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[narrator] Join us
on Tomorrow's World Today
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00:00:02,503 --> 00:00:05,337
as we journey through
the worlds of inspiration,
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00:00:05,339 --> 00:00:08,507
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 the final part
of our four-part exploration,
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we explore how nuclear energy
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is helping
with space exploration.
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We close with a round table
conversation
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with some of nuclear energy's
top minds
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00:00:25,126 --> 00:00:27,326
to discuss what
nuclear energy looks like
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in tomorrow's world.
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Hi everyone.
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Welcome to episode four
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of our four-part exploration
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on nuclear energy.
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Now, in the previous
three episodes,
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we learned
about the past, present,
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and future of nuclear power
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including how microreactors
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are bringing energy
to some of the most remote
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and hardest to power locations
on earth.
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But today, we are heading
out of this world.
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That's right, we're gonna
learn about nuclear energy
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and space exploration,
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specifically nuclear propulsion
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and power.
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Now, we're gonna start
right here in DC.
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We're gonna head over
to X-energy
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and learn about fuels
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and next generation reactors.
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Then, we're gonna head
back out to Idaho
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to learn how nuclear energy
is powering
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the Mars Perseverance Rover.
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Right now, let's head over
and meet Clay Sell,
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he's the CEO of X-energy.
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- Hey, Clay.
- Hey, Greg.
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- Welcome.
- Oh, thanks for having me.
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I'm so excited to be here today.
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I'm super excited to learn
what it is you guys do here.
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Well, we're a nuclear reactor
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and fuel design
engineering company.
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Great. Now, I know
that you're also doing
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some really innovative things
with fuel
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for space travel and such.
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We'll learn about that
in a little bit
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but right now,
tell me about this reactor.
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Well, we are first focused
on applications
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for this earth, this planet,
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and this is our standard
utility model.
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This is the reactor,
it's about 25 meters tall.
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It's filled with uranium fuel
and it produces heat.
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The heat then goes
to the steam generator
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where it's turned into steam,
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and that steam spins
a turbine generator
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to produce electricity
for about 80,000
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- American homes.
- That is awesome.
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Now, space travel
and nuclear power,
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not usually something
that people think of
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at the same time, you know,
reactors are big and heavy
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and, you know, in space travel,
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you need light and compact,
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but I know
that you're really doing
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some really advanced stuff
with fuel
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and I'd like
to find out more about that.
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We're doing some
amazing things with fuel.
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Let me take you next door
and show you.
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Lead the way.
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So Clay,
I know that one of the areas
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where you're making real
innovations
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is in nuclear fuel and TRISO-X
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is what's happening right now.
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So, explain to me how we're...
What we're looking at?
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Well, the most important thing
about this fuel
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is we've designed it
and engineered it
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so it cannot melt
in any scenario
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inside the reactor.
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And that's one of the key
safety attributes
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that are central
to the reactor design.
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Let me tell you how we do it.
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So, we start
with the uranium chemistry,
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in this case,
it's uranium-enriched
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to fifteen and a half percent.
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This little kernel is about
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half a millimeter in diameter.
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And then, we have a process
by we coat it four times
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in various types
of ceramic material.
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So, you end up with a little
containment vessel
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about the size of a poppy seed
and this containment vessel
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during the life of the uranium,
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when it burns up,
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it will contain 99.999%
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of all the waste produced
burnt during burn up.
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So it makes
for a very robust fuel,
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it makes for an incredibly
safe fuel.
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It makes for a fuel
that cannot melt down.
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And then, we take 19,000
of these kernels
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and we put it into a fuel form,
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we evenly space them out,
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they're evenly dispersed,
we can measure that
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and we put
a graphite rayon on it,
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and then, this is the fuel form
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that actually goes
into the reactor.
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So it can't melt and you're also
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containing the nuclear waste.
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That's true.
And you know what's exciting?
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This single pebble
has enough energy in it
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to power an electric vehicle
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- almost 100,000 miles.
- Wow.
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Which would take you
around the earth four times.
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That's amazing.
You're ready to go?
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- Let's do it.
- So, say we're not fueling up
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the family station wagon
with this thing.
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We're using it
in one of your reactors.
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- Tell me how that works.
- Well, we would take
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220,000 of these.
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We would load them
into the reactor core barrel,
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just like gumballs
in a gumball machine.
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We would pull
the control rods out
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and that would start
the nuclear chain reaction
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which produces heat.
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That heat would be transferred
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from the reactor core barrel
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to the steam generator
with helium,
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that's our heat-transfer fluid.
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This pebble
would work its way down
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through the core barrel
for about six months
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and then it would get
to the bottom
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where we have a burn up
measurement system
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to see if there's
still fuel in it.
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If there's still
good fuel in it,
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it goes back to the top
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and will take
another six-month trip
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through the core barrel.
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A typical fuel pebble like this
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2in our design
will take six trips
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through the reactor core barrel.
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And at the end
of those six trips,
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you have essentially
an empty vessel
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but anything that is
and still in there
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is gonna be contained
right within that pebble.
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Well, almost all of the usable
special nuclear material
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has been burned up,
so that's a huge benefit.
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This ceramic
and graphite fuel form
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retains all
of the long-lived waste
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that has been produced
during the burn up.
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So, this great,
beautiful fuel form
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actually becomes
a spectacular waste form
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because this thing
will last forever
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and it will keep
all of the waste in here
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for tens of thousands of years.
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Excellent. So, how would you
control a reactor like this?
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Greg, do you like to play
video games?
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- A lot.
- Then you need to see
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our reactor room
simulator mock up.
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- Let me show you.
- Lead the way.
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[mellow music playing]
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Greg, let me introduce you
to Yvotte Brits.
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Greg, welcome.
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Oh, great to meet you, Yvotte.
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Thanks Clay.
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Well Yvotte, I mean,
it goes without saying
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that this looks like
the arcade room of my dreams,
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but I know that it's a lot
more than that.
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This is an actual
graphic representation
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of the reactor that Clay and I
were just discussing.
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[Yvotte] Yes, Greg.
This is very exciting.
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This is the toolset
that we are using
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to train our operators.
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We have a single
control room to operate
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four reactors, four turbines
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for a total of three operators
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in the control room.
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The control room
is also modular,
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we can add more reactor units
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as the client wants more.
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On the screen here, you will see
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we have a nuclear island
and a conventional island.
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The nuclear island
stays consistent
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no matter what the client wants
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- on the conventional island.
- So the client can determine
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if they want steam
or electricity
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or co-generation,
they'd get to pick that.
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- Yes Greg, that is correct.
- That's cool.
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Let me show you the toolset
that we are using
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for the maintenance and
for the security personnel.
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In the absence of a real plant,
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we are relying
on 3D virtual reality models
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to train up our maintenance
and security personnel.
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So, please put on
the virtual reality goggles.
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Oh, I have been
looking forward to this.
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Greg, so what you see
in front of you is the reactor
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coupled to the steam generator
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and of the fuel handling system
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doing the online refilling.
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That's amazing. You can see...
Even see the pebbles
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going through the system
and these are the fuel pebbles
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that Clay and I
discussed earlier.
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[Yvotte] Yes, that is correct.
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That is absolutely awesome,
Yvotte.
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- Hey, Clay.
- Hey, Greg.
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- So, what do you think?
- Well, I think
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this is all pretty amazing but
what I really want to know now
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is how you're gonna take all
of this terrestrial technology
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and send it up into space?
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Well, the great thing about it
is the same fuel
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and the same engineers
that have been
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so successful here on earth
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are perfectly suited
for space applications.
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- Let me explain it to you.
- Sounds great.
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- Yvotte, thank you very much.
- Thanks. Great to meet you.
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Hey Greg, do you have any idea
how long it takes
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to take a rocket to Mars?
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Well, from everything I've read,
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00:08:03,383 --> 00:08:04,983
between six and nine months.
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That's right.
And what's exciting
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00:08:06,987 --> 00:08:09,087
with the technology
we've developed here,
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a version of that
can be used to build
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00:08:11,124 --> 00:08:13,425
a thermal nuclear
propulsion system
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that will shorten that trip
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- to half the time.
- That's amazing.
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00:08:17,564 --> 00:08:20,532
It's really important
for astronauts,
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they're exposed
to tremendous cosmic radiation
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during that contemplated
long trip to Mars,
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and if we can shorten
that trip, cut it in half,
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00:08:28,442 --> 00:08:30,175
that has a huge benefit
for the astronauts.
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Right. That's one
of those things that folks
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don't really consider
'coz they think,
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well, there's space stations
up there
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for years and years and years,
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but there's space,
and then, there's outer space.
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And you know the space stations
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actually still contain within
the earth's magnetosphere
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so it's protected from all
of that cosmic radiation.
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But once you get beyond that,
all bets are off.
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00:08:47,127 --> 00:08:49,094
Yeah.
Let me tell about something
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that we're working on
that's one step further out
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00:08:51,265 --> 00:08:53,832
and that is a permanent
installation
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00:08:53,834 --> 00:08:55,267
on the lunar surface.
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00:08:55,269 --> 00:08:57,769
It's something that's really
being talked about a lot.
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00:08:57,771 --> 00:09:00,438
We're talking about humans
on the surface of the moon
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00:09:00,440 --> 00:09:03,308
for long periods of time
and they need a power source.
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00:09:03,310 --> 00:09:07,178
But with the lunar night,
which lasts 14 earth days,
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00:09:07,180 --> 00:09:09,347
they need something better
than solar arrays
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00:09:09,349 --> 00:09:11,850
and batteries to survive
the lunar night.
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00:09:11,852 --> 00:09:15,754
And that's where a nuclear
fission surface power system
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00:09:15,756 --> 00:09:17,923
that applies a lot
of the same principles
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00:09:17,925 --> 00:09:20,158
that we've developed here
on earth
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00:09:20,160 --> 00:09:22,193
is being developed for the moon.
250
00:09:22,195 --> 00:09:24,029
So, that's gonna get us
to the moon,
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00:09:24,031 --> 00:09:26,131
get us to Mars,
and then even beyond.
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00:09:26,133 --> 00:09:28,033
That's true. And again,
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00:09:28,035 --> 00:09:29,968
it relates to a lot
of the technology
254
00:09:29,970 --> 00:09:30,969
we developed here.
255
00:09:30,971 --> 00:09:32,737
From our fuel form
256
00:09:32,739 --> 00:09:35,140
which is, you know,
ceramic encapsulated
257
00:09:35,142 --> 00:09:37,275
can achieve
very high temperatures,
258
00:09:37,277 --> 00:09:40,045
has very long life,
that's important.
259
00:09:40,047 --> 00:09:42,080
The instrumentation
and control system
260
00:09:42,082 --> 00:09:44,215
that we've developed
for our reactors here
261
00:09:44,217 --> 00:09:45,917
will be necessary on the moon.
262
00:09:45,919 --> 00:09:48,486
A lot of the materials
that were produced
263
00:09:48,488 --> 00:09:50,422
to achieve
very high temperatures
264
00:09:50,424 --> 00:09:52,357
will be necessary
to that nuclear
265
00:09:52,359 --> 00:09:54,092
thermal propulsion system
266
00:09:54,094 --> 00:09:56,161
and many other
of the technologies
267
00:09:56,163 --> 00:09:59,230
that we're developing
are directly applicable
268
00:09:59,232 --> 00:10:01,900
- to nuclear space application.
- Even this control room?
269
00:10:01,902 --> 00:10:03,768
- Even this control room.
- All right.
270
00:10:03,770 --> 00:10:05,604
Well, I know that there's
nuclear power right now
271
00:10:05,606 --> 00:10:07,072
on the surface of Mars
272
00:10:07,074 --> 00:10:08,473
powering the Perseverance Rover
273
00:10:08,475 --> 00:10:10,075
and I'm heading out
to Idaho Falls
274
00:10:10,077 --> 00:10:11,776
to find out all about that.
275
00:10:11,778 --> 00:10:13,411
Well, thanks so much
for being here.
276
00:10:13,413 --> 00:10:15,280
- Have a great trip to Idaho.
- Thank you, Clay.
277
00:10:15,282 --> 00:10:16,481
This has been amazing.
278
00:10:19,385 --> 00:10:21,186
Now, if you've ever blown up
a balloon
279
00:10:21,188 --> 00:10:22,554
and then the air out
and watched it
280
00:10:22,556 --> 00:10:25,090
whizz around the room,
that's a similar concept
281
00:10:25,092 --> 00:10:26,925
to nuclear thermal propulsion.
282
00:10:26,927 --> 00:10:29,260
Now, nuclear thermal
propulsion rockets
283
00:10:29,262 --> 00:10:32,330
use a nuclear reaction
to heat up liquid hydrogen.
284
00:10:32,332 --> 00:10:34,599
Once that hydrogen
is heated up, it expands,
285
00:10:34,601 --> 00:10:36,101
then it's forced
through a nozzle
286
00:10:36,103 --> 00:10:37,836
and that produces thrust.
287
00:10:37,838 --> 00:10:39,871
I'm at the Idaho
National Laboratory
288
00:10:39,873 --> 00:10:41,973
Space & Security
Power Systems Facility.
289
00:10:41,975 --> 00:10:43,608
I'm gonna talk to Steve Johnson
290
00:10:43,610 --> 00:10:45,644
and we're gonna learn
how nuclear propulsion
291
00:10:45,646 --> 00:10:48,346
is going to help get humans
to Mars faster.
292
00:10:57,089 --> 00:10:58,289
- Hey, Steve.
- Hey, Greg.
293
00:10:58,291 --> 00:11:00,058
- Welcome to Idaho.
- Thanks for having me.
294
00:11:00,060 --> 00:11:01,826
I'll tell you,
your work with NASA
295
00:11:01,828 --> 00:11:03,228
and the Mars Perseverance Rover,
296
00:11:03,230 --> 00:11:04,496
it really couldn't be
more exciting,
297
00:11:04,498 --> 00:11:05,964
so please tell me more about it.
298
00:11:05,966 --> 00:11:07,866
All right. Let's take a look
at this selfie
299
00:11:07,868 --> 00:11:09,300
taken by the Perseverance Rover.
300
00:11:09,302 --> 00:11:11,770
You can see
our power system here,
301
00:11:11,772 --> 00:11:14,472
you can the ingenuity
helicopter here,
302
00:11:15,007 --> 00:11:16,508
and you can see
303
00:11:16,510 --> 00:11:19,344
with this 3D model
behind us here,
304
00:11:19,346 --> 00:11:21,279
you can see the thermoelectrics
305
00:11:21,281 --> 00:11:23,782
which turn the heat
from the heat sources inside
306
00:11:23,784 --> 00:11:25,216
into electrical power.
307
00:11:25,218 --> 00:11:26,551
It's 2 feet in diameter,
308
00:11:26,553 --> 00:11:29,220
it's 2 feet tall,
it weighs about 100 pounds...
309
00:11:29,222 --> 00:11:32,223
Well, 110 to 120 watts electric.
310
00:11:32,225 --> 00:11:36,761
Similar to the Curiosity Rover
that landed in 2012,
311
00:11:36,763 --> 00:11:40,398
they last for several years
in terms of the power system
312
00:11:40,400 --> 00:11:43,168
and it's a great way
to get around Mars.
313
00:11:43,170 --> 00:11:45,837
We have the acceptance
testing facilities here
314
00:11:45,839 --> 00:11:47,305
and fueling facilities.
315
00:11:47,307 --> 00:11:48,373
I'd really like
to show this to you.
316
00:11:48,375 --> 00:11:49,541
Do you have time for that?
317
00:11:49,543 --> 00:11:51,176
- Absolutely.
- All right. Let's go.
318
00:11:51,178 --> 00:11:54,512
[mellow music playing]
319
00:12:05,324 --> 00:12:07,726
[mellow music playing]
320
00:12:19,839 --> 00:12:21,573
So Steve,
this is where you would
321
00:12:21,575 --> 00:12:24,409
actually put the fuel source
for the rover together?
322
00:12:24,411 --> 00:12:26,544
Yes, Greg.
This is where we take
323
00:12:26,546 --> 00:12:29,180
the general-purpose
heat source modules,
324
00:12:29,182 --> 00:12:31,883
we stack up a total
of eight of these
325
00:12:31,885 --> 00:12:34,953
inside the glove box
326
00:12:34,955 --> 00:12:38,156
and each of those has four
of these heat sources in it.
327
00:12:38,158 --> 00:12:41,292
And we will stack them up
in the specialized fixture
328
00:12:41,294 --> 00:12:43,061
and pick them up with this tool,
329
00:12:43,063 --> 00:12:45,563
put them down
inside the power system,
330
00:12:45,565 --> 00:12:47,766
that's a multi-mission
radioisotope
331
00:12:47,768 --> 00:12:49,200
thermoelectric generator
332
00:12:49,202 --> 00:12:51,436
or MMRTG for short.
333
00:12:51,438 --> 00:12:54,339
This operation takes about
three weeks.
334
00:12:54,341 --> 00:12:56,207
Most of it is prep time
and everything
335
00:12:56,209 --> 00:12:58,209
but there's a couple
or three days
336
00:12:58,211 --> 00:12:59,477
of exciting stuff in the middle.
337
00:12:59,479 --> 00:13:02,947
Once it comes out of here,
it's a fully functioning RTG.
338
00:13:02,949 --> 00:13:05,183
It needs to go through
acceptance testing
339
00:13:05,185 --> 00:13:08,853
which is vibrational testing,
center of mass testing,
340
00:13:08,855 --> 00:13:13,158
magnetic field testing,
and the vacuum testing.
341
00:13:13,160 --> 00:13:14,592
The first thing
we do out of here
342
00:13:14,594 --> 00:13:16,361
is the vibrational testing.
343
00:13:16,363 --> 00:13:17,896
Would you like to take
a look at that?
344
00:13:17,898 --> 00:13:19,230
Absolutely. Let's go see it.
345
00:13:19,232 --> 00:13:20,298
Follow me.
346
00:13:23,502 --> 00:13:25,069
So Steve,
347
00:13:25,071 --> 00:13:27,105
I know that all elements
of testing in this
348
00:13:27,107 --> 00:13:29,340
have to be vitally important
but I can't imagine
349
00:13:29,342 --> 00:13:31,142
that there's a better
opportunity for something
350
00:13:31,144 --> 00:13:32,977
to go wrong
than during a launch.
351
00:13:32,979 --> 00:13:34,479
You're absolutely right, Greg.
352
00:13:34,481 --> 00:13:37,182
So, that's why we place
a lot of emphasis
353
00:13:37,184 --> 00:13:38,750
on vibrational testing.
354
00:13:38,752 --> 00:13:40,752
We do it on all three axes.
355
00:13:40,754 --> 00:13:42,587
This is the horizontal
flip table.
356
00:13:42,589 --> 00:13:44,923
We will mount the MMRTG on here.
357
00:13:44,925 --> 00:13:47,826
Our vibrator head here
will then agitate
358
00:13:47,828 --> 00:13:49,027
in the X direction.
359
00:13:49,029 --> 00:13:52,497
We'll rotate
the MMRTG ninety degrees,
360
00:13:52,499 --> 00:13:54,933
we'll call that Y agitation.
361
00:13:54,935 --> 00:13:56,601
And then we can decouple it
362
00:13:56,603 --> 00:13:58,203
from that horizontal flip table,
363
00:13:58,205 --> 00:13:59,571
rotate the head up,
364
00:13:59,573 --> 00:14:01,206
mount the MMRTG in the top
365
00:14:01,208 --> 00:14:03,541
and we'll get our Z direction.
366
00:14:03,543 --> 00:14:06,945
We typically look
at zero to 5,000 hertz,
367
00:14:06,947 --> 00:14:09,047
sine, random sine shock
368
00:14:09,049 --> 00:14:11,516
and that gives us
the information we need.
369
00:14:11,518 --> 00:14:13,251
Okay. Now, you're gathering
that information
370
00:14:13,253 --> 00:14:14,886
by monitoring this how?
371
00:14:14,888 --> 00:14:17,856
Yes, yes. We have 31
separate transducers
372
00:14:17,858 --> 00:14:20,258
and accelerometers
that are wired to the body
373
00:14:20,260 --> 00:14:22,493
of the MMRTG that allows us
374
00:14:22,495 --> 00:14:24,028
to carefully monitor it,
375
00:14:24,030 --> 00:14:25,730
make certain nothing is damaged
376
00:14:25,732 --> 00:14:27,365
and then we get all
the information we need.
377
00:14:27,367 --> 00:14:29,033
Great. Well, can we see
this thing in action?
378
00:14:29,035 --> 00:14:31,135
- Can we fire it up?
- Yes, yes. We can.
379
00:14:31,137 --> 00:14:33,271
Why don't we put
our safety gear in?
380
00:14:33,273 --> 00:14:34,973
- Our...
- [Greg] All right.
381
00:14:34,975 --> 00:14:36,274
earplugs...
382
00:14:37,877 --> 00:14:40,111
and let me give the guys a call.
383
00:14:40,113 --> 00:14:41,980
Hey, are we ready
to shake this thing?
384
00:14:42,882 --> 00:14:45,516
[whirring]
385
00:15:07,640 --> 00:15:09,607
So, Steve. Pretty impressive.
386
00:15:09,609 --> 00:15:11,109
Now, I know this is meant
387
00:15:11,111 --> 00:15:12,977
to simulate the stresses
of a launch,
388
00:15:12,979 --> 00:15:14,512
and when we talk about stress
in a launch,
389
00:15:14,514 --> 00:15:16,014
we talk about g-forces.
390
00:15:16,016 --> 00:15:17,548
So, where were we on that scale?
391
00:15:17,550 --> 00:15:19,817
X-axis, 10 g's.
392
00:15:19,819 --> 00:15:21,953
Flight test would be 13 g's.
393
00:15:21,955 --> 00:15:25,123
And again, we'll through
that for X, Y, and Z axis.
394
00:15:25,125 --> 00:15:26,491
So you test
all the different ways
395
00:15:26,493 --> 00:15:27,759
that it could possibly
be vibrated
396
00:15:27,761 --> 00:15:28,960
to make sure that you're ready
397
00:15:28,962 --> 00:15:30,295
- for launch time.
- Yes.
398
00:15:30,297 --> 00:15:31,529
Tell me about a little bit about
399
00:15:31,531 --> 00:15:32,997
the rest of the testing
that we'll go through
400
00:15:32,999 --> 00:15:34,098
before it heads down to Florida
401
00:15:34,100 --> 00:15:35,233
and to end up in space.
402
00:15:35,235 --> 00:15:37,769
So next we would do
a center of mass,
403
00:15:37,771 --> 00:15:39,938
we'll do a magnetic field
measurement
404
00:15:39,940 --> 00:15:42,240
- and a vacuum chamber test.
- Sounds great.
405
00:15:42,242 --> 00:15:45,410
Now, if I were to ask you
to sum up just briefly
406
00:15:45,412 --> 00:15:47,812
what you think
nuclear power's role will be
407
00:15:47,814 --> 00:15:50,081
in space exploration,
what would you say?
408
00:15:50,083 --> 00:15:53,484
Simply put, we would support
a manned mission to Mars.
409
00:15:53,486 --> 00:15:55,853
Get guys there,
get them back again,
410
00:15:55,855 --> 00:15:58,489
and that would be the ultimate
for nuclear power.
411
00:15:58,491 --> 00:16:00,191
All right. Well Steve,
thank you very much.
412
00:16:00,193 --> 00:16:01,526
This has been awesome.
413
00:16:01,528 --> 00:16:02,927
George is having
a bunch of the folks
414
00:16:02,929 --> 00:16:04,395
that we've been talking to
back in Inventionland
415
00:16:04,397 --> 00:16:05,363
for a round table,
416
00:16:05,365 --> 00:16:07,131
love to invite you to be there.
417
00:16:07,133 --> 00:16:08,933
Fantastic.
Look forward to it, Greg.
418
00:16:08,935 --> 00:16:10,735
All right. Well, see you back
in Inventionland.
419
00:16:10,737 --> 00:16:14,305
[mellow music playing]
420
00:16:25,084 --> 00:16:27,452
[mellow music playing]
421
00:16:37,997 --> 00:16:40,064
- Hi everyone.
- Hey George.
422
00:16:40,066 --> 00:16:41,566
Well, welcome to Inventionland.
423
00:16:41,568 --> 00:16:43,468
- Thank you.
- We've been looking forward
424
00:16:43,470 --> 00:16:46,604
to hosting this round table
discussion.
425
00:16:46,606 --> 00:16:50,008
And this field
of nuclear technology
426
00:16:50,010 --> 00:16:51,943
is just so exciting
to all of us.
427
00:16:51,945 --> 00:16:53,911
I think you're in good hands
with Greg
428
00:16:53,913 --> 00:16:55,947
as you guys get through
this meeting.
429
00:16:55,949 --> 00:16:57,648
I'm gonna see all of you
a little later, okay?
430
00:16:59,118 --> 00:17:00,451
[man] All right.
Thanks, George.
431
00:17:00,453 --> 00:17:01,685
[George] Bye now.
432
00:17:02,988 --> 00:17:04,956
So, as we get this started,
I'm just gonna dive right in.
433
00:17:04,958 --> 00:17:06,224
Dr. Rita Baranwal,
434
00:17:06,226 --> 00:17:07,892
how do you see nuclear energy
435
00:17:07,894 --> 00:17:10,161
helping us with decarbonization?
436
00:17:10,163 --> 00:17:13,297
So nuclear energy has always
been a clean energy resource,
437
00:17:13,299 --> 00:17:15,900
so that's really important
to know right up front.
438
00:17:15,902 --> 00:17:18,136
So as communities
start to consider
439
00:17:18,138 --> 00:17:19,871
what they need to do
to decarbonize
440
00:17:19,873 --> 00:17:22,040
and meet their goals
and objectives,
441
00:17:22,042 --> 00:17:24,542
nuclear, if it already exists
in that community,
442
00:17:24,544 --> 00:17:26,477
is the cheapest way
to decarbonize
443
00:17:26,479 --> 00:17:28,279
the electricity sector.
444
00:17:28,281 --> 00:17:31,082
Also we have to consider
deploying new nuclear
445
00:17:31,084 --> 00:17:33,518
and then finally
it's really important
446
00:17:33,520 --> 00:17:35,453
to consider
that the electricity market
447
00:17:35,455 --> 00:17:38,456
is just one sector
that needs to be decarbonized.
448
00:17:38,458 --> 00:17:41,059
If you look at
the transportation sector,
449
00:17:41,061 --> 00:17:42,860
which is a very,
very large sector
450
00:17:42,862 --> 00:17:44,529
that really needs
decarbonization,
451
00:17:44,531 --> 00:17:46,431
nuclear reactors
and nuclear power
452
00:17:46,433 --> 00:17:49,233
can also make a big, big impact.
453
00:17:49,235 --> 00:17:51,335
Great. Now Dr. Kathy McCarthy,
454
00:17:51,337 --> 00:17:53,838
working into that answer
to that question,
455
00:17:53,840 --> 00:17:56,207
how do you see our...
The world's energy needs
456
00:17:56,209 --> 00:17:58,309
- changing in the future?
- From a volume perspective,
457
00:17:58,311 --> 00:17:59,544
you know,
we think about countries
458
00:17:59,546 --> 00:18:00,878
like the Unites States
459
00:18:00,880 --> 00:18:01,979
and we're developed
460
00:18:01,981 --> 00:18:03,014
and we've got access
461
00:18:03,016 --> 00:18:04,148
to electricity
462
00:18:04,150 --> 00:18:05,550
but now let's talk about
463
00:18:05,552 --> 00:18:06,617
we want everybody to have access
464
00:18:06,619 --> 00:18:07,952
to broadband.
465
00:18:07,954 --> 00:18:09,220
We need to have storage
466
00:18:09,222 --> 00:18:11,189
to be able to store that data.
467
00:18:11,191 --> 00:18:14,092
That storage takes a lot
of cooling, that takes energy.
468
00:18:14,094 --> 00:18:16,127
So, it's really both
reducing carbon
469
00:18:16,129 --> 00:18:18,062
- as well as increasing volume.
- Okay.
470
00:18:18,064 --> 00:18:19,964
So those are some
very earthbound things
471
00:18:19,966 --> 00:18:22,567
that we need to think about.
So Dr. Stephen Johnson,
472
00:18:22,569 --> 00:18:24,936
how is nuclear propulsion
gonna work into our future
473
00:18:24,938 --> 00:18:26,237
out in space?
474
00:18:26,239 --> 00:18:27,972
One of our greatest challenges
475
00:18:27,974 --> 00:18:29,540
is getting to Mars.
476
00:18:29,542 --> 00:18:31,676
And nuclear thermal propulsion
477
00:18:31,678 --> 00:18:33,945
can help us do that
by cutting down
478
00:18:33,947 --> 00:18:36,481
the amount of time it takes
to get there.
479
00:18:36,483 --> 00:18:40,017
For example,
if we were going to the moon,
480
00:18:40,019 --> 00:18:43,387
the Apollo shots,
Apollo 12, 14, et cetera,
481
00:18:43,389 --> 00:18:45,289
in the '69, '70 timeframe,
482
00:18:45,291 --> 00:18:47,258
they took three days
to get to the moon
483
00:18:47,260 --> 00:18:49,827
with their human payload
and equipment
484
00:18:49,829 --> 00:18:51,529
to survive there.
485
00:18:51,531 --> 00:18:54,832
When we were firing
the Pluto New Horizons' shot
486
00:18:54,834 --> 00:18:57,301
in 2006, January 19th,
487
00:18:57,303 --> 00:19:00,838
it took nine hours
to get to the moon from earth.
488
00:19:00,840 --> 00:19:04,242
We need to be able to use
nuclear thermal propulsion
489
00:19:04,244 --> 00:19:06,410
to get there
in a safe amount of time,
490
00:19:06,412 --> 00:19:08,146
do our mission,
and get people back.
491
00:19:08,148 --> 00:19:10,214
Okay. Great.
Now Dr. Corey McDaniel,
492
00:19:10,216 --> 00:19:11,749
thank you for being here.
493
00:19:11,751 --> 00:19:13,851
Are there policy changes
that can help us move forward
494
00:19:13,853 --> 00:19:15,887
with all of this as we...
As we get into the future?
495
00:19:15,889 --> 00:19:18,022
Well Greg, I'm somebody
of the opinion
496
00:19:18,024 --> 00:19:19,957
that the free market
breeds innovation
497
00:19:19,959 --> 00:19:21,559
and it's innovation
498
00:19:21,561 --> 00:19:23,728
that is the culture
in the United States,
499
00:19:23,730 --> 00:19:25,496
that our freedom allows us
500
00:19:25,498 --> 00:19:30,034
to have the freedom to pursue
market-based solutions
501
00:19:30,036 --> 00:19:32,303
that support
investments in technology
502
00:19:32,305 --> 00:19:34,372
like fusion and space nuclear
503
00:19:34,374 --> 00:19:36,374
and the advanced reactors
we see today.
504
00:19:36,376 --> 00:19:38,976
Really over the last decade,
505
00:19:38,978 --> 00:19:40,978
the marketplace has dictated
506
00:19:40,980 --> 00:19:43,414
that investors like Bill Gates
and Warren Buffett
507
00:19:43,416 --> 00:19:45,483
have invested
in advanced nuclear
508
00:19:45,485 --> 00:19:48,319
because of the attributes
of that power,
509
00:19:48,321 --> 00:19:51,122
clean, as Dr. Baranwal
mentioned,
510
00:19:51,124 --> 00:19:53,591
it's also reliable
and it can be integrated
511
00:19:53,593 --> 00:19:55,293
with other clean energy sources
512
00:19:55,295 --> 00:19:57,795
and work with other
renewable energy sources
513
00:19:57,797 --> 00:20:00,031
to reduce greenhouse gases
514
00:20:00,033 --> 00:20:02,099
which is obviously something
that a lot of people
515
00:20:02,101 --> 00:20:03,267
are concerned with today.
516
00:20:03,269 --> 00:20:05,002
So, I think that the policies
517
00:20:05,004 --> 00:20:07,038
that we have around innovation,
518
00:20:07,040 --> 00:20:08,306
the policies we have
that support
519
00:20:08,308 --> 00:20:11,075
our 17 national laboratories,
520
00:20:11,077 --> 00:20:14,111
that really allows the US
to be competitive
521
00:20:14,113 --> 00:20:16,180
and to out-innovate
other countries.
522
00:20:16,182 --> 00:20:18,049
So I wanna thank you all
very much for being here
523
00:20:18,051 --> 00:20:19,917
and thank all of you
for joining us
524
00:20:19,919 --> 00:20:21,919
on our exploration
of nuclear energy.
525
00:20:21,921 --> 00:20:24,889
For Tomorrow's World Today,
I'm Greg Constantino.
526
00:20:24,891 --> 00:20:27,358
So, the big question is,
if you could go to Mars,
527
00:20:27,360 --> 00:20:28,726
- would you?
- No.
528
00:20:28,728 --> 00:20:30,261
- Yes.
- Absolutely.
529
00:20:30,263 --> 00:20:31,362
- No?
- I'm the only honest one here.
530
00:20:31,364 --> 00:20:33,331
No. [laughs]
531
00:20:33,333 --> 00:20:35,466
- No?
- We're going without you.
532
00:20:35,468 --> 00:20:37,101
Okay.
533
00:20:37,103 --> 00:20:40,104
[dramatic music playing]
40898
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