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male narrator: In the beginning, there was darkness,
and then, bang,
giving birth to an endless expanding existence
of time, space, and matter.
Every day, new discoveries are unlocking the mysterious,
the mind-blowing, the deadly secrets
of a place we call The Universe.
Chart a daring course with comets,
the cosmic time travelers of the skies.
- These mysterious objects have been agents of change.
They've been agents of destruction.
narrator: Discover why these celestial bodies
carry secrets from our past
and cast doom over our future.
- If it's getting into our on-ramp,
we need to worry about it.
- There's very little we can do
other than sending a giant bomb toward them
and trying to deflect them.
narrator: Brace yourself as we rendevous
with the frozen intruders from the great beyond
on an epic journey to ''Ride the Comet.''
They appear out of nowhere,
gliding slowly across the nighttime sky
and then disappearing from sight.
Throughout human history, ancient cultures
believed these celestial intruders
carried special powers from the gods,
mystical messengers of life and death.
- Scientists like to think
that comets are fairly mysterious objects,
because we know that they're very old.
They're like frozen time capsules
from when our solar system was first formed.
- Comets are a bit of show-offs.
They come into the night sky unannounced, unpredicted.
ln the Middle Ages, they were thought to be fireballs
thrown at a sinful Earth
from the right hand of an avenging god.
And so they've always been feared or seen as mysterious.
narrator: We're going to hitch a ride
Our daring quest begins 4.5 billion years ago,
as our futuristic spacecraft time-travels
back to the birth of our solar system.
We zigzag through a maelstrom of debris
to catch our first glimpse of comets,
the wayward rocks that didn't meld into planets.
- Comets are basically dirty snowballs
or icy dirtballs.
They consist of rocks and dust and dirt
held together by ices-
water ice, ammonia, methane, carbon dioxide, dry ice.
That's sort of like the glue
that holds all these little pebbles
and particles of dust together.
narrator: The heart of these cosmic icebergs is the nucleus,
or central core, which averages in size
from a half mile wide to as big as a modern city.
- One of the things we've learned
by flying close by and observing the nuclei of comets
is that they're these strange
sort of compacted conglomerates of ice and rock.
They're not uniform.
They're not perfectly mixed.
They're quite chunky and oddly shaped.
- The nuclei of comets are...
very fragile entities.
lf you had a chunk,
you could probably break it easily in your hands.
narrator: Up close,
comets look like bland chunks of charcoal
rather than supersized snowballs.
They don't even remotely resemble
the glowing orbs we see in our pitch-black skies.
- We think that most comets are extremely dark
on their surfaces, that the surfaces are covered
with something kind of like barbecue soot,
this really dark, black material
that makes them very difficult to see.
narrator: While their asteroid cousins
share similar properties, such as rock and metal,
scientists suspect that comets were born farther out,
near the gas giant planets,
I where it's much colder
so they possess more ices and volatile elements.
About 3.8 billion years ago,
many of these icy bodies were whisked away
to the Kuiper belt, a frigid neighborhood
just beyond the outermost planet, Neptune.
- Icy objects in the Kuiper belt probably formed
closer in toward the Sun, where the giant planets are,
but then gravitational interactions
with those giant planets made those icy objects
migrate outward.
narrator: Our spacecraft navigates
through this dark, disklike region,
which is almost 2 billion miles wide
and is estimated to hold over 6 billion comets.
We eventually touch down
on the surface of one of these icy boulders.
- Landing on a comet would be a pretty tricky affair.
[engine whirring]
So you could kind of imagine dirty snow
that's covered with exhaust,
and if you step on it,
in places, you can punch through
to places where there's more fresh material underneath it.
narrator: The Kuiper belt objects
appear to have fairly stable orbits,
so they won't be that much fun to ride.
We lift off in search of a comet
that will cut a more exciting path
through our solar system.
We navigate farther out
to a sparsely populated region called the scattered disc,
which is home to icy bodies with long, elliptical orbits.
The slightest disturbance can send these unstable objects
careening into the inner solar system,
where they become known as short-period comets,
those which orbit the Sun every 20 to 200 years.
- The scattered disc region
is thought to be the primary source
of the short-period comets.
They are kicked into the inner solar system
either by interacting with Neptune
or possibly passing stars.
narrator: Our spacecraft witnesses
Neptune's gravitational influence at work,
dislodging a comet out of the scattered disc.
This comet would be too dangerous to land on,
so we'll track alongside it
on its transformational flight through our solar system.
- So what would happen if it was on a journey toward the Sun?
Well, it would start off Iooking like a dark asteroid.
Nothing much is happening.
lt doesn't have an atmosphere around it.
- As you start to travel toward the inner solar system,
get up to Jupiter or even closer to the Sun,
the comet would start to become active.
- The warmth from the Sun starts to heat up the comet,
and all the frozen material that's trapped on the inside
starts to convert from ice into gaseous material,
and so these gas jets can actually punch through
the crust of the comet and form jets.
As these jets flow away from the surface,
they can start to pull dust and rocks with them,
and this forms a kind of hazy atmosphere
around the comet's nucleus.
We call this the coma.
narrator: As it zooms by Earth,
the coma of a comet can grow to be larger
than the diameter of our Sun.
Solar radiation eventually pushes this cosmic halo
behind the nucleus, forming two bright tails:
one of dust and the other of gas.
- There will be a tail growing and growing and growing,
and you would eventually become engulfed
in just a really rocky, icy, particle-filled environment.
lt would be very difficult on your spacecraft
because it'd be like flying through a blizzard.
narrator: Some tails can stretch for 1 OO million miles,
more than the distance between the Sun and the Earth,
as it travels towards our home star.
lt's one of the most spectacular spectacles of our solar system.
- Today we're going to see what happens
when we take a comet
that's been in the cold, dark, icy outer reaches
of the solar system,
and we're going to send it inward towards its perihelion,
or the point of closest approach to the Sun.
Now, dry ice is frozen carbon dioxide,
and this is a very common constituent of comets.
Let's see what happens.
When we take this piece of dry ice,
and we drop it into the warm water
the dry ice starts to sublimate.
That means it converts directly from a solid, frozen state
into a gaseous state.
And as the water starts to warm up
certain parts of the dry ice first,
you can start to see that little jets kind of form on it,
and this forms a hazy atmosphere called a coma.
You can see that the little chips of dry ice
are constantly changing as they sublimate away.
Sometimes they speed up.
Sometimes they slow down.
So if this was a comet,
you can get the idea that, as the comet approaches the Sun,
and the volatiles start to vaporize,
this can actually change the comet's rotational state
and even its orbit.
narrator: Comets are brightest and fastest
when they're closest to the Sun.
The searing heat and immense gravity of our mother star
can accelerate a comet's speed
to nearly 2 million miles per hour.
- The speed increases a lot, and it whips around the Sun,
so it goes zoom, like that,
like being propelled
at the bottom of a giant roller coaster.
A roller coaster starts out high, very slowly,
picks up speed due to the gravity,
goes zooming past the bottom,
and then slows down again on its outward journey.
- Eventually, as our comet Ieaves the vicinity of the Sun,
it's going to travel back out
into the far reaches of the solar system.
Everything's going to quiet down.
All of the gas and dust is going to settle
back onto its surface.
And eventually, it'll cruise away into the quiet dark.
narrator: Back in the cold region of the scattered disc,
a comet transforms
back into a dull, black lump of rock and ice
until it makes its journey around the Sun once again.
Haley, the most famous short-period comet,
was first recorded in 240 B.C.
and has passed by Earth every 76 years.
Estimated to be the size of Manhattan,
this superstar comet is sometimes so bright,
it has been seen in broad daylight.
Throughout history,
the appearance of Haley has inspired awe and dread
among earthly observers.
- In 1910, it was feared,
because spectroscopy had just been introduced,
and they had determined that comets contain cyanogen,
which is an odorless and poisonous gas,
and so astronomers predicted that there'd be problems
because of this poisonous gas sweeping the Earth,
and so there were actually comet pills manufactured.
Life insurance policies on the comet were taken out.
narrator: While comets have been thought to be
extraterrestrial harbingers of doom,
astronomers have long wondered if these glowing rocks
contain precious information about our past.
By the 21st century, NASA was ready to ignite
a bold offensive strike, one that would hopefully expose
one of the holy grails of planetary science.
Could these interplanetary vagabonds
have been the cosmic transporters of life?
So far, we've traveled with comets
from the frozen hinterlands of the Kuiper belt
and scattered disc
to an exhilarating orbit around the Sun.
We've watched these dark bodies come alive
as they formed brilliant comas and tails.
But scientists are still puzzled
about what's really inside these cosmic interlopers.
- Man, l wish l knew
what the interior of a comet Iooked like.
You would love to be able
to look inside the nucleus of a comet,
to see if it's clumpy, if it's uniform.
ls there crystalline ice?
ls there glassy ice?
narrator: Our protective spacecraft
time-travels back to 2005
and meets up with NASA's Deep Impact space probe
on a comet-hunting mission.
lt zeroes in on a short-period comet named Tempel 1
with an aggressive plan of attack.
We hover at a safe distance as Deep Impact
launches an 800-pound projectile into the passing comet.
Debris sprays out for thousands of miles
as the impactor excavates a crater
and sends tons of blinding gas, rocks, and dust into space.
For the first time in history,
scientists are able to peer inside
the icy, muddy interior of a comet.
- Right after the impact,
you could see silicate grains fluorescing and glowing.
This tells us that comets are very primitive material
and that they pretty much do preserve in pristine state
the materials that we find
in the youngest star-forming systems.
So indeed, they really are time capsules
that let us look back on our own solar system
at the very beginning.
narrator: While Deep Impact
captures a rare glimpse of a comet's interior
it is unable to snap clear images of the crater,
which was obscured by an enormous plume of debris.
ln February 201 1, another spacecraft,
named Stardust-NExT,
catches up to Tempel 1
as it completes its five-year orbit around the Sun.
To everyone's surprise,
the impact crater is much smaller than had been expected
from the historic smash-up that occurred five years earlier.
- Amazing...
But the crater looked like it was small.
So this now creates this issue:
Was the crater always small?
We know the crater isn't what we expected.
So we're going to do some experiments
to see if we can explain why the crater looks like it does.
- Sunlamp's coming on.
- Can we move it up a bit?
narrator: At NASA's Ames Vertical Gun Range,
Stardust-NExT coinvestigator Pete Schultz
is conducting high-velocity impact experiments
to find out why Deep Impact produced such a tiny crater.
He will use a massive
.30-caliber high-velocity gas gun
to fire tiny projectile beads at various targets
located inside a vacuum chamber.
- We're trying to simulate
what the nature of the surface of comet 9P/Tempel 1 is like,
so we're putting in perlite,
which is this low-density material
that you find in gardens,
then we're adding in hollow microspheres,
and this also resemble what the nature of the comet is like.
The purpose of the experiment is to see what happens
to the crater after formation.
Does it stay there? Does it collapse?
With this experiment, we should be able to find out.
Okay, l'm out of the tank.
Lock and load.
narrator: High-speed cameras
mounted around the vacuum chamber
will document the impact.
- We've got this one covered.
We just have to hit the target.
Okay.
[claps hands]
Let's shoot this puppy.
J.P., are you ready?
- Yeah.
narrator: As the crew anxiously awaits in the control room,
Pete mixes science with a little superstition.
- There's always a risk.
Sometimes you miss. Sometimes you hit.
- Whoa!
- Oh, sweet.
The whole thing sort of collapses in on itself.
lt's getting smaller now.
lt was bigger. Now it's getting smaller.
So what we see here is that there's a lot of dust and ejecta
sent upwards, and that blocked the view.
We couldn't see the crater forming.
So what started off being a nice-looking crater,
it just doesn't stay there.
lt just simply heals itself.
So what may have happened for 9P/Tempel 1 ,
the nucleus, is that that crater healed itself.
The nucleus healed itself from the scar created
by us with Deep Impact.
Let's see what we did.
[groans]
So the results were fantastic.
We got to see just what we planned to.
There may be more to the story,
so we're going to try a different experiment as well.
narrator: Pete has a hunch
there's a missing piece to the Deep Impact mission.
He now wants to see if the space probe
created a different type of crater on Tempel 1 ,
due to the makeup of the comet's nucleus.
- So this time, we're going to put
a denser layer below that perlite,
so we want to find out whether or not
we'll get a different type of crater
if we have two different types of material:
one very soft on top
and one denser on the bottom.
narrator: Pete and his crew return to the control room
to see what happens to the new target of perlite
poured over a heavier layer of sand.
[small explosion]
- [laughs]
Now, that formed a big crater in the perlite.
Boy, look at that.
Oh, oh, man, that is gorgeous.
Okay.
The projectile went deep,
and now the stuff is coming back out that hole,
while, on the surface, it's excavating debris.
Pow! Okay.
narrator: The double-layered target created not one
but two craters,
a small crater inside a larger, shallower crater.
- This could be what happened for 9P/Tempel 1.
lt went so deep into the nucleus,
and then itjust simply collapses away,
and we're left with just this very, very faint rim
on the outside with a small pit in the center.
narrator: These impact experiments
yield surprising clues about the interior of Tempel 1
and perhaps all comets.
- Now we know that comets have history.
We see layers.
l don't know if these layers go all the way
through the nucleus,
or are they only in one part?
narrator: Unraveling the secrets
of what's inside comets will help scientists understand
what causes them to exhibit some really bizarre behavior.
Our spaceship now shadows NASA's EPOXl mission
as it encounters Hartley 2,
a fast-spinning comet that tumbles through space
like a hyperactive cosmic peanut.
- Hartley 2 is a smaller comet.
lt's only about a mile or so aCrOSS,
and so it's kind of a surprise that it's so active.
lt's putting off huge amounts
of C02 and, actually, cyanide gas.
And the question is,
are all small comets active like this
or only a few?
And what makes them so active?
l've got a peanut-shaped plastic bottle here
that's supposed to represent comet Hartley 2.
lt's full of dry ice and warm water
and as you can see,
as the warm water starts to make the dry ice sublimate,
it shoots out these jets
through the holes that we've got poked in the bottle.
lf l drop it into the water,
instead of holding it fixed in space,
you can see that the jets actually start
pushing the bottle around,
causing the comet's rotational state to change.
This is very similar to what's going on
on the surface of comet Hartley 2.
The C02 jets are actually changing the rotational state
of the comet, causing it to speed up and slow down.
narrator: When tracking Hartley 2,
our spacecraft gets caught in a cosmic blizzard
as the spastic comet burps and belches out
a trail of frozen snowballs that extend for millions of miles.
- One of the big surprises about Hartley 2
is that it was surrounded by this posse of mini comets.
This is simply ices that are coming off,
about the size of a snowball all the way up to a basketball.
narrator: Scientists suspect the snowball-sized debris
rains back down on Hartley 2,
producing its unusual landscape of craters and towering spires.
- Because these comets have very little gravities,
most of the gas is blown out into space,
but a very small fraction can actually redeposit
on the surface, generating very smooth textures,
and on other locations, generating these very bumpy
or spire-like texture.
narrator: From Hartley 2,
we blast off to the extreme outer edge of our solar system,
a vast, eerie place,
barely within the gravitational grasp of our Sun
and impossible to see, even with modern telescopes.
Here, we come upon the largest and perhaps most elusive
icy bodies in our galactic neighborhood.
Our journey through the fascinating world of comets
has provided us a ringside seat to some of the greatest
cosmic shows observed from Earth and space.
We now change course and travel
over 50,OOO times the distance between Earth and the Sun
to the outermost edge of our solar system.
We arrive at the Oort cloud,
an even larger fraternity of comets,
perhaps over a trillion of them.
- If we'd actually got in a spaceship
and tried to go out and, say, visit the Oort cloud,
this would have been a long journey.
There's billions and billions of these objects,
and there's a lot of space in between them.
narrator: Like the Kuiper belt and scattered disc,
the Oort cloud objects may have formed closer to the Sun,
but about 800 million years
after the solar system was formed,
the gravitational influence of the gas giant planets
flung these comets
out to the frigid edge of our solar system.
- Some of these objects were flung
into very highly elliptical orbits
out into the Oort cloud.
Passing stars could circularize those orbits,
making somewhat stable orbits for them.
narrator: Most of the Oort cloud bodies
have been in frozen hibernation
since the birth of our solar system.
They only become Iong-period comets
when they get sucked into orbits
that carry them inward towards the planets and the Sun.
Scientists have never actually captured
an image of the Oort cloud,
but they have good reason to believe it's there.
- Even though scientists can't directly observe the Oort cloud
because it's so far away and so faint,
what they are able to do is infer its existence
because we can look at
where all these long-period comets come from on the sky,
and they seem to come from all different directions.
There doesn't really seem to be a preferred direction for them.
This suggests that the Oort cloud,
if it exists, is probably roughly spherical.
narrator: One of the big mysteries
is what knocks these icy bodies off course
and sends them cruising by our neighborhood of Earth.
- The comets in the Oort cloud are very susceptible
to gravitational pulls from other things
outside the solar system.
One thing is passing stars.
lf a star happens to come close to our Sun,
it can scatter comets from the outer Oort cloud.
- Icy objects in the Oort cloud can also be dislodged
by gravitational perturbations that occur
when the solar system goes through the plane of our galaxy.
So the solar system is basically orbiting
around the center of our galaxy,
but it's also oscillating up and down,
and when it goes through the plane,
then gravitational interactions can perturb objects
from the Oort cloud into the inner solar system.
narrator: Some long-period comets
take up to about 30 million years
to complete one round trip around the Sun.
Our spacecraft tracks a long-period comet
for hundreds of thousands of miles
until we approach planet Earth.
As its icy tails unfurl,
a layer of dust and ice zips through
our planet's thin atmosphere,
leaving visible trails known as a meteor shower.
- l like to think of comets
as sort of the pigpens of the solar system,
because, as they orbit around the Sun,
they leave a big, messy trail of debris.
But sometimes the Earth's orbit can intersect
some of these dust bands,
and when it does, we can sometimes see meteor showers.
Those beautiful bright streaks of light
that you see coming through the night sky
are actually produced by particles
that are most often no bigger than a sand grain.
narrator: While long- and short-period comets
make up the bulk of comets that have been observed,
new evidence suggests that not all icy bodies
come from the subzero suburbs of our solar system.
Some have secretly taken up residence
in a much warmer neighborhood.
Scientists have now discovered
there are comets masquerading as asteroids
I in the asteroid belt
located between Jupiter and Mars.
- The only reason that we've discovered
these main-belt comets is because, occasionally,
the warming rays of the Sun get into the interior,
vaporize the ices,
and so the comet just bursts forth for a while,
and then they go back to being inactive objects or asteroids.
- Scientists used to think that there were strong distinctions
between asteroids and comets
and that they were two totally different types of objects,
but what we're finding nowadays is,
there are some asteroids that have comet-like properties,
and there are some comets that eventually kind of look
like asteroids.
narrator: Some scientists think main-belt comets
may have delivered water to early Earth
and the materials to create life.
We blast back to January 2004
and follow NASA's Stardust spacecraft
on an unprecedented mission
to collect pure comet dust in space.
Just beyond the planet Mars,
we meet up with a comet named Wild 2.
Upon approaching its enormous coma,
Stardust flips open a paddle-shaped collector tray
filled with a durable foam-like substance called aerogel.
Cometary particles no bigger than specks of dust
fly into the aerogel
at six times the speed of a rifle bullet.
The mission's task is to preserve the precious particles
without damaging or altering them.
But this is no easy feat, as we show here on Earth.
- We're here at a firing range with Sergeant Connacht Brewer,
a former army paratrooper,
who is going to demonstrate for us what happens
when this birdshot strikes a large block of modeling clay.
This is an excellent analogy for what happened
when cometary particles impacted the aerogel
on the Stardust spacecraft.
Except there, the particles were moving
about 50 times faster than this birdshot.
Ready to give it a go?
- Yes, l am.
Go ahead and put on your eye protection
and your earplugs.
What we're using for this today
is a 12-gauge Model 1 100 Remington shotgun
at a distance of about 35 yards.
Basically, l'm just gonna Ioad a 1 2-gauge shot shell
into the shotgun...
[gun clicks]
And we're hot.
[gunshot]
- Whoa.
lt really did some damage to that clay.
You want to go take a look?
- Yeah, we're clear.
- All right.
Wow, look at the damage it did to the clay.
- Yeah.
- Each pellet created one of these holes.
So what do you say we cut this open
and try to find some pieces?
- Sounds good. - All right.
So you see, the trail here that's formed inside the clay
is going to lead you, ultimately,
to where the birdshot pellets are located.
You can imagine how difficult it would have been
and how time-consuming
for the Stardust team to locate these microscopic pieces
of cometary material inside the aerogel.
narrator: Upon Stardust's return to Earth,
scientists recovered over 1 O,OOO cometary fragments
from the aerogel.
Chemical analysis revealed that the particles
contained the organic compound glycine,
a fundamental building block of life
that had been preserved in ice for over 4 billion years.
- The discovery of organic compounds in comets
suggests that organic compounds can form pretty easily.
Now, it doesn't mean that there was ever anything truly alive
in those comets, but at least the building blocks of life
could have been built in comets.
narrator: Comets appear to hold invaluable information
about the origin of our solar system
and perhaps life itself.
But astronomers have discovered
that these icy bodies are not immortal.
Now state-of-the-art satellites have captured images
of a select group of comets that will end their life
in a suicidal death dive.
While our journey with the comets
has felt like an endless cosmic roller coaster ride,
these icy objects will not orbit our Sun forever.
Most will make the voyage for several thousand years
before evaporating into specks of dust.
Even massive comets, like Haley,
only have 1 50,OOO years left.
That's because, every second, a comet loses tons of ice.
- Comets gradually wither away or fade away,
because every time they pass close to the Sun,
they lose some of their ices.
They evaporate away.
Eventually, there's very little ice left,
and so the comet coma and tail doesn't form.
lt just looks like an asteroid.
Or it may even break apart
into a whole bunch of little objects
because the icy glue is no longer there
or because tidal effects actually break it apart.
narrator: But not all comets quietly fade into the sunset.
We're now in hot pursuit of a group of comets
called sungrazers that live fast and die young.
lnside our spacecraft, we feel the heat
as the comets' extremely elongated orbits
bring us very close to the Sun...
within a few hundred thousand miles.
As we enter this danger zone,
we see that some of these kamikaze comets
occasionally plunge right into our home star,
creating a ferocious spectacle.
- Sungrazer comets start out their life as normal comets.
They probably live either in the Oort cloud,
or they're short-period comets,
but they've had an unlucky encounter with another planet,
probably Jupiter.
lf they're really, really lucky,
they might just escape and be able to get away
with one close passage by the Sun,
but if they're not lucky,
they just get swallowed up whole by the Sun.
narrator: The Solar and Heliospheric Observatory,
or SOHO, is a space satellite
that has observed 2,OOO comets on suicidal orbits.
The most famous sungrazers are the Kreutz family,
which originated from one giant comet
that broke up into many smaller pieces.
- It's a kind of cool thing to think of a comet
that's lived in the outer solar system
just falling all the way and smashing into the Sun,
but they do.
We see them all the time.
narrator: And some comets do more than self-destruct.
They become the messengers of mass destruction.
lt's estimated that a large comet
may have struck Earth roughly every 40 million years,
based on the amount of craters still visible on our planet.
A comet may have even been responsible
for the most famous extinction event of all time.
- For the Cretaceous-Tertiary extinction event,
the one that took out the dinosaurs
65 million years ago, the jury is still out.
That was thought to be a 1 O-kilometer-sized object,
and there are no asteroids in near-Earth space
that are that large that could impact the Earth,
and there are a number of comets that are that large.
And since it occurred 65 million years ago,
and you would expect a cometary impact
every 40 million years or so,
it may well have been a comet.
narrator: While comets likely slammed into Earth
countless times in the past,
it's been difficult to determine
if an impact crater was made by a comet or asteroid
because the two bodies appear to be similar.
- When we study the fossil records,
a lot of the material is gone,
and just- we simply can't find it,
and it turns out that asteroids and comets
have a lot of materials in common,
so even if you do find extraterrestrial material,
it's really hard to tell
whether it came from an asteroid or from a comet.
narrator: And to complicate matters,
a comet doesn't even have to impact Earth's surface
to ignite a catastrophe.
ln 1 908, a fireball exploded in the atmosphere
above the Tunguska wilderness in Siberia.
The heat and energy from the airburst
propelled downward like a hot tornado.
lt propagated across the forest,
flattening over 800 square miles of trees.
For over a century, some scientists have wondered
if the cosmic intruder was a comet or an asteroid.
- If it were caused by a comet,
you would imagine you'd find in the sediment
some record of unusual things,
like a ratio of helium 3 to helium 4.
That could be an indication that it may have been a comet.
Now, another possibility is if you find
some strange isotope buried in a lake somewhere.
That's tough. This is not easy.
narrator: While it's been difficult
to substantiate cometary impacts on Earth,
physical proof of their colossal power
exists on the gas giant planets.
And these dramatic events warn that far worse collisions
loom in the future,
with Earth as the potential bull's-eye.
As we have followed the trail of comets through space,
we have passed through the chilliest
and warmest places in our solar system.
We've also investigated whether these icy bodies
have been deliverers and destroyers of life.
And new observations prove many of these ancient bodies
haven't quietly retired to the frigid outer limits
of our solar system.
- We think there are several possible end states for comets.
ln one case, they can actually get pulled right into the Sun.
ln other cases, they can actually get scattered
by one of the planets and kind of get kicked out,
maybe back into the Oort cloud and never seen again.
And finally they can also actually impact a planet.
narrator: We now shuttle back to July 1 994.
We follow a string of 21 comet fragments
called Shoemaker-Levy 9
as they're gravitationally pulled toward the gas giant
planet Jupiter.
- If we were riding on
one of the fragments of the comet Shoemaker-Levy 9,
it would have been truly spectacular
because we're heading toward Jupiter,
and this giant planet is looming ever bigger,
and then-splat!
We crash into it.
We throw up a whole bunch of material from the insides.
lt would be really an amazing journey.
The plumes of material coming out of Jupiter
were superheated gas heated by this collision
and also excavated from the interior of Jupiter.
narrator: Shoemaker-Levy 9 Ieft impact scars
the size of Earth,
driving home the scale of violence
that comets can produce if they slam into our planet.
- If any of those fragments had hit the Earth
rather than Jupiter, we'd have been in serious trouble,
because they were large
and they were coming in extremely rapidly.
But fortunately, big brother Jupiter
took all the hits for us and didn't seem to suffer much
in the way of damage.
narrator: But even with Jupiter acting
as a planetary shield,
comets still sneak by the gas giants
and have close encounters with Earth.
- The good news is,
asteroid impacts are far more likely to occur
because asteroids outnumber comets 1 OO to 1
in near-Earth space.
The bad news is, if we do find a comet
on an Earth-impacting trajectory,
we wouldn't realize it
till it got inside the orbit of Jupiter,
when it started throwing off gas and dust.
- In the very unlikely event that a comet
could get close to the Earth, you would worry about it
because they tend to have high average velocities
relative to an asteroid,
as high as tens of miles a second.
So in other words, they would pack a bigger punch.
narrator: While the frequency of near-Earth asteroids
heightens the risk of impacts,
the speed of comets is equally troubling.
This sobering fact has prompted
I viewer Robin W. from Boulder Colorado, to...
- Robin, that's an important question.
The asteroids are mOre n U merOUS,
so there's more of them that could hit us.
But we can track their trajectories
and maybe do something about one that's gonna hit us,
deflect it for example.
The comets are more rare,
but we have very little warning when they come in.
And also, they move much faster than asteroids,
so there's more energy impacting Earth.
So l would say comets are the most hazardous objects.
narrator: NASA is taking the threat of comets seriously.
So far, tracking satellites
have tagged 84 near-Earth comets,
objects with orbits that come within 28 million miles
of Earth's path around the Sun.
- There are no periodic comets
that currently have Earth's name written on them.
But Jupiter and the other giant planets
occasionally perturb the orbits of comets.
So there could be a periodic comet in the future
that will collide with Earth.
narrator: Since the beginning of recorded history,
over 4,200 comets have been observed,
a mere fraction of the total number of these icy bodies.
This means billions of unknown comets
still lie in wait in the outer reaches of space.
One day, a doomsday comet could be nudged out
and sent on a collision course with Earth.
- If we're on that cosmic highway,
and it's getting into our on-ramp,
we need to worry about it.
And we need to worry about it with very little lead time.
- There is very little we can do,
other than sending a giant bomb toward them
and trying to deflect them.
But that's very difficult
when there's only a few months' warning.
narrator: Just as comets have inspired awe and fear
among our ancestors,
they remain a force to reckon with.
By continuing to track their tails of dust,
we may uncover more clues about these frozen artifacts
of our ancient past.
- It's pretty remarkable if you think about it.
Just a few hundred years ago, we had no idea what they were.
We had no idea what they meant.
And now we've actually been to the surfaces of comets.
We've seen up close and personal what they're really like
and what they're made out of.
So these mysterious objects have meant a lot to humans
throughout our history.
They've been agents of change.
They've been agents of destruction sometimes.
They've maybe been agents of creation.
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