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Male narrator: In the beginning,
there was darkness,
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and then, bang,
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giving birth to an endless
expanding existence
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of time, space, and matter.
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Every day, new discoveries
are unlocking the mysterious,
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00:00:13,346 --> 00:00:15,848
the mind-blowing,
the deadly secrets
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of a place we call
The Universe.
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Chart a daring course
with comets,
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the cosmic time travelers
of the skies.
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- These mysterious objects
have been agents of change.
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00:00:30,905 --> 00:00:33,574
They've been agents
of destruction.
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00:00:33,574 --> 00:00:36,410
Narrator: Discover why
these celestial bodies
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carry secrets from our past
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and cast doom
over our future.
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- If it's getting into
our on-ramp,
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we need to worry about it.
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- There's very little
we can do
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other than sending
a giant bomb toward them
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and trying to deflect them.
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Narrator. Brace yourself
as we rendezvous
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with the frozen intruders
from the great beyond
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on an epic journey
to "Ride the Comet."
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They appear out of nowhere,
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gliding slowly
across the nighttime sky
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and then disappearing
from sight.
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Throughout human history,
ancient cultures
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believed these
celestial intruders
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carried special powers
from the gods,
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mystical messengers
of life and death.
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- Scientists like to think
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that comets are fairly
mysterious objects,
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because we know
that they're very old.
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They're like frozen
time capsules
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from when our solar system
was first formed.
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- Comets are a bit
of show-offs.
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They come into the night sky
unannounced, unpredicted.
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In the Middle Ages, they were
thought to be fireballs
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thrown at a sinful Earth
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from the right hand
of an avenging god.
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And so they've always been
feared or seen as mysterious.
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00:02:11,547 --> 00:02:13,048
Narrator: We're going
to hitch a ride
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on a bold, uncharted journey
through the secret life
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of our solar system's
comets.
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Our daring quest begins
4.5 billion years ago,
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as our futuristic spacecraft
time-travels
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back to the birth
of our solar system.
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We zigzag through
a maelstrom of debris
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to catch our first glimpse
of comets,
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00:02:42,536 --> 00:02:47,036
the wayward rocks that
didn't meld into planets.
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- Comets are basically
dirty snowballs
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or icy dirtballs.
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They consist of rocks
and dust and dirt
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held together by ices—
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Water ice, ammonia, methane,
carbon dioxide, dry ice.
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00:03:01,639 --> 00:03:02,806
That's sort of like the glue
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that holds
all these little pebbles
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and particles of dust
together.
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00:03:08,646 --> 00:03:12,316
Narrator: The heart of these
cosmic icebergs is the nucleus,
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or central core,
which averages in size
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from a half mile wide
to as big as a modern city.
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- One of the things
we've learned
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by flying close by and observing
the nuclei of comets
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is that they're these strange
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sort of compacted conglomerates
of ice and rock.
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They're not uniform.
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They're not perfectly mixed.
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They're quite chunky
and oddly shaped.
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- The nuclei of comets are...
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very fragile entities.
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If you had a chunk,
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you could probably break it
easily in your hands.
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Narrator: Up close,
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comets look like bland chunks
of charcoal
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rather than supersized
snowballs.
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They don't even remotely
resemble
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the glowing orbs we see
in our pitch-black skies.
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- We think that most comets
are extremely dark
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on their surfaces,
that the surfaces are covered
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with something
kind of like barbecue soot,
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this really dark,
black material
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that makes them very difficult
to see.
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Narrator:
While their asteroid cousins
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share similar properties,
such as rock and metal,
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scientists suspect that comets
were born farther out,
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near the gas giant planets,
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where it's much colder,
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so they possess more ices
and volatile elements.
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About 3.8 billion years ago,
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many of these icy bodies
were whisked away
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to the Kuiper belt,
a frigid neighborhood
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just beyond the outermost
planet, Neptune.
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- Icy objects in the Kuiper belt
probably formed
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closer in toward the Sun,
where the giant planets are,
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but then gravitational
interactions
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with those giant planets
made those icy objects
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migrate outward.
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Narrator:
Our spacecraft navigates
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through this dark,
disk like region,
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which is almost
2 billion miles wide
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and is estimated to hold
over 6 billion comets.
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We eventually touch down
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on the surface of one
of these icy boulders.
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- Landing on a comet would be
a pretty tricky affair.
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[engine whirring]
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So you could kind of imagine
dirty snow
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that's covered
with exhaust,
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and if you step on it,
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in places,
you can punch through
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to places where there's more
fresh material underneath it.
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Narrator:
The Kuiper belt objects
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appear to have fairly stable
orbits,
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so they won't be that much fun
to ride.
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We lift off
in search of a comet
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that will cut
a more exciting path
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through our solar system.
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We navigate farther out
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to a sparsely populated region
called the scattered disc,
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which is home to icy bodies
with long, elliptical orbits.
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The slightest disturbance
can send these unstable objects
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careening into
the inner solar system,
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where they become known
as short-period comets,
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those which orbit the Sun
every 20 to 200 years.
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- The scattered disc region
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is thought to be
the primary source
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of the short-period comets.
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They are kicked into
the inner solar system
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either by interacting
with Neptune
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or possibly passing stars.
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Narrator:
Our spacecraft witnesses
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Neptune's gravitational
influence at work,
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dislodging a comet
out of the scattered disc.
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This comet would be
too dangerous to land on,
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so we'll track alongside it
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on its transformational flight
through our solar system.
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- So what would happen if it
was on a journey toward the Sun?
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Well, it would start off
looking like a dark asteroid.
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Nothing much is happening.
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It doesn't have an atmosphere
around it.
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- As you start to travel toward
the inner solar system,
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get up to Jupiter
or even closer to the Sun,
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the comet would start
to become active.
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- The warmth from the Sun
starts to heat up the comet,
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and all the frozen material
that's trapped on the inside
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starts to convert from ice
into gaseous material,
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and so these gas jets
can actually punch through
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the crust of the comet
and form jets.
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As these jets flow away
from the surface,
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they can start to pull
dust and rocks with them,
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and this forms
a kind of hazy atmosphere
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around the comet's nucleus.
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We call this the coma.
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Narrator:
As it zooms by Earth,
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the coma of a comet
can grow to be larger
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than the diameter
of our Sun.
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Solar radiation eventually
pushes this cosmic halo
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behind the nucleus,
forming two bright tails:
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one of dust
and the other of gas.
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- There will be a tail growing
and growing and growing,
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and you would eventually
become engulfed
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in just a really rocky, icy,
particle-filled environment.
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It would be very difficult
on your spacecraft
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because it'd be like flying
through a blizzard.
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Narrator: Some tails can stretch
for 100 million miles,
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more than the distance between
the Sun and the Earth,
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as it travels
towards our home star.
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It's one of the most spectacular
spectacles of our solar system.
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- Today we're going to see
what happens
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when we take a comet
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that's been in the cold, dark,
icy outer reaches
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of the solar system,
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and we're going to send it
inward towards its perihelion,
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or the point of closest approach
to the Sun.
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Now, dry ice
is frozen carbon dioxide,
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and this is a very common
constituent of comets.
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Let's see what happens.
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When we take
this piece of dry ice,
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and we drop it
into the warm water,
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the dry ice starts
to sublimate.
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That means it converts directly
from a solid, frozen state
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into a gaseous state.
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And as the water
starts to warm up
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certain parts
of the dry ice first,
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you can start to see that
little jets kind of form on it,
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and this forms a hazy atmosphere
called a coma.
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You can see that
the little chips of dry ice
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are constantly changing
as they sublimate away.
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Sometimes they speed up.
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Sometimes they slow down.
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So if this was a comet,
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you can get the idea that,
as the comet approaches the Sun,
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and the volatiles
start to vaporize,
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this can actually change
the comet's rotational state
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and even its orbit.
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Narrator. Comets
are brightest and fastest
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when they're closest
to the Sun.
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The searing heat and immense
gravity of our mother star
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can accelerate
a comet's speed
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to nearly 2 million miles
per hour.
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- The speed increases a lot,
and it whips around the Sun,
200
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so it goes zoom,
like that,
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like being propelled
202
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at the bottom
of a giant roller coaster.
203
00:10:02,810 --> 00:10:06,480
A roller coaster
starts out high, very slowly,
204
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picks up speed
due to the gravity,
205
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goes zooming past the bottom,
206
00:10:10,818 --> 00:10:14,154
and then slows down again
on its outward journey.
207
00:10:15,781 --> 00:10:18,283
- Eventually, as our comet
leaves the vicinity of the Sun,
208
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it's going to travel
back out
209
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into the far reaches
of the solar system.
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Everything's going
to quiet down.
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All of the gas and dust
is going to settle
212
00:10:24,957 --> 00:10:26,458
back onto its surface.
213
00:10:26,458 --> 00:10:29,461
And eventually, it'll cruise
away into the quiet dark.
214
00:10:32,506 --> 00:10:35,509
Narrator: Back in the cold
region of the scattered disc,
215
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a comet transforms
216
00:10:37,177 --> 00:10:40,513
back into a dull, black lump
of rock and ice
217
00:10:40,514 --> 00:10:44,351
until it makes its journey
around the Sun once again.
218
00:10:47,688 --> 00:10:51,358
Haley, the most famous
short-period comet,
219
00:10:51,358 --> 00:10:54,361
was first recorded
in 240 B.C.
220
00:10:54,361 --> 00:10:58,531
and has passed by Earth
every 76 years.
221
00:10:58,532 --> 00:11:01,368
Estimated to be the size
of Manhattan,
222
00:11:01,368 --> 00:11:04,371
this superstar comet
is sometimes so bright,
223
00:11:04,371 --> 00:11:07,582
it has been seen
in broad daylight.
224
00:11:07,583 --> 00:11:09,918
Throughout history,
225
00:11:09,918 --> 00:11:13,421
the appearance of Haley
has inspired awe and dread
226
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among earthly observers.
227
00:11:16,091 --> 00:11:18,760
-In 1910, it was feared,
228
00:11:18,760 --> 00:11:21,596
because spectroscopy
had just been introduced,
229
00:11:21,597 --> 00:11:25,267
and they had determined
that comets contain cyanogen,
230
00:11:25,267 --> 00:11:28,270
which is an odorless
and poisonous gas,
231
00:11:28,270 --> 00:11:30,939
and so astronomers predicted
that there'd be problems
232
00:11:30,939 --> 00:11:33,107
because of this poisonous gas
sweeping the Earth,
233
00:11:33,108 --> 00:11:36,277
and so there were actually
comet pills manufactured.
234
00:11:36,278 --> 00:11:39,281
Life insurance policies
on the comet were taken out.
235
00:11:41,742 --> 00:11:43,744
Narrator: While comets
have been thought to be
236
00:11:43,744 --> 00:11:46,246
extraterrestrial
harbingers of doom,
237
00:11:46,246 --> 00:11:49,916
astronomers have long wondered
if these glowing rocks
238
00:11:49,917 --> 00:11:53,921
contain precious information
about our past.
239
00:11:56,256 --> 00:11:59,759
By the 21st century,
NASA was ready to ignite
240
00:11:59,760 --> 00:12:04,260
a bold offensive strike,
one that would hopefully expose
241
00:12:04,431 --> 00:12:08,601
one of the holy grails
of planetary science.
242
00:12:08,602 --> 00:12:11,271
Could these
interplanetary vagabonds
243
00:12:11,271 --> 00:12:15,108
have been the cosmic
transporters of life?
244
00:12:20,614 --> 00:12:23,617
So far, we've traveled
with comets
245
00:12:23,617 --> 00:12:25,952
from the frozen hinterlands
of the Kuiper belt
246
00:12:25,953 --> 00:12:27,746
and scattered disc
247
00:12:27,746 --> 00:12:31,458
to an exhilarating orbit
around the Sun.
248
00:12:31,458 --> 00:12:34,127
We've watched these dark bodies
come alive
249
00:12:34,127 --> 00:12:37,964
as they formed brilliant comas
and tails.
250
00:12:37,965 --> 00:12:40,133
But scientists
are still puzzled
251
00:12:40,133 --> 00:12:44,633
about what's really inside
these cosmic interlopers.
252
00:12:46,098 --> 00:12:47,265
- Man, I wish I knew
253
00:12:47,266 --> 00:12:48,850
what the interior of a comet
looked like.
254
00:12:48,850 --> 00:12:50,017
You would love to be able
255
00:12:50,018 --> 00:12:53,021
to look inside
the nucleus of a comet,
256
00:12:53,021 --> 00:12:56,357
to see if it's clumpy,
if it's uniform.
257
00:12:56,358 --> 00:12:57,859
Is there crystalline ice?
258
00:12:57,859 --> 00:12:59,402
Is there glassy ice?
259
00:13:05,492 --> 00:13:07,160
Narrator:
Our protective spacecraft
260
00:13:07,160 --> 00:13:10,163
time-travels back to 2005
261
00:13:10,163 --> 00:13:14,000
and meets up with NASA's
Deep Impact space probe
262
00:13:14,001 --> 00:13:17,004
on a comet-hunting mission.
263
00:13:17,004 --> 00:13:21,504
It zeroes in on a short-period
comet named Tempel 1
264
00:13:21,508 --> 00:13:24,010
with an aggressive
plan of attack.
265
00:13:26,847 --> 00:13:30,183
We hover at a safe distance
as Deep Impact
266
00:13:30,183 --> 00:13:34,353
launches an 800-pound projectile
into the passing comet.
267
00:13:37,357 --> 00:13:40,526
Debris sprays out
for thousands of miles
268
00:13:40,527 --> 00:13:43,196
as the impact or
excavates a crater
269
00:13:43,196 --> 00:13:47,696
and sends tons of blinding gas,
rocks, and dust into space.
270
00:13:49,036 --> 00:13:51,204
For the first time
in history,
271
00:13:51,204 --> 00:13:54,040
scientists are able
to peer inside
272
00:13:54,041 --> 00:13:58,378
the icy, muddy interior
of a comet.
273
00:13:58,378 --> 00:14:00,004
- Right after the impact,
274
00:14:00,005 --> 00:14:03,008
you could see silicate grains
fluorescing and glowing.
275
00:14:03,008 --> 00:14:06,344
This tells us that comets
are very primitive material
276
00:14:06,345 --> 00:14:09,514
and that they pretty much
do preserve in pristine state
277
00:14:09,514 --> 00:14:11,015
the materials that we find
278
00:14:11,016 --> 00:14:13,518
in the youngest
star-forming systems.
279
00:14:13,518 --> 00:14:15,686
So indeed,
they really are time capsules
280
00:14:15,687 --> 00:14:17,855
that let us look back
on our own solar system
281
00:14:17,856 --> 00:14:19,858
at the very beginning.
282
00:14:22,319 --> 00:14:23,653
Narrator: While Deep Impact
283
00:14:23,653 --> 00:14:27,156
captures a rare glimpse
of a comet's interior,
284
00:14:27,157 --> 00:14:30,827
it is unable to snap
clear images of the crater,
285
00:14:30,827 --> 00:14:34,831
which was obscured by
an enormous plume of debris.
286
00:14:37,584 --> 00:14:41,087
In February 2011,
another spacecraft,
287
00:14:41,088 --> 00:14:42,756
named Stardust-NExT,
288
00:14:42,756 --> 00:14:44,591
catches up to Tempel 1
289
00:14:44,591 --> 00:14:48,261
as it completes its five-year
orbit around the Sun.
290
00:14:50,430 --> 00:14:53,266
To everyone's surprise,
291
00:14:53,266 --> 00:14:56,936
the impact crater is much
smaller than had been expected
292
00:14:56,937 --> 00:15:01,274
from the historic smash-up that
occurred five years earlier.
293
00:15:01,274 --> 00:15:03,109
- Amazing...
294
00:15:03,110 --> 00:15:05,445
But the crater looked like
it was small.
295
00:15:05,445 --> 00:15:07,280
So this now creates
this issue:
296
00:15:07,280 --> 00:15:09,115
Was the crater always small?
297
00:15:09,116 --> 00:15:13,120
We know the crater
isn't what we expected.
298
00:15:13,120 --> 00:15:14,955
So we're going
to do some experiments
299
00:15:14,955 --> 00:15:18,708
to see if we can explain why
the crater looks like it does.
300
00:15:18,708 --> 00:15:21,460
- Sunlamp's coming on.
301
00:15:21,461 --> 00:15:24,464
- Can we move it up a bit?
302
00:15:24,464 --> 00:15:27,300
Narrator. At NASA's
Ames Vertical Gun Range,
303
00:15:27,300 --> 00:15:30,469
Stardust-NExT
co-investigator Pete Schultz
304
00:15:30,470 --> 00:15:33,973
is conducting high-velocity
impact experiments
305
00:15:33,974 --> 00:15:38,474
to find out why Deep Impact
produced such a tiny crater.
306
00:15:39,104 --> 00:15:40,939
He will use a massive
307
00:15:40,939 --> 00:15:44,108
.30-caliber high-velocity
gas gun
308
00:15:44,109 --> 00:15:47,946
to fire tiny projectile beads
at various targets
309
00:15:47,946 --> 00:15:50,782
located inside
a vacuum chamber.
310
00:15:55,162 --> 00:15:57,664
- We're trying to simulate
311
00:15:57,664 --> 00:16:01,250
what the nature of the surface
of comet 9P/Tempel 1 is like,
312
00:16:01,251 --> 00:16:03,086
so we're putting in per lite,
313
00:16:03,086 --> 00:16:04,754
which is this low-density
material
314
00:16:04,754 --> 00:16:06,088
that you find in gardens,
315
00:16:06,089 --> 00:16:08,174
then we're adding in
hollow micro spheres,
316
00:16:08,175 --> 00:16:12,345
and this also resemble what
the nature of the comet is like.
317
00:16:12,345 --> 00:16:15,348
The purpose of the experiment
is to see what happens
318
00:16:15,348 --> 00:16:17,183
to the crater
after formation.
319
00:16:17,184 --> 00:16:19,311
Does it stay there?
Does it collapse?
320
00:16:19,311 --> 00:16:21,771
With this experiment,
we should be able to find out.
321
00:16:23,023 --> 00:16:24,524
Okay, I'm out of the tank.
322
00:16:24,524 --> 00:16:26,192
Lock and load.
323
00:16:26,193 --> 00:16:27,527
Narrator: High-speed cameras
324
00:16:27,527 --> 00:16:29,862
mounted around
the vacuum chamber
325
00:16:29,863 --> 00:16:31,865
will document the impact.
326
00:16:31,865 --> 00:16:33,491
- We've got this one covered.
327
00:16:33,492 --> 00:16:36,661
We just have to hit
the target.
328
00:16:36,661 --> 00:16:37,828
Okay.
329
00:16:37,829 --> 00:16:39,330
[claps hands]
330
00:16:39,331 --> 00:16:41,082
Let's shoot this puppy.
331
00:16:41,082 --> 00:16:42,416
J.P., are you ready?
332
00:16:42,417 --> 00:16:43,584
- Yeah.
333
00:16:45,086 --> 00:16:48,547
Narrator: As the crew anxiously
awaits in the control room,
334
00:16:48,548 --> 00:16:52,385
Pete mixes science
with a little superstition.
335
00:16:52,385 --> 00:16:53,719
- There's always a risk.
336
00:16:53,720 --> 00:16:56,764
Sometimes you miss.
Sometimes you hit.
337
00:17:01,019 --> 00:17:02,645
- Whoa!
338
00:17:02,646 --> 00:17:03,855
- Oh, sweet.
339
00:17:03,855 --> 00:17:06,524
The whole thing sort of
collapses in on itself.
340
00:17:06,525 --> 00:17:07,901
It's getting smaller now.
341
00:17:07,901 --> 00:17:10,069
It was bigger.
Now it's getting smaller.
342
00:17:10,070 --> 00:17:13,907
So what we see here is that
there's a lot of dust and ejecta
343
00:17:13,907 --> 00:17:16,743
sent upwards,
and that blocked the view.
344
00:17:16,743 --> 00:17:19,078
We couldn't see
the crater forming.
345
00:17:19,079 --> 00:17:21,289
So what started off
being a nice-looking crater,
346
00:17:21,289 --> 00:17:22,790
it just doesn't stay there.
347
00:17:22,791 --> 00:17:24,250
It just simply heals itself.
348
00:17:24,251 --> 00:17:27,754
So what may have happened
for 9P/Tempel 1,
349
00:17:27,754 --> 00:17:31,591
the nucleus, is that
that crater healed itself.
350
00:17:31,591 --> 00:17:34,760
The nucleus healed itself
from the scar created
351
00:17:34,761 --> 00:17:37,054
by us with Deep Impact.
352
00:17:37,055 --> 00:17:39,057
Let's see what we did.
353
00:17:42,102 --> 00:17:44,229
[groans]
354
00:17:44,229 --> 00:17:46,147
So the results
were fantastic.
355
00:17:46,147 --> 00:17:48,816
We got to see
just what we planned to.
356
00:17:48,817 --> 00:17:50,485
There may be more
to the story,
357
00:17:50,485 --> 00:17:54,155
so we're going to try
a different experiment as well.
358
00:17:54,155 --> 00:17:55,823
Narrator: Pete has a hunch
359
00:17:55,824 --> 00:17:59,494
there's a missing piece
to the Deep Impact mission.
360
00:17:59,494 --> 00:18:01,996
He now wants to see
if the space probe
361
00:18:01,997 --> 00:18:05,667
created a different type
of crater on Tempel 1,
362
00:18:05,667 --> 00:18:09,837
due to the makeup
of the comet's nucleus.
363
00:18:09,838 --> 00:18:11,840
- So this time,
we're going to put
364
00:18:11,840 --> 00:18:16,340
a denser layer
below that per lite,
365
00:18:17,012 --> 00:18:18,847
so we want to find out
whether or not
366
00:18:18,847 --> 00:18:20,348
we'll get a different type
of crater
367
00:18:20,348 --> 00:18:22,850
if we have two different types
of material:
368
00:18:22,851 --> 00:18:24,727
one very soft on top
369
00:18:24,728 --> 00:18:28,732
and one denser
on the bottom.
370
00:18:28,732 --> 00:18:31,484
Narrator: Pete and his crew
return to the control room
371
00:18:31,484 --> 00:18:34,320
to see what happens
to the new target of per lite
372
00:18:34,321 --> 00:18:37,157
poured over a heavier layer
of sand.
373
00:18:41,369 --> 00:18:42,536
[small explosion]
374
00:18:42,537 --> 00:18:44,205
- [laughs]
375
00:18:44,205 --> 00:18:47,583
Now, that formed a big crater
in the per lite.
376
00:18:47,584 --> 00:18:50,086
Boy, look at that.
377
00:18:50,086 --> 00:18:53,756
Oh, oh, man,
that is gorgeous.
378
00:18:53,757 --> 00:18:55,425
Okay.
379
00:18:55,425 --> 00:18:57,301
The projectile went deep,
380
00:18:57,302 --> 00:19:00,138
and now the stuff
is coming back out that hole,
381
00:19:00,138 --> 00:19:03,307
while, on the surface,
it's excavating debris.
382
00:19:05,310 --> 00:19:06,644
Pow!
Okay.
383
00:19:06,645 --> 00:19:08,980
Narrator: The double-layered
target created not one
384
00:19:08,980 --> 00:19:10,856
but two craters,
385
00:19:10,857 --> 00:19:15,357
a small crater inside
a larger, shallower crater.
386
00:19:15,528 --> 00:19:19,114
- This could be what happened
for 9P/Tempel 1.
387
00:19:19,115 --> 00:19:21,951
It went so deep
into the nucleus,
388
00:19:21,951 --> 00:19:25,287
and then it just simply
collapses away,
389
00:19:25,288 --> 00:19:28,124
and we're left with just
this very, very faint rim
390
00:19:28,124 --> 00:19:31,210
on the outside with
a small pit in the center.
391
00:19:31,211 --> 00:19:33,546
Narrator:
These impact experiments
392
00:19:33,546 --> 00:19:37,716
yield surprising clues about
the interior of Tempel 1
393
00:19:37,717 --> 00:19:40,720
and perhaps all comets.
394
00:19:40,720 --> 00:19:43,222
- Now we know that comets
have history.
395
00:19:43,223 --> 00:19:44,891
We see layers.
396
00:19:44,891 --> 00:19:46,893
I don't know if these layers
go all the way
397
00:19:46,893 --> 00:19:48,895
through the nucleus,
398
00:19:48,895 --> 00:19:51,564
or are they only
in one part?
399
00:19:52,732 --> 00:19:54,233
Narrator:
Unraveling the secrets
400
00:19:54,234 --> 00:19:57,570
of what's inside comets
will help scientists understand
401
00:19:57,570 --> 00:20:01,574
what causes them to exhibit
some really bizarre behavior.
402
00:20:08,331 --> 00:20:12,168
Our spaceship now shadows
NASA's EPOXI mission
403
00:20:12,168 --> 00:20:14,420
as it encounters Hartley 2,
404
00:20:14,421 --> 00:20:18,091
a fast-spinning comet
that tumbles through space
405
00:20:18,091 --> 00:20:21,928
like a hyperactive
cosmic peanut.
406
00:20:21,928 --> 00:20:23,596
- Hartley 2
is a smaller comet.
407
00:20:23,596 --> 00:20:25,431
It's only about a mile or so
across,
408
00:20:25,432 --> 00:20:28,101
and so it's kind of a surprise
that it's so active.
409
00:20:28,101 --> 00:20:29,435
It's putting off huge amounts
410
00:20:29,436 --> 00:20:31,938
of CO2 and, actually,
cyanide gas.
411
00:20:31,938 --> 00:20:33,105
And the question is,
412
00:20:33,106 --> 00:20:34,607
are all small comets
active like this
413
00:20:34,607 --> 00:20:35,608
or only a few?
414
00:20:35,608 --> 00:20:37,610
And what makes them
so active?
415
00:20:39,946 --> 00:20:42,448
I've got a peanut-shaped
plastic bottle here
416
00:20:42,449 --> 00:20:44,951
that's supposed to represent
comet Hartley 2.
417
00:20:44,951 --> 00:20:46,786
It's full of dry ice
and warm water,
418
00:20:46,786 --> 00:20:48,120
and as you can see,
419
00:20:48,121 --> 00:20:50,456
as the warm water starts to make
the dry ice sublimate,
420
00:20:50,457 --> 00:20:52,125
it shoots out these jets
421
00:20:52,125 --> 00:20:53,960
through the holes that
we've got poked in the bottle.
422
00:20:53,960 --> 00:20:55,461
If I drop it into the water,
423
00:20:55,462 --> 00:20:57,797
instead of holding it
fixed in space,
424
00:20:57,797 --> 00:20:59,465
you can see that the jets
actually start
425
00:20:59,466 --> 00:21:00,800
pushing the bottle around,
426
00:21:00,800 --> 00:21:03,093
causing the comet's
rotational state to change.
427
00:21:03,094 --> 00:21:04,762
This is very similar
to what's going on
428
00:21:04,763 --> 00:21:06,473
on the surface
of comet Hartley 2.
429
00:21:06,473 --> 00:21:09,642
The CO2 jets are actually
changing the rotational state
430
00:21:09,642 --> 00:21:13,312
of the comet, causing it
to speed up and slow down.
431
00:21:15,356 --> 00:21:17,441
Narrator:
When tracking Hartley 2,
432
00:21:17,442 --> 00:21:21,279
our spacecraft gets caught
in a cosmic blizzard
433
00:21:21,279 --> 00:21:24,448
as the spastic comet
burps and belches out
434
00:21:24,449 --> 00:21:28,949
a trail of frozen snowballs that
extend for millions of miles.
435
00:21:30,789 --> 00:21:32,791
- One of the big surprises
about Hartley 2
436
00:21:32,791 --> 00:21:37,003
is that it was surrounded
by this posse of mini comets.
437
00:21:37,003 --> 00:21:40,172
This is simply ices
that are coming off,
438
00:21:40,173 --> 00:21:42,842
about the size of a snowball
all the way up to a basketball.
439
00:21:42,842 --> 00:21:47,012
Narrator: Scientists suspect
the snowball-sized debris
440
00:21:47,013 --> 00:21:50,016
rains back down on Hartley 2,
441
00:21:50,016 --> 00:21:54,516
producing its unusual landscape
of craters and towering spires.
442
00:21:55,855 --> 00:21:58,190
- Because these comets
have very little gravities,
443
00:21:58,191 --> 00:22:00,193
most of the gas
is blown out into space,
444
00:22:00,193 --> 00:22:03,029
but a very small fraction
can actually redeposit
445
00:22:03,029 --> 00:22:05,865
on the surface, generating
very smooth textures,
446
00:22:05,865 --> 00:22:08,367
and on other locations,
generating these very bumpy
447
00:22:08,368 --> 00:22:10,536
or spire-like texture.
448
00:22:10,537 --> 00:22:12,372
Narrator: From Hartley 2,
449
00:22:12,372 --> 00:22:16,751
we blast off to the extreme
outer edge of our solar system,
450
00:22:16,751 --> 00:22:19,420
a vast, eerie place,
451
00:22:19,420 --> 00:22:22,881
barely within the gravitational
grasp of our Sun
452
00:22:22,882 --> 00:22:27,382
and impossible to see,
even with modern telescopes.
453
00:22:27,720 --> 00:22:32,220
Here, we come upon the largest
and perhaps most elusive
454
00:22:32,225 --> 00:22:36,062
icy bodies in
our galactic neighborhood.
455
00:22:44,362 --> 00:22:47,365
Our journey through
the fascinating world of comets
456
00:22:47,365 --> 00:22:51,202
has provided us a ringside seat
to some of the greatest
457
00:22:51,202 --> 00:22:55,539
cosmic shows observed
from Earth and space.
458
00:22:59,919 --> 00:23:02,421
We now change course
and travel
459
00:23:02,422 --> 00:23:06,922
over 50,000 times the distance
between Earth and the Sun
460
00:23:06,926 --> 00:23:11,426
to the outermost edge
of our solar system.
461
00:23:11,931 --> 00:23:14,266
We arrive at the Oort cloud,
462
00:23:14,267 --> 00:23:17,228
an even larger fraternity
of comets,
463
00:23:17,228 --> 00:23:21,398
perhaps over a trillion
of them.
464
00:23:21,399 --> 00:23:23,067
- If we'd actually
got in a spaceship
465
00:23:23,067 --> 00:23:26,236
and tried to go out and, say,
visit the Oort cloud,
466
00:23:26,237 --> 00:23:28,614
this would have been
a long journey.
467
00:23:28,615 --> 00:23:32,785
There's billions and billions
of these objects,
468
00:23:32,785 --> 00:23:35,454
and there's a lot of space
in between them.
469
00:23:37,290 --> 00:23:40,626
Narrator: Like the Kuiper belt
and scattered disc,
470
00:23:40,627 --> 00:23:44,631
the Oort cloud objects may
have formed closer to the Sun,
471
00:23:44,631 --> 00:23:46,799
but about 800 million years
472
00:23:46,799 --> 00:23:49,426
after the solar system
was formed,
473
00:23:49,427 --> 00:23:53,431
the gravitational influence
of the gas giant planets
474
00:23:53,431 --> 00:23:54,765
flung these comets
475
00:23:54,766 --> 00:23:57,769
out to the frigid edge
of our solar system.
476
00:23:59,187 --> 00:24:00,688
- Some of these objects
were flung
477
00:24:00,688 --> 00:24:02,690
into very highly elliptical
orbits
478
00:24:02,690 --> 00:24:04,358
out into the Oort cloud.
479
00:24:04,359 --> 00:24:06,527
Passing stars could
circularize those orbits,
480
00:24:06,527 --> 00:24:10,197
making somewhat stable orbits
for them.
481
00:24:10,198 --> 00:24:11,866
Narrator: Most of
the Oort cloud bodies
482
00:24:11,866 --> 00:24:13,701
have been
in frozen hibernation
483
00:24:13,701 --> 00:24:17,204
since the birth
of our solar system.
484
00:24:17,205 --> 00:24:19,874
They only become
long-period comets
485
00:24:19,874 --> 00:24:21,542
when they get sucked
into orbits
486
00:24:21,542 --> 00:24:26,042
that carry them inward towards
the planets and the Sun.
487
00:24:27,048 --> 00:24:29,216
Scientists have never
actually captured
488
00:24:29,217 --> 00:24:31,385
an image of the Oort cloud,
489
00:24:31,386 --> 00:24:35,056
but they have good reason
to believe it's there.
490
00:24:35,056 --> 00:24:37,558
- Even though scientists can't
directly observe the Oort cloud
491
00:24:37,558 --> 00:24:40,060
because it's so far away
and so faint,
492
00:24:40,061 --> 00:24:42,396
what they are able to do
is infer its existence
493
00:24:42,397 --> 00:24:43,898
because we can look at
494
00:24:43,898 --> 00:24:46,901
where all these long-period
comets come from on the sky,
495
00:24:46,901 --> 00:24:49,069
and they seem to come
from all different directions.
496
00:24:49,070 --> 00:24:51,739
There doesn't really seem to be
a preferred direction for them.
497
00:24:51,739 --> 00:24:53,574
This suggests that
the Oort cloud,
498
00:24:53,574 --> 00:24:56,410
if it exists,
is probably roughly spherical.
499
00:24:58,454 --> 00:25:00,372
Narrator:
One of the big mysteries
500
00:25:00,373 --> 00:25:03,876
is what knocks these icy bodies
off course
501
00:25:03,876 --> 00:25:08,213
and sends them cruising
by our neighborhood of Earth.
502
00:25:08,214 --> 00:25:10,883
- The comets in the Oort cloud
are very susceptible
503
00:25:10,883 --> 00:25:13,385
to gravitational pulls
from other things
504
00:25:13,386 --> 00:25:15,054
outside the solar system.
505
00:25:15,054 --> 00:25:17,056
One thing is passing stars.
506
00:25:17,056 --> 00:25:20,142
If a star happens to come
close to our Sun,
507
00:25:20,143 --> 00:25:23,980
it can scatter comets
from the outer Oort cloud.
508
00:25:25,440 --> 00:25:28,609
- Icy objects in the Oort cloud
can also be dislodged
509
00:25:28,609 --> 00:25:31,153
by gravitational perturbations
that occur
510
00:25:31,154 --> 00:25:34,198
when the solar system goes
through the plane of our galaxy.
511
00:25:34,198 --> 00:25:35,866
So the solar system
is basically orbiting
512
00:25:35,867 --> 00:25:37,368
around the center
of our galaxy,
513
00:25:37,368 --> 00:25:39,536
but it's also oscillating
up and down,
514
00:25:39,537 --> 00:25:41,372
and when it goes
through the plane,
515
00:25:41,372 --> 00:25:44,375
then gravitational interactions
can perturb objects
516
00:25:44,375 --> 00:25:48,712
from the Oort cloud
into the inner solar system.
517
00:25:48,713 --> 00:25:50,548
Narrator:
Some long-period comets
518
00:25:50,548 --> 00:25:53,050
take up to about
30 million years
519
00:25:53,051 --> 00:25:56,721
to complete one round trip
around the Sun.
520
00:25:59,932 --> 00:26:02,434
Our spacecraft
tracks a long-period comet
521
00:26:02,435 --> 00:26:04,937
for hundreds of thousands
of miles
522
00:26:04,937 --> 00:26:07,940
until we approach
planet Earth.
523
00:26:08,983 --> 00:26:11,151
As its icy tails unfurl,
524
00:26:11,152 --> 00:26:13,487
a layer of dust and ice
zips through
525
00:26:13,488 --> 00:26:15,823
our planet's
thin atmosphere,
526
00:26:15,823 --> 00:26:19,660
leaving visible trails
known as a meteor shower.
527
00:26:22,288 --> 00:26:23,622
- I like to think of comets
528
00:26:23,623 --> 00:26:25,625
as sort of the pigpens
of the solar system,
529
00:26:25,625 --> 00:26:27,460
because, as they orbit
around the Sun,
530
00:26:27,460 --> 00:26:29,670
they leave a big, messy trail
of debris.
531
00:26:29,670 --> 00:26:31,838
But sometimes the Earth's orbit
can intersect
532
00:26:31,839 --> 00:26:33,674
some of these dust bands,
533
00:26:33,674 --> 00:26:36,927
and when it does, we can
sometimes see meteor showers.
534
00:26:36,928 --> 00:26:38,763
Those beautiful bright streaks
of light
535
00:26:38,763 --> 00:26:40,431
that you see coming through
the night sky
536
00:26:40,431 --> 00:26:41,932
are actually produced
by particles
537
00:26:41,933 --> 00:26:44,602
that are most often no bigger
than a sand grain.
538
00:26:46,437 --> 00:26:49,106
Narrator: While long-
and short-period comets
539
00:26:49,107 --> 00:26:52,527
make up the bulk of comets
that have been observed,
540
00:26:52,527 --> 00:26:56,364
new evidence suggests
that not all icy bodies
541
00:26:56,364 --> 00:27:00,701
come from the subzero suburbs
of our solar system.
542
00:27:00,701 --> 00:27:03,036
Some have secretly
taken up residence
543
00:27:03,037 --> 00:27:06,040
in a much warmer
neighborhood.
544
00:27:10,128 --> 00:27:12,964
Scientists have now
discovered
545
00:27:12,964 --> 00:27:16,133
there are comets masquerading
as asteroids
546
00:27:16,134 --> 00:27:18,136
in the asteroid belt,
547
00:27:18,136 --> 00:27:21,139
located between
Jupiter and Mars.
548
00:27:23,683 --> 00:27:25,518
- The only reason
that we've discovered
549
00:27:25,518 --> 00:27:29,021
these main-belt comets
is because, occasionally,
550
00:27:29,021 --> 00:27:33,025
the warming rays of the Sun
get into the interior,
551
00:27:33,025 --> 00:27:34,526
vaporize the ices,
552
00:27:34,527 --> 00:27:37,696
and so the comet just
bursts forth for a while,
553
00:27:37,697 --> 00:27:42,197
and then they go back to being
inactive objects or asteroids.
554
00:27:43,369 --> 00:27:46,038
- Scientists used to think that
there were strong distinctions
555
00:27:46,038 --> 00:27:47,873
between asteroids and comets
556
00:27:47,874 --> 00:27:50,376
and that they were two totally
different types of objects,
557
00:27:50,376 --> 00:27:52,211
but what we're
finding nowadays is,
558
00:27:52,211 --> 00:27:55,047
there are some asteroids
that have comet-like properties,
559
00:27:55,047 --> 00:27:57,382
and there are some comets
that eventually kind of look
560
00:27:57,383 --> 00:27:59,385
like asteroids.
561
00:28:02,388 --> 00:28:05,057
Narrator: Some scientists
think main-belt comets
562
00:28:05,057 --> 00:28:08,101
may have delivered water
to early Earth
563
00:28:08,102 --> 00:28:11,105
and the materials
to create life.
564
00:28:13,441 --> 00:28:16,735
We blast back
to January 2004
565
00:28:16,736 --> 00:28:20,239
and follow NASA's
Stardust spacecraft
566
00:28:20,239 --> 00:28:22,574
on an unprecedented mission
567
00:28:22,575 --> 00:28:26,245
to collect pure comet dust
in space.
568
00:28:26,245 --> 00:28:29,957
Just beyond the planet Mars,
569
00:28:29,957 --> 00:28:33,627
we meet up with
a comet named Wild 2.
570
00:28:33,628 --> 00:28:36,464
Upon approaching
its enormous coma,
571
00:28:36,464 --> 00:28:39,758
Stardust flips open
a paddle-shaped collector tray
572
00:28:39,759 --> 00:28:44,259
filled with a durable foam-like
substance called aerogel.
573
00:28:46,599 --> 00:28:50,603
Cometary particles no bigger
than specks of dust
574
00:28:50,603 --> 00:28:52,271
fly into the aerogel
575
00:28:52,271 --> 00:28:55,607
at six times the speed
of a rifle bullet.
576
00:28:55,608 --> 00:28:59,945
The mission's task is to
preserve the precious particles
577
00:28:59,946 --> 00:29:03,407
without damaging
or altering them.
578
00:29:03,407 --> 00:29:07,907
But this is no easy feat,
as we show here on Earth.
579
00:29:10,581 --> 00:29:13,041
- We're here at a firing range
with Sergeant Connacht Brewer,
580
00:29:13,042 --> 00:29:14,334
a former army paratrooper,
581
00:29:14,335 --> 00:29:16,462
who is going to demonstrate
for us what happens
582
00:29:16,462 --> 00:29:19,465
when this birds hot strikes
a large block of modeling clay.
583
00:29:19,465 --> 00:29:21,633
This is an excellent analogy
for what happened
584
00:29:21,634 --> 00:29:24,303
when cometary particles
impacted the aerogel
585
00:29:24,303 --> 00:29:25,971
on the Stardust spacecraft.
586
00:29:25,972 --> 00:29:27,807
Except there,
the particles were moving
587
00:29:27,807 --> 00:29:30,267
about 50 times faster
than this birds hot.
588
00:29:30,268 --> 00:29:31,310
Ready to give it a go?
589
00:29:31,310 --> 00:29:32,477
-Yes, I am.
590
00:29:32,478 --> 00:29:34,021
Go ahead and put on
your eye protection
591
00:29:34,021 --> 00:29:35,022
and your earplugs.
592
00:29:35,022 --> 00:29:36,356
What we're using
for this today
593
00:29:36,357 --> 00:29:38,817
is a 12-gauge Model 1100
Remington shotgun
594
00:29:38,818 --> 00:29:40,528
at a distance
of about 35 yards.
595
00:29:40,528 --> 00:29:44,365
Basically, I'm just gonna
load a 12-gauge shot shell
596
00:29:44,365 --> 00:29:45,699
into the shotgun...
597
00:29:45,700 --> 00:29:46,701
[gun clicks]
598
00:29:46,701 --> 00:29:48,369
And we're hot.
599
00:29:51,163 --> 00:29:52,330
[gunshot]
600
00:29:52,331 --> 00:29:53,790
- Whoa.
601
00:29:53,791 --> 00:29:55,334
It really did some damage
to that clay.
602
00:29:55,334 --> 00:29:56,501
You want to go take a look?
603
00:29:56,502 --> 00:29:57,669
- Yeah, we're clear.
604
00:29:57,670 --> 00:30:01,173
- All right.
605
00:30:01,173 --> 00:30:03,341
Wow, look at the damage
it did to the clay.
606
00:30:03,342 --> 00:30:04,509
- Yeah.
607
00:30:04,510 --> 00:30:06,178
- Each pellet
created one of these holes.
608
00:30:06,178 --> 00:30:07,512
So what do you say
we cut this open
609
00:30:07,513 --> 00:30:08,680
and try to find some pieces?
610
00:30:08,681 --> 00:30:10,349
- Sounds good.
- All right.
611
00:30:14,478 --> 00:30:17,147
So you see, the trail here
that's formed inside the clay
612
00:30:17,148 --> 00:30:18,649
is going to lead you,
ultimately,
613
00:30:18,649 --> 00:30:21,193
to where the birds hot pellets
are located.
614
00:30:21,193 --> 00:30:23,361
You can imagine how difficult
it would have been
615
00:30:23,362 --> 00:30:24,863
and how time-consuming
616
00:30:24,864 --> 00:30:27,741
for the Stardust team to locate
these microscopic pieces
617
00:30:27,742 --> 00:30:30,077
of cometary material
inside the aerogel.
618
00:30:33,497 --> 00:30:36,208
Narrator: Upon Stardust's
return to Earth,
619
00:30:36,208 --> 00:30:40,045
scientists recovered
over 10,000 cometary fragments
620
00:30:40,046 --> 00:30:42,715
from the aerogel.
621
00:30:42,715 --> 00:30:45,551
Chemical analysis revealed
that the particles
622
00:30:45,551 --> 00:30:48,554
contained the organic compound
glycine,
623
00:30:48,554 --> 00:30:51,557
a fundamental building block
of life
624
00:30:51,557 --> 00:30:55,811
that had been preserved in ice
for over 4 billion years.
625
00:30:57,146 --> 00:31:00,149
- The discovery of
organic compounds in comets
626
00:31:00,149 --> 00:31:03,610
suggests that organic compounds
can form pretty easily.
627
00:31:03,611 --> 00:31:06,780
Now, it doesn't mean that there
was ever anything truly alive
628
00:31:06,781 --> 00:31:10,451
in those comets, but at least
the building blocks of life
629
00:31:10,451 --> 00:31:12,953
could have been built
in comets.
630
00:31:15,164 --> 00:31:17,666
Narrator: Comets appear to hold
invaluable information
631
00:31:17,666 --> 00:31:20,877
about the origin
of our solar system
632
00:31:20,878 --> 00:31:24,047
and perhaps life itself.
633
00:31:24,048 --> 00:31:25,716
But astronomers
have discovered
634
00:31:25,716 --> 00:31:30,053
that these icy bodies
are not immortal.
635
00:31:30,054 --> 00:31:33,891
Now state-of-the-art satellites
have captured images
636
00:31:33,891 --> 00:31:37,394
of a select group of comets
that will end their life
637
00:31:37,395 --> 00:31:40,398
in a suicidal death dive.
638
00:31:47,613 --> 00:31:49,781
While our journey
with the comets
639
00:31:49,782 --> 00:31:54,119
has felt like an endless
cosmic roller coaster ride,
640
00:31:54,120 --> 00:31:58,620
these icy objects will not orbit
our Sun forever.
641
00:31:59,291 --> 00:32:02,961
Most will make the voyage
for several thousand years
642
00:32:02,962 --> 00:32:06,131
before evaporating
into specks of dust.
643
00:32:09,677 --> 00:32:12,513
Even massive comets,
like Haley,
644
00:32:12,513 --> 00:32:16,350
only have 150,000 years left.
645
00:32:16,350 --> 00:32:20,850
That's because, every second,
a comet loses tons of ice.
646
00:32:22,690 --> 00:32:25,526
- Comets gradually wither away
or fade away,
647
00:32:25,526 --> 00:32:28,028
because every time
they pass close to the Sun,
648
00:32:28,028 --> 00:32:30,196
they lose some of their ices.
649
00:32:30,197 --> 00:32:31,698
They evaporate away.
650
00:32:31,699 --> 00:32:34,535
Eventually,
there's very little ice left,
651
00:32:34,535 --> 00:32:37,996
and so the comet coma and tail
doesn't form.
652
00:32:37,997 --> 00:32:39,999
It just looks like
an asteroid.
653
00:32:39,999 --> 00:32:41,333
Or it may even break apart
654
00:32:41,333 --> 00:32:43,168
into a whole bunch
of little objects
655
00:32:43,169 --> 00:32:46,172
because the icy glue
is no longer there
656
00:32:46,172 --> 00:32:49,341
or because tidal effects
actually break it apart.
657
00:32:51,302 --> 00:32:54,972
Narrator: But not all comets
quietly fade into the sunset.
658
00:32:58,100 --> 00:33:01,603
We're now in hot pursuit
of a group of comets
659
00:33:01,604 --> 00:33:06,104
called sun grazers
that live fast and die young.
660
00:33:08,360 --> 00:33:11,863
Inside our spacecraft,
we feel the heat
661
00:33:11,864 --> 00:33:15,033
as the comets' extremely
elongated orbits
662
00:33:15,034 --> 00:33:17,703
bring us very close
to the Sun...
663
00:33:17,703 --> 00:33:20,455
within a few hundred thousand
miles.
664
00:33:22,583 --> 00:33:25,085
As we enter this danger zone,
665
00:33:25,085 --> 00:33:28,088
we see that some of these
kamikaze comets
666
00:33:28,088 --> 00:33:31,758
occasionally plunge
right into our home star,
667
00:33:31,759 --> 00:33:34,428
creating
a ferocious spectacle.
668
00:33:37,223 --> 00:33:40,059
- Sun grazer comets start out
their life as normal comets.
669
00:33:40,059 --> 00:33:41,894
They probably live
either in the Oort cloud,
670
00:33:41,894 --> 00:33:43,562
or they're short-period
comets,
671
00:33:43,562 --> 00:33:46,064
but they've had an unlucky
encounter with another planet,
672
00:33:46,065 --> 00:33:48,734
probably Jupiter.
673
00:33:48,734 --> 00:33:50,569
If they're really,
really lucky,
674
00:33:50,569 --> 00:33:53,071
they might just escape
and be able to get away
675
00:33:53,072 --> 00:33:55,032
with one close passage
by the Sun,
676
00:33:55,032 --> 00:33:56,199
but if they're not lucky,
677
00:33:56,200 --> 00:33:58,535
they just get swallowed up whole
by the Sun.
678
00:34:01,705 --> 00:34:04,207
Narrator: The Solar and
Heliospheric Observatory,
679
00:34:04,208 --> 00:34:07,544
or SOHO,
is a space satellite
680
00:34:07,545 --> 00:34:11,549
that has observed 2,000 comets
on suicidal orbits.
681
00:34:13,926 --> 00:34:18,263
The most famous sun grazers
are the Kreutz family,
682
00:34:18,264 --> 00:34:21,267
which originated
from one giant comet
683
00:34:21,267 --> 00:34:25,604
that broke up into
many smaller pieces.
684
00:34:25,604 --> 00:34:28,273
- It's a kind of cool thing
to think of a comet
685
00:34:28,274 --> 00:34:29,942
that's lived
in the outer solar system
686
00:34:29,942 --> 00:34:32,277
just falling all the way
and smashing into the Sun,
687
00:34:32,278 --> 00:34:33,612
but they do.
688
00:34:33,612 --> 00:34:35,280
We see them all the time.
689
00:34:39,910 --> 00:34:43,747
Narrator: And some comets
do more than self-destruct.
690
00:34:43,747 --> 00:34:46,791
They become the messengers
of mass destruction.
691
00:34:48,877 --> 00:34:51,212
It's estimated
that a large comet
692
00:34:51,213 --> 00:34:55,383
may have struck Earth
roughly every 40 million years,
693
00:34:55,384 --> 00:34:58,845
based on the amount of craters
still visible on our planet.
694
00:35:02,182 --> 00:35:04,851
A comet may have
even been responsible
695
00:35:04,852 --> 00:35:08,522
for the most famous
extinction event of all time.
696
00:35:11,942 --> 00:35:14,945
- For the Cretaceous-Tertiary
extinction event,
697
00:35:14,945 --> 00:35:16,446
the one that took out
the dinosaurs
698
00:35:16,447 --> 00:35:19,491
65 million years ago,
the jury is still out.
699
00:35:19,491 --> 00:35:22,327
That was thought to be
a 10-kilometer-sized object,
700
00:35:22,328 --> 00:35:25,497
and there are no asteroids
in near-Earth space
701
00:35:25,497 --> 00:35:29,334
that are that large
that could impact the Earth,
702
00:35:29,335 --> 00:35:32,671
and there are a number of comets
that are that large.
703
00:35:32,671 --> 00:35:35,465
And since it occurred
65 million years ago,
704
00:35:35,466 --> 00:35:37,134
and you would expect
a cometary impact
705
00:35:37,134 --> 00:35:40,637
every 40 million years or so,
706
00:35:40,638 --> 00:35:43,974
it may well have been
a comet.
707
00:35:43,974 --> 00:35:46,476
Narrator: While comets
likely slammed into Earth
708
00:35:46,477 --> 00:35:49,146
countless times in the past,
709
00:35:49,146 --> 00:35:50,814
it's been difficult
to determine
710
00:35:50,814 --> 00:35:55,314
if an impact crater
was made by a comet or asteroid
711
00:35:55,486 --> 00:35:58,322
because the two bodies
appear to be similar.
712
00:36:00,491 --> 00:36:02,576
- When we study
the fossil records,
713
00:36:02,576 --> 00:36:04,244
a lot of the material is gone,
714
00:36:04,244 --> 00:36:06,246
and just-—
we simply can't find it,
715
00:36:06,246 --> 00:36:08,081
and it turns out that
asteroids and comets
716
00:36:08,082 --> 00:36:09,541
have a lot of materials
in common,
717
00:36:09,541 --> 00:36:12,502
so even if you do find
extraterrestrial material,
718
00:36:12,503 --> 00:36:13,837
it's really hard to tell
719
00:36:13,837 --> 00:36:16,172
whether it came from an asteroid
or from a comet.
720
00:36:17,883 --> 00:36:19,718
Narrator:
And to complicate matters,
721
00:36:19,718 --> 00:36:22,887
a comet doesn't even
have to impact Earth's surface
722
00:36:22,888 --> 00:36:25,390
to ignite a catastrophe.
723
00:36:27,851 --> 00:36:31,896
In 1908, a fireball exploded
in the atmosphere
724
00:36:31,897 --> 00:36:35,233
above the Tunguska wilderness
in Siberia.
725
00:36:35,234 --> 00:36:37,736
The heat and energy
from the air burst
726
00:36:37,736 --> 00:36:41,740
propelled downward
like a hot tornado.
727
00:36:41,740 --> 00:36:44,075
It propagated
across the forest,
728
00:36:44,076 --> 00:36:48,080
flattening over 800 square miles
of trees.
729
00:36:49,665 --> 00:36:52,834
For over a century,
some scientists have wondered
730
00:36:52,835 --> 00:36:57,335
if the cosmic intruder
was a comet or an asteroid.
731
00:36:58,966 --> 00:37:00,550
- If it were caused
by a comet,
732
00:37:00,551 --> 00:37:02,719
you would imagine you'd find
in the sediment
733
00:37:02,720 --> 00:37:04,888
some record of unusual things,
734
00:37:04,888 --> 00:37:07,974
like a ratio of helium 3
to helium 4.
735
00:37:07,975 --> 00:37:10,978
That could be an indication
that it may have been a comet.
736
00:37:10,978 --> 00:37:12,813
Now, another possibility
is if you find
737
00:37:12,813 --> 00:37:16,149
some strange isotope
buried in a lake somewhere.
738
00:37:16,150 --> 00:37:18,819
That's tough.
This is not easy.
739
00:37:21,238 --> 00:37:22,739
Narrator: While it's
been difficult
740
00:37:22,740 --> 00:37:27,240
to substantiate
cometary impacts on Earth,
741
00:37:27,411 --> 00:37:30,580
physical proof
of their colossal power
742
00:37:30,581 --> 00:37:34,293
exists on
the gas giant planets.
743
00:37:34,293 --> 00:37:38,130
And these dramatic events
warn that far worse collisions
744
00:37:38,130 --> 00:37:40,465
loom in the future,
745
00:37:40,466 --> 00:37:43,969
with Earth as
the potential bull's-eye.
746
00:37:51,769 --> 00:37:55,522
As we have followed the trail
of comets through space,
747
00:37:55,522 --> 00:37:57,315
we have passed through
the chilliest
748
00:37:57,316 --> 00:38:00,819
and warmest places
in our solar system.
749
00:38:00,819 --> 00:38:04,155
We've also investigated
whether these icy bodies
750
00:38:04,156 --> 00:38:08,656
have been deliverers
and destroyers of life.
751
00:38:09,119 --> 00:38:13,619
And new observations prove
many of these ancient bodies
752
00:38:14,833 --> 00:38:18,002
haven't quietly retired
to the frigid outer limits
753
00:38:18,003 --> 00:38:22,007
of our solar system.
754
00:38:22,007 --> 00:38:24,968
- We think there are several
possible end states for comets.
755
00:38:24,968 --> 00:38:28,680
In one case, they can actually
get pulled right into the Sun.
756
00:38:28,680 --> 00:38:30,682
In other cases, they can
actually get scattered
757
00:38:30,682 --> 00:38:32,517
by one of the planets
and kind of get kicked out,
758
00:38:32,518 --> 00:38:35,687
maybe back into the Oort cloud
and never seen again.
759
00:38:35,687 --> 00:38:38,481
And finally they can also
actually impact a planet.
760
00:38:43,654 --> 00:38:47,157
Narrator: We now shuttle back
to July 1994,
761
00:38:50,118 --> 00:38:53,454
We follow a string of
21 comet fragments
762
00:38:53,455 --> 00:38:55,957
called Shoemaker-Levy 9
763
00:38:55,958 --> 00:38:59,461
as they're gravitationally
pulled toward the gas giant
764
00:38:59,461 --> 00:39:01,963
planet Jupiter.
765
00:39:01,964 --> 00:39:03,298
- If we were riding on
766
00:39:03,298 --> 00:39:06,301
one of the fragments of
the comet Shoemaker-Levy 9,
767
00:39:06,301 --> 00:39:08,136
it would have been
truly spectacular
768
00:39:08,136 --> 00:39:10,054
because we're heading
toward Jupiter,
769
00:39:10,055 --> 00:39:13,266
and this giant planet
is looming ever bigger,
770
00:39:13,267 --> 00:39:14,601
and then-splat!
771
00:39:14,601 --> 00:39:16,102
We crash into it.
772
00:39:16,103 --> 00:39:20,603
We throw up a whole bunch
of material from the insides.
773
00:39:21,108 --> 00:39:23,235
It would be really
an amazing journey.
774
00:39:23,235 --> 00:39:26,071
The plumes of material
coming out of Jupiter
775
00:39:26,071 --> 00:39:29,074
were super heated gas
heated by this collision
776
00:39:29,074 --> 00:39:32,577
and also excavated from
the interior of Jupiter.
777
00:39:33,996 --> 00:39:36,999
Narrator. Shoemaker-Levy 9
left impact scars
778
00:39:36,999 --> 00:39:39,334
the size of Earth,
779
00:39:39,334 --> 00:39:41,502
driving home
the scale of violence
780
00:39:41,503 --> 00:39:45,840
that comets can produce
if they slam into our planet.
781
00:39:47,593 --> 00:39:49,928
- If any of those fragments
had hit the Earth
782
00:39:49,928 --> 00:39:53,097
rather than Jupiter, we'd have
been in serious trouble,
783
00:39:53,098 --> 00:39:54,432
because they were large
784
00:39:54,433 --> 00:39:57,185
and they were coming in
extremely rapidly.
785
00:39:57,185 --> 00:39:58,769
But fortunately,
big brother Jupiter
786
00:39:58,770 --> 00:40:01,439
took all the hits for us
and didn't seem to suffer much
787
00:40:01,440 --> 00:40:03,775
in the way of damage.
788
00:40:03,775 --> 00:40:05,610
Narrator: But even with
Jupiter acting
789
00:40:05,611 --> 00:40:07,613
as a planetary shield,
790
00:40:07,613 --> 00:40:10,449
comets still
sneak by the gas giants
791
00:40:10,449 --> 00:40:14,286
and have close encounters
with Earth.
792
00:40:14,286 --> 00:40:15,620
- The good news is,
793
00:40:15,621 --> 00:40:18,457
asteroid impacts are far more
likely to occur
794
00:40:18,457 --> 00:40:22,127
because asteroids
outnumber comets 100 to 1
795
00:40:22,127 --> 00:40:23,628
in near-Earth space.
796
00:40:23,629 --> 00:40:25,797
The bad news is,
if we do find a comet
797
00:40:25,797 --> 00:40:27,757
on an Earth-impacting
trajectory,
798
00:40:27,758 --> 00:40:29,593
we wouldn't realize it
799
00:40:29,593 --> 00:40:31,928
till it got inside
the orbit of Jupiter,
800
00:40:31,929 --> 00:40:35,599
when it started throwing off
gas and dust.
801
00:40:35,599 --> 00:40:37,767
- In the very unlikely event
that a comet
802
00:40:37,768 --> 00:40:39,936
could get close to the Earth,
you would worry about it
803
00:40:39,937 --> 00:40:42,105
because they tend to have
high average velocities
804
00:40:42,105 --> 00:40:43,606
relative to an asteroid,
805
00:40:43,607 --> 00:40:46,026
as high as tens of miles
a second.
806
00:40:46,026 --> 00:40:49,362
So in other words, they would
pack a bigger punch.
807
00:40:49,363 --> 00:40:51,865
Narrator: While the frequency
of near-Earth asteroids
808
00:40:51,865 --> 00:40:54,492
heightens
the risk of impacts,
809
00:40:54,493 --> 00:40:58,205
the speed of comets
is equally troubling.
810
00:40:58,205 --> 00:41:00,373
This sobering fact
has prompted
811
00:41:00,374 --> 00:41:04,086
viewer Robin W. from Boulder,
Colorado, to...
812
00:41:12,427 --> 00:41:14,429
- Robin,
that's an important question.
813
00:41:14,429 --> 00:41:16,264
The asteroids
are more numerous,
814
00:41:16,264 --> 00:41:18,182
so there's more of them
that could hit us.
815
00:41:18,183 --> 00:41:20,685
But we can track
their trajectories
816
00:41:20,686 --> 00:41:23,689
and maybe do something about
one that's gonna hit us,
817
00:41:23,689 --> 00:41:25,691
deflect it for example.
818
00:41:25,691 --> 00:41:27,693
The comets are more rare,
819
00:41:27,693 --> 00:41:30,696
but we have very little warning
when they come in.
820
00:41:30,696 --> 00:41:33,699
And also, they move much faster
than asteroids,
821
00:41:33,699 --> 00:41:36,868
so there's more energy
impacting Earth.
822
00:41:36,868 --> 00:41:40,037
So I would say comets are
the most hazardous objects.
823
00:41:43,709 --> 00:41:47,379
Narrator: NASA is taking
the threat of comets seriously.
824
00:41:47,379 --> 00:41:49,547
So far, tracking satellites
825
00:41:49,548 --> 00:41:52,884
have tagged 84
near-Earth comets,
826
00:41:52,884 --> 00:41:56,554
objects with orbits that
come within 28 million miles
827
00:41:56,555 --> 00:41:59,891
of Earth's path
around the Sun.
828
00:41:59,891 --> 00:42:01,559
- There are no periodic comets
829
00:42:01,560 --> 00:42:04,229
that currently have Earth's name
written on them.
830
00:42:04,229 --> 00:42:06,397
But Jupiter
and the other giant planets
831
00:42:06,398 --> 00:42:09,067
occasionally perturb
the orbits of comets.
832
00:42:09,067 --> 00:42:11,694
So there could be
a periodic comet in the future
833
00:42:11,695 --> 00:42:14,864
that will collide
with Earth.
834
00:42:22,581 --> 00:42:25,584
Narrator: Since the beginning
of recorded history,
835
00:42:25,584 --> 00:42:29,588
over 4,200 comets
have been observed,
836
00:42:29,588 --> 00:42:34,088
a mere fraction of the total
number of these icy bodies.
837
00:42:34,426 --> 00:42:37,595
This means billions
of unknown comets
838
00:42:37,596 --> 00:42:42,096
still lie in wait
in the outer reaches of space.
839
00:42:42,100 --> 00:42:46,437
One day, a doomsday comet
could be nudged out
840
00:42:46,438 --> 00:42:49,274
and sent on a collision course
with Earth.
841
00:42:51,485 --> 00:42:54,321
- If we're on
that cosmic highway,
842
00:42:54,321 --> 00:42:57,157
and it's getting
into our on-ramp,
843
00:42:57,157 --> 00:42:58,658
we need to worry about it.
844
00:42:58,658 --> 00:43:01,661
And we need to worry about it
with very little lead time.
845
00:43:01,661 --> 00:43:03,954
- There is very little
we can do,
846
00:43:03,955 --> 00:43:06,123
other than sending
a giant bomb toward them
847
00:43:06,124 --> 00:43:07,458
and trying to deflect them.
848
00:43:07,459 --> 00:43:08,960
But that's very difficult
849
00:43:08,960 --> 00:43:10,586
when there's only
a few months' warning.
850
00:43:12,631 --> 00:43:15,467
Narrator: Just as comets
have inspired awe and fear
851
00:43:15,467 --> 00:43:18,636
among our ancestors,
852
00:43:18,637 --> 00:43:21,806
they remain a force
to reckon with.
853
00:43:21,807 --> 00:43:25,435
By continuing to track
their tails of dust,
854
00:43:25,435 --> 00:43:29,439
we may uncover more clues
about these frozen artifacts
855
00:43:29,439 --> 00:43:32,650
of our ancient past.
856
00:43:32,651 --> 00:43:34,653
- It's pretty remarkable
if you think about it.
857
00:43:34,653 --> 00:43:37,656
Just a few hundred years ago,
we had no idea what they were.
858
00:43:37,656 --> 00:43:39,157
We had no idea
what they meant.
859
00:43:39,157 --> 00:43:41,659
And now we've actually been
to the surfaces of comets.
860
00:43:41,660 --> 00:43:44,037
We've seen up close and personal
what they're really like
861
00:43:44,037 --> 00:43:45,496
and what they're made out of.
862
00:43:45,497 --> 00:43:48,166
So these mysterious objects
have meant a lot to humans
863
00:43:48,166 --> 00:43:49,333
throughout our history.
864
00:43:49,334 --> 00:43:51,210
They've been agents of change.
865
00:43:51,211 --> 00:43:54,714
They've been agents
of destruction sometimes.
866
00:43:54,714 --> 00:43:57,049
They've maybe been agents
of creation.
68801
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