1 00:00:00,280 --> 00:00:02,880 Speaker 1: The information provided in this program is of a general nature. 2 00:00:02,920 --> 00:00:05,480 Speaker 1: It is not intended to be personalized financial advice. We 3 00:00:05,559 --> 00:00:08,240 Speaker 1: encourage you to seek appropriate advice from a qualified professional 4 00:00:08,320 --> 00:00:11,319 Speaker 1: to suit your individual circumstances. It's in the sun and 5 00:00:11,400 --> 00:00:14,239 Speaker 1: it's in the stars. Now a number of startups are 6 00:00:14,280 --> 00:00:18,520 Speaker 1: trying to create nuclear fusion here on Earth. This episode 7 00:00:18,560 --> 00:00:21,639 Speaker 1: takes you behind one of the companies edging closer to 8 00:00:21,840 --> 00:00:22,800 Speaker 1: abundant energy. 9 00:00:23,200 --> 00:00:25,320 Speaker 2: This is like humans discovering fire again. 10 00:00:25,760 --> 00:00:27,640 Speaker 3: That is effectively energy. You Toldia right. 11 00:00:27,720 --> 00:00:30,800 Speaker 1: It is clean, abundant, affordable. 12 00:00:31,040 --> 00:00:35,000 Speaker 4: Energy, and that will unlock huge business applications, but also 13 00:00:35,280 --> 00:00:39,800 Speaker 4: really good societal outcomes. Families won't worry about continuing to 14 00:00:39,840 --> 00:00:55,400 Speaker 4: pay the power bill to keep their houses warm. 15 00:00:56,000 --> 00:00:58,320 Speaker 1: We could be on the cusp of a breakthrough in 16 00:00:58,440 --> 00:01:03,280 Speaker 1: nuclear energy, with billions being spent on achieving fusion or 17 00:01:03,440 --> 00:01:08,479 Speaker 1: reviving fission. Amazon, Microsoft and Google have all made commitments 18 00:01:08,560 --> 00:01:11,600 Speaker 1: to nuclear as a source to power their data centers 19 00:01:11,640 --> 00:01:15,240 Speaker 1: ahead of an AI boom. Even open Ayes sam Oltman 20 00:01:15,480 --> 00:01:19,360 Speaker 1: is involved. Around seven billion US dollars has been invested 21 00:01:19,440 --> 00:01:23,600 Speaker 1: into companies trying to commercialize fusion, with most of them 22 00:01:23,680 --> 00:01:26,839 Speaker 1: targeting a date in the twenty thirties to start adding 23 00:01:26,959 --> 00:01:31,080 Speaker 1: nuclear energy to the grid. According to the Fusion Industry Association, 24 00:01:31,920 --> 00:01:34,280 Speaker 1: most of them are in the USA, but there is 25 00:01:34,319 --> 00:01:37,760 Speaker 1: an effort underway in a small corner of the world. 26 00:01:38,400 --> 00:01:41,840 Speaker 1: This blitting of atoms nuclear fission was done for the 27 00:01:41,880 --> 00:01:45,640 Speaker 1: first time by a New Zealander, Ernest Rutherford. Could this 28 00:01:45,720 --> 00:01:48,600 Speaker 1: company in the same country be the first in the 29 00:01:48,640 --> 00:01:50,480 Speaker 1: world to fuse atoms? 30 00:01:50,640 --> 00:01:51,720 Speaker 3: Hey, Ratu, how are you? 31 00:01:51,840 --> 00:01:53,800 Speaker 2: Aye Madison, nice to meet here. 32 00:01:54,400 --> 00:01:55,440 Speaker 3: Thank you so much for having us. 33 00:01:55,560 --> 00:01:56,360 Speaker 2: Absolute pleasure. 34 00:01:56,640 --> 00:01:57,560 Speaker 3: This is the experiment. 35 00:01:57,760 --> 00:01:59,800 Speaker 4: Yeah, no, this is where it all happens. It's pleasure 36 00:01:59,800 --> 00:02:01,080 Speaker 4: to have here. We're going to be able to show 37 00:02:01,080 --> 00:02:02,000 Speaker 4: you lots of ritical stuff. 38 00:02:02,040 --> 00:02:03,480 Speaker 3: I can't wait. One of the coolest things to come 39 00:02:03,480 --> 00:02:04,560 Speaker 3: out of Wellington. 40 00:02:04,760 --> 00:02:06,520 Speaker 2: In New Zealand the world. 41 00:02:07,040 --> 00:02:10,320 Speaker 3: This is Open Star Technologies, a startup. 42 00:02:09,919 --> 00:02:14,040 Speaker 1: Developing a nuclear fusion reactor in Wellington's Hills. It was 43 00:02:14,080 --> 00:02:17,520 Speaker 1: founded by Ratuma Tider and his university flat. In the 44 00:02:17,520 --> 00:02:20,800 Speaker 1: past two years it's raised twelve million at US dollars 45 00:02:21,160 --> 00:02:24,880 Speaker 1: and just had a major milestone heading plasma for the 46 00:02:24,880 --> 00:02:25,640 Speaker 1: first time. 47 00:02:25,960 --> 00:02:28,360 Speaker 3: And this five meter wide its steel chamber. 48 00:02:28,720 --> 00:02:31,360 Speaker 4: So the thing they made first plasma special for us 49 00:02:31,639 --> 00:02:33,399 Speaker 4: is there's so many things they have to go right, 50 00:02:33,520 --> 00:02:35,720 Speaker 4: and there's so many bits of a technology that no 51 00:02:35,760 --> 00:02:36,760 Speaker 4: one's ever done before. 52 00:02:37,240 --> 00:02:39,840 Speaker 2: And first plasma is that moment where you know that 53 00:02:40,120 --> 00:02:42,640 Speaker 2: everything actually worked for the first time, all at the 54 00:02:42,680 --> 00:02:45,639 Speaker 2: same time, and you get really bright height and you 55 00:02:45,680 --> 00:02:48,359 Speaker 2: know a lot of sharing about it as well. It's 56 00:02:48,440 --> 00:02:49,800 Speaker 2: just spent so much work with the team. 57 00:02:49,960 --> 00:02:54,359 Speaker 1: Basically, here's the moment they made that glowing gas field. 58 00:02:58,080 --> 00:03:02,960 Speaker 1: Why is heading playma so critical as a first stage 59 00:03:03,040 --> 00:03:03,600 Speaker 1: for fusion. 60 00:03:04,240 --> 00:03:07,160 Speaker 4: So for fusion, there's a whole bunch of ingredients that 61 00:03:07,200 --> 00:03:09,359 Speaker 4: you need. You need a magnet to confine a plasma, 62 00:03:09,400 --> 00:03:11,639 Speaker 4: you need a heating system to make it, you need 63 00:03:11,680 --> 00:03:15,079 Speaker 4: all the supporting technology, and actually plasma is one of 64 00:03:15,160 --> 00:03:18,160 Speaker 4: the last things to appear once you've got all those pieces, 65 00:03:18,600 --> 00:03:21,000 Speaker 4: and so a lot of what you would see in 66 00:03:21,000 --> 00:03:23,760 Speaker 4: a real fusion machine is actually right in front of you, 67 00:03:23,880 --> 00:03:26,399 Speaker 4: just at some smaller scale and late lower performance because 68 00:03:26,400 --> 00:03:29,000 Speaker 4: it's a prototype. But getting that plasma shows that we 69 00:03:29,000 --> 00:03:31,639 Speaker 4: can connect all the pieces and that the next step 70 00:03:31,680 --> 00:03:34,200 Speaker 4: is to increase for power, make a more powerful magnet, 71 00:03:34,639 --> 00:03:37,520 Speaker 4: make a bigger chamber, a better chamber, and actually start 72 00:03:37,600 --> 00:03:38,800 Speaker 4: driving fusion performance. 73 00:03:39,000 --> 00:03:41,320 Speaker 1: So this is what will be the beginning of a 74 00:03:41,320 --> 00:03:42,200 Speaker 1: fusion reactor. 75 00:03:43,160 --> 00:03:44,960 Speaker 2: Its descendants will bet yes. 76 00:03:44,840 --> 00:03:47,640 Speaker 4: So the next machine that we build will actually make 77 00:03:47,640 --> 00:03:51,240 Speaker 4: fusion reactions and that will be the headline, and then 78 00:03:51,320 --> 00:03:53,800 Speaker 4: the machine after that will make so many fusion reactions 79 00:03:53,800 --> 00:03:55,640 Speaker 4: you might actually be able to do something useful with it. 80 00:03:56,000 --> 00:03:58,000 Speaker 3: This is the next working prototype. 81 00:03:58,000 --> 00:04:02,280 Speaker 1: They're developing another magnet to make the dipole levitate. 82 00:04:02,720 --> 00:04:05,760 Speaker 2: This is actually one of the smaller magnets at open style. 83 00:04:05,760 --> 00:04:06,920 Speaker 2: We call it the top magnet. 84 00:04:07,120 --> 00:04:10,080 Speaker 4: When we design this machine, we have a really powerful 85 00:04:10,080 --> 00:04:12,360 Speaker 4: magnet in the center of a machine in our big chamber, 86 00:04:12,760 --> 00:04:14,760 Speaker 4: and that magnet is the one that has to levitate. 87 00:04:14,960 --> 00:04:17,720 Speaker 2: But why does it levitate. We use another magnet on 88 00:04:17,800 --> 00:04:20,640 Speaker 2: top that actually provides that force. And so this is 89 00:04:20,680 --> 00:04:21,920 Speaker 2: the top magnet goes on top. 90 00:04:22,000 --> 00:04:24,159 Speaker 4: It lifts the other one up and allows us to 91 00:04:24,200 --> 00:04:26,480 Speaker 4: disconnect everything and confine the plasma. 92 00:04:26,520 --> 00:04:30,760 Speaker 2: And that's a levitated dipoles, hated dipole, and this does 93 00:04:30,800 --> 00:04:32,400 Speaker 2: the levitate. Well, yeah, the lifting. 94 00:04:32,800 --> 00:04:35,880 Speaker 1: So this is like New Zealand's LK ninety nine superconductor. 95 00:04:36,440 --> 00:04:39,120 Speaker 2: Yeah no, no, let's not tagte anything like that. 96 00:04:39,520 --> 00:04:42,400 Speaker 3: So this is you know, if that actually did happen. 97 00:04:42,480 --> 00:04:43,360 Speaker 3: This is kind of it. 98 00:04:43,560 --> 00:04:44,520 Speaker 2: This is the real deal. 99 00:04:44,640 --> 00:04:47,320 Speaker 4: So all the hype around our something like LK ninety 100 00:04:47,360 --> 00:04:50,359 Speaker 4: nine was all really about the promise of superconductors. This 101 00:04:50,480 --> 00:04:53,000 Speaker 4: is a superconducting coil made out of materials that you 102 00:04:53,040 --> 00:04:55,880 Speaker 4: can procure today, and the quantity is to be useful, 103 00:04:55,920 --> 00:04:59,719 Speaker 4: like we can actually build things and we have to 104 00:04:59,720 --> 00:05:01,880 Speaker 4: make it cold for it to work, but we can 105 00:05:02,000 --> 00:05:05,720 Speaker 4: engineer around that. We don't have to wait for room 106 00:05:05,720 --> 00:05:08,760 Speaker 4: temperature superconductivity like LK nine nine for this to be 107 00:05:08,880 --> 00:05:10,040 Speaker 4: useful and applicable. 108 00:05:10,440 --> 00:05:12,680 Speaker 1: And tell me why livitation is so critical. It's because 109 00:05:12,720 --> 00:05:14,200 Speaker 1: it's hotter carpetarged, right. 110 00:05:14,400 --> 00:05:18,200 Speaker 4: Yeah, So this particular design is really inspired by how 111 00:05:18,240 --> 00:05:20,760 Speaker 4: planets can find plasma. So there's a plasma above our 112 00:05:20,760 --> 00:05:23,480 Speaker 4: head right now, but the highest energy particles hit the 113 00:05:23,560 --> 00:05:25,960 Speaker 4: poles and we call that the Aurora australis and the 114 00:05:26,000 --> 00:05:26,920 Speaker 4: Aurora borealis. 115 00:05:26,960 --> 00:05:30,239 Speaker 2: So it's very pretty. But that's about plasma cooling down. 116 00:05:30,600 --> 00:05:32,400 Speaker 4: So in order to stop that, we have to have 117 00:05:32,440 --> 00:05:34,360 Speaker 4: a magnet with a hole in the middle, so that 118 00:05:34,520 --> 00:05:37,400 Speaker 4: a plasma can keep going around without touching anything. But 119 00:05:37,480 --> 00:05:39,320 Speaker 4: if you try to grab on to our magnet. 120 00:05:39,320 --> 00:05:41,800 Speaker 2: If you have any kind of connection, plasma will have 121 00:05:41,880 --> 00:05:44,560 Speaker 2: the connection right, and that sounds bad for the connection, 122 00:05:44,640 --> 00:05:46,719 Speaker 2: but it's also very bad for the plasma. You're not 123 00:05:46,839 --> 00:05:48,840 Speaker 2: going to get their plasma hot enough to fuse if 124 00:05:48,839 --> 00:05:50,120 Speaker 2: it's touching anything physical. 125 00:05:50,640 --> 00:05:55,200 Speaker 1: Open Star is continuing the initial levitated dipole experiment in 126 00:05:55,200 --> 00:05:58,440 Speaker 1: the United States that was shut down at MIT and 127 00:05:58,520 --> 00:06:00,279 Speaker 1: Columbia University. 128 00:06:00,160 --> 00:06:01,880 Speaker 3: In the early two thousands. 129 00:06:02,480 --> 00:06:05,920 Speaker 1: Darren Gania was one of those physicists behind it. Now 130 00:06:05,960 --> 00:06:09,200 Speaker 1: he's working here in Wellington with open Star. How do 131 00:06:09,279 --> 00:06:12,919 Speaker 1: you feel having been part of the initial experiment that 132 00:06:13,080 --> 00:06:16,640 Speaker 1: proved it could work, to now being part of extending 133 00:06:16,680 --> 00:06:19,120 Speaker 1: that and in all places New Zealand. 134 00:06:19,520 --> 00:06:23,239 Speaker 5: Yeah, well, I mean it's we lost our funding for 135 00:06:23,680 --> 00:06:27,120 Speaker 5: LDX in the majority of our funding about twenty ten. 136 00:06:27,160 --> 00:06:29,120 Speaker 5: We kind of kept it going a little bit until 137 00:06:29,120 --> 00:06:31,560 Speaker 5: twenty fourteen, but most of our funding we lost in 138 00:06:31,560 --> 00:06:34,640 Speaker 5: twenty ten, and I really felt we left so much science, 139 00:06:35,080 --> 00:06:38,960 Speaker 5: so much interesting promise on the table, and it was 140 00:06:39,000 --> 00:06:41,240 Speaker 5: always I mean, it was a long period of grief, 141 00:06:41,279 --> 00:06:44,359 Speaker 5: tell you the truth, sort of you know, missing it, 142 00:06:45,200 --> 00:06:47,080 Speaker 5: and there was like that grief thing you like, don't 143 00:06:47,080 --> 00:06:49,840 Speaker 5: even want to think about it for a while, so 144 00:06:50,000 --> 00:06:52,080 Speaker 5: it was a while before I even thought about it again. 145 00:06:52,240 --> 00:06:54,120 Speaker 5: I didn't think about a little bit in between time. 146 00:06:54,160 --> 00:06:56,320 Speaker 5: Trying to get a refunded didn't work out. One of 147 00:06:56,360 --> 00:06:58,400 Speaker 5: the reasons that didn't get work out was we didn't 148 00:06:58,400 --> 00:07:02,600 Speaker 5: have the technology the magnetechnology required and the AXT fact 149 00:07:02,600 --> 00:07:05,600 Speaker 5: so I actually in twenty seventeen asked the US Department 150 00:07:05,640 --> 00:07:08,599 Speaker 5: of Energy for more money, but they said, actually, the 151 00:07:08,640 --> 00:07:12,520 Speaker 5: magnet technology you're you're asking for doesn't exist, and we 152 00:07:12,560 --> 00:07:14,960 Speaker 5: don't like the risk of funding you to do with 153 00:07:15,040 --> 00:07:17,240 Speaker 5: this plasma science even because the magnets aren't there. 154 00:07:17,920 --> 00:07:19,840 Speaker 2: So what happened was. 155 00:07:20,560 --> 00:07:23,440 Speaker 5: Ratu Openstar called me and they said, hey, we've been 156 00:07:23,440 --> 00:07:26,240 Speaker 5: developed this magnet technology and I said, oh, you mean 157 00:07:26,280 --> 00:07:27,360 Speaker 5: the stuff I've been waiting. 158 00:07:27,120 --> 00:07:28,840 Speaker 3: For all this time, and you've got it. 159 00:07:28,960 --> 00:07:29,720 Speaker 2: Let's go. Yeah. 160 00:07:29,760 --> 00:07:33,240 Speaker 5: So that's so it was like, oh, Wellington, yeah, no problem. 161 00:07:33,280 --> 00:07:36,840 Speaker 5: I mean, you've developed it here and I'm like so 162 00:07:37,000 --> 00:07:39,080 Speaker 5: happy to join. And it's like, you know, absolutely, it 163 00:07:39,120 --> 00:07:40,600 Speaker 5: was all this stuff I wanted to do was just 164 00:07:40,640 --> 00:07:43,760 Speaker 5: sitting on the table waiting for waiting for New Zealand 165 00:07:43,760 --> 00:07:45,400 Speaker 5: to come up with the magnet technology for us to 166 00:07:45,440 --> 00:07:45,840 Speaker 5: do it. 167 00:07:46,000 --> 00:07:49,760 Speaker 1: That they're not the only company chasing fusion. So how 168 00:07:49,800 --> 00:07:54,360 Speaker 1: does open Stars stack up against the competition worldwide? What 169 00:07:54,440 --> 00:07:56,440 Speaker 1: makes you think that you can solve this and be 170 00:07:56,560 --> 00:07:57,760 Speaker 1: first from New Zealand. 171 00:07:58,360 --> 00:08:00,560 Speaker 2: So I'll say a humble thing first. 172 00:08:00,880 --> 00:08:03,320 Speaker 4: I mean, we're picking up a technology that is less 173 00:08:03,360 --> 00:08:05,640 Speaker 4: mature than some of those other approaches. Bad amount of 174 00:08:05,680 --> 00:08:09,120 Speaker 4: money that's been thrown into tocmacs and stellarators and mirrors 175 00:08:09,160 --> 00:08:12,000 Speaker 4: and all sorts of things has driven a level of 176 00:08:12,080 --> 00:08:15,080 Speaker 4: understanding and the development that we do need to compete with, 177 00:08:15,280 --> 00:08:17,080 Speaker 4: we need to catch up to it. The thing that 178 00:08:17,120 --> 00:08:20,120 Speaker 4: makes us really excited about this machine is that it's 179 00:08:20,160 --> 00:08:23,840 Speaker 4: actually surprisingly easy to put together once you solve some 180 00:08:24,680 --> 00:08:28,160 Speaker 4: key challenges, and once you can start putting together, you 181 00:08:28,240 --> 00:08:30,760 Speaker 4: realize you can do it quickly. And so from actually 182 00:08:30,760 --> 00:08:33,920 Speaker 4: getting funded to building this machine took us about two 183 00:08:33,960 --> 00:08:36,360 Speaker 4: years to turn it on for the first time, and 184 00:08:36,400 --> 00:08:40,000 Speaker 4: in the world of fusion, that's at least double the speed, 185 00:08:40,000 --> 00:08:41,840 Speaker 4: if not more, depending on what kind of project you 186 00:08:41,840 --> 00:08:42,240 Speaker 4: look at. 187 00:08:42,760 --> 00:08:44,480 Speaker 2: And I'll give you another example. 188 00:08:44,800 --> 00:08:47,880 Speaker 4: These machines are basically big magnets and they hold onto 189 00:08:47,960 --> 00:08:52,040 Speaker 4: that plasma using magnetic field and if you build a TOCMAC, 190 00:08:52,400 --> 00:08:54,840 Speaker 4: and you've designed the magnets, you've built them, you've turned 191 00:08:54,880 --> 00:08:56,800 Speaker 4: it on, and then one of your engineers has a 192 00:08:56,800 --> 00:08:59,440 Speaker 4: clever way of improving the field by thirty percent. 193 00:09:00,120 --> 00:09:02,280 Speaker 2: You're going to have to build a new tokamac right, 194 00:09:02,360 --> 00:09:02,800 Speaker 2: and you're. 195 00:09:02,640 --> 00:09:05,520 Speaker 4: Going to spend three five years are going to build it, 196 00:09:05,720 --> 00:09:07,640 Speaker 4: and then you're going to spend five or ten years 197 00:09:07,640 --> 00:09:11,880 Speaker 4: building it. So the iteration cycle is like fifteen years easily. 198 00:09:12,800 --> 00:09:14,960 Speaker 4: Whereas with a dipole, if one of my engineers has 199 00:09:15,000 --> 00:09:16,920 Speaker 4: an idea to build a new magnet, we build it 200 00:09:16,960 --> 00:09:19,040 Speaker 4: and then we can swap it with the magnet that's 201 00:09:19,040 --> 00:09:21,800 Speaker 4: inside the chamber and testa train away and testa straight away. 202 00:09:21,800 --> 00:09:24,000 Speaker 4: So it literally takes us once that new magnet is ready, 203 00:09:24,000 --> 00:09:25,920 Speaker 4: it takes us about a week to do the swapover 204 00:09:26,280 --> 00:09:29,040 Speaker 4: and then we can start getting the results of whatever 205 00:09:29,120 --> 00:09:30,040 Speaker 4: that improvement is. 206 00:09:30,520 --> 00:09:34,040 Speaker 2: And so whilst the dipole that we're working on is behind, 207 00:09:34,480 --> 00:09:37,040 Speaker 2: our ability to catch up we think will mean that 208 00:09:37,120 --> 00:09:40,440 Speaker 2: we can actually overtake and make a meaningful contribution to 209 00:09:40,480 --> 00:09:42,120 Speaker 2: trying to solve fusion energy. 210 00:09:42,120 --> 00:09:46,280 Speaker 3: What is currently solved and still unsolved. 211 00:09:46,320 --> 00:09:50,160 Speaker 4: So nuclear fusion as a whole, what we know is 212 00:09:50,400 --> 00:09:54,880 Speaker 4: that if you heat these particles hot enough so Adam's nuclei, 213 00:09:55,360 --> 00:09:57,319 Speaker 4: you can heap them hot enough to actually fuse together 214 00:09:57,440 --> 00:09:59,560 Speaker 4: and release energy. So when we think about all the 215 00:09:59,640 --> 00:10:02,040 Speaker 4: numbers that are involved with that part of a process 216 00:10:02,120 --> 00:10:04,440 Speaker 4: that has been solved for a very long time, the 217 00:10:04,480 --> 00:10:06,960 Speaker 4: part that's unsolved is how do you get them that 218 00:10:07,120 --> 00:10:09,560 Speaker 4: hot in the first place in a way that's actually 219 00:10:09,800 --> 00:10:11,000 Speaker 4: economic and manageable. 220 00:10:11,320 --> 00:10:13,440 Speaker 3: So what are you here at Open Star trying to 221 00:10:13,480 --> 00:10:14,520 Speaker 3: solve in that puzzle? 222 00:10:14,960 --> 00:10:17,280 Speaker 4: So it always comes down to how do you hold 223 00:10:17,320 --> 00:10:20,720 Speaker 4: on to this superheated gas which ends up being a plasma. 224 00:10:21,400 --> 00:10:23,640 Speaker 4: And there's different ways of holding onto a plasma. So 225 00:10:23,640 --> 00:10:26,280 Speaker 4: we have a particular approach here called the levitated dipole. 226 00:10:26,480 --> 00:10:28,959 Speaker 4: We think we're the only team in the world really 227 00:10:29,000 --> 00:10:32,439 Speaker 4: working on this for fusion, and it has a lot 228 00:10:32,480 --> 00:10:35,120 Speaker 4: of advantages for holding onto that plasma that should allow 229 00:10:35,200 --> 00:10:37,360 Speaker 4: us to get it hot but also do it in 230 00:10:37,360 --> 00:10:38,680 Speaker 4: a much more economic fashion. 231 00:10:38,960 --> 00:10:41,800 Speaker 3: How much of a step is that to unlocking everything else? 232 00:10:42,360 --> 00:10:45,920 Speaker 4: So if we were to look back in a thousand 233 00:10:46,040 --> 00:10:48,880 Speaker 4: years at what we're doing today versus like humans discovering 234 00:10:48,920 --> 00:10:51,800 Speaker 4: fire again, and so just like we made a little 235 00:10:51,800 --> 00:10:52,480 Speaker 4: fire pit. 236 00:10:52,440 --> 00:10:54,439 Speaker 2: One day, and we're all going to gather around it. 237 00:10:55,040 --> 00:10:58,559 Speaker 4: We eventually learn how to build power plants and jet 238 00:10:58,559 --> 00:11:02,840 Speaker 4: turbines and really manit pulate fire. Plasma is our version 239 00:11:02,840 --> 00:11:05,160 Speaker 4: of fire, but for doing fusion. 240 00:11:06,320 --> 00:11:09,599 Speaker 3: What's your timeline for nuclear? When do we start. 241 00:11:09,440 --> 00:11:12,360 Speaker 1: Creating and adding nuclear energy to the grid, not just 242 00:11:12,440 --> 00:11:15,080 Speaker 1: here but anywhere or everywhere in the world. 243 00:11:15,240 --> 00:11:17,840 Speaker 3: Most people think it's twenty thirties. Is that actually realistic? 244 00:11:17,880 --> 00:11:22,200 Speaker 4: Right? It's you have to be ambitious about these things 245 00:11:22,640 --> 00:11:25,640 Speaker 4: you have otherwise we've actually seen what happens when these 246 00:11:25,679 --> 00:11:28,600 Speaker 4: projects give themselves too much space and too much time 247 00:11:28,640 --> 00:11:31,280 Speaker 4: to do it. They don't They won't hit twenty fifty. 248 00:11:31,320 --> 00:11:34,040 Speaker 4: They'll just never finish, right. And so you can make 249 00:11:34,160 --> 00:11:36,320 Speaker 4: arguments about whether or not we'll set an ambitious goal 250 00:11:36,320 --> 00:11:38,560 Speaker 4: and it will push back and we'll miss it. But 251 00:11:38,600 --> 00:11:39,880 Speaker 4: at the end of the day, the thing that gets 252 00:11:39,920 --> 00:11:41,719 Speaker 4: us excited here at Openstar and a lot of the 253 00:11:41,760 --> 00:11:43,880 Speaker 4: other companies is that we actually have a chance of 254 00:11:43,920 --> 00:11:47,360 Speaker 4: contributing to solving the climate crisis. And so that means 255 00:11:47,360 --> 00:11:49,560 Speaker 4: they have a first reactor really probably needs to turn 256 00:11:49,600 --> 00:11:52,360 Speaker 4: on in the twenty thirties, because then we still need 257 00:11:52,400 --> 00:11:55,240 Speaker 4: to build thousands more of them to actually decarbonize for 258 00:11:55,320 --> 00:11:57,199 Speaker 4: grit So a lot of people think that there is 259 00:11:57,240 --> 00:12:00,600 Speaker 4: a scientific challenge getting to break even first, but then 260 00:12:00,600 --> 00:12:03,080 Speaker 4: there is a huge industrial challenge actually building out these 261 00:12:03,120 --> 00:12:04,000 Speaker 4: machines afterwards. 262 00:12:04,320 --> 00:12:07,760 Speaker 3: What does end adoption of nuclear look like in your mind? 263 00:12:07,920 --> 00:12:08,800 Speaker 3: Is it small. 264 00:12:08,600 --> 00:12:12,240 Speaker 1: Nuclear reactors everywhere because that would be perhaps more commercially viable, 265 00:12:12,360 --> 00:12:16,800 Speaker 1: or is this industrial scale type stuff that government's control. 266 00:12:17,360 --> 00:12:20,400 Speaker 4: So for fusion, it does end up depending on the 267 00:12:20,440 --> 00:12:23,280 Speaker 4: different type of reactor you're looking at, and so you 268 00:12:23,280 --> 00:12:26,480 Speaker 4: could end up in that utility scale replacing co fire 269 00:12:26,559 --> 00:12:30,360 Speaker 4: power plants hundreds of megawatts up to a gigawatt. But actually, 270 00:12:30,440 --> 00:12:34,280 Speaker 4: from a commercial perspective, really what you're hoping for is 271 00:12:34,320 --> 00:12:37,400 Speaker 4: the smallest viable machine where you can find a market 272 00:12:37,480 --> 00:12:40,920 Speaker 4: for that just keeps the capitalization risk under control and 273 00:12:41,040 --> 00:12:44,560 Speaker 4: allows the iteration driven by revenue to allow you to 274 00:12:44,600 --> 00:12:47,040 Speaker 4: keep scaling machines and building better and better ones as 275 00:12:47,040 --> 00:12:47,640 Speaker 4: time moves on. 276 00:12:48,080 --> 00:12:48,920 Speaker 2: So actually, I. 277 00:12:48,840 --> 00:12:51,920 Speaker 4: Don't think it's too much about the end state. The 278 00:12:52,000 --> 00:12:54,000 Speaker 4: n state is some kind of energy utope here, and 279 00:12:54,000 --> 00:12:55,240 Speaker 4: I'm looking forward to it. 280 00:12:55,720 --> 00:12:58,199 Speaker 2: But actually it's like, what's that first machine we're going. 281 00:12:58,160 --> 00:13:01,280 Speaker 4: To build that people find useful, probably like a fifty 282 00:13:01,400 --> 00:13:06,120 Speaker 4: megawatt electric machine that is probably bohowering a data center that. 283 00:13:06,160 --> 00:13:09,320 Speaker 1: Is effectively energy you Tolkia, right, it is clean, abundant, 284 00:13:09,720 --> 00:13:15,240 Speaker 1: affordable energy forever. What does that mean for economies? What 285 00:13:15,360 --> 00:13:18,559 Speaker 1: does that unleash? It would mean we're entirely independent. 286 00:13:19,040 --> 00:13:20,800 Speaker 2: So there's a There's a couple of things. 287 00:13:20,880 --> 00:13:24,120 Speaker 4: One is I think fusion is a really exciting industry 288 00:13:24,400 --> 00:13:27,200 Speaker 4: because it rewards countries for their innovation culture and their 289 00:13:27,200 --> 00:13:30,640 Speaker 4: hard work rather than their luck on what natural resources 290 00:13:30,720 --> 00:13:32,040 Speaker 4: they happen to be founded upon. 291 00:13:32,160 --> 00:13:32,319 Speaker 2: Right. 292 00:13:32,840 --> 00:13:36,440 Speaker 4: And so we in New Zealand we kind of worship 293 00:13:36,480 --> 00:13:39,079 Speaker 4: our own innovation culture number eight wire and this is 294 00:13:39,080 --> 00:13:41,760 Speaker 4: a chance for us to actually translate that into full 295 00:13:41,800 --> 00:13:47,520 Speaker 4: blown economic juggernaut. The other interesting thing about what their 296 00:13:47,600 --> 00:13:51,600 Speaker 4: energy utopia looks like is that it really stretches my imagination. 297 00:13:51,760 --> 00:13:54,480 Speaker 4: I don't have a fantastic argument like answer rather than 298 00:13:54,480 --> 00:13:58,760 Speaker 4: like flying cars and really cheap rocket trips to Mars, right, 299 00:13:59,800 --> 00:14:02,839 Speaker 4: But to give people a sense of what that change 300 00:14:02,840 --> 00:14:05,280 Speaker 4: could look like from an every day perspective, I think 301 00:14:05,320 --> 00:14:07,240 Speaker 4: the Internet gives us a pretty good example. 302 00:14:07,559 --> 00:14:08,800 Speaker 2: We all remember dial up. 303 00:14:08,880 --> 00:14:11,600 Speaker 4: We all remember broadband being rolled out, and we remember 304 00:14:11,720 --> 00:14:15,520 Speaker 4: paying for data by the gigabyte and then running out 305 00:14:15,520 --> 00:14:18,319 Speaker 4: and having to pay more. That's effectively how we sell 306 00:14:18,520 --> 00:14:21,080 Speaker 4: energy today, right, every bit of energy you use you 307 00:14:21,160 --> 00:14:24,160 Speaker 4: have to pay for, whereas with data that's actually moved 308 00:14:24,200 --> 00:14:27,120 Speaker 4: towards a transmission model. You pay for the bandwidth like 309 00:14:27,200 --> 00:14:29,800 Speaker 4: you want a faster Internet connection. And so we think 310 00:14:29,920 --> 00:14:32,680 Speaker 4: you could probably achieve the same thing with energy, which is, yeah, 311 00:14:32,720 --> 00:14:34,560 Speaker 4: you pay for a connection. If you're running a factory, 312 00:14:34,680 --> 00:14:36,920 Speaker 4: you're going to pay for a bigger connection, but the 313 00:14:37,000 --> 00:14:39,200 Speaker 4: amount of energy that you use is no longer a 314 00:14:39,280 --> 00:14:43,120 Speaker 4: driving force of the economics, and that will unlock huge 315 00:14:43,560 --> 00:14:47,760 Speaker 4: business applications but also really good societal outcomes. Families won't 316 00:14:47,800 --> 00:14:51,280 Speaker 4: worry about continuing to pay the power bill to keep 317 00:14:51,320 --> 00:14:54,200 Speaker 4: their houses warm. All of that infrastructure already exists, it's 318 00:14:54,240 --> 00:14:55,640 Speaker 4: just the powers too expensive today. 319 00:14:55,760 --> 00:14:57,960 Speaker 1: So there's not only primary use cases in your mind, 320 00:14:58,000 --> 00:14:59,520 Speaker 1: but certainly secondary. 321 00:14:59,120 --> 00:14:59,920 Speaker 3: Use cases as well. 322 00:15:00,160 --> 00:15:04,680 Speaker 4: Absolutely, and that's probably actually we talked about that MVP 323 00:15:04,840 --> 00:15:09,040 Speaker 4: in terms of electricity, but really the true MVP for 324 00:15:09,120 --> 00:15:12,520 Speaker 4: fusion is probably a different application. One really exciting one 325 00:15:12,560 --> 00:15:14,920 Speaker 4: is medical isotopes. For example, So if you go to 326 00:15:14,920 --> 00:15:16,840 Speaker 4: a hospital and you need to get like a pet 327 00:15:16,880 --> 00:15:19,280 Speaker 4: scan or a cat scan, you're ingesting some kind of 328 00:15:19,320 --> 00:15:22,560 Speaker 4: substance that's a little bit radioactive, and that allows doctors 329 00:15:22,600 --> 00:15:25,640 Speaker 4: to see where that substance went and find either tumors 330 00:15:25,720 --> 00:15:30,320 Speaker 4: or abnormalities in your body. And those substances come from 331 00:15:30,360 --> 00:15:33,880 Speaker 4: a supply chain that will collapse by twenty thirty five, 332 00:15:34,360 --> 00:15:37,040 Speaker 4: and we don't as a society have a good replacement 333 00:15:37,080 --> 00:15:40,440 Speaker 4: for that. So modern medicine has been adopting these techniques 334 00:15:40,480 --> 00:15:43,960 Speaker 4: to great success. It's a multi billion dollar perannum industry. 335 00:15:44,520 --> 00:15:46,680 Speaker 4: We're going to run out a supply in twenty thirty five. 336 00:15:46,960 --> 00:15:49,880 Speaker 4: Populations are getting older and wealthier, so the demand is 337 00:15:49,960 --> 00:15:53,440 Speaker 4: absolutely there, and we think smaller fusion reactors are probably 338 00:15:53,480 --> 00:15:57,200 Speaker 4: a great source of those materials. So that's probably the 339 00:15:57,240 --> 00:15:58,880 Speaker 4: most immediate market that we're looking for. 340 00:15:58,880 --> 00:16:00,760 Speaker 2: Of that's kind of adjacent power. 341 00:16:01,200 --> 00:16:03,480 Speaker 1: You mentioned something interesting and one of your earlier answers 342 00:16:03,520 --> 00:16:07,040 Speaker 1: about how abundant energy from future and would mean that 343 00:16:07,080 --> 00:16:11,000 Speaker 1: we are no longer reliant on resources like oil, like coal, 344 00:16:11,120 --> 00:16:14,320 Speaker 1: things that are resources that we currently pull up out 345 00:16:14,360 --> 00:16:17,400 Speaker 1: of the ground. As that is our future for energy 346 00:16:18,000 --> 00:16:20,560 Speaker 1: that disrupts the world order as we know it, Like, 347 00:16:20,640 --> 00:16:23,080 Speaker 1: do you recognize that is the possibility of what you're 348 00:16:23,120 --> 00:16:23,600 Speaker 1: doing here? 349 00:16:24,000 --> 00:16:25,080 Speaker 2: Uh? Yeah. 350 00:16:25,240 --> 00:16:28,160 Speaker 4: I think the challenge that we have in front of us, 351 00:16:28,480 --> 00:16:31,120 Speaker 4: if we do nothing, the world order will be disrupted. 352 00:16:31,200 --> 00:16:31,320 Speaker 5: Right. 353 00:16:31,400 --> 00:16:35,640 Speaker 4: Climate change is an existential threat for humanity that needs 354 00:16:35,680 --> 00:16:40,080 Speaker 4: to be solved. And I think even countries that produce 355 00:16:40,320 --> 00:16:44,480 Speaker 4: the existing kind of energy sources like oil and gas 356 00:16:44,480 --> 00:16:48,440 Speaker 4: and coal, they do recognize this in the long run, 357 00:16:48,960 --> 00:16:52,200 Speaker 4: and be at a company or a nation state, often 358 00:16:52,280 --> 00:16:54,640 Speaker 4: the point of view is we're not in the oil business. 359 00:16:54,720 --> 00:16:56,359 Speaker 2: We're in the energy business. 360 00:16:56,240 --> 00:17:00,600 Speaker 4: And whatever form energy takes, you know, for humanity, that's 361 00:17:00,640 --> 00:17:02,600 Speaker 4: the business we want to be in. And so you 362 00:17:02,720 --> 00:17:08,240 Speaker 4: do see existing fossil fuel industry investing in new energy technologies. 363 00:17:08,600 --> 00:17:10,440 Speaker 4: Now you can get into an argument about whether or 364 00:17:10,480 --> 00:17:13,600 Speaker 4: not that's greenwashing, whether or not a believer's technologies will 365 00:17:13,640 --> 00:17:14,280 Speaker 4: be successful. 366 00:17:14,600 --> 00:17:16,679 Speaker 2: But we're at a company like Open Style. All we 367 00:17:16,720 --> 00:17:18,800 Speaker 2: can dedicate ourselves to is actually trying to solve a 368 00:17:18,840 --> 00:17:19,920 Speaker 2: problem that's in front of us. 369 00:17:20,320 --> 00:17:24,120 Speaker 1: In twenty ten, Stephen Hawking said fusion could provide an 370 00:17:24,160 --> 00:17:27,600 Speaker 1: inexhaustible supply of energy without pollution. 371 00:17:27,920 --> 00:17:28,840 Speaker 3: Or global warming. 372 00:17:29,480 --> 00:17:33,760 Speaker 6: It's considered to be clean, cheap, efficient, and endless, yet 373 00:17:33,760 --> 00:17:41,880 Speaker 6: its nuclear association is often unappealing for reasons History can explain, and. 374 00:17:41,960 --> 00:17:46,120 Speaker 2: This is smoke that towered and mushroomed August sixth, nineteen 375 00:17:46,280 --> 00:17:51,720 Speaker 2: forty five over the ademized remains of Hiroshima when. 376 00:17:51,560 --> 00:17:53,439 Speaker 3: A new Zealanders split the atom. 377 00:17:54,240 --> 00:17:57,480 Speaker 1: History now tells us how that ended up when it 378 00:17:57,520 --> 00:18:02,480 Speaker 1: became uncontrolled. What is the potential risk of what we're 379 00:18:02,480 --> 00:18:07,160 Speaker 1: talking about here? Could this lead to devastation and destruction 380 00:18:07,800 --> 00:18:09,240 Speaker 1: if it falls into the wrong hands again. 381 00:18:10,240 --> 00:18:13,440 Speaker 4: So there are risks, probably on two aspects to talk 382 00:18:13,440 --> 00:18:14,040 Speaker 4: about a risk. 383 00:18:14,200 --> 00:18:16,600 Speaker 2: One is from a local risk. 384 00:18:16,960 --> 00:18:19,000 Speaker 4: So if you've built one of these machines, is it 385 00:18:19,040 --> 00:18:20,920 Speaker 4: safe to have in your backyard? And I think that's 386 00:18:20,920 --> 00:18:25,639 Speaker 4: something that people ready care about and rightfully so fusion 387 00:18:26,280 --> 00:18:29,160 Speaker 4: why we're so excited about it is well, there are risks, 388 00:18:29,520 --> 00:18:31,920 Speaker 4: we're confident that they can be managed in the same 389 00:18:31,960 --> 00:18:35,080 Speaker 4: way we manage other industrial risks. So a fusion power 390 00:18:35,080 --> 00:18:38,160 Speaker 4: plant should really be no more dangerous than a chemical 391 00:18:38,200 --> 00:18:42,800 Speaker 4: plant or a big manufacturing facility. It's big voltages, it's 392 00:18:42,840 --> 00:18:45,080 Speaker 4: big machines, it's things that can go pop if they're 393 00:18:45,080 --> 00:18:48,160 Speaker 4: not handled properly and humans can do this, we know 394 00:18:48,280 --> 00:18:50,240 Speaker 4: we can make that work because our whole modern world 395 00:18:50,240 --> 00:18:55,280 Speaker 4: depends on that and traditional nuclear so nuclear fission takes 396 00:18:55,280 --> 00:18:57,240 Speaker 4: it a step on that. If you look at the 397 00:18:57,320 --> 00:19:01,120 Speaker 4: clean up cost for Fukushima Daichi all costs for Japanese 398 00:19:01,119 --> 00:19:04,560 Speaker 4: taxpayer two hundred and fifty billion dollars over the course 399 00:19:04,560 --> 00:19:07,480 Speaker 4: of that project. That's not something you can get insurance 400 00:19:07,520 --> 00:19:10,800 Speaker 4: for and not something that we expect to be necessary 401 00:19:10,840 --> 00:19:14,959 Speaker 4: for fusion machines. In terms of communicating that safety, like, 402 00:19:15,080 --> 00:19:16,920 Speaker 4: my commitment is just to be as open an eyes 403 00:19:17,720 --> 00:19:21,080 Speaker 4: with people and share their concerns and show how we're 404 00:19:21,080 --> 00:19:21,920 Speaker 4: going to manage those. 405 00:19:23,200 --> 00:19:24,440 Speaker 2: So that's one aspect. 406 00:19:24,760 --> 00:19:28,600 Speaker 4: The second aspect is kind of is this a pathway 407 00:19:28,600 --> 00:19:33,200 Speaker 4: to global apocalypse? And I think pretty clearly know and 408 00:19:33,280 --> 00:19:37,040 Speaker 4: it is a really good example of this eat that big, 409 00:19:37,080 --> 00:19:41,959 Speaker 4: gargantuan project I spoke about as a collaboration between Russia, China, 410 00:19:42,119 --> 00:19:46,600 Speaker 4: vu Japan, the United States, and these are all entities 411 00:19:46,680 --> 00:19:49,480 Speaker 4: or countries that don't necessarily like each other all the time, 412 00:19:49,800 --> 00:19:51,919 Speaker 4: And in fact, when Russia joined, I'm pretty sure it 413 00:19:51,960 --> 00:19:55,360 Speaker 4: was still the Soviet Union. Fusion was always seen as 414 00:19:55,359 --> 00:20:00,000 Speaker 4: a safe technology that you know, rival nations could actual 415 00:20:00,240 --> 00:20:03,440 Speaker 4: collaborate on and be an olive branch between them without 416 00:20:03,520 --> 00:20:06,560 Speaker 4: sharing secrets that would let the other one figure out 417 00:20:06,560 --> 00:20:09,880 Speaker 4: how to destroy the other. And so fusion has always 418 00:20:09,920 --> 00:20:12,560 Speaker 4: been able to take on like a peaceful role in 419 00:20:12,560 --> 00:20:15,720 Speaker 4: our geopolitics, and we think that sure it can continue, 420 00:20:15,760 --> 00:20:17,680 Speaker 4: and we will continue over the next few decades. 421 00:20:17,800 --> 00:20:21,320 Speaker 1: The ultimate question, though, is can we control fusion? 422 00:20:21,600 --> 00:20:21,879 Speaker 2: Sure? 423 00:20:22,920 --> 00:20:23,240 Speaker 3: Can we? 424 00:20:24,720 --> 00:20:28,880 Speaker 4: So control is an interesting one. The thing that when 425 00:20:28,920 --> 00:20:31,200 Speaker 4: we look at these other machines, one of the reasons 426 00:20:31,240 --> 00:20:34,119 Speaker 4: why they become so complicated is because that's exactly what 427 00:20:34,119 --> 00:20:36,320 Speaker 4: they're trying to do. They're trying to control the plasma 428 00:20:36,640 --> 00:20:39,320 Speaker 4: in a way that keeps it locked up, allows you 429 00:20:39,359 --> 00:20:41,840 Speaker 4: to heat it up without it kind of breaking free. 430 00:20:42,359 --> 00:20:44,879 Speaker 4: And that's actually the one thing that we wanted to 431 00:20:44,920 --> 00:20:48,640 Speaker 4: avoid the most. And we think we have the only 432 00:20:48,800 --> 00:20:52,479 Speaker 4: method for confining a plasma using a magnet that doesn't 433 00:20:52,480 --> 00:20:55,240 Speaker 4: have that particular problem. And so the way to put 434 00:20:55,240 --> 00:20:58,280 Speaker 4: it is, if you build a plasma in a lab 435 00:20:58,359 --> 00:21:00,600 Speaker 4: like this one, but you want it to look and 436 00:21:00,640 --> 00:21:04,040 Speaker 4: behave like a plasma that's actually stable in nature, the 437 00:21:04,119 --> 00:21:05,600 Speaker 4: dipole is the only way to do it. 438 00:21:05,680 --> 00:21:08,520 Speaker 2: There's a big dipole plasma above our heads right now. 439 00:21:08,600 --> 00:21:12,439 Speaker 4: It's called the magnetosphere, and that magnetosphere captures particles that 440 00:21:12,480 --> 00:21:16,880 Speaker 4: come from the Sun. And really importantly, if that magnetosphere 441 00:21:16,960 --> 00:21:20,040 Speaker 4: wasn't there, that solar wind would have wiped out the 442 00:21:20,040 --> 00:21:22,760 Speaker 4: atmosphere millions of years ago, if not billions of years ago, 443 00:21:22,800 --> 00:21:23,120 Speaker 4: and there. 444 00:21:23,000 --> 00:21:24,119 Speaker 2: Wouldn't be life on Earth. 445 00:21:24,359 --> 00:21:28,359 Speaker 4: So we already owe our existence to magnetospheres and controlling 446 00:21:28,600 --> 00:21:30,679 Speaker 4: our plasmas, and so we're just trying to do that 447 00:21:30,760 --> 00:21:32,960 Speaker 4: in a lab and take advantage of stability. 448 00:21:33,480 --> 00:21:38,399 Speaker 1: What makes you think that countries would take on fusion when. 449 00:21:38,320 --> 00:21:41,400 Speaker 3: They have historically been so against using fission. 450 00:21:42,720 --> 00:21:45,680 Speaker 4: I think it's hard to argue that fission doesn't have 451 00:21:45,760 --> 00:21:48,639 Speaker 4: pretty serious challenges from an engineering point of view that 452 00:21:48,880 --> 00:21:51,240 Speaker 4: have to be managed in a way that makes communities 453 00:21:51,280 --> 00:21:51,879 Speaker 4: feel safe. 454 00:21:52,080 --> 00:21:53,080 Speaker 2: And it's really up. 455 00:21:53,000 --> 00:21:55,280 Speaker 4: To the judgment of those communities whether or not that's 456 00:21:55,320 --> 00:21:57,040 Speaker 4: been a successful arrangement. 457 00:21:57,880 --> 00:21:59,720 Speaker 2: And so you even have really. 458 00:21:59,480 --> 00:22:02,760 Speaker 4: Like people would absolutely say, well the Germans, no engineering, 459 00:22:02,880 --> 00:22:04,560 Speaker 4: like that's a that's a country that should be on 460 00:22:04,600 --> 00:22:07,480 Speaker 4: top of the stuff. And even they have moved seriously 461 00:22:07,520 --> 00:22:11,800 Speaker 4: away from fission. As an engineer, I can see the 462 00:22:11,880 --> 00:22:14,480 Speaker 4: merits of how you would keep a fission reactor safe, 463 00:22:14,640 --> 00:22:17,800 Speaker 4: but I really do think it's it's legitimate that communities 464 00:22:17,960 --> 00:22:21,480 Speaker 4: need to be convinced, and if they don't understand that, 465 00:22:21,760 --> 00:22:23,840 Speaker 4: I think that's that's kind of the end of a 466 00:22:23,880 --> 00:22:28,399 Speaker 4: picture for fusion. We think that fundamentally the technology is 467 00:22:28,520 --> 00:22:32,000 Speaker 4: safer to start with, which means that the safety issues 468 00:22:32,000 --> 00:22:34,919 Speaker 4: are easy, easier for us to solve, and then easier 469 00:22:34,920 --> 00:22:38,360 Speaker 4: for us to communicate with communities on how it's being managed, 470 00:22:38,680 --> 00:22:42,159 Speaker 4: and the absolute level of risk is just lower to 471 00:22:42,200 --> 00:22:47,640 Speaker 4: begin with. And then finally, since bringing the company out 472 00:22:47,640 --> 00:22:50,840 Speaker 4: of stealth, from a personal perspective, I've been talking to 473 00:22:51,040 --> 00:22:55,200 Speaker 4: normal people about fusion, and people can tell the difference 474 00:22:55,320 --> 00:22:59,480 Speaker 4: between fission and fusion, and people as long as you're 475 00:22:59,520 --> 00:23:01,800 Speaker 4: open and honest about how those risks are going to 476 00:23:01,800 --> 00:23:04,520 Speaker 4: be managed, I think they're very welcoming that we give 477 00:23:04,600 --> 00:23:06,199 Speaker 4: us a shot and we see if this is a 478 00:23:06,240 --> 00:23:07,440 Speaker 4: solution that we're looking for. 479 00:23:07,800 --> 00:23:11,160 Speaker 1: Appetite for fusion is growing where the cost of existing 480 00:23:11,280 --> 00:23:16,000 Speaker 1: energy has hit crisis levels. For example, Germany is funding 481 00:23:16,040 --> 00:23:19,320 Speaker 1: a research effort to construct its first fusion power plant 482 00:23:19,640 --> 00:23:23,679 Speaker 1: by twenty forty, but power companies are already spending billions 483 00:23:23,720 --> 00:23:28,680 Speaker 1: on more renewable energy generation infrastructure, such as wind and solar. 484 00:23:29,040 --> 00:23:31,480 Speaker 3: I also want to talk to you about renewable generation. 485 00:23:31,880 --> 00:23:35,000 Speaker 1: Elon Musk tweeted even this morning saying that he thinks 486 00:23:35,040 --> 00:23:40,159 Speaker 1: solar will be the biggest edition of electricity generation in 487 00:23:40,200 --> 00:23:43,879 Speaker 1: the world. Obviously that's what he's doing with Tesla. Is 488 00:23:43,920 --> 00:23:46,680 Speaker 1: this a bet against Elon Musk? Is this a bet 489 00:23:46,760 --> 00:23:48,400 Speaker 1: against renewable generation. 490 00:23:49,520 --> 00:23:52,440 Speaker 4: One of the things that Elon I think prides himself 491 00:23:52,480 --> 00:23:56,520 Speaker 4: on is he backs technologies that are actually very mature, 492 00:23:57,080 --> 00:24:00,199 Speaker 4: and he doesn't actually like solving technical rescue for can 493 00:24:00,240 --> 00:24:02,679 Speaker 4: avoid it. Right, So solar panels are something that you 494 00:24:02,720 --> 00:24:06,960 Speaker 4: can now procure in mass like. Industry is making those 495 00:24:06,960 --> 00:24:10,040 Speaker 4: things cheaper and cheaper and cheaper. But ultimately renewables have 496 00:24:10,080 --> 00:24:14,040 Speaker 4: a really big problem, which is that they're on supply technologies. 497 00:24:14,080 --> 00:24:16,000 Speaker 2: They give you the power when they want, not when 498 00:24:16,000 --> 00:24:16,720 Speaker 2: you want. 499 00:24:16,920 --> 00:24:20,560 Speaker 4: And the answer to this has traditionally been batteries, that 500 00:24:20,680 --> 00:24:22,480 Speaker 4: we're going to store the power and then sell it 501 00:24:22,520 --> 00:24:25,680 Speaker 4: back to people. But the economic model around that, whilst 502 00:24:25,720 --> 00:24:30,800 Speaker 4: it can enable renewables, is not actually a detriment to 503 00:24:30,960 --> 00:24:33,840 Speaker 4: something like fusion. So if you build a fusion power plant, 504 00:24:33,880 --> 00:24:36,879 Speaker 4: it makes a great baseload generator and that means it 505 00:24:36,880 --> 00:24:38,679 Speaker 4: can sell you power during the day, but it can 506 00:24:38,720 --> 00:24:42,320 Speaker 4: also produce power overnight when people don't actually demand that much. 507 00:24:42,520 --> 00:24:44,760 Speaker 4: And so if you've told me that we've solved the 508 00:24:44,800 --> 00:24:47,520 Speaker 4: battery problem for renewables, I'm just going to tell you cool, 509 00:24:47,520 --> 00:24:49,919 Speaker 4: We'll build a battery pack, we'll charge that overnight with 510 00:24:49,960 --> 00:24:52,040 Speaker 4: our fusion power, and we'll sell it back into the grid. 511 00:24:52,200 --> 00:24:55,399 Speaker 2: So our ability to actually compete with renewables as they 512 00:24:55,400 --> 00:24:56,440 Speaker 2: get cheaper and cheaper. 513 00:24:56,320 --> 00:25:01,040 Speaker 4: Should be viable. Batteries are not the killer from that perspective. 514 00:25:01,240 --> 00:25:04,239 Speaker 1: So you see an energy future where there's fusion and 515 00:25:04,320 --> 00:25:05,560 Speaker 1: also renewables in the group. 516 00:25:06,200 --> 00:25:09,600 Speaker 4: If fusion takes us as far as we think it can, no, 517 00:25:09,720 --> 00:25:13,680 Speaker 4: it will just be fusion eventually, so my lifetime, but 518 00:25:14,160 --> 00:25:17,800 Speaker 4: that's that's the ultimate. So there's a physical limit on 519 00:25:17,840 --> 00:25:19,800 Speaker 4: how good you can make a solar panel, right, and 520 00:25:19,840 --> 00:25:21,360 Speaker 4: we will probably hit that. 521 00:25:21,359 --> 00:25:22,520 Speaker 2: Limit within my lifetime. 522 00:25:22,840 --> 00:25:25,920 Speaker 4: And then there you're looking at, well sunlight hits for 523 00:25:25,960 --> 00:25:28,440 Speaker 4: the Earth there about one killer wat per square meta 524 00:25:29,240 --> 00:25:31,440 Speaker 4: and you can't do any better than that other than 525 00:25:31,560 --> 00:25:32,160 Speaker 4: taking up more. 526 00:25:32,119 --> 00:25:32,800 Speaker 2: And more space. 527 00:25:33,080 --> 00:25:35,680 Speaker 4: Whereas a fusion reactor can be made better and better 528 00:25:35,680 --> 00:25:38,000 Speaker 4: and better as we discover new materials and we get 529 00:25:38,000 --> 00:25:41,320 Speaker 4: better at the engineering, our ability to produce power and 530 00:25:41,440 --> 00:25:44,400 Speaker 4: compact to useful units that we can actually plug into 531 00:25:44,440 --> 00:25:48,440 Speaker 4: society should outpace the diffuse energy source. 532 00:25:48,440 --> 00:25:49,080 Speaker 2: Fatter is our. 533 00:25:49,080 --> 00:25:50,520 Speaker 3: Sum sort of sum that up. 534 00:25:50,560 --> 00:25:53,359 Speaker 1: Then the billions of dollars, including in this country, that 535 00:25:53,400 --> 00:25:56,960 Speaker 1: has been thrown at renewable generation will one day be 536 00:25:57,000 --> 00:25:58,720 Speaker 1: wasted because fusuon is just gonna own. 537 00:25:58,640 --> 00:26:01,040 Speaker 2: No, absolutely not, that's ridiculous. 538 00:26:02,240 --> 00:26:05,000 Speaker 4: Any investment has some time horizon to give you a return, 539 00:26:05,520 --> 00:26:07,800 Speaker 4: right And so what I've just talked about is like 540 00:26:07,840 --> 00:26:10,159 Speaker 4: a multi decade or like this is this thing that 541 00:26:10,240 --> 00:26:12,240 Speaker 4: my kids and grandkids are going to watch happen. Right 542 00:26:13,160 --> 00:26:15,040 Speaker 4: for now, what we need to do is get as 543 00:26:15,240 --> 00:26:19,280 Speaker 4: much renewable and clean energy on the grid to displace 544 00:26:19,720 --> 00:26:23,520 Speaker 4: carbon emitting energy sources. And renewables are fantastic at that 545 00:26:23,680 --> 00:26:26,040 Speaker 4: right now. And what's going to happen is that they're 546 00:26:26,040 --> 00:26:28,040 Speaker 4: going to take up more and more capacity, and then 547 00:26:28,040 --> 00:26:30,480 Speaker 4: we're going to have the sticky base load problem that 548 00:26:30,520 --> 00:26:32,840 Speaker 4: hopefully we can crack fusion in time. 549 00:26:32,680 --> 00:26:34,119 Speaker 2: To then a replace out. 550 00:26:34,240 --> 00:26:37,040 Speaker 4: So I think it's renewables now the infusion and infusion 551 00:26:37,040 --> 00:26:39,880 Speaker 4: will just make all the renewables we used originally obsolete. 552 00:26:40,400 --> 00:26:43,119 Speaker 3: The big question as of course, commercial viability. 553 00:26:43,720 --> 00:26:47,080 Speaker 1: Even if this experiment works out, will this become a 554 00:26:47,160 --> 00:26:48,200 Speaker 1: profitable company. 555 00:26:48,960 --> 00:26:52,399 Speaker 4: So the pathway that we see in building prototypes and 556 00:26:52,520 --> 00:26:55,159 Speaker 4: timelines is to get to that minimum viable products and 557 00:26:55,240 --> 00:26:58,760 Speaker 4: that's probably like an isotope generation machine rather than a 558 00:26:58,800 --> 00:27:01,560 Speaker 4: power plant that it's addressing a problem in a multi 559 00:27:01,600 --> 00:27:06,360 Speaker 4: billion dollar global market. You've got huge pharmaceutical companies trying 560 00:27:06,359 --> 00:27:09,240 Speaker 4: to find solutions in that space. And really what we 561 00:27:09,320 --> 00:27:11,520 Speaker 4: want to show is revenue into a company so that 562 00:27:11,560 --> 00:27:15,120 Speaker 4: you could potentially pay back investors. But more importantly, if 563 00:27:15,119 --> 00:27:17,680 Speaker 4: you're building a profitable business, you're not having money go out. 564 00:27:17,680 --> 00:27:19,920 Speaker 4: You're having money go in to allow you to continue 565 00:27:19,960 --> 00:27:21,439 Speaker 4: capitalizing and building on it. 566 00:27:21,880 --> 00:27:24,520 Speaker 2: I mean, Tiesla still sucks money in rather than paying 567 00:27:24,520 --> 00:27:24,760 Speaker 2: it out. 568 00:27:24,800 --> 00:27:28,239 Speaker 4: And they're a very large, successful business with a lot 569 00:27:28,240 --> 00:27:28,879 Speaker 4: of investments. 570 00:27:28,920 --> 00:27:31,960 Speaker 1: With a lot of investment, So what's the future for 571 00:27:32,080 --> 00:27:32,600 Speaker 1: open Star? 572 00:27:32,800 --> 00:27:36,840 Speaker 3: What valuation do you foresee for this business? A trillion 573 00:27:36,880 --> 00:27:38,400 Speaker 3: a billion? Like what are we looking. 574 00:27:38,160 --> 00:27:43,160 Speaker 4: At I think it's absolutely a trillion dollar market, right 575 00:27:43,240 --> 00:27:44,800 Speaker 4: and you do want to capture as much of it 576 00:27:44,920 --> 00:27:48,480 Speaker 4: as you can. Really, the way that I view it 577 00:27:48,680 --> 00:27:51,200 Speaker 4: is we have a problem to solve, and I think 578 00:27:51,320 --> 00:27:55,639 Speaker 4: free markets investment building companies is the best mechanism to 579 00:27:55,680 --> 00:27:58,119 Speaker 4: create a flywheel to make that happen, which means that 580 00:27:58,160 --> 00:27:59,479 Speaker 4: we need to have a commercial model and we need 581 00:27:59,480 --> 00:28:01,119 Speaker 4: to be able to show how we're going to get returns, 582 00:28:01,119 --> 00:28:02,840 Speaker 4: and we need to be pretty hard nosed about how 583 00:28:02,880 --> 00:28:03,240 Speaker 4: we're going. 584 00:28:03,160 --> 00:28:04,480 Speaker 2: To capture value. 585 00:28:05,119 --> 00:28:07,640 Speaker 4: But I don't think open Star will literally capture all 586 00:28:07,640 --> 00:28:10,520 Speaker 4: of it, and there's plenty to go around. I mean, 587 00:28:10,720 --> 00:28:13,800 Speaker 4: if you look at probably the best example is for 588 00:28:13,880 --> 00:28:18,520 Speaker 4: global hydrocarbon industry, right oil. There's trillions of dollars of 589 00:28:18,560 --> 00:28:22,600 Speaker 4: invested infrastructure that keeps our modern energy economy working, and 590 00:28:22,720 --> 00:28:24,800 Speaker 4: all of that needs to be replaced, I mean owned 591 00:28:24,840 --> 00:28:27,719 Speaker 4: by someone, maybe not one person, but hopefully a lot 592 00:28:27,760 --> 00:28:28,080 Speaker 4: of us. 593 00:28:28,880 --> 00:28:30,840 Speaker 2: But open Star wants to be a huge part of that. 594 00:28:31,119 --> 00:28:32,320 Speaker 3: I'm excited to watch you do it. 595 00:28:32,720 --> 00:28:33,480 Speaker 2: Thank you, thanks so. 596 00:28:33,440 --> 00:28:35,040 Speaker 1: Much having us Rouster appreciate it. 597 00:28:35,080 --> 00:28:35,439 Speaker 2: Cheeruz