively dim in comparison. 751 00:39:28,360 --> 00:39:30,239 Speaker 1: You mean if there was an alien looking at us 752 00:39:30,280 --> 00:39:33,279 Speaker 1: for these gamma ray bursts, Yeah, exactly. If aliens were 753 00:39:33,280 --> 00:39:37,280 Speaker 1: watching our nuclear explosions and they had technology similar to hours, 754 00:39:37,680 --> 00:39:40,399 Speaker 1: they would not be able to see our explosions from 755 00:39:40,480 --> 00:39:43,160 Speaker 1: very very far away because our explosions are not that 756 00:39:43,280 --> 00:39:46,960 Speaker 1: bright compared to gamma ray bursts. Well, sort of depends 757 00:39:46,960 --> 00:39:49,759 Speaker 1: on how many nukes we detonate at the same time. 758 00:39:49,960 --> 00:39:52,360 Speaker 1: It does. But if you imagine, like a doomsday scenario, 759 00:39:52,400 --> 00:39:54,520 Speaker 1: you take all of our nuclear weapons, you set them 760 00:39:54,560 --> 00:39:57,400 Speaker 1: all off at the same time, you can calculate, like 761 00:39:57,440 --> 00:40:00,600 Speaker 1: how much energy in gamma ray bursts would be emitted. 762 00:40:00,840 --> 00:40:05,320 Speaker 1: It's only like ten to the nineteen jewels, Like obviously cataclysmic, 763 00:40:05,560 --> 00:40:09,480 Speaker 1: terrible scenario, enough energy to devastate civilization on Earth. But 764 00:40:09,560 --> 00:40:11,719 Speaker 1: compared to gamma ray bursts, which are ten to the 765 00:40:11,880 --> 00:40:14,800 Speaker 1: forty four jewels, we're talking about ten to the twenty 766 00:40:14,800 --> 00:40:18,480 Speaker 1: five times less powerful than a gamma ray burst, So 767 00:40:18,520 --> 00:40:22,600 Speaker 1: they're relatively dim compared to these other astrophysical sources. It's 768 00:40:22,680 --> 00:40:27,000 Speaker 1: twenty five orders of magnitude weaker, but I guess you're saying, like, 769 00:40:27,080 --> 00:40:30,440 Speaker 1: if we do see a gamma ray burst and we're 770 00:40:30,520 --> 00:40:33,000 Speaker 1: not sure if it's an alien or a star collapsing, 771 00:40:33,280 --> 00:40:36,120 Speaker 1: I mean that would mean that this alien civilization blew 772 00:40:36,200 --> 00:40:40,399 Speaker 1: up twenty five orders of magnude, many more bombs than 773 00:40:40,400 --> 00:40:42,919 Speaker 1: we did. We're a bomb that was twenty five orders 774 00:40:43,000 --> 00:40:45,399 Speaker 1: of magnitude bigger than ours. Yeah, it depends on how 775 00:40:45,440 --> 00:40:47,640 Speaker 1: far away they are. If they are as far away 776 00:40:47,640 --> 00:40:50,399 Speaker 1: as some of these really distant gamma ray bursts, then 777 00:40:50,440 --> 00:40:53,400 Speaker 1: you're right, they would have like much much bigger nuclear 778 00:40:53,520 --> 00:40:56,759 Speaker 1: arsenals than we have, like ten to twenty five times 779 00:40:56,800 --> 00:41:01,960 Speaker 1: as powerful, or they had or they exactly exactly kind 780 00:41:02,000 --> 00:41:04,879 Speaker 1: of tense. But if you're imagining an alien civilization with 781 00:41:04,920 --> 00:41:07,440 Speaker 1: the power of our nuclear weapons and they had some 782 00:41:07,480 --> 00:41:09,960 Speaker 1: sort of cataclysmic event where they blew them all up 783 00:41:10,000 --> 00:41:12,479 Speaker 1: at once, then you can ask how far away would 784 00:41:12,480 --> 00:41:14,839 Speaker 1: they be for us to detect it. Our gamma ray 785 00:41:14,880 --> 00:41:18,080 Speaker 1: sensors are pretty sensitive, but remember that things get much 786 00:41:18,200 --> 00:41:20,920 Speaker 1: dimmer as you get further away, so the sources have 787 00:41:21,000 --> 00:41:24,040 Speaker 1: to be very bright to be visible. For an alien 788 00:41:24,120 --> 00:41:27,640 Speaker 1: nuclear war at human levels to look about as bright 789 00:41:27,680 --> 00:41:30,600 Speaker 1: as a typical gamma ray burst, that we see it 790 00:41:30,640 --> 00:41:34,480 Speaker 1: could only be around eight to ten astronomical units away 791 00:41:35,040 --> 00:41:38,120 Speaker 1: because it wouldn't be nearly as bright as its source 792 00:41:38,520 --> 00:41:41,359 Speaker 1: as gamma ray bursts that are typically much further. So 793 00:41:41,480 --> 00:41:44,280 Speaker 1: eight to ten AU that's like the distance to Pluto. 794 00:41:44,480 --> 00:41:47,040 Speaker 1: Beyond that, we might still be able to pick it up, 795 00:41:47,040 --> 00:41:50,080 Speaker 1: but it would start getting dimmer very fast because remember 796 00:41:50,360 --> 00:41:53,760 Speaker 1: the next star over is much further away than Pluto. 797 00:41:53,960 --> 00:41:56,720 Speaker 1: So it's possible to see it in another star system, 798 00:41:57,000 --> 00:42:00,680 Speaker 1: but not a guarantee, and our abilities fade very quickly 799 00:42:00,920 --> 00:42:04,680 Speaker 1: as you consider even further star systems. So if like 800 00:42:04,760 --> 00:42:07,080 Speaker 1: there are aliens in Pluto and they had a nuclear 801 00:42:07,120 --> 00:42:09,799 Speaker 1: war and they detonated all their nuclear weapons, then we 802 00:42:09,800 --> 00:42:13,160 Speaker 1: would see it through the gamma ray radiation. But if 803 00:42:13,200 --> 00:42:15,719 Speaker 1: it happened like and in another source system, it'd be 804 00:42:15,800 --> 00:42:18,440 Speaker 1: way too dim, or would it, or maybe maybe just 805 00:42:18,520 --> 00:42:21,480 Speaker 1: need better instruments. I mean, you're not saying it's impossible, 806 00:42:21,600 --> 00:42:23,560 Speaker 1: or you're saying it's impossible, or that it's really hard. 807 00:42:23,680 --> 00:42:25,520 Speaker 1: I'm not saying it's impossible. I'm saying it's at the 808 00:42:25,680 --> 00:42:28,959 Speaker 1: edge of our ability currently, like we can barely pick 809 00:42:29,080 --> 00:42:33,480 Speaker 1: up super bright, very distant gamma ray bursts, or we 810 00:42:33,520 --> 00:42:37,759 Speaker 1: could pick up less bright closer gamma ray bursts. Right, 811 00:42:37,920 --> 00:42:40,560 Speaker 1: there's sort of a line there between distance and brightness. 812 00:42:40,640 --> 00:42:42,719 Speaker 1: But we could also improve our technology and make our 813 00:42:42,719 --> 00:42:46,000 Speaker 1: gamma ray detectors more sensitive. Then we could see dimmer 814 00:42:46,040 --> 00:42:48,719 Speaker 1: things that were further away, including gamma ray bursts or 815 00:42:48,800 --> 00:42:52,040 Speaker 1: alien technology. Is definitely not impossible. But I think you 816 00:42:52,200 --> 00:42:54,680 Speaker 1: said that gamma ray are only one of the things 817 00:42:54,719 --> 00:42:56,759 Speaker 1: that come out of a nuclear explosion. There's also like 818 00:42:56,800 --> 00:42:59,919 Speaker 1: the actual visible light flash tour, and that's like many 819 00:43:00,080 --> 00:43:02,560 Speaker 1: times bigger than the gamma ray burst. Do we see 820 00:43:02,680 --> 00:43:06,400 Speaker 1: a star war happening just on the visible spectrum? We 821 00:43:06,480 --> 00:43:08,520 Speaker 1: might be able to, but the universe is a little 822 00:43:08,520 --> 00:43:11,839 Speaker 1: bit less transparent to that kind of light. Gamma rays 823 00:43:11,920 --> 00:43:15,160 Speaker 1: are awesome because most of the universe is transparent to them, 824 00:43:15,239 --> 00:43:17,439 Speaker 1: but visible life, for example, is more likely to get 825 00:43:17,440 --> 00:43:20,400 Speaker 1: blocked by gas or dust or these kinds of things. 826 00:43:20,640 --> 00:43:25,279 Speaker 1: But it is possible, and we should look for multiple signatures. Right, 827 00:43:25,320 --> 00:43:27,200 Speaker 1: So we can look at the gamma rays, we can 828 00:43:27,239 --> 00:43:29,520 Speaker 1: look in the visible light. We certainly should keep an 829 00:43:29,520 --> 00:43:32,520 Speaker 1: eye on that. There are also other more subtle ways 830 00:43:32,560 --> 00:43:36,319 Speaker 1: that we might be able to detect nuclear weapons explosions 831 00:43:36,440 --> 00:43:40,160 Speaker 1: on other planets and to distinguish them from gamma ray bursts. 832 00:43:40,200 --> 00:43:43,240 Speaker 1: The point you were making earlier about telling the difference 833 00:43:43,239 --> 00:43:46,239 Speaker 1: between nuclear weapons and gamma rays. All right, let's get 834 00:43:46,280 --> 00:43:49,280 Speaker 1: into those other ways we could detect an alien nuclear 835 00:43:49,280 --> 00:43:52,440 Speaker 1: war and whether or not it might ever happen. But 836 00:43:52,560 --> 00:44:08,680 Speaker 1: first let's take another quick break. All right, So what 837 00:44:08,719 --> 00:44:10,719 Speaker 1: do you think is the scenaro here where aliens have 838 00:44:10,760 --> 00:44:14,360 Speaker 1: a nuclear war? Do you think they just disagree about something? 839 00:44:15,080 --> 00:44:18,280 Speaker 1: Do you think it's inevitable for all civilizations to eventually 840 00:44:18,320 --> 00:44:21,440 Speaker 1: snuff themselves out? I don't know. I've heard this theory, 841 00:44:21,480 --> 00:44:24,600 Speaker 1: you know, the great filter that the reason we haven't 842 00:44:24,680 --> 00:44:28,160 Speaker 1: seen aliens or been visited by their probes is that 843 00:44:28,320 --> 00:44:31,839 Speaker 1: technological civilizations don't tend to last very long because they 844 00:44:31,880 --> 00:44:35,480 Speaker 1: tend to destroy themselves through climate change or annihilation or 845 00:44:35,560 --> 00:44:38,719 Speaker 1: war or whatever. And that's possible, I suppose, but it 846 00:44:38,760 --> 00:44:41,600 Speaker 1: seems to me like a huge amount of projection. It's 847 00:44:41,640 --> 00:44:44,439 Speaker 1: imagining that aliens are a lot like humans, and their 848 00:44:44,480 --> 00:44:47,879 Speaker 1: psychology and their struggles and their sociology is a lot 849 00:44:47,920 --> 00:44:50,480 Speaker 1: like ours. And that's possible, But it also seems to 850 00:44:50,520 --> 00:44:52,680 Speaker 1: me to be possible for it to be completely different, 851 00:44:52,719 --> 00:44:54,520 Speaker 1: for their politics to be totally different, and they never 852 00:44:54,560 --> 00:44:58,200 Speaker 1: even invent nuclear weapons. So I think it's too big 853 00:44:58,200 --> 00:45:01,839 Speaker 1: a question without really data to speculate on. Yeah, it's 854 00:45:01,840 --> 00:45:03,759 Speaker 1: a big unknown, but I think it has maybe kind 855 00:45:03,760 --> 00:45:05,840 Speaker 1: of the basis and the idea that, you know, anything 856 00:45:05,880 --> 00:45:10,640 Speaker 1: that evolves evolution works by competition, right, and so basically 857 00:45:10,680 --> 00:45:14,560 Speaker 1: any intelligent society will most likely it kind of come 858 00:45:14,600 --> 00:45:17,520 Speaker 1: up like we did, being having this kind of balanced, 859 00:45:17,600 --> 00:45:21,280 Speaker 1: this idea of competition and killing each other but also 860 00:45:21,520 --> 00:45:24,279 Speaker 1: being nice to each other. Yeah. We had an astrozoologist 861 00:45:24,360 --> 00:45:26,879 Speaker 1: on the podcast recently who made that point. He said, 862 00:45:26,880 --> 00:45:30,200 Speaker 1: predation is inevitable in evolution. You will eventually have one 863 00:45:30,239 --> 00:45:33,200 Speaker 1: guy that wants to eat the neighboring guy. And that's 864 00:45:33,280 --> 00:45:36,319 Speaker 1: probably true, but it doesn't mean that it doesn't mean 865 00:45:36,360 --> 00:45:39,759 Speaker 1: you can't like progress past your evolutionary impulses. Right. Our 866 00:45:39,760 --> 00:45:42,759 Speaker 1: behavior now is quite different from the behavior in which 867 00:45:42,800 --> 00:45:46,399 Speaker 1: we evolve, much more complex cooperative society. So I don't 868 00:45:46,400 --> 00:45:50,320 Speaker 1: know that it's inevitable that you're dominated by that competitive nature, 869 00:45:50,400 --> 00:45:53,399 Speaker 1: but hey, let's find out hopefully, listen, let's not find 870 00:45:53,400 --> 00:45:57,200 Speaker 1: out the negative outcome the hard way. So you're saying 871 00:45:57,239 --> 00:46:00,799 Speaker 1: before that for us to see alien nuclear explosions in 872 00:46:00,880 --> 00:46:04,040 Speaker 1: other planets, I mean they would have to basically detonate 873 00:46:04,200 --> 00:46:07,319 Speaker 1: twenty five orders of Maude, many more bombs that all 874 00:46:07,320 --> 00:46:10,160 Speaker 1: of humanity has for us to even have a chance 875 00:46:10,200 --> 00:46:12,360 Speaker 1: to see it. Yes, for us to detect these bright flashes, 876 00:46:12,680 --> 00:46:15,280 Speaker 1: they would have to have a much more substantial arsenal 877 00:46:15,360 --> 00:46:18,000 Speaker 1: than we have twenty five orders of magnitude more right, 878 00:46:18,360 --> 00:46:22,040 Speaker 1: like bombs that could destroy you. I don't even know 879 00:46:22,120 --> 00:46:24,920 Speaker 1: the number for that, but twenty five orders of magnitude 880 00:46:24,920 --> 00:46:27,239 Speaker 1: many more planets. Yeah, sorry, I don't know if I 881 00:46:27,280 --> 00:46:29,560 Speaker 1: said twenty five times right, it's ten to the twenty 882 00:46:29,560 --> 00:46:32,240 Speaker 1: five times, So it's one with a lot of zeros 883 00:46:32,320 --> 00:46:34,840 Speaker 1: in front of it. Absolutely, But if they do have 884 00:46:34,920 --> 00:46:38,440 Speaker 1: a canterclismic nuclear war, there will also be other impacts 885 00:46:38,640 --> 00:46:41,280 Speaker 1: on their planet that we might be able to detect 886 00:46:41,320 --> 00:46:43,759 Speaker 1: even if we don't spot the gamma ray burst. And 887 00:46:43,800 --> 00:46:45,759 Speaker 1: these are the kind of things we might be able 888 00:46:45,760 --> 00:46:48,920 Speaker 1: to spot from planets in other solar systems. And number 889 00:46:48,920 --> 00:46:53,000 Speaker 1: one on that list is changes in their atmosphere. You mean, 890 00:46:53,040 --> 00:46:56,400 Speaker 1: like maybe we don't detect the explosion itself, that of 891 00:46:56,480 --> 00:47:00,480 Speaker 1: the nuclear war. But we can detect their nuclear winter exactly, 892 00:47:00,760 --> 00:47:03,640 Speaker 1: their nuclear winter. If you do have this kind of 893 00:47:03,680 --> 00:47:05,800 Speaker 1: event where you blow up a lot of nuclear bombs 894 00:47:05,800 --> 00:47:09,319 Speaker 1: in your atmosphere, it would really change your atmosphere. Number One, 895 00:47:09,360 --> 00:47:13,080 Speaker 1: it would very briefly make your atmosphere glow. Right, you're 896 00:47:13,160 --> 00:47:16,000 Speaker 1: dumping a huge amount of energy into your atmosphere. It 897 00:47:16,040 --> 00:47:19,240 Speaker 1: would ionize a bunch of the gases from the radiation 898 00:47:19,400 --> 00:47:22,480 Speaker 1: produced by a lot of the byproducts, and so the 899 00:47:22,520 --> 00:47:25,640 Speaker 1: atmosphere itself would glow sort of like the Northern lights. 900 00:47:25,840 --> 00:47:28,520 Speaker 1: Ionized air tends to emit this kind of glow. We've 901 00:47:28,520 --> 00:47:30,279 Speaker 1: seen it on Earth, we've seen it on Venus, we've 902 00:47:30,280 --> 00:47:32,759 Speaker 1: seen it on Mars. And so if you have a 903 00:47:32,760 --> 00:47:35,839 Speaker 1: lot of nuclear bombs, then their atmosphere would have this 904 00:47:36,000 --> 00:47:38,040 Speaker 1: air glow and we might be able to spot that. 905 00:47:38,200 --> 00:47:40,920 Speaker 1: Wait wait, wait, we could see their atmosphere glow like 906 00:47:41,000 --> 00:47:44,640 Speaker 1: how like with telescopes. Yeah, telescopes pointed at these planets 907 00:47:44,920 --> 00:47:47,680 Speaker 1: might be able to gather some information about the light 908 00:47:47,719 --> 00:47:50,360 Speaker 1: that's coming directly from the planet. Right, we now have 909 00:47:50,600 --> 00:47:54,720 Speaker 1: direct imaging of exoplanets. And if you see, for example, 910 00:47:55,000 --> 00:47:58,839 Speaker 1: a spike in the oxygen line, that increases the oxygen 911 00:47:59,000 --> 00:48:02,480 Speaker 1: rapidly by a factor of ten than our telescopes could 912 00:48:02,480 --> 00:48:05,280 Speaker 1: spot that. But wait, if we can see their amosphere glow, 913 00:48:05,400 --> 00:48:09,840 Speaker 1: surely we would see their explosions themselves, right, Like explosions 914 00:48:09,840 --> 00:48:12,400 Speaker 1: would be pretty flashy, right, he said, forty percent of 915 00:48:12,400 --> 00:48:16,040 Speaker 1: a nuclear explosions energy goes into visible light. I mean, 916 00:48:16,040 --> 00:48:18,399 Speaker 1: if we can see their atmospherre glow, surely we would 917 00:48:18,400 --> 00:48:21,360 Speaker 1: see their like a big flash before the explosion or 918 00:48:21,880 --> 00:48:24,839 Speaker 1: during the explosion. The explosion itself might not be bright 919 00:48:24,960 --> 00:48:27,480 Speaker 1: enough for us to see. It'll also be really short lived. 920 00:48:27,680 --> 00:48:29,920 Speaker 1: What we're talking about here is seeing a change in 921 00:48:29,960 --> 00:48:33,200 Speaker 1: the atmosphere chemistry, which we usually detect from how the 922 00:48:33,320 --> 00:48:37,000 Speaker 1: light from the planet's star passes through its atmosphere or 923 00:48:37,080 --> 00:48:39,759 Speaker 1: reflex off its atmosphere. So the light we get from 924 00:48:39,800 --> 00:48:42,560 Speaker 1: these planets is not from any source on the planet itself, 925 00:48:42,680 --> 00:48:45,600 Speaker 1: but from the star, which is why it's visible at all. 926 00:48:45,719 --> 00:48:48,719 Speaker 1: The air glow might last longer than the flash, and 927 00:48:48,760 --> 00:48:50,920 Speaker 1: so it might be easier to spot. But what we're 928 00:48:50,920 --> 00:48:53,759 Speaker 1: doing is thinking about, like what are the multiple signatures, 929 00:48:54,400 --> 00:48:56,359 Speaker 1: Because in the end, the story is going to be 930 00:48:56,480 --> 00:48:59,959 Speaker 1: that you probably can't conclude that you've seen an alien 931 00:49:00,040 --> 00:49:02,680 Speaker 1: an explosion based on only one of these signatures, because 932 00:49:02,680 --> 00:49:05,000 Speaker 1: there are other ways to mimic any one of them. 933 00:49:05,440 --> 00:49:08,040 Speaker 1: So to conclude you've seen alien signatures, what you're going 934 00:49:08,080 --> 00:49:12,440 Speaker 1: to want is multiple pieces of evidence. I see, like 935 00:49:12,480 --> 00:49:15,400 Speaker 1: the afterglow will last longer, so there's more likelihood that 936 00:49:15,440 --> 00:49:17,160 Speaker 1: will see it. But also it's sort of like more 937 00:49:17,200 --> 00:49:21,080 Speaker 1: of a telltale sign. If planet is glowing more than 938 00:49:21,120 --> 00:49:23,520 Speaker 1: it should, then you can maybe infer that there was 939 00:49:23,520 --> 00:49:25,880 Speaker 1: an explosion there exactly, like maybe you see a gamma 940 00:49:25,920 --> 00:49:27,879 Speaker 1: ray burst and you see a bright flash of light 941 00:49:28,000 --> 00:49:30,200 Speaker 1: from the visible light emission and you're wondering, like, well, 942 00:49:30,400 --> 00:49:33,320 Speaker 1: was that some sort of star collapsing or was it 943 00:49:33,400 --> 00:49:35,400 Speaker 1: an alien nuclear bomb? Then you can look for the 944 00:49:35,440 --> 00:49:38,040 Speaker 1: air glow. There are other effects in the atmosphere as well, 945 00:49:38,440 --> 00:49:41,040 Speaker 1: like these blasts tend to produce a lot of nitrogen 946 00:49:41,080 --> 00:49:45,080 Speaker 1: oxides which react with and deplete ozone, And so if 947 00:49:45,080 --> 00:49:48,120 Speaker 1: you're watching the atmosphere of this planet, then you're looking 948 00:49:48,120 --> 00:49:50,799 Speaker 1: in the UV light, you can detect changes in the 949 00:49:50,840 --> 00:49:53,920 Speaker 1: ozone layer. So a lot of these other signals require 950 00:49:53,920 --> 00:49:56,600 Speaker 1: you to be looking at one of these planets already 951 00:49:56,640 --> 00:50:01,239 Speaker 1: in studying its atmosphere and seeing change in its atmosphere, 952 00:50:01,280 --> 00:50:03,920 Speaker 1: so it increases an ionization of the gases that lead 953 00:50:03,960 --> 00:50:07,520 Speaker 1: to air glow or decrease in the ozone layer by 954 00:50:07,560 --> 00:50:10,560 Speaker 1: interaction from some of the byproducts of the blast. Or 955 00:50:10,600 --> 00:50:14,040 Speaker 1: if you just like see the atmosphere become opaque, Right, 956 00:50:14,080 --> 00:50:15,920 Speaker 1: you have a bunch of nuclear bombs go off, it's 957 00:50:15,960 --> 00:50:18,040 Speaker 1: going to throw up a huge amount of either vapor 958 00:50:18,480 --> 00:50:21,759 Speaker 1: or dust or something to make the atmosphere more opaque, 959 00:50:22,040 --> 00:50:24,600 Speaker 1: and that could last for years. Right, We're talking about 960 00:50:24,600 --> 00:50:27,360 Speaker 1: a nuclear winter. And so if you see an atmosphere 961 00:50:27,400 --> 00:50:30,479 Speaker 1: becomes suddenly more opaque than it was before, that tells 962 00:50:30,480 --> 00:50:34,720 Speaker 1: you something big happened in that atmosphere, Like if there's 963 00:50:34,800 --> 00:50:36,680 Speaker 1: more dust in the atmosphere, Although that could also be 964 00:50:36,719 --> 00:50:40,440 Speaker 1: an asteroid, right, Like if an asteroid hits planet, it 965 00:50:40,480 --> 00:50:43,480 Speaker 1: would also cause a big flash of light and also 966 00:50:43,520 --> 00:50:45,560 Speaker 1: a lot put a lot of stuff in the atmosphere, right, 967 00:50:46,040 --> 00:50:48,759 Speaker 1: Or would it look differently? Is it's not radioactive? Yeah, 968 00:50:48,800 --> 00:50:51,960 Speaker 1: an asteroid wouldn't look exactly the same as a nuclear 969 00:50:52,000 --> 00:50:54,480 Speaker 1: bomb because it wouldn't deplete the ozone in the same way. 970 00:50:54,520 --> 00:50:56,400 Speaker 1: It might not cause the same amount of air glow 971 00:50:56,719 --> 00:50:59,359 Speaker 1: because it wouldn't have the same sort of radioactive byproducts, 972 00:50:59,520 --> 00:51:01,560 Speaker 1: but a lot of the signatures would be the same. 973 00:51:01,800 --> 00:51:03,640 Speaker 1: It would throw up a lot of dust in the atmosphere, 974 00:51:03,680 --> 00:51:06,880 Speaker 1: probably make the atmosphere opaque for years as well, but 975 00:51:06,880 --> 00:51:09,160 Speaker 1: you probably wouldn't also get the gamma ray burst. So 976 00:51:09,200 --> 00:51:11,719 Speaker 1: there's lots of things out there in the universe that 977 00:51:11,800 --> 00:51:16,400 Speaker 1: could make signatures similar to alien nuclear total annihilation, global 978 00:51:16,400 --> 00:51:19,440 Speaker 1: thermonuclear war, but not all of them. So if you 979 00:51:19,560 --> 00:51:22,680 Speaker 1: happen to see like several of these signatures all together 980 00:51:23,200 --> 00:51:26,319 Speaker 1: from an exoplanet, then you could probably conclude that there 981 00:51:26,360 --> 00:51:28,560 Speaker 1: were aliens and they had just had a very very 982 00:51:28,640 --> 00:51:32,600 Speaker 1: bad day. Or maybe they were celebrating something, you know, 983 00:51:33,280 --> 00:51:35,800 Speaker 1: it's just how they do fireworks in that ailing culture. 984 00:51:36,120 --> 00:51:39,960 Speaker 1: Maybe they detected us and they were celebrating because they 985 00:51:39,960 --> 00:51:41,759 Speaker 1: were going to get to eat a good mule latter. 986 00:51:42,080 --> 00:51:44,120 Speaker 1: Or maybe they try to have some fireworks and they 987 00:51:44,160 --> 00:51:47,560 Speaker 1: accidentally shot the fireworks right at their nuclear arsenal and 988 00:51:47,640 --> 00:51:50,600 Speaker 1: set it off. I think I've seen that on TikTok. 989 00:51:50,880 --> 00:51:52,560 Speaker 1: All right, well, I kind of feel like we have 990 00:51:52,600 --> 00:51:55,640 Speaker 1: to be looking for these things though, right, like gamma rays, 991 00:51:55,680 --> 00:51:57,840 Speaker 1: it's not like we have a camera looking out the 992 00:51:57,880 --> 00:52:01,200 Speaker 1: whole universe looking for gamma ray. Gamma detectors here on 993 00:52:01,239 --> 00:52:03,440 Speaker 1: Earth are very specific. Likely we have to point them 994 00:52:03,480 --> 00:52:06,680 Speaker 1: at specific stars and stuff, right, So it seems kind 995 00:52:06,680 --> 00:52:10,360 Speaker 1: of unlikely that will just happen to catch another civilization 996 00:52:10,840 --> 00:52:14,160 Speaker 1: having their nuclear war just as we're pointing our telescope 997 00:52:14,160 --> 00:52:16,319 Speaker 1: at them. I yeah, exactly. I think some people were 998 00:52:16,360 --> 00:52:18,680 Speaker 1: hoping that this would be a very easy way, a 999 00:52:18,760 --> 00:52:23,279 Speaker 1: very obvious way to identify alien civilizations. But unfortunately they're 1000 00:52:23,280 --> 00:52:25,920 Speaker 1: not as bright as you might imagine, and the universe 1001 00:52:26,040 --> 00:52:28,000 Speaker 1: is very very large, and there are other ways to 1002 00:52:28,040 --> 00:52:30,080 Speaker 1: create a lot of these signals, and so you have 1003 00:52:30,160 --> 00:52:31,960 Speaker 1: to be very lucky. You'd have to be looking at 1004 00:52:31,960 --> 00:52:35,120 Speaker 1: a planet basically when this happens, and have been looking 1005 00:52:35,160 --> 00:52:38,160 Speaker 1: at it beforehand so you could see the changes. And 1006 00:52:38,239 --> 00:52:40,560 Speaker 1: this is one of the big problems in detecting alien 1007 00:52:40,560 --> 00:52:44,680 Speaker 1: civilizations is just the deep length of time. Right, Maybe 1008 00:52:44,719 --> 00:52:47,640 Speaker 1: alien civilizations have existed and they've all killed each other 1009 00:52:47,719 --> 00:52:49,839 Speaker 1: and those signals came to Earth, but like a few 1010 00:52:49,960 --> 00:52:53,120 Speaker 1: hundred years ago and we missed it, right. Jill Tarter 1011 00:52:53,239 --> 00:52:56,040 Speaker 1: is famous for saying that we've been watching for aliens 1012 00:52:56,040 --> 00:53:00,520 Speaker 1: for a cosmically insignificant amount of time, and adding looking 1013 00:53:00,520 --> 00:53:03,719 Speaker 1: for nuclear explosions is a good way to increase our 1014 00:53:03,760 --> 00:53:07,800 Speaker 1: ability to see them, But it doesn't change this problem 1015 00:53:07,840 --> 00:53:10,600 Speaker 1: that we've only been looking very very briefly, and aliens 1016 00:53:10,640 --> 00:53:13,359 Speaker 1: could have existed and lived for millions of years and 1017 00:53:13,440 --> 00:53:16,040 Speaker 1: died off recently and we still wouldn't have seen it. Yeah, 1018 00:53:16,040 --> 00:53:17,600 Speaker 1: I see what you're saying. You're saying like, maybe these 1019 00:53:17,640 --> 00:53:20,759 Speaker 1: star wars happened a long long time ago and the 1020 00:53:20,840 --> 00:53:23,480 Speaker 1: galaxy far far away. Is that kind of what the 1021 00:53:23,600 --> 00:53:28,839 Speaker 1: conclusion of scientists is, Yes, exactly, that's entirely possible. Which 1022 00:53:28,880 --> 00:53:31,080 Speaker 1: I feel like I've seen that in a movie already. 1023 00:53:31,280 --> 00:53:33,920 Speaker 1: Did somebody have that idea already? Dang it, man, every 1024 00:53:33,920 --> 00:53:36,040 Speaker 1: time I have a good idea, it's still your Nobel 1025 00:53:36,120 --> 00:53:41,240 Speaker 1: Prize again and my ten billion dollars in box office receipts. 1026 00:53:41,360 --> 00:53:43,200 Speaker 1: All right, Well, I think it's still kind of interesting 1027 00:53:43,239 --> 00:53:45,840 Speaker 1: to think about, right, It's still worth thinking about because 1028 00:53:46,000 --> 00:53:49,480 Speaker 1: we do happen to see the city signals, right then 1029 00:53:49,600 --> 00:53:52,240 Speaker 1: we would know a lot about not only the idea 1030 00:53:52,280 --> 00:53:54,920 Speaker 1: that we're out there alone or not, but also like 1031 00:53:55,719 --> 00:53:58,759 Speaker 1: what these other aliens are capable of. Yeah, and these 1032 00:53:58,800 --> 00:54:01,800 Speaker 1: aliens could have court developed technologies that are far beyond 1033 00:54:01,880 --> 00:54:04,560 Speaker 1: what we have and create flashes of light much much 1034 00:54:04,600 --> 00:54:07,640 Speaker 1: brighter than the kinds of things we're imagining, and we 1035 00:54:07,640 --> 00:54:09,560 Speaker 1: should keep our eyes open for that. I think the 1036 00:54:09,600 --> 00:54:11,840 Speaker 1: spirit of this is just to try to be inclusive 1037 00:54:11,880 --> 00:54:13,760 Speaker 1: about the kind of things we're looking for, to increase 1038 00:54:13,800 --> 00:54:17,359 Speaker 1: our chances of seeing anything at all. Yeah, or I think, 1039 00:54:17,400 --> 00:54:19,560 Speaker 1: as we talked about in other episodes, like you might 1040 00:54:19,600 --> 00:54:22,160 Speaker 1: be limited in your imagination, right, Like maybe if you 1041 00:54:22,160 --> 00:54:26,800 Speaker 1: imagine giant space civilizations and have bombs that are twenty 1042 00:54:26,800 --> 00:54:30,240 Speaker 1: five orders of mine need to bigger than our bombs, 1043 00:54:30,400 --> 00:54:33,319 Speaker 1: then we would be able to see that kind of spectacle. Yeah, 1044 00:54:33,360 --> 00:54:36,680 Speaker 1: we talked about the Kardaship scale of civilizations. Some aliens 1045 00:54:36,760 --> 00:54:39,359 Speaker 1: might have tapped into all of the energy output of 1046 00:54:39,400 --> 00:54:43,920 Speaker 1: their sun and built a huge laser capable of vaporizing planets. 1047 00:54:44,280 --> 00:54:45,960 Speaker 1: You know, I think I've seen that in the movie also, 1048 00:54:46,239 --> 00:54:48,719 Speaker 1: but it could be real, and if they shoot that 1049 00:54:48,800 --> 00:54:50,920 Speaker 1: laser in our direction, we might be able to see it. 1050 00:54:51,040 --> 00:54:54,280 Speaker 1: That is exactly the plot of these Star Wars trilogies. 1051 00:54:55,280 --> 00:54:58,239 Speaker 1: They literally suck a son into their gun and then 1052 00:54:58,280 --> 00:55:01,120 Speaker 1: shoot it at other planets. Not something we're recommending, but 1053 00:55:01,160 --> 00:55:03,479 Speaker 1: if it happens, we might be able to see it. Yeah, 1054 00:55:03,520 --> 00:55:06,480 Speaker 1: and you'll be there with your popcorn, gleefully looking at 1055 00:55:06,520 --> 00:55:10,839 Speaker 1: the extinction of thousands or billions of alien lives as 1056 00:55:10,880 --> 00:55:13,440 Speaker 1: they melt my eyeballs. All right, well, we hope they 1057 00:55:13,680 --> 00:55:16,399 Speaker 1: give you something to think about, and maybe think about 1058 00:55:16,440 --> 00:55:20,080 Speaker 1: the trajectory of our own civilization, Like do we want 1059 00:55:20,120 --> 00:55:23,640 Speaker 1: to be known to other alien species by our last moments? 1060 00:55:24,440 --> 00:55:27,440 Speaker 1: Or should we be working harder to work things out 1061 00:55:27,520 --> 00:55:30,000 Speaker 1: between us so that they see us for other reasons. 1062 00:55:30,200 --> 00:55:32,240 Speaker 1: Or maybe we should take all of our nuclear bombs 1063 00:55:32,239 --> 00:55:34,160 Speaker 1: and launch them into space and blow them up out 1064 00:55:34,200 --> 00:55:36,920 Speaker 1: there so aliens know we're here. You mean, like a 1065 00:55:36,960 --> 00:55:41,080 Speaker 1: dinner bell, Like ring a different dinner bell. No, like 1066 00:55:41,120 --> 00:55:45,680 Speaker 1: an invitation to a party, right, a dinner party? Sounds 1067 00:55:45,680 --> 00:55:47,560 Speaker 1: like maybe we should put that up for a vote 1068 00:55:47,760 --> 00:55:50,279 Speaker 1: before we do that. All right, Well, we hope you 1069 00:55:50,360 --> 00:55:52,920 Speaker 1: enjoyed that. Thanks for joining us, See you next time. 1070 00:56:00,880 --> 00:56:03,680 Speaker 1: Thanks for listening, and remember that Daniel and Jorge Explain 1071 00:56:03,760 --> 00:56:07,680 Speaker 1: the Universe is a production of iHeartRadio. For more podcasts 1072 00:56:07,800 --> 00:56:12,360 Speaker 1: from iHeartRadio, visit the iHeartRadio, app, Apple podcasts, or wherever 1073 00:56:12,480 --> 00:56:14,160 Speaker 1: you listen to your favorite shows.