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(technological music)
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- [Narrator] NASA's latest
robotic lander, InSight,
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descends to the surface of Mars,
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the challenging effort
greeted with elation.
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- [Operator] Touchdown confirmed.
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(crowd cheers)
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- [Narrator] Meanwhile,
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an orbiting ESA satellite, ExoMars,
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begins its own exploration
of this enthralling planet.
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(flames roar)
(intense music)
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(flame roars)
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(flames roar)
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(flames roar)
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(meteor strikes)
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(space whooshes)
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(light explodes)
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(logo soars)
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(soothing music)
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The majestic stereo imagery
of Mars as seen from orbit
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reveals a planet of
dynamic texture and form
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slowly revealing its secrets.
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(soothing music)
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- We've sent a lot of
missions to Mars in the past.
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We've sent rovers, we've sent orbiters,
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and they've done a lot of
really, really great science
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and a lot of really
interesting measurements,
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but those measurements just
scratch the surface of Mars.
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We know a lot about the surface of Mars,
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we know a lot about its atmosphere,
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and even about its ionosphere,
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but we don't know very much about
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what goes on a mile below the surface,
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much less 2000 miles below the
surface down to the center.
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And this will be the first mission
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that's going to Mars specifically
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to investigate the huge extent
of Mars below the surface.
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(soothing music)
(machinery whirring)
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The basic idea of InSight is to map out
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the deep structure of Mars
for the very first time.
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We're gonna map out the
thickness of the crust,
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the size of the core,
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the composition of the mantle
and core of the planet.
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Sort of get the first map
of the deep inside of Mars.
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(machinery whirring)
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It's going to Mars to do the science,
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to make the measurements,
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that scientifically and personally,
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I've been waiting for over 30 years for.
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As a graduate student, I
was doing research on Mars
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and I just needed to have
the thickness of the crust.
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I just needed the thickness of the crust,
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and we didn't have it.
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And seismology was the way to do it,
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and so I thought, well maybe
someday somebody will put
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a seismometer on Mars
and get this measurement
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so I can do my research.
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And so it's kind of an amazing
journey for me to look back
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and say, I'm the guy who's
actually going to put
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that seismometer on Mars,
get that information,
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and now I can go back and finish the job
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I was trying to do 30 years ago.
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It's an amazing feeling.
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- The InSight mission will finally provide
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a seismic information of Mars
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that scientists have been wanting for
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since the very first Mars lander, Viking.
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It has a seismometer on it,
but for a variety of reasons
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it never got back any seismic data.
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There's been many other
attempts to get seismometers
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onto the surface of Mars for
very good science reasons,
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but they've, for one reason or another,
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never been successful.
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So now, we're right on the very edge
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of getting a seismometer on Mars
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that will finally give
us back seismic data.
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That seismic data's incredibly
important to scientists
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because it gives them an idea
what the size of the crust,
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the mantle, and the core are,
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as well as the properties
of each of those,
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which are the basic internals
of every rocky planet.
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(intense music)
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- The most fun or interesting
thing about InSight
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from an engineer's point of view
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is really that we're playing the claw game
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super far away on Mars.
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We're taking this grapple,
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and we're gonna pick up an instrument,
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and lift it up off the deck
and put it down on Mars.
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So, I like to say that
we're playing the claw game,
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on Mars, with no joystick.
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(machinery clinking)
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(machinery whirring)
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- [Narrator] Next, a
wind and thermal shield
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will be lowered over
the seismic instrument
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to protect it from the environment.
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The second instrument,
the heat flow probe,
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will be placed on the
ground, and over time
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will hammer itself down to
take subsurface readings.
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- There's a lot of international
partners on InSight.
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It really takes a whole world to produce
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an exciting mission like this.
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So most of our science missions
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are actually being supported
by our international partners.
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So for example, the SEIS
instrument, our seismometer,
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has support from the French, the Germans,
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the Swiss, the UK folks.
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So we have a variety of those people.
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The Heat Flow and
Physical Properties Probe
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is being provided by the Germans
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with some support from Poland.
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(energetic music)
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- InSight is a mission to Mars,
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but it's much, much more
than a Mars mission.
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In some sense, it's like a time machine.
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It's measuring the structure of Mars
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that was put in place
4.5 billion years ago.
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So we can go back and
understand the processes
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that formed Mars just shortly after
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it was accreted from the solar nebula.
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By studying Mars, we'll
be able to learn more
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about Earth, Venus,
Mercury, even the moon,
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even exoplanets around other stars.
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(energetic music)
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(light explodes)
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(upbeat music)
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(flame roars)
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- [Narrator] ESA's Trace
Gas Orbiter mission
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arrived at Mars some time ago.
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Since then, this 3.5 ton spacecraft
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has been gently brushing the atmosphere
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to gradually adjust its orbit.
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In ESA's Planetary Missions Control Room
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in Darmstadt, Germany,
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flight controllers have
been checking systems
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and commissioning instruments
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on the ExoMars Trace Gas Orbiter.
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Now it's ready to begin
its science mission.
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- It has been a long time
since we arrived at Mars
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in October 2016,
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and we have had a long, very long period,
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one year of aerobraking,
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which consisted in
reducing the orbital period
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from the time when we arrived
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where it was actually
several days, to two hours,
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which is the nominal period
for science observations.
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(mumbling)
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I'm looking forward to the
next few months enormously
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because with TGO,
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we'll finally be able to
show its full capability,
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the full capability of its instruments
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in terms of accuracy and
the quantity and quality
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of data, pictures, spectra.
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And also because we will
be able to do joint starts,
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joint observations, with our
previous space traffic Mars,
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Mars Express, which is
still alive and working
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after 15 years, actually.
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And having two space craft around Mars
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in complementary orbits, from
a scientific point of view,
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is very exciting and
will allow, certainly,
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some very interesting
discoveries and observations.
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(machinery rumbles)
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- [Narrator] ExoMars
will fill a double role
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when its partner rover
is dispatched to Mars
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in the coming months
in the search for life
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on the dusty planet.
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(machinery rumbles)
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- It is a communications satellite,
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on top of being a science orbiter.
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And the so-called relay function
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allows us to communicate
with all landers and rovers
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on the surface of Mars.
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At the moment, we are only
rovers and landers from NASA,
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Curiosity and Opportunity.
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Some tests had been done already,
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soon after arrival at Mars.
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And now we are gonna start a campaign
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to calibrate and datamine
the best performance
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to relay data.
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- [Narrator] The Trace Gas Orbiter's
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primary mission, however,
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is to identify gasses in
the Martian atmosphere,
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particularly methane,
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first hinted at by Mars Express,
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and then by NASA's Curiosity Rover
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as it sniffed the atmosphere
with special sensors.
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- Well, we know that the lifetime
on methane is very short,
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just a few hundred years.
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It will be broken down by the sunlight,
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by the UV, ultraviolet
component of the sunlight,
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so if it is there now, we knew
that it has to be refilled
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all the time.
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And where does it come from?
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That's the big question.
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It cannot be synthesized
really in that atmosphere.
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It has to come from the
surface or from the subsurface.
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But what are the processes
that produces it?
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This is what we want to find out.
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One possibility is that it
is some geological reaction
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between minerals and water.
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Another possibility is that
actually those are microbes
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down buried underneath the surface
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that is producing it
today or has produced it
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a long time ago and they are all dead now,
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but that the methane had
been kept underground
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and with some mechanism is released
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to get up into the atmosphere.
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So these are all these kind
of things we try to find out.
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(calming music)
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- [Narrator] By using the
orbiter's powerful spectrometer,
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scientists hope to discover
whether the methane
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comes from a geological
or biological source.
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95% of methane on our own planet
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comes from living organisms.
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The ExoMars Rover, landing in 2021,
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will drill up to two
meters beneath the surface
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to search for this evidence of life.
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And the rover, as well as
NASA rovers and landers,
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will use the orbiter to
keep in touch with Earth.
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Mars exploration is an
international endeavor,
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and every mission adds
to our understanding
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of this alien world.
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A place that some of us
might someday call home.
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- Planetary exploration
is always very exciting,
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but Mars, of course, has
its very special thing,
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is that there's actually a place
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that you can imagine yourself
walking on eventually,
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within a not-too-far time in the future.
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Surely, people will be walking on Mars.
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That makes us very exciting.
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And then to think about
this idea that there might
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have been some kind of life,
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or even exist today underground on Mars.
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That makes it a very special place.
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(energetic music)
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(light explodes)
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(machinery rumbles)
(eerie music)
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- [Narrator] Curiosity
landed in Gale Crater
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on an ancient lake bed.
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A few months after arrival,
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it drilled into sedimentary rocks
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and detected traces of organic molecules
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using an instrument called SAM.
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(machinery rumbles)
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(machinery whirrs)
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- Well, the SAM instrument detected
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a variety of organic
molecules in a sediment
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that is from an ancient lake bed
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in the middle of Gale Crater.
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And what's important about these
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is that we now have a lot more certainty
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that there's organic molecules preserved
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at the surface of Mars.
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We didn't know that before.
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But what's interesting
is that we don't know
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what the source of these
organic molecules is right now.
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There's just not enough
information from that.
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However, if we drill deeper
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and we look around a little bit more,
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we might actually be able
to get to that information
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and tell, did they come from life?
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Did they come from geological processes?
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Or maybe they were from meteorites
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that were deposited in the lake.
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We just don't know right now,
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but hopefully we'll figure that out.
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(dramatic music)
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- [Narrator] Curiosity is searching
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for carbon-based organics.
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- SAM made the new detections
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by heating samples of crushed
rock to very high temperatures
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above 1000 degrees fahrenheit.
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This vaporized the samples,
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and released several species
of small hydrocarbons
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like benzene and propane.
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Because the hydrocarbons
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were released at such high temperatures,
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they may be the fragments of bigger,
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heavier molecules within the
rock, similar to kerogens.
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On Earth, kerogens are found in rocks
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like black shale and coal,
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and are the products of
ancient plant and bacteria.
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(technological music)
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- [Narrator] Some other
organics have been detected
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like thiophene, which contains sulfur.
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Introduced by geological processes,
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this sulfur acts as a preservative,
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binding organic molecules together
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and making them resistant to oxidation,
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so preserving them for millennia.
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- Organic molecules could
be the food for life,
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or they could be the product of life,
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or maybe they're from
something altogether different,
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such as geology or meteorites
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that were deposited into the lake.
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We don't know what the source
is, but there's a story there
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and we're going to uncover what that is.
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(machinery hums)
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- [Narrator] Scientists still
don't know if the discovered
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organics on Mars are biological in origin,
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but it's exciting to
find such old material
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preserved right at the surface.
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This finding is also encouraging
for future exploration.
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So for a time, Curiosity
continued to travel,
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find interesting outcrops,
drill holes, take samples.
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Then, inexplicably, something went wrong.
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- [Man] The drill's feed mechanism,
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which is responsible for
moving Curiosity's drill bit
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into and out of rocks,
didn't move when commanded.
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When Curiosity drills into a rock
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the way it was designed to,
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the drill's two stabilizer
posts touch the rock first
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to steady the arm while
the drill's feed mechanism
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moves the bit forward into the rock.
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(beeping)
(machinery hums)
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Without the feed mechanism
working, we can't drill that way.
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To solve this problem,
we do what we always do.
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We worked it out in the testbed
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using Curiosity's twin, Honor.
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Our team of engineers
and scientists have been
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working for months to figure out a way
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to collect and deliver rock samples
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without using the feed mechanism.
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Here's what we came up with.
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Using our new technique,
called Feed Extended Drilling,
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the stabilizers are not used.
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The bit is now in a forward position
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extended past the stabilizers.
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Moving the drill straight into
a rock and retracting safely
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without the stabilizers is challenging.
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We move the arm instead
of the feed mechanism
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to place the bit onto the rock
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and press it forward as it drills.
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- [Operator] Now let's
start holes beginning, over.
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- [Man] After making contact,
we apply a light preload
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and drill a shallow pilot hole.
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We use a force sensor in the robotic arm
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to give Curiosity a sense of touch.
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(machine whirring)
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This lets Curiosity adjust its arm motion
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and avoid getting stuck while drilling.
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Kind of like you might adjust your arm
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while drilling into a wall at home.
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After drilling, we use a similar technique
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to retract from the hole
without getting stuck.
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(technological music)
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- [Narrator] With Rover
2020 design and construction
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well underway,
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engineers will be sure
to avoid such a problem
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with Curiosity's cousin,
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which will land in the
Jezero Crater in 2020.
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(upbeat music)
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00:18:30,017 --> 00:18:32,289
(energetic music)
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00:18:32,289 --> 00:18:35,039
(light explodes)
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(inspiring music)
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2020 will be a banner year
for the exploration of Mars.
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In addition to the launch
of NASA's Mars 2020 Rover,
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the European Space Agency and Roscosmos
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are sending the ExoMars
Rover to the red planet.
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(machinery whirring)
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Rover 2020 and its companion helicopter
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will no doubt expand our search
for life, past or present.
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However, the big advance
forward in organic analysis
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will be the game changer.
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Both rovers will carry onboard a MOMA.
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(cool music)
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- The Mars Organic
Molecule Analyzer, or MOMA,
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is the largest and most complex
instrument on the rover.
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Its mass spectrometer subsystem
and its main electronics
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were built and tested at NASA's
Goddard Space Flight Center,
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which also contributed mass spectrometers
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to NASA's Curiosity
Rover and MAVEN Orbiter.
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MOMA is designed with a
mix of proven hardware
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and innovative new technologies.
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Here's how it works.
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In gas chromatrograph
mode, crushed Martian rock
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is put into an oven and
heated to 900 degrees celsius
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in just two minutes,
vaporizing the sample.
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Molecules of hot gas rise up
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and flow into a narrow,
20 meter long tube.
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Special coatings inside
the tube cause molecules
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with certain chemistries to
slow down more than others,
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separating the mixture
of molecules over time.
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Next, a beam of electrons
ionizes the molecules,
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giving them a positive electric charge
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and deflecting them towards
the linear ion trap.
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00:21:08,130 --> 00:21:11,100
The ions are caught by a
fluctuating electric field
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and sent to a detector to
determine their chemical makeup.
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While gas chromatography
has been used to study Mars
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since the Viking Program,
390
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MOMA has a second method
for preparing samples
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that has never been
used on another planet.
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00:21:24,733 --> 00:21:25,566
(shards clinking)
393
00:21:25,566 --> 00:21:26,960
In laser desorption mode,
394
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a sample is placed beneath a
powerful ultraviolet laser.
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00:21:31,185 --> 00:21:32,018
(laser bloops)
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A beam of energetic light
builds within the laser
397
00:21:34,570 --> 00:21:36,610
and fires in a billionth of a second,
398
00:21:36,610 --> 00:21:38,610
concentrating its energy onto a spot
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00:21:38,610 --> 00:21:40,407
smaller than a grain of sand.
400
00:21:40,407 --> 00:21:41,240
(laser boops)
401
00:21:41,240 --> 00:21:43,720
This rapidly vaporizes
a portion of the sample,
402
00:21:43,720 --> 00:21:45,640
releasing large organic molecules
403
00:21:45,640 --> 00:21:48,360
that could be broken down by oven heating.
404
00:21:48,360 --> 00:21:51,540
The laser shot also ionizes
some of the molecules,
405
00:21:51,540 --> 00:21:53,300
allowing the vapor to head directly
406
00:21:53,300 --> 00:21:55,460
to the linear ion trap.
407
00:21:55,460 --> 00:21:58,120
Neutral molecules are ejected by a vacuum
408
00:21:58,120 --> 00:22:00,470
while the remaining ions
are sent to the detector
409
00:22:00,470 --> 00:22:02,930
to determine their chemical makeup.
410
00:22:02,930 --> 00:22:04,810
Laser desorption will enable MOMA
411
00:22:04,810 --> 00:22:07,470
to detect long molecules like lipids,
412
00:22:07,470 --> 00:22:09,620
the building blocks of cell membranes,
413
00:22:09,620 --> 00:22:12,412
a leap forward in the
search for life on Mars.
414
00:22:12,412 --> 00:22:15,579
(inspirational music)
415
00:22:49,260 --> 00:22:50,880
- [Narrator] The question of life on Mars
416
00:22:50,880 --> 00:22:53,453
is among the most important
in planetary science.
417
00:22:55,200 --> 00:22:58,253
And the evidence may be
buried just below the surface.
418
00:23:00,010 --> 00:23:03,190
With the help of MOMA, we
will take one step closer
419
00:23:03,190 --> 00:23:04,813
to uncovering the answer.
420
00:23:05,760 --> 00:23:08,620
These images will pave the
way to a new understanding
421
00:23:08,620 --> 00:23:10,912
of life in our solar system.
422
00:23:10,912 --> 00:23:13,745
(energetic music)
32820
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