WEBVTT

00:00:03.938 --> 00:00:06.471
JOSH: It takes a lot of power
to run a space program.

00:00:06.473 --> 00:00:08.708
And in some places where NASA
will go in the future, they

00:00:08.710 --> 00:00:11.376
don't have access to anything
like this.

00:00:11.378 --> 00:00:14.080
So agency scientists and
engineers are looking to do

00:00:14.081 --> 00:00:17.716
some huge things... on a very
small scale.

00:00:17.718 --> 00:00:21.620
NASA goes nuclear, next on Real
World.

00:00:21.621 --> 00:00:24.868
? [music] ?

00:00:29.400 --> 00:00:32.798
JOSH: NASA's mission to explore
worlds beyond our own would

00:00:32.800 --> 00:00:35.435
never get off the ground
without innovative ways to

00:00:35.436 --> 00:00:38.638
power all the operations that
make that possible.

00:00:38.640 --> 00:00:40.740
MIKE HOUTS: To explore the
universe, you need

00:00:40.741 --> 00:00:43.141
lots of energy...
JOSH: Mike Houts is a nuclear

00:00:43.143 --> 00:00:46.111
research manager at Marshall
Space Flight Center.

00:00:46.113 --> 00:00:48.815
MIKE: One of the areas that
NASA is looking at right now is

00:00:48.816 --> 00:00:51.350
fission. And so this is
actually using the nuclear

00:00:51.351 --> 00:00:53.753
fission process to generate
energy that can be

00:00:53.755 --> 00:00:56.288
used for any of our exploration
needs.

00:00:56.290 --> 00:00:59.391
JOSH: Atoms are the most basic
units of matter.

00:00:59.393 --> 00:01:02.828
The nucleus of an atom contains
positively charged particles

00:01:02.830 --> 00:01:06.598
called protons. The number of
protons in an atom determines

00:01:06.600 --> 00:01:10.036
the atomic number of an
element. Elements are arranged

00:01:10.038 --> 00:01:13.473
on the periodic table according
to their atomic number

00:01:13.475 --> 00:01:17.176
Atoms of the same element have
the same number of protons and

00:01:17.178 --> 00:01:20.313
electrons, but might have
different number of neutrons.

00:01:20.315 --> 00:01:24.283
Atoms with different numbers of
neutrons are called isotopes.

00:01:24.285 --> 00:01:27.920
Some elements have isotopes
that are unstable... that is,

00:01:27.921 --> 00:01:31.523
they do not hold together well.
When they break apart, they

00:01:31.525 --> 00:01:35.628
undergo a nuclear reaction and
become radioactive. Two new

00:01:35.630 --> 00:01:38.365
elements are produced. The
atomic number of these two

00:01:38.366 --> 00:01:41.868
elements adds up to the atomic
number of the original element.

00:01:41.870 --> 00:01:45.505
Here's an example. Start with
an atom of Uranium.

00:01:45.506 --> 00:01:49.841
Its atomic number is 92. When
this atom splits, through

00:01:49.843 --> 00:01:52.911
nuclear fission, you get two
new elements.

00:01:52.913 --> 00:01:57.416
One might be say, Barium with
an atomic number of 56.

00:01:57.418 --> 00:02:01.153
So what would the other one be?
Do the math.

00:02:01.155 --> 00:02:05.358
Subtract the atomic number of
barium, 56 from the atomic

00:02:05.360 --> 00:02:07.726
number of Uranium, 92.

00:02:07.728 --> 00:02:09.828
You're left with 36.

00:02:09.830 --> 00:02:13.866
And that is the atomic number
of krypton, the other element.

00:02:13.868 --> 00:02:17.470
When uranium splits, many
elements can result, but the

00:02:17.471 --> 00:02:20.606
atomic number of the new
elements will always be between

00:02:20.608 --> 00:02:24.176
32 and 60 and the sum of their
atomic numbers will always be

00:02:24.178 --> 00:02:27.746
92, the atomic number of
uranium.

00:02:27.748 --> 00:02:31.885
Okay, back to Mike Hauts.
He and his team are working to

00:02:31.886 --> 00:02:34.520
develop a viable energy source
that would satisfy

00:02:34.521 --> 00:02:37.223
many needs of space
exploration.

00:02:37.225 --> 00:02:39.358
MIKE: The applications...
Everything from life support

00:02:39.360 --> 00:02:42.495
systems, to in-situ resource
utilization, some

00:02:42.496 --> 00:02:44.863
communications, really just all
of the outpost activities is

00:02:44.865 --> 00:02:47.666
what they're looking at using
the electricity for.

00:02:47.668 --> 00:02:50.970
JOSH: The system is based on
old technology, the Stirling

00:02:50.971 --> 00:02:54.540
Engine, which was originally
developed in the 19th century.

00:02:54.541 --> 00:02:57.276
The engine converts heat into
electricity.

00:02:57.278 --> 00:03:00.213
So nuclear fission would create
the heat that the sterling

00:03:00.215 --> 00:03:02.715
engine would turn into useable
electricity to power

00:03:02.716 --> 00:03:07.120
operations. This system is
designed for about 40 kilowatts

00:03:07.121 --> 00:03:11.256
of power. That would power
about 8 houses here on earth.

00:03:11.258 --> 00:03:13.860
That's a little more than a
solar array on the space

00:03:13.861 --> 00:03:16.796
station, which can produce 32
kilowatts.

00:03:16.798 --> 00:03:21.000
Plus with the nuclear power
plant, you don't need sunlight.

00:03:21.001 --> 00:03:24.303
MIKE: It's a very high power by
NASA standards.

00:03:24.305 --> 00:03:26.538
It really gives us the
opportunity to have a power

00:03:26.540 --> 00:03:28.741
rich environment. It can also
be operated anywhere on the

00:03:28.743 --> 00:03:31.043
surface of the moon, anywhere
on the surface of Mars. So it

00:03:31.045 --> 00:03:33.145
gives us a lot of flexibility,
a lot of power capability,

00:03:33.146 --> 00:03:35.848
but as reactors go, it's
actually very, very tiny.

00:03:35.850 --> 00:03:38.016
Compared to a terrestrial
reactor,

00:03:38.018 --> 00:03:41.620
it's about 1/20,000th the power
level.

00:03:41.621 --> 00:03:44.623
JOSH: And the safety concerns
associated with nuclear power

00:03:44.625 --> 00:03:47.926
are virtually non-existent with
this system.

00:03:47.928 --> 00:03:50.603
MIKE: They have whatĎs called a
negative temperature reactivity

00:03:50.605 --> 00:03:53.400
feedback coefficient. What that
basically means is if the

00:03:53.401 --> 00:03:56.670
reactor starts to warm up, the
system itself actually gets

00:03:56.671 --> 00:03:59.438
less reactive, and that'll tend
to cool the system down.

00:03:59.440 --> 00:04:02.175
The system starts to cool down
too much, they system will

00:04:02.176 --> 00:04:04.610
actually shrink and become
slightly more reactive.

00:04:04.611 --> 00:04:06.946
That'll cause it to heat back
up. So the systems

00:04:06.948 --> 00:04:10.016
themselves are very stable.
JOSH: And any fears about the

00:04:10.018 --> 00:04:12.585
nuclear material creating a
disaster in the event of a

00:04:12.586 --> 00:04:16.723
launch mishap would be erased
thanks to good engineering.

00:04:16.725 --> 00:04:19.791
MIKE: The nice point about
reactors is they operate

00:04:19.793 --> 00:04:23.061
basically by having the right
materials get in the right

00:04:23.063 --> 00:04:25.331
geometry, and that will cause
the reactor to turn on.

00:04:25.333 --> 00:04:28.166
And so what's been done in this
system is to basically make

00:04:28.168 --> 00:04:30.370
sure it only turns on when you
want it to turn on. And the

00:04:30.371 --> 00:04:33.573
system is designed such that
during launch, any credible

00:04:33.575 --> 00:04:37.476
launch accident, that it will
not inadvertently turn on.

00:04:37.478 --> 00:04:41.848
JOSH: So very safe... and
incredibly efficient...

00:04:41.850 --> 00:04:44.516
MIKE: The amount of fuel we
have on board, we burn about 1

00:04:44.518 --> 00:04:47.386
percent of our fuel every 12
years. And so we're not going

00:04:47.388 --> 00:04:50.123
to run out of fuel, however
there will be other parts of

00:04:50.125 --> 00:04:52.591
the system that might limit the
lifetime.

00:04:52.593 --> 00:04:55.561
JOSH: The prototype system
doesn't use nuclear fission.

00:04:55.563 --> 00:04:59.165
That's for a future iteration
of the concept. For now, it

00:04:59.166 --> 00:05:02.468
uses resistance heaters that
closely mimic

00:05:02.470 --> 00:05:05.471
the heat from fission. The
Sterling engine turns

00:05:05.473 --> 00:05:08.708
that heat into electricity.
Here's how it works...

00:05:08.710 --> 00:05:11.811
MIKE: What that simulator does
is it heats the coolant and in

00:05:11.813 --> 00:05:14.613
this case we're using a coolant
that is a mixture of sodium and

00:05:14.615 --> 00:05:17.883
potassium, heats that coolant
to about 850 Kelvin.

00:05:17.885 --> 00:05:20.420
And then that hot coolant is
used to provide power to the

00:05:20.421 --> 00:05:23.188
sterling power conversion
subsystem. And what that does

00:05:23.190 --> 00:05:26.191
is it takes a portion of the
energy that's in the NaK

00:05:26.193 --> 00:05:29.295
Coolant and converts it into
electricity.

00:05:29.296 --> 00:05:31.363
About 25 percent of that energy
is converted from heat to

00:05:31.365 --> 00:05:34.000
electricity. Now in the process
of that energy being

00:05:34.001 --> 00:05:37.570
transferred to the sterling
engine, it actually cools the

00:05:37.571 --> 00:05:41.273
NaK down. And so that slightly
cooler NaK, then goes though

00:05:41.275 --> 00:05:44.376
the circuit, it's
re-pressurized in a pump and

00:05:44.378 --> 00:05:47.313
back through the core
stimulator, where it's heated

00:05:47.315 --> 00:05:50.583
goes back up and then
continues in the circuit.

00:05:50.585 --> 00:05:53.486
JOSH: NASA scientists, working
with the Department of Energy

00:05:53.488 --> 00:05:56.188
think that they could have a
nuclear fission based version

00:05:56.190 --> 00:05:59.891
of this system in place within
5 to 6 years

00:05:59.893 --> 00:06:02.961
Keep track of this project and
all of NASA's missions,

00:06:02.963 --> 00:06:06.733
at www.nasa.gov.

00:06:08.690 --> 00:06:11.653
? [music] ?

00:06:25.283 --> 00:06:28.445
[sfx]