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(dark mysterious music)
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- [Narrator] Asteroids.
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Remnants from the birth
of our solar system.
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From planetoid-sized monsters
down to tiny pebbles,
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they have orbited our sun
for billions of years.
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We have seen some up close,
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even touched their surface.
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We count their numbers,
chart their courses,
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and keep a wary eye on
these mountains in the dark.
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(exciting music)
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(dark mysterious music)
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Several spacecraft have ventured out
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towards these rocky worlds.
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Some have touched down and taken samples
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with surprising results,
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then returned them to Earth.
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Scientists have found these
remnants to be complex
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and full of secrets.
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There are different types of asteroids,
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and two new robotic
probes are ready to study
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some of these unique targets.
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One is called Psyche,
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and it is perhaps one
of the most interesting.
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(rousing music)
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- 16 Psyche is an asteroid
that orbits the sun
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out between Mars and Jupiter.
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It's called 16 Psyche because
it was the 16th asteroid
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discovered, and they were all being named
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after gods and goddesses at that time.
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- So the Psyche mission is
going to visit an asteroid
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which is called Psyche, and
it is a large metal asteroid,
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a unique body in the solar system.
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150 miles in diameter, approximately,
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and made of 40 to 60% iron nickel metal.
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That makes it a unique
body in the solar system.
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We visited worlds made of
ice, and worlds made of rock,
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and worlds made of gas before,
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but we've never visited a metal world.
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So we'll get to see something unique
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and different for the first time.
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- All the rocky planets
that we know of, the Earth,
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Mercury, Venus, Mars, and the Moon
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all have got a metal core in their center,
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and especially for the Earth,
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it's the source of our magnetic field,
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which may be tied to
holding onto our atmosphere
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and making our planet habitable.
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There's a lot of study that's
going on to understand that,
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but we don't know a lot about our core.
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What we've learned about
it, we learn indirectly,
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because we can't go there,
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and so Psyche gives us the
opportunity to visit a core
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the only way that humankind can ever do.
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And so we hope to learn
something about what's inside
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the Earth and other rocky
planets by visiting Psyche.
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But it also tells us about the processes
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in the very beginning of the solar system.
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It helps us understand how
planets form in the first place.
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(exciting music)
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- [Kalyani] So the Psyche payload consists
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of three science instruments.
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One of them is what's called
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a gamma ray neutron spectrometer.
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It's actually two separate
pieces of hardware.
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One is the gamma ray spectrometer,
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and the other one is the
neutron spectrometer.
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Both combined study the
elemental composition of Psyche.
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- If you know the surface composition,
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what is made of in
terms of iron and nickel
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and silicon and oxygen,
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you can then start to say
something about its history,
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and how it formed, and how it evolved.
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- By using gamma ray spectroscopy
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we can measure those elements remotely.
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We don't have to touch the surface,
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we don't have to dig into the surface.
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- For Psyche we're building kind of what
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we call the Cadillac.
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It's a very high precision,
high sensitivity instrument.
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It's very similar to the
messenger instrument.
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- That technology that we developed
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for the Messenger spacecraft
gave us a huge headstart
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going to Psyche
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- For our types of
instruments, we don't get
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to fly 'em very often,
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so when we actually get
selected for something,
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that's a big deal for us,
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where we can take what we
learned from the prior missions
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and implement it now and make
an even better instrument.
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- Only one body like this that's this big
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and made of metal in the solar system.
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So the big mystery is
where did it come from?
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How was it created?
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One of the theories about it
is that it was once the inside
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of a forming planet, because
the planets that we know,
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Earth, Mars, Venus, Jupiter,
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have metal cores inside of them.
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So this may have been the
metal core that was forming
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inside of a baby planet,
which then collided
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with other planets that
stripped off, forming planets,
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that stripped off that rocky mantel,
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just leaving a piece
of that core in space.
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And if that's the case,
then by studying this body
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we'll be able to study the
cores of planets like our own,
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the Earth, in a way that
we can never do otherwise.
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(bright music)
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- Psyche is a larger
asteroid in the main belt
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that is in between Mars and Jupiter.
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Our experience so far
in terms of exploring
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the solar system has been with
either rocky or icy bodies.
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What's particularly
interesting about Psyche
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is we think it's a metallic object.
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We have a common understanding
perhaps of how regular
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common rocks behave, but metal behave
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in a very different way.
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What I contribute to
the mission is trying to
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understand how cratering
and the process of collision
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and interaction of work
for a metallic object.
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And we'll use this information then
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to understand what we see at
the surface once we get there.
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What we did is take an iron meteorite,
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put it in in the chamber,
and use it as a target
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for our input experiment.
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And when we're shooting quartz bid
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at high speed in order
to produce a crater.
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Everything has been filmed
with the high speed cameras,
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so we have a tremendous
amount of data that shows
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in high resolution what
happened during the contact,
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during the explosion,
and how the crater forms
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on the surface, so everything
has been documented
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in great details.
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Here we have a piece of
the Gibeon meteorite,
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and what we see here is a
crater that was produced
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as a result of one of our experiments.
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And traditionally with rocks,
the rim would be blasted away
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and would be a sort of flattish feature.
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But here we see these flaps
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that basically are frozen into place,
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and this is because the metal
is much harder than rocks.
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And so you can then retain
this interesting morphology.
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There's gonna be a very exciting phase
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of the mission when we
actually start gathering data,
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and there's gonna be lots of surprises.
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I just can't wait to be there
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and see whether or not
there is any resemblance
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with this model or not.
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(bright music)
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- There is nothing like the
experience of sitting on console
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on launch day, and hearing all
the people go around and say
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we go for launch.
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And then finally getting to say yourself,
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we are go for launch.
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It's the culmination of
all those years of effort,
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and all those hundreds of people working.
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And so it's super
exciting when you actually
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finally say we're go, and we're gonna get
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that beast into space.
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We're gonna go launch and
do a Mars gravity assist,
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go by planet Mars, and then
continue onto the asteroid
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using electric propulsion.
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(bright inspiring music)
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- I think no matter what
we think it is right now,
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and how much we hypothesize
what it might look like,
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I think it's gonna really
surprise us and change our views
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about our solar system when we get there,
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and it's an incredible
opportunity to be a part
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of the team making that happen.
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(bright piano music)
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- [Narrator] The Psyche
mission has suffered
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several launch delays.
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However, it should be underway
in the next year or two.
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- [Announcer] 3, 2, 1, 0.
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(space engine rumbling)
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Lift off.
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Atlas V takes flight.
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- [Narrator] Another ambitious
mission that has launched
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is Lucy to study several asteroid targets.
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- [Announcer] All clear.
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- So Lucy is going to
survey eight asteroids
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over a 12 year mission life.
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The first asteroid is in
the main belt asteroids,
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it's Donald Johanson.
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And then the remaining
asteroids are the ones
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that we call the Trojans.
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And because we believe
that they are remnants
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of our solar system, by
studying their geology,
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as well as their
composition and their mass,
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then that will give us
insight into planets,
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planet formations, and in
particular the outer planets.
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- The Trojan asteroids, which are located
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in these Goldilock zones
of gravity-stable orbits,
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or in between the sun and Jupiter,
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are really leftover
fossils from the formation
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of the solar system.
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And these fossils are
around 4 billion years old.
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And when the solar system was
forming, they were brought
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into these locations,
and the Trojan asteroids
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which have been there since the formation
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of the solar system, are
these last unexplored remnants
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from the cosmic neighborhood creation.
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And we're extremely excited
to go and visit them
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because of our total lack of understanding
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of exactly what is out there.
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And so it's gonna be extremely exciting
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when the Lucy spacecraft explores them.
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- Some of the most important
planetary science questions
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we're trying to answer
are focused on the origin
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and the evolution of the solar system.
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Asteroids and other small
bodies are really important keys
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to understanding that history.
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Amazingly, many of these mysterious worlds
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have been altered very little
in the 4.6 billion years
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since they first formed.
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The relatively pristine state
makes comets, asteroids,
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and some meteorites,
wonderful storytellers
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that have preserved clues
they can share with us
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about conditions in
the early solar system.
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In particular, by studying
the Trojan asteroids,
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we can gain more insight into the history
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of the outer solar system
in the giant planets,
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Jupiter, Saturn, Uranus, and Neptune.
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We actually find asteroids
across the solar system,
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including near Earth
asteroids that are in orbits
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that periodically bring
them close to Earth,
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main belt asteroids that orbit the sun
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between Mars and Jupiter,
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the Trojans that Lucy will explore,
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and the Copperbelt, just beyond Pluto,
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which contains some of
the most primitive objects
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in our solar system.
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Not all of these asteroids are the same,
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and Lucy is part of a
collection of ambitious missions
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to study the diversity of
these asteroid populations
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that'll help us fill in more
pieces of that cosmic puzzle.
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(rousing music)
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- [Narrator] Lucy will
slingshot out from Earth's orbit
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and pass by the first target, a C-class
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or carbon-based asteroid
named Donald Johanson,
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after the famed archeologist.
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Lucy will continue to the orbit of Jupiter
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and intercept four more targets.
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Eurybates, Orus, Leucus and Polymele.
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Some are DMP class
asteroids never seen before,
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and theorized to be rich
in volatiles and organics.
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The probe will then return to Earth
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for another gravity assist
to the trailing Trojans
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of Jupiter, intercepting the
twins Patroclus and Menoetius,
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more P-class objects.
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- And Lucy spacecraft was
named after the Lucy Fossil,
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because we will be studying asteroids,
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which are the fossils of planet formation.
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But the Lucy spacecraft and
the Lucy Fossil was named
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by archeologist Donald
Johanson and his team,
254
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because apparently when
they discovered the hominid,
255
00:14:10,020 --> 00:14:12,397
they were listening to The Beatles song,
256
00:14:12,397 --> 00:14:14,610
"Lucy in the Sky with Diamonds".
257
00:14:14,610 --> 00:14:16,020
Now we do have a diamond.
258
00:14:16,020 --> 00:14:20,910
It's our beam splitter, which
is on the LTES instrument,
259
00:14:20,910 --> 00:14:23,433
which is used to split the beam,
260
00:14:24,390 --> 00:14:26,400
is actually made of diamonds.
261
00:14:26,400 --> 00:14:29,130
- My job as a mission architect
here at Lockheed Martin,
262
00:14:29,130 --> 00:14:31,890
it's very interesting,
and it sort of encompasses
263
00:14:31,890 --> 00:14:34,020
the biggest picture of the mission.
264
00:14:34,020 --> 00:14:35,430
What is the trajectory?
265
00:14:35,430 --> 00:14:38,400
What sort of propulsion do you
need to fly that trajectory?
266
00:14:38,400 --> 00:14:40,170
What does the spacecraft look like?
267
00:14:40,170 --> 00:14:42,420
So in the case of, for
example, Lucy, it's like okay,
268
00:14:42,420 --> 00:14:44,850
it's going out five times
further from the sun
269
00:14:44,850 --> 00:14:45,810
than the Earth is.
270
00:14:45,810 --> 00:14:47,970
And so it's gonna need
big, huge solar rays
271
00:14:47,970 --> 00:14:49,350
just because of that.
272
00:14:49,350 --> 00:14:52,080
- [Cathy] Lucy has three
scientific instruments
273
00:14:52,080 --> 00:14:54,840
onboard the spacecraft,
and we'll also be using
274
00:14:54,840 --> 00:14:57,630
two of the spacecraft
subsystems to contribute
275
00:14:57,630 --> 00:14:59,250
to the science investigation.
276
00:14:59,250 --> 00:15:00,360
With the LORRI instrument
277
00:15:00,360 --> 00:15:02,340
we'll be able to get panchromatic images,
278
00:15:02,340 --> 00:15:04,770
which will tell us about the geology,
279
00:15:04,770 --> 00:15:07,080
and the crater history, which gives us
280
00:15:07,080 --> 00:15:08,700
the age of the surface.
281
00:15:08,700 --> 00:15:10,800
With the TES instrument,
we'll be able to measure
282
00:15:10,800 --> 00:15:13,200
the temperature of the
surface at different points,
283
00:15:13,200 --> 00:15:15,120
and with the Ralph
instrument we'll be able to
284
00:15:15,120 --> 00:15:18,123
measure the composition of the surfaces.
285
00:15:21,480 --> 00:15:24,660
The Jupiter Trojans, they have a variety
286
00:15:24,660 --> 00:15:26,430
of surface characteristics.
287
00:15:26,430 --> 00:15:27,570
They have different colors,
288
00:15:27,570 --> 00:15:29,550
and different surface compositions,
289
00:15:29,550 --> 00:15:30,750
and that leads us to believe
290
00:15:30,750 --> 00:15:32,913
that maybe they formed somewhere else.
291
00:15:48,210 --> 00:15:50,160
- [Narrator] After launch,
the Lucy probe failed
292
00:15:50,160 --> 00:15:52,770
to lock one of its solar panels in place.
293
00:15:52,770 --> 00:15:55,743
Engineers are working on a
resolution to this problem.
294
00:16:04,140 --> 00:16:08,370
- The Lucy spacecraft will
travel 4 billion miles
295
00:16:08,370 --> 00:16:10,620
over its mission,
296
00:16:10,620 --> 00:16:15,620
and it is a very sophisticated,
well-orchestrated trajectory
297
00:16:17,310 --> 00:16:18,510
that gets us there.
298
00:16:18,510 --> 00:16:21,630
- I cannot wait for those gorgeous images
299
00:16:21,630 --> 00:16:23,880
that our instruments are gonna take,
300
00:16:23,880 --> 00:16:25,200
and bring back to Earth.
301
00:16:25,200 --> 00:16:27,540
What that's gonna tell me and the world
302
00:16:27,540 --> 00:16:30,780
is how gorgeous these objects are,
303
00:16:30,780 --> 00:16:32,640
what secrets they have to hold,
304
00:16:32,640 --> 00:16:35,730
and it's gonna start us
unlocking these mysteries
305
00:16:35,730 --> 00:16:37,830
of the solar system that are out there.
306
00:16:37,830 --> 00:16:41,370
I can't wait, and words can't
describe just how excited I am
307
00:16:41,370 --> 00:16:43,410
to share with everyone these images
308
00:16:43,410 --> 00:16:44,710
when they first come back.
309
00:16:49,080 --> 00:16:50,430
- [Narrator] This animation is drawn
310
00:16:50,430 --> 00:16:54,153
from the recent data release
of the ESA Gaia satellite.
311
00:16:58,320 --> 00:17:01,080
It reveals the locations
of the larger asteroids
312
00:17:01,080 --> 00:17:02,583
within our solar system.
313
00:17:13,740 --> 00:17:16,350
This tapestry of orbits shows that several
314
00:17:16,350 --> 00:17:19,113
near-Earth objects
cross our orbital plane.
315
00:17:27,870 --> 00:17:31,350
Geological history records
that some have hit the Earth
316
00:17:31,350 --> 00:17:33,213
with devastating effects.
317
00:17:34,271 --> 00:17:37,188
(slow tense music)
318
00:17:38,910 --> 00:17:41,670
- We've seen asteroids
come through the atmosphere
319
00:17:41,670 --> 00:17:44,880
and kind of explode,
and cause some damage,
320
00:17:44,880 --> 00:17:47,820
and thankfully so far
nothing recent enough
321
00:17:47,820 --> 00:17:49,950
that it really has a large, large impact
322
00:17:49,950 --> 00:17:52,950
on our civilization, but it could happen.
323
00:17:52,950 --> 00:17:55,170
- There are multiple different ways
324
00:17:55,170 --> 00:17:57,030
that you might attack the problem of,
325
00:17:57,030 --> 00:17:59,370
oh no, doomsday asteroid is inbound.
326
00:17:59,370 --> 00:18:01,410
One of those ways is
a kinetic interceptor,
327
00:18:01,410 --> 00:18:03,480
which is what DART is working on.
328
00:18:03,480 --> 00:18:05,250
- [Lori] As part of planetary defense,
329
00:18:05,250 --> 00:18:08,670
DART, which stands for Double
Asteroid Redirection Test,
330
00:18:08,670 --> 00:18:13,670
its mission is to impact an
asteroid in a binary system.
331
00:18:13,920 --> 00:18:17,430
- The reason we're doing
this test is to try and prove
332
00:18:17,430 --> 00:18:19,470
out the technologies
that would be needed to,
333
00:18:19,470 --> 00:18:22,950
say, save Earth if an asteroid
were coming our direction
334
00:18:22,950 --> 00:18:25,350
and we needed to adjust its trajectory
335
00:18:25,350 --> 00:18:26,640
so that it would miss the planet.
336
00:18:26,640 --> 00:18:30,000
- SMART Nav is the autonomous
algorithm on board,
337
00:18:30,000 --> 00:18:33,270
and the purpose of
SMART Nav is to identify
338
00:18:33,270 --> 00:18:36,030
Dimorphos, which is the
smaller of the two asteroids
339
00:18:36,030 --> 00:18:37,170
in the Didymos system.
340
00:18:37,170 --> 00:18:40,860
And we send maneuver
commands to the spacecraft
341
00:18:40,860 --> 00:18:43,053
for the spacecraft to hit Dimorphos.
342
00:18:44,160 --> 00:18:48,570
- And we understand where about
40% of those asteroids are.
343
00:18:48,570 --> 00:18:51,780
We know that no known asteroid
344
00:18:51,780 --> 00:18:54,060
is a danger to the Earth right now,
345
00:18:54,060 --> 00:18:55,680
but the concern is about the asteroids
346
00:18:55,680 --> 00:18:57,570
we don't know about yet.
347
00:18:57,570 --> 00:18:59,970
And if we should ever discover an asteroid
348
00:18:59,970 --> 00:19:01,920
that's on a collision course with Earth,
349
00:19:01,920 --> 00:19:04,980
we wanna be able to discover
this years in advance
350
00:19:04,980 --> 00:19:08,130
so we can give the asteroid
a push, not to destroy it.
351
00:19:08,130 --> 00:19:10,320
We probably wouldn't be
able to do that anyway.
352
00:19:10,320 --> 00:19:12,600
But just to prevent that collision.
353
00:19:12,600 --> 00:19:15,600
And the DART mission, the Double
Asteroid Redirection Test,
354
00:19:15,600 --> 00:19:18,961
is our first test of
one way of doing that.
355
00:19:18,961 --> 00:19:22,461
(soft atmospheric music)
356
00:19:26,100 --> 00:19:29,190
- [Narrator] Launched aboard
a SpaceX Falcon rocket,
357
00:19:29,190 --> 00:19:31,803
DART is well on its way to its target.
358
00:19:38,010 --> 00:19:40,950
- So the way an ion thruster
works is that it utilizes
359
00:19:40,950 --> 00:19:45,120
electrical energy to ionize
propellant and accelerate it
360
00:19:45,120 --> 00:19:47,430
using electric and magnetic fields.
361
00:19:47,430 --> 00:19:50,490
What it next does is that it
increases the power level,
362
00:19:50,490 --> 00:19:53,640
you get more thrust out of
it, it's more fuel efficient,
363
00:19:53,640 --> 00:19:57,990
it lasts longer, basically
kinda improves things
364
00:19:57,990 --> 00:20:00,750
in almost every way, and
makes it very beneficial
365
00:20:00,750 --> 00:20:04,060
for end users to utilize
366
00:20:13,020 --> 00:20:14,910
- [Luke] When they're rolled
out and fully deployed,
367
00:20:14,910 --> 00:20:16,443
they're almost 10 meters long.
368
00:20:17,370 --> 00:20:20,580
This is the last time
that anyone will ever see
369
00:20:20,580 --> 00:20:22,470
these arrays fully deployed.
370
00:20:22,470 --> 00:20:24,960
Once we stow them here at DSS,
371
00:20:24,960 --> 00:20:28,110
they will not be deployed
again until we're in space
372
00:20:28,110 --> 00:20:29,850
on the DART spacecraft.
373
00:20:29,850 --> 00:20:31,620
Part of our detailed inspection
374
00:20:31,620 --> 00:20:34,650
entails Andrew looking at the cell by cell
375
00:20:34,650 --> 00:20:37,620
on these arrays again that
are almost 10 meters long.
376
00:20:37,620 --> 00:20:40,050
He'll look at them at
different wavelengths of light,
377
00:20:40,050 --> 00:20:42,480
different angles, just to assure ourselves
378
00:20:42,480 --> 00:20:44,910
that we've found every anomaly
possible in these cells,
379
00:20:44,910 --> 00:20:48,150
and they're fully characterized
with the entire array,
380
00:20:48,150 --> 00:20:49,980
and we know exactly what we have,
381
00:20:49,980 --> 00:20:52,030
and the condition it's in when we launch.
382
00:20:52,920 --> 00:20:56,190
- DART's going to a binary
asteroid, a double asteroid,
383
00:20:56,190 --> 00:20:57,930
for two really good reasons.
384
00:20:57,930 --> 00:21:00,570
The little asteroid,
Dimorphos, which is in orbit
385
00:21:00,570 --> 00:21:03,060
around the big asteroid, Didymos,
386
00:21:03,060 --> 00:21:05,640
that asteroid is about the size of object
387
00:21:05,640 --> 00:21:07,890
that we would tend to be concerned about.
388
00:21:07,890 --> 00:21:10,890
The most abundant asteroids
are the small ones.
389
00:21:10,890 --> 00:21:13,710
And this one, about 160 meters across,
390
00:21:13,710 --> 00:21:15,720
or about the size of a football stadium,
391
00:21:15,720 --> 00:21:19,170
is large enough that it really
would cause severe damage
392
00:21:19,170 --> 00:21:20,970
if it struck the Earth.
393
00:21:20,970 --> 00:21:24,060
Now, by impacting, by
doing our experiment,
394
00:21:24,060 --> 00:21:27,750
a kinetic impact experiment
on the small moonlet asteroid,
395
00:21:27,750 --> 00:21:30,300
we're able to measure our effectiveness
396
00:21:30,300 --> 00:21:33,030
in deflecting the asteroid
by watching the change
397
00:21:33,030 --> 00:21:35,790
in the orbit of the little
asteroid around the big one.
398
00:21:35,790 --> 00:21:37,710
It makes that measurement
a lot more precise
399
00:21:37,710 --> 00:21:40,440
and a lot easier to do
with telescopes on Earth.
400
00:21:40,440 --> 00:21:42,720
The other reason we're doing
it is that the presence
401
00:21:42,720 --> 00:21:45,450
of the large asteroid
there keeps the little one
402
00:21:45,450 --> 00:21:48,660
in orbit around it as the
pair go around the sun.
403
00:21:48,660 --> 00:21:51,750
So that means that this
asteroid, which is not a danger
404
00:21:51,750 --> 00:21:55,080
to Earth now, will never
become a danger to the Earth
405
00:21:55,080 --> 00:21:58,334
because of anything that
we do in the DART mission.
406
00:21:58,334 --> 00:22:01,167
(exciting music)
407
00:22:17,220 --> 00:22:19,500
DART is carrying a small cube set,
408
00:22:19,500 --> 00:22:20,970
it's called the LICIACube.
409
00:22:20,970 --> 00:22:23,460
It was contributed by
the Italian Space Agency.
410
00:22:23,460 --> 00:22:26,490
And its job basically
is to watch the impact
411
00:22:26,490 --> 00:22:28,230
from a little distance away.
412
00:22:28,230 --> 00:22:30,360
It's riding along on the DART spacecraft
413
00:22:30,360 --> 00:22:32,790
and it's going to be deployed a few days
414
00:22:32,790 --> 00:22:34,890
before the kinetic impact.
415
00:22:34,890 --> 00:22:36,870
It's going to maneuver and offset itself
416
00:22:36,870 --> 00:22:39,990
to the side so that it doesn't
run into the same asteroid
417
00:22:39,990 --> 00:22:41,160
that DART is running into.
418
00:22:41,160 --> 00:22:43,260
And it's got two cameras on it
419
00:22:43,260 --> 00:22:44,550
that are going to try to,
420
00:22:44,550 --> 00:22:48,450
first, catch the actual
impact of DART on camera,
421
00:22:48,450 --> 00:22:52,290
but then more importantly, see the ejecta,
422
00:22:52,290 --> 00:22:54,440
the plume of material
that's blown off the surface
423
00:22:54,440 --> 00:22:56,670
of the asteroid and how that develops.
424
00:22:56,670 --> 00:23:00,510
If we're fortunate, we'll be
able to see the impact crater
425
00:23:00,510 --> 00:23:02,490
newly formed by the DART impact.
426
00:23:02,490 --> 00:23:05,160
And then, of course, LICIACube
is going to do something
427
00:23:05,160 --> 00:23:08,820
that DART can't do, that
is fly past the asteroid,
428
00:23:08,820 --> 00:23:11,820
look back, and get the full
three dimensional shape
429
00:23:11,820 --> 00:23:14,730
of the object that we
hit, which we won't know
430
00:23:14,730 --> 00:23:16,130
until we actually get there.
431
00:23:18,180 --> 00:23:19,710
- [Narrator] One other threat to Earth
432
00:23:19,710 --> 00:23:23,073
is the interstellar object
passing through our solar system.
433
00:23:24,690 --> 00:23:27,840
They arrive without warning, fast moving,
434
00:23:27,840 --> 00:23:29,763
and having no known orbit.
435
00:23:30,750 --> 00:23:33,723
Another hazardous mountain in the dark.
436
00:23:41,598 --> 00:23:44,348
(exciting music)
437
00:23:46,355 --> 00:23:49,522
(asteroids whooshing)
35321
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