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Narrator:
In the universe,

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everything seems
to orbit something.

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Planets orbit stars,
and moons orbit planets.

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Some moons are volcanic,
but the volcanoes are ice.

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Others are awash
with great oceans.

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There may be more
habitable moons in our galaxy

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than there are
habitable planets.

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Narrator: Moons tell the unknown
stories of our solar system

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and show us how it all works.

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In our own solar system,
there are just eight planets.

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But orbiting six
of those planets are moons...

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...lots and lots of moons --
more than 300 of them.

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Each one is different...

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...each one a world all its own.

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Dr. McKay: Well, when we look
out on our solar system,

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we see a lot of planets.

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But even more than planets,
we see moons.

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And in many ways,
they're more interesting

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than the planets
that they go around.

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We have moons that are airless
and apparently dead, like ours.

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Then, out in
the outer solar system,

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we have moons
with oceans inside them

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and moons with atmospheres
around them.

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I'm for moons.
You can keep the planets.

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Narrator:
The biggest eruptions...

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...the coldest temperatures...

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...and the largest oceans
in the solar system --

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they're all on moons.

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There are moons
with ice volcanoes.

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There are moons with lakes of
methane and methane rainfall,

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smog clouds...

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...moons that are
so volcanically active

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that they keep remaking
their surface...

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Moons with all kinds of plumes
shooting off into space --

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really a much wider range
of environments

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than we ever
could have imagined.

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Dr. McKay:
Often, when I'm describing

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to the general public,
or even to my fellow scientists,

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these moons of Saturn
and Jupiter,

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I call them "worlds"
because they really do have

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the complexity and mystery
of a whole world.

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Narrator: Jupiter and Saturn
have over 60 moons each.

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These giant gas planets
and their moons

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are like mini solar systems,

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and each moon
has a distinct personality.

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Iapetus, a two-toned moon
in black and white.

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Titan, with a dense,
orange atmosphere.

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And icy Enceladus, blasting ice
geysers 200 miles into space.

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Each moon is unique.

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But they all have
one thing in common.

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All moons
are natural satellites,

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held in place by gravity.

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But moons do more
than just go around planets.

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They help stabilize the planets
in their orbits

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and keep the machinery
of the solar system

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running smoothly.

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Dr. Grinspoon:
The diversity of moons

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is an interesting combination
of predictable laws of science

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and then complete randomness
of just things smashing together

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and the chips kind of falling
where they did

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in a way that you could
never predict.

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Narrator: Planets and moons
begin the same way.

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Once a star turns on,

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there's a lot of dust and gas
leftover.

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Slowly, the dust particles clump
together, forming rocks.

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The rocks smash into each other
and form boulders.

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Slowly, the objects
get bigger and bigger.

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The process
is called accretion.

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Dr. Durda: One can think of it
as forming a snowball

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and rolling it down a hill.

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As it rolls down the hill,

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it collects and gathers up
yet more snow,

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which makes it roll
faster and harder.

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And so that process
of runaway accretion

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actually happens

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in the formation of the planets

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and in the formation
of moons, as well.

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Narrator:
It sounds simple enough,

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but nobody knew for sure
how it worked until 2003.

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On the International
Space Station,

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astronaut Don Pettit was
experimenting in zero gravity.

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He put grains of salt and sugar
inside a plastic baggie.

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Instead of floating apart,
they began to clump together.

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This is how both planets
and moons build up.

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But instead of taking shape
around stars,

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most big moons take shape
around planets.

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If the same process
makes them all,

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what makes all of them
so different from each other?

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Take two of Jupiter's moons,
Callisto and Ganymede...

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...two very different moons,

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each born from the same debris
when Jupiter was still young.

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Ganymede formed
close to Jupiter,

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where there was lots of debris.

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Because there was
so much material,

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it came together quickly --
in about 10,000 years --

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and it was hot.

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The heat separated the ice
from the rock.

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You can still see it in
Ganymede's distinct landscape.

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Dr. Hendrix:
The primary factor that affects

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why moons are the way
they are today

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is energy "

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how much energy
was put into them

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as heat during accretion

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and how much energy
has been lost.

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All of those factors go
into telling us

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why moons behave the way they do

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and why they look the way
they do today.

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Narrator: Callisto's surface
tells a different story.

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It formed much farther out,

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where there was less debris
and less heat.

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It took longer
and cooled faster.

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Unlike Ganymede,
Callisto's surface is uniform.

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Rock and ice never separated.

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Where a moon forms
can also mean the difference

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between survival
and destruction.

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Get too close,

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and a planet's gravity
will rip a moon to shreds.

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Scientists believe this
is what happened to many moons

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when Jupiter was young.

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Dr. Durda: And it's very likely
that Jupiter had

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an entire conveyor belt
of large moons

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that were wanting to form,

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only to be swallowed up
by the planet itself.

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The large moons we see today

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are only the last ones
that were able to stabilize

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right at the end
of that process,

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stop their death spiral,

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and survive into the position
we see today.

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Narrator: But Jupiter keeps
trying to eat them.

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The gravity of the giant planet

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reaches out and pulls hard
on the orbiting moons.

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It transforms them
from lifeless balls of rock

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into strange and dramatic
worlds.

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Narrator:
Jupiter is the largest planet

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in our solar system.

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It has 63 moons.

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The four largest are called
the Galilean moons,

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named after the astronomer
Galileo,

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who discovered them in 1610.

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They show how gravity controls

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both what moons look like

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and how they behave.

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The first
of the Galilean moons, lo,

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orbits closest to the planet,

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just 260,000 miles
above Jupiter.

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That's about the same distance
as our Moon is from Earth.

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But unlike our Moon,

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the surface of lo
has no impact craters.

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Scientists realized that meant
the surface was new.

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But how could that be?

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Every time you look at lo,

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with a spacecraft
or even with a telescope,

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it's a little bit different.

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So the geology on lo changes

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like the weather
on other planets.

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It's that active.

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Narrator: When NASA first sent
probes to fly past lo,

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they were shocked.

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They saw dozens
of active volcanoes.

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This is footage of an erupting
supervolcano on lo,

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blasting 200 miles into space.

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Everyone had
the same question --

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how could there be
active volcanoes on a moon?

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The answer was simple --
gravity.

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Jupiter's gravity is so huge

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that it reaches out
and crunches the moon.

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And it's not just Jupiter's
gravity pulling on lo.

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Other nearby moons
also pull on it as they pass by.

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So the core of the moon

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is being worked back and forth
all the time.

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It's called tidal friction

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and generates extreme heat
in lo's core.

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Dr. Durda: Almost like bending a
wire coat hanger until it breaks.

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And you feel the inside
of the coat hanger there --

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it feels rather warm.

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That tidal friction --
that internal friction --

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heats the interior of lo
until it's become,

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actually, one of the most
volcanically active worlds

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in the solar system.

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Narrator: The constant
pushing and pulling

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generates temperatures
thousands of degrees high

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inside lo.

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It blasts out
in gigantic eruptions of lava.

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Lo is the prime example

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of tidal forces
and gravitational interactions

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in the solar system.

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It is constantly being pulled
by Jupiter,

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and it's
constantly getting pulled

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by the other moons, as well.

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And so, as a result,

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there's a tremendous amount
of heat created.

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Narrator:
The floods of erupting lava

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constantly resurface lo,

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which is why there are
no visible impact craters

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on this moon.

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Gravity also heats
lo's neighbor, Europa.

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Europa's orbit is farther away
from Jupiter,

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00:13:25,305 --> 00:13:26,568
so it's much colder.

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Instead of lava,
the surface of Europa is ice.

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The lowest recorded temperature
in Antarctica

201
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is minus-128 degrees.

202
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Europa's surface
is twice as cold.

203
00:13:44,257 --> 00:13:47,249
But underneath all the ice,

204
00:13:47,260 --> 00:13:50,025
there may be an ocean of water

205
00:13:50,030 --> 00:13:52,556
heated by
the same tidal friction

206
00:13:52,565 --> 00:13:54,795
that makes lo volcanic.

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00:13:57,671 --> 00:13:59,799
Dr. Hendrix:
Europa has a subsurface ocean,

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00:13:59,806 --> 00:14:02,002
almost certainly.

209
00:14:02,008 --> 00:14:07,174
And that subsurface ocean is in
contact with the rocky mantle,

210
00:14:07,180 --> 00:14:08,944
which provides heat

211
00:14:08,948 --> 00:14:11,645
and also provides,
probably,

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00:14:11,651 --> 00:14:14,382
appropriate nutrients
to sustain life.

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00:14:16,556 --> 00:14:19,025
Narrator:
Someday we'll send a probe

214
00:14:19,025 --> 00:14:21,790
to explore beneath the ice
on Europa.

215
00:14:25,398 --> 00:14:28,561
And maybe we'll discover
life-forms living there

216
00:14:28,568 --> 00:14:32,334
in warm European oceans.

217
00:14:36,910 --> 00:14:41,575
Out beyond lo and Europa
are nearly 60 more moons.

218
00:14:46,886 --> 00:14:49,412
They orbit much further away
from Jupiter,

219
00:14:49,422 --> 00:14:52,221
where the effects
of the giant planet's gravity

220
00:14:52,225 --> 00:14:55,092
are much weaker.

221
00:14:59,399 --> 00:15:01,493
Out here, it's too weak

222
00:15:01,501 --> 00:15:04,869
to generate tidal friction
and heat the moons.

223
00:15:06,806 --> 00:15:10,367
So these remote worlds

224
00:15:10,377 --> 00:15:13,074
are cold and barren...

225
00:15:13,079 --> 00:15:16,140
But not featureless.

226
00:15:16,149 --> 00:15:19,414
They bear the scars
of countless collisions,

227
00:15:19,419 --> 00:15:23,686
and scientists believe
it was collisions that created

228
00:15:23,690 --> 00:15:28,287
the most extraordinary
moon system of them all.

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00:15:36,169 --> 00:15:39,002
Narrator: The planet with
the most unusual moon system

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is Saturn.

231
00:15:42,075 --> 00:15:47,479
It's spread out
over more than 200,000 miles.

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Technically, there are
more than a billion moons.

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00:15:51,818 --> 00:15:54,844
That's right --
a billion moons.

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00:15:54,854 --> 00:15:58,620
And all together,
they make up Saturn's rings.

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00:16:01,628 --> 00:16:06,361
A moon can be a hunk of rock
or ice no bigger than a pebble,

236
00:16:06,366 --> 00:16:08,528
as long as it orbits a planet.

237
00:16:08,535 --> 00:16:10,560
The rings of Saturn are made

238
00:16:10,570 --> 00:16:13,369
of countless pieces
of rock and ice.

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00:16:13,373 --> 00:16:15,865
They go from the size
of a pebble

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00:16:15,875 --> 00:16:17,639
up to the size of a city.

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00:16:17,644 --> 00:16:21,103
We don't refer
to all the ring particles

242
00:16:21,114 --> 00:16:24,379
that can get to be as big
as 10 or 20 meters across.

243
00:16:24,384 --> 00:16:26,944
We don't refer to them
as individual moons.

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00:16:26,953 --> 00:16:28,819
But when we find a body

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00:16:28,822 --> 00:16:32,053
that is maybe a kilometer
or two across,

246
00:16:32,058 --> 00:16:35,460
then you can start talking
about it as a moon or a moonlet.

247
00:16:38,465 --> 00:16:39,955
Narrator: Saturn's rings

248
00:16:39,966 --> 00:16:42,799
are one of the oldest mysteries
of astronomy.

249
00:16:42,802 --> 00:16:45,669
Where did they come from?

250
00:16:45,672 --> 00:16:49,472
To try and find out,

251
00:16:49,476 --> 00:16:51,945
NASA sent the Cassini probe
on a 12-year mission

252
00:16:51,945 --> 00:16:56,781
to study Saturn, its rings,
and its moons.

253
00:17:02,856 --> 00:17:04,950
Dr. Porco:
We took, with Cassini,

254
00:17:04,958 --> 00:17:08,019
probably the most beautiful
picture that's ever been taken,

255
00:17:08,027 --> 00:17:11,156
and I'm not the only one
who has said this.

256
00:17:11,164 --> 00:17:15,067
Cassini was in the shadow
of Saturn, cast by the Sun,

257
00:17:15,068 --> 00:17:17,127
and so you don't see the Sun.

258
00:17:17,136 --> 00:17:21,403
You see the backlit planet of
Saturn and its beautiful rings.

259
00:17:21,407 --> 00:17:24,638
You see the refracted image
of the Sun

260
00:17:24,644 --> 00:17:27,670
poking out from the side
of Saturn.

261
00:17:27,680 --> 00:17:29,944
And nestled
in all of that splendor

262
00:17:29,949 --> 00:17:32,008
is this small little dot.

263
00:17:33,953 --> 00:17:36,979
Narrator:
That tiny dot is not a moon.

264
00:17:36,990 --> 00:17:39,789
That is
the distant planet Earth,

265
00:17:39,792 --> 00:17:42,557
nearly a billion miles away.

266
00:17:45,598 --> 00:17:47,896
Most of what we know
about Saturn,

267
00:17:47,901 --> 00:17:51,303
of its rings and moons,
comes from Cassini.

268
00:17:51,304 --> 00:17:55,070
Before Cassini, we thought
there were only eight rings.

269
00:17:55,074 --> 00:17:58,977
Today we can see over 30.

270
00:17:58,978 --> 00:18:01,276
<i>Dr. Porno".
What we have found at Saturn</i>

271
00:18:01,281 --> 00:18:04,444
has been just literally
an embarrassment of riches.

272
00:18:04,450 --> 00:18:06,714
We're seeing something
that we had seen before,

273
00:18:06,719 --> 00:18:09,416
but now we're seeing it with
a level of detail and clarity

274
00:18:09,422 --> 00:18:10,821
that was just mind-blowing.

275
00:18:19,766 --> 00:18:21,928
Narrator:
Scientists used to think

276
00:18:21,935 --> 00:18:24,427
the rings were made
of the icy leftovers

277
00:18:24,437 --> 00:18:28,032
after Saturn was formed
about 4 billion years ago.

278
00:18:28,041 --> 00:18:29,770
But anything that old

279
00:18:29,776 --> 00:18:34,304
should be covered
with cosmic dust, and dirty.

280
00:18:36,149 --> 00:18:38,641
So why does Saturn's rings

281
00:18:38,651 --> 00:18:42,645
appear bright and clean,
almost new?

282
00:18:46,859 --> 00:18:48,418
To get the answer,

283
00:18:48,428 --> 00:18:52,456
Mission Control maneuvered
Cassini close to the rings.

284
00:18:54,834 --> 00:18:58,395
The probe saw that
all the ice pieces in the rings

285
00:18:58,404 --> 00:19:01,806
are constantly colliding
and breaking up.

286
00:19:06,479 --> 00:19:09,938
And each collision
exposes new surfaces

287
00:19:09,949 --> 00:19:12,418
that are clean and polished.

288
00:19:21,327 --> 00:19:24,957
This is what astronomers
think happened.

289
00:19:24,964 --> 00:19:26,830
When Saturn was young,

290
00:19:26,833 --> 00:19:30,770
it had no rings,
just lots of moons.

291
00:19:30,770 --> 00:19:33,398
At some point, an icy comet

292
00:19:33,406 --> 00:19:35,500
zoomed in from deep space

293
00:19:35,508 --> 00:19:38,136
and smashed
into one of those moons.

294
00:19:38,144 --> 00:19:42,047
The comet broke up
into billions of pieces.

295
00:19:45,685 --> 00:19:49,849
The impact also pushed
the moon closer to Saturn,

296
00:19:49,856 --> 00:19:53,315
where the planet's
enormous gravity broke it up.

297
00:20:00,566 --> 00:20:05,436
Now debris from the moon
and ice from the comet mixed.

298
00:20:07,674 --> 00:20:09,938
Gradually, Saturn's gravity

299
00:20:09,942 --> 00:20:14,470
pulled all those fragments
into rings around it.

300
00:20:17,283 --> 00:20:21,254
The story of moons
is the story of gravity.

301
00:20:21,254 --> 00:20:23,951
Gravity holds them in orbit.

302
00:20:23,956 --> 00:20:28,917
It heats up their insides
and shapes their surfaces.

303
00:20:28,928 --> 00:20:33,388
In the end, it controls
everything about moons,

304
00:20:33,399 --> 00:20:36,130
even their survival
and destruction.

305
00:20:38,971 --> 00:20:41,804
Gravity can even create
new moons

306
00:20:41,808 --> 00:20:48,305
by kidnapping asteroids,
comets, and even whole planets.

307
00:20:55,288 --> 00:20:57,882
Narrator: We know
that gravity makes moons.

308
00:21:00,693 --> 00:21:03,492
The standard way
is to assemble them

309
00:21:03,496 --> 00:21:06,761
from debris leftover
when planets are formed.

310
00:21:09,402 --> 00:21:12,702
But gravity makes moons
a second way, too.

311
00:21:12,705 --> 00:21:14,571
It captures them.

312
00:21:17,944 --> 00:21:21,278
Imagine a wandering comet
or asteroid.

313
00:21:21,280 --> 00:21:24,272
Somehow it gets knocked
off course.

314
00:21:24,283 --> 00:21:28,117
It wanders too close
to a planet.

315
00:21:28,121 --> 00:21:32,957
Gravity acts like
a science-fiction tractor beam

316
00:21:32,959 --> 00:21:34,222
and grabs it.

317
00:21:34,227 --> 00:21:37,356
Not quite enough gravity,
and it escapes.

318
00:21:38,965 --> 00:21:43,368
Too much gravity, and it
collides with the planet.

319
00:21:43,369 --> 00:21:47,135
Just enough,
and the comet or asteroid

320
00:21:47,140 --> 00:21:49,768
goes into orbit
around the planet

321
00:21:49,776 --> 00:21:52,006
and becomes a new moon.

322
00:21:57,483 --> 00:22:02,182
Mars has two tiny moons,
named Phobos and Deimos.

323
00:22:02,188 --> 00:22:05,920
Both are captured asteroids.

324
00:22:05,925 --> 00:22:09,486
One is pushing outward
as it circles the planet

325
00:22:09,495 --> 00:22:11,486
and will eventually break free

326
00:22:11,497 --> 00:22:14,558
and continue on its journey
through space.

327
00:22:14,567 --> 00:22:17,195
The other is circling inwards,

328
00:22:17,203 --> 00:22:20,229
a little closer to Mars
all the time.

329
00:22:20,239 --> 00:22:23,402
Eventually,
it'll smash into it.

330
00:22:31,050 --> 00:22:33,314
This is Cruithne.

331
00:22:33,319 --> 00:22:36,516
It's an asteroid, really,
just three miles across.

332
00:22:36,522 --> 00:22:41,392
But it's sometimes described
as Earth's second moon.

333
00:22:41,394 --> 00:22:44,022
Dr. Durda:
With the little object Cruithne,

334
00:22:44,030 --> 00:22:46,328
which was discovered
back in 1986,

335
00:22:46,332 --> 00:22:49,063
we start to get
into this realm of --

336
00:22:49,068 --> 00:22:51,765
of what does it mean
to be a moon.

337
00:22:51,771 --> 00:22:55,071
Narrator:
Only a few thousand years ago,

338
00:22:55,074 --> 00:22:57,600
Cruithne was
an ordinary asteroid,

339
00:22:57,610 --> 00:23:00,477
orbiting the Sun
like billions of others.

340
00:23:00,479 --> 00:23:02,379
But eventually, it wobbled

341
00:23:02,381 --> 00:23:04,748
out of its orbit
in the Asteroid Belt

342
00:23:04,750 --> 00:23:07,151
and got snagged
by Earth's gravity.

343
00:23:09,589 --> 00:23:13,457
But then Cruithne
did something unusual.

344
00:23:13,459 --> 00:23:16,053
Instead of orbiting
around the Earth,

345
00:23:16,062 --> 00:23:17,621
like a normal moon,

346
00:23:17,630 --> 00:23:20,759
Cruithne began to follow
behind it.

347
00:23:20,766 --> 00:23:24,930
And so one might call it
a sort of a moon of the Earth --

348
00:23:24,937 --> 00:23:27,269
not exactly, though,
because that object is on --

349
00:23:27,273 --> 00:23:29,401
you know, it's
on its own independent orbit

350
00:23:29,408 --> 00:23:30,910
around the Sun,
not the Earth.

351
00:23:35,047 --> 00:23:39,245
Narrator: Sometimes asteroids
capture their own moons.

352
00:23:39,252 --> 00:23:42,415
In 1993, the Galileo spacecraft

353
00:23:42,421 --> 00:23:44,890
flew past the asteroid Ida

354
00:23:44,891 --> 00:23:48,054
and found something
nobody expected --

355
00:23:48,060 --> 00:23:51,553
a tiny half-mile-wide moon.

356
00:23:53,232 --> 00:23:55,599
Dr. Durda:
The fact that we saw a satellite

357
00:23:55,601 --> 00:23:57,126
around only
the second asteroid

358
00:23:57,136 --> 00:23:59,036
ever to be encountered
with a spacecraft

359
00:23:59,038 --> 00:24:00,335
immediately tells us

360
00:24:00,339 --> 00:24:03,570
that moons around asteroids
must be incredibly common.

361
00:24:07,680 --> 00:24:10,342
Narrator: Not all
captured moons are small.

362
00:24:10,349 --> 00:24:13,979
The mother of all
captured moons is Triton.

363
00:24:13,986 --> 00:24:19,152
It orbits the planet Neptune,
and it is big --

364
00:24:19,158 --> 00:24:22,093
about 1,700 miles in diameter.

365
00:24:22,094 --> 00:24:26,361
But Triton is a moon
with an unusual story.

366
00:24:27,767 --> 00:24:30,168
Triton was
a very puzzling problem

367
00:24:30,169 --> 00:24:31,864
for planetary scientists,

368
00:24:31,871 --> 00:24:33,703
because our traditional view

369
00:24:33,706 --> 00:24:35,697
would tend to make
all the moons orbit

370
00:24:35,708 --> 00:24:38,268
in the same direction
that the planet itself spins.

371
00:24:38,277 --> 00:24:40,439
In the case of Triton
around Neptune,

372
00:24:40,446 --> 00:24:41,914
it's the other way around.

373
00:24:41,914 --> 00:24:43,507
Neptune is spinning this way.

374
00:24:43,516 --> 00:24:46,383
Triton is orbiting around
in the opposite direction.

375
00:24:46,385 --> 00:24:50,720
Narrator: This means
it didn't form like most moons,

376
00:24:50,723 --> 00:24:53,852
out of the debris leftover
from the birth of the planet,

377
00:24:53,859 --> 00:24:57,352
or it would orbit
in the same direction.

378
00:24:57,363 --> 00:24:59,889
So something wasn't right.

379
00:24:59,899 --> 00:25:04,200
Dr. Grinspoon: Triton is huge,
and its orbit is funny.

380
00:25:04,203 --> 00:25:05,193
It's anomalous.

381
00:25:05,204 --> 00:25:07,104
It does not seem
as though it formed

382
00:25:07,106 --> 00:25:10,508
as a part of the Neptune system.

383
00:25:10,509 --> 00:25:15,174
It seems much more
like a captured planet.

384
00:25:15,181 --> 00:25:18,640
Narrator:
Scientists now think Triton

385
00:25:18,651 --> 00:25:21,245
was once a dwarf planet,
like Pluto.

386
00:25:21,253 --> 00:25:24,985
And a giant planet like Neptune
certainly has enough gravity

387
00:25:24,991 --> 00:25:28,791
to capture a moon
the size of Triton.

388
00:25:28,794 --> 00:25:31,354
Dr. Hendrix: Triton
was almost certainly formed

389
00:25:31,364 --> 00:25:33,264
way out
in the outer solar system

390
00:25:33,265 --> 00:25:35,825
and then at some point
was captured by Neptune.

391
00:25:35,835 --> 00:25:38,099
Perhaps Triton, early on,
had its own moon,

392
00:25:38,104 --> 00:25:39,503
they both were captured,

393
00:25:39,505 --> 00:25:42,805
and then that moon was destroyed
during the capture process.

394
00:25:44,877 --> 00:25:47,574
Narrator:
But Triton is in danger.

395
00:25:47,580 --> 00:25:51,483
Neptune is dragging it
closer and closer.

396
00:25:53,552 --> 00:25:57,580
Eventually,
it will get too close,

397
00:25:57,590 --> 00:26:02,027
and Neptune's immense gravity
will tear it apart.

398
00:26:13,839 --> 00:26:17,298
Triton the moon will be reborn

399
00:26:17,309 --> 00:26:20,540
as a ring system
around the planet.

400
00:26:32,792 --> 00:26:35,056
But what about our Moon?

401
00:26:35,061 --> 00:26:36,893
How did it get there?

402
00:26:36,896 --> 00:26:39,263
Was it captured?

403
00:26:42,568 --> 00:26:46,368
The truth
is even more extraordinary.

404
00:26:46,372 --> 00:26:50,605
It was born in extreme violence.

405
00:26:56,082 --> 00:26:58,210
Narrator:
Our Moon, like a lot of moons,

406
00:26:58,217 --> 00:27:03,747
is rocky, barren,
and pockmarked with craters.

407
00:27:03,756 --> 00:27:09,058
But in one way, our Moon
is unique in the solar system.

408
00:27:13,165 --> 00:27:14,564
For a long time,

409
00:27:14,567 --> 00:27:16,729
astronomers thought
the Moon formed

410
00:27:16,735 --> 00:27:20,103
from debris leftover
from the birth of the Earth.

411
00:27:20,106 --> 00:27:21,972
But researchers in the 1960s

412
00:27:21,974 --> 00:27:25,171
came up with
a radically different idea.

413
00:27:25,177 --> 00:27:29,614
They suggested
it came from a giant impact.

414
00:27:43,762 --> 00:27:45,958
Dr. Hartmann:
When we first had the idea

415
00:27:45,965 --> 00:27:49,230
of forming the Moon
from a giant impact,

416
00:27:49,235 --> 00:27:52,569
that was not
a terribly popular idea.

417
00:27:52,571 --> 00:27:55,700
And I actually did have good
science friends -- colleagues --

418
00:27:55,708 --> 00:27:58,973
coming to me, saying, you know,
we really have to exhaust

419
00:27:58,978 --> 00:28:01,606
all the slow
evolutionary theories

420
00:28:01,614 --> 00:28:04,640
before we start talking
about cataclysms.

421
00:28:04,650 --> 00:28:07,950
Narrator: The evidence
Bill Hartmann needed

422
00:28:07,953 --> 00:28:09,682
was on the Moon itself.

423
00:28:12,858 --> 00:28:14,451
And the proof had to wait

424
00:28:14,460 --> 00:28:19,626
until Apollo astronauts
finally went there in 1969.

425
00:28:21,901 --> 00:28:25,428
They brought back hundreds
of pounds of Moon rocks.

426
00:28:27,239 --> 00:28:31,176
Scientists analyzed the rocks
and were amazed.

427
00:28:31,177 --> 00:28:34,841
They were identical to rocks
in the Earth's crust,

428
00:28:34,847 --> 00:28:38,909
and they'd been superheated.

429
00:28:38,918 --> 00:28:43,048
So, how did
pieces of the Earth's crust

430
00:28:43,055 --> 00:28:45,524
become superhot
and wind up on the Moon?

431
00:28:45,524 --> 00:28:48,619
Hartmann was pretty sure
he knew.

432
00:28:48,627 --> 00:28:51,494
Dr. Hartmann: This whole idea
was that the Earth forms.

433
00:28:51,497 --> 00:28:53,158
Now you hit it with something.

434
00:28:53,165 --> 00:28:56,066
You blow all this light,
rocky material off the top.

435
00:28:56,068 --> 00:28:58,799
That material goes into orbit
and makes the Moon.

436
00:28:58,804 --> 00:29:01,739
The Moon's just made
out of rocky debris.

437
00:29:05,411 --> 00:29:08,836
Narrator: Imagine our
chaotic solar system

438
00:29:08,847 --> 00:29:10,679
4.5 billion years ago.

439
00:29:17,089 --> 00:29:19,387
The young Earth is just one

440
00:29:19,391 --> 00:29:22,986
of a hundred or so new planets
orbiting the Sun.

441
00:29:28,200 --> 00:29:32,694
One of them is a Mars-sized
planet called Theia,

442
00:29:32,705 --> 00:29:35,697
and it's on a collision course
with Earth.

443
00:29:40,613 --> 00:29:42,547
They smash into each other

444
00:29:42,548 --> 00:29:45,483
at many thousands of miles
an hour.

445
00:29:57,763 --> 00:30:02,030
Theia is destroyed,
and Earth barely survives.

446
00:30:02,034 --> 00:30:06,699
The impact blasts billions
of tons of debris into space.

447
00:30:06,705 --> 00:30:11,541
The Earth's gravity pulls it
into orbit around the planet.

448
00:30:11,543 --> 00:30:14,706
Now these hunks
of leftover Earth

449
00:30:14,713 --> 00:30:18,013
clump together
and form our Moon.

450
00:30:33,432 --> 00:30:38,097
That's the theory, anyway.
But how do you test it for real?

451
00:30:40,372 --> 00:30:42,466
Here at NASA's
Vertical Gun Range,

452
00:30:42,474 --> 00:30:46,911
they're re-creating
that ancient collision in a lab.

453
00:30:49,048 --> 00:30:52,074
This 30-foot-long gun
fires a tiny projectile

454
00:30:52,084 --> 00:30:54,212
at 18,000 miles an hour.

455
00:30:57,723 --> 00:31:00,124
The projectile is Theia.

456
00:31:00,125 --> 00:31:02,719
This ball represents the Earth.

457
00:31:02,728 --> 00:31:05,925
By changing
the angle of Theia's impact,

458
00:31:05,931 --> 00:31:08,263
the team can figure out
how precise

459
00:31:08,267 --> 00:31:11,897
the ancient collision had to be
in order to make the Moon.

460
00:31:11,904 --> 00:31:13,895
In the first shot,

461
00:31:13,906 --> 00:31:18,468
Theia hits the top of the Earth
with a glancing blow.

462
00:31:18,477 --> 00:31:21,378
So, here's the Earth,
if you will, suspended in space.

463
00:31:21,380 --> 00:31:22,643
And now it's gotten hit.

464
00:31:24,350 --> 00:31:27,718
So, now we see
the planet ejecta

465
00:31:27,720 --> 00:31:30,417
is being ripped
out of the Earth

466
00:31:30,422 --> 00:31:33,084
and is forming
this giant impact basin.

467
00:31:33,092 --> 00:31:34,958
And if this
really were the Earth,

468
00:31:34,960 --> 00:31:37,986
this basin would be
thousands of kilometers --

469
00:31:37,996 --> 00:31:40,328
thousands of miles -- across.

470
00:31:40,332 --> 00:31:42,960
Narrator:
In this simulation,

471
00:31:42,968 --> 00:31:46,233
Theia only skims
off the surface of the planet,

472
00:31:46,238 --> 00:31:50,436
and very little debris
is thrown out into space --

473
00:31:50,442 --> 00:31:53,070
not nearly enough
to build our Moon.

474
00:31:53,078 --> 00:31:55,274
[indistinct conversation]

475
00:31:55,280 --> 00:31:57,647
[ Buzzer]

476
00:31:57,649 --> 00:31:59,151
[Crash]

477
00:31:59,151 --> 00:32:02,416
The second shot
is a head-on collision.

478
00:32:05,858 --> 00:32:07,257
Dr. Schultz: Ka-pow!

479
00:32:07,259 --> 00:32:11,787
That's the end of planet Earth.
It's gone.

480
00:32:11,797 --> 00:32:14,596
Some of the debris is gonna go
out of the solar system.

481
00:32:14,600 --> 00:32:16,432
Some of the debris
will reaccrete

482
00:32:16,435 --> 00:32:19,029
to form small planetesimals
within the solar system.

483
00:32:27,279 --> 00:32:29,077
Narrator:
There's no Earth left,

484
00:32:29,081 --> 00:32:30,515
so there's no gravity

485
00:32:30,516 --> 00:32:33,076
to gather the debris
and form the Moon.

486
00:32:35,154 --> 00:32:39,284
Now the gun is set
to just the right angle --

487
00:32:39,291 --> 00:32:43,524
halfway between a glancing blow
and a direct hit.

488
00:32:43,529 --> 00:32:47,830
So we'll see what happens
if the Earth barely survives.

489
00:32:54,673 --> 00:32:58,940
Oh, oh, gorgeous!
Oh, my gosh!

490
00:32:58,944 --> 00:33:00,002
<i>Kill-pow'!</i>

491
00:33:00,012 --> 00:33:02,640
Now we have the entire part
of the Earth

492
00:33:02,648 --> 00:33:04,138
being ripped apart,

493
00:33:04,149 --> 00:33:07,278
but the vapor plume is --
oh, my gosh.

494
00:33:07,286 --> 00:33:09,880
AW! QGGZ!

495
00:33:09,888 --> 00:33:11,822
That is gorgeous.

496
00:33:18,063 --> 00:33:23,661
But this was the beginning --
the beginning of our Moon.

497
00:33:25,471 --> 00:33:27,269
Narrator:
The experiment shows

498
00:33:27,272 --> 00:33:30,071
that Theia could have
smashed into the Earth

499
00:33:30,075 --> 00:33:32,976
and formed the Moon.

500
00:33:32,978 --> 00:33:36,539
But the collision
had to be just right.

501
00:33:36,548 --> 00:33:39,245
And lucky for us, it was.

502
00:33:45,257 --> 00:33:49,888
Today, the Moon orbits
250,000 miles from Earth.

503
00:33:51,430 --> 00:33:53,421
But when it first formed,

504
00:33:53,432 --> 00:33:56,424
the Moon orbited
just 15,000 miles

505
00:33:56,435 --> 00:33:58,369
above the Earth's surface.

506
00:34:01,039 --> 00:34:04,236
Dr. Schultz: 500 million years
after the Moon formed,

507
00:34:04,243 --> 00:34:05,677
if we looked up in the sky,

508
00:34:05,677 --> 00:34:08,703
the Moon would have comprised
a tremendous portion of the sky.

509
00:34:08,714 --> 00:34:10,182
It would have been enormous,

510
00:34:10,182 --> 00:34:12,446
because the Moon
would have been much closer.

511
00:34:14,319 --> 00:34:18,290
Narrator: Back then,
the Earth was rotating so fast,

512
00:34:18,290 --> 00:34:20,190
a day lasted just six hours.

513
00:34:23,028 --> 00:34:28,296
But the Moon was so close,
its gravity acted like a brake.

514
00:34:31,937 --> 00:34:34,406
It slowed our planet down

515
00:34:34,406 --> 00:34:38,434
until a day now lasts 24 hours.

516
00:34:40,345 --> 00:34:44,009
The Moon's gravity
also created giant tides

517
00:34:44,016 --> 00:34:46,007
that surged across the planet,

518
00:34:46,018 --> 00:34:50,148
churning up the seas,
mixing minerals and nutrients.

519
00:34:50,155 --> 00:34:52,852
This created
the primordial soup

520
00:34:52,858 --> 00:34:56,021
from which the first forms
of life arose.

521
00:34:56,028 --> 00:34:59,794
Without our Moon, life on Earth
may never have happened.

522
00:35:02,868 --> 00:35:07,863
And there may be other moons
with a link to life, as well.

523
00:35:07,873 --> 00:35:12,640
Moons may be the great biology
experiments of the universe --

524
00:35:12,644 --> 00:35:17,377
the true laboratories
of life itself.

525
00:35:23,655 --> 00:35:26,989
Narrator:
Moons are full of surprises.

526
00:35:26,992 --> 00:35:30,826
There are moons
with giant volcanoes,

527
00:35:30,829 --> 00:35:35,596
moons with vast oceans
sealed under thick ice.

528
00:35:38,437 --> 00:35:43,637
And now we know a few
are rich in organic compounds.

529
00:35:43,642 --> 00:35:47,613
In the right combination,
they might even support life.

530
00:35:47,613 --> 00:35:50,275
Dr. McKay: In our solar system,
the biological window

531
00:35:50,282 --> 00:35:53,047
through which we can understand
the rest of the universe

532
00:35:53,051 --> 00:35:55,918
may be through these moons
of the outer solar system.

533
00:35:55,921 --> 00:35:58,856
That may be where we find
our second genesis,

534
00:35:58,857 --> 00:36:00,325
and that second genesis

535
00:36:00,325 --> 00:36:03,056
is really
our first deep understanding

536
00:36:03,061 --> 00:36:05,428
of the biological nature
of the universe.

537
00:36:14,039 --> 00:36:18,272
Narrator: At first glance,
moons don't look ideal for life.

538
00:36:21,813 --> 00:36:24,976
Take Enceladus.

539
00:36:24,983 --> 00:36:29,250
It's a shiny ball of ice,
300 miles across,

540
00:36:29,254 --> 00:36:32,519
orbiting Saturn.

541
00:36:32,524 --> 00:36:34,822
It's the brightest object
in the solar system.

542
00:36:34,826 --> 00:36:37,488
It reflects 100% of the light
that hits it,

543
00:36:37,496 --> 00:36:38,793
so it's superbright,

544
00:36:38,797 --> 00:36:40,993
and that's because
it's water ice.

545
00:36:40,999 --> 00:36:43,491
Narrator:
In 2005, the Cassini probe

546
00:36:43,502 --> 00:36:48,440
spotted ice volcanoes erupting
from the surface of Enceladus.

547
00:36:48,440 --> 00:36:52,001
That meant there had to be
heat under all that ice --

548
00:36:52,010 --> 00:36:55,105
heat that created
oceans of water.

549
00:36:55,113 --> 00:36:59,710
And where there's water,
there's the possibility of life.

550
00:36:59,718 --> 00:37:03,848
So, this is Beehive Geyser
here in Yellowstone,

551
00:37:03,855 --> 00:37:06,449
and it is shooting water vapor
and water

552
00:37:06,458 --> 00:37:09,052
about 150 feet into the sky.

553
00:37:09,061 --> 00:37:11,496
And it's pretty incredible.

554
00:37:11,496 --> 00:37:14,158
So, now imagine if you're
on the surface of Enceladus.

555
00:37:14,166 --> 00:37:16,567
You would see geysers
that look a lot like this,

556
00:37:16,568 --> 00:37:21,233
and they are shooting ice grains
and water vapor into space

557
00:37:21,239 --> 00:37:23,867
thousands of times higher
than this geyser here.

558
00:37:23,875 --> 00:37:29,143
Narrator: The ice volcanoes
are powered by gravity.

559
00:37:29,147 --> 00:37:30,546
Here's how.

560
00:37:30,549 --> 00:37:33,610
Saturn's gravity works
on the core of the moon,

561
00:37:33,618 --> 00:37:34,983
heating it up.

562
00:37:34,986 --> 00:37:37,045
The underground water expands

563
00:37:37,055 --> 00:37:40,958
and forces its way up through
cracks in the surface ice

564
00:37:40,959 --> 00:37:45,260
and blasts out into space
as ice crystals.

565
00:37:45,263 --> 00:37:49,029
These are some of
the most spectacular eruptions

566
00:37:49,034 --> 00:37:50,593
in our solar system.

567
00:37:50,602 --> 00:37:54,470
They make Beehive Geyser
look like a squirt gun.

568
00:37:54,473 --> 00:37:56,965
From the ice in the volcanoes,

569
00:37:56,975 --> 00:38:01,674
scientists have detected salt
and simple organic compounds.

570
00:38:01,680 --> 00:38:04,843
That means
the water under the ice

571
00:38:04,850 --> 00:38:08,047
is not only warm
but full of nutrients.

572
00:38:08,053 --> 00:38:10,283
Sound familiar?

573
00:38:10,288 --> 00:38:13,053
Heat, water, and nutrients --

574
00:38:13,058 --> 00:38:15,493
that's how life on Earth began.

575
00:38:15,494 --> 00:38:18,293
Dr. Porco: We realize
you could have all the things

576
00:38:18,296 --> 00:38:20,663
that we associate
with oceans on the Earth

577
00:38:20,665 --> 00:38:21,962
going on inside a moon.

578
00:38:21,967 --> 00:38:24,095
It's the discovery
of a lifetime.

579
00:38:24,102 --> 00:38:27,766
Narrator: Saturn's
Enceladus has an ocean.

580
00:38:27,773 --> 00:38:29,935
So does Jupiter's Europa.

581
00:38:29,941 --> 00:38:34,742
But these aren't the only moons
where life could emerge.

582
00:38:34,746 --> 00:38:38,114
Saturn has another moon <i>--</i>
Titan --

583
00:38:38,116 --> 00:38:41,211
with an even greater potential
for life.

584
00:38:43,188 --> 00:38:48,092
In 2005, Cassini sent a probe,
called Huygens,

585
00:38:48,093 --> 00:38:50,050
on a one-way mission to Titan.

586
00:38:51,997 --> 00:38:54,796
For just 3 1/2 hours,

587
00:38:54,800 --> 00:38:57,098
Huygens transmitted
live pictures

588
00:38:57,102 --> 00:39:02,541
from the hostile surface,
nearly a billion miles away.

589
00:39:02,541 --> 00:39:05,875
Then the battery died.

590
00:39:05,877 --> 00:39:08,369
Dr. Porco:
It was just incredible.

591
00:39:08,380 --> 00:39:12,112
This was the first time humans
had ever touched this moon

592
00:39:12,117 --> 00:39:13,881
with something
of our own making.

593
00:39:13,885 --> 00:39:15,080
It was just an event

594
00:39:15,086 --> 00:39:17,350
that should have been
celebrated the world over.

595
00:39:17,355 --> 00:39:19,483
We should have had
ticker-tape parades

596
00:39:19,491 --> 00:39:21,585
in every major city
across the U.S. and Europe

597
00:39:21,593 --> 00:39:22,856
to celebrate this.

598
00:39:22,861 --> 00:39:26,456
It was that history-making
and that astonishing.

599
00:39:33,572 --> 00:39:36,041
Narrator:
Raindrops on Titan

600
00:39:36,041 --> 00:39:38,601
are twice as big
as raindrops on Earth.

601
00:39:40,645 --> 00:39:43,546
But the rain isn't water.

602
00:39:43,548 --> 00:39:46,347
It's methane.

603
00:39:46,351 --> 00:39:48,285
[thunder crashes]

604
00:39:50,488 --> 00:39:53,480
On Earth, methane is a gas,

605
00:39:53,491 --> 00:39:57,962
but on Titan, it's a liquid
because the moon is so cold.

606
00:40:01,600 --> 00:40:03,932
Dr. McKay:
There may be methane icebergs.

607
00:40:03,935 --> 00:40:06,427
There are certainly
methane lakes and rivers,

608
00:40:06,438 --> 00:40:08,839
and there's methane rain
and methane clouds

609
00:40:08,840 --> 00:40:10,865
and maybe bugs
swimming in methane.

610
00:40:10,876 --> 00:40:14,574
Narrator:
Bugs living in liquid methane

611
00:40:14,579 --> 00:40:16,775
may sound unbelievable.

612
00:40:16,781 --> 00:40:19,273
But scientists have discovered

613
00:40:19,284 --> 00:40:22,777
that Enceladus, Europa,
and Titan

614
00:40:22,787 --> 00:40:26,451
are all covered
with a substance called tholin.

615
00:40:26,458 --> 00:40:29,257
Tholin contains
the chemical building blocks

616
00:40:29,261 --> 00:40:31,423
for life to begin.

617
00:40:31,429 --> 00:40:36,230
So could life emerge
on any or all of these moons?

618
00:40:40,639 --> 00:40:43,404
We can't get our hands
on the tholin from the moons,

619
00:40:43,408 --> 00:40:46,434
so Chris McKay
makes it in the lab.

620
00:40:46,444 --> 00:40:51,143
He zaps a mixture of gases
found on Titan with electricity.

621
00:40:51,149 --> 00:40:56,485
What he gets
is a reddish-brown mud.

622
00:40:56,488 --> 00:40:58,445
So, this is
what we make -- tholin,

623
00:40:58,456 --> 00:41:02,017
this sort of nonbiological
organic material.

624
00:41:02,027 --> 00:41:04,121
It's produced by chemical energy

625
00:41:04,129 --> 00:41:06,757
put into simple molecules,
like methane and nitrogen,

626
00:41:06,765 --> 00:41:08,255
and here we got it.

627
00:41:08,266 --> 00:41:11,167
And that's the material
we see on Titan.

628
00:41:11,169 --> 00:41:14,730
We see evidence for something
like this on Enceladus.

629
00:41:14,739 --> 00:41:16,104
We see it on the surface

630
00:41:16,107 --> 00:41:18,701
of many of the moons
in the outer solar system.

631
00:41:18,710 --> 00:41:21,077
This is nature's recipe

632
00:41:21,079 --> 00:41:25,016
for making the stuff that life
eventually emerges from.

633
00:41:25,016 --> 00:41:29,510
Narrator: Somewhere in the outer
reaches of our solar system,

634
00:41:29,521 --> 00:41:32,013
OH some remote moon,

635
00:41:32,023 --> 00:41:35,857
life may have already emerged.

636
00:41:35,860 --> 00:41:39,922
But it probably won't be life
as we know it.

637
00:41:39,931 --> 00:41:42,127
Life 2.0 doesn't
necessarily have to have

638
00:41:42,133 --> 00:41:44,192
the same genetics
as life 1.0, right?

639
00:41:44,202 --> 00:41:47,263
In fact, the more different it
is, the more interesting it is.

640
00:41:49,808 --> 00:41:52,869
Narrator: Whether it's the same
or very different,

641
00:41:52,877 --> 00:41:56,472
the discovery of life
on the moons of our solar system

642
00:41:56,481 --> 00:41:59,678
will change the way
we look at the universe.

643
00:42:02,921 --> 00:42:06,118
Dr. Porco: I think that,
should we ever find

644
00:42:06,124 --> 00:42:07,455
that life had originated

645
00:42:07,459 --> 00:42:11,327
not once but twice
in our solar system,

646
00:42:11,329 --> 00:42:15,300
then you -- you can
easily dismiss any arguments

647
00:42:15,300 --> 00:42:19,533
that say that life
is unique to the Earth.

648
00:42:21,673 --> 00:42:23,573
Narrator:
Moons are small,

649
00:42:23,575 --> 00:42:27,273
but they're still
diverse and dynamic worlds.

650
00:42:27,278 --> 00:42:31,272
They help us understand
how the universe works.

651
00:42:31,282 --> 00:42:35,014
They're essential cogs
in the cosmic machine.

652
00:42:35,020 --> 00:42:37,250
Without any moons,

653
00:42:37,255 --> 00:42:40,919
our solar system would be
a very different place.

654
00:42:40,925 --> 00:42:45,590
Without our Moon, life may
never have evolved on Earth.

655
00:42:45,597 --> 00:42:47,065
And who knows --

656
00:42:47,065 --> 00:42:51,468
when and if we find new life
somewhere else in the universe,

657
00:42:51,469 --> 00:42:55,269
its home may not be
another planet at all.

658
00:42:55,273 --> 00:42:58,538
It might be...a moon.


