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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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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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They've been agents
of destruction.
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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 rendevous
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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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ln 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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narrator: We're going
to hitch a ride
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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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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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That's sort of like the glue
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that holds
all these little pebbles
55
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and particles of dust
together.
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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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lf 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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I
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,
disklike 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
Iooking like a dark asteroid.
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Nothing much is happening.
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lt 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,
139
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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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lt 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 1 OO 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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lt'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,
189
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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,
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so it goes zoom,
like that,
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like being propelled
200
00:10:00,183 --> 00:10:02,084
at the bottom
of a giant roller coaster.
201
00:10:02,117 --> 00:10:05,753
A roller coaster
starts out high, very slowly,
202
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picks up speed
due to the gravity,
203
00:10:07,953 --> 00:10:10,088
goes zooming past the bottom,
204
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and then slows down again
on its outward journey.
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- Eventually, as our comet
Ieaves the vicinity of the Sun,
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it's going to travel
back out
207
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into the far reaches
of the solar system.
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Everything's going
to quiet down.
209
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All of the gas and dust
is going to settle
210
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back onto its surface.
211
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And eventually, it'll cruise
away into the quiet dark.
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narrator: Back in the cold
region of the scattered disc,
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a comet transforms
214
00:10:36,496 --> 00:10:39,799
back into a dull, black lump
of rock and ice
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00:10:39,831 --> 00:10:43,668
until it makes its journey
around the Sun once again.
216
00:10:47,000 --> 00:10:50,636
Haley, the most famous
short-period comet,
217
00:10:50,668 --> 00:10:53,637
was first recorded
in 240 B.C.
218
00:10:53,669 --> 00:10:57,806
and has passed by Earth
every 76 years.
219
00:10:57,837 --> 00:11:00,639
Estimated to be the size
of Manhattan,
220
00:11:00,672 --> 00:11:03,641
this superstar comet
is sometimes so bright,
221
00:11:03,673 --> 00:11:06,842
it has been seen
in broad daylight.
222
00:11:06,874 --> 00:11:09,176
Throughout history,
223
00:11:09,208 --> 00:11:12,678
the appearance of Haley
has inspired awe and dread
224
00:11:12,710 --> 00:11:15,345
among earthly observers.
225
00:11:15,377 --> 00:11:18,012
- In 1910, it was feared,
226
00:11:18,045 --> 00:11:20,847
because spectroscopy
had just been introduced,
227
00:11:20,879 --> 00:11:24,515
and they had determined
that comets contain cyanogen,
228
00:11:24,547 --> 00:11:27,516
which is an odorless
and poisonous gas,
229
00:11:27,549 --> 00:11:30,184
and so astronomers predicted
that there'd be problems
230
00:11:30,216 --> 00:11:32,351
because of this poisonous gas
sweeping the Earth,
231
00:11:32,383 --> 00:11:35,519
and so there were actually
comet pills manufactured.
232
00:11:35,551 --> 00:11:38,553
Life insurance policies
on the comet were taken out.
233
00:11:41,020 --> 00:11:42,988
narrator: While comets
have been thought to be
234
00:11:43,021 --> 00:11:45,456
extraterrestrial
harbingers of doom,
235
00:11:45,488 --> 00:11:49,124
astronomers have long wondered
if these glowing rocks
236
00:11:49,156 --> 00:11:53,159
contain precious information
about our past.
237
00:11:55,525 --> 00:11:58,995
By the 21st century,
NASA was ready to ignite
238
00:11:59,026 --> 00:12:03,663
a bold offensive strike,
one that would hopefully expose
239
00:12:03,694 --> 00:12:07,831
one of the holy grails
of planetary science.
240
00:12:07,863 --> 00:12:10,498
Could these
interplanetary vagabonds
241
00:12:10,530 --> 00:12:14,367
have been the cosmic
transporters of life?
242
00:12:19,867 --> 00:12:22,836
So far, we've traveled
with comets
243
00:12:22,868 --> 00:12:25,170
from the frozen hinterlands
of the Kuiper belt
244
00:12:25,203 --> 00:12:26,938
and scattered disc
245
00:12:26,970 --> 00:12:30,673
to an exhilarating orbit
around the Sun.
246
00:12:30,704 --> 00:12:33,339
We've watched these dark bodies
come alive
247
00:12:33,373 --> 00:12:37,176
as they formed brilliant comas
and tails.
248
00:12:37,207 --> 00:12:39,342
But scientists
are still puzzled
249
00:12:39,375 --> 00:12:44,046
about what's really inside
these cosmic interlopers.
250
00:12:45,310 --> 00:12:46,444
- Man, l wish l knew
251
00:12:46,477 --> 00:12:48,045
what the interior of a comet
Iooked like.
252
00:12:48,077 --> 00:12:49,211
You would love to be able
253
00:12:49,244 --> 00:12:52,213
to look inside
the nucleus of a comet,
254
00:12:52,246 --> 00:12:55,549
to see if it's clumpy,
if it's uniform.
255
00:12:55,580 --> 00:12:57,048
ls there crystalline ice?
256
00:12:57,080 --> 00:12:58,614
ls there glassy ice?
257
00:13:04,684 --> 00:13:06,318
narrator:
Our protective spacecraft
258
00:13:06,351 --> 00:13:09,320
time-travels back to 2005
259
00:13:09,352 --> 00:13:13,155
and meets up with NASA's
Deep Impact space probe
260
00:13:13,186 --> 00:13:16,155
on a comet-hunting mission.
261
00:13:16,187 --> 00:13:20,658
lt zeroes in on a short-period
comet named Tempel 1
262
00:13:20,689 --> 00:13:23,191
with an aggressive
plan of attack.
263
00:13:26,025 --> 00:13:29,328
We hover at a safe distance
as Deep Impact
264
00:13:29,359 --> 00:13:33,529
launches an 800-pound projectile
into the passing comet.
265
00:13:36,561 --> 00:13:39,697
Debris sprays out
for thousands of miles
266
00:13:39,729 --> 00:13:42,364
as the impactor
excavates a crater
267
00:13:42,398 --> 00:13:48,203
and sends tons of blinding gas,
rocks, and dust into space.
268
00:13:48,233 --> 00:13:50,368
For the first time
in history,
269
00:13:50,400 --> 00:13:53,202
scientists are able
to peer inside
270
00:13:53,235 --> 00:13:57,539
the icy, muddy interior
of a comet.
271
00:13:57,569 --> 00:13:59,137
- Right after the impact,
272
00:13:59,170 --> 00:14:02,139
you could see silicate grains
fluorescing and glowing.
273
00:14:02,171 --> 00:14:05,474
This tells us that comets
are very primitive material
274
00:14:05,506 --> 00:14:08,642
and that they pretty much
do preserve in pristine state
275
00:14:08,674 --> 00:14:10,142
the materials that we find
276
00:14:10,174 --> 00:14:12,643
in the youngest
star-forming systems.
277
00:14:12,675 --> 00:14:14,810
So indeed,
they really are time capsules
278
00:14:14,842 --> 00:14:16,977
that let us look back
on our own solar system
279
00:14:17,009 --> 00:14:19,010
at the very beginning.
280
00:14:21,478 --> 00:14:22,779
narrator: While Deep Impact
281
00:14:22,812 --> 00:14:26,282
captures a rare glimpse
of a comet's interior
282
00:14:26,314 --> 00:14:29,950
it is unable to snap
clear images of the crater,
283
00:14:29,981 --> 00:14:33,984
which was obscured by
an enormous plume of debris.
284
00:14:36,750 --> 00:14:40,220
ln February 201 1,
another spacecraft,
285
00:14:40,252 --> 00:14:41,886
named Stardust-NExT,
286
00:14:41,919 --> 00:14:43,720
catches up to Tempel 1
287
00:14:43,752 --> 00:14:47,422
as it completes its five-year
orbit around the Sun.
288
00:14:49,555 --> 00:14:52,357
To everyone's surprise,
289
00:14:52,389 --> 00:14:56,025
the impact crater is much
smaller than had been expected
290
00:14:56,058 --> 00:15:00,362
from the historic smash-up that
occurred five years earlier.
291
00:15:00,392 --> 00:15:02,193
- Amazing...
292
00:15:02,226 --> 00:15:04,528
But the crater looked like
it was small.
293
00:15:04,560 --> 00:15:06,361
So this now creates
this issue:
294
00:15:06,394 --> 00:15:08,195
Was the crater always small?
295
00:15:08,228 --> 00:15:12,198
We know the crater
isn't what we expected.
296
00:15:12,229 --> 00:15:14,030
So we're going
to do some experiments
297
00:15:14,064 --> 00:15:17,801
to see if we can explain why
the crater looks like it does.
298
00:15:17,832 --> 00:15:20,534
- Sunlamp's coming on.
299
00:15:20,566 --> 00:15:23,535
- Can we move it up a bit?
300
00:15:23,567 --> 00:15:26,403
narrator: At NASA's
Ames Vertical Gun Range,
301
00:15:26,435 --> 00:15:29,571
Stardust-NExT
coinvestigator Pete Schultz
302
00:15:29,602 --> 00:15:33,072
is conducting high-velocity
impact experiments
303
00:15:33,104 --> 00:15:38,175
to find out why Deep Impact
produced such a tiny crater.
304
00:15:38,206 --> 00:15:40,007
He will use a massive
305
00:15:40,040 --> 00:15:43,176
.30-caliber high-velocity
gas gun
306
00:15:43,207 --> 00:15:47,010
to fire tiny projectile beads
at various targets
307
00:15:47,042 --> 00:15:49,878
located inside
a vacuum chamber.
308
00:15:54,244 --> 00:15:56,713
- We're trying to simulate
309
00:15:56,746 --> 00:16:00,316
what the nature of the surface
of comet 9P/Tempel 1 is like,
310
00:16:00,348 --> 00:16:02,149
so we're putting in perlite,
311
00:16:02,181 --> 00:16:03,815
which is this low-density
material
312
00:16:03,848 --> 00:16:05,149
that you find in gardens,
313
00:16:05,182 --> 00:16:07,250
then we're adding in
hollow microspheres,
314
00:16:07,283 --> 00:16:11,387
and this also resemble what
the nature of the comet is like.
315
00:16:11,417 --> 00:16:14,386
The purpose of the experiment
is to see what happens
316
00:16:14,419 --> 00:16:16,220
to the crater
after formation.
317
00:16:16,252 --> 00:16:18,354
Does it stay there?
Does it collapse?
318
00:16:18,387 --> 00:16:20,856
With this experiment,
we should be able to find out.
319
00:16:22,122 --> 00:16:23,590
Okay, l'm out of the tank.
320
00:16:23,622 --> 00:16:25,256
Lock and load.
321
00:16:25,290 --> 00:16:26,591
narrator: High-speed cameras
322
00:16:26,623 --> 00:16:28,925
mounted around
the vacuum chamber
323
00:16:28,957 --> 00:16:30,892
will document the impact.
324
00:16:30,925 --> 00:16:32,526
- We've got this one covered.
325
00:16:32,559 --> 00:16:35,695
We just have to hit
the target.
326
00:16:35,727 --> 00:16:36,861
Okay.
327
00:16:36,893 --> 00:16:38,361
[claps hands]
328
00:16:38,394 --> 00:16:40,129
Let's shoot this puppy.
329
00:16:40,161 --> 00:16:41,462
J.P., are you ready?
330
00:16:41,495 --> 00:16:42,662
- Yeah.
331
00:16:44,163 --> 00:16:47,566
narrator: As the crew anxiously
awaits in the control room,
332
00:16:47,597 --> 00:16:51,434
Pete mixes science
with a little superstition.
333
00:16:51,466 --> 00:16:52,767
- There's always a risk.
334
00:16:52,799 --> 00:16:55,835
Sometimes you miss.
Sometimes you hit.
335
00:17:00,068 --> 00:17:01,669
- Whoa!
336
00:17:01,702 --> 00:17:02,869
- Oh, sweet.
337
00:17:02,903 --> 00:17:05,538
The whole thing sort of
collapses in on itself.
338
00:17:05,571 --> 00:17:06,905
lt's getting smaller now.
339
00:17:06,938 --> 00:17:09,073
lt was bigger.
Now it's getting smaller.
340
00:17:09,106 --> 00:17:12,909
So what we see here is that
there's a lot of dust and ejecta
341
00:17:12,940 --> 00:17:15,742
sent upwards,
and that blocked the view.
342
00:17:15,774 --> 00:17:18,076
We couldn't see
the crater forming.
343
00:17:18,109 --> 00:17:20,311
So what started off
being a nice-looking crater,
344
00:17:20,343 --> 00:17:21,811
it just doesn't stay there.
345
00:17:21,844 --> 00:17:23,278
lt just simply heals itself.
346
00:17:23,311 --> 00:17:26,781
So what may have happened
for 9P/Tempel 1 ,
347
00:17:26,811 --> 00:17:30,614
the nucleus, is that
that crater healed itself.
348
00:17:30,646 --> 00:17:33,782
The nucleus healed itself
from the scar created
349
00:17:33,814 --> 00:17:36,049
by us with Deep Impact.
350
00:17:36,082 --> 00:17:38,083
Let's see what we did.
351
00:17:41,150 --> 00:17:43,218
[groans]
352
00:17:43,251 --> 00:17:45,152
So the results
were fantastic.
353
00:17:45,185 --> 00:17:47,820
We got to see
just what we planned to.
354
00:17:47,853 --> 00:17:49,487
There may be more
to the story,
355
00:17:49,520 --> 00:17:53,156
so we're going to try
a different experiment as well.
356
00:17:53,188 --> 00:17:54,822
narrator: Pete has a hunch
357
00:17:54,856 --> 00:17:58,492
there's a missing piece
to the Deep Impact mission.
358
00:17:58,523 --> 00:18:00,992
He now wants to see
if the space probe
359
00:18:01,024 --> 00:18:04,660
created a different type
of crater on Tempel 1 ,
360
00:18:04,692 --> 00:18:08,829
due to the makeup
of the comet's nucleus.
361
00:18:08,861 --> 00:18:10,829
- So this time,
we're going to put
362
00:18:10,861 --> 00:18:15,999
a denser layer
below that perlite,
363
00:18:16,029 --> 00:18:17,830
so we want to find out
whether or not
364
00:18:17,864 --> 00:18:19,332
we'll get a different type
of crater
365
00:18:19,364 --> 00:18:21,833
if we have two different types
of material:
366
00:18:21,865 --> 00:18:23,700
one very soft on top
367
00:18:23,732 --> 00:18:27,702
and one denser
on the bottom.
368
00:18:27,734 --> 00:18:30,470
narrator: Pete and his crew
return to the control room
369
00:18:30,502 --> 00:18:33,304
to see what happens
to the new target of perlite
370
00:18:33,336 --> 00:18:36,172
poured over a heavier layer
of sand.
371
00:18:40,372 --> 00:18:41,506
[small explosion]
372
00:18:41,539 --> 00:18:43,173
- [laughs]
373
00:18:43,206 --> 00:18:46,542
Now, that formed a big crater
in the perlite.
374
00:18:46,574 --> 00:18:49,043
Boy, look at that.
375
00:18:49,075 --> 00:18:52,711
Oh, oh, man,
that is gorgeous.
376
00:18:52,743 --> 00:18:54,377
Okay.
377
00:18:54,411 --> 00:18:56,246
The projectile went deep,
378
00:18:56,277 --> 00:18:59,079
and now the stuff
is coming back out that hole,
379
00:18:59,112 --> 00:19:02,281
while, on the surface,
it's excavating debris.
380
00:19:04,280 --> 00:19:05,581
Pow!
Okay.
381
00:19:05,614 --> 00:19:07,916
narrator: The double-layered
target created not one
382
00:19:07,948 --> 00:19:09,783
but two craters,
383
00:19:09,816 --> 00:19:14,453
a small crater inside
a larger, shallower crater.
384
00:19:14,484 --> 00:19:18,054
- This could be what happened
for 9P/Tempel 1.
385
00:19:18,085 --> 00:19:20,887
lt went so deep
into the nucleus,
386
00:19:20,920 --> 00:19:24,223
and then itjust simply
collapses away,
387
00:19:24,255 --> 00:19:27,057
and we're left with just
this very, very faint rim
388
00:19:27,089 --> 00:19:30,158
on the outside with
a small pit in the center.
389
00:19:30,190 --> 00:19:32,492
narrator:
These impact experiments
390
00:19:32,524 --> 00:19:36,661
yield surprising clues about
the interior of Tempel 1
391
00:19:36,692 --> 00:19:39,661
and perhaps all comets.
392
00:19:39,693 --> 00:19:42,162
- Now we know that comets
have history.
393
00:19:42,194 --> 00:19:43,828
We see layers.
394
00:19:43,861 --> 00:19:45,829
l don't know if these layers
go all the way
395
00:19:45,862 --> 00:19:47,830
through the nucleus,
396
00:19:47,862 --> 00:19:50,531
or are they only
in one part?
397
00:19:51,697 --> 00:19:53,165
narrator:
Unraveling the secrets
398
00:19:53,198 --> 00:19:56,501
of what's inside comets
will help scientists understand
399
00:19:56,533 --> 00:20:00,536
what causes them to exhibit
some really bizarre behavior.
400
00:20:07,270 --> 00:20:11,073
Our spaceship now shadows
NASA's EPOXl mission
401
00:20:11,105 --> 00:20:13,307
as it encounters Hartley 2,
402
00:20:13,338 --> 00:20:16,974
a fast-spinning comet
that tumbles through space
403
00:20:17,007 --> 00:20:20,810
like a hyperactive
cosmic peanut.
404
00:20:20,841 --> 00:20:22,475
- Hartley 2
is a smaller comet.
405
00:20:22,508 --> 00:20:24,309
lt's only about a mile or so
aCrOSS,
406
00:20:24,342 --> 00:20:26,977
and so it's kind of a surprise
that it's so active.
407
00:20:27,010 --> 00:20:28,311
lt's putting off huge amounts
408
00:20:28,344 --> 00:20:30,813
of C02 and, actually,
cyanide gas.
409
00:20:30,845 --> 00:20:31,979
And the question is,
410
00:20:32,012 --> 00:20:33,480
are all small comets
active like this
411
00:20:33,512 --> 00:20:34,512
or only a few?
412
00:20:34,547 --> 00:20:36,548
And what makes them
so active?
413
00:20:38,848 --> 00:20:41,317
l've got a peanut-shaped
plastic bottle here
414
00:20:41,348 --> 00:20:43,817
that's supposed to represent
comet Hartley 2.
415
00:20:43,850 --> 00:20:45,651
lt's full of dry ice
and warm water
416
00:20:45,684 --> 00:20:46,985
and as you can see,
417
00:20:47,018 --> 00:20:49,320
as the warm water starts to make
the dry ice sublimate,
418
00:20:49,351 --> 00:20:50,985
it shoots out these jets
419
00:20:51,019 --> 00:20:52,820
through the holes that
we've got poked in the bottle.
420
00:20:52,853 --> 00:20:54,321
lf l drop it into the water,
421
00:20:54,353 --> 00:20:56,655
instead of holding it
fixed in space,
422
00:20:56,688 --> 00:20:58,322
you can see that the jets
actually start
423
00:20:58,355 --> 00:20:59,656
pushing the bottle around,
424
00:20:59,689 --> 00:21:01,957
causing the comet's
rotational state to change.
425
00:21:01,989 --> 00:21:03,623
This is very similar
to what's going on
426
00:21:03,657 --> 00:21:05,358
on the surface
of comet Hartley 2.
427
00:21:05,391 --> 00:21:08,527
The C02 jets are actually
changing the rotational state
428
00:21:08,559 --> 00:21:12,229
of the comet, causing it
to speed up and slow down.
429
00:21:14,260 --> 00:21:16,295
narrator:
When tracking Hartley 2,
430
00:21:16,328 --> 00:21:20,131
our spacecraft gets caught
in a cosmic blizzard
431
00:21:20,163 --> 00:21:23,299
as the spastic comet
burps and belches out
432
00:21:23,331 --> 00:21:29,637
a trail of frozen snowballs that
extend for millions of miles.
433
00:21:29,667 --> 00:21:31,635
- One of the big surprises
about Hartley 2
434
00:21:31,667 --> 00:21:35,837
is that it was surrounded
by this posse of mini comets.
435
00:21:35,869 --> 00:21:39,005
This is simply ices
that are coming off,
436
00:21:39,037 --> 00:21:41,672
about the size of a snowball
all the way up to a basketball.
437
00:21:41,704 --> 00:21:45,841
narrator: Scientists suspect
the snowball-sized debris
438
00:21:45,872 --> 00:21:48,841
rains back down on Hartley 2,
439
00:21:48,873 --> 00:21:54,678
producing its unusual landscape
of craters and towering spires.
440
00:21:54,709 --> 00:21:57,011
- Because these comets
have very little gravities,
441
00:21:57,043 --> 00:21:59,044
most of the gas
is blown out into space,
442
00:21:59,077 --> 00:22:01,879
but a very small fraction
can actually redeposit
443
00:22:01,911 --> 00:22:04,713
on the surface, generating
very smooth textures,
444
00:22:04,745 --> 00:22:07,214
and on other locations,
generating these very bumpy
445
00:22:07,247 --> 00:22:09,349
or spire-like texture.
446
00:22:09,380 --> 00:22:11,181
narrator: From Hartley 2,
447
00:22:11,215 --> 00:22:15,586
we blast off to the extreme
outer edge of our solar system,
448
00:22:15,616 --> 00:22:18,251
a vast, eerie place,
449
00:22:18,284 --> 00:22:21,687
barely within the gravitational
grasp of our Sun
450
00:22:21,718 --> 00:22:26,522
and impossible to see,
even with modern telescopes.
451
00:22:26,553 --> 00:22:31,024
Here, we come upon the largest
and perhaps most elusive
452
00:22:31,055 --> 00:22:34,892
icy bodies in
our galactic neighborhood.
453
00:22:43,193 --> 00:22:46,162
Our journey through
the fascinating world of comets
454
00:22:46,194 --> 00:22:49,997
has provided us a ringside seat
to some of the greatest
455
00:22:50,028 --> 00:22:54,365
cosmic shows observed
from Earth and space.
456
00:22:58,732 --> 00:23:01,201
We now change course
and travel
457
00:23:01,233 --> 00:23:05,704
over 50,OOO times the distance
between Earth and the Sun
458
00:23:05,734 --> 00:23:10,705
to the outermost edge
of our solar system.
459
00:23:10,736 --> 00:23:13,038
We arrive at the Oort cloud,
460
00:23:13,071 --> 00:23:16,007
an even larger fraternity
of comets,
461
00:23:16,038 --> 00:23:20,175
perhaps over a trillion
of them.
462
00:23:20,206 --> 00:23:21,840
- If we'd actually
got in a spaceship
463
00:23:21,874 --> 00:23:25,010
and tried to go out and, say,
visit the Oort cloud,
464
00:23:25,041 --> 00:23:27,376
this would have been
a long journey.
465
00:23:27,408 --> 00:23:31,545
There's billions and billions
of these objects,
466
00:23:31,577 --> 00:23:34,246
and there's a lot of space
in between them.
467
00:23:36,079 --> 00:23:39,382
narrator: Like the Kuiper belt
and scattered disc,
468
00:23:39,413 --> 00:23:43,383
the Oort cloud objects may
have formed closer to the Sun,
469
00:23:43,414 --> 00:23:45,549
but about 800 million years
470
00:23:45,582 --> 00:23:48,184
after the solar system
was formed,
471
00:23:48,216 --> 00:23:52,186
the gravitational influence
of the gas giant planets
472
00:23:52,218 --> 00:23:53,519
flung these comets
473
00:23:53,552 --> 00:23:56,554
out to the frigid edge
of our solar system.
474
00:23:57,987 --> 00:23:59,455
- Some of these objects
were flung
475
00:23:59,487 --> 00:24:01,455
into very highly elliptical
orbits
476
00:24:01,488 --> 00:24:03,122
out into the Oort cloud.
477
00:24:03,155 --> 00:24:05,290
Passing stars could
circularize those orbits,
478
00:24:05,322 --> 00:24:08,958
making somewhat stable orbits
for them.
479
00:24:08,991 --> 00:24:10,625
narrator: Most of
the Oort cloud bodies
480
00:24:10,658 --> 00:24:12,459
have been
in frozen hibernation
481
00:24:12,492 --> 00:24:15,962
since the birth
of our solar system.
482
00:24:15,993 --> 00:24:18,628
They only become
Iong-period comets
483
00:24:18,661 --> 00:24:20,295
when they get sucked
into orbits
484
00:24:20,328 --> 00:24:25,800
that carry them inward towards
the planets and the Sun.
485
00:24:25,830 --> 00:24:27,965
Scientists have never
actually captured
486
00:24:27,998 --> 00:24:30,133
an image of the Oort cloud,
487
00:24:30,164 --> 00:24:33,800
but they have good reason
to believe it's there.
488
00:24:33,833 --> 00:24:36,302
- Even though scientists can't
directly observe the Oort cloud
489
00:24:36,333 --> 00:24:38,802
because it's so far away
and so faint,
490
00:24:38,835 --> 00:24:41,137
what they are able to do
is infer its existence
491
00:24:41,168 --> 00:24:42,636
because we can look at
492
00:24:42,669 --> 00:24:45,638
where all these long-period
comets come from on the sky,
493
00:24:45,671 --> 00:24:47,806
and they seem to come
from all different directions.
494
00:24:47,838 --> 00:24:50,473
There doesn't really seem to be
a preferred direction for them.
495
00:24:50,505 --> 00:24:52,306
This suggests that
the Oort cloud,
496
00:24:52,339 --> 00:24:55,175
if it exists,
is probably roughly spherical.
497
00:24:57,208 --> 00:24:59,076
narrator:
One of the big mysteries
498
00:24:59,109 --> 00:25:02,579
is what knocks these icy bodies
off course
499
00:25:02,610 --> 00:25:06,914
and sends them cruising
by our neighborhood of Earth.
500
00:25:06,945 --> 00:25:09,580
- The comets in the Oort cloud
are very susceptible
501
00:25:09,612 --> 00:25:12,081
to gravitational pulls
from other things
502
00:25:12,114 --> 00:25:13,748
outside the solar system.
503
00:25:13,781 --> 00:25:15,749
One thing is passing stars.
504
00:25:15,781 --> 00:25:18,850
lf a star happens to come
close to our Sun,
505
00:25:18,882 --> 00:25:22,719
it can scatter comets
from the outer Oort cloud.
506
00:25:24,184 --> 00:25:27,320
- Icy objects in the Oort cloud
can also be dislodged
507
00:25:27,352 --> 00:25:29,854
by gravitational perturbations
that occur
508
00:25:29,886 --> 00:25:32,888
when the solar system goes
through the plane of our galaxy.
509
00:25:32,921 --> 00:25:34,555
So the solar system
is basically orbiting
510
00:25:34,588 --> 00:25:36,056
around the center
of our galaxy,
511
00:25:36,088 --> 00:25:38,223
but it's also oscillating
up and down,
512
00:25:38,256 --> 00:25:40,057
and when it goes
through the plane,
513
00:25:40,090 --> 00:25:43,059
then gravitational interactions
can perturb objects
514
00:25:43,091 --> 00:25:47,395
from the Oort cloud
into the inner solar system.
515
00:25:47,426 --> 00:25:49,227
narrator:
Some long-period comets
516
00:25:49,260 --> 00:25:51,729
take up to about
30 million years
517
00:25:51,761 --> 00:25:55,431
to complete one round trip
around the Sun.
518
00:25:58,630 --> 00:26:01,099
Our spacecraft
tracks a long-period comet
519
00:26:01,131 --> 00:26:03,600
for hundreds of thousands
of miles
520
00:26:03,632 --> 00:26:06,634
until we approach
planet Earth.
521
00:26:07,700 --> 00:26:09,835
As its icy tails unfurl,
522
00:26:09,868 --> 00:26:12,170
a layer of dust and ice
zips through
523
00:26:12,201 --> 00:26:14,503
our planet's
thin atmosphere,
524
00:26:14,536 --> 00:26:18,373
leaving visible trails
known as a meteor shower.
525
00:26:21,005 --> 00:26:22,306
- l like to think of comets
526
00:26:22,339 --> 00:26:24,274
as sort of the pigpens
of the solar system,
527
00:26:24,307 --> 00:26:26,108
because, as they orbit
around the Sun,
528
00:26:26,140 --> 00:26:28,342
they leave a big, messy trail
of debris.
529
00:26:28,374 --> 00:26:30,509
But sometimes the Earth's orbit
can intersect
530
00:26:30,542 --> 00:26:32,343
some of these dust bands,
531
00:26:32,375 --> 00:26:35,578
and when it does, we can
sometimes see meteor showers.
532
00:26:35,610 --> 00:26:37,411
Those beautiful bright streaks
of light
533
00:26:37,444 --> 00:26:39,078
that you see coming through
the night sky
534
00:26:39,111 --> 00:26:40,579
are actually produced
by particles
535
00:26:40,612 --> 00:26:43,281
that are most often no bigger
than a sand grain.
536
00:26:45,113 --> 00:26:47,748
narrator: While long-
and short-period comets
537
00:26:47,782 --> 00:26:51,185
make up the bulk of comets
that have been observed,
538
00:26:51,215 --> 00:26:55,018
new evidence suggests
that not all icy bodies
539
00:26:55,051 --> 00:26:59,355
come from the subzero suburbs
of our solar system.
540
00:26:59,385 --> 00:27:01,687
Some have secretly
taken up residence
541
00:27:01,720 --> 00:27:04,722
in a much warmer
neighborhood.
542
00:27:08,789 --> 00:27:11,591
Scientists have now
discovered
543
00:27:11,623 --> 00:27:14,759
there are comets masquerading
as asteroids
544
00:27:14,791 --> 00:27:16,759
I
in the asteroid belt
545
00:27:16,792 --> 00:27:19,794
located between
Jupiter and Mars.
546
00:27:22,328 --> 00:27:24,129
- The only reason
that we've discovered
547
00:27:24,161 --> 00:27:27,631
these main-belt comets
is because, occasionally,
548
00:27:27,662 --> 00:27:31,632
the warming rays of the Sun
get into the interior,
549
00:27:31,664 --> 00:27:33,132
vaporize the ices,
550
00:27:33,165 --> 00:27:36,301
and so the comet just
bursts forth for a while,
551
00:27:36,333 --> 00:27:41,971
and then they go back to being
inactive objects or asteroids.
552
00:27:42,001 --> 00:27:44,636
- Scientists used to think that
there were strong distinctions
553
00:27:44,668 --> 00:27:46,469
between asteroids and comets
554
00:27:46,502 --> 00:27:49,004
and that they were two totally
different types of objects,
555
00:27:49,037 --> 00:27:50,838
but what we're
finding nowadays is,
556
00:27:50,870 --> 00:27:53,672
there are some asteroids
that have comet-like properties,
557
00:27:53,706 --> 00:27:56,008
and there are some comets
that eventually kind of look
558
00:27:56,039 --> 00:27:58,040
like asteroids.
559
00:28:01,041 --> 00:28:03,676
narrator: Some scientists
think main-belt comets
560
00:28:03,709 --> 00:28:06,711
may have delivered water
to early Earth
561
00:28:06,743 --> 00:28:09,745
and the materials
to create life.
562
00:28:12,079 --> 00:28:15,315
We blast back
to January 2004
563
00:28:15,347 --> 00:28:18,817
and follow NASA's
Stardust spacecraft
564
00:28:18,848 --> 00:28:21,150
on an unprecedented mission
565
00:28:21,182 --> 00:28:24,818
to collect pure comet dust
in space.
566
00:28:24,850 --> 00:28:28,553
Just beyond the planet Mars,
567
00:28:28,584 --> 00:28:32,220
we meet up with
a comet named Wild 2.
568
00:28:32,252 --> 00:28:35,054
Upon approaching
its enormous coma,
569
00:28:35,087 --> 00:28:38,323
Stardust flips open
a paddle-shaped collector tray
570
00:28:38,355 --> 00:28:43,526
filled with a durable foam-like
substance called aerogel.
571
00:28:45,224 --> 00:28:49,194
Cometary particles no bigger
than specks of dust
572
00:28:49,225 --> 00:28:50,859
fly into the aerogel
573
00:28:50,892 --> 00:28:54,195
at six times the speed
of a rifle bullet.
574
00:28:54,227 --> 00:28:58,531
The mission's task is to
preserve the precious particles
575
00:28:58,562 --> 00:29:01,965
without damaging
or altering them.
576
00:29:01,997 --> 00:29:07,001
But this is no easy feat,
as we show here on Earth.
577
00:29:09,165 --> 00:29:11,600
- We're here at a firing range
with Sergeant Connacht Brewer,
578
00:29:11,634 --> 00:29:12,901
a former army paratrooper,
579
00:29:12,934 --> 00:29:15,002
who is going to demonstrate
for us what happens
580
00:29:15,035 --> 00:29:18,004
when this birdshot strikes
a large block of modeling clay.
581
00:29:18,036 --> 00:29:20,171
This is an excellent analogy
for what happened
582
00:29:20,203 --> 00:29:22,838
when cometary particles
impacted the aerogel
583
00:29:22,871 --> 00:29:24,505
on the Stardust spacecraft.
584
00:29:24,538 --> 00:29:26,339
Except there,
the particles were moving
585
00:29:26,373 --> 00:29:28,808
about 50 times faster
than this birdshot.
586
00:29:28,840 --> 00:29:29,840
Ready to give it a go?
587
00:29:29,873 --> 00:29:31,007
- Yes, l am.
588
00:29:31,041 --> 00:29:32,575
Go ahead and put on
your eye protection
589
00:29:32,608 --> 00:29:33,575
and your earplugs.
590
00:29:33,608 --> 00:29:34,909
What we're using
for this today
591
00:29:34,942 --> 00:29:37,377
is a 12-gauge Model 1 100
Remington shotgun
592
00:29:37,409 --> 00:29:39,077
at a distance
of about 35 yards.
593
00:29:39,110 --> 00:29:42,913
Basically, l'm just gonna
Ioad a 1 2-gauge shot shell
594
00:29:42,945 --> 00:29:44,246
into the shotgun...
595
00:29:44,278 --> 00:29:45,245
[gun clicks]
596
00:29:45,278 --> 00:29:46,946
And we're hot.
597
00:29:49,748 --> 00:29:50,882
[gunshot]
598
00:29:50,914 --> 00:29:52,315
- Whoa.
599
00:29:52,348 --> 00:29:53,882
lt really did some damage
to that clay.
600
00:29:53,915 --> 00:29:55,049
You want to go take a look?
601
00:29:55,082 --> 00:29:56,216
- Yeah, we're clear.
602
00:29:56,249 --> 00:29:59,719
- All right.
603
00:29:59,751 --> 00:30:01,886
Wow, look at the damage
it did to the clay.
604
00:30:01,918 --> 00:30:03,052
- Yeah.
605
00:30:03,085 --> 00:30:04,719
- Each pellet
created one of these holes.
606
00:30:04,753 --> 00:30:06,054
So what do you say
we cut this open
607
00:30:06,086 --> 00:30:07,220
and try to find some pieces?
608
00:30:07,253 --> 00:30:08,921
- Sounds good.
- All right.
609
00:30:13,023 --> 00:30:15,658
So you see, the trail here
that's formed inside the clay
610
00:30:15,690 --> 00:30:17,158
is going to lead you,
ultimately,
611
00:30:17,190 --> 00:30:19,725
to where the birdshot pellets
are located.
612
00:30:19,758 --> 00:30:21,893
You can imagine how difficult
it would have been
613
00:30:21,925 --> 00:30:23,393
and how time-consuming
614
00:30:23,426 --> 00:30:26,262
for the Stardust team to locate
these microscopic pieces
615
00:30:26,293 --> 00:30:28,628
of cometary material
inside the aerogel.
616
00:30:32,030 --> 00:30:34,699
narrator: Upon Stardust's
return to Earth,
617
00:30:34,730 --> 00:30:38,567
scientists recovered
over 1 O,OOO cometary fragments
618
00:30:38,598 --> 00:30:41,233
from the aerogel.
619
00:30:41,266 --> 00:30:44,068
Chemical analysis revealed
that the particles
620
00:30:44,100 --> 00:30:47,069
contained the organic compound
glycine,
621
00:30:47,101 --> 00:30:50,070
a fundamental building block
of life
622
00:30:50,102 --> 00:30:54,339
that had been preserved in ice
for over 4 billion years.
623
00:30:55,672 --> 00:30:58,641
- The discovery of
organic compounds in comets
624
00:30:58,673 --> 00:31:02,109
suggests that organic compounds
can form pretty easily.
625
00:31:02,140 --> 00:31:05,276
Now, it doesn't mean that there
was ever anything truly alive
626
00:31:05,307 --> 00:31:08,943
in those comets, but at least
the building blocks of life
627
00:31:08,976 --> 00:31:11,478
could have been built
in comets.
628
00:31:13,678 --> 00:31:16,147
narrator: Comets appear to hold
invaluable information
629
00:31:16,178 --> 00:31:19,347
about the origin
of our solar system
630
00:31:19,379 --> 00:31:22,515
and perhaps life itself.
631
00:31:22,547 --> 00:31:24,181
But astronomers
have discovered
632
00:31:24,214 --> 00:31:28,518
that these icy bodies
are not immortal.
633
00:31:28,550 --> 00:31:32,353
Now state-of-the-art satellites
have captured images
634
00:31:32,384 --> 00:31:35,854
of a select group of comets
that will end their life
635
00:31:35,886 --> 00:31:38,888
in a suicidal death dive.
636
00:31:46,089 --> 00:31:48,224
While our journey
with the comets
637
00:31:48,257 --> 00:31:52,561
has felt like an endless
cosmic roller coaster ride,
638
00:31:52,591 --> 00:31:57,729
these icy objects will not orbit
our Sun forever.
639
00:31:57,760 --> 00:32:01,396
Most will make the voyage
for several thousand years
640
00:32:01,429 --> 00:32:04,598
before evaporating
into specks of dust.
641
00:32:08,164 --> 00:32:10,966
Even massive comets,
like Haley,
642
00:32:10,999 --> 00:32:14,802
only have 1 50,OOO years left.
643
00:32:14,833 --> 00:32:21,139
That's because, every second,
a comet loses tons of ice.
644
00:32:21,169 --> 00:32:23,971
- Comets gradually wither away
or fade away,
645
00:32:24,003 --> 00:32:26,472
because every time
they pass close to the Sun,
646
00:32:26,504 --> 00:32:28,639
they lose some of their ices.
647
00:32:28,671 --> 00:32:30,139
They evaporate away.
648
00:32:30,172 --> 00:32:32,974
Eventually,
there's very little ice left,
649
00:32:33,006 --> 00:32:36,442
and so the comet coma and tail
doesn't form.
650
00:32:36,474 --> 00:32:38,442
lt just looks like
an asteroid.
651
00:32:38,475 --> 00:32:39,776
Or it may even break apart
652
00:32:39,809 --> 00:32:41,610
into a whole bunch
of little objects
653
00:32:41,643 --> 00:32:44,612
because the icy glue
is no longer there
654
00:32:44,644 --> 00:32:47,813
or because tidal effects
actually break it apart.
655
00:32:49,746 --> 00:32:53,416
narrator: But not all comets
quietly fade into the sunset.
656
00:32:56,548 --> 00:33:00,018
We're now in hot pursuit
of a group of comets
657
00:33:00,049 --> 00:33:04,720
called sungrazers
that live fast and die young.
658
00:33:06,785 --> 00:33:10,255
lnside our spacecraft,
we feel the heat
659
00:33:10,287 --> 00:33:13,423
as the comets' extremely
elongated orbits
660
00:33:13,455 --> 00:33:16,090
bring us very close
to the Sun...
661
00:33:16,122 --> 00:33:18,891
within a few hundred thousand
miles.
662
00:33:21,024 --> 00:33:23,493
As we enter this danger zone,
663
00:33:23,524 --> 00:33:26,493
we see that some of these
kamikaze comets
664
00:33:26,525 --> 00:33:30,161
occasionally plunge
right into our home star,
665
00:33:30,194 --> 00:33:32,863
creating
a ferocious spectacle.
666
00:33:35,663 --> 00:33:38,465
- Sungrazer comets start out
their life as normal comets.
667
00:33:38,497 --> 00:33:40,298
They probably live
either in the Oort cloud,
668
00:33:40,331 --> 00:33:41,965
or they're short-period
comets,
669
00:33:41,998 --> 00:33:44,433
but they've had an unlucky
encounter with another planet,
670
00:33:44,466 --> 00:33:47,101
probably Jupiter.
671
00:33:47,133 --> 00:33:48,934
lf they're really,
really lucky,
672
00:33:48,967 --> 00:33:51,436
they might just escape
and be able to get away
673
00:33:51,468 --> 00:33:53,403
with one close passage
by the Sun,
674
00:33:53,435 --> 00:33:54,569
but if they're not lucky,
675
00:33:54,602 --> 00:33:56,937
they just get swallowed up whole
by the Sun.
676
00:34:00,105 --> 00:34:02,574
narrator: The Solar and
Heliospheric Observatory,
677
00:34:02,605 --> 00:34:05,908
or SOHO,
is a space satellite
678
00:34:05,940 --> 00:34:09,943
that has observed 2,OOO comets
on suicidal orbits.
679
00:34:12,342 --> 00:34:16,646
The most famous sungrazers
are the Kreutz family,
680
00:34:16,677 --> 00:34:19,646
which originated
from one giant comet
681
00:34:19,678 --> 00:34:23,982
that broke up into
many smaller pieces.
682
00:34:24,013 --> 00:34:26,648
- It's a kind of cool thing
to think of a comet
683
00:34:26,681 --> 00:34:28,315
that's lived
in the outer solar system
684
00:34:28,348 --> 00:34:30,650
just falling all the way
and smashing into the Sun,
685
00:34:30,682 --> 00:34:31,983
but they do.
686
00:34:32,016 --> 00:34:33,684
We see them all the time.
687
00:34:38,285 --> 00:34:42,088
narrator: And some comets
do more than self-destruct.
688
00:34:42,120 --> 00:34:45,189
They become the messengers
of mass destruction.
689
00:34:47,255 --> 00:34:49,557
lt's estimated
that a large comet
690
00:34:49,589 --> 00:34:53,726
may have struck Earth
roughly every 40 million years,
691
00:34:53,758 --> 00:34:57,228
based on the amount of craters
still visible on our planet.
692
00:35:00,559 --> 00:35:03,194
A comet may have
even been responsible
693
00:35:03,228 --> 00:35:06,898
for the most famous
extinction event of all time.
694
00:35:10,296 --> 00:35:13,265
- For the Cretaceous-Tertiary
extinction event,
695
00:35:13,297 --> 00:35:14,765
the one that took out
the dinosaurs
696
00:35:14,798 --> 00:35:17,800
65 million years ago,
the jury is still out.
697
00:35:17,832 --> 00:35:20,634
That was thought to be
a 1 O-kilometer-sized object,
698
00:35:20,667 --> 00:35:23,803
and there are no asteroids
in near-Earth space
699
00:35:23,835 --> 00:35:27,638
that are that large
that could impact the Earth,
700
00:35:27,669 --> 00:35:30,972
and there are a number of comets
that are that large.
701
00:35:31,004 --> 00:35:33,773
And since it occurred
65 million years ago,
702
00:35:33,805 --> 00:35:35,439
and you would expect
a cometary impact
703
00:35:35,472 --> 00:35:38,942
every 40 million years or so,
704
00:35:38,974 --> 00:35:42,277
it may well have been
a comet.
705
00:35:42,308 --> 00:35:44,777
narrator: While comets
likely slammed into Earth
706
00:35:44,809 --> 00:35:47,444
countless times in the past,
707
00:35:47,476 --> 00:35:49,110
it's been difficult
to determine
708
00:35:49,144 --> 00:35:53,781
if an impact crater
was made by a comet or asteroid
709
00:35:53,812 --> 00:35:56,648
because the two bodies
appear to be similar.
710
00:35:58,814 --> 00:36:00,882
- When we study
the fossil records,
711
00:36:00,915 --> 00:36:02,549
a lot of the material is gone,
712
00:36:02,582 --> 00:36:04,550
and just-
we simply can't find it,
713
00:36:04,583 --> 00:36:06,384
and it turns out that
asteroids and comets
714
00:36:06,416 --> 00:36:07,817
have a lot of materials
in common,
715
00:36:07,850 --> 00:36:10,786
so even if you do find
extraterrestrial material,
716
00:36:10,819 --> 00:36:12,120
it's really hard to tell
717
00:36:12,153 --> 00:36:14,488
whether it came from an asteroid
or from a comet.
718
00:36:16,187 --> 00:36:17,988
narrator:
And to complicate matters,
719
00:36:18,021 --> 00:36:21,157
a comet doesn't even
have to impact Earth's surface
720
00:36:21,189 --> 00:36:23,691
to ignite a catastrophe.
721
00:36:26,158 --> 00:36:30,195
ln 1 908, a fireball exploded
in the atmosphere
722
00:36:30,225 --> 00:36:33,528
above the Tunguska wilderness
in Siberia.
723
00:36:33,560 --> 00:36:36,029
The heat and energy
from the airburst
724
00:36:36,060 --> 00:36:40,030
propelled downward
like a hot tornado.
725
00:36:40,062 --> 00:36:42,364
lt propagated
across the forest,
726
00:36:42,396 --> 00:36:46,399
flattening over 800 square miles
of trees.
727
00:36:47,965 --> 00:36:51,101
For over a century,
some scientists have wondered
728
00:36:51,133 --> 00:36:55,971
if the cosmic intruder
was a comet or an asteroid.
729
00:36:57,269 --> 00:36:58,803
- If it were caused
by a comet,
730
00:36:58,836 --> 00:37:00,971
you would imagine you'd find
in the sediment
731
00:37:01,004 --> 00:37:03,139
some record of unusual things,
732
00:37:03,171 --> 00:37:06,240
like a ratio of helium 3
to helium 4.
733
00:37:06,272 --> 00:37:09,241
That could be an indication
that it may have been a comet.
734
00:37:09,273 --> 00:37:11,074
Now, another possibility
is if you find
735
00:37:11,107 --> 00:37:14,410
some strange isotope
buried in a lake somewhere.
736
00:37:14,441 --> 00:37:17,110
That's tough.
This is not easy.
737
00:37:19,510 --> 00:37:20,978
narrator: While it's
been difficult
738
00:37:21,011 --> 00:37:25,648
to substantiate
cometary impacts on Earth,
739
00:37:25,679 --> 00:37:28,815
physical proof
of their colossal power
740
00:37:28,847 --> 00:37:32,550
exists on
the gas giant planets.
741
00:37:32,581 --> 00:37:36,384
And these dramatic events
warn that far worse collisions
742
00:37:36,416 --> 00:37:38,718
loom in the future,
743
00:37:38,751 --> 00:37:42,254
with Earth as
the potential bull's-eye.
744
00:37:50,021 --> 00:37:53,758
As we have followed the trail
of comets through space,
745
00:37:53,789 --> 00:37:55,557
we have passed through
the chilliest
746
00:37:55,590 --> 00:37:59,060
and warmest places
in our solar system.
747
00:37:59,091 --> 00:38:02,394
We've also investigated
whether these icy bodies
748
00:38:02,425 --> 00:38:07,329
have been deliverers
and destroyers of life.
749
00:38:07,360 --> 00:38:13,032
And new observations prove
many of these ancient bodies
750
00:38:13,063 --> 00:38:16,199
haven't quietly retired
to the frigid outer limits
751
00:38:16,231 --> 00:38:20,201
of our solar system.
752
00:38:20,232 --> 00:38:23,168
- We think there are several
possible end states for comets.
753
00:38:23,200 --> 00:38:26,903
ln one case, they can actually
get pulled right into the Sun.
754
00:38:26,935 --> 00:38:28,903
ln other cases, they can
actually get scattered
755
00:38:28,936 --> 00:38:30,737
by one of the planets
and kind of get kicked out,
756
00:38:30,769 --> 00:38:33,905
maybe back into the Oort cloud
and never seen again.
757
00:38:33,937 --> 00:38:36,706
And finally they can also
actually impact a planet.
758
00:38:41,873 --> 00:38:45,376
narrator: We now shuttle back
to July 1 994.
759
00:38:48,342 --> 00:38:51,645
We follow a string of
21 comet fragments
760
00:38:51,677 --> 00:38:54,146
called Shoemaker-Levy 9
761
00:38:54,177 --> 00:38:57,647
as they're gravitationally
pulled toward the gas giant
762
00:38:57,679 --> 00:39:00,148
planet Jupiter.
763
00:39:00,180 --> 00:39:01,481
- If we were riding on
764
00:39:01,514 --> 00:39:04,483
one of the fragments of
the comet Shoemaker-Levy 9,
765
00:39:04,515 --> 00:39:06,316
it would have been
truly spectacular
766
00:39:06,349 --> 00:39:08,217
because we're heading
toward Jupiter,
767
00:39:08,249 --> 00:39:11,452
and this giant planet
is looming ever bigger,
768
00:39:11,483 --> 00:39:12,784
and then-splat!
769
00:39:12,818 --> 00:39:14,286
We crash into it.
770
00:39:14,319 --> 00:39:19,290
We throw up a whole bunch
of material from the insides.
771
00:39:19,320 --> 00:39:21,422
lt would be really
an amazing journey.
772
00:39:21,454 --> 00:39:24,256
The plumes of material
coming out of Jupiter
773
00:39:24,288 --> 00:39:27,257
were superheated gas
heated by this collision
774
00:39:27,289 --> 00:39:30,792
and also excavated from
the interior of Jupiter.
775
00:39:32,191 --> 00:39:35,160
narrator: Shoemaker-Levy 9
Ieft impact scars
776
00:39:35,192 --> 00:39:37,494
the size of Earth,
777
00:39:37,527 --> 00:39:39,662
driving home
the scale of violence
778
00:39:39,694 --> 00:39:44,031
that comets can produce
if they slam into our planet.
779
00:39:45,796 --> 00:39:48,098
- If any of those fragments
had hit the Earth
780
00:39:48,130 --> 00:39:51,266
rather than Jupiter, we'd have
been in serious trouble,
781
00:39:51,298 --> 00:39:52,599
because they were large
782
00:39:52,632 --> 00:39:55,334
and they were coming in
extremely rapidly.
783
00:39:55,366 --> 00:39:56,900
But fortunately,
big brother Jupiter
784
00:39:56,933 --> 00:39:59,568
took all the hits for us
and didn't seem to suffer much
785
00:39:59,602 --> 00:40:01,904
in the way of damage.
786
00:40:01,935 --> 00:40:03,736
narrator: But even with
Jupiter acting
787
00:40:03,769 --> 00:40:05,737
as a planetary shield,
788
00:40:05,770 --> 00:40:08,572
comets still
sneak by the gas giants
789
00:40:08,605 --> 00:40:12,408
and have close encounters
with Earth.
790
00:40:12,440 --> 00:40:13,741
- The good news is,
791
00:40:13,773 --> 00:40:16,575
asteroid impacts are far more
likely to occur
792
00:40:16,608 --> 00:40:20,244
because asteroids
outnumber comets 1 OO to 1
793
00:40:20,276 --> 00:40:21,744
in near-Earth space.
794
00:40:21,776 --> 00:40:23,911
The bad news is,
if we do find a comet
795
00:40:23,943 --> 00:40:25,878
on an Earth-impacting
trajectory,
796
00:40:25,911 --> 00:40:27,712
we wouldn't realize it
797
00:40:27,745 --> 00:40:30,047
till it got inside
the orbit of Jupiter,
798
00:40:30,079 --> 00:40:33,715
when it started throwing off
gas and dust.
799
00:40:33,747 --> 00:40:35,882
- In the very unlikely event
that a comet
800
00:40:35,915 --> 00:40:38,050
could get close to the Earth,
you would worry about it
801
00:40:38,082 --> 00:40:40,217
because they tend to have
high average velocities
802
00:40:40,250 --> 00:40:41,718
relative to an asteroid,
803
00:40:41,750 --> 00:40:44,152
as high as tens of miles
a second.
804
00:40:44,184 --> 00:40:47,487
So in other words, they would
pack a bigger punch.
805
00:40:47,518 --> 00:40:49,987
narrator: While the frequency
of near-Earth asteroids
806
00:40:50,020 --> 00:40:52,589
heightens
the risk of impacts,
807
00:40:52,621 --> 00:40:56,324
the speed of comets
is equally troubling.
808
00:40:56,355 --> 00:40:58,490
This sobering fact
has prompted
809
00:40:58,522 --> 00:41:02,225
I
viewer Robin W. from Boulder Colorado, to...
810
00:41:10,560 --> 00:41:12,528
- Robin,
that's an important question.
811
00:41:12,561 --> 00:41:14,362
The asteroids
are mOre n U merOUS,
812
00:41:14,395 --> 00:41:16,263
so there's more of them
that could hit us.
813
00:41:16,296 --> 00:41:18,765
But we can track
their trajectories
814
00:41:18,796 --> 00:41:21,765
and maybe do something about
one that's gonna hit us,
815
00:41:21,797 --> 00:41:23,765
deflect it for example.
816
00:41:23,798 --> 00:41:25,766
The comets are more rare,
817
00:41:25,799 --> 00:41:28,768
but we have very little warning
when they come in.
818
00:41:28,800 --> 00:41:31,769
And also, they move much faster
than asteroids,
819
00:41:31,801 --> 00:41:34,937
so there's more energy
impacting Earth.
820
00:41:34,969 --> 00:41:38,138
So l would say comets are
the most hazardous objects.
821
00:41:41,805 --> 00:41:45,441
narrator: NASA is taking
the threat of comets seriously.
822
00:41:45,473 --> 00:41:47,608
So far, tracking satellites
823
00:41:47,641 --> 00:41:50,977
have tagged 84
near-Earth comets,
824
00:41:51,009 --> 00:41:54,645
objects with orbits that
come within 28 million miles
825
00:41:54,676 --> 00:41:57,979
of Earth's path
around the Sun.
826
00:41:58,011 --> 00:41:59,612
- There are no periodic comets
827
00:41:59,645 --> 00:42:02,280
that currently have Earth's name
written on them.
828
00:42:02,312 --> 00:42:04,447
But Jupiter
and the other giant planets
829
00:42:04,480 --> 00:42:07,149
occasionally perturb
the orbits of comets.
830
00:42:07,180 --> 00:42:09,749
So there could be
a periodic comet in the future
831
00:42:09,782 --> 00:42:12,951
that will collide
with Earth.
832
00:42:20,686 --> 00:42:23,655
narrator: Since the beginning
of recorded history,
833
00:42:23,687 --> 00:42:27,657
over 4,200 comets
have been observed,
834
00:42:27,688 --> 00:42:32,459
a mere fraction of the total
number of these icy bodies.
835
00:42:32,490 --> 00:42:35,626
This means billions
of unknown comets
836
00:42:35,658 --> 00:42:40,129
still lie in wait
in the outer reaches of space.
837
00:42:40,159 --> 00:42:44,463
One day, a doomsday comet
could be nudged out
838
00:42:44,495 --> 00:42:47,331
and sent on a collision course
with Earth.
839
00:42:49,562 --> 00:42:52,364
- If we're on
that cosmic highway,
840
00:42:52,397 --> 00:42:55,199
and it's getting
into our on-ramp,
841
00:42:55,232 --> 00:42:56,700
we need to worry about it.
842
00:42:56,732 --> 00:42:59,701
And we need to worry about it
with very little lead time.
843
00:42:59,733 --> 00:43:01,968
- There is very little
we can do,
844
00:43:02,000 --> 00:43:04,135
other than sending
a giant bomb toward them
845
00:43:04,168 --> 00:43:05,469
and trying to deflect them.
846
00:43:05,502 --> 00:43:06,970
But that's very difficult
847
00:43:07,002 --> 00:43:08,636
when there's only
a few months' warning.
848
00:43:10,704 --> 00:43:13,506
narrator: Just as comets
have inspired awe and fear
849
00:43:13,538 --> 00:43:16,641
among our ancestors,
850
00:43:16,673 --> 00:43:19,809
they remain a force
to reckon with.
851
00:43:19,840 --> 00:43:23,443
By continuing to track
their tails of dust,
852
00:43:23,475 --> 00:43:27,445
we may uncover more clues
about these frozen artifacts
853
00:43:27,476 --> 00:43:30,645
of our ancient past.
854
00:43:30,678 --> 00:43:32,646
- It's pretty remarkable
if you think about it.
855
00:43:32,679 --> 00:43:35,648
Just a few hundred years ago,
we had no idea what they were.
856
00:43:35,680 --> 00:43:37,181
We had no idea
what they meant.
857
00:43:37,213 --> 00:43:39,682
And now we've actually been
to the surfaces of comets.
858
00:43:39,714 --> 00:43:42,049
We've seen up close and personal
what they're really like
859
00:43:42,082 --> 00:43:43,483
and what they're made out of.
860
00:43:43,516 --> 00:43:46,151
So these mysterious objects
have meant a lot to humans
861
00:43:46,183 --> 00:43:47,317
throughout our history.
862
00:43:47,350 --> 00:43:49,218
They've been agents of change.
863
00:43:49,251 --> 00:43:52,721
They've been agents
of destruction sometimes.
864
00:43:52,752 --> 00:43:55,087
They've maybe been agents
of creation.
865
00:43:55,137 --> 00:43:59,687
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