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♪

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narrator: The earth is taking us
    on the ride of our lives,

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     hurtling through space
   in ways we never imagined.

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 The earth is extremely dynamic.

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   It is spinning on its axis.

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  It's whirling about the sun.

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        It's corkscrewing
     throughout this galaxy.

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 It's just never a dull moment.

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     It's like doing a waltz
      on top of a carousel

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          that's on top
     of a high-speed train.

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            Narrator:
Now we're unlocking the secrets

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   of our planet's voyage and
discovering that earth's journey

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         affects us all.

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                     ♪

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 we see evidence of this motion
       everywhere we look,

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     not just in the motions
     of objects in the sky,

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         but in the land
    and the seas themselves.

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          Life on earth
      wouldn't be the same

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   if we didn't find ourselves

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  in this dramatic environment
            in space.

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                     ♪

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narrator: But the ride
       can be dangerous...

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                     ♪

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          [ explosion ]

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       plunging our planet
     into the deep freeze...

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        [ ice cracking ]

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     putting us in the path
         of supernovas,

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                     ♪

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  pulling earth and the entire
   galaxy toward the unknown.

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     The galaxy is traveling
         through space.

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       Where is it going?

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     It's an area of really
         cosmic mystery.

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    Narrator: So strap in for
earth's cosmic journey.

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    [ electricity crackles ]

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          [ explosion ]

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     -- captions by vitac --
          www.Vitac.Com

37
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      captions paid for by
    discovery communications

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                     ♪

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    we are earth's passengers
       as our home planet

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   travels through the cosmos.

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                     ♪

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  to us, everything seems calm.

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    Nothing could be further
         from the truth.

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Contrary to what you might think

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       just based on your
      everyday experience,

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      the earth is actually
     hurtling through space

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        at amazing speeds
   in a lot of different ways.

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      [ crickets chirping ]

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   even just the motion of the
 stars through the sky at night

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 gives you a clue that the earth
      is not sitting still.

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                     ♪

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      the earth is spinning
        at every moment,

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and we can see this most clearly
in the fact

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   that we have day and night.

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            Narrator:
  We might not think about it,

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     but our lives are tuned

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       to earth's journey
   as it spins through space.

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                     ♪

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     there's really nothing
        more basic to us

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     than that cycle of day
 and night, that 24-hour cycle.

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  All of life on earth evolved
    with the day-night cycle,

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     so it's ingrained into
 every organism on this planet.

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                     ♪

64
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narrator:
    Life evolved in lockstep

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  with earth's spinning motion.

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                     ♪

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    but in the ocean, corals
   take things a step further

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                     ♪

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       by keeping a record
    of every planetary turn.

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                     ♪

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    they have a daily cycle,
     which creates a deposit

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    almost like a tree ring,

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     but instead of it being
  once a year, it's once a day.

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      So, you look a bunch
         of tree rings,

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you can count the number
  of years the tree was alive.

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                     ♪

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     corals record not just
        the yearly cycle,

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       but the daily cycle
        of night and day.

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       These are recorded
  in these little growth bands

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          in the coral.

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      Narrator: By counting
    the corals' growth bands,

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         we can work out
  the number of days in a year.

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 Sounds simple, but when we look
  at ancient, fossilized coral,

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we discover something strange.

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We can look at fossils of corals

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  that are hundreds of millions
          of years old,

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 and if we do that, we find that
 the year is not 365 days long.

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  It's more like 420 days long.

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                     ♪

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       narrator: When the
   ancient corals were alive,

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       there were 420 days
       in one earth year,

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                     ♪

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          meaning a day
     was just 21 hours long.

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                     ♪

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         to find out how
this was possible,

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 we need to go back to the start
   of earth's cosmic journey.

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                     ♪

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     4.6 billion years ago,

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       our planet traveled
        a dangerous path

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        through a chaotic
    and violent solar system.

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                     ♪

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          [ explosion ]

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    collisions were frequent.

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                     ♪

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 one giant impact set our planet
       spinning rapidly...

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          [ explosion ]

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                     ♪

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                     ♪

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and formed the moon.

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    Going all the way back to
 the time that the moon formed,

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  the earth may have had a day
    as short as 2 1/2 hours.

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                     ♪

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     narrator: As the earth
      continued on its path

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 through the early solar system,

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       our planet cooled,
  and the surface became solid.

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                     ♪

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  but the violence wasn't over.

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  The young earth was bombarded

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        in the early days
      of the solar system,

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and when these rocks
         hit the earth,

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      they almost never hit
          directly on.

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     They'd hit at an angle.

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                     ♪

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  with each collision, it adds
   a little bit more momentum

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   and a little bit more spin
          to the earth.

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 The added spin that you get is
a kind of like a merry-go-round.

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  You can imagine with each kid
      that pushes and jumps

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     on the merry-go-round,
     you have greater spin.

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     Narrator: As our planet
journeyed on, asteroid impacts

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       set the young earth

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    spinning 12 times faster
       than it does today.

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  Our planet's rotational speed
 has huge consequences for life.

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On earth, the spin of our planet

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     actually has an effect
         on our weather.

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       With a shorter day,

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  one of the effects that might
   have been apparent on earth

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          at that time
   was more storms developing.

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       [ thunder crashes ]

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     narrator: A phenomenon
still in action today

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      drove these powerful
         ancient storms.

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 We call it the coriolis effect.

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        The earth's spin
        creates phenomena

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      in earth's atmosphere
           and oceans.

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    This determines patterns
         of circulation

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       in combination with
  the heat energy from the sun.

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       [ thunder crashes ]

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    the rotation of the earth
   matched with solar heating,

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   especially at the equator,
      causes air to rise up

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and then also sort of to move
   sideways and sets up spin.

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  Narrator: As the young earth
     continued its journey,

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the planet's rotation whipped up
 ferocious, planet-wide storms.

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  The fast spin would have been
    disastrous for any life.

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      The storms would have
          been so big,

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    it's hard to say if life
   would have evolved at all.

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      Narrator: Fortunately
         for humankind,

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           earth has a
     traveling companion --

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the moon, and it helped
     slow our planet's spin.

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 What happened next was kind of
 a wonderful gravitational dance

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    between these two bodies.

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     As they were spinning,
   they were also interacting

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        with each other.

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  Narrator: The moon's gravity
    pulled on earth's oceans,

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    generating tidal bulges.

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 Materials moving in and out of
 the tidal bulges as they spun,

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    and this creates friction
       and a kind of drag

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    that actually slowed down
the rotation.

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                     ♪

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    narrator: The tides also
       helped create life.

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   Giant tides swept nutrients
          from the land

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         into the oceans
       for the first time.

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A primordial soup began brewing.

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                     ♪

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         and life arose.

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                     ♪

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    as earth's spin continued
          to slow down,

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                     ♪

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 life spread across the planet.

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                     ♪

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  but our planet's spin is just
one part of our cosmic ride.

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    Realizing how complicated
     our larger environment

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       in the universe is
      is a wonderful thing.

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   There's so many things that
 affect the orbit of the earth,

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     the tilt of the earth,
 things that affect our climate.

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                     ♪

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   narrator: Clues to earth's
     space voyage are hidden

186
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      all across the world.

187
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       Could our planet's
        wild ride explain

188
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  how one of the driest places
on the planet was once wet?

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                     ♪

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                     ♪

191
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                     ♪

192
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 narrator: The sahara desert --
      dry, dusty, desolate.

193
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                     ♪

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but hidden deep in a desert cave

195
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         is a clue that
     thousands of years ago,

196
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     the sahara was a lush,
         green paradise.

197
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       Archaeologists have
       unearthed rock art

198
00:10:38,739 --> 00:10:45,343
  which clearly depicts humans
 and animals swimming in lakes,

199
00:10:45,345 --> 00:10:47,345
         and by looking
at satellite images,

200
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  we can trace out the outlines
    of ancient river valleys.

201
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                     ♪

202
00:10:54,621 --> 00:10:56,921
   narrator: The earth's fast
       rotation influenced

203
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      our planet's ancient
        weather patterns.

204
00:11:00,761 --> 00:11:05,163
      Could another motion
have changed the desert climate?

205
00:11:05,165 --> 00:11:08,199
     To unravel the mystery,
   we need to rewind the clock

206
00:11:08,201 --> 00:11:10,735
        4.6 billion years

207
00:11:10,737 --> 00:11:14,639
                     ♪

208
00:11:14,641 --> 00:11:18,343
 to when the infant solar system

209
00:11:18,345 --> 00:11:20,545
         was a planetary
        shooting gallery

210
00:11:20,547 --> 00:11:27,218
♪

211
00:11:27,220 --> 00:11:32,857
 and the earth spun through the
solar system with a slight tilt.

212
00:11:32,859 --> 00:11:34,826
       Earlier on, before
   the formation of the moon,

213
00:11:34,828 --> 00:11:36,895
      the earth didn't have
         much of a tilt,

214
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    and the impact knocked us
     completely out of whack

215
00:11:39,166 --> 00:11:40,999
      to about 80 degrees.

216
00:11:41,001 --> 00:11:44,035
          [ explosion ]

217
00:11:47,808 --> 00:11:50,642
 narrator: Our planet might have
      continued its journey

218
00:11:50,644 --> 00:11:53,978
       tilted right over,
   but over billions of years,

219
00:11:53,980 --> 00:11:57,048
    the moon's gravity pulled
       the earth upright,

220
00:11:57,050 --> 00:11:59,084
just not completely.

221
00:11:59,086 --> 00:12:03,421
  The moon is not quite in the
 equatorial plane of the earth.

222
00:12:03,423 --> 00:12:05,356
It's above the equatorial plane,

223
00:12:05,358 --> 00:12:12,263
  and it pulls the earth's axis
   into a 23 1/2-degree tilt.

224
00:12:12,265 --> 00:12:14,799
   Stricker: If we didn't have
  the tilt to about 23 degrees,

225
00:12:14,801 --> 00:12:16,301
      then we wouldn't have
          the seasons,

226
00:12:16,303 --> 00:12:19,704
and these seasons drive a lot of
    the crops and the growth

227
00:12:19,706 --> 00:12:24,409
   and the ability to survive
      all across the globe.

228
00:12:24,411 --> 00:12:26,945
    Narrator: But the ancient
     greening of the sahara

229
00:12:26,947 --> 00:12:31,116
can't be explained
    by the changing seasons.

230
00:12:31,118 --> 00:12:35,587
    Another planetary motion
        must be in play.

231
00:12:35,589 --> 00:12:40,058
     A clue is found in the
          night sky --

232
00:12:40,060 --> 00:12:43,261
         the north star.

233
00:12:43,263 --> 00:12:47,198
   Right now, the earth's axis
    is pointed towards a star

234
00:12:47,200 --> 00:12:50,368
        in the sky called
   the north star -- polaris.

235
00:12:50,370 --> 00:12:52,437
     We've actually named it
         after the fact

236
00:12:52,439 --> 00:12:56,107
that the north pole of the earth
  points toward it in the sky.

237
00:12:56,109 --> 00:13:00,712
  Narrator: But polaris hasn't
   always been the north star.

238
00:13:00,714 --> 00:13:03,081
5,000 years ago,
it was a totally different star.

239
00:13:03,083 --> 00:13:04,883
         It was thuban,
       which is in draco,

240
00:13:04,885 --> 00:13:06,417
   a different constellation.

241
00:13:06,419 --> 00:13:08,419
     Sometime in the future,
         it'll be vega,

242
00:13:08,421 --> 00:13:10,755
       the brightest star
   in the constellation lyra,

243
00:13:10,757 --> 00:13:12,590
        so the north star
        actually changes

244
00:13:12,592 --> 00:13:16,995
    because the north pole's
  position in the sky changes.

245
00:13:16,997 --> 00:13:19,597
Narrator: The changing pole star
           is evidence

246
00:13:19,599 --> 00:13:23,001
     that earth is wobbling
         through space.

247
00:13:23,003 --> 00:13:26,171
It's a process called
           precession,

248
00:13:26,173 --> 00:13:29,707
   something that also affects
         spinning tops.

249
00:13:29,709 --> 00:13:32,343
    Plait: If you take a top
 and let it spin really rapidly

250
00:13:32,345 --> 00:13:33,711
          and poke it,

251
00:13:33,713 --> 00:13:36,981
      the axis of rotation
   will spin around like this,

252
00:13:36,983 --> 00:13:40,118
    and it's much slower than
 the actual spin of the object.

253
00:13:40,120 --> 00:13:44,823
 That is precession, this circle
    that the axis is making.

254
00:13:44,825 --> 00:13:46,991
   This happens to the earth,
            as well.

255
00:13:46,993 --> 00:13:50,595
                     ♪

256
00:13:50,597 --> 00:13:55,066
 narrator: A cosmic poke caused
earth's space wobble,

257
00:13:55,068 --> 00:13:57,602
     but what has the power
        to poke a planet?

258
00:13:57,604 --> 00:14:00,905
                     ♪

259
00:14:00,907 --> 00:14:04,242
 once again, the key is gravity,

260
00:14:04,244 --> 00:14:07,312
        this time earth's
   gravitational interactions

261
00:14:07,314 --> 00:14:10,949
     with the moon and sun.

262
00:14:10,951 --> 00:14:14,419
   These forces are that poke
     on the spinning earth,

263
00:14:14,421 --> 00:14:17,722
    and that's what makes the
earth's axis spin in precession,

264
00:14:17,724 --> 00:14:22,861
 and it takes about 20,000 years
 to make a complete circle once.

265
00:14:22,863 --> 00:14:26,130
Narrator: As the earth continues
   its journey around the sun,

266
00:14:26,132 --> 00:14:29,934
this precession changes the
 planet's climate dramatically.

267
00:14:29,936 --> 00:14:33,271
   When the earth's north pole
      leans toward the sun,

268
00:14:33,273 --> 00:14:35,907
       northern hemisphere
     summers are sunnier...

269
00:14:35,909 --> 00:14:40,411
                     ♪

270
00:14:40,413 --> 00:14:44,148
  with unexpected consequences
         for the sahara.

271
00:14:44,150 --> 00:14:47,252
                     ♪

272
00:14:47,254 --> 00:14:49,587
      rampino: It turns out
       that at times when

273
00:14:49,589 --> 00:14:53,157
    the climate in the sahara
       gets more sunshine,

274
00:14:53,159 --> 00:14:55,126
   that warms the climate up,

275
00:14:55,128 --> 00:14:57,695
      and the winds come in
         from the ocean.

276
00:14:57,697 --> 00:15:01,266
It's called the monsoon effect
       and brings water --

277
00:15:01,268 --> 00:15:04,702
      rain into the sahara,
       where now it's dry.

278
00:15:04,704 --> 00:15:07,305
                     ♪

279
00:15:07,307 --> 00:15:10,575
     olsen: This pattern of
      wet and dry climates

280
00:15:10,577 --> 00:15:12,911
        that produce this
        20,000-year cycle

281
00:15:12,913 --> 00:15:16,948
  is what we see in the sahara,

282
00:15:16,950 --> 00:15:19,117
         where at times
       of strong monsoon,

283
00:15:19,119 --> 00:15:23,421
      the sahara is wetter,
         a green sahara.

284
00:15:23,423 --> 00:15:25,156
   Narrator: 10,000 years ago,

285
00:15:25,158 --> 00:15:27,592
      as the earth wobbled
         around the sun,

286
00:15:27,594 --> 00:15:32,697
monsoons were unleashed,
    turning the desert green.

287
00:15:32,699 --> 00:15:35,767
     Humans migrated to the
        newly lush sahara

288
00:15:35,769 --> 00:15:38,803
 and created the cave paintings
          we see today.

289
00:15:38,805 --> 00:15:40,939
                     ♪

290
00:15:40,941 --> 00:15:45,376
 but this wasn't the first time
 humans crossed a green sahara.

291
00:15:45,378 --> 00:15:48,212
                     ♪

292
00:15:48,214 --> 00:15:51,049
     dartnell: A dry sahara
      would have presented

293
00:15:51,051 --> 00:15:53,451
    an insurmountable barrier

294
00:15:53,453 --> 00:15:57,155
        to our ancestors
  for migrating out of africa,

295
00:15:57,157 --> 00:16:02,260
 but during one of these cycles
   when the sahara was green,

296
00:16:02,262 --> 00:16:04,028
it would have been a corridor

297
00:16:04,030 --> 00:16:06,130
   that we could have migrated
        and dispersed on.

298
00:16:06,132 --> 00:16:08,232
                     ♪

299
00:16:08,234 --> 00:16:10,234
     narrator: As the earth
      traveled the cosmos,

300
00:16:10,236 --> 00:16:13,304
     our planet's precession
       changed the sahara

301
00:16:13,306 --> 00:16:18,543
   and the fate of humankind,
but there are more cosmic forces

302
00:16:18,545 --> 00:16:22,313
      affecting our journey
      through the universe.

303
00:16:22,315 --> 00:16:24,382
The earth's orbit around the sun
        is another thing

304
00:16:24,384 --> 00:16:26,017
  that seems very, very solid.

305
00:16:26,019 --> 00:16:29,120
   We understand how it works,
but everything in the universe

306
00:16:29,122 --> 00:16:31,723
      is a delicately tuned
        dance of gravity,

307
00:16:31,725 --> 00:16:36,861
   and things can change even
  from tiny little influences.

308
00:16:36,863 --> 00:16:39,364
     Narrator: As our planet
     hurtles through space,

309
00:16:39,366 --> 00:16:43,534
other worlds influence our path.

310
00:16:43,536 --> 00:16:48,339
  Could a planetary bully push
 earth's climate to the extreme?

311
00:16:48,341 --> 00:16:51,843
        [ ice cracking ]

312
00:16:54,314 --> 00:17:00,985
                     ♪

313
00:17:00,987 --> 00:17:04,856
 narrator: Earth carries us on a
wild journey through the cosmos.

314
00:17:04,858 --> 00:17:07,592
                     ♪

315
00:17:07,594 --> 00:17:09,894
    and clues to the effects
of this trip

316
00:17:09,896 --> 00:17:12,030
 are hiding in our own backyard.

317
00:17:12,032 --> 00:17:17,168
                     ♪

318
00:17:17,170 --> 00:17:20,171
      [ car horns honking ]

319
00:17:20,173 --> 00:17:22,206
                     ♪

320
00:17:22,208 --> 00:17:27,245
  in new york city, amongst the
     buildings and traffic,

321
00:17:27,247 --> 00:17:30,281
        we find moraines,

322
00:17:30,283 --> 00:17:33,751
        rocks left behind
     by retreating glaciers.

323
00:17:33,753 --> 00:17:38,389
                     ♪

324
00:17:38,391 --> 00:17:39,957
        18,000 years ago,

325
00:17:39,959 --> 00:17:46,097
 a sheet of ice taller than any
  skyscraper covered manhattan.

326
00:17:46,099 --> 00:17:50,001
 Ice ages have struck regularly
   throughout earth's history,

327
00:17:52,172 --> 00:17:55,039
       putting our planet
in a deep freeze.

328
00:17:55,041 --> 00:17:58,076
        [ ice cracking ]

329
00:17:58,078 --> 00:17:59,710
    durda: There was a period
       in earth's history

330
00:17:59,712 --> 00:18:01,746
         several hundred
       million years ago,

331
00:18:01,748 --> 00:18:02,980
   the snowball earth period,

332
00:18:02,982 --> 00:18:06,017
      when we went through
   a very extreme glaciation,

333
00:18:06,019 --> 00:18:07,418
          if you will,
     a very extreme ice age

334
00:18:07,420 --> 00:18:09,687
     where we think perhaps
        the entire earth

335
00:18:09,689 --> 00:18:11,289
  was covered in an ice sheet.

336
00:18:13,259 --> 00:18:15,993
     Narrator: The trigger?

337
00:18:15,995 --> 00:18:18,963
      Earth's orbital dance
         around the sun.

338
00:18:18,965 --> 00:18:21,999
♪

339
00:18:22,001 --> 00:18:23,201
  we tend to think of ourselves

340
00:18:23,203 --> 00:18:24,902
  sitting relatively stationary
          on the earth.

341
00:18:24,904 --> 00:18:26,637
     It's pretty comforting,
            actually,

342
00:18:26,639 --> 00:18:32,176
   but we're orbiting the sun
 at about 66,000 miles per hour.

343
00:18:32,178 --> 00:18:36,147
   Narrator: Every day, earth
 travels over 1.6 million miles

344
00:18:36,149 --> 00:18:40,017
         on its journey
         around the sun.

345
00:18:40,019 --> 00:18:43,121
     This orbit isn't always
        completely round.

346
00:18:43,123 --> 00:18:47,091
                     ♪

347
00:18:47,093 --> 00:18:48,826
    earth is generally going
         around the sun

348
00:18:48,828 --> 00:18:51,529
in more or less
        a circular orbit,

349
00:18:51,531 --> 00:18:56,200
  but over time, the massaging
   of this orbit from the sun,

350
00:18:56,202 --> 00:18:58,536
          from the moon
      on the earth's orbit

351
00:18:58,538 --> 00:19:02,006
  causes the orbit of the earth
            to change

352
00:19:02,008 --> 00:19:03,674
        so that sometimes
        it's an ellipse.

353
00:19:03,676 --> 00:19:05,476
            Sometimes
     it's more of a circle.

354
00:19:05,478 --> 00:19:08,146
                     ♪

355
00:19:08,148 --> 00:19:09,580
     right now on the earth,

356
00:19:09,582 --> 00:19:12,150
    we're in kind of the most
   circular time in the orbit,

357
00:19:12,152 --> 00:19:14,819
    so that means the summers
are relatively mild,

358
00:19:14,821 --> 00:19:16,821
         and the winters
      are relatively mild,

359
00:19:16,823 --> 00:19:19,190
  but imagine not that long ago
          in the past,

360
00:19:19,192 --> 00:19:22,593
    it could have been really
     dramatically different.

361
00:19:22,595 --> 00:19:26,164
 When the earth is a little bit
       closer to the sun,

362
00:19:26,166 --> 00:19:28,466
         maybe you have
     a really severe summer,

363
00:19:28,468 --> 00:19:29,901
   and then on the other side
          of the orbit,

364
00:19:29,903 --> 00:19:31,602
  you're a little farther away
    from the sun than normal,

365
00:19:31,604 --> 00:19:33,671
           so you have
     a really severe winter.

366
00:19:33,673 --> 00:19:37,108
♪

367
00:19:37,110 --> 00:19:40,878
    our environment is very,
 very sensitive to these things,

368
00:19:40,880 --> 00:19:42,914
   and when the earth's orbit
        is stretched out,

369
00:19:42,916 --> 00:19:45,349
        that can actually
       trigger an ice age.

370
00:19:45,351 --> 00:19:48,986
                     ♪

371
00:19:48,988 --> 00:19:51,789
     narrator: Our planet's
   100,000-year orbital cycle

372
00:19:51,791 --> 00:19:54,592
       caused the ice age
      that buried new york.

373
00:19:58,798 --> 00:20:04,635
   And ice ages have had a big
    effect on human history.

374
00:20:04,637 --> 00:20:06,437
        15,000 years ago,

375
00:20:06,439 --> 00:20:08,739
      plunging temperatures
        locked water away

376
00:20:08,741 --> 00:20:11,542
in glaciers and ice caps.

377
00:20:11,544 --> 00:20:17,415
  Sea levels dropped, creating
land bridges between continents.

378
00:20:17,417 --> 00:20:22,420
    Humans migrated from asia
       to america by foot,

379
00:20:22,422 --> 00:20:26,157
     and for the first time,
     america was inhabited.

380
00:20:26,159 --> 00:20:29,527
                     ♪

381
00:20:29,529 --> 00:20:34,498
 may 2018 -- scientists revealed
       a whole new dynamic

382
00:20:34,500 --> 00:20:36,100
       to earth's journey.

383
00:20:36,102 --> 00:20:38,269
                     ♪

384
00:20:38,271 --> 00:20:41,072
      every 405,000 years,

385
00:20:41,074 --> 00:20:45,243
   our planet's orbital voyage
    stretches to the extreme,

386
00:20:45,245 --> 00:20:50,414
 and earth's planetary neighbors
are to blame.

387
00:20:50,416 --> 00:20:52,850
   Because jupiter is the most
         massive planet

388
00:20:52,852 --> 00:20:54,218
      in our solar system,

389
00:20:54,220 --> 00:20:57,221
  it is in many ways the bully
    on the playground, right?

390
00:20:57,223 --> 00:21:00,725
    Its dynamics, its gravity
  sculpts a lot of the dynamics

391
00:21:00,727 --> 00:21:02,326
      of the solar system.

392
00:21:02,328 --> 00:21:04,562
                     ♪

393
00:21:04,564 --> 00:21:06,797
     durda: It actually tugs
     and pulls on the orbit

394
00:21:06,799 --> 00:21:08,299
      of the earth itself.

395
00:21:08,301 --> 00:21:10,501
  It's responsible for some of
        the very changes

396
00:21:10,503 --> 00:21:13,170
  that drive our climatic cycle
       here on our planet.

397
00:21:13,172 --> 00:21:16,307
♪

398
00:21:16,309 --> 00:21:19,010
narrator: Jupiter isn't the only
    bully in the playground.

399
00:21:19,012 --> 00:21:20,878
                     ♪

400
00:21:20,880 --> 00:21:22,580
        thaller: Venus is
       a fairly big planet

401
00:21:22,582 --> 00:21:24,282
   about the size of the earth

402
00:21:24,284 --> 00:21:26,684
     and also comes closest
       to us in its orbit,

403
00:21:26,686 --> 00:21:30,254
  so these two planets put just
    a little tiny elongation

404
00:21:30,256 --> 00:21:31,789
     onto our earth's orbit,

405
00:21:31,791 --> 00:21:34,458
   and as the cycle continues,
    the more extreme it gets,

406
00:21:34,460 --> 00:21:36,594
     we can actually notice
    a temperature difference

407
00:21:36,596 --> 00:21:40,230
that happens about once
      every 405,000 years.

408
00:21:40,232 --> 00:21:43,501
                     ♪

409
00:21:43,503 --> 00:21:47,038
narrator: Jupiter and venus gang
  up on earth gravitationally,

410
00:21:47,040 --> 00:21:52,243
      pulling earth's orbit
  into an even greater ellipse.

411
00:21:52,245 --> 00:21:54,845
    Our planet's hot weather
         becomes hotter,

412
00:21:54,847 --> 00:21:58,082
      and its cold weather
        gets much colder.

413
00:21:58,084 --> 00:22:02,887
                     ♪

414
00:22:02,889 --> 00:22:05,756
   today, we're in a moderate
       part of the cycle,

415
00:22:05,758 --> 00:22:08,659
           but in just
       60,000 years time,

416
00:22:08,661 --> 00:22:14,031
         we could plunge
into another deep freeze.

417
00:22:14,033 --> 00:22:16,067
     It's a little bit like
   a cosmic butterfly effect.

418
00:22:16,069 --> 00:22:18,235
          I mean, even
      the smallest effects

419
00:22:18,237 --> 00:22:21,539
       can have, you know,
   a big influence over time.

420
00:22:21,541 --> 00:22:24,542
                     ♪

421
00:22:24,544 --> 00:22:26,110
            narrator:
  Earth's orbit around the sun

422
00:22:26,112 --> 00:22:29,680
       is just part of our
   far larger cosmic journey.

423
00:22:29,682 --> 00:22:32,249
                     ♪

424
00:22:32,251 --> 00:22:35,753
   the entire solar system is
 hurtling around the milky way,

425
00:22:35,755 --> 00:22:38,856
                     ♪

426
00:22:38,858 --> 00:22:43,227
        taking us places
we don't want to be.

427
00:22:43,229 --> 00:22:45,796
      Sometimes our planet
          might wander

428
00:22:45,798 --> 00:22:48,466
     into what's essentially
       a bad neighborhood.

429
00:22:48,468 --> 00:22:50,267
Narrator: What dangers await us?

430
00:22:50,269 --> 00:22:53,671
  And could these neighborhoods
         spell disaster

431
00:22:53,673 --> 00:22:55,272
       for life on earth?

432
00:22:56,809 --> 00:23:03,414
                     ♪

433
00:23:03,416 --> 00:23:09,954
                     ♪

434
00:23:09,956 --> 00:23:14,291
     narrator: Over the last
       3.7 billion years,

435
00:23:14,293 --> 00:23:16,961
  a series of extinction events
            wiped out

436
00:23:16,963 --> 00:23:20,898
        almost 95 percent
    of all species on earth.

437
00:23:22,568 --> 00:23:24,769
[ explosion ]

438
00:23:24,771 --> 00:23:28,038
                     ♪

439
00:23:28,040 --> 00:23:30,908
      now research suggests
       our planet's orbit

440
00:23:30,910 --> 00:23:33,277
    could be partly to blame,

441
00:23:33,279 --> 00:23:36,714
    but not the earth's orbit
         around the sun,

442
00:23:36,716 --> 00:23:42,253
 our planet's larger and longer
  journey around the milky way.

443
00:23:42,255 --> 00:23:45,456
  Our solar system and our sun
 is shooting through the galaxy

444
00:23:45,458 --> 00:23:51,395
 at about 530,000 miles per hour
around the center of our galaxy.

445
00:23:51,397 --> 00:23:54,665
And that center of the galaxy is
 about 26,000 light-years away,

446
00:23:54,667 --> 00:23:57,735
    so it should take the sun
about 230 million years

447
00:23:57,737 --> 00:24:01,038
   to trace out one full orbit
around the center of the galaxy.

448
00:24:01,040 --> 00:24:03,574
                     ♪

449
00:24:03,576 --> 00:24:05,609
    narrator: Despite racing
      around the milky way

450
00:24:05,611 --> 00:24:08,913
  at 1/2 million miles an hour,

451
00:24:08,915 --> 00:24:12,716
  earth has completed less than
      20 laps of the galaxy

452
00:24:12,718 --> 00:24:16,520
 in our planet's entire history,

453
00:24:16,522 --> 00:24:19,990
        and it turns out
       this galactic ride

454
00:24:19,992 --> 00:24:22,860
       is more complicated
         than it seems.

455
00:24:22,862 --> 00:24:24,995
  Now, if you look at the earth
      going around the sun,

456
00:24:24,997 --> 00:24:26,430
it defines an ellipse,

457
00:24:26,432 --> 00:24:28,933
    but that's a flat figure,
        and you'd think,

458
00:24:28,935 --> 00:24:32,336
  "well, the sun probably goes
  around in a plane, as well,"

459
00:24:32,338 --> 00:24:34,805
        and it turns out
        not that simple.

460
00:24:34,807 --> 00:24:37,641
                     ♪

461
00:24:37,643 --> 00:24:39,777
   narrator: Most of the mass
       of the solar system

462
00:24:39,779 --> 00:24:42,079
   is concentrated in the sun,

463
00:24:42,081 --> 00:24:46,784
 so earth and the other planets
    smoothly orbit our star.

464
00:24:46,786 --> 00:24:50,187
                     ♪

465
00:24:50,189 --> 00:24:55,359
  but the mass of the milky way
     is spread out unevenly.

466
00:24:55,361 --> 00:24:57,862
    That changes the gravity
of the galaxy,

467
00:24:57,864 --> 00:25:00,831
  and so it changes how things
    move in it, and in fact,

468
00:25:00,833 --> 00:25:03,934
 if you give something a little
  bit of an up or down motion,

469
00:25:03,936 --> 00:25:07,371
      it'll bob up and down
       as it goes around.

470
00:25:07,373 --> 00:25:10,574
  Oluseyi: Riding the earth is
 almost like riding a carousel.

471
00:25:10,576 --> 00:25:13,477
    As the sun and the earth
      go around the galaxy,

472
00:25:13,479 --> 00:25:15,246
  the sun also goes up and down

473
00:25:15,248 --> 00:25:17,381
      like you're on one of
   those horses with the pole,

474
00:25:17,383 --> 00:25:19,049
     and so what this can do

475
00:25:19,051 --> 00:25:22,820
    is take us into different
galactic environments.

476
00:25:22,822 --> 00:25:26,156
                     ♪

477
00:25:26,158 --> 00:25:29,426
  narrator: This bobbing motion
takes earth and the solar system

478
00:25:29,428 --> 00:25:31,662
    on a 60,000-year journey

479
00:25:31,664 --> 00:25:35,432
       up and down through
 the milky way's galactic plane.

480
00:25:35,434 --> 00:25:37,868
                     ♪

481
00:25:37,870 --> 00:25:39,370
     our orbit also takes us

482
00:25:39,372 --> 00:25:41,872
        through different
     galactic neighborhoods.

483
00:25:41,874 --> 00:25:45,376
                     ♪

484
00:25:45,378 --> 00:25:50,948
 today, we're traveling through
  a calm suburb of the galaxy.

485
00:25:50,950 --> 00:25:55,352
      But sometimes things
       get a little bumpy.

486
00:25:55,354 --> 00:25:59,089
Sometimes our sun and our planet
          might wander

487
00:25:59,091 --> 00:26:01,659
     into what's essentially
       a bad neighborhood.

488
00:26:01,661 --> 00:26:02,993
  You know, maybe it's an area

489
00:26:02,995 --> 00:26:04,962
     where there's a lot of
    star formation going on,

490
00:26:04,964 --> 00:26:07,898
  where there's a lot of young
   stars that are very active,

491
00:26:07,900 --> 00:26:11,101
    or maybe it's a location
  where there are dying stars,

492
00:26:11,103 --> 00:26:14,104
      and things are about
       to get really hot.

493
00:26:14,106 --> 00:26:16,774
      Narrator: The baddest
   neighborhoods in the galaxy

494
00:26:16,776 --> 00:26:19,310
     may be the spiral arms.

495
00:26:19,312 --> 00:26:21,845
♪

496
00:26:21,847 --> 00:26:25,282
 these gas-filled regions orbit
       the galactic center

497
00:26:25,284 --> 00:26:28,819
   more slowly than the earth,

498
00:26:28,821 --> 00:26:31,989
          so our planet
      passes through an arm

499
00:26:31,991 --> 00:26:35,559
roughly every 150 million years.

500
00:26:35,561 --> 00:26:39,296
   Plait: These arms are where
  gas clouds tend to hang out,

501
00:26:39,298 --> 00:26:43,834
   and if they get compressed,
    they form a lot of stars.

502
00:26:43,836 --> 00:26:48,205
 When they form a lot of stars,
  they make bright, blue stars.

503
00:26:48,207 --> 00:26:51,642
    And they don't last long,
 and they blow up as supernovae.

504
00:26:51,644 --> 00:26:56,680
                     ♪

505
00:26:56,682 --> 00:27:00,351
[ explosion ]

506
00:27:00,353 --> 00:27:03,887
 so it's possible that as we're
 passing through these regions,

507
00:27:03,889 --> 00:27:06,824
 these are places you might not
         want to be in,

508
00:27:06,826 --> 00:27:08,225
     so in the distant past,

509
00:27:08,227 --> 00:27:10,127
          this may have
       affected the earth.

510
00:27:10,129 --> 00:27:15,432
                     ♪

511
00:27:15,434 --> 00:27:17,501
   narrator: When giant stars
          go supernova,

512
00:27:17,503 --> 00:27:20,237
     the stars' outer layers
        blast into space

513
00:27:20,239 --> 00:27:23,907
                     ♪

514
00:27:23,909 --> 00:27:25,409
     along with a shock wave

515
00:27:25,411 --> 00:27:28,212
          traveling at
     20,000 miles a second.

516
00:27:28,214 --> 00:27:31,615
                     ♪

517
00:27:31,617 --> 00:27:37,154
supernovas also release
         cosmic rays --

518
00:27:37,156 --> 00:27:39,890
          space bullets
  that shoot across the galaxy

519
00:27:39,892 --> 00:27:41,792
 at close to the speed of light.

520
00:27:41,794 --> 00:27:44,461
                     ♪

521
00:27:44,463 --> 00:27:46,630
 plait: And you don't want to be
  exposed to too many of them,

522
00:27:46,632 --> 00:27:47,998
    but in high enough doses,

523
00:27:48,000 --> 00:27:50,634
these things penetrate our cells
       and damage our dna

524
00:27:50,636 --> 00:27:54,538
and over the long-term can cause
        really bad damage

525
00:27:54,540 --> 00:27:57,074
        to human bodies.

526
00:27:57,076 --> 00:27:58,676
            Narrator:
    As we ride through space,

527
00:27:58,678 --> 00:28:04,782
earth's magnetic field protects
    us from most cosmic rays.

528
00:28:04,784 --> 00:28:08,719
          But in 2018,
     we discovered evidence

529
00:28:08,721 --> 00:28:10,688
  that a hail of space bullets

530
00:28:10,690 --> 00:28:15,559
    overwhelmed our planet's
   magnetic field in the past.

531
00:28:15,561 --> 00:28:17,561
          In many ways,
   we really take for granted

532
00:28:17,563 --> 00:28:20,631
          how the earth
     protects us from space,

533
00:28:20,633 --> 00:28:22,199
      but there are records
   that we've actually bounced

534
00:28:22,201 --> 00:28:25,869
       a little too close
       to exploding stars.

535
00:28:25,871 --> 00:28:28,005
  Plait: Sediments in the ocean
            show that

536
00:28:28,007 --> 00:28:30,107
about 2 million years ago,

537
00:28:30,109 --> 00:28:33,310
      iron-60 was deposited
         in our oceans.

538
00:28:33,312 --> 00:28:36,046
          Iron-60 is a
  radioactive isotope of iron,

539
00:28:36,048 --> 00:28:38,749
 and there's only way we know of
 it being made in the universe,

540
00:28:38,751 --> 00:28:41,351
  and that is exploding stars.

541
00:28:41,353 --> 00:28:45,689
                     ♪

542
00:28:45,691 --> 00:28:47,725
            narrator:
  Around 2.8 million years ago,

543
00:28:47,727 --> 00:28:52,162
      a supernova exploded
just 150 light-years from earth.

544
00:28:54,567 --> 00:28:56,200
   A few hundred years later,

545
00:28:56,202 --> 00:29:00,104
    a blizzard of cosmic rays
     slammed into the earth,

546
00:29:00,106 --> 00:29:02,406
tearing through
       our magnetic field.

547
00:29:02,408 --> 00:29:06,443
                     ♪

548
00:29:06,445 --> 00:29:10,481
     these space bullets are
 prime suspect in the extinction

549
00:29:10,483 --> 00:29:13,450
         of over 1/3 of
   all coastal marine species.

550
00:29:13,452 --> 00:29:16,120
                     ♪

551
00:29:16,122 --> 00:29:18,422
     plait: Now, this is not
  necessarily tied to the earth

552
00:29:18,424 --> 00:29:21,125
       passing through one
      of these spiral arms,

553
00:29:21,127 --> 00:29:23,861
        but it shows you
 that being close to a supernova

554
00:29:23,863 --> 00:29:28,098
   is not necessarily a thing
         you want to do.

555
00:29:28,100 --> 00:29:30,067
            Narrator:
Millions of years in the future,

556
00:29:30,069 --> 00:29:33,637
     earth will pass through
       another spiral arm

557
00:29:33,639 --> 00:29:39,409
   as our planet continues its
 journey through the milky way.

558
00:29:39,411 --> 00:29:43,781
       And we will wander
   into harm's way once again.

559
00:29:46,619 --> 00:29:49,019
 But there's another part of our
      journey through space

560
00:29:49,021 --> 00:29:51,889
     that remains a mystery.

561
00:29:51,891 --> 00:29:54,825
The earth is spinning like a top
          on its axis.

562
00:29:54,827 --> 00:29:56,260
  It's orbiting around the sun.

563
00:29:56,262 --> 00:29:58,662
   The sun itself is orbiting
        around the center

564
00:29:58,664 --> 00:30:03,500
        of the milky way,
but that's far from it.

565
00:30:03,502 --> 00:30:06,170
   Narrator: The milky way is
 speeding through the universe,

566
00:30:06,172 --> 00:30:11,375
    and we are being dragged
       along for the ride.

567
00:30:11,377 --> 00:30:14,912
   The problem is we can't see
       where we're going.

568
00:30:14,914 --> 00:30:18,582
      Could earth be headed
      for a galactic crash?

569
00:30:18,584 --> 00:30:20,851
                     ♪

570
00:30:22,388 --> 00:30:27,658
                     ♪

571
00:30:27,660 --> 00:30:30,627
          [ screaming ]

572
00:30:30,629 --> 00:30:32,763
                     ♪

573
00:30:32,765 --> 00:30:35,399
   narrator: Like the craziest
      of theme park rides,

574
00:30:35,401 --> 00:30:39,703
  we are riding the earth on a
wild journey through the cosmos.

575
00:30:39,705 --> 00:30:46,443
♪

576
00:30:46,445 --> 00:30:50,981
  our planet spins, tilts, and
 wobbles around the solar system

577
00:30:50,983 --> 00:30:53,116
                     ♪

578
00:30:53,118 --> 00:30:56,720
  while bobbing like a carousel
     through the milky way.

579
00:30:56,722 --> 00:30:59,223
                     ♪

580
00:30:59,225 --> 00:31:03,026
    the dynamics of the earth
  moving in the cosmic void is,

581
00:31:03,028 --> 00:31:06,697
   like, the most unbelievable
 journey you could ever imagine,

582
00:31:06,699 --> 00:31:08,699
and as you get to larger scales,

583
00:31:08,701 --> 00:31:12,169
 the motions only become grander
  and larger and more dynamic.

584
00:31:12,171 --> 00:31:16,039
                     ♪

585
00:31:16,041 --> 00:31:19,176
       narrator: In 1977,
we tried to work out

586
00:31:19,178 --> 00:31:21,078
  the largest motion of all --

587
00:31:21,080 --> 00:31:23,647
                     ♪

588
00:31:23,649 --> 00:31:27,851
   the movement of our galaxy
      through the universe.

589
00:31:27,853 --> 00:31:31,154
        Clues hide in the
  cosmic microwave background,

590
00:31:31,156 --> 00:31:34,524
    a remnant from the birth
        of the universe.

591
00:31:34,526 --> 00:31:37,094
  Bullock: The cosmic microwave
   background is the radiation

592
00:31:37,096 --> 00:31:40,397
        that's left over
     from the hot big bang.

593
00:31:40,399 --> 00:31:43,166
 The cosmic microwave background
  is shining in all directions

594
00:31:43,168 --> 00:31:44,902
  as sort of this fixed thing,

595
00:31:44,904 --> 00:31:47,337
and if we're moving through it
        with some speed,

596
00:31:47,339 --> 00:31:49,373
        we will see that
      in the light itself.

597
00:31:49,375 --> 00:31:51,275
      You can measure that,
     and by measuring that,

598
00:31:51,277 --> 00:31:55,946
 you can get a sense of how fast
we're moving through that space.

599
00:31:55,948 --> 00:31:58,115
    Narrator: By tracking our
  movement through the universe

600
00:31:58,117 --> 00:31:59,716
     against a fixed point,

601
00:31:59,718 --> 00:32:03,553
 we can work out the milky way's
      speed and direction.

602
00:32:03,555 --> 00:32:06,390
                     ♪

603
00:32:06,392 --> 00:32:13,030
 but in 1977, telescopes weren't
   the best tool for the job.

604
00:32:13,032 --> 00:32:15,565
Tremblay:
   During the cold war, 1977,

605
00:32:15,567 --> 00:32:18,201
 you have the newly declassified
         u-2 spy plane,

606
00:32:18,203 --> 00:32:21,238
     this very high-altitude
    reconnaissance aircraft.

607
00:32:21,240 --> 00:32:24,775
  Nasa retrofitted one of them
  with an upward-facing window,

608
00:32:24,777 --> 00:32:26,710
          and with very
      sensitive receivers,

609
00:32:26,712 --> 00:32:29,379
      this spy plane became
      the first experiment

610
00:32:29,381 --> 00:32:32,849
      to for the first time
 definitively measure the motion

611
00:32:32,851 --> 00:32:35,018
          of the galaxy
      through the universe.

612
00:32:35,020 --> 00:32:38,121
 Narrator: As the u-2 spy plane
soared above the earth,

613
00:32:38,123 --> 00:32:41,024
         it measured the
   cosmic microwave background

614
00:32:41,026 --> 00:32:42,893
    in unprecedented detail.

615
00:32:42,895 --> 00:32:46,096
                     ♪

616
00:32:46,098 --> 00:32:49,366
        the data revealed
      that our galaxy races

617
00:32:49,368 --> 00:32:53,537
      through the universe
     at 370 miles a second.

618
00:32:53,539 --> 00:32:57,374
                     ♪

619
00:32:57,376 --> 00:32:59,476
   that's over 1 million miles
            an hour.

620
00:32:59,478 --> 00:33:03,347
                     ♪

621
00:33:03,349 --> 00:33:05,949
    sutter: Think of how big
          a galaxy is.

622
00:33:05,951 --> 00:33:08,819
 Hundreds of millions of stars,

623
00:33:08,821 --> 00:33:12,622
       and we're moving at
hundreds of miles per second.

624
00:33:12,624 --> 00:33:14,725
     That's just a tiny bit
          mind-blowing.

625
00:33:14,727 --> 00:33:16,860
                     ♪

626
00:33:16,862 --> 00:33:20,130
 narrator: The milky way's speed
  isn't the most alarming part

627
00:33:20,132 --> 00:33:22,766
    of our galactic journey.

628
00:33:22,768 --> 00:33:26,703
  From earth, we can't even see
   in the direction our galaxy

629
00:33:26,705 --> 00:33:28,071
          is taking us.

630
00:33:28,073 --> 00:33:29,639
       We're flying blind.

631
00:33:29,641 --> 00:33:33,110
       Our view is blocked
    by the milky way itself.

632
00:33:33,112 --> 00:33:36,079
                     ♪

633
00:33:36,081 --> 00:33:38,682
  so if you're actually looking
through the plane of the galaxy,

634
00:33:38,684 --> 00:33:40,584
through the plane
         of the pancake,

635
00:33:40,586 --> 00:33:43,220
     your view of the galaxy
           is obscured

636
00:33:43,222 --> 00:33:47,924
   by curtains of dust and gas
 that envelop our solar system.

637
00:33:47,926 --> 00:33:49,726
   Bullock: It's very bright.
     There's a lot of stars.

638
00:33:49,728 --> 00:33:53,130
     And our view is blocked
      by the galaxy itself,

639
00:33:53,132 --> 00:33:56,166
        so there's a zone
   directly behind the galaxy

640
00:33:56,168 --> 00:33:58,402
       as we look towards
       the galactic center

641
00:33:58,404 --> 00:34:00,270
 that's really an unknown area.

642
00:34:00,272 --> 00:34:02,305
       It's a zone we call
     the zone of avoidance,

643
00:34:02,307 --> 00:34:05,075
and it's an area of really
         cosmic mystery.

644
00:34:05,077 --> 00:34:07,310
                     ♪

645
00:34:07,312 --> 00:34:11,081
    narrator: Thanks to this
        mysterious zone,

646
00:34:11,083 --> 00:34:14,851
  we thought we could be headed
    for a galactic car crash.

647
00:34:14,853 --> 00:34:20,323
                     ♪

648
00:34:20,325 --> 00:34:22,459
   then we had a breakthrough.

649
00:34:22,461 --> 00:34:28,665
                     ♪

650
00:34:28,667 --> 00:34:31,268
        we used powerful
        radio telescopes

651
00:34:31,270 --> 00:34:33,570
         to look through
      the zone of avoidance

652
00:34:33,572 --> 00:34:35,072
       for the first time.

653
00:34:35,074 --> 00:34:41,678
                     ♪

654
00:34:41,680 --> 00:34:44,247
 bullock: One of the nice things
about using light that's

655
00:34:44,249 --> 00:34:47,784
 in the radio is that this kind
of light actually can go through

656
00:34:47,786 --> 00:34:50,353
       pretty dense kinds
        of gas and stars

657
00:34:50,355 --> 00:34:53,757
          and allows us
 to sort of look through things.

658
00:34:53,759 --> 00:34:55,926
  Using these radio telescopes
     has given us a glimpse

659
00:34:55,928 --> 00:35:00,530
      into what lies beyond
     the zone of avoidance.

660
00:35:00,532 --> 00:35:03,366
    Narrator: Peering through
     the zone of avoidance,

661
00:35:03,368 --> 00:35:07,070
  we found that the milky way's
         path is clear,

662
00:35:07,072 --> 00:35:08,872
       but that's not all.

663
00:35:08,874 --> 00:35:12,442
We also discovered we are just
          one tiny part

664
00:35:12,444 --> 00:35:14,978
  of a vast cluster of galaxies

665
00:35:14,980 --> 00:35:18,081
         sailing through
      the cosmos together.

666
00:35:18,083 --> 00:35:20,383
    We think that our galaxy,
         the milky way,

667
00:35:20,385 --> 00:35:24,354
    is part of a much grander
    cosmic flow of galaxies,

668
00:35:24,356 --> 00:35:26,056
 and it is part of what might be

669
00:35:26,058 --> 00:35:28,391
    the laniakea supercluster
          of galaxies,

670
00:35:28,393 --> 00:35:30,861
        this giant, giant
        cosmic structure

671
00:35:30,863 --> 00:35:33,463
     filled with potentially
      thousands of galaxies

672
00:35:33,465 --> 00:35:35,565
     that is moving together
in this beautiful,

673
00:35:35,567 --> 00:35:37,400
     like, slow-moving river

674
00:35:37,402 --> 00:35:40,437
  that is sculpted and dictated
       by gravity itself.

675
00:35:40,439 --> 00:35:43,206
                     ♪

676
00:35:43,208 --> 00:35:47,043
 narrator: Earth voyages through
space along gravitational rivers

677
00:35:47,045 --> 00:35:50,680
      hundreds of millions
       of light-years long

678
00:35:50,682 --> 00:35:54,618
       along with a fleet
   of 100,000 other galaxies,

679
00:35:54,620 --> 00:35:58,622
        all moving toward
    a single point in space,

680
00:35:58,624 --> 00:36:04,728
      a gravitational drain
  known as the great attractor.

681
00:36:04,730 --> 00:36:10,500
 Sutter: The great attractor is
the local region of gravity,

682
00:36:10,502 --> 00:36:13,670
        of strong gravity
 in this patch of the universe.

683
00:36:13,672 --> 00:36:16,973
   It's where all the galaxies
  in this chunk of the universe

684
00:36:16,975 --> 00:36:20,043
      are flowing towards.

685
00:36:20,045 --> 00:36:22,812
     At the location of the
         great attractor

686
00:36:22,814 --> 00:36:23,980
    is a bunch of material --

687
00:36:23,982 --> 00:36:25,882
         a bunch of gas,
      a bunch of galaxies,

688
00:36:25,884 --> 00:36:29,085
  an extremely massive cluster,

689
00:36:29,087 --> 00:36:33,290
         and over time,
     more and more galaxies

690
00:36:33,292 --> 00:36:35,659
 add themselves to this cluster

691
00:36:35,661 --> 00:36:40,230
    as they continue to join
the great attractor.

692
00:36:40,232 --> 00:36:42,933
  Narrator: It's unlikely earth
         will ever reach

693
00:36:42,935 --> 00:36:45,669
      the great attractor.

694
00:36:45,671 --> 00:36:52,442
It seems the milky way is headed
   for a collision after all.

695
00:36:52,444 --> 00:36:55,579
         Is this how our
      cosmic journey ends?

696
00:36:55,581 --> 00:36:57,280
                     ♪

697
00:36:58,650 --> 00:37:06,890
                     ♪

698
00:37:06,892 --> 00:37:08,959
    narrator: Earth's voyage
        across the cosmos

699
00:37:08,961 --> 00:37:12,762
           has lasted
     for 4.5 billion years.

700
00:37:12,764 --> 00:37:17,634
                     ♪

701
00:37:17,636 --> 00:37:21,938
the big question -- how will our
      journey finally end?

702
00:37:21,940 --> 00:37:25,008
♪

703
00:37:25,010 --> 00:37:27,043
        a clue comes from
         the milky way's

704
00:37:27,045 --> 00:37:31,114
     traveling companion --
   another galaxy, andromeda,

705
00:37:31,116 --> 00:37:34,584
                     ♪

706
00:37:34,586 --> 00:37:37,320
         filled with up
       to a trillion stars

707
00:37:37,322 --> 00:37:40,090
         that's charting
      a similar path to us.

708
00:37:40,092 --> 00:37:44,995
                     ♪

709
00:37:44,997 --> 00:37:47,897
 the andromeda galaxy is another
       big spiral galaxy,

710
00:37:47,899 --> 00:37:49,532
    a lot like our milky way,

711
00:37:49,534 --> 00:37:54,604
 and it turns out the two of us
   are heading for each other.

712
00:37:54,606 --> 00:37:56,640
       Narrator: Andromeda
and the milky way

713
00:37:56,642 --> 00:38:00,677
    are currently 2.5 million
       light-years apart,

714
00:38:00,679 --> 00:38:03,280
      but they're hurtling
       towards each other

715
00:38:03,282 --> 00:38:06,016
 at over 250,000 miles an hour.

716
00:38:06,018 --> 00:38:08,818
                     ♪

717
00:38:08,820 --> 00:38:12,255
   a collision is inevitable.

718
00:38:12,257 --> 00:38:13,923
  Stricker: Galaxies colliding
         with each other

719
00:38:13,925 --> 00:38:15,759
  sounds like science fiction,

720
00:38:15,761 --> 00:38:17,861
      but the collision of
      the andromeda galaxy

721
00:38:17,863 --> 00:38:22,565
    and the milky way galaxy
  will be a spectacular event.

722
00:38:22,567 --> 00:38:25,101
 Oluseyi: When the andromeda and
milky way galaxies collide,

723
00:38:25,103 --> 00:38:28,872
          it's gonna be
    a ridiculous light show.

724
00:38:28,874 --> 00:38:32,876
    The stars don't collide,
 but the giant clouds of gas do,

725
00:38:32,878 --> 00:38:35,111
    and that's gonna trigger
         star formation,

726
00:38:35,113 --> 00:38:38,381
   so we're gonna have what's
  known as a starburst galaxy.

727
00:38:38,383 --> 00:38:40,517
                     ♪

728
00:38:40,519 --> 00:38:43,453
  when andromeda finally merges
       with the milky way,

729
00:38:43,455 --> 00:38:45,488
        all bets are off.

730
00:38:45,490 --> 00:38:48,525
    All of a sudden, a system
of hundreds of billions of stars

731
00:38:48,527 --> 00:38:52,362
    will be added to our own,
and there will be mass chaos,

732
00:38:52,364 --> 00:38:54,130
          but one thing
      you can guarantee --

733
00:38:54,132 --> 00:38:56,633
      there is going to be
      celestial fireworks.

734
00:38:56,635 --> 00:38:59,869
                     ♪

735
00:38:59,871 --> 00:39:02,939
   narrator: This could be the
 biggest light show in history,

736
00:39:02,941 --> 00:39:07,911
    resulting in the creation
     of a brand-new galaxy.

737
00:39:07,913 --> 00:39:11,214
       We will have become
        one giant galaxy.

738
00:39:11,216 --> 00:39:13,483
      Call it milkdromeda,
          if you will,

739
00:39:13,485 --> 00:39:15,251
 so we will look very different.

740
00:39:15,253 --> 00:39:18,822
    Our grand-design, spiral
        milky way galaxy

741
00:39:18,824 --> 00:39:21,891
will have probably
       transformed itself

742
00:39:21,893 --> 00:39:26,296
        into an entirely
        different shape.

743
00:39:26,298 --> 00:39:28,531
 Narrator: The merging galaxies
          could create

744
00:39:28,533 --> 00:39:31,668
            a giant,
    elliptical-shaped galaxy,

745
00:39:31,670 --> 00:39:35,271
       but earth might not
      be around to see it.

746
00:39:35,273 --> 00:39:38,742
   Billions of stars are gonna
 come careening into our galaxy,

747
00:39:38,744 --> 00:39:43,012
  very, very easily disrupting
     the orbit of the earth.

748
00:39:43,014 --> 00:39:46,049
     The sun could be thrown
   out of the galaxy entirely.

749
00:39:46,051 --> 00:39:49,819
                     ♪

750
00:39:49,821 --> 00:39:53,289
narrator: As stars, dust, and
  gas swirl around each other,

751
00:39:53,291 --> 00:39:55,959
                     ♪

752
00:39:55,961 --> 00:40:00,096
   gravitational interactions
could slingshot our solar system

753
00:40:00,098 --> 00:40:02,799
  out into intergalactic space.

754
00:40:02,801 --> 00:40:08,204
                     ♪

755
00:40:08,206 --> 00:40:10,206
   we'll still orbit the sun,
  and everything will be fine,

756
00:40:10,208 --> 00:40:11,841
   kind of, but it just means

757
00:40:11,843 --> 00:40:14,110
       we'll see something
    very different in our sky

758
00:40:14,112 --> 00:40:19,215
      in 4.6 billion years
         than we do now.

759
00:40:19,217 --> 00:40:20,683
            Narrator:
    Our planet could be sent

760
00:40:20,685 --> 00:40:23,686
         on a whole new
intergalactic ride,

761
00:40:23,688 --> 00:40:25,722
                     ♪

762
00:40:25,724 --> 00:40:32,695
 shot out into the cosmos, away
from the new milkdromeda galaxy.

763
00:40:32,697 --> 00:40:35,098
    There's no way of knowing
 exactly what's going to happen,

764
00:40:35,100 --> 00:40:38,101
       and in that sense,
        journey's end...

765
00:40:38,103 --> 00:40:42,272
                     ♪

766
00:40:42,274 --> 00:40:43,873
we'll just have to wait and see.

767
00:40:43,875 --> 00:40:51,414
                     ♪

768
00:40:51,416 --> 00:40:53,850
   narrator: We might not know
      the final destination

769
00:40:53,852 --> 00:40:57,887
   for earth's cosmic journey,
     but we do know this --

770
00:40:57,889 --> 00:41:02,425
       so far, it has been
       an incredible ride.

771
00:41:02,427 --> 00:41:04,594
We've had a fantastic journey

772
00:41:04,596 --> 00:41:07,897
        over the history
      of earth's existence.

773
00:41:07,899 --> 00:41:11,234
 We may not be immediately aware
         of our motions

774
00:41:11,236 --> 00:41:14,437
 through the universe, but that
 doesn't mean they're not there.

775
00:41:14,439 --> 00:41:16,806
                     ♪

776
00:41:16,808 --> 00:41:18,508
 many people think of the earth

777
00:41:18,510 --> 00:41:23,079
    as this blue, calm marble
            in space.

778
00:41:23,081 --> 00:41:26,216
 But in reality, it's violently
     ripping around the sun,

779
00:41:26,218 --> 00:41:28,952
     and the sun is ripping
        about the galaxy.

780
00:41:28,954 --> 00:41:31,254
                     ♪

781
00:41:31,256 --> 00:41:33,456
    there's a lot of dynamics
happening.

782
00:41:33,458 --> 00:41:35,525
                     ♪

783
00:41:35,527 --> 00:41:37,293
       it boggles the mind
          just to think

784
00:41:37,295 --> 00:41:41,664
        of what the earth
         will have done.

785
00:41:41,666 --> 00:41:44,767
       The earth will have
    actually orbited the sun

786
00:41:44,769 --> 00:41:46,202
        10 billion times.

787
00:41:46,204 --> 00:41:49,606
 It will have spun on its axis,
     like, a trillion times

788
00:41:49,608 --> 00:41:52,408
           in a galaxy
  that's moving through space.

789
00:41:52,410 --> 00:41:55,545
           [ exhales ]

790
00:41:55,547 --> 00:41:58,781
  riding the earth is anything
       but a boring trip.

791
00:41:58,783 --> 00:42:03,520
                     ♪


