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In the 1970s, we
sent them to the outer
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planets, thinking they
might last five years.
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Forty years later, two little machines
called Voyager, with hearts of gold,
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are still going strong.
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I have to say, you know, Voyager is sort
of the love of my life.
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Now, more than 10
billion miles away, they're
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waving a long goodbye
to our solar system.
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A solar system that we hardly knew before
their fantastic journeys.
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Facing harsh radiation, crazy
temperatures, hails of particles,
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whiplash speeds.
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They faced mission-ending
catastrophes, failed, and were
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reborn, thanks to the
ingenuity of their human parents.
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The stunning payoff?
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Close encounters with our giant outer
planets and their moons.
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Completely unknown worlds with massive
volcanoes, some of lava, some of ice,
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internal seas, and lakes of methane.
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Places where life might take hold.
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And now, they're creatures of deep space.
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The Voyagers will be our silent
ambassadors to the Milky Way galaxy.
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And they're still phoning home with new
answers to our cosmic questions.
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These are the stories of a lonely blue
marble.
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Sending its intrepid little machines to
places no human can yet go.
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To the far ends of the solar system and
beyond.
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Landing a man on the moon and returning
him safely to the Earth.
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In 1964, as the world was riveted by the
race to the moon, a graduate student named
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Gary Fladro noticed something that would
ultimately take us far beyond the moon.
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The planets of the outer solar system were
spinning towards a rare alignment that
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would make it possible, in theory,
to hurl something off of Earth and have it
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slingshot past all the outer planets of
the solar system.
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Best of all, the craft could be sent close
enough to each planet to get whipped by
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gravity to higher and higher speeds using
almost no fuel.
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It was called the Grand Tour.
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And it wouldn't happen again for quite a
while.
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The Grand Tour was an opportunity that
happens once every 176 years when Jupiter,
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Saturn, Uranus and
Neptune were all lined up so a
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spacecraft could fly
by all four in its journey.
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It was a chance NASA couldn't pass up.
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The Grand Tour itself was
a very ambitious journey
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with four spacecraft flying
by all the outer planets.
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But it was much too
expensive for everything
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that was trying to be
done by NASA at the time.
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And they scaled it back to just a
four-year mission to Jupiter and Saturn.
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Unofficially, they never
gave up on the idea
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of a full Grand Tour
to Uranus and Neptune.
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They just kept their heads
down and tried to engineer
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the living daylights out of
the Voyagers, just in case.
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And so they would kind of fudge things
here and there or buy different parts that
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might cost a little bit more but would
make the mission last longer.
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So in some sense they went against what
their management would say, tell them they
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need to do, but they never told their
management.
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They just went and did
that and made that selection
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so the Voyager could
fly as long as possible.
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Voyagers 1 and 2 are identical spacecraft
made up of 65,000 separate parts.
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Each is equipped with instruments to
conduct 10 different experiments including
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television cameras,
infrared and UV
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sensors, magnetometers
and particle sensors.
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Each could radio
information directly to Earth or
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record data for sending
later on an 8-track tape.
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How 70s is that?
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Each Voyager also carried
a radical new computer
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that was self-testing
and self-repairing.
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Each craft weighed about the same as a
two-seater smart car, one that would have
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to be accelerated to 25,000 miles per hour
to escape the Earth's gravity.
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So, weeks apart in late summer 1977,
Titan Centaur rockets prepared to tear
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away from Cape Canaveral with their little
charges aboard.
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Voyager 2 left first.
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But Voyager 1 was sent on
a more direct route, meaning
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it would reach the outer
planets weeks ahead of its twin.
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Let us learn together and laugh together.
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Jimmy Carter was president.
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Star Wars had taken the world by storm.
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And two dropouts in a garage had invented
a personal computer named Apple.
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The Voyagers had
mothers who would be in
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charge of their day-to-day
care and feeding.
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Actually, the minutely detailed lines of
code telling them exactly what to do.
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Among them, Linda Spilker.
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I felt very maternal toward Voyager.
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And I know if anything would go wrong with
Voyager, we'd all worry until we got that
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signal back and the sign that everything
is okay and we're ready to go on.
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And later, Susie Dodd.
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It was super exciting.
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This is my first job out of college.
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And during the time of the encounters,
all the scientists came.
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Carl Sagan was here.
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And they would all come to JPL and look at
the data as it was coming down.
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The beginnings were not auspicious.
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Voyager 2 had computer glitches on the
launch pad.
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It appeared to get vertigo during lift-off
and almost didn't make it out of orbit.
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The first stage of the launch vehicle
underperformed.
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And the upper stage was just barely able
to do anything.
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It had to fix it on its own by literally
burning itself out of fuel.
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There's nothing you can do when that
happens.
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Then, just two hours
into the flight, Voyager 2
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seemed determined not to
speak to her human handlers.
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Her primary radio receiver failed.
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Very shortly after launch, we lost one of
the command receivers.
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So that's the way you can send a command
to let the spacecraft get new instructions.
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The other remaining command receiver was
tone-deaf.
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It could not tune to the frequency that we
were sending.
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And so that meant we had to learn on the
ground how to send the right frequency.
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So when it got to the spacecraft, it
was the one the spacecraft could listen to.
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And we learned how to do that.
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We flew the whole mission, our flying
mission today, always knowing where to
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find that frequency that is needed for
Voyager to actually hear it.
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The Voyager's first
encounters with Jupiter would
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take place during the
spring and summer of 1979.
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Jupiter is a very dangerous place.
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The massive planet emits incredibly harsh
radiation.
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No human would have survived aboard
Voyager.
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And during the approach,
Jupiter started attacking the
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probes, invisibly and
potentially catastrophically.
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The radiation was pinging the clock that
controlled the camera and putting it out
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of sync with the clock that controlled the
exposure.
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The engineers at JPL managed to come up
with a workaround.
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And everyone held their breaths as Jupiter
got larger and larger in the images.
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The Great Red Spot, discovered 300 years
earlier, turned out to be not one storm
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but hundreds swirling
within and around a giant,
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multicolored vortex more
than three Earths across.
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As we started 30 days out from Jupiter,
began to make a movie of the very complex
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storm systems in
Jupiter's atmosphere, the
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Great Red Spot is just
the largest hurricane.
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There are literally dozens of these storms
in this giant planet.
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And that was our first taste of the
discovery that was waiting for us.
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As Voyager 1 swung through
the system at 35,000 miles
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per hour, JPL went wild
at the quality of the images.
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But if Jupiter had amazed
them, the real shock
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would come from the
giant planet's moons.
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Io is Jupiter's innermost moon.
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A close look at the images revealed the
driest object in the solar system.
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But nobody was prepared for what showed up
next.
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And it took a graduate
student who was looking in
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the details of the images
and saw this big arc.
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And she said, hey, come and look at this.
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And people said, oh my God, volcano.
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It had eight active volcanoes when Voyager
flew by.
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It has ten times more
volcanic activity than
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the Earth, even though
it's just a small moon.
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And it had lakes of hot lava on its
surface.
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Let's not forget that before the Voyager
encounter with Jupiter and its moons,
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the only example of volcanoes we knew
about was Earth.
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How was it possible that this moon,
so far from the sun, in the deep cold,
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was erupting hot lava?
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Scientists had just started theorizing
that the incredible push and pull of
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Jupiter's gravity would squish and stretch
the moons, heating them up.
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And boy, did they.
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It turns out these moons are in orbit
around the giant Jupiter, and that creates
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a tide in the moon, just like the moon
creates a tide in our ocean.
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Well, Jupiter creates a tide in the moon
and deforms it.
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And that deformation as it works around
heats the moon.
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In the case of Io, it causes volcanic
activity.
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The team didn't think
they would run across other
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discoveries that were that
outrageous in the Jovian system.
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But Voyager's images at Jupiter's
second-closest big moon, Europa,
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were a shock as well.
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It was smooth as a bowling ball,
but scratched.
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It looked like the surface consisted of
millions of little plates, sort of what
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you would see when an ice pack is breaking
up during the spring.
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Could they possibly be skating over an
ocean?
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Europa essentially has a shell of ice that
could be as deep as 20 kilometers or more.
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And underneath that, however, there is
liquid water.
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And the ice itself is not absolutely
impermeable because we see cracks.
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We see stuff that has come from underneath
at various times.
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The implications were stunning.
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Life on Earth probably arose in a
primitive ocean.
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Did Europa have one?
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Later mission Galileo showed that it did
indeed.
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The largest ocean in the solar system.
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You have all the ingredients that we now
know constitute the elements of life.
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You have water.
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You've got apparently organic material.
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And you've got the source of energy,
which is the heat generated by the
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gravitational pull from
Europa and Jupiter and Io that
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continuously charms this
underground under-ice ocean.
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And the other moons followed suit.
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Europa, Ganymede, and possibly even
Callisto appear to have vast oceans of
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liquid water under relatively thin shells
of ice.
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Where scientists had expected dark,
dead cratered moons like our own,
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they found mysteriously dynamic worlds.
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And those tiny moons that
were basically points of light and
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telescopes from the ground
suddenly started to be revealed.
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First Callisto, ancient and cratered,
then Ganymede with its grooves and
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tectonic activity, bright white icy
Europa, and then active Io.
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So these points of light became worlds in
their own right.
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There was little time to celebrate.
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In just 16 months, the Voyagers were
hurtled by the crown jewel of our solar
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system, Saturn, which
turned out to be more beautiful
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than anyone could have
imagined and nearly as dangerous.
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It was a time of Pac-Man, Reagan,
and the birth of the 24-hour news cycle.
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In November 1980, Voyager 1 swung through
the Saturnian system, around behind the
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rings, and made a beeline for its largest
moon, Titan.
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Earth-based telescopes
had shown that Titan had an
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atmosphere, making it the
must-see destination for scientists.
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Voyager 1 could not see through the haze
to the surface, but it could register that
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the atmosphere was largely nitrogen,
just like Earth's.
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There was methane as well.
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Methane, we'd later discover, was so cold
that it probably snowed on Titan's surface.
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Enceladus, Saturn's sixth
largest moon, was brilliant
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white, the most reflective
body in the solar system.
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It was another candidate for having a
liquid ocean beneath its icy surface.
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And later, the Hubble telescope would catch
it in the act of actually erupting water.
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Voyager also found that Saturn didn't have
three rings.
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It had thousands.
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Some with spokes.
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Some that twisted, and braided,
in ways that stumped the scientists.
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The shimmering rings were made up of three
rings.
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Full of tiny grains of water ice.
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And were unbelievably thin.
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For comparison, if Saturn were shrunk down
to the size of a basketball, then the
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thickness of the rings would be about
1,250th the width of a human hair.
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We didn't know what the rings would look
like.
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We thought we'd see bland sheets of
material separated by gaps.
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But instead we found incredible,
wonderful detailed structure.
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00:14:19,951 --> 00:14:23,750
And I remember in those days you didn't
have a computer screen where you could
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call up a picture of the
rings and instead you had to
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get the data and plot it
out in this long roll of paper.
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And I remember taking those rolls and
unrolling it in the hall and just walking
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slowly, looking down thinking,
I'm walking through the rings of Saturn.
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And what a wonderful feeling.
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Having finished its official
mission, Voyager 1 was
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slung up and out of the
plane of the solar system.
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This cleared the way for what everyone had
in mind.
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That Voyager 2 could complete the grand
tour and visit more planets after Saturn.
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But only by sending it
careening dangerously close to
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Saturn's surface to make
a hard left toward Uranus.
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Then Voyager 2 slipped into the shadow of
the planet.
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And the images suddenly went dark.
227
00:15:24,100 --> 00:15:25,620
Had they come this far?
228
00:15:25,780 --> 00:15:27,940
With Uranus and Neptune in their sights?
229
00:15:28,540 --> 00:15:30,700
Only to have lost their robotic eyes.
230
00:15:33,400 --> 00:15:36,940
After the Saturn flyby, the Voyager 2 scan
platform got stuck.
231
00:15:37,140 --> 00:15:38,580
And it just wouldn't move.
232
00:15:38,720 --> 00:15:41,420
And so we just saw outbound these pictures
of Saturn.
233
00:15:41,460 --> 00:15:45,040
We wondered, could we fix it in time to
get to Uranus?
234
00:15:46,080 --> 00:15:48,360
Voyager 2 emerged from behind the planet.
235
00:15:48,820 --> 00:15:49,820
Directly on course.
236
00:15:50,260 --> 00:15:51,920
And accelerating like mad.
237
00:15:52,320 --> 00:15:54,680
Thanks to the gravity boost from the close
flyby.
238
00:15:56,000 --> 00:15:59,185
But it looked like the camera
platform had balked at the sheer
239
00:15:59,186 --> 00:16:02,160
speed of the commands it had
to execute to take stable images.
240
00:16:03,800 --> 00:16:08,760
The engineers studied the phenomenon and
figured out a way of how to pulse it
241
00:16:08,761 --> 00:16:13,800
enough to make the platform move at a
fairly constant rate.
242
00:16:16,600 --> 00:16:21,540
And just the hours of people studying and
thinking and finding ways to fix it.
243
00:16:21,640 --> 00:16:22,676
And then we were all cheering.
244
00:16:22,700 --> 00:16:25,380
Yes, we found a way to keep the Voyager
mission going.
245
00:16:28,820 --> 00:16:31,133
But how would they take
pictures at Uranus when
246
00:16:31,134 --> 00:16:33,981
they'd be moving 20,000
miles per hour faster?
247
00:16:34,330 --> 00:16:36,700
And the sunlight would be four times
fainter.
248
00:16:37,780 --> 00:16:40,100
It would require the most ingenuity yet.
249
00:16:44,820 --> 00:16:48,400
Susie Dodd joined the Voyager team in time
for the approach to Uranus.
250
00:16:50,160 --> 00:16:53,734
So in order to make what
you want to look at bright
251
00:16:53,735 --> 00:16:56,861
enough, you really have
to stare at it for a while.
252
00:16:57,310 --> 00:17:00,184
But your spacecraft is
tracking so fast, it'd be like trying
253
00:17:00,185 --> 00:17:03,340
to take a picture of a sign
as your car is whizzing by it.
254
00:17:03,440 --> 00:17:04,860
You know, you have to track that.
255
00:17:05,420 --> 00:17:09,800
And we designed attitude control software
so that we could track the target we were
256
00:17:09,801 --> 00:17:14,340
looking at in order for the exposure not
to be smeared or to be too dark an image.
257
00:17:15,470 --> 00:17:18,880
Five years after the Saturn flyby,
they were ready for Uranus.
258
00:17:19,000 --> 00:17:20,300
Or so they hoped.
259
00:17:21,940 --> 00:17:24,660
I'll do my utmost to be deserving of your
trust.
260
00:17:28,600 --> 00:17:31,540
Uranus rolls around the Sun rather than
spins.
261
00:17:32,580 --> 00:17:37,560
Voyager 2 would fly through the bullseye
of its system like an arrow at 51,000
262
00:17:37,561 --> 00:17:41,080
miles per hour, passing close to the
innermost Moon.
263
00:17:41,920 --> 00:17:42,920
Tiny Miranda.
264
00:17:44,020 --> 00:17:48,000
As crazy as the Saturn flyby had been,
it had taken three days.
265
00:17:48,600 --> 00:17:51,040
This time, they would have just ten hours.
266
00:17:55,000 --> 00:17:58,740
Miranda turned out to be one of the most
geologically bizarre bodies in the solar
267
00:17:58,741 --> 00:18:04,320
system, with crazy V-shaped grooves and
50,000-foot-tall ice cliffs.
268
00:18:05,080 --> 00:18:09,940
To this day, we don't fully understand this
strange patchwork quilt of a mini-moon.
269
00:18:10,480 --> 00:18:13,320
I kind of like Miranda, which is one of
Uranus's moons.
270
00:18:13,420 --> 00:18:16,720
It's a small moon, and it has this big
checkmark in the middle of it.
271
00:18:16,760 --> 00:18:18,700
It's like, okay, you know, I'm okay.
272
00:18:18,740 --> 00:18:19,440
I'm here, Mom.
273
00:18:19,560 --> 00:18:20,820
I'm here, planet Uranus.
274
00:18:22,180 --> 00:18:26,580
The Uranus flyby and images completely
surpassed what JPL had hoped for.
275
00:18:27,655 --> 00:18:31,900
Voyager 2 was now five years beyond her
original mission, all those years ago.
276
00:18:32,520 --> 00:18:35,025
The engineers' secret
plans to keep the probe
277
00:18:35,026 --> 00:18:38,081
going through the Grand
Tour were paying off.
278
00:18:38,760 --> 00:18:42,980
And now, Voyager 2 was headed towards its
last planet, Neptune.
279
00:18:44,520 --> 00:18:50,566
It arrived just 62 miles off its target,
just above Neptune, after traveling 4.
280
00:18:50,567 --> 00:18:51,641
4 billion miles.
281
00:18:52,100 --> 00:18:56,800
Something lead designer Charlie Culhays
estimated was roughly equivalent to a
282
00:18:56,801 --> 00:18:59,960
golfer sinking a putt from Washington,
D.C.
283
00:19:00,540 --> 00:19:01,940
to Phoenix, Arizona.
284
00:19:08,190 --> 00:19:10,130
The movies of the approach are eerie.
285
00:19:12,460 --> 00:19:16,170
There was a large, dark, oval-shaped
feature in Neptune's southern hemisphere,
286
00:19:17,470 --> 00:19:19,830
similar in shape to Jupiter's great red
spot.
287
00:19:22,210 --> 00:19:26,550
And when small white clouds came into
view, it confirmed another giant
288
00:19:26,551 --> 00:19:30,110
Earth-sized storm system, which shouldn't
be there.
289
00:19:31,110 --> 00:19:35,527
Neptune has about 900 times
less light than here on Earth,
290
00:19:35,528 --> 00:19:38,810
yet it has the fastest winds
that we saw in the solar system.
291
00:19:39,090 --> 00:19:42,350
Well, I think nobody knew that there was
this giant storm at Neptune.
292
00:19:42,550 --> 00:19:44,770
Now, that storm doesn't exist anymore.
293
00:19:45,245 --> 00:19:50,020
From 1990 to 2016, where
we are today, that storm has
294
00:19:50,021 --> 00:19:53,311
dissipated and is no longer seen
in the atmosphere of Neptune.
295
00:19:53,450 --> 00:19:54,450
That's kind of neat.
296
00:19:55,430 --> 00:19:59,070
After swinging just 3,000 miles,
above the cloud tops of Neptune,
297
00:19:59,750 --> 00:20:04,170
Voyager 2's trajectory would take it past
one final, glorious, unknown destination.
298
00:20:05,050 --> 00:20:06,590
The moon, Triton.
299
00:20:08,410 --> 00:20:12,830
And yet again, the scientists would be
greeted by an inexplicable object.
300
00:20:14,510 --> 00:20:16,030
An explosive one.
301
00:20:18,850 --> 00:20:20,090
Triton was a very big surprise.
302
00:20:20,150 --> 00:20:23,050
It's very cold, only 40 degrees above
absolute zero.
303
00:20:23,580 --> 00:20:26,670
The nitrogen is frozen into an icy polar
cap that's so cold.
304
00:20:26,671 --> 00:20:30,358
And yet, we found several
active geysers erupting
305
00:20:30,359 --> 00:20:33,471
from that surface at 40
degrees above absolute zero.
306
00:20:33,670 --> 00:20:34,670
Another big surprise.
307
00:20:36,990 --> 00:20:41,590
With that last flyby, Voyager 2 was hurled
slightly south of the plane of the solar
308
00:20:41,591 --> 00:20:44,910
system, on its own search for interstellar
space.
309
00:20:48,090 --> 00:20:51,250
For the team at JPL, it was a bittersweet
time.
310
00:20:52,050 --> 00:20:53,470
We were all excited.
311
00:20:53,590 --> 00:20:54,270
The press was here.
312
00:20:54,350 --> 00:20:55,350
It was in the news all the time.
313
00:20:55,351 --> 00:20:56,090
It was very thrilling.
314
00:20:56,270 --> 00:20:59,490
And then the press kind of left,
and the news died down.
315
00:21:00,270 --> 00:21:02,470
And you still had the spacecraft,
which was kind of sad.
316
00:21:02,530 --> 00:21:08,330
It was now off, going out into the cold,
dark space on its own, alone.
317
00:21:09,610 --> 00:21:14,330
It's estimated that a total of 11,000 work
years were devoted to the Voyager Grand
318
00:21:14,331 --> 00:21:16,690
Tour, equivalent to a
third of the labor force
319
00:21:16,691 --> 00:21:19,911
needed to complete the
Great Pyramid at Giza.
320
00:21:20,090 --> 00:21:22,410
The results were nothing short of
revolutionary.
321
00:21:23,470 --> 00:21:25,978
The Voyagers really changed
our visions of the outer solar system
322
00:21:25,979 --> 00:21:30,350
by showing it to be a far more
dynamic place than expected.
323
00:21:32,730 --> 00:21:34,650
But the Voyagers weren't done yet.
324
00:21:34,870 --> 00:21:36,110
Not by a long shot.
325
00:21:36,990 --> 00:21:39,740
Now, both probes were
headed out of the plane of
326
00:21:39,741 --> 00:21:41,991
the solar system, still
functioning perfectly.
327
00:21:42,690 --> 00:21:46,350
There was a chance that if they could hold
on for another five or ten years,
328
00:21:46,610 --> 00:21:51,310
they could reach interstellar space,
beyond the influence of our sun.
329
00:21:51,810 --> 00:21:54,110
Well, Voyager flew very quietly.
330
00:21:54,850 --> 00:22:00,250
And I would say very much sort of in the
background while we were landing
331
00:22:00,251 --> 00:22:04,190
spacecraft on Mars and Cassini was up
taking great images of Saturn.
332
00:22:05,050 --> 00:22:09,950
For another dozen years, the Voyagers,
now 30 years past their sell-by dates,
333
00:22:10,130 --> 00:22:16,331
logged the diminishing force of the sun's
gravity, its magnetism, and the solar wind.
334
00:22:16,790 --> 00:22:21,310
They found all kinds of bizarre
formations, including a magnetic bubbling
335
00:22:21,311 --> 00:22:26,010
at the outer limits that protects us from
deadly cosmic rays, blasted out of the
336
00:22:26,011 --> 00:22:28,170
hearts of supernovas throughout the
galaxy.
337
00:22:29,590 --> 00:22:34,890
Today is a historic moment for NASA,
the Voyager team, and in fact, humankind.
338
00:22:35,030 --> 00:22:38,370
Well, this is the spacecraft, the first to
interstellar space.
339
00:22:38,590 --> 00:22:39,590
We made it!
340
00:22:39,810 --> 00:22:44,810
It was tremendously exciting to think that
a spacecraft I had worked on, I had been a
341
00:22:44,811 --> 00:22:48,382
part of, was actually now
leaving our solar system and
342
00:22:48,383 --> 00:22:51,570
going out for the first
time into interstellar space.
343
00:22:53,080 --> 00:22:56,160
Any of the particles that are hitting
Voyager now are coming from other stars.
344
00:22:56,270 --> 00:22:57,550
They're not coming from our sun.
345
00:22:57,990 --> 00:23:00,898
So we're actually measuring
for Voyager 1 particles
346
00:23:00,899 --> 00:23:03,371
and dusts and winds that
are coming from other stars.
347
00:23:03,850 --> 00:23:10,170
It's the very first time that humanity
sort of moved out of the cocoon of the
348
00:23:10,171 --> 00:23:13,581
solar atmosphere to
venture beyond the solar
349
00:23:13,582 --> 00:23:17,411
system and into the
source of the galaxy.
350
00:23:17,890 --> 00:23:21,150
That only happens once, and it happened in
our lifetime.
351
00:23:22,830 --> 00:23:26,610
The Voyagers are now flying blind,
feeling their way through the universe.
352
00:23:27,460 --> 00:23:29,549
Their cameras shut down
to preserve the tiny bit
353
00:23:29,550 --> 00:23:31,910
of power left in their
little nuclear power plants.
354
00:23:33,740 --> 00:23:38,170
With a little luck and pluck, these will
keep generating energy for another decade.
355
00:23:39,650 --> 00:23:42,970
So we think we can operate all the
instruments until 2020.
356
00:23:43,110 --> 00:23:44,670
We should have enough power to do that.
357
00:23:44,770 --> 00:23:47,206
But after that, we'll be turning off one
instrument at a time.
358
00:23:47,230 --> 00:23:52,090
And probably by 2025, we won't be able to
have any more science instruments on.
359
00:23:52,091 --> 00:23:55,270
But my personal goal is to operate the
spacecraft for 50 years.
360
00:23:55,660 --> 00:23:58,570
So I want to see it operating at least
until 2027.
361
00:24:01,110 --> 00:24:05,390
Remarkably, Voyager's controllers still
talk to the probes every day, despite the
362
00:24:05,391 --> 00:24:07,839
fact that the signal
from so far away is
363
00:24:07,851 --> 00:24:10,551
down to about a
billion billionth of a watt.
364
00:24:10,980 --> 00:24:12,330
But it can't last forever.
365
00:24:14,120 --> 00:24:18,810
Yeah, one day, it's going to be a very sad
day, but one day we will expect to hear
366
00:24:18,811 --> 00:24:20,610
from the spacecraft, and we won't hear
from it anymore.
367
00:24:20,611 --> 00:24:26,070
And we will send a lot of commands from
the ground to try and recover it,
368
00:24:26,305 --> 00:24:29,430
and we'll try different things,
but eventually it won't have enough power
369
00:24:29,431 --> 00:24:32,210
for the transmitter, and so it'll just
stop transmitting data.
370
00:24:32,945 --> 00:24:35,702
And then it will just be
our silent ambassador
371
00:24:35,703 --> 00:24:38,391
traveling around the center
of the Milky Way galaxy.
372
00:24:38,760 --> 00:24:40,190
But it's still on a big adventure.
373
00:24:40,770 --> 00:24:43,051
It's just that I won't get to know what
that adventure is.
374
00:24:44,570 --> 00:24:47,247
It will be another 40,000
years before Voyager 1
375
00:24:47,248 --> 00:24:50,031
drifts within shouting
distance of another star.
376
00:24:51,305 --> 00:24:54,561
Just in case there's
intelligent life out there ready to
377
00:24:54,562 --> 00:24:57,610
snag it, they'll discover
Voyager's message to the universe.
378
00:24:58,190 --> 00:25:02,290
A 12-inch gold-plated record containing
greetings in dozens of languages.
379
00:25:02,510 --> 00:25:05,050
Hello from the children of planet Earth.
380
00:25:07,010 --> 00:25:10,330
Samples of music and sounds of nature.
381
00:25:11,170 --> 00:25:14,450
Hints of an Earth and a people that may
long have perished.
382
00:25:15,970 --> 00:25:18,666
That record has the
sights and sounds of the
383
00:25:18,667 --> 00:25:21,190
Earth, pictures, songs,
people saying hello.
384
00:25:21,510 --> 00:25:26,410
And so maybe someday some other
civilization will find Voyager.
385
00:25:26,550 --> 00:25:29,162
And there's even
directions on the cover of
386
00:25:29,182 --> 00:25:32,050
the record of how to
find us, where we are.
387
00:25:34,170 --> 00:25:36,726
They will be orbiting
every 240 million years
388
00:25:36,727 --> 00:25:40,031
around the center of
the Milky Way galaxy.
389
00:25:40,170 --> 00:25:45,450
Year after year after year for billions of
years, carrying this plaque and record
390
00:25:45,451 --> 00:25:48,930
saying we sent this to the Milky Way
galaxy.
391
00:25:50,310 --> 00:25:55,590
This kind of adventure doesn't happen
often in human affairs, and I think
392
00:25:55,591 --> 00:26:01,410
Voyager is the the Columbus, if you like,
of the space era of discovery.
393
00:26:03,690 --> 00:26:07,183
Voyager is still doing
path-breaking science
394
00:26:07,195 --> 00:26:10,311
as we speak, and it
continues to do so.
395
00:26:10,490 --> 00:26:13,170
You can't do it any better than that.
37262
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