WEBVTT - The Nuclear Tech Breakthrough That Could Make Oil Obsolete

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<v Speaker 1>So, like I said, the reactors pretty gold. So it

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<v Speaker 1>was commissioned inn and it was really commissioned because of

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<v Speaker 1>a scientist whose name was Glenn Seaboor. A few weeks

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<v Speaker 1>ago I made a trip to oak Ridge National Laboratory.

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<v Speaker 1>It's an eastern Tennessee nestled in beautiful green hills and

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<v Speaker 1>valleys down a long road flanked by forest. Some of

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<v Speaker 1>the things we're working on will not occur during my career.

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<v Speaker 1>How does that make you feel? It feels great. This

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<v Speaker 1>is Ellen Eisenhower. He's a former nuclear submarine officer and

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<v Speaker 1>now helps direct nuclear science research at the lab. The

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<v Speaker 1>research done here helped develop the atomic bomb, and its

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<v Speaker 1>scientists are still at it today, working toward a vision

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<v Speaker 1>that's a little bit hard to imagine. Right now. You've

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<v Speaker 1>probably heard the story the cathedral building story before. It's

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<v Speaker 1>about two workers laying brick on a cathedral that they'll

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<v Speaker 1>never see completed in their lifetimes. It's hard, repetitive work,

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<v Speaker 1>but one of them is always cheerful, saying that one day, thousands,

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<v Speaker 1>even millions of people will use what he's building today,

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<v Speaker 1>and he could get the vision for what even though

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<v Speaker 1>he knew he'd never see it he knew what he

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<v Speaker 1>was enabling for the future. Alan and his peers have

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<v Speaker 1>to think like this because what they're working on will

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<v Speaker 1>most likely never be fully realized in their careers, even

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<v Speaker 1>in their lifetimes, and when their cathedral is finally completed,

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<v Speaker 1>it will reshape the global economy and transform the power

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<v Speaker 1>dynamic between countries. And that is not an understatement. These

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<v Speaker 1>scientists are working on a new source for electricity. They're

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<v Speaker 1>trying to achieve nuclear fusion, essentially recreating the Sun on Earth.

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<v Speaker 1>M Hi, I'm Akito and I'm Jane caw and this

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<v Speaker 1>week on Decrypted work exploring just how close we are

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<v Speaker 1>to realizing the silver bullet for clean, cheap, abundant energy.

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<v Speaker 1>While nuclear power plants currently work by splitting atoms apart,

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<v Speaker 1>this is called nuclear fission, this other type of nuclear

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<v Speaker 1>energy works by smashing particles together, and that is called

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<v Speaker 1>nuclear fusion. Nuclear fusion has been a particularly hard nut

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<v Speaker 1>to crack. After decades of research, scientists are still years

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<v Speaker 1>away from building a commercially viable power plant, but scientists

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<v Speaker 1>say they're on the edge of a major breakthrough if

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<v Speaker 1>they can find a way to make a nuclear fusion

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<v Speaker 1>reaction take place. In a sustainable, controlled environment, the world's

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<v Speaker 1>energy needs would be taken care of, possibly forever. Stay

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<v Speaker 1>with us, okay, let's we're all signed in. I do.

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<v Speaker 1>We do have a couple of rules. Actually, I think

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<v Speaker 1>we can take photos today. So you wanted to take

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<v Speaker 1>a picture. Back at oak Ridge National Lab, I caught

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<v Speaker 1>up with Ned southof who oversees a big fusion project.

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<v Speaker 1>This this is not just you know, it's more efficient.

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<v Speaker 1>You know, this is ten million times more efficient. Okay,

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<v Speaker 1>So if we could make it work, it would change

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<v Speaker 1>the world that has piercing gray blue eyes and a

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<v Speaker 1>mop of floppy silver white hair. I spent almost three

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<v Speaker 1>hours with him and felt like we could have talked

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<v Speaker 1>for twenty more. Ned's in his sixties and has been

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<v Speaker 1>working on nuclear fusion since the nineteen seventies. He's still

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<v Speaker 1>an evangelist when it comes to the potential that this

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<v Speaker 1>technology has to solve the world's ever grow energy needs.

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<v Speaker 1>In sixteen, the world used more than thirty billion barrels

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<v Speaker 1>of oil, and more than eight of energy used for

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<v Speaker 1>things like powering homes came from fossil fuels, which are coal, oil,

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<v Speaker 1>and natural gas. Not only are these finite resources, but

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<v Speaker 1>The need for countries to maintain a steady supply has

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<v Speaker 1>sparked recessions, riots, and even wars around the world. Goddamn government,

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<v Speaker 1>he's gonna police this goddamn police situation. I will not

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<v Speaker 1>take the plan for this thing. I will not take

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<v Speaker 1>the crap and the harassment from these customers. Now let

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<v Speaker 1>him police it or stop telling gas anger and bewilderment

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<v Speaker 1>are growing. Is more and more Americans cope with gasoline

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<v Speaker 1>lines and empty pumps. Let himself experienced the turmoil the

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<v Speaker 1>follow the energy crisis of the nineteen seventies. I grew

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<v Speaker 1>up in the mid seventies when they add gas lines

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<v Speaker 1>because of the oil embargo. If we can solve this

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<v Speaker 1>challenging scientific problem, we can solve the world's energy problem forever.

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<v Speaker 1>That's how Ned turns to nuclear fusion, and decades later

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<v Speaker 1>he's still a true believer. So you go by a

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<v Speaker 1>typical power point. Did you know that to keep it

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<v Speaker 1>powered and cold takes roughly railroad cars of coal every

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<v Speaker 1>day to produce the same energy by fusion? Ready, three

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<v Speaker 1>pounds of tradium and two pounds of deuterium. Yeah, that's

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<v Speaker 1>a game change. Tridium deuterium. These are all parts of

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<v Speaker 1>nuclear fusion that will explain in just a moment. For now,

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<v Speaker 1>when that's trying to say is that if scientists can

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<v Speaker 1>make nuclear fusion work, will have found a source of

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<v Speaker 1>energy that comes with no carbon emissions, much less radioactive

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<v Speaker 1>waste than the nuclear reactors we have today, and most

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<v Speaker 1>importan hortuntly and almost unlimited supply of raw materials that

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<v Speaker 1>can be accessed basically anywhere. Okay, so let's explain how

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<v Speaker 1>it works. First, a quick review of the periodic table.

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<v Speaker 1>Remember that from high school chemistry, the first element is hydrogen.

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<v Speaker 1>It's the latest, simplest element in the universe, with one proton,

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<v Speaker 1>one electron, and usually one neutron. Hydrogen is also the

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<v Speaker 1>most abundant element in the universe, so unlike crude oil,

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<v Speaker 1>we won't be running out of it anytime soon. Protons

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<v Speaker 1>have a positive charge, electrons a corresponding negative charge, and

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<v Speaker 1>neutrons are well neutral. Protons and neutrons usually sit together

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<v Speaker 1>in the center of an atom, while electrons fly around

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<v Speaker 1>orbiting them. I mean, as you know, the Sun million

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<v Speaker 1>miles away produces power by transforming hydrogen into helium. Okay, well,

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<v Speaker 1>we want to do the same thing. Down here on Earth.

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<v Speaker 1>Nuclear fusion occurs naturally in stars, including our own Sun,

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<v Speaker 1>where hydrogen atoms are placed under extreme heat and pressure

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<v Speaker 1>two seventy four thousand times hotter than the human body

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<v Speaker 1>and pressure that's like being crushed under a mountain. These

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<v Speaker 1>conditions allows something extraordinary to happen. Normally, atoms would never

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<v Speaker 1>come close enough to fuse together right, but under the

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<v Speaker 1>intense conditions at the center of the Sun, the atomic

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<v Speaker 1>structure of the hydrogen starts to break down. The gas

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<v Speaker 1>turns into something called plasma, which enables the particles to

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<v Speaker 1>move faster and more freely because the positive particles, which

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<v Speaker 1>are the nuclei, things like deuterium and tridium, which normally

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<v Speaker 1>repel each other because they're both positive, can now get

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<v Speaker 1>close enough together, like ten to the minus twelve centimeters

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<v Speaker 1>that's a millions of a millions of a centimeter together,

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<v Speaker 1>Suddenly they stick. Deuterium and tritium, by the way, are

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<v Speaker 1>what's known as heavy hydrogen, basically hydrogen with extra neutrons.

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<v Speaker 1>They're the raw materials used in fusion reactions and can

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<v Speaker 1>be sucked out of sea water or produced in nuclear reactors,

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<v Speaker 1>and then they form this complene nucleus for a very

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<v Speaker 1>very short period of time, and then they break apart.

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<v Speaker 1>When that happens, a whole lot of energy is released,

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<v Speaker 1>mostly carried by the extra neutrons, super hot moving super quickly.

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<v Speaker 1>That energy is what we'd harness to make electricity. So

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<v Speaker 1>it's nuclear fusion reactions happening inside the Sun that make

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<v Speaker 1>it so hot. But those kinds of extreme conditions don't

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<v Speaker 1>exist anywhere on the surface of the Earth, not even

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<v Speaker 1>inside the molten lava of a volcano. The Sun's huge

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<v Speaker 1>mass creates a really strong gravitational force that keeps the

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<v Speaker 1>hot hydrogen from escaping. The Sun's gravity is twenty eight

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<v Speaker 1>times stronger than the Earth's. That means if you weighed

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<v Speaker 1>a hundred pounds, you'd feel like you weighed eight hundred

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<v Speaker 1>pounds on the Sun. This is a huge challenge for scientists.

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<v Speaker 1>How do you build a power plant that can resist

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<v Speaker 1>the pressure and the heat the reactor needs for these

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<v Speaker 1>fusions to start taking place On Earth, it needs to

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<v Speaker 1>be more than a hundred million degrees celsius inside the

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<v Speaker 1>reactor for fusion to occur, which is easier said than done.

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<v Speaker 1>Plasma is a very complex nonlinear system, and then we

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<v Speaker 1>had to learn how to understand it, and I'll control

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<v Speaker 1>how to control it. And so it took us a

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<v Speaker 1>few decades to really understand how do you control the plasma.

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<v Speaker 1>One of the most ostensively researched ways is using huge

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<v Speaker 1>and powerful magnets laid out in an arrangement called the tocomac.

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<v Speaker 1>Imagine this. The hydrogen plasma that's the super hot gas,

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<v Speaker 1>is contained within electro magnetic coils shaped like a donut.

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<v Speaker 1>More magnets surround the doughnut to give more control. The

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<v Speaker 1>leading configuration, the best demonstrated, the one that has the

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<v Speaker 1>most scientific and engineering basis, is the totomac. To give

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<v Speaker 1>you one example, the biggest fusion device functioning in Europe

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<v Speaker 1>right now, known as the jet, has a magnetic field

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<v Speaker 1>ten thousand times stronger than the Earth's magnetic field. The

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<v Speaker 1>larger the tocomac, the more powerful the magnetic fields, the

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<v Speaker 1>easier it is to get a fusion reaction going. In

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<v Speaker 1>the last sixty plus years, the world has built more

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<v Speaker 1>than two hundred of these machines, forty five or so

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<v Speaker 1>that are still functioning, but no experiment has been able

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<v Speaker 1>to sustain a fusion reaction long enough to produce more

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<v Speaker 1>energy than was required to get it going, which is

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<v Speaker 1>needed if we ever want to use fusion to generate electricity.

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<v Speaker 1>The exciting thing though, with how far science has progressed

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<v Speaker 1>and with today's technology, we're on the cusp of making

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<v Speaker 1>it happen. The scientific principles have been demonstrated and it's

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<v Speaker 1>a matter now of raising it to industrial scale. This

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<v Speaker 1>is reality. But of course moving this technology out of

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<v Speaker 1>the lab and raising it to an industrial scale involves

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<v Speaker 1>huge challenges. What those are and how the industry could

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<v Speaker 1>overcome them is coming up next. The story really starts

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<v Speaker 1>almost eighty years ago in the early nineties. Oakridge was

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<v Speaker 1>a secret town owned and operated by the US government.

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<v Speaker 1>It was a big part of the Manhattan Project. The

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<v Speaker 1>Manhattan Project was created in the middle of World War

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<v Speaker 1>Two to develop the ability to use nuclear fission as

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<v Speaker 1>a weapon. Okay, Germans discovered fish and right, we're worried

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<v Speaker 1>about this. That's Alison Hummel, who took me on a

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<v Speaker 1>tour of the historical sites at the oak Ridge Lab.

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<v Speaker 1>Back in scientists feared what the Germans could do with

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<v Speaker 1>the technology to split atoms. They even convinced a reluctant

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<v Speaker 1>star colleague to write a letter to the President about

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<v Speaker 1>the possibility fission reactions posed. This new phenomenon would also

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<v Speaker 1>lead to the construction of bombs. And it is conceivable,

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<v Speaker 1>though much less certain, that extremely powerful bombs of this

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<v Speaker 1>type may thus be constructed. A single bomb of this type,

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<v Speaker 1>carried by a boat and exploded into port, might very

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<v Speaker 1>well destroy the whole port, together with some of the

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<v Speaker 1>surrounding territory. Yours truly, Albert Einstein. By the end of

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<v Speaker 1>the war, there were eight people working here um, and

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<v Speaker 1>that was from the pretty much zero population in December

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<v Speaker 1>of nineteen. Their work was so secret that most of

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<v Speaker 1>them didn't even know what they were working on. I

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<v Speaker 1>have just returned from the White House where it has

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<v Speaker 1>just been announced that the United States is now using

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<v Speaker 1>an atomic bomb, the most powerful explosive yet. Then the

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<v Speaker 1>US dropped two atomic bombs on Japan, and the residents

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<v Speaker 1>finally learned the truth of what they were doing. Oakridge

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<v Speaker 1>had actually delivered the enriched uranium used in the first bomb.

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<v Speaker 1>The world will note that the first atomic bomb was

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<v Speaker 1>dropped on Hiroshima, a military base. We run the race

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<v Speaker 1>of discovery against the German After the war, the facility

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<v Speaker 1>has eventually became one part civilian research lab, which is

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<v Speaker 1>today's Oakridge National Lab, and one part military operations. Today

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<v Speaker 1>Oakridge is home to a group of scientists man is

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<v Speaker 1>by ned working on building the world's biggest pokomac, the

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<v Speaker 1>magnetic Donut reactor that we talked about earlier. They're the

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<v Speaker 1>U S arm of a multibillion dollar multidecade joint venture

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<v Speaker 1>in nuclear fusion between seven entities in the world, including

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<v Speaker 1>the US, European Union, China, and Russia. It's called the

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<v Speaker 1>International Thermonuclear Experimental Reactor or EATER for short. This thing

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<v Speaker 1>is expensive, estimated to cost tens of billions of dollars

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<v Speaker 1>to complete. It's too much and too complex for any

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<v Speaker 1>one country, so each of the seven participants has pledged

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<v Speaker 1>to fund and build portions of it. There is ever

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<v Speaker 1>growing confidence that either when operated, will achieve the plasma

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<v Speaker 1>that we predict, but it won't be completed until if

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<v Speaker 1>things go according to plan. That's when scientists are aiming

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<v Speaker 1>to get the reactor up and running and forming its

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<v Speaker 1>first fusion reactions. But while we're trying to focus on

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<v Speaker 1>RACK right now is to have a plasma where we

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<v Speaker 1>inject fifty million wants of power and we get out

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<v Speaker 1>million wats of fusion power. Most power plants that exist

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<v Speaker 1>today work the same way that they did a hundred

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<v Speaker 1>years ago. You heat water to make steam, and the

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<v Speaker 1>steam turns turbines, which generates electricity. The difference is in

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<v Speaker 1>what kind of fuel you're using to heat the water.

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<v Speaker 1>That fuel source it can be coal, oil, natural gas,

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<v Speaker 1>nuclear fission reactors, and hopefully one day, a nuclear fusion reactor.

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<v Speaker 1>When that happens, scientists believe that we will have found

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<v Speaker 1>the ultimate way to generate energy. That thinks that at

0:15:53.480 --> 0:15:56.480
<v Speaker 1>this point nuclear fusion is all but a sure thing.

0:15:56.880 --> 0:15:59.680
<v Speaker 1>It will work, we just have to build it, and

0:15:59.800 --> 0:16:02.880
<v Speaker 1>a lot of international scientists are pinning their hopes on

0:16:02.920 --> 0:16:06.960
<v Speaker 1>the EATER project. While there are maybe faster and cheaper

0:16:07.000 --> 0:16:10.360
<v Speaker 1>paths to fusion energy, Ned says that this is the

0:16:10.440 --> 0:16:15.960
<v Speaker 1>least risky. EATER is on the high reliability but high

0:16:16.040 --> 0:16:22.440
<v Speaker 1>cost end of the spectrum. Okay, but there's one huge problem.

0:16:22.480 --> 0:16:26.360
<v Speaker 1>At this moment. The fusion program was limited by money.

0:16:27.680 --> 0:16:30.760
<v Speaker 1>It suffers from the same same thing that all advanced

0:16:30.840 --> 0:16:36.920
<v Speaker 1>energy research suffers. Advanced energy research is not a priority.

0:16:37.280 --> 0:16:40.400
<v Speaker 1>Ned tells me that when you look at adjusted dollars.

0:16:40.760 --> 0:16:44.240
<v Speaker 1>US funding for fusion peeked in the late seventies and

0:16:44.320 --> 0:16:48.160
<v Speaker 1>early eighties after the oil shocks. Well I was working

0:16:48.240 --> 0:16:52.960
<v Speaker 1>on on a series of devices. I was actually at

0:16:53.000 --> 0:16:56.800
<v Speaker 1>that point running US a collaboration on a variety of

0:16:56.840 --> 0:17:02.480
<v Speaker 1>devices around the world, and what we saw was that

0:17:03.160 --> 0:17:06.719
<v Speaker 1>we had many, many ideas that we could not afford

0:17:06.760 --> 0:17:10.520
<v Speaker 1>to follow up on. It doesn't help that most of

0:17:10.600 --> 0:17:14.840
<v Speaker 1>us non scientists don't really understand how nuclear technology works.

0:17:15.520 --> 0:17:19.440
<v Speaker 1>Throughout history, there have been some major accidents involving nuclear

0:17:19.480 --> 0:17:23.960
<v Speaker 1>reactor meltdowns. A year after these reactors at the Fukushima

0:17:24.040 --> 0:17:29.960
<v Speaker 1>Nuclear plant exploded in a triple meltdown, reporters were reminded

0:17:30.000 --> 0:17:32.719
<v Speaker 1>this is still one of the most hazardous places on

0:17:32.760 --> 0:17:36.160
<v Speaker 1>the plants. One of the atomic reactors at the Churnibyl

0:17:36.200 --> 0:17:38.840
<v Speaker 1>Atomic Power plant in the city of Kiev was damaged

0:17:39.280 --> 0:17:41.959
<v Speaker 1>and there is speculation in Moscow that people were injured

0:17:42.000 --> 0:17:45.240
<v Speaker 1>and may have died. Experts tonight say that cloud of

0:17:45.359 --> 0:17:48.600
<v Speaker 1>radiation is now dissipating over the North Atlantic and poses

0:17:48.640 --> 0:17:51.440
<v Speaker 1>no further threat to anyone, But as the Soviets treat

0:17:51.480 --> 0:17:54.359
<v Speaker 1>an unknown number of casualties, there's no way to say

0:17:54.359 --> 0:17:57.920
<v Speaker 1>how much lasting damage that cloud may have already caused.

0:17:58.520 --> 0:18:02.800
<v Speaker 1>Dean Reynolds, ABC News London. It's important to note that

0:18:02.840 --> 0:18:07.720
<v Speaker 1>the big nuclear disasters like Fukushima or churnobil involved a

0:18:07.760 --> 0:18:12.080
<v Speaker 1>different process altogether, where atoms are being split apart inside

0:18:12.080 --> 0:18:16.240
<v Speaker 1>the reactor instead of being fused together. That's the difference

0:18:16.280 --> 0:18:21.479
<v Speaker 1>between nuclear fission and nuclear fusion. Here's Alan again, and

0:18:21.480 --> 0:18:27.399
<v Speaker 1>there's a lot of hyperbole about it that has played

0:18:27.440 --> 0:18:32.360
<v Speaker 1>out over the years that we have not been effective

0:18:33.840 --> 0:18:40.600
<v Speaker 1>at at countering, which is unfortunate. The damage to public

0:18:40.680 --> 0:18:44.359
<v Speaker 1>perception is hard to erase, and it doesn't help nuclear's

0:18:44.400 --> 0:18:47.720
<v Speaker 1>case that the US still has plenty of hydrocarbons, which

0:18:47.760 --> 0:18:50.879
<v Speaker 1>is oil, gas and coal. In two thousand and eight,

0:18:51.119 --> 0:18:53.920
<v Speaker 1>the US Eater Project was hoping to get a hundred

0:18:53.960 --> 0:18:58.159
<v Speaker 1>sixty million dollars in funding for the following year. I

0:18:58.320 --> 0:19:06.240
<v Speaker 1>was actually driving to Florida for Christmas vacations and pulled

0:19:06.320 --> 0:19:08.520
<v Speaker 1>up in the driveway of my parents house and I

0:19:08.600 --> 0:19:13.119
<v Speaker 1>got a phone call and it was they just passed

0:19:13.119 --> 0:19:16.440
<v Speaker 1>in appropriation for ten point six instead of one sixty.

0:19:18.240 --> 0:19:21.120
<v Speaker 1>Ned got less than ten of the funding that they

0:19:21.119 --> 0:19:24.640
<v Speaker 1>had asked for. The team had to toss the original

0:19:24.680 --> 0:19:28.120
<v Speaker 1>plan out the window. There was some restructuring. The main

0:19:28.160 --> 0:19:30.680
<v Speaker 1>thing was to not spend all the money they had

0:19:31.320 --> 0:19:36.679
<v Speaker 1>or it was game over. So that particular year, the

0:19:36.800 --> 0:19:39.520
<v Speaker 1>strategy was lived to fight the battle the next year.

0:19:41.040 --> 0:19:43.640
<v Speaker 1>We knew we couldn't do what we intended to do

0:19:43.720 --> 0:19:47.280
<v Speaker 1>that year, but we had to try to preserve the

0:19:47.320 --> 0:19:51.399
<v Speaker 1>capability to rebound. That was smack dab in the middle

0:19:51.440 --> 0:19:56.040
<v Speaker 1>of the global financial crisis. Other countries also pulled back funding.

0:19:56.600 --> 0:19:59.919
<v Speaker 1>Ned told me, that's at Eaters timeline back five years.

0:20:00.440 --> 0:20:03.760
<v Speaker 1>In November of last year, Ned and his team presented

0:20:03.800 --> 0:20:06.000
<v Speaker 1>a budget that laid out how much money they would

0:20:06.080 --> 0:20:10.040
<v Speaker 1>need to complete Eaters construction and achieved the first fusion

0:20:10.119 --> 0:20:14.840
<v Speaker 1>reaction in At this point, the US has already spent

0:20:14.880 --> 0:20:18.360
<v Speaker 1>about a billion dollars, with more than three billion dollars

0:20:18.359 --> 0:20:22.639
<v Speaker 1>to go to see it through. For seventeen, Ned requested

0:20:22.680 --> 0:20:25.800
<v Speaker 1>a hundred million dollars. You know, we just got a

0:20:25.880 --> 0:20:29.800
<v Speaker 1>seventeen budget, and they just passed a budget in April, okay,

0:20:31.119 --> 0:20:36.280
<v Speaker 1>and it was complicated. Essentially, they were given fifty million dollars,

0:20:36.280 --> 0:20:39.240
<v Speaker 1>but the Department of Energy has the options at another

0:20:39.320 --> 0:20:44.359
<v Speaker 1>fifty million. Today we've not received the second fifty. Okay,

0:20:44.440 --> 0:20:48.679
<v Speaker 1>so so we're positioning ourselves to survive at the fifty

0:20:48.800 --> 0:20:52.840
<v Speaker 1>level for fiscal year eighteen. The situation is also dire.

0:20:53.359 --> 0:20:56.920
<v Speaker 1>President Trump, who made fossil fuels and especially cole a

0:20:57.040 --> 0:21:00.960
<v Speaker 1>focus of his administration, has only approved about half of

0:21:01.000 --> 0:21:04.359
<v Speaker 1>what NET has requested, and now we're being impacted because

0:21:04.400 --> 0:21:07.240
<v Speaker 1>we're not getting the money, and so we are now

0:21:07.280 --> 0:21:12.240
<v Speaker 1>struggling to try to stay with Getting us here has

0:21:12.280 --> 0:21:16.320
<v Speaker 1>taken decades. Every element we just described took years of

0:21:16.359 --> 0:21:20.240
<v Speaker 1>dedicated research to just understand, and then many more years

0:21:20.280 --> 0:21:23.040
<v Speaker 1>to move past the theory and come up with actual

0:21:23.160 --> 0:21:26.879
<v Speaker 1>experiment results. Just getting Eater up and running won't be

0:21:27.040 --> 0:21:29.040
<v Speaker 1>enough to get us to the stage where we can

0:21:29.160 --> 0:21:33.320
<v Speaker 1>use fusion to generate electricity. The real question is, in

0:21:33.359 --> 0:21:36.320
<v Speaker 1>the next generation and a frill fusion reactor, what would

0:21:36.320 --> 0:21:38.840
<v Speaker 1>you build it out? And if you were to use

0:21:38.920 --> 0:21:41.680
<v Speaker 1>the search of things we're using on Eater, it would

0:21:41.720 --> 0:21:47.960
<v Speaker 1>turn to a powder. You know, when Ned says it

0:21:48.000 --> 0:21:51.320
<v Speaker 1>would turn into powder, he means that the materials that

0:21:51.400 --> 0:21:55.440
<v Speaker 1>exists today can't handle the kinds of harsh conditions fusion

0:21:55.560 --> 0:21:58.960
<v Speaker 1>requires over a long period of time. But a power

0:21:59.000 --> 0:22:01.639
<v Speaker 1>plant that uses usion will need to be running the

0:22:01.720 --> 0:22:04.800
<v Speaker 1>reactions constantly and for many months at a time to

0:22:04.840 --> 0:22:10.040
<v Speaker 1>make economic sense. You would chew up the material completely

0:22:10.040 --> 0:22:13.159
<v Speaker 1>and suddenly if you don't do anything about it. You

0:22:13.280 --> 0:22:17.679
<v Speaker 1>know you can reach the lifetime of thecal material within

0:22:18.280 --> 0:22:21.920
<v Speaker 1>a few days to a week. That's you're gonna wrap

0:22:21.960 --> 0:22:25.639
<v Speaker 1>a plasma. Physicist at oak Ridge National Lab, he and

0:22:25.680 --> 0:22:28.399
<v Speaker 1>Allen are working on a bunch of other things that

0:22:28.440 --> 0:22:32.080
<v Speaker 1>will be necessary to make a commercial fusion power plant work.

0:22:32.680 --> 0:22:35.840
<v Speaker 1>If you're going to have a successful power plant, it's

0:22:35.880 --> 0:22:38.320
<v Speaker 1>more than this plasma. You have to be able to

0:22:38.359 --> 0:22:40.199
<v Speaker 1>fuel it, you have to be able to extract the

0:22:40.200 --> 0:22:42.360
<v Speaker 1>heat from it. You have to have materials that can

0:22:42.400 --> 0:22:47.080
<v Speaker 1>withstand that type of environment. The best way is to

0:22:47.160 --> 0:22:52.560
<v Speaker 1>do start this development now instead of waiting until Eater

0:22:52.960 --> 0:22:56.160
<v Speaker 1>has produced its burning plasma and then we start only

0:22:56.200 --> 0:22:58.840
<v Speaker 1>developing the materials. We know that we have to develop

0:22:58.880 --> 0:23:03.359
<v Speaker 1>new maters. Innovating on these elements all require funding and

0:23:03.400 --> 0:23:07.280
<v Speaker 1>even new facilities, But like NED, they're also held back

0:23:07.359 --> 0:23:13.359
<v Speaker 1>by money. Although we build more community beyond it, is

0:23:13.359 --> 0:23:18.560
<v Speaker 1>it enough. You know, under the budget constraints, I do

0:23:18.640 --> 0:23:21.280
<v Speaker 1>not want to make a firm prediction, because it's also

0:23:21.320 --> 0:23:24.960
<v Speaker 1>out of my hands. We are ready, I would say,

0:23:25.000 --> 0:23:29.200
<v Speaker 1>we are ready, I hope so that the people in

0:23:29.280 --> 0:23:34.480
<v Speaker 1>Washington already to for now. All the uncertainty around funding,

0:23:34.800 --> 0:23:38.359
<v Speaker 1>combined with all the false starts throughout history, has made

0:23:38.560 --> 0:23:41.720
<v Speaker 1>most of these scientists hesitant to offer a timeline for

0:23:41.760 --> 0:23:45.159
<v Speaker 1>when the fusion power plant will be a reality. I

0:23:45.200 --> 0:23:49.320
<v Speaker 1>won't speculate on the exact time frame because many haven't.

0:23:49.359 --> 0:23:55.679
<v Speaker 1>Many have been wrong over and over again. Right, only

0:23:55.800 --> 0:23:59.960
<v Speaker 1>Ned would entertain that question. Looking at either if all

0:24:00.000 --> 0:24:02.800
<v Speaker 1>goes to plan, he estimates that we might get a

0:24:02.880 --> 0:24:08.520
<v Speaker 1>working fusion power plant around by which point Ned would

0:24:08.560 --> 0:24:13.040
<v Speaker 1>be a hundred and one years old. I I truly hope.

0:24:13.080 --> 0:24:17.280
<v Speaker 1>I mean I realized this that this endeavored to make

0:24:17.440 --> 0:24:24.879
<v Speaker 1>fusion energy a reality takes many generations. And I'm not

0:24:25.160 --> 0:24:29.560
<v Speaker 1>somebody who is discouraged by it. Um and some people

0:24:29.600 --> 0:24:31.640
<v Speaker 1>make fun of them. Maybe it's because I come from

0:24:31.640 --> 0:24:34.240
<v Speaker 1>Europe and I come from Cologne, and the Cologne Cathedra

0:24:34.440 --> 0:24:39.159
<v Speaker 1>was built over eight hundred years, you know, so so

0:24:39.720 --> 0:24:42.480
<v Speaker 1>you know it is it is worth while to wait

0:24:42.560 --> 0:24:59.720
<v Speaker 1>for it. And that's it for this week's episode of

0:24:59.720 --> 0:25:02.679
<v Speaker 1>The Did Thanks for listening. We want to know what

0:25:02.720 --> 0:25:05.439
<v Speaker 1>you think of this episode. Record a voice message and

0:25:05.480 --> 0:25:09.520
<v Speaker 1>send it to Decrypted at Bloomberg dot net. Also, you

0:25:09.520 --> 0:25:12.560
<v Speaker 1>can find me on Twitter at jingle bells cow and

0:25:12.640 --> 0:25:15.919
<v Speaker 1>I've met aki Eto seven. If you haven't already subscribed

0:25:15.960 --> 0:25:19.320
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0:25:19.320 --> 0:25:21.840
<v Speaker 1>you're there, please leave us a rating and a review.

0:25:22.200 --> 0:25:26.160
<v Speaker 1>This really helps more listeners find our show. This episode

0:25:26.240 --> 0:25:30.879
<v Speaker 1>was produced by Pia Ga Kari, Liz Smith, and Magnus Henrikson.

0:25:31.280 --> 0:25:34.320
<v Speaker 1>Thanks to Nico Grant and Isabel Gottlieb for their help

0:25:34.320 --> 0:25:37.840
<v Speaker 1>with the show. Alec McCabe is head of Bloomberg Podcast.

0:25:38.119 --> 0:25:39.120
<v Speaker 1>We'll see you next week.