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