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Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated: 1 00:00:01,234 --> 00:00:03,902 [narrator] Join us on Tomorrow's World Today 2 00:00:03,904 --> 00:00:06,438 as we journey through the worlds of inspiration, 3 00:00:06,440 --> 00:00:09,708 creation, innovation and production, 4 00:00:09,710 --> 00:00:12,277 to find the ideas and technologies 5 00:00:12,279 --> 00:00:14,213 that are shaping our future. 6 00:00:14,215 --> 00:00:17,449 In part two of this four-part exploration, 7 00:00:17,451 --> 00:00:21,787 George sends Greg to discover the history of nuclear energy, 8 00:00:21,789 --> 00:00:25,391 how nuclear energy is being used in today's world, 9 00:00:25,393 --> 00:00:29,128 and what tomorrow's nuclear reactors might look like. 10 00:00:38,972 --> 00:00:40,973 Hi, everyone. I'm Greg Constantino. 11 00:00:40,975 --> 00:00:43,375 Now, George has me on a very special assignment. 12 00:00:43,377 --> 00:00:46,245 I'm gonna be looking at the past, present and future 13 00:00:46,247 --> 00:00:47,346 of nuclear energy. 14 00:00:47,348 --> 00:00:49,148 Now, we're gonna start off 15 00:00:49,150 --> 00:00:52,251 by looking at the beginnings of nuclear research and the creation of fission. 16 00:00:52,253 --> 00:00:54,820 Next, we'll look at nuclear power today, 17 00:00:54,822 --> 00:00:57,322 and safety, a topic on a lot of people's minds. 18 00:00:57,324 --> 00:00:59,725 And lastly, we're going to leap into the future, 19 00:00:59,727 --> 00:01:02,728 look at some of the innovations happening with this amazing technology, 20 00:01:02,730 --> 00:01:05,998 and also get a look at the advanced reactors of tomorrow. 21 00:01:15,508 --> 00:01:20,045 Now, I can't think of any better way to start this off than by talking to Don Miley. 22 00:01:20,047 --> 00:01:22,448 Now, Don is a legend in the nuclear world, 23 00:01:22,450 --> 00:01:24,917 because of his encyclopedic knowledge of the industry. 24 00:01:24,919 --> 00:01:26,018 Let's go meet him now. 25 00:01:34,060 --> 00:01:34,893 Hey, Don. 26 00:01:34,895 --> 00:01:36,295 Greg, welcome to Idaho National Lab. 27 00:01:36,297 --> 00:01:37,896 [Greg] Thanks for having me. 28 00:01:37,898 --> 00:01:40,099 - I'm very excited to be here today. - We're excited to have you. 29 00:01:40,101 --> 00:01:42,134 So, Don, here we are at EBR-I, 30 00:01:42,136 --> 00:01:44,269 the EBR-I Museum, tell me about that. 31 00:01:44,271 --> 00:01:46,472 [Don] So, "Experimental Breeder Reactor One", 32 00:01:46,474 --> 00:01:48,040 this was the first reactor built 33 00:01:48,042 --> 00:01:50,109 at the National Reactor Testing Station. 34 00:01:50,111 --> 00:01:52,311 It was built by Argonne National Laboratory. 35 00:01:52,313 --> 00:01:55,314 First of 52 reactors built here in Idaho. 36 00:01:55,316 --> 00:01:57,883 And this was the first place in the world 37 00:01:57,885 --> 00:02:00,986 to make a useable amount of electricity from splitting atoms. 38 00:02:00,988 --> 00:02:03,288 And that's really what we're here to learn about today. 39 00:02:03,290 --> 00:02:04,723 Tell me about fission. 40 00:02:04,725 --> 00:02:06,258 So, fission, splitting atoms. 41 00:02:06,260 --> 00:02:08,427 That is exactly what nuclear reactors do. 42 00:02:08,429 --> 00:02:12,364 We use atoms of Uranium-235 that are naturally occurring in nature. 43 00:02:12,366 --> 00:02:14,700 We mine those like most other elements. 44 00:02:14,702 --> 00:02:17,569 And Uranium-235 has this wonderful ability 45 00:02:17,571 --> 00:02:19,671 that when struck by a neutron, 46 00:02:19,673 --> 00:02:22,174 it will split into two new atoms. 47 00:02:22,176 --> 00:02:25,477 And the energy that had bound that together as a cohesive atom, 48 00:02:25,479 --> 00:02:27,312 when you break that bond, 49 00:02:27,314 --> 00:02:30,082 a lot of that energy is released in the form of heat. 50 00:02:30,084 --> 00:02:31,850 And what makes this useful, 51 00:02:31,852 --> 00:02:35,220 is as that atom is splitting into two new atoms, 52 00:02:35,222 --> 00:02:36,989 two to three neutrons are released, 53 00:02:36,991 --> 00:02:40,225 which will go on to strike more atoms of Uranium-235, 54 00:02:40,227 --> 00:02:42,861 getting more heat for more neutrons and heat. 55 00:02:42,863 --> 00:02:45,430 So, that's the chain reaction we talk about. 56 00:02:45,432 --> 00:02:48,400 And we harness that heat to turn water into steam, 57 00:02:48,402 --> 00:02:50,536 steam turns a turbine, which turns a generator, 58 00:02:50,538 --> 00:02:52,504 just like a coal-fired power plant. 59 00:02:52,506 --> 00:02:54,139 But, we're not physically burning anything, 60 00:02:54,141 --> 00:02:55,307 we're splitting atoms. 61 00:02:55,309 --> 00:02:57,809 Right, which is keeping that carbon footprint small. 62 00:02:57,811 --> 00:02:59,578 Exactly what we wanna do, yeah. 63 00:02:59,580 --> 00:03:01,713 Great, well, I wanna find out everything about everything 64 00:03:01,715 --> 00:03:03,282 you do here, so how about a tour? 65 00:03:03,284 --> 00:03:05,083 Might as well, you're in the right place. 66 00:03:13,760 --> 00:03:16,328 [Don] Greg, here we are in the control room for EBR-I. 67 00:03:16,330 --> 00:03:19,965 When this was operating, one operator sat right here and ran the reactor. 68 00:03:19,967 --> 00:03:21,600 [Greg] Wow, that's amazing. 69 00:03:21,602 --> 00:03:23,502 Now, Don, explain to me, what's it mean when a reactor "goes critical"? 70 00:03:23,504 --> 00:03:26,605 "Critical" just means it's at full power and that's what we want. 71 00:03:26,607 --> 00:03:28,207 All right, well, let's take a look at a reactor. 72 00:03:28,209 --> 00:03:29,408 Let's go. 73 00:03:34,781 --> 00:03:37,816 So, Don, we're actually looking at the top of the reactor. 74 00:03:37,818 --> 00:03:41,353 [Don] Correct. That is the reactor head, the lid, if you will. 75 00:03:41,355 --> 00:03:43,355 Beneath that lid would be the fuel rods, 76 00:03:43,357 --> 00:03:45,324 which we have on the display here. 77 00:03:45,326 --> 00:03:47,259 Very small diameter, 10-foot long, 78 00:03:47,261 --> 00:03:51,129 only eight-and-a-half inches of Uranium-235 fuel. 79 00:03:51,131 --> 00:03:54,700 And that is something amazing about nuclear, is energy density. 80 00:03:54,702 --> 00:03:57,703 The core at eight-and-a-half inches tall, about that big around, 81 00:03:57,705 --> 00:03:58,837 generated a lot of heat. 82 00:03:58,839 --> 00:04:02,441 The primary coolant entered at 440 degrees Fahrenheit, 83 00:04:02,443 --> 00:04:05,844 flowed up the rods and out these holes at 600 degrees, 84 00:04:05,846 --> 00:04:07,379 at 300 gallons a minute. 85 00:04:07,381 --> 00:04:09,715 And that's how we get to the point where this reactor 86 00:04:09,717 --> 00:04:12,084 generated the first and usable electricity. 87 00:04:12,086 --> 00:04:13,318 That is right. 88 00:04:13,320 --> 00:04:15,187 - Why don't we go look at the turbine? - Okay. 89 00:04:15,189 --> 00:04:16,421 [Don] Let's go. 90 00:04:22,228 --> 00:04:25,264 So, Don, is this the actual turbine 91 00:04:25,266 --> 00:04:27,933 that generated the electricity from EBR-I? 92 00:04:27,935 --> 00:04:30,035 Yes, it is. This turbine is what they were 93 00:04:30,037 --> 00:04:31,937 spinning with the steam which turned the generator. 94 00:04:31,939 --> 00:04:36,308 They made electricity, lighting four light bulbs on December 20th, 1951. 95 00:04:36,310 --> 00:04:39,344 [Greg] Now, I know you had bigger goals that just lighting up a few light bulbs. 96 00:04:39,346 --> 00:04:41,880 Is this also the generator that lit up the town of Arco? 97 00:04:41,882 --> 00:04:43,682 [Don] It is not, actually. 98 00:04:43,684 --> 00:04:47,085 That was at a reactor about a half-mile away from here that was called BORAX-III. 99 00:04:47,087 --> 00:04:51,556 Okay, now I know that EBR-I led you down the road to learn a lot of new safety protocols. 100 00:04:51,558 --> 00:04:53,859 And I'm very interested in that, so can we take a look? 101 00:04:53,861 --> 00:04:55,127 Let's go take a look. 102 00:05:00,133 --> 00:05:01,733 Greg, here we have a replica of what 103 00:05:01,735 --> 00:05:04,803 the Experimental Breeder Reactor-II control room looked like. 104 00:05:04,805 --> 00:05:06,471 So, this is where you put all of the safety things that 105 00:05:06,473 --> 00:05:08,740 you learned doing EBR-I into practice. 106 00:05:08,742 --> 00:05:10,242 That's right, let me show you how. 107 00:05:12,245 --> 00:05:14,546 Greg, this is probably the best way to show 108 00:05:14,548 --> 00:05:18,283 the importance of the safety of EBR-II and how they achieved it. 109 00:05:18,285 --> 00:05:22,854 The reactor itself sat in a tank of 86,000 gallons of sodium coolant. 110 00:05:22,856 --> 00:05:26,892 Argonne, in 1986 ran an experiment with EBR-II, 111 00:05:26,894 --> 00:05:29,361 in which they had the reactor at full power, 112 00:05:29,363 --> 00:05:31,196 they disabled all safety systems, 113 00:05:31,198 --> 00:05:32,931 automatic safety systems, 114 00:05:32,933 --> 00:05:35,067 and they turned their primary pumps off. 115 00:05:35,069 --> 00:05:38,470 Nobody in the world thought that was a great idea with the reactor. 116 00:05:38,472 --> 00:05:40,238 In this case, what happened was, 117 00:05:40,240 --> 00:05:42,708 without the coolant flowing, the static coolant, 118 00:05:42,710 --> 00:05:44,276 the temperature began to rise. 119 00:05:44,278 --> 00:05:46,078 So, that rose to the surface, 120 00:05:46,080 --> 00:05:48,880 dissipated the heat and fell to the bottom again. 121 00:05:48,882 --> 00:05:50,816 Convection currents formed. 122 00:05:50,818 --> 00:05:53,185 And at the same time, the fuel in EBR-II 123 00:05:53,187 --> 00:05:55,854 is a little different than our powerplants today. 124 00:05:55,856 --> 00:05:57,322 This was metallic uranium, 125 00:05:57,324 --> 00:06:00,926 instead of uranium oxide that the light water reactors use. 126 00:06:00,928 --> 00:06:03,729 Metallic fuel will begin to expand 127 00:06:03,731 --> 00:06:05,731 and neutrons leak out of the core 128 00:06:05,733 --> 00:06:07,232 and it shuts itself down. 129 00:06:07,234 --> 00:06:09,868 It is inherently safe in this design. 130 00:06:09,870 --> 00:06:10,969 Well, Don, thank you very much. 131 00:06:10,971 --> 00:06:12,170 - This has been excellent. - Thank you. 132 00:06:12,172 --> 00:06:14,272 I'm heading out to Oak Ridge National Labs now. 133 00:06:14,274 --> 00:06:16,241 - Say hi to my friends there. - Will do. 134 00:06:38,164 --> 00:06:40,499 Now, that we've learned about the history of nuclear energy, 135 00:06:40,501 --> 00:06:42,167 I'd like to dive a little bit more deeply 136 00:06:42,169 --> 00:06:44,202 into the safety of this technology. 137 00:06:44,204 --> 00:06:45,904 I'm gonna meet with Dr. Rita Baranwal. 138 00:06:45,906 --> 00:06:48,039 She's with the Electric Power Research Institute. 139 00:06:48,041 --> 00:06:49,441 And we're gonna talk about safety 140 00:06:49,443 --> 00:06:53,111 and also about nuclear power's contribution to today's energy mix. 141 00:06:59,852 --> 00:07:01,420 - Hi, Rita. - Hi, Greg. 142 00:07:01,422 --> 00:07:04,122 So, Rita, we've learned that nuclear energy 143 00:07:04,124 --> 00:07:06,958 is going to be a major part of the clean energy mix, 144 00:07:06,960 --> 00:07:09,094 for the entire world, moving forward. 145 00:07:09,096 --> 00:07:10,929 But, people do have concerns 146 00:07:10,931 --> 00:07:12,464 and they're generally about safety. 147 00:07:12,466 --> 00:07:13,432 Is it safe? 148 00:07:13,434 --> 00:07:15,066 It's absolutely safe. 149 00:07:15,068 --> 00:07:17,302 But, let me talk about the energy mix for a moment. 150 00:07:17,304 --> 00:07:19,538 Moving forward, the clean energy mix, 151 00:07:19,540 --> 00:07:21,206 studies have shown, are gonna be 152 00:07:21,208 --> 00:07:23,408 about 80% renewables. 153 00:07:23,410 --> 00:07:27,145 The remaining 20% really needs to come from nuclear. 154 00:07:27,147 --> 00:07:30,182 Nuclear powerplants follow the strictest 155 00:07:30,184 --> 00:07:32,317 and highest standard of safety, 156 00:07:32,319 --> 00:07:36,822 security, cyber-security, and emergency preparedness. 157 00:07:36,824 --> 00:07:39,925 And nuclear powerplants are designed such that 158 00:07:39,927 --> 00:07:41,993 they operate as remote islands. 159 00:07:41,995 --> 00:07:44,429 And, so they are protected from cyber-threats. 160 00:07:44,431 --> 00:07:47,933 All right, well, there's a thing called value proposition, 161 00:07:47,935 --> 00:07:49,134 as regards to nuclear energy, 162 00:07:49,136 --> 00:07:51,036 and I want to find out a little bit more about that. 163 00:07:53,239 --> 00:07:56,875 So, Rita, when we talk about the value proposition of nuclear energy, 164 00:07:56,877 --> 00:07:59,511 what we're really talking about is the carbon footprint. 165 00:07:59,513 --> 00:08:03,281 Nuclear has always been a clean energy source. 166 00:08:03,283 --> 00:08:06,384 It's really important in a clean energy mix 167 00:08:06,386 --> 00:08:08,386 when we talk about de-carbonization. 168 00:08:08,388 --> 00:08:11,156 For example, in 2019, 169 00:08:11,158 --> 00:08:16,094 nuclear energy avoided 476 million metric tons of CO2 emissions. 170 00:08:16,096 --> 00:08:17,529 What that really equates to, 171 00:08:17,531 --> 00:08:21,132 is the equivalent of taking 100 million cars off the road. 172 00:08:21,134 --> 00:08:22,501 Wow. 173 00:08:22,503 --> 00:08:25,103 Now, in terms of an actual footprint, 174 00:08:25,105 --> 00:08:28,373 a 1,000-megawatt nuclear powerplant 175 00:08:28,375 --> 00:08:32,143 will require about one square mile of land area. 176 00:08:32,145 --> 00:08:36,381 Compare that to a windmill farm of an equivalent output, 177 00:08:36,383 --> 00:08:39,818 that'll require about 360 times the landmass. 178 00:08:39,820 --> 00:08:43,421 And a similar sized output from a solar photovoltaic plant, 179 00:08:43,423 --> 00:08:46,558 is going to require about 75 times the landmass. 180 00:08:46,560 --> 00:08:50,328 While it's very important that we have all of those clean energy sources 181 00:08:50,330 --> 00:08:53,131 in a clean energy portfolio going forward, 182 00:08:53,133 --> 00:08:56,134 nuclear powerplants require the smallest actual footprint. 183 00:08:56,136 --> 00:08:58,403 Right, and in terms of reliability as well. 184 00:08:58,405 --> 00:09:01,206 I mean, wind and solar, they are great and amazing 185 00:09:01,208 --> 00:09:02,340 and they're going to be a big part of this. 186 00:09:02,342 --> 00:09:03,875 But, they are weather-dependent. 187 00:09:03,877 --> 00:09:07,579 Absolutely, and nuclear energy and nuclear power 188 00:09:07,581 --> 00:09:13,351 are a 24/7, 365 available energy source for electricity. 189 00:09:13,353 --> 00:09:16,221 And given our unfortunate climate events 190 00:09:16,223 --> 00:09:18,790 that we're seeing around the globe recently, 191 00:09:18,792 --> 00:09:21,927 it's really important to have nuclear energy as part of that mix, 192 00:09:21,929 --> 00:09:24,996 so that you do have reliable and resilient power. 193 00:09:24,998 --> 00:09:26,364 And that's a part of the key, too, 194 00:09:26,366 --> 00:09:28,967 in what we're learning about energy poverty 195 00:09:28,969 --> 00:09:31,036 and getting power to places that, 196 00:09:31,038 --> 00:09:32,203 either have no electricity, 197 00:09:32,205 --> 00:09:35,173 or have very unreliable electricity. 198 00:09:35,175 --> 00:09:38,443 And I talked about those larger 1000-megwatt plants. 199 00:09:38,445 --> 00:09:41,112 The exciting part of this industry is that 200 00:09:41,114 --> 00:09:44,082 we're innovating and developing smaller reactors. 201 00:09:44,084 --> 00:09:45,250 Including micro-reactors 202 00:09:45,252 --> 00:09:47,819 which are 10 to 20 megawatts in size. 203 00:09:47,821 --> 00:09:51,256 And small modular reactors which are up to 300 megawatts in size. 204 00:09:51,258 --> 00:09:54,926 Those can be deployed more rapidly to communities 205 00:09:54,928 --> 00:09:57,429 that either have no electricity, as you mentioned, 206 00:09:57,431 --> 00:10:01,032 or don't have reliable electricity much faster 207 00:10:01,034 --> 00:10:04,903 than a larger 1,000-megawatt scale plant could be deployed. 208 00:10:04,905 --> 00:10:07,105 So, this is a great way to get remote locations 209 00:10:07,107 --> 00:10:09,207 - clean and reliable power. - Exactly. 210 00:10:13,112 --> 00:10:15,280 So, Rita, when it comes to nuclear energy, 211 00:10:15,282 --> 00:10:18,850 one of the main things that people are concerned about is nuclear waste. 212 00:10:18,852 --> 00:10:21,820 So, tell me, what is it, and how are we handling it? 213 00:10:21,822 --> 00:10:25,757 Nuclear waste, or used nuclear fuel from a commercial powerplant, 214 00:10:25,759 --> 00:10:28,293 actually goes into the reactor as a solid 215 00:10:28,295 --> 00:10:30,762 and it also comes out of the reactor as a solid. 216 00:10:30,764 --> 00:10:33,598 After that, there's two different paths that can be pursued. 217 00:10:33,600 --> 00:10:37,402 One is, to prepare that used fuel for permanent storage. 218 00:10:37,404 --> 00:10:41,106 And the other, is to recycle that used fuel for reuse. 219 00:10:41,108 --> 00:10:43,875 And what's really exciting about advanced reactor designs 220 00:10:43,877 --> 00:10:45,443 is that some of those concepts 221 00:10:45,445 --> 00:10:48,413 are planning to use used fuel in their designs, 222 00:10:48,415 --> 00:10:51,282 thereby reducing the amount of used fuel that's really out there. 223 00:10:51,284 --> 00:10:54,052 That's great, but, now, when we talk about that permeant storage, 224 00:10:54,054 --> 00:10:55,787 how much are we talking about? 225 00:10:55,789 --> 00:10:59,891 Well, for example, in the United States since the 1950s, 226 00:10:59,893 --> 00:11:02,327 the amount of used fuel that's been generated 227 00:11:02,329 --> 00:11:08,066 is only enough to cover a American football field, 10-yards deep. 228 00:11:08,068 --> 00:11:09,467 That's amazing. Rita, this has been great. 229 00:11:09,469 --> 00:11:10,969 Thanks for all the great information. 230 00:11:10,971 --> 00:11:13,104 I'm heading over to Oak Ridge National Laboratory. 231 00:11:13,106 --> 00:11:14,706 I'm gonna meet with Kathy McCarthy. 232 00:11:43,569 --> 00:11:45,770 [Kathy] We're standing at Oak Ridge National Laboratory 233 00:11:45,772 --> 00:11:47,338 in the visitors' center 234 00:11:47,406 --> 00:11:50,208 and actually in front of a mural that has highlights of all sorts of 235 00:11:50,210 --> 00:11:52,277 amazing things that have happened here. 236 00:11:52,279 --> 00:11:54,746 Oak Ridge National Laboratory has both 237 00:11:54,748 --> 00:11:57,949 the facilities and the expertise 238 00:11:57,951 --> 00:11:59,384 to solve some of the hardest problems 239 00:11:59,386 --> 00:12:01,219 that are facing humankind. 240 00:12:01,221 --> 00:12:03,922 Oak Ridge has a long history 241 00:12:03,924 --> 00:12:06,958 in nuclear science and technology and reactors, specifically, 242 00:12:06,960 --> 00:12:09,360 over seven decades of experience. 243 00:12:09,362 --> 00:12:11,129 In the work that we're doing currently, 244 00:12:11,131 --> 00:12:14,966 we're supporting both, the current fleet of nuclear reactors. 245 00:12:14,968 --> 00:12:18,903 They provide over half of the carbon-free electricity generation 246 00:12:18,905 --> 00:12:20,138 in the United States. 247 00:12:20,140 --> 00:12:22,941 Bu we're also supporting advanced nuclear reactors. 248 00:12:22,943 --> 00:12:24,876 The US ITER project office 249 00:12:24,878 --> 00:12:27,545 is located here at Oak Ridge National Laboratory. 250 00:12:27,547 --> 00:12:31,316 ITER's an experiment that's being built in southern France 251 00:12:31,318 --> 00:12:34,486 to demonstrate sustainable fusion energy. 252 00:12:34,488 --> 00:12:37,489 A step towards practical fusion energy. 253 00:12:42,928 --> 00:12:44,562 - Hi, Kathy. - Hey, Greg. 254 00:12:44,564 --> 00:12:46,798 Now, Kathy, Oak Ridge National Laboratory 255 00:12:46,800 --> 00:12:50,368 has over seven decades of experience in the nuclear power industry. 256 00:12:50,370 --> 00:12:52,737 That's a lot of history, but as I look around this room, 257 00:12:52,739 --> 00:12:55,206 I feel like I see the future of nuclear energy. 258 00:12:55,208 --> 00:12:56,241 That's exactly right. 259 00:12:56,243 --> 00:12:58,009 What you see here is an example 260 00:12:58,011 --> 00:13:00,445 of the kind of modelling and simulation that we can do. 261 00:13:00,447 --> 00:13:02,981 We can do that because we have very powerful computers, 262 00:13:02,983 --> 00:13:05,817 and we also understand the nuclear science and technology 263 00:13:05,819 --> 00:13:08,353 that goes into the models that we're developing. 264 00:13:08,355 --> 00:13:10,989 These models can be used in a lot of different ways. 265 00:13:10,991 --> 00:13:13,958 One of the applications is we can use these models 266 00:13:13,960 --> 00:13:18,062 to look at if we make changes to a design, for example, 267 00:13:18,064 --> 00:13:19,731 what kind of benefit does that have on the economics? 268 00:13:19,733 --> 00:13:20,832 And that's an important part. 269 00:13:20,834 --> 00:13:23,001 Right, and I guess that would also play into 270 00:13:23,003 --> 00:13:24,903 keeping the current nuclear fleet 271 00:13:24,905 --> 00:13:27,705 operating past its initial life expectancy. 272 00:13:27,707 --> 00:13:28,740 Tell me about that. 273 00:13:28,742 --> 00:13:30,441 So, the original licensing period 274 00:13:30,443 --> 00:13:32,477 for nuclear reactors is 40 years. 275 00:13:32,479 --> 00:13:35,213 That was based on the Atomic Energy Act, 276 00:13:35,215 --> 00:13:38,183 on antitrust and depreciation laws. 277 00:13:38,185 --> 00:13:40,885 No, it was not a connection to the technical length 278 00:13:40,887 --> 00:13:42,754 of time that a reactor could operate. 279 00:13:42,756 --> 00:13:44,189 So, there's the 40 years, 280 00:13:44,191 --> 00:13:46,991 and there's also a process for 20-year extensions to that 40 years. 281 00:13:46,993 --> 00:13:48,393 So, for each of those extensions, 282 00:13:48,395 --> 00:13:50,528 the owner-operator needs to show that they can 283 00:13:50,530 --> 00:13:53,865 operate safely through these extended licensing periods. 284 00:13:53,867 --> 00:13:57,135 So, this was an economic concern, not a safety concern. 285 00:13:57,137 --> 00:13:58,169 Yeah, that's true. 286 00:13:58,171 --> 00:13:59,704 Because what the plants need to demonstrate 287 00:13:59,706 --> 00:14:01,306 is that it'll continue to operate safely. 288 00:14:01,308 --> 00:14:03,274 And that may require investments 289 00:14:03,276 --> 00:14:06,211 in replacing components, in repairing components, 290 00:14:06,213 --> 00:14:08,112 and so, in the end, it's that economic decision. 291 00:14:08,114 --> 00:14:12,150 And as more technical innovations are made in reactor construction, 292 00:14:12,152 --> 00:14:14,986 there might come a point of diminishing returns on that upgrade? 293 00:14:14,988 --> 00:14:15,787 That's absolutely right, 294 00:14:15,789 --> 00:14:17,255 and the other piece of that is, 295 00:14:17,257 --> 00:14:19,524 with some of the advanced reactors under development, 296 00:14:19,526 --> 00:14:22,227 you can use them in a broader range of applications. 297 00:14:22,229 --> 00:14:23,795 So, for example, 298 00:14:23,797 --> 00:14:28,333 in some of the reactors they have a hotter outlet temperature. 299 00:14:28,335 --> 00:14:31,536 That means you can apply it into different things, like, for example, 300 00:14:31,538 --> 00:14:32,904 in the chemical industry, 301 00:14:32,906 --> 00:14:34,505 where currently they use natural gas 302 00:14:34,507 --> 00:14:36,040 that produces greenhouse gases. 303 00:14:36,042 --> 00:14:37,909 If they want to reduce their carbon footprint, 304 00:14:37,911 --> 00:14:39,477 nuclear's a potential option. 305 00:14:39,479 --> 00:14:41,446 These reactors, some of them, 306 00:14:41,448 --> 00:14:43,248 give you this higher outlet temperature, 307 00:14:43,250 --> 00:14:44,816 which allows these other applications. 308 00:14:44,818 --> 00:14:46,851 Right, well, the chemistry thing kind of brings us 309 00:14:46,853 --> 00:14:50,021 to my next question which is fission versus fusion. 310 00:14:50,023 --> 00:14:52,857 So, fission and fusion, they're both nuclear reactions. 311 00:14:52,859 --> 00:14:55,526 They involve the nucleus of the atoms. 312 00:14:55,528 --> 00:14:57,262 So, if you think about your periodic table, 313 00:14:57,264 --> 00:14:59,130 and you've got the lighter ones up at the top, 314 00:14:59,132 --> 00:15:00,665 down to the heavier ones. 315 00:15:00,966 --> 00:15:04,569 The heavier ones, fission, you're actually breaking apart these heavy atoms, 316 00:15:04,571 --> 00:15:06,638 that produces energy, 317 00:15:06,640 --> 00:15:09,073 what we call fission products, which are radioactive, 318 00:15:09,241 --> 00:15:10,842 and neutrons. 319 00:15:10,844 --> 00:15:13,945 In fusion, you're putting together lighter atoms. 320 00:15:13,947 --> 00:15:15,780 And, so, hydrogen isotopes, for example, 321 00:15:15,782 --> 00:15:18,983 you get energy, helium and neutrons. 322 00:15:18,985 --> 00:15:22,153 So, the difference really is the radioactivity of the fission products. 323 00:15:22,155 --> 00:15:23,888 Okay, and that leads us to 324 00:15:23,890 --> 00:15:26,824 one of the most exciting developments in nuclear energy today. 325 00:15:26,826 --> 00:15:27,792 It's called ITER. 326 00:15:27,794 --> 00:15:29,360 I know that you have an ITER pellet lab 327 00:15:29,362 --> 00:15:31,129 here on site, and I'd really like to see it. 328 00:15:31,131 --> 00:15:32,597 Great, I'd be happy to show it to you. 329 00:16:01,093 --> 00:16:04,262 So, Kathy, this is the pellet smashing injector, 330 00:16:04,264 --> 00:16:07,231 which is by far my favorite name for a high-tech piece of scientific gear. 331 00:16:07,233 --> 00:16:09,767 And this is part of the safety protocol for ITER, 332 00:16:09,769 --> 00:16:11,369 we'll get into that in just a minute. 333 00:16:11,371 --> 00:16:14,305 But first, tell me what can we expect from ITER. 334 00:16:14,307 --> 00:16:17,041 So, ITER, which means "the way" in Latin, 335 00:16:17,043 --> 00:16:19,744 was designed, and now is being assembled 336 00:16:19,746 --> 00:16:22,246 first and foremost, so that we can understand 337 00:16:22,248 --> 00:16:24,882 the physics behind a self-sustained plasma, 338 00:16:24,884 --> 00:16:26,250 what we call a burning plasma. 339 00:16:26,252 --> 00:16:28,252 So, you heat that plasma up, 340 00:16:28,254 --> 00:16:30,822 but then you don't to have to keep having external heating. 341 00:16:30,824 --> 00:16:32,390 You want it to be self-sustaining. 342 00:16:32,392 --> 00:16:35,393 Okay, so, I know that plasma's really hot, 343 00:16:35,395 --> 00:16:36,828 and this is meant to cool it down. 344 00:16:36,830 --> 00:16:38,296 So, explain to me how this works. 345 00:16:38,298 --> 00:16:40,331 [Kathy] So, the shattered pellet injector 346 00:16:40,333 --> 00:16:45,636 actually is used to dissipate the heat from the plasma. 347 00:16:45,638 --> 00:16:48,006 So, ITER is, first and foremost, an experiment. 348 00:16:48,008 --> 00:16:49,173 And in an experiment, 349 00:16:49,175 --> 00:16:51,275 you have to be prepared for things 350 00:16:51,277 --> 00:16:53,311 not operating quite the way that they'll need to 351 00:16:53,313 --> 00:16:55,446 ultimately in a commercial plant. 352 00:16:55,448 --> 00:16:58,249 This is actually what the fuel pellet looks like, 353 00:16:58,251 --> 00:17:00,151 in terms of size and shape. 354 00:17:00,153 --> 00:17:01,919 And the way that this test stand works... 355 00:17:01,921 --> 00:17:04,255 And this will be similar to how it works in ITER. 356 00:17:04,757 --> 00:17:06,391 We form the pellets here. 357 00:17:06,393 --> 00:17:09,961 And the way we do that is, we've got liquid helium. 358 00:17:09,963 --> 00:17:12,063 So, about four degrees kelvin, 359 00:17:12,065 --> 00:17:14,365 which is minus 269 degrees centigrade. 360 00:17:14,367 --> 00:17:17,068 And we use a process called de-sublimation. 361 00:17:17,070 --> 00:17:20,405 So, we're basically turning a gas into a solid. 362 00:17:20,407 --> 00:17:21,372 Very, very cold. 363 00:17:21,374 --> 00:17:23,174 - You can think about freezing. - Mmm-hmm. 364 00:17:23,176 --> 00:17:25,309 That's done in this section right here. 365 00:17:25,311 --> 00:17:28,579 Now, in ITER, those pellets will be there in the system 366 00:17:28,581 --> 00:17:30,915 - already ready to go. - Okay. 367 00:17:30,917 --> 00:17:33,317 We use gas to push the pellet 368 00:17:33,519 --> 00:17:36,220 into this section. 369 00:17:36,222 --> 00:17:39,057 And we've got all of this instrumented with cameras. 370 00:17:39,059 --> 00:17:40,324 So that we'll be able to see what happens, 371 00:17:40,326 --> 00:17:44,295 because how this pellet shatters is key to the experiment. 372 00:17:45,297 --> 00:17:48,066 In this section here and this section here, 373 00:17:48,068 --> 00:17:49,400 we're pulling the gas off 374 00:17:49,402 --> 00:17:52,036 that you used to push the pellet through. 375 00:17:52,038 --> 00:17:54,505 Because, all you want to go into the plasma 376 00:17:54,507 --> 00:17:55,840 is the pellet itself. 377 00:17:55,842 --> 00:17:57,542 Because, the gas will actually 378 00:17:57,544 --> 00:17:59,744 cause us to lose confinement of the plasma. 379 00:17:59,746 --> 00:18:00,945 And we don't wanna do that. 380 00:18:00,947 --> 00:18:03,181 Then, the pellet comes into this section. 381 00:18:03,183 --> 00:18:07,952 And this is what simulates the tokamak, inside of the tokamak. 382 00:18:07,954 --> 00:18:09,353 - [Greg] Okay. - [Kathy] And then, we want to understand again 383 00:18:09,355 --> 00:18:11,389 how this pellet shatters. 384 00:18:11,391 --> 00:18:14,425 So that we can make sure that it will uniformly dissipate the heat. 385 00:18:14,427 --> 00:18:17,028 And, I guess that's the same, sort of, theory 386 00:18:17,030 --> 00:18:19,030 as take a hot cup of tea and you drop an ice cube in it. 387 00:18:19,032 --> 00:18:20,298 It'll cool it down, but it takes a while. 388 00:18:20,300 --> 00:18:22,233 But, if you dumped a bunch of crushed ice into it, 389 00:18:22,235 --> 00:18:24,102 it cools it down much more quickly. 390 00:18:24,104 --> 00:18:25,937 That's right, and it's not just the much more quickly, 391 00:18:25,939 --> 00:18:28,206 it's also the uniformity of cooling, 392 00:18:28,208 --> 00:18:30,441 it's much better when you've got those different pieces. 393 00:18:30,443 --> 00:18:34,212 [Greg] Okay, now, I know that just one of these injectors is not gonna be enough 394 00:18:34,214 --> 00:18:36,180 to cool down that kind of a reaction. 395 00:18:36,182 --> 00:18:37,782 How many of these injectors will be 396 00:18:37,784 --> 00:18:39,083 positioned around the tokamak? 397 00:18:39,085 --> 00:18:42,019 So, ITER will have 27 shattered pellet injectors. 398 00:18:42,021 --> 00:18:44,722 24 of them around the circumference, 399 00:18:44,724 --> 00:18:47,358 and then three from up on top. 400 00:18:47,360 --> 00:18:50,795 And exactly how will the cooling action take place? 401 00:18:50,797 --> 00:18:54,065 So, what happens is these shattered pellet injectors 402 00:18:54,067 --> 00:18:56,734 will fire, basically, simultaneously. 403 00:18:56,736 --> 00:18:59,337 They'll fire their pellets into the very hot plasma. 404 00:18:59,339 --> 00:19:01,839 And how do you make sure that they all fire off at the same time? 405 00:19:01,841 --> 00:19:05,076 [Kathy] So, we can do that via sending an electronic signal. 406 00:19:05,078 --> 00:19:09,480 And the reason why we need to have it happen, basically simultaneously, 407 00:19:09,482 --> 00:19:11,449 is the plasma will cool very, very quickly. 408 00:19:11,451 --> 00:19:13,017 We're talking on the order of milliseconds. 409 00:19:13,019 --> 00:19:14,552 [Greg] Wow. 410 00:19:14,554 --> 00:19:16,587 [Kathy] And you don't want one side to cool before the other side. 411 00:19:16,589 --> 00:19:18,356 You want to uniformly dissipate the heat 412 00:19:18,358 --> 00:19:19,357 and it will dissipate quickly. 413 00:19:19,359 --> 00:19:21,125 Okay, so, we're going from 414 00:19:21,127 --> 00:19:22,727 really high temperatures to really low temperatures. 415 00:19:22,729 --> 00:19:25,129 What kind of temperatures are we actually talking about? 416 00:19:25,131 --> 00:19:27,465 So, think about the temperature of the center of the sun, 417 00:19:27,467 --> 00:19:29,634 which is 15 million degrees centigrade. 418 00:19:29,636 --> 00:19:32,503 The plasma is actually ten times hotter than that. 419 00:19:32,505 --> 00:19:34,172 That's a 150 million degrees. 420 00:19:34,174 --> 00:19:35,473 How do you even know you can do that? 421 00:19:35,475 --> 00:19:37,542 It's been done in laboratories already. 422 00:19:37,544 --> 00:19:40,411 Our challenge here is to do it for longer periods of time. 423 00:19:40,413 --> 00:19:41,946 That's one of the big challenges. 424 00:19:41,948 --> 00:19:43,614 Okay, now, when ITER goes online, 425 00:19:43,616 --> 00:19:47,318 which is around the mid-2020s, around 2025, 426 00:19:47,320 --> 00:19:49,520 what can we expect? 427 00:19:49,522 --> 00:19:52,423 So, in the mid-2020s, in what's called "first plasma", 428 00:19:52,425 --> 00:19:55,993 that's where we'll demonstrate an integrated operation of these major systems. 429 00:19:55,995 --> 00:19:58,196 We've got super-conducting magnets. 430 00:19:58,198 --> 00:20:01,098 We've got the system that keeps the super-conducting magnets cold. 431 00:20:01,100 --> 00:20:03,234 We have this large vacuum vessel. 432 00:20:03,236 --> 00:20:04,969 All of this at plant scale. 433 00:20:04,971 --> 00:20:06,904 So, first demonstrating that those systems 434 00:20:06,906 --> 00:20:09,941 all work in an integrated sense. 435 00:20:09,943 --> 00:20:13,377 Then, we move towards full deuterium, tritium operations. 436 00:20:13,379 --> 00:20:17,481 This is the fueled portion of the ITER operations. 437 00:20:17,916 --> 00:20:19,050 And at that point, 438 00:20:19,052 --> 00:20:21,152 that's when we'll be able to demonstrate 439 00:20:21,154 --> 00:20:23,955 a self-sustained plasma, or a burning plasma. 440 00:20:23,957 --> 00:20:26,624 And that would be in the mid-2030s. 441 00:20:26,626 --> 00:20:28,593 Well, Kathy, this is super exciting stuff 442 00:20:28,595 --> 00:20:30,061 that we'll be sure to keep an eye on. 443 00:20:30,063 --> 00:20:31,095 Thank you very much. 444 00:20:31,097 --> 00:20:33,264 And thank all of you for being with us 445 00:20:33,266 --> 00:20:35,733 for a continuing exploration of nuclear energy. 446 00:20:35,735 --> 00:20:37,101 Now, in our next episode, 447 00:20:37,103 --> 00:20:39,737 we're gonna look at more of this amazing technology 448 00:20:39,739 --> 00:20:41,606 and its role in tomorrow's world. 449 00:20:41,608 --> 00:20:43,074 For Tomorrow's World Today, 450 00:20:43,076 --> 00:20:44,208 I'm Greg Constantino. 37972

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