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Narrator: Nasa's revolutionary
           juno probe

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      is on a daring voyage
           to jupiter.

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      Its goal -- to reveal
    the the deepest mysteries

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      of our solar system.

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        Everything we see
    in the solar system today

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     is affected by jupiter
   somehow in the past or now,

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       all the asteroids,
        all the planets,

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           the moons,
     the comets, everything.

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    So in many ways, juno is
    actually giving us a view

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into the history
    of our planetary system,

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   even the history of earth.

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            Narrator:
    Juno's mission is risky.

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        Jupiter could eat
    the spacecraft like that.

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     Narrator: But by diving
        perilously close

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    to this monstrous world,

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  juno could change everything
 we know about our solar system.

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       If you want to know
        what's happening,

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        you got to get up
       close and personal.

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                     ♪

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[ electricity crackles ]

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          [ explosion ]

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     -- captions by vitac --
          www.Vitac.Com

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      captions paid for by
    discovery communications

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                     ♪

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            narrator:
    Independence day, 2016--

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     juno arrives at jupiter

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        and gets to work.

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      The probe angles its
     high-resolution camera

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   towards this stormy world.

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 Juno's snaps do not disappoint.

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♪

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  the images returned from juno
       are just beautiful.

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                     ♪

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                     ♪

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  plait: Suddenly you have this
       magnificent mosaic

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         of this planet.

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                     ♪

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   as a human being, I'm like,
   "oh, my gosh, look at this.

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    This is amazing. This is
   coming back from jupiter."

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       narrator: These are
     the closest-ever views

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           of jupiter,
 a world 500 million miles away.

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♪

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     but we didn't send juno
     just to take pictures.

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One of its main goals is to peer
 deep into jupiter's dark heart.

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    One of the big questions
    we have about jupiter is,

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      does it have a core?

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     And you'd think, well,
     of course it has a core

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  like every planet has a core.

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      The earth has a core.
        Everything does.

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       Well, it turns out,
       jupiter might not.

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 Narrator: Knowing what lies at
a planet's core

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 allows scientists to wind back
   the clock billions of years

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        to the formation
         of the planets.

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  If juno can reveal what lies
      deep within jupiter,

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         it could change
        our understanding

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  of how the gas giant formed.

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   If juno finds a solid core,
          it could mean

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      jupiter first formed
  as a rocky planet like earth

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       then kept growing,

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   but if juno finds no core,

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       it could mean that
jupiter skipped the rocky stage

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       and formed straight
      from a cloud of gas.

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                     ♪

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     answering this question
       could shine a light

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    on other mysteries, too.

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      If we can figure out
       how jupiter formed,

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  we can figure out the rest of
 the story of the solar system.

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                     ♪

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    so how do you probe down
  into the interior of a planet

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   when all you can really see
are the very tops of the clouds?

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Well, incredibly,
      you can use gravity.

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     As juno orbits jupiter,

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    it can sense in its orbit

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     tiny little variations

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    in the gravitational pull
           of jupiter.

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            Narrator:
 As juno speeds around jupiter,

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      gravitational spikes
        tug on the craft.

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Turns out, some parts of jupiter
     are denser than others.

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If jupiter were some solid ball,
   then as juno passes by it,

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     as it passes very close
      above its cloud tops,

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the orbit, the trajectory
      would be very smooth,

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          but in fact,
     if jupiter has layers,

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         or places where
       there is more mass

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 and places where there's less,
  then it's gonna pull on juno

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    a little bit differently.

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  Narrator: Passing over areas
      of concentrated mass

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    gives juno a speed boost.

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       So what they do is,
   the engineers back on earth

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     can basically just say,

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     "how fast is it moving
           right now?

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How about now?
         How about now?"

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    and you build up a map of
  where the mass is in jupiter

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    underneath the spacecraft
      as it passes around.

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  Narrator: Juno's instruments
        begin to map out

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     the heart of gas giant,

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  revealing the mysterious core
       for the first time.

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       What juno found was
      this amorphous mass,

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          a fuzzy thing
    in the center of jupiter.

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It's not as solid as we expected

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         if it were just
a metal and rock core,

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  but there is something there.

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            Narrator:
  In the center of the planet,

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      juno detects hydrogen
       and rocky material

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 dissolved and blended together.

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  It's a type of planetary core
    we've never seen before.

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           Astronomers
      describe it as fuzzy.

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  We thought we were gonna find
           an avocado.

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        Instead, we found
        a bowl of chili.

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      It's a hydrogen fluid
        chili con carne.

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♪

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      so none of our models
   of the interior of jupiter

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    turned out to be correct.

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  That means we have to go back
      to the drawing board.

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            Narrator:
   One theory is that jupiter

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  didn't form from rocks or gas

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      but from tiny pebbles
  less than an inch wide strewn

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  across the early solar system
     4.6 billion years ago.

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  These pebbles came together.

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      They accreted to form
        a massive object

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that was the sort of seed,
      the core of jupiter.

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 Narrator: The swarm of pebbles

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        clumped together
     to form one giant core

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   20 times the mass of earth,

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 but these pebbles can't sustain
  this growing planet for long.

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           Eventually,
     we need to make a jump

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   from those centimeter-size
            particles

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 up to really large things, like
  100-kilometer planetesimals,

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   to really kick-start growth
          of a planet.

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                     ♪

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narrator: As jupiter grows,
its appetite becomes insatiable.

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       The cores of other
  would-be planets are drawn in

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       by its immense pull
      and absorb on impact,

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     causing jupiter's core
          to transform.

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  Huge chunks of incoming rock
      are mixed up with gas

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         and the pebbles
 that originally built the core.

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We think that core material that
 might've been there is actually

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     dissolved and mixed in
  with the rest of the planet.

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Narrator: This mix of rock,
        gas, and pebbles

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         leaves the core
       in a strange state

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            somewhere
    between solid and liquid

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   or, in other words, fuzzy.

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   Once jupiter's core reaches
        a critical mass,

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        its gravity pulls
   in all nearby hydrogen gas,

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 building the jovian atmosphere

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   and leaving the fuzzy core

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    trapped beneath thousands
    of miles of thick clouds.

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 And that is what formed jupiter
as we know and love it today.

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  Narrator: Juno's discovery of
      jupiter's fuzzy core

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    could rewrite the book on

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 jupiter's early years, but juno
    is just getting started.

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    We haven't even scratched
           the surface

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          of the number
     of mysteries there are.

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    Narrator: There's more to
   jupiter than meets the eye

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      as juno's instruments
  begin to reveal a darker side

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      to this giant world.

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      Jupiter's environment
is one of the most vicious

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      in the solar system,
       and that's because

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        of its incredibly
     strong magnetic field.

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  Narrator: And juno is caught
   right in the middle of it.

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                     ♪

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 narrator: The gas giant jupiter

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  holds clues to the mysteries
      of our solar system,

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          and in 2011,

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 nasa launched a billion-dollar
    mission to uncover them.

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 Man: Three, two, one, ignition.

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   And liftoff of the atlas v

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with juno on a trek to jupiter.

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 Narrator: To reach its target,

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          juno embarks
     on a five-year journey.

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                     ♪

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     sending any spacecraft
        to another planet

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       is gonna be tough,
   but sending one to jupiter

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            is really
   pushing things pretty hard.

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  Narrator: Juno weaves through
        the solar system

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     with extreme precision.

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    The craft battles violent
       temperature changes

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     and navigates carefully
through the asteroid belt.

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   If there's a fleck of dust
          in your path

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      and that thing slams
      into your spacecraft,

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 it could do significant damage.

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   Narrator: 1.7 billion miles
        into its mission,

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 juno finally nears its target,

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    but the probe is hurtling
         towards jupiter

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    at 165,000 miles an hour.

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   Juno is moving really fast.

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           It's one of
  the fastest spacecraft ever.

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   You need to go fast enough
to get there, but then you need

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to be slow enough to be captured
  by the gravity of the planet.

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 You need to get it just right.

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            Narrator:
      Entering orbit around

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  jupiter is the trickiest part
         of the mission.

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Get it wrong and juno could slam
         into the planet

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  or drift out into deep space.

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    To successfully get juno
 to enter a stable orbit around

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             jupiter
   as almost the same as, say,

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      shooting a basketball
from london

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  and having it on the land on
the front of the rim in new york

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     and just sitting there
            balanced.

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   I could do it, but can nasa
        do it with juno?

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          [ laughing ]

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            narrator:
   Nasa has a neat game plan.

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    Juno performs a backflip
            in space

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     and fires its thruster
        towards jupiter.

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  Everything is going smoothly.

205
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    We're continuing to burn
    and change our velocity.

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00:10:41,174 --> 00:10:44,709
Narrator: The rocket burns for
     35 nail-biting minutes,

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   reducing the craft's speed
     by 1,200 miles an hour.

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                     ♪

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00:10:53,854 --> 00:10:55,286
          [ cheering ]

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  narrator: Finally, the probe
 achieves orbit around jupiter.

211
00:10:59,026 --> 00:11:01,426
    Bolton: Right on July 4th
      during the fireworks

212
00:11:01,428 --> 00:11:02,694
     we just got into orbit.

213
00:11:02,696 --> 00:11:05,330
          In many ways,
  we're firing a rocket motor.

214
00:11:05,332 --> 00:11:09,834
    I mean, it is fireworks.

215
00:11:09,836 --> 00:11:11,002
    Narrator: Safe in orbit,

216
00:11:11,004 --> 00:11:13,238
           juno turns
  its instruments to the planet

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00:11:13,240 --> 00:11:15,674
for a crucial part
        of the mission --

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     investigating jupiter's
         magnetic field.

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                     ♪

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 deep below the stormy surface,
    liquid metallic hydrogen

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         flows endlessly
       around the planet,

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        producing a huge
         magnetic field.

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       This magnetosphere
stretches over 600 million miles

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00:11:36,997 --> 00:11:41,966
       beyond the planet,
 reaching all the way to saturn.

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 If your eyes could actually see
     jupiter's magnetosphere

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00:11:45,372 --> 00:11:48,206
and you tried to look at it
    while standing on earth,

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00:11:48,208 --> 00:11:52,410
   it would look about as big
     in the sky as the moon.

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00:11:52,412 --> 00:11:54,713
            Narrator:
 And within this magnetic field,

229
00:11:54,715 --> 00:11:58,917
 juno faces an invisible threat.

230
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     Jupiter has an enormous
         magnetic field.

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00:12:02,389 --> 00:12:05,490
        It is so enormous
       in terms of space,

232
00:12:05,492 --> 00:12:09,627
   but also in terms of power.

233
00:12:09,629 --> 00:12:12,263
 Narrator: High-energy particles
          from the sun

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00:12:12,265 --> 00:12:14,933
        are funneled into
     deadly radiation belts

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       guided by the giant
planet's magnetic field.

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00:12:19,873 --> 00:12:24,109
The magnetic field traps charged
  particles coming from the sun

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       and circulates them
       around that system

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00:12:26,947 --> 00:12:30,215
        and just bombards
    anything in the vicinity,

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00:12:30,217 --> 00:12:34,586
      including our fragile
       little spacecraft.

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            Narrator:
      Closer to the planet,

241
00:12:36,089 --> 00:12:38,723
   radiation levels are up to
        30 times greater

242
00:12:38,725 --> 00:12:41,426
      than they were inside
      the reactor core room

243
00:12:41,428 --> 00:12:44,095
 during the chernobyl disaster.

244
00:12:44,097 --> 00:12:45,864
       This is radiation.

245
00:12:45,866 --> 00:12:47,599
This is bad news.

246
00:12:47,601 --> 00:12:49,300
        These particles,
       they would hit you.

247
00:12:49,302 --> 00:12:52,537
  They would rupture your dna,
  rupture your cell structures,

248
00:12:52,539 --> 00:12:55,406
       and you would die.

249
00:12:55,408 --> 00:12:57,842
    Narrator: This blistering
      radiation is bad news

250
00:12:57,844 --> 00:13:01,279
   for the spacecraft as well.

251
00:13:01,281 --> 00:13:04,382
 The charged particles threaten
      to destroy electronic

252
00:13:04,384 --> 00:13:09,854
    and navigational systems,
    but juno has armored up.

253
00:13:09,856 --> 00:13:13,858
 Plait: It's not some delicate,
    beautiful, gossamer thing

254
00:13:13,860 --> 00:13:16,361
      that you are sending
to orbit jupiter.

255
00:13:16,363 --> 00:13:18,196
     It's more like a tank.

256
00:13:18,198 --> 00:13:20,098
 You have to protect this thing
             or else

257
00:13:20,100 --> 00:13:24,035
     it's not going to last
        very long at all.

258
00:13:24,037 --> 00:13:27,172
   We've got a couple hundred
       pounds of titanium

259
00:13:27,174 --> 00:13:29,541
        on the spacecraft
    just trying to shield us

260
00:13:29,543 --> 00:13:31,743
        from what jupiter
       might throw at us,

261
00:13:31,745 --> 00:13:36,080
 so it is in a sense we're like
 an armored tank going into war.

262
00:13:36,082 --> 00:13:40,485
            Narrator:
 Lightweight titanium is tough.

263
00:13:40,487 --> 00:13:44,055
      Juno's 1/2-inch-thick
shielding blocks 99%

264
00:13:44,057 --> 00:13:48,126
 of jupiter's vicious radiation.

265
00:13:48,128 --> 00:13:49,727
 But even at this reduced rate,

266
00:13:49,729 --> 00:13:53,464
       juno can't survive
    the bombardment for long,

267
00:13:53,466 --> 00:13:56,801
    so the craft sets itself
        on a unique orbit

268
00:13:56,803 --> 00:13:59,571
      around the gas giant.

269
00:13:59,573 --> 00:14:01,973
     It actually has a very
           long orbit

270
00:14:01,975 --> 00:14:04,642
         where it spends
   most of its time far away,

271
00:14:04,644 --> 00:14:07,278
       and then every once
  in a while dives in and goes,

272
00:14:07,280 --> 00:14:09,080
    "oh, hot, hot, hot, hot.
     I zoomed in too much,"

273
00:14:09,082 --> 00:14:11,783
    and then goes safely away
to communicate and process

274
00:14:11,785 --> 00:14:15,520
     and then back in again.

275
00:14:15,522 --> 00:14:17,322
            Narrator:
   Juno takes a mighty gamble

276
00:14:17,324 --> 00:14:20,024
           diving deep
   into these radiation belts

277
00:14:20,026 --> 00:14:22,861
           to achieve
  one of its key objectives --

278
00:14:22,863 --> 00:14:26,831
        mapping jupiter's
      giant magnetic field,

279
00:14:26,833 --> 00:14:29,701
       and as juno swoops
       around the planet,

280
00:14:29,703 --> 00:14:35,473
 it reveals something scientists
     have never seen before.

281
00:14:35,475 --> 00:14:36,641
   When you look at the earth,

282
00:14:36,643 --> 00:14:38,910
        we have a fairly
     simple magnetic field.

283
00:14:38,912 --> 00:14:40,845
It's like a giant bar magnet
          with a north

284
00:14:40,847 --> 00:14:42,881
    and south magnetic pole.

285
00:14:42,883 --> 00:14:44,883
 Well, jupiter has that as well.

286
00:14:44,885 --> 00:14:46,684
 This is called a dipolar field.

287
00:14:46,686 --> 00:14:51,556
       It's got two poles,
  but it also has a third pole.

288
00:14:51,558 --> 00:14:53,891
            Narrator:
   Juno's magnetic field maps

289
00:14:53,893 --> 00:14:56,361
   show a north and south pole

290
00:14:56,363 --> 00:15:00,465
     and a bizarre magnetic
   disturbance at the equator.

291
00:15:00,467 --> 00:15:04,068
      And it's like jupiter
   just sprouted a third arm,

292
00:15:04,070 --> 00:15:06,871
 and that's kind of mysterious.

293
00:15:06,873 --> 00:15:08,406
            Narrator:
On magnetic field maps,

294
00:15:08,408 --> 00:15:11,976
     north poles show up red
      and south poles blue,

295
00:15:11,978 --> 00:15:15,647
    so scientists are calling
     this second south pole

296
00:15:15,649 --> 00:15:17,882
      the great blue spot.

297
00:15:17,884 --> 00:15:20,518
      Everyone knows about
       the great red spot,

298
00:15:20,520 --> 00:15:24,055
       but jupiter now has
   a great blue spot as well.

299
00:15:24,057 --> 00:15:26,257
     Narrator: This magnetic
      disturbance reflects

300
00:15:26,259 --> 00:15:28,726
   jupiter's stormy interior.

301
00:15:28,728 --> 00:15:32,497
You have these fast-moving winds
 blowing on the magnetic field,

302
00:15:32,499 --> 00:15:34,899
      and they're actually
shearing it apart

303
00:15:34,901 --> 00:15:36,534
  and moving the field around.

304
00:15:36,536 --> 00:15:38,036
        Bolton: It's not
      necessarily a storm,

305
00:15:38,038 --> 00:15:39,437
      although it could be.

306
00:15:39,439 --> 00:15:41,973
   It maybe is better to think
   of it as a magnetic storm.

307
00:15:41,975 --> 00:15:44,609
                     ♪

308
00:15:44,611 --> 00:15:46,811
   narrator: Turbulence inside
        jupiter could be

309
00:15:46,813 --> 00:15:51,349
 twisting up the magnetic field
  to drive the great blue spot

310
00:15:51,351 --> 00:15:56,321
 and the deadly radiation belts
that juno must navigate through.

311
00:15:56,323 --> 00:16:00,224
      Unlike earth, jupiter
   is not really a solid mass

312
00:16:00,226 --> 00:16:04,295
for the most part,
 so all of its clouds and gases

313
00:16:04,297 --> 00:16:06,698
           are moving
  at slightly different rates,

314
00:16:06,700 --> 00:16:09,233
     and that actually makes
       the magnetic field

315
00:16:09,235 --> 00:16:14,072
 that's generated very variable
      and highly changing.

316
00:16:14,074 --> 00:16:15,606
    For us to have a variable
         magnetic field

317
00:16:15,608 --> 00:16:17,175
       like jupiter does,

318
00:16:17,177 --> 00:16:19,344
        the entire earth
    would have to be molten.

319
00:16:19,346 --> 00:16:21,779
      We really don't want
         that to happen.

320
00:16:21,781 --> 00:16:25,116
   Narrator: With each orbit,
  juno unravels more mysteries

321
00:16:25,118 --> 00:16:29,320
of this giant planet,
  but jupiter's deepest secret

322
00:16:29,322 --> 00:16:32,323
       could shine a light
       on our own origins.

323
00:16:32,325 --> 00:16:33,992
    If we want to understand
            the earth

324
00:16:33,994 --> 00:16:35,660
          and our place
      in the solar system,

325
00:16:35,662 --> 00:16:38,162
    juno has found that a lot
       of those mysteries

326
00:16:38,164 --> 00:16:39,564
 are locked up there in jupiter.

327
00:16:39,566 --> 00:16:42,867
                     ♪

328
00:16:49,609 --> 00:16:53,611
                     ♪

329
00:16:53,613 --> 00:16:55,113
  narrator: The juno spacecraft

330
00:16:55,115 --> 00:16:57,815
          is uncovering
     the secrets of jupiter

331
00:16:57,817 --> 00:17:02,353
  from its swirling cloud tops
to its dark heart,

332
00:17:02,355 --> 00:17:07,158
     but juno's discoveries
 go beyond the gas giant itself.

333
00:17:07,160 --> 00:17:12,030
 They could also solve mysteries
   surrounding our own planet.

334
00:17:12,032 --> 00:17:14,465
       Jupiter is the key

335
00:17:14,467 --> 00:17:16,801
        to the formation
      of the solar system,

336
00:17:16,803 --> 00:17:18,870
    which means it's the key
        to understanding

337
00:17:18,872 --> 00:17:21,372
      how the earth formed.

338
00:17:21,374 --> 00:17:22,974
   Juno is actually giving us
             a view

339
00:17:22,976 --> 00:17:24,942
        into the history
    of our planetary system,

340
00:17:24,944 --> 00:17:28,679
   even the history of earth.

341
00:17:28,681 --> 00:17:31,082
            Narrator:
4.6 billion years ago,

342
00:17:31,084 --> 00:17:35,153
     a cloud of hydrogen gas
   and cosmic dust collapses,

343
00:17:35,155 --> 00:17:38,723
    sparking nuclear fusion.

344
00:17:38,725 --> 00:17:41,192
    From the resulting chaos,

345
00:17:41,194 --> 00:17:44,328
  one star, four rocky worlds,

346
00:17:44,330 --> 00:17:47,131
 and four gassy giants are born

347
00:17:47,133 --> 00:17:52,270
   and form our solar system.

348
00:17:52,272 --> 00:17:54,472
  There's these distinct zones
     of the solar system --

349
00:17:54,474 --> 00:17:56,340
       rocky and metallic
       in the inner part,

350
00:17:56,342 --> 00:17:58,609
     gaseous and water-rich
       in the outer part,

351
00:17:58,611 --> 00:18:01,312
    and even without thinking
      about that too hard,

352
00:18:01,314 --> 00:18:04,382
it kind of makes sense
  because in close to the sun,

353
00:18:04,384 --> 00:18:05,650
          it's warmer.

354
00:18:05,652 --> 00:18:09,120
 Out farther away from the sun,
          it's cooler.

355
00:18:09,122 --> 00:18:12,623
     Narrator: But the earth
        breaks the mold.

356
00:18:12,625 --> 00:18:17,628
  Our planet has far more water
     than theories predict.

357
00:18:17,630 --> 00:18:19,697
   The earth formed in a part
    of the solar system that,

358
00:18:19,699 --> 00:18:21,766
   well, you'd think normally
  should be probably pretty dry

359
00:18:21,768 --> 00:18:24,335
      because it was pretty
        close to the sun.

360
00:18:24,337 --> 00:18:28,039
  Narrator: Our planet is just
150 million miles from the sun,

361
00:18:28,041 --> 00:18:33,377
     putting us inside what
 scientists call the snow line.

362
00:18:33,379 --> 00:18:36,314
        Inside this line,
   the sun is powerful enough

363
00:18:36,316 --> 00:18:42,186
       to evaporate water
  during a planet's formation.

364
00:18:42,188 --> 00:18:44,555
      Inside the snow line,
   the temperatures are high,

365
00:18:44,557 --> 00:18:47,492
   and there's a lot of energy
      from the sun nearby.

366
00:18:47,494 --> 00:18:48,926
      Too close to the sun,

367
00:18:48,928 --> 00:18:52,296
   those gaseous and ice-rich
   materials just can't exist.

368
00:18:52,298 --> 00:18:55,600
     They're evaporate away
     by the heat of the sun.

369
00:18:55,602 --> 00:19:00,872
Narrator: Our watery world
 should be a dry rock in space.

370
00:19:00,874 --> 00:19:03,474
   Understanding how water got
  to the earth is so important

371
00:19:03,476 --> 00:19:07,545
  because it wouldn't be there
  in the very, very beginning.

372
00:19:07,547 --> 00:19:11,916
Narrator: But jupiter could hold
   the answer to this mystery.

373
00:19:11,918 --> 00:19:14,452
       To solve the riddle
        of earth's water,

374
00:19:14,454 --> 00:19:19,423
      juno aims to discover
   where our jupiter was born.

375
00:19:19,425 --> 00:19:21,726
   Understanding how and where

376
00:19:21,728 --> 00:19:24,162
     and when jupiter formed
           is critical

377
00:19:24,164 --> 00:19:25,630
 because it has really dominated

378
00:19:25,632 --> 00:19:28,466
the entire evolution
      of the solar system.

379
00:19:28,468 --> 00:19:30,301
 It's the biggest planet by far.

380
00:19:30,303 --> 00:19:34,772
It's the biggest thing out there
that's moving everything around.

381
00:19:34,774 --> 00:19:36,908
Narrator: Any water in the early
          solar system

382
00:19:36,910 --> 00:19:40,545
   could've been moved around
  by jupiter's mighty gravity,

383
00:19:40,547 --> 00:19:44,515
so if juno can trace the history
      of this giant planet,

384
00:19:44,517 --> 00:19:49,320
 that could explain why we find
 h2o where it's least expected.

385
00:19:49,322 --> 00:19:51,989
  We know that planets can move
        closer to the sun

386
00:19:51,991 --> 00:19:53,858
         and farther out
while they're forming

387
00:19:53,860 --> 00:19:55,660
    and even after they form,

388
00:19:55,662 --> 00:19:59,096
     so how do we figure out
      where jupiter formed?

389
00:19:59,098 --> 00:20:01,332
            Narrator:
  The key is how much water is

390
00:20:01,334 --> 00:20:04,035
    locked up inside jupiter.

391
00:20:04,037 --> 00:20:09,173
If we can understand how jupiter
built a relationship with water,

392
00:20:09,175 --> 00:20:11,676
        we can understand
    how water got distributed

393
00:20:11,678 --> 00:20:17,114
all throughout the solar system,
    including here on earth.

394
00:20:17,116 --> 00:20:20,451
  Narrator: If juno can measure
  the water content of jupiter,

395
00:20:20,453 --> 00:20:23,854
          it will solve
a 20-year-old mystery.

396
00:20:23,856 --> 00:20:25,856
                     ♪

397
00:20:25,858 --> 00:20:28,459
        December 1995 --

398
00:20:28,461 --> 00:20:32,129
      nasa's galileo probe
       begins a fatal dive

399
00:20:32,131 --> 00:20:35,299
   into jupiter's atmosphere.

400
00:20:35,301 --> 00:20:39,503
   When it did, it was able to
measure the atmosphere around it

401
00:20:39,505 --> 00:20:43,207
        and detect water,
 and the thing is -- it didn't.

402
00:20:43,209 --> 00:20:46,444
       It didn't find any,
        and that's weird.

403
00:20:46,446 --> 00:20:49,547
    Everything was bone-dry,
       so why in the world

404
00:20:49,549 --> 00:20:52,516
    did jupiter's atmosphere
            look dry?

405
00:20:52,518 --> 00:20:55,586
  Narrator: If the results from
the galileo probe are correct,

406
00:20:55,588 --> 00:20:58,055
   then 4.6 billion years ago,

407
00:20:58,057 --> 00:21:02,126
         jupiter formed
       closer to the sun,

408
00:21:02,128 --> 00:21:04,495
 but that's not the whole story.

409
00:21:04,497 --> 00:21:10,134
   20 years later, nasa sends
  juno to get a second opinion.

410
00:21:10,136 --> 00:21:13,571
  Juno is an orbiter, and so it
   is loaded with instruments

411
00:21:13,573 --> 00:21:15,706
          and detectors
     to look down on jupiter

412
00:21:15,708 --> 00:21:19,543
      and try to figure out
   everything that's going on.

413
00:21:19,545 --> 00:21:21,212
            Narrator:
    Juno doesn't have to risk

414
00:21:21,214 --> 00:21:24,081
   its life to hunt for water.

415
00:21:24,083 --> 00:21:26,951
The craft peers through
     jupiter's thick clouds

416
00:21:26,953 --> 00:21:32,723
 using a microwave radiometer to
detect h2o from a safe distance.

417
00:21:32,725 --> 00:21:34,358
     Using these microwaves,

418
00:21:34,360 --> 00:21:38,462
   juno builds up a global map
       of jupiter's water.

419
00:21:38,464 --> 00:21:39,930
     What juno has found is,
              yeah,

420
00:21:39,932 --> 00:21:42,933
     there's plenty of water
           in jupiter,

421
00:21:42,935 --> 00:21:46,203
     it's just that galileo
   happened to hit a dry spot,

422
00:21:46,205 --> 00:21:49,006
     but in fact, if it had
  come in almost anywhere else,

423
00:21:49,008 --> 00:21:53,010
        it would've seen
        plenty of water.

424
00:21:53,012 --> 00:21:55,579
Narrator: Juno's findings
         may give a clue

425
00:21:55,581 --> 00:21:59,717
        to where jupiter
       originally formed.

426
00:21:59,719 --> 00:22:02,820
   It seems apparent now that
             jupiter

427
00:22:02,822 --> 00:22:06,857
           didn't form
    in its present location.

428
00:22:06,859 --> 00:22:08,059
            Narrator:
   The leading theory is that

429
00:22:08,061 --> 00:22:10,895
         jupiter formed
   just beyond the snow line,

430
00:22:10,897 --> 00:22:14,165
      the boundary between
   the dry inner solar system

431
00:22:14,167 --> 00:22:16,634
        and the wet outer
          solar system.

432
00:22:16,636 --> 00:22:19,804
  But we find jupiter is twice
as far away from the sun

433
00:22:19,806 --> 00:22:22,640
     as where that original
    snow line would've been,

434
00:22:22,642 --> 00:22:26,510
      so this is telling us
     something interesting.

435
00:22:26,512 --> 00:22:27,678
            Narrator:
 Jupiter may have wandered from

436
00:22:27,680 --> 00:22:29,547
     its original position,

437
00:22:29,549 --> 00:22:33,050
   causing unimaginable chaos.

438
00:22:33,052 --> 00:22:35,219
    As jupiter moved around,
         things got hit

439
00:22:35,221 --> 00:22:37,421
         and knocked out
      of the solar system.

440
00:22:37,423 --> 00:22:39,724
 Walsh: It essentially scatters
     everything in its path.

441
00:22:39,726 --> 00:22:42,526
    It's the biggest player.
    It's the biggest planet.

442
00:22:42,528 --> 00:22:44,662
Everything moves for it.

443
00:22:44,664 --> 00:22:48,132
 Narrator: As jupiter bulldozes
 toward the outer solar system,

444
00:22:48,134 --> 00:22:50,234
  it slings ice-rich asteroids

445
00:22:50,236 --> 00:22:55,373
  and comets in towards the sun
     and towards the earth.

446
00:22:55,375 --> 00:22:59,910
                     ♪

447
00:22:59,912 --> 00:23:01,645
     jupiter would literally
          in some sense

448
00:23:01,647 --> 00:23:04,749
         have snowplowed
   into the inner solar system

449
00:23:04,751 --> 00:23:06,851
          a whole wave
   of water-rich planetesimals

450
00:23:06,853 --> 00:23:11,856
     that would've delivered
   much of our earth's oceans.

451
00:23:11,858 --> 00:23:15,359
Narrator: Juno has helped answer
why our earth is habitable

452
00:23:15,361 --> 00:23:17,962
     despite being so close
           to the sun.

453
00:23:17,964 --> 00:23:20,264
    So it was worth going all
         that distance,

454
00:23:20,266 --> 00:23:23,200
  sending juno all the way out
 there to get that closer look.

455
00:23:23,202 --> 00:23:26,737
                     ♪

456
00:23:26,739 --> 00:23:28,472
            narrator:
    Juno continues to explore

457
00:23:28,474 --> 00:23:33,077
       jupiter's mysteries
    and its famous features.

458
00:23:33,079 --> 00:23:35,379
  There is nothing more iconic
          about jupiter

459
00:23:35,381 --> 00:23:37,381
    than the great red spot.

460
00:23:37,383 --> 00:23:41,652
   Narrator: And juno reveals
 that this 300-year-old cyclone

461
00:23:41,654 --> 00:23:44,688
may soon vanish.

462
00:23:51,431 --> 00:23:57,268
                     ♪

463
00:23:57,270 --> 00:23:59,103
            narrator:
   Our solar system plays host

464
00:23:59,105 --> 00:24:01,472
 to some epic natural wonders --

465
00:24:01,474 --> 00:24:03,541
  the ice geysers of enceladus,

466
00:24:03,543 --> 00:24:06,677
   the giant rings of saturn,

467
00:24:06,679 --> 00:24:10,648
    the martian mega volcano
          olympus mons,

468
00:24:10,650 --> 00:24:13,184
      but in July of 2017,

469
00:24:13,186 --> 00:24:17,021
     nasa's juno probe skims
     the surface of jupiter

470
00:24:17,023 --> 00:24:22,193
 and photographs the most famous
        natural wonder --

471
00:24:22,195 --> 00:24:24,728
 a fierce, hurricane-like storm

472
00:24:24,730 --> 00:24:29,033
       that's been raging
     for hundreds of years.

473
00:24:29,035 --> 00:24:30,334
When you think of jupiter,

474
00:24:30,336 --> 00:24:32,636
         one of the most
        visually stunning

475
00:24:32,638 --> 00:24:34,839
    and most iconic features
        of the atmosphere

476
00:24:34,841 --> 00:24:36,841
     is that great red spot.

477
00:24:36,843 --> 00:24:38,676
      There is nothing like
       jupiter's red spot

478
00:24:38,678 --> 00:24:42,079
   in our entire solar system.

479
00:24:42,081 --> 00:24:45,015
     Narrator: As juno soars
    over the great red spot,

480
00:24:45,017 --> 00:24:49,453
   it looks down onto a storm
    over 10,000 miles across.

481
00:24:49,455 --> 00:24:52,990
                     ♪

482
00:24:52,992 --> 00:24:55,025
        thaller: This is
     the most extreme storm.

483
00:24:55,027 --> 00:24:56,727
          The winds are
blowing continuously

484
00:24:56,729 --> 00:24:59,964
      at 400 miles an hour.

485
00:24:59,966 --> 00:25:03,567
  Narrator: On earth, the most
 powerful category 5 hurricanes

486
00:25:03,569 --> 00:25:06,537
           can unleash
    almost total destruction,

487
00:25:06,539 --> 00:25:09,473
       but these are less
      than half as powerful

488
00:25:09,475 --> 00:25:11,775
    as the storm on jupiter.

489
00:25:11,777 --> 00:25:14,345
      The great red spot is
     the greatest hurricane

490
00:25:14,347 --> 00:25:16,413
   that you've ever imagined.

491
00:25:16,415 --> 00:25:17,882
  Narrator: But that's not all.

492
00:25:17,884 --> 00:25:22,419
   Juno's microwave radiometer
allows scientists to see through

493
00:25:22,421 --> 00:25:26,457
     jupiter's cloud layers
for the first time.

494
00:25:26,459 --> 00:25:30,160
    Juno has instrumentation
 that's able to look underneath,

495
00:25:30,162 --> 00:25:31,595
      so one of the things
      we did was we looked

496
00:25:31,597 --> 00:25:33,564
   at how deep are the roots.

497
00:25:33,566 --> 00:25:35,799
            Narrator:
  Juno peers down into the eye

498
00:25:35,801 --> 00:25:37,535
    of this monstrous storm.

499
00:25:37,537 --> 00:25:40,804
  It spots temperature changes
      far below the surface

500
00:25:40,806 --> 00:25:43,474
     that follow the storm's
          iconic shape,

501
00:25:43,476 --> 00:25:46,510
        tracing the roots
      of the great red spot

502
00:25:46,512 --> 00:25:49,179
            deep into
     the jovian atmosphere.

503
00:25:49,181 --> 00:25:50,814
They found out that
        it goes down over

504
00:25:50,816 --> 00:25:54,351
            200 miles
    deep into the atmosphere.

505
00:25:54,353 --> 00:25:56,253
         There's nothing
       like that on earth.

506
00:25:56,255 --> 00:25:59,557
                     ♪

507
00:25:59,559 --> 00:26:02,226
 narrator: The greatest cyclones
        of our own planet

508
00:26:02,228 --> 00:26:05,429
        can reach heights
       of around 10 miles,

509
00:26:05,431 --> 00:26:10,601
  but jupiter's great red spot
    is over 20 times taller.

510
00:26:10,603 --> 00:26:12,670
   I think that really brings
        into perspective

511
00:26:12,672 --> 00:26:14,772
        the massive scale
         of this planet.

512
00:26:14,774 --> 00:26:18,075
                     ♪

513
00:26:18,077 --> 00:26:20,611
narrator: Jupiter's vast,
      turbulent atmosphere

514
00:26:20,613 --> 00:26:24,248
     hosts the deepest storm
     mankind has ever seen,

515
00:26:24,250 --> 00:26:28,385
     and juno's discoveries
    get scientists wondering.

516
00:26:28,387 --> 00:26:31,322
    Could the great red spot
          help explain

517
00:26:31,324 --> 00:26:34,124
 another of jupiter's mysteries,

518
00:26:34,126 --> 00:26:39,396
    the planet's surprisingly
        warm atmosphere?

519
00:26:39,398 --> 00:26:42,232
        Jupiter looks out
    in our outer solar system

520
00:26:42,234 --> 00:26:43,701
        where everything
          is very cold.

521
00:26:43,703 --> 00:26:47,371
       The sun is very dim
   when you get that far away.

522
00:26:47,373 --> 00:26:50,441
Jupiter is five times farther
    from the sun than we are,

523
00:26:50,443 --> 00:26:52,176
     so it's only getting 4%

524
00:26:52,178 --> 00:26:54,745
     of the amount of energy
    from the sun that we do.

525
00:26:54,747 --> 00:26:56,013
            Thaller:
But there's something heating up

526
00:26:56,015 --> 00:26:57,348
   the atmosphere of jupiter.

527
00:26:57,350 --> 00:27:00,351
      There are parts of it
   that are many times warmer

528
00:27:00,353 --> 00:27:01,852
      than we could explain
         with sunlight.

529
00:27:01,854 --> 00:27:03,587
   The question is, of course,
      where is that energy

530
00:27:03,589 --> 00:27:06,290
          coming from?

531
00:27:06,292 --> 00:27:09,360
  Narrator: Juno swoops in for
another pass on jupiter,

532
00:27:09,362 --> 00:27:11,629
           turning its
     high-resolution cameras

533
00:27:11,631 --> 00:27:16,266
   on the raging storm below.

534
00:27:16,268 --> 00:27:18,535
       The storm unleashes
       vicious turbulence

535
00:27:18,537 --> 00:27:20,437
into the surrounding atmosphere,

536
00:27:20,439 --> 00:27:22,940
   giving scientists the clue
            they need

537
00:27:22,942 --> 00:27:26,243
           to explain
 the planet's high temperature.

538
00:27:26,245 --> 00:27:29,480
       The great red spot
      is a giant hurricane

539
00:27:29,482 --> 00:27:34,018
   that's powered by heat deep
     in the core of jupiter,

540
00:27:34,020 --> 00:27:37,821
     but it has such violent
       and chaotic motion,

541
00:27:37,823 --> 00:27:40,290
it's mixing up
    the atmosphere around it.

542
00:27:40,292 --> 00:27:43,794
                     ♪

543
00:27:43,796 --> 00:27:46,030
  the thunderstorms on jupiter
     are gonna be generating

544
00:27:46,032 --> 00:27:48,032
         booming thunder
        just the same way

545
00:27:48,034 --> 00:27:52,169
 that they do here on the earth.

546
00:27:52,171 --> 00:27:54,338
            Narrator:
 Thunderclouds send sound waves

547
00:27:54,340 --> 00:27:58,976
   rippling through the storm.

548
00:27:58,978 --> 00:28:03,547
     A sound wave is a wave
          of pressure,

549
00:28:03,549 --> 00:28:06,617
         of compression
       where air molecules

550
00:28:06,619 --> 00:28:09,319
       or water molecules
         get compacted.

551
00:28:09,321 --> 00:28:10,754
They get squeezed together,

552
00:28:10,756 --> 00:28:12,723
      and when you squeeze
       something together,

553
00:28:12,725 --> 00:28:14,024
  they're a lot closer together

554
00:28:14,026 --> 00:28:15,459
        and they're gonna
         get pretty hot.

555
00:28:15,461 --> 00:28:18,228
                     ♪

556
00:28:18,230 --> 00:28:20,064
            narrator:
   These sounds waves shoot up

557
00:28:20,066 --> 00:28:23,434
    500 miles above the storm

558
00:28:23,436 --> 00:28:26,837
  where they break, converting
     sound energy into heat.

559
00:28:26,839 --> 00:28:30,708
       These sound waves,
      they crash together,

560
00:28:30,710 --> 00:28:32,776
      creating a tremendous
        amount of energy

561
00:28:32,778 --> 00:28:36,980
      and heating the gases
around them.

562
00:28:36,982 --> 00:28:39,583
    Narrator: Jupiter's great
    red spot has helped heat

563
00:28:39,585 --> 00:28:42,486
      the jovian atmosphere
     for hundreds of years,

564
00:28:42,488 --> 00:28:48,292
   but new images suggest that
  this may be about to change.

565
00:28:48,294 --> 00:28:50,194
  Jupiter's red spot is so big,

566
00:28:50,196 --> 00:28:53,363
 I mean, it's bigger than earth
         by a long shot.

567
00:28:53,365 --> 00:28:56,400
    It seems like it would be
   an incredibly stable thing.

568
00:28:56,402 --> 00:28:59,803
 It's just there and it's always
 been there and always will be.

569
00:28:59,805 --> 00:29:03,507
            Recently,
     we've seen it changing.

570
00:29:03,509 --> 00:29:05,809
Narrator: When nasa's voyager
       space probe visited

571
00:29:05,811 --> 00:29:07,945
        jupiter in 1979,

572
00:29:07,947 --> 00:29:11,181
       it observed a storm
  twice the diameter of earth.

573
00:29:11,183 --> 00:29:15,686
                     ♪

574
00:29:15,688 --> 00:29:20,190
     in 2017, juno's images
     show the great red spot

575
00:29:20,192 --> 00:29:24,628
 has lost a third of its width,
       but that's not all.

576
00:29:24,630 --> 00:29:28,866
  Despite the storm shrinking,
  it's actually getting taller.

577
00:29:28,868 --> 00:29:31,735
   The great red spot is being
      stretched and forced

578
00:29:31,737 --> 00:29:34,805
into jupiter's upper atmosphere.

579
00:29:34,807 --> 00:29:36,373
          The storms in
the great red spot,

580
00:29:36,375 --> 00:29:39,042
   it's kind of like the clay
      on a potter's wheel,

581
00:29:39,044 --> 00:29:41,178
  where as you bring your hands
         closer together

582
00:29:41,180 --> 00:29:43,914
      to draw the clay in,
   the closer your hands are,

583
00:29:43,916 --> 00:29:47,251
 the taller the pottery becomes,
  and similarly, for the storm,

584
00:29:47,253 --> 00:29:49,620
          as it becomes
      smaller at the base,

585
00:29:49,622 --> 00:29:53,457
     it raises taller toward
      the upper atmosphere.

586
00:29:53,459 --> 00:29:55,325
      It's getting taller,
        and we see storms

587
00:29:55,327 --> 00:29:57,694
   do the same thing on earth,
and when it does that,

588
00:29:57,696 --> 00:30:00,197
  the wind shear will actually
  take the top of the storm off

589
00:30:00,199 --> 00:30:02,499
       and drag it apart,
   and so we'll be watching it

590
00:30:02,501 --> 00:30:04,034
          very intently
     over the next few years

591
00:30:04,036 --> 00:30:08,572
to see if that's what happens on
        jupiter as well.

592
00:30:08,574 --> 00:30:10,374
    Narrator: It may be only
        a matter of time

593
00:30:10,376 --> 00:30:13,410
        before jupiter's
       high-altitude winds

594
00:30:13,412 --> 00:30:16,313
     tear this iconic storm
           to shreds.

595
00:30:16,315 --> 00:30:18,515
      The most famous storm
       of the solar system

596
00:30:18,517 --> 00:30:20,484
may soon disappear,

597
00:30:20,486 --> 00:30:23,053
  but juno reveals other storms

598
00:30:23,055 --> 00:30:26,790
     hidden in the strangest
           of places.

599
00:30:26,792 --> 00:30:29,159
 The storm in the great red spot
             is one,

600
00:30:29,161 --> 00:30:32,763
  but not the only, giant storm
  that's happening on jupiter.

601
00:30:32,765 --> 00:30:36,667
                     ♪

602
00:30:43,442 --> 00:30:49,213
                     ♪

603
00:30:49,215 --> 00:30:52,816
   narrator: Nasa's juno probe
 has traveled billions of miles

604
00:30:52,818 --> 00:30:54,551
     across the solar system

605
00:30:54,553 --> 00:30:58,488
     to reveal the mysteries
      of gas giant jupiter,

606
00:30:58,490 --> 00:31:00,924
      but there's one part
           of jupiter

607
00:31:00,926 --> 00:31:04,695
that has remained hidden
           until now.

608
00:31:04,697 --> 00:31:07,497
Before juno, our view of jupiter
        was very limited.

609
00:31:07,499 --> 00:31:10,367
    We'd never actually flown
         over the poles.

610
00:31:10,369 --> 00:31:12,069
 It's something that's very hard
        to do on jupiter.

611
00:31:12,071 --> 00:31:15,539
  We don't have other missions
      that have done this.

612
00:31:15,541 --> 00:31:19,209
  Narrator: In August of 2016,
    juno's flight plan takes

613
00:31:19,211 --> 00:31:22,579
         the spacecraft
into unknown territory to reveal

614
00:31:22,581 --> 00:31:27,985
   jupiter's mysterious polar
   regions for the first time.

615
00:31:27,987 --> 00:31:29,620
Well, and the first time
     we looked at the pole,

616
00:31:29,622 --> 00:31:31,922
     it didn't look anything
    like the jupiter we knew.

617
00:31:31,924 --> 00:31:35,626
                     ♪

618
00:31:35,628 --> 00:31:37,327
    we never would've guessed
        that was jupiter

619
00:31:37,329 --> 00:31:38,562
         if somebody had
        shown that to us.

620
00:31:38,564 --> 00:31:42,399
                     ♪

621
00:31:42,401 --> 00:31:46,203
 narrator: Juno's camera reveals
     a strange blue expanse

622
00:31:46,205 --> 00:31:49,106
    that puzzles scientists.

623
00:31:49,108 --> 00:31:50,274
      The electronic color

624
00:31:50,276 --> 00:31:52,943
could be due to chemical changes
          in the clouds

625
00:31:52,945 --> 00:31:56,880
      brought on by a lack
of sunlight,

626
00:31:56,882 --> 00:32:00,284
       but what juno spots
     inside the blue clouds

627
00:32:00,286 --> 00:32:03,387
       is even stranger --

628
00:32:03,389 --> 00:32:08,191
   giant central cyclones spin
  around each pole at 200 miles

629
00:32:08,193 --> 00:32:10,460
  an hour, with these cyclones

630
00:32:10,462 --> 00:32:14,965
       surrounded by eight
  stormy vortices in the north

631
00:32:14,967 --> 00:32:18,302
     and five in the south.

632
00:32:18,304 --> 00:32:21,605
 There are these weird cyclones,
        gigantic swirls,

633
00:32:21,607 --> 00:32:25,575
 vortices of gas swirling around
        jupiter's poles,

634
00:32:25,577 --> 00:32:28,912
           and they're
    clearly forming patterns.

635
00:32:28,914 --> 00:32:30,847
        It's hard to get
a sense of scale here.

636
00:32:30,849 --> 00:32:32,916
       Now the north polar
        central cyclone,

637
00:32:32,918 --> 00:32:36,820
   that one right at the pole,
   that's 2,500 miles across.

638
00:32:36,822 --> 00:32:40,624
    That is almost as big as
 the continental united states.

639
00:32:40,626 --> 00:32:42,092
     What is going on there?

640
00:32:42,094 --> 00:32:44,761
      This is nothing like
      what we see on earth.

641
00:32:44,763 --> 00:32:47,798
                     ♪

642
00:32:47,800 --> 00:32:51,835
 narrator: On earth, our weather
 is driven by heat from the sun

643
00:32:51,837 --> 00:32:53,804
      that hits our planet
         at the equator

644
00:32:53,806 --> 00:32:57,207
  and flows across the surface.

645
00:32:57,209 --> 00:33:00,477
Powerful cyclones form
      over tropical waters

646
00:33:00,479 --> 00:33:04,348
   and move around the planet,

647
00:33:04,350 --> 00:33:07,517
  but the polar regions receive
    less energy from the sun,

648
00:33:07,519 --> 00:33:11,254
           so cyclones
    can't form at the poles.

649
00:33:11,256 --> 00:33:13,357
    We see that if you're at
          the equator,

650
00:33:13,359 --> 00:33:14,591
 it's warmer and it's stormier.

651
00:33:14,593 --> 00:33:15,993
     If you're at the poles,

652
00:33:15,995 --> 00:33:20,998
where the sun is slightly harder
to see, that activity goes away.

653
00:33:21,000 --> 00:33:22,766
            Narrator:
   But the weather on jupiter

654
00:33:22,768 --> 00:33:25,135
   couldn't be more different.

655
00:33:25,137 --> 00:33:27,371
We see lightning
  and convective thunderstorms

656
00:33:27,373 --> 00:33:29,606
     at the poles of jupiter
     but not at the equator,

657
00:33:29,608 --> 00:33:32,376
 and that's sort of the opposite
  of what we see on the earth.

658
00:33:32,378 --> 00:33:36,847
        The question is,
what's driving jupiter's storms?

659
00:33:36,849 --> 00:33:38,415
            Narrator:
  Jupiter is five times further

660
00:33:38,417 --> 00:33:40,517
        away from the sun
         than the earth

661
00:33:40,519 --> 00:33:44,955
  and receives only a fraction
      of the sun's energy.

662
00:33:44,957 --> 00:33:47,991
          Unlike earth,
     jupiter's polar regions

663
00:33:47,993 --> 00:33:50,594
seem to be where the action is.

664
00:33:50,596 --> 00:33:53,930
      Something is driving
   the planet's weird weather,

665
00:33:53,932 --> 00:33:57,601
  and juno's scans of the giant
   planet's thermal emissions

666
00:33:57,603 --> 00:34:01,705
      suggests it could be
         jupiter itself.

667
00:34:01,707 --> 00:34:04,441
       We can actually see
  the internal heat of jupiter

668
00:34:04,443 --> 00:34:05,809
    coming right up through,

669
00:34:05,811 --> 00:34:08,045
         and so jupiter
 will look very bright in areas

670
00:34:08,047 --> 00:34:11,281
   where we can see that heat.

671
00:34:11,283 --> 00:34:13,417
     Narrator: Juno detects
          searing heat

672
00:34:13,419 --> 00:34:16,420
 beneath jupiter's cloud bands.

673
00:34:16,422 --> 00:34:19,189
Jupiter has so much material,
          so much mass,

674
00:34:19,191 --> 00:34:22,059
      so much gravity that
the interior is incredibly dense

675
00:34:22,061 --> 00:34:23,760
       and very, very hot.

676
00:34:23,762 --> 00:34:26,730
  At the core, it's probably at
many thousands of degrees hotter

677
00:34:26,732 --> 00:34:29,633
  than the surface of the sun.

678
00:34:29,635 --> 00:34:33,837
  Narrator: This fiery inferno
 buried in jupiter's dark heart

679
00:34:33,839 --> 00:34:37,441
    is a relic from its birth
     billions of years ago.

680
00:34:37,443 --> 00:34:40,210
     The violent collisions
     that formed the planet

681
00:34:40,212 --> 00:34:42,746
   left its core seething hot,

682
00:34:42,748 --> 00:34:45,649
           a heat that
remains to this day,

683
00:34:45,651 --> 00:34:50,120
 buried under thousands of miles
       of insulating gas.

684
00:34:50,122 --> 00:34:52,789
    As the heat slowly leaks
            outward,

685
00:34:52,791 --> 00:34:55,725
     jupiter's fast-rotating
           atmosphere

686
00:34:55,727 --> 00:34:59,463
    creates vicious cyclones
       and thunderstorms.

687
00:34:59,465 --> 00:35:02,232
    And that's what's really
  driving most of the weather.

688
00:35:02,234 --> 00:35:06,269
        It's not the sun.
      It's jupiter itself.

689
00:35:06,271 --> 00:35:08,872
   Narrator: And as juno soars
        over the planet,

690
00:35:08,874 --> 00:35:13,143
           it reveals
    another weather mystery.

691
00:35:13,145 --> 00:35:16,113
The craft detects bursts
         of radio waves

692
00:35:16,115 --> 00:35:19,850
           spiking up
    to four times a second --

693
00:35:19,852 --> 00:35:24,855
        the telltale sign
 of ferocious lightning strikes.

694
00:35:24,857 --> 00:35:26,490
    Clouds are moving around
        in the atmosphere

695
00:35:26,492 --> 00:35:28,358
 and building up electric charge

696
00:35:28,360 --> 00:35:30,894
        and causing bolts
      of lightning to form,

697
00:35:30,896 --> 00:35:35,132
  and we've actually seen this
    with the juno spacecraft.

698
00:35:35,134 --> 00:35:38,201
      These are mega storms
   orders of magnitude bigger

699
00:35:38,203 --> 00:35:39,536
       than here on earth.

700
00:35:39,538 --> 00:35:43,507
       [ thunder crashes ]

701
00:35:43,509 --> 00:35:46,643
narrator: And juno finds there's
   more to these thunderclouds

702
00:35:46,645 --> 00:35:50,013
  than just flashes of light --

703
00:35:50,015 --> 00:35:54,317
  giant icy hailstones of water
          and ammonia,

704
00:35:54,319 --> 00:35:57,020
          the chemical
  which gives jupiter's clouds

705
00:35:57,022 --> 00:36:01,725
       their orange color.

706
00:36:01,727 --> 00:36:03,360
             High up
    in jupiter's atmosphere,

707
00:36:03,362 --> 00:36:07,030
      the ammonia is mixing
         with the water,

708
00:36:07,032 --> 00:36:09,232
  and it becomes a liquid ball

709
00:36:09,234 --> 00:36:11,902
   that starts to collect ice
           around it,

710
00:36:11,904 --> 00:36:17,107
 and it will fall like hail does
deep into jupiter's atmosphere.

711
00:36:17,109 --> 00:36:20,977
 Narrator: On earth, hail falls
    to the ground and melts,

712
00:36:20,979 --> 00:36:24,681
         but on jupiter,
       there is no ground.

713
00:36:24,683 --> 00:36:26,917
       And it gets lifted
        in the atmosphere

714
00:36:26,919 --> 00:36:29,085
      because of an updraft
       and then more ice,

715
00:36:29,087 --> 00:36:31,321
      and it builds bigger,
     and then it falls down,

716
00:36:31,323 --> 00:36:32,689
        and then it gets
        carried back up,

717
00:36:32,691 --> 00:36:38,061
      and so hail is often
    many layers being built.

718
00:36:38,063 --> 00:36:41,698
 Narrator: These ice balls grow
 layer by layer as they soar up

719
00:36:41,700 --> 00:36:44,734
and down the atmosphere.

720
00:36:44,736 --> 00:36:47,270
    If they formed in storms
         here on earth,

721
00:36:47,272 --> 00:36:50,540
          they'd cause
      some serious damage.

722
00:36:50,542 --> 00:36:52,976
  So if you were buzzing around
             jupiter

723
00:36:52,978 --> 00:36:55,612
        and you were near
    where these storms were,

724
00:36:55,614 --> 00:36:59,983
    you might get hit by hail
    coming up or going down.

725
00:36:59,985 --> 00:37:04,120
This is one of the most violent,
      energetic atmospheres

726
00:37:04,122 --> 00:37:07,824
   in the entire solar system.

727
00:37:07,826 --> 00:37:09,893
            Narrator:
  Juno is revealing the secrets

728
00:37:09,895 --> 00:37:12,662
     that jupiter has hidden
for decades,

729
00:37:12,664 --> 00:37:17,334
      including the mystery
  of jupiter's northern lights.

730
00:37:17,336 --> 00:37:19,803
  When juno studied the lights

731
00:37:19,805 --> 00:37:21,905
     coming from the aurora
           on jupiter,

732
00:37:21,907 --> 00:37:24,908
     it found that something
    really weird is going on.

733
00:37:24,910 --> 00:37:27,944
                     ♪

734
00:37:34,786 --> 00:37:42,826
                     ♪

735
00:37:42,828 --> 00:37:46,429
  narrator: On earth, dazzling
   auroras light up the skies

736
00:37:46,431 --> 00:37:48,632
      as charged particles
          from the sun

737
00:37:48,634 --> 00:37:51,268
    interact with atoms high
       in the atmosphere.

738
00:37:51,270 --> 00:37:54,638
                     ♪

739
00:37:54,640 --> 00:37:58,742
deep in the outer solar system,
 jupiter is too far from the sun

740
00:37:58,744 --> 00:38:01,811
       for strong auroras
      to form in this way,

741
00:38:01,813 --> 00:38:05,048
         but high above
    the giant planet's poles,

742
00:38:05,050 --> 00:38:09,119
     juno spots a seemingly
     impossible light show.

743
00:38:09,121 --> 00:38:11,354
                     ♪

744
00:38:11,356 --> 00:38:14,357
     the auroras of jupiter
     are tremendously larger

745
00:38:14,359 --> 00:38:15,925
          than the ones
   that we find here on earth.

746
00:38:15,927 --> 00:38:17,961
   In fact, the auroral rings
         near the poles

747
00:38:17,963 --> 00:38:20,430
           are bigger
     than our planet itself.

748
00:38:20,432 --> 00:38:21,731
Jupiter's auroras emit

749
00:38:21,733 --> 00:38:24,167
      primarily ultraviolet
        and x-ray light,

750
00:38:24,169 --> 00:38:26,636
       so you can't see it
    with the naked human eye,

751
00:38:26,638 --> 00:38:29,606
    but if you could see them
    and you were at jupiter,

752
00:38:29,608 --> 00:38:32,509
          that would be
      an amazing light show

753
00:38:32,511 --> 00:38:37,647
      because those auroras
           are strong.

754
00:38:37,649 --> 00:38:39,049
            Narrator:
   These glowing displays are

755
00:38:39,051 --> 00:38:41,751
  evidence of charged particles

756
00:38:41,753 --> 00:38:45,221
          slamming into
      jupiter's atmosphere.

757
00:38:45,223 --> 00:38:47,624
    But if they're not coming
from the sun,

758
00:38:47,626 --> 00:38:50,327
   where are they coming from?

759
00:38:50,329 --> 00:38:52,862
Narrator: Hunting for an answer,
       juno snaps an image

760
00:38:52,864 --> 00:38:54,497
  of jupiter's southern lights

761
00:38:54,499 --> 00:38:59,469
      with its ultraviolet
      imaging spectrometer.

762
00:38:59,471 --> 00:39:03,873
       Inside the aurora,
 it glimpses something strange.

763
00:39:03,875 --> 00:39:06,276
  When juno studied the lights

764
00:39:06,278 --> 00:39:08,345
     coming from the aurora
           on jupiter,

765
00:39:08,347 --> 00:39:11,614
     it found that they were
  even stronger than expected,

766
00:39:11,616 --> 00:39:13,249
          and in fact,
        when you look at

767
00:39:13,251 --> 00:39:15,985
 jupiter's poles in wavelengths
that our eyes can't see,

768
00:39:15,987 --> 00:39:20,290
    for example, ultraviolet,
       you see a hot spot.

769
00:39:20,292 --> 00:39:22,459
            Narrator:
  This hot spot marks the point

770
00:39:22,461 --> 00:39:25,762
    where huge concentrations
      of charged particles

771
00:39:25,764 --> 00:39:28,765
  strike jupiter's atmosphere.

772
00:39:28,767 --> 00:39:31,801
    Tracing their trajectory
       reveals the culprit

773
00:39:31,803 --> 00:39:34,404
      of jupiter's dazzling
         light shows --

774
00:39:34,406 --> 00:39:36,973
          the volcanoes
       of jupiter's moons.

775
00:39:36,975 --> 00:39:39,709
                     ♪

776
00:39:39,711 --> 00:39:42,579
 jupiter's moon, io has hundreds
       of active volcanoes

777
00:39:42,581 --> 00:39:45,115
spewing out materials
       way out into space,

778
00:39:45,117 --> 00:39:49,386
and many of those get trapped by
 the magnetic field of jupiter.

779
00:39:49,388 --> 00:39:53,390
  Narrator: Io's volcanoes fire
 out jets of charged particles,

780
00:39:53,392 --> 00:39:57,560
  which are swept by the giant
    planet's magnetic field.

781
00:39:57,562 --> 00:39:59,129
      It's funneling those
         particles down

782
00:39:59,131 --> 00:40:04,167
and slamming into specific spots
    in jupiter's atmosphere.

783
00:40:04,169 --> 00:40:06,436
     Narrator: But io isn't
    the only moon responsible

784
00:40:06,438 --> 00:40:09,439
          for jupiter's
        polar light show.

785
00:40:09,441 --> 00:40:12,776
If we go further out,
        europa, ganymede,

786
00:40:12,778 --> 00:40:14,110
            callisto,
       those are more icy.

787
00:40:14,112 --> 00:40:16,913
     They don't necessarily
         have volcanoes.

788
00:40:16,915 --> 00:40:18,915
            Narrator:
    These icy moons twist up

789
00:40:18,917 --> 00:40:22,285
    jupiter's magnetic field
        in their own way.

790
00:40:22,287 --> 00:40:24,854
    Some of these moons have
  magnetic fields that interact

791
00:40:24,856 --> 00:40:26,456
 with jupiter's magnetic field,

792
00:40:26,458 --> 00:40:31,761
  and that actually intensifies
 the aurora display on jupiter.

793
00:40:31,763 --> 00:40:33,630
            Narrator:
  Jupiter's moons work together

794
00:40:33,632 --> 00:40:37,934
to energize the greatest auroras
      in the solar system,

795
00:40:37,936 --> 00:40:40,136
          but in these
       beautiful displays

796
00:40:40,138 --> 00:40:45,141
       is a stark reminder
    of the danger juno faces.

797
00:40:45,143 --> 00:40:47,277
 When you look at these pictures
    of the aurora on jupiter,

798
00:40:47,279 --> 00:40:48,545
         and you think,
      oh, that's beautiful.

799
00:40:48,547 --> 00:40:49,979
      Wouldn't it be great
     to see that in person?

800
00:40:49,981 --> 00:40:52,515
        The answer is no,
         no, it wouldn't

801
00:40:52,517 --> 00:40:54,417
   because they will kill you.

802
00:40:54,419 --> 00:40:57,921
  What's causing these displays
     are subatomic particles

803
00:40:57,923 --> 00:41:00,790
accelerated to tremendously
           high speeds

804
00:41:00,792 --> 00:41:03,526
     by the magnetic fields
            involved.

805
00:41:03,528 --> 00:41:06,629
 Narrator: The radiation around
        jupiter is lethal

806
00:41:06,631 --> 00:41:08,965
    and not just for humans.

807
00:41:08,967 --> 00:41:11,534
    The lifetime of the juno
     mission is very limited

808
00:41:11,536 --> 00:41:14,504
    by the extreme conditions
      it has to survive in.

809
00:41:14,506 --> 00:41:15,872
  We think that in the future,

810
00:41:15,874 --> 00:41:17,640
    a lot of the instruments
     will be so irradiated,

811
00:41:17,642 --> 00:41:21,277
 they won't really work anymore.

812
00:41:21,279 --> 00:41:23,980
 Narrator: When juno's titanium
armor finally fails,

813
00:41:23,982 --> 00:41:29,652
 jupiter's deadly radiation will
 damage the craft beyond repair,

814
00:41:29,654 --> 00:41:32,722
   so the team plan to go out
          with a bang,

815
00:41:32,724 --> 00:41:36,459
       thrusting juno into
      jupiter's atmosphere,

816
00:41:36,461 --> 00:41:39,562
         where the craft
     will be torn to pieces.

817
00:41:39,564 --> 00:41:42,866
 Eventually, it'll be drawn down
      into jupiter's depths

818
00:41:42,868 --> 00:41:46,002
        and become a part
      of the planet itself.

819
00:41:46,004 --> 00:41:47,604
   Narrator: But before then,

820
00:41:47,606 --> 00:41:51,307
          juno has many
    more mysteries to unlock.

821
00:41:51,309 --> 00:41:54,310
We'll answer some questions,
   and we'll raise some more.

822
00:41:54,312 --> 00:41:56,079
      That's what I expect

823
00:41:56,081 --> 00:41:59,616
       and we'll get some
        fantastic images.

824
00:41:59,618 --> 00:42:03,052
  Every single thing has turned
      out to be a surprise.

825
00:42:03,054 --> 00:42:05,522
  There are so many things that
juno has opened our eyes to that

826
00:42:05,524 --> 00:42:08,491
         I can't imagine
       having not sent it.

827
00:42:08,493 --> 00:42:10,093
 So we're in for at least a year

828
00:42:10,095 --> 00:42:13,830
    more of the most profound
    surprises about jupiter.

829
00:42:13,832 --> 00:42:16,799
      What we're learning,
      what we're unlocking,

830
00:42:16,801 --> 00:42:18,301
not just about jupiter,

831
00:42:18,303 --> 00:42:20,270
        but the formation
       of the solar system

832
00:42:20,272 --> 00:42:23,239
     and potential formation
         of life itself

833
00:42:23,241 --> 00:42:24,974
         here on earth,

834
00:42:24,976 --> 00:42:26,109
       it's mind-blowing.

835
00:42:26,111 --> 00:42:28,478
                     ♪


