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We've seen the movie.
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A huge asteroid heads towards Earth,
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It smashes through
the atmosphere
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slams into the surface.
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Sends up a huge fireball
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and a deadly shockwave.
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The Earth dies screaming.
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But this is not one of those films.
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This is how the Earth
and humans fight back.
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Putting the apocalypse on hold.
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Planet Earth.
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A cradle of life floating
peacefully through space.
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Or is it?
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Our planet can be one of
the most hostile places in the universe.
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Think about what natural
disasters befall humanity.
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Earthquakes, hurricanes, tornadoes,
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all of these sorts of things,
we can't do anything about those.
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But an asteroid?
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Hey, this is a huge natural disaster
that we can actually prevent.
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When people hear the word asteroid
the first thing that comes to mind
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are the Sci-Fi movies of these very
dangerous asteroids coming to hit us.
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The story of how the
dinosaurs became extinct.
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Yes, there are some asteroids
out there that are dangerous.
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When it comes to finding asteroids
in defending the Earth,
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Scientists are very solidly the heroes.
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Across the world,
teams of planetary protectors
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are working out ways
to cancel the apocalypse.
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They're scanning the skies,
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doing the math,
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designing the tech,
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and making the plans that could ensure
planetary extinctions from space,
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are nothing more than science fiction.
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If you're facing an opponent.
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You need to know a lot about them
in order to defeat them.
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Their size, their strength,
what they're made of, how they move.
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Well, we need to know the
same things about these asteroids.
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Cause we want to knock them out.
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To better understand this opponent,
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Cathy Plesko from Los Alamos
National Laboratory travels to Arizona.
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Around 50 thousand years ago,
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this was Ground Zero for an impact
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that left a crater over 550 ft deep.
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This is Meteor Crater.
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This is, awe inspiring to stand
on the rim of the crater like this and
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see the, the scale of something this large
and feeling this small.
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Understanding just
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how much energy it must have taken
to excavate this much rock.
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The meteor that carved out the crater
landed with the power of a hydrogen bomb.
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But the sky rock was just
130 ft across.
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Meteor Crater is helping us understand
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how speed can turn a small projectile
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into a killer.
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The asteroid came in at about
27 thousand miles an hour
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that is ten times faster than the muzzle
velocity of a bullet coming out of a rifle.
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It comes slamming into the
surface and just explodes
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and that explosion
then opens up the crater.
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The impact shocked the
surrounding solid rock into dust
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and sent an immense shockwave
barreling outwards.
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So it's pretty windy here today,
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but that's nothing
like it would have been
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in the shockwave from an impact.
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Anywhere near by here
would have seen winds
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of thousands of miles an hour
as the shockwave came out.
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Scientists calculate
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there's a 20% chance of such
a hit on earth every century.
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If an asteroid like this struck today,
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it could level a city.
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But Cathy's research
is helping build up our defenses.
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So we think that there's a
variety of ways that we might
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prevent an asteroid
from hitting the Earth.
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My colleagues and I at Los Alamos
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and at Livermore and other places
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can use computer models
on super computers
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to do very careful
high-fidelity simulations.
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To tell us, what's a good idea.
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Maybe what's not a good idea.
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And then be able to
present to policymakers
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okay here's what we can do.
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In comparison to what
Bruce Willis could do.
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The most potent weapon in
the planetary protectors arsenal,
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a nuclear bomb.
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Blowing up an asteroid this
way has its drawbacks,
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it risks showering the Earth
with hundreds of smaller meteors.
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But Cathy's team is working on plans
that would avoid this risk,
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instead, they use a nuclear
weapon to deflect an asteroid.
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So one of the things I do study
is nuclear deflection.
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In some cases
and in the near-term future
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there could be a scenario
where we might need to
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shove something fairly
large out of the way
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and those sorts of things,
if they're large enough,
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we might need to use
a nuclear device to do that.
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We might launch a nuclear device
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detonate it above the surface of the object
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changing its velocity a little bit.
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Detonating a nuclear
device near an asteroid
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vaporizes part of its surface
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pushing the asteroid off course.
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But firing nuclear
weapons into space
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is no one's first choice.
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So there's some pros and cons
to using nuclear deflection
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there's some situations
where it is definitely
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an appropriate technology
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where it may be the
only option at the time.
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But we hope in the future,
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that will have other methods
at our disposal that are not as
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challenging, diplomatically or politically.
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The race is on, for scientists to
find a way to deflect an asteroid
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without using nuclear weapons.
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We're discovering more
and more about the asteroids
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we're understanding them
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and we're realizing that there
really are ways we can mitigate
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the destructive effects
of an impact on Earth.
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This could be the most important scientific
endeavor humanity has ever undertaken.
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And the best way to cancel the asteroid
apocalypse could be to take them out
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before they even become a threat.
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Our solar system is a dangerous place.
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Fast moving asteroids hurtle through space.
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And many of these rocks are headed our way.
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To counter the asteroid threat
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scientists are drawing up battle plans.
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The very first step
in understanding this hazard
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and in preventing this hazard,
is to find them.
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Not just the big ones that
could end our civilization
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but even the small that
could devastate your city.
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High in the mountains at the
Catalina Sky survey in Arizona
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asteroid Hunter Greg Leonard
is leading the search.
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We are the eyes for the world
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on this night, at this telescope,
on the summit of this mountain.
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By comparing four images
of the same patch of sky
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taken over a 20 minute period.
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Greg can hunt for elusive asteroids
hidden among the stars.
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Because in these images, stars don't move.
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But asteroids do.
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If it's a really bright asteroid,
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we will see some bright points of light
tracking across the four images.
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You have to kiss a lot of frogs
before you get a prince or a princess
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and this is the case tonight
as it is almost every night.
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Here we go!
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This is a real object.
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You can see it's moving
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across the sky hear from
the lower right to the upper left
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we are very, very excited to
have discovered one tonight.
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Because this is an object that's
approaching near Earth space.
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Likely in the neighborhood of Earth.
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Greg's research reveals
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this 100 ft asteroid could get
as close as 630 thousand miles to Earth.
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That's less than three times
the distance to the Moon.
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And in the future, this asteroid's orbit
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could move closer to Earth.
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Even onto a collision course.
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If that happens,
we need to be ready for it.
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The earlier we spot it,
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the best chance we
have of altering its course.
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Space is so big and
the Earth is so small
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and the asteroid would be
starting from so far away,
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that if you just
deflected it a little bit
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gave it a little nudge,
a tiny course correction
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by the time it got to where
the Earth's region is,
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it would miss us completely.
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To do that, we need to move
asteroids off their trajectory.
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Think of a golf swing,
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hook or shank the ball by just
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one degree off of the tee
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and you'll miss the green completely.
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Now, scale that up to asteroids.
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Over time, space rocks can leave
their home turf of the asteroid belt
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becoming threatening near-earth objects
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30 million miles away
that could one day hit our planet.
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But if planetary protectors can
change the course of a dangerous object
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by just a tenth of a degree,
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they'd miss the Earth completely.
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And scientists have come up
with a very direct way to do it.
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In a football game, if
somebody on the defense has
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seen the quarterback running
into the endzone, what do they do?
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Boom, hit him, knock him out of bounds,
knock them down, do something like that.
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That's what we want to do with asteroids.
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So if we send something moving
towards an asteroid very quickly to hit it
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we call that a kinetic impactor.
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Slams into it really hard,
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changes not just the velocity of
the asteroid but also its trajectory.
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Scientists have already intercepted
asteroid like objects in space
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2005, the Deep Impact Spacecraft
arrived at Temple One
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a comet half the size of Manhattan.
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This spacecraft shot a
little probe at the comet.
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Like a bullet, it slammed into Temple One
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picking up material from the surface.
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Research into kinetics impactors continues.
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In 2022,
a spacecraft called Dart
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will slam into an asteroid
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at over 13 thousand miles an hour.
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That transfer of momentum,
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would change the velocity
of the asteroid, just a little bit
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maybe, a fraction of a mile per hour.
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But over maybe a decade
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that change in velocity,
even though it's very tiny, would add up
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to a change in position big enough
to completely miss the Earth.
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Knocking a giant space rock
off course may sound unusual
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but astronomers have discovered,
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that in space, it's happened a lot.
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When you have a lot of
traffic driving on the highway
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and a lot of lane
changing going on.
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Sooner or later there's
going to be a fender bender
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and that happens in
our solar system as well.
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It's a busy place out
there in the asteroid belt
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asteroids will run into each other
at many miles per second.
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Relative speeds.
And when that happens, the sparks fly.
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If you started with two asteroids
and they collided,
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suddenly, you'd have ten asteroids.
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Those ten asteroids are
now going to collide again
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and now you have
a hundred asteroids.
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Those asteroids will collide
and now you have
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a thousand, a million, a billion,
possible impactors for the Earth.
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But this war isn't just a numbers game,
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because asteroids aren't
all built out of the same stuff.
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So we're going to need,
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different kinds of weapons
to take each type out.
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Across the world
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planetary protectors are
developing battle strategies
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to save us from a
major asteroid impact.
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But there's millions of
asteroids in the solar system
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and each one presents
a different type of threat.
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Their speed, size and
distance from the earth
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help dictate the
degree of danger.
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The more we can really
understand about an asteroid,
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the better prepared we are
to be able to defend against it.
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This is definitely a case of
'Know thy enemy'
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we need to know something
about the properties of these objects
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if we have any hope of a moving a
threatening one out of our path one day.
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But scientists are realizing
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that an asteroid's composition
could be the deadliest factor.
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Knowing what asteroids are made of
can help us find chinks in their armor.
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Marina Brozovic from the
center for near-earth object studies
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uses a technology developed
during World War II.
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00:16:36,190 --> 00:16:37,589
Radar.
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00:16:40,390 --> 00:16:45,766
Planetary radar is really like a
big cousin of airport radar and so
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the same way like the airport is tracking
airplanes we are tracking asteroids.
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That are, you know, hundreds of thousands
sometimes millions of kilometers away.
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00:16:54,990 --> 00:16:57,177
Another thing that radars do is
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they tell us about how
this asteroid looks like.
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00:17:01,290 --> 00:17:04,262
You to know: What's their size?
What's their shape?
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00:17:04,287 --> 00:17:06,666
What's their chemical composition?
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Considering the detail
that we see on the surface,
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00:17:08,910 --> 00:17:11,824
short of sending a spacecraft,
you cannot achieve that.
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So radar is, in a way, it's
own little space mission.
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Radar shows that asteroids
can be made of rock,
246
00:17:20,990 --> 00:17:22,284
metal,
247
00:17:23,109 --> 00:17:26,166
or a combination of the two.
248
00:17:27,190 --> 00:17:31,966
This is crucial information for
calculating how to deal with them.
249
00:17:33,690 --> 00:17:37,300
So metallic asteroids are far more dense
250
00:17:37,370 --> 00:17:39,113
then a normal rocky asteroid.
251
00:17:39,138 --> 00:17:43,733
So an impact from a big iron asteroid
could have much more energy
252
00:17:43,770 --> 00:17:47,140
for the same size asteroid
that was just rocky.
253
00:17:48,030 --> 00:17:49,630
Just as a metal cannonball
254
00:17:49,655 --> 00:17:53,006
would do more damage
than a similar sized rock,
255
00:17:53,030 --> 00:17:58,406
metallic asteroids could be far
more deadly than rocky asteroids.
256
00:17:59,430 --> 00:18:04,106
But scientists have now discovered that
most asteroids are less like cannonballs
257
00:18:04,130 --> 00:18:08,106
and more like vast
cosmic shotgun shells.
258
00:18:10,130 --> 00:18:12,176
Most of the asteroids,
they're not a single object,
259
00:18:12,201 --> 00:18:15,130
they're not monolithic
but instead, their rubble piles.
260
00:18:15,230 --> 00:18:18,278
So they consist of many
smaller rocks and pebbles
261
00:18:18,303 --> 00:18:21,370
and grains and pieces of sand.
262
00:18:21,470 --> 00:18:24,846
And all of this is held
very loosely with gravity.
263
00:18:25,770 --> 00:18:29,813
Rubble pile asteroids like
the peanut shaped Itokawa
264
00:18:29,838 --> 00:18:34,246
probably formed from violent
collisions between asteroids.
265
00:18:36,370 --> 00:18:41,546
Initially, the rocky debris from
these collisions scatters like shrapnel.
266
00:18:42,170 --> 00:18:48,146
Then gravity can draw some of the
rocks loosely back together again.
267
00:18:50,970 --> 00:18:53,689
The structure of rubble
pile asteroids presents
268
00:18:53,714 --> 00:18:57,370
a major challenge to
our planetary protectors.
269
00:18:59,370 --> 00:19:04,346
How can our science heroes
save us from a pile of rubble?
270
00:19:04,370 --> 00:19:06,570
If the object is a
solid mass of metal.
271
00:19:06,720 --> 00:19:11,090
It's going to respond to an impact
or an explosion in a far different way
272
00:19:11,140 --> 00:19:14,100
than if it's just a loosely
bound rubble pile
273
00:19:14,125 --> 00:19:16,340
barely held together
by its own gravity.
274
00:19:16,440 --> 00:19:18,709
Well, they're very, very
delicate objects
275
00:19:18,734 --> 00:19:22,516
and so those objects need
some special consideration.
276
00:19:22,540 --> 00:19:26,316
We can't just go slamming
into them necessarily.
277
00:19:28,040 --> 00:19:30,633
Smashing into a rubble pile asteroid
278
00:19:30,658 --> 00:19:34,340
would be like
kicking a pile of leaves.
279
00:19:34,440 --> 00:19:39,516
Thousands of smaller rocks would
go hurtling out in every direction.
280
00:19:39,915 --> 00:19:45,915
They'd be undetectable, unpredictable
and could continue to head our way.
281
00:19:47,340 --> 00:19:50,816
But we have a plan.
282
00:19:52,040 --> 00:19:54,530
Instead of using violent force,
283
00:19:54,555 --> 00:19:58,716
we could use the
gentle tug of gravity.
284
00:20:00,040 --> 00:20:03,950
So instead of this ham-fisted approach
of whacking it and then just walking away.
285
00:20:04,020 --> 00:20:05,096
We need something.
286
00:20:05,220 --> 00:20:07,911
We need something more careful,
something more precise
287
00:20:07,936 --> 00:20:11,020
and that's where the
gravity tractor comes in.
288
00:20:14,120 --> 00:20:16,996
Rubble piles of rock may be small,
289
00:20:17,020 --> 00:20:18,535
but it has gravity.
290
00:20:18,560 --> 00:20:21,904
And if we send up a probe
that has the mass of say, a ton.
291
00:20:21,970 --> 00:20:24,150
It has gravity too.
Now, not much.
292
00:20:24,230 --> 00:20:25,430
But it's there.
293
00:20:25,560 --> 00:20:27,916
And if you put it near the asteroid,
294
00:20:27,940 --> 00:20:30,107
You can actually use
the mutual gravity,
295
00:20:30,132 --> 00:20:35,340
the attraction between them,
to tug the asteroid into a safe orbit.
296
00:20:37,090 --> 00:20:40,266
All you have to do is park a
spacecraft next to the asteroid,
297
00:20:40,290 --> 00:20:41,317
Hover it there,
298
00:20:41,342 --> 00:20:44,926
don't let the gravity of the asteroid and
the spacecraft pull each other together,
299
00:20:44,950 --> 00:20:47,492
and let the gravity of the spacecraft
300
00:20:47,517 --> 00:20:51,250
act as a tow line to pull
the asteroid out of the way.
301
00:20:53,450 --> 00:20:55,089
This sounds like science fiction,
302
00:20:55,114 --> 00:20:58,844
but it turns out the physics
of this is relatively simple.
303
00:20:58,880 --> 00:21:00,956
And we can do it.
304
00:21:04,180 --> 00:21:06,329
But gravity tractors only work
305
00:21:06,354 --> 00:21:10,380
if we can accurately track the
movements of these asteroids.
306
00:21:12,480 --> 00:21:16,756
Problem is, there's a
massive complicating factor
307
00:21:16,780 --> 00:21:19,570
at the center of
our solar system.
308
00:21:20,500 --> 00:21:22,776
The Sun.
309
00:21:40,500 --> 00:21:45,376
Planetary protectors want to
put the apocalypse on hold.
310
00:21:48,000 --> 00:21:49,569
Their mission:
311
00:21:49,594 --> 00:21:54,800
Protect the Earth from these
seemingly inevitable asteroid impacts.
312
00:21:57,100 --> 00:22:02,176
But to do that, they need
to predict their every move.
313
00:22:03,600 --> 00:22:07,961
In a constantly changing
Solar system, that's not easy.
314
00:22:07,986 --> 00:22:10,957
We measure their orbits
and we can draw up maps of
315
00:22:10,982 --> 00:22:13,724
all their orbits as
we see them today.
316
00:22:13,780 --> 00:22:16,398
But we know that it's
not a static population,
317
00:22:16,423 --> 00:22:22,356
that it's dynamic, things are
constantly evolving in the asteroid belt.
318
00:22:22,380 --> 00:22:24,895
It's not just about size with asteroids.
319
00:22:24,920 --> 00:22:26,656
You have to understand the density,
320
00:22:26,680 --> 00:22:30,556
the orbit, the speed,
in order to really tackle it.
321
00:22:32,180 --> 00:22:36,856
Collisions can set asteroid
debris off on new orbits.
322
00:22:38,880 --> 00:22:46,656
But there's another factor at play, the
immense gravity of the gas giant, Jupiter.
323
00:22:46,680 --> 00:22:49,422
Jupiter is the most massive
planet in the solar system and
324
00:22:49,447 --> 00:22:51,556
it's sitting outside
the asteroid belt.
325
00:22:51,600 --> 00:22:54,333
It's gravity can tweak
and tug these asteroids
326
00:22:54,358 --> 00:22:56,306
and make their
orbits more elliptical.
327
00:22:56,330 --> 00:22:58,120
Sending them in towards the Sun.
328
00:22:58,170 --> 00:23:00,050
Crossing Earth's orbit.
329
00:23:01,570 --> 00:23:06,846
Modeling Jupiter's effect on
millions of asteroids is hard enough.
330
00:23:06,870 --> 00:23:13,146
Now add the influence of some
of the asteroid belts biggest bruisers.
331
00:23:13,170 --> 00:23:16,539
300 mile wide rocks like Vesta
332
00:23:17,464 --> 00:23:20,546
and Pallas.
333
00:23:21,370 --> 00:23:26,146
A tricky task becomes near impossible.
334
00:23:29,670 --> 00:23:36,646
But gravity isn't the only
force creating orbital chaos.
335
00:23:36,670 --> 00:23:41,048
This is the asteroid Bennu.
336
00:23:41,073 --> 00:23:46,346
There's one chance in 2700
it'll hit the Earth.
337
00:23:46,370 --> 00:23:50,068
But Bennu's orbit keeps changing.
338
00:23:50,093 --> 00:23:56,546
In the last 18 years, it shifted
over a hundred miles off course
339
00:23:56,570 --> 00:24:00,746
and the culprit could be the Sun.
340
00:24:00,770 --> 00:24:03,086
So what can change
the orbit of an asteroid?
341
00:24:03,110 --> 00:24:05,300
It's easy to think
of these large rocks
342
00:24:05,325 --> 00:24:08,386
passing by each other tugging
on each other gravitationally.
343
00:24:08,410 --> 00:24:12,786
But could the most dramatic changes
be due something as gentle as sunlight?
344
00:24:12,810 --> 00:24:15,092
It might feel very subtle,
but the sunlight,
345
00:24:15,117 --> 00:24:18,614
on our bodies,
exerts a subtle pressure.
346
00:24:18,680 --> 00:24:22,340
The fact that you're hotter on one side
than on the other side,
347
00:24:22,390 --> 00:24:27,080
actually exerts a kind of a
thrust that can move you around.
348
00:24:27,670 --> 00:24:32,646
Sunlight is made up of tiny
packets of energy called photons.
349
00:24:32,670 --> 00:24:34,649
When photons hit an asteroid
350
00:24:34,674 --> 00:24:37,546
they pass on a tiny
amount of momentum
351
00:24:37,570 --> 00:24:40,446
and a tiny amount of heat.
352
00:24:41,570 --> 00:24:44,006
Let's actually, you know,
let's imagine this situation,
353
00:24:44,031 --> 00:24:47,037
here's our asteroid,
in reality, this might be,
354
00:24:47,062 --> 00:24:49,593
10 miles across or a mile across,
something like that.
355
00:24:49,620 --> 00:24:52,320
Here's our asteroid,
here's the Sun.
356
00:24:52,390 --> 00:24:55,120
This asteroid is orbiting the Sun this way.
357
00:24:55,150 --> 00:24:58,916
This face of the asteroid is being
warmed by the heat from the Sun.
358
00:24:58,940 --> 00:25:03,261
Out here on the back side facing the
cold vacuum of space it's a lot colder.
359
00:25:03,286 --> 00:25:06,754
In fact, I can even feel
it already with my hands.
360
00:25:06,800 --> 00:25:09,490
The warm side that's being
illuminated by sunshine
361
00:25:09,530 --> 00:25:13,710
actually re-radiates that heat in
the infrared portion of the spectrum.
362
00:25:13,760 --> 00:25:17,050
All of that infrared radiation
off the side of the asteroid
363
00:25:17,075 --> 00:25:19,536
acts like a like a little
rocket motor in a way.
364
00:25:19,560 --> 00:25:22,936
It actually pushes on the asteroid.
365
00:25:22,960 --> 00:25:26,551
This is known as the Yarkovsky effect,
366
00:25:26,576 --> 00:25:29,036
it's a slow process.
367
00:25:29,060 --> 00:25:31,900
The asteroid is pushed by a force
368
00:25:31,925 --> 00:25:37,660
equal to the weight of
a few grapes on Earth.
369
00:25:37,760 --> 00:25:43,136
But as Bennu circles the Sun
it heats up on one side
370
00:25:43,160 --> 00:25:47,236
which moves it into a different orbit.
371
00:25:49,760 --> 00:25:52,536
The Yarkovsky effect is
actually a bit of a problem.
372
00:25:52,560 --> 00:25:55,217
If there were just gravity
acting on these asteroids
373
00:25:55,242 --> 00:25:58,125
then we can predict where all
the asteroids and planets will be
374
00:25:58,150 --> 00:26:01,086
and we'd be able to figure out
the trajectory of these asteroids
375
00:26:01,111 --> 00:26:02,608
many years in the future.
376
00:26:02,660 --> 00:26:04,450
But with the Yarkovsky effect,
377
00:26:04,490 --> 00:26:07,276
that actually changes it in
ways that are difficult to predict.
378
00:26:07,301 --> 00:26:09,877
Because it depends on
how dark the asteroid is,
379
00:26:09,902 --> 00:26:12,214
whether it's spinning,
what shape it is
380
00:26:12,290 --> 00:26:15,830
and so it makes the orbit of the asteroid
much, much more difficult to predict
381
00:26:15,920 --> 00:26:18,441
a long time into the future.
382
00:26:19,766 --> 00:26:24,938
The Yarkovsky effect makes predicting
the movement of asteroids like Bennu,
383
00:26:24,963 --> 00:26:26,795
even harder.
384
00:26:26,820 --> 00:26:31,324
But our planetary protectors
are an ingenious bunch
385
00:26:31,349 --> 00:26:34,189
and they're attempting to
use the Yarkovsky effect
386
00:26:34,214 --> 00:26:37,621
to create a new
weapon for their armory.
387
00:26:37,720 --> 00:26:39,860
So the Yarkovsky effect we know can
388
00:26:39,885 --> 00:26:44,095
change asteroid orbits pretty dramatically.
389
00:26:44,119 --> 00:26:46,544
It's an effect that we could use
390
00:26:46,620 --> 00:26:48,540
to move asteroids ourselves.
391
00:26:48,570 --> 00:26:51,456
If we could change the way
the asteroid is heated by the Sun.
392
00:26:51,480 --> 00:26:54,020
By changing its color or
393
00:26:54,080 --> 00:26:57,456
changing its shape so that it
gets heated in a very specific way,
394
00:26:57,480 --> 00:27:00,656
That we could change its orbit that way.
395
00:27:01,580 --> 00:27:05,280
If scientists could send
a satellite to an asteroid,
396
00:27:05,305 --> 00:27:08,040
it could use black or white paint
397
00:27:08,065 --> 00:27:11,604
to increase or decrease
the heating effect.
398
00:27:12,780 --> 00:27:15,556
But at the University
of Southern California,
399
00:27:15,580 --> 00:27:19,666
a team of scientists are
working on a higher tech solution.
400
00:27:19,691 --> 00:27:22,380
They're trying to one-up
the Yarkovsky effect
401
00:27:22,480 --> 00:27:28,256
using a space-based
laser called D-Star.
402
00:27:28,280 --> 00:27:31,880
Let's say we see an asteroid
that's on its way towards the Earth.
403
00:27:31,940 --> 00:27:35,452
We can use space
lasers to zap the asteroid.
404
00:27:35,477 --> 00:27:37,454
You vaporize the surface material.
405
00:27:37,530 --> 00:27:40,602
That turns into a gas
which expands very quickly
406
00:27:40,627 --> 00:27:42,526
and that acts like a rocket.
407
00:27:42,550 --> 00:27:45,485
And so you can use
that to push the asteroid
408
00:27:45,510 --> 00:27:47,750
into a safer path as well.
409
00:27:49,650 --> 00:27:52,435
Space lasers are
another powerful weapon
410
00:27:52,460 --> 00:27:56,776
for our planetary protectors
fight against asteroids.
411
00:27:57,950 --> 00:28:00,726
They joined gravity tractors,
412
00:28:00,750 --> 00:28:03,767
kinetic impactors
413
00:28:03,792 --> 00:28:07,650
and nuclear weapons
in the armory.
414
00:28:07,750 --> 00:28:11,626
But there is one very big problem.
415
00:28:11,750 --> 00:28:14,651
All of the methods of defending
against asteroids that we've mentioned
416
00:28:14,776 --> 00:28:16,550
are technologically possible.
417
00:28:16,650 --> 00:28:18,828
The thing that's a little
bit nerve-wracking is that
418
00:28:18,853 --> 00:28:23,526
none of them are actually
ready to go right now.
419
00:28:23,550 --> 00:28:26,700
So it's not time to cancel
the apocalypse yet.
420
00:28:26,725 --> 00:28:29,712
We've made a lot of progress
especially in the last few years.
421
00:28:29,737 --> 00:28:31,406
But we're not really there yet.
422
00:28:31,431 --> 00:28:36,974
But we could get to that point
within the next maybe 10 or 15 years.
423
00:28:39,850 --> 00:28:42,326
But don't panic just yet.
424
00:28:42,350 --> 00:28:46,481
Turns out the Earth has
a built-in defense system
425
00:28:46,506 --> 00:28:51,826
that can burn up asteroids,
before they ever hit the ground.
426
00:29:08,930 --> 00:29:14,106
Arizona, June 2nd 2016.
427
00:29:14,130 --> 00:29:19,506
A 5 ft wide rock hurdles
towards the Earth.
428
00:29:19,530 --> 00:29:24,606
It's moving at over
40 thousand miles per hour
429
00:29:24,630 --> 00:29:29,706
and as it streaks overhead,
it lights up the sky.
430
00:29:32,030 --> 00:29:33,951
In the very early morning hours,
431
00:29:33,976 --> 00:29:37,206
an asteroid came screaming
into the Earth's atmosphere
432
00:29:37,230 --> 00:29:39,020
far faster than a rifle bullet.
433
00:29:39,060 --> 00:29:43,616
There was a fireball that lit up the
Red Rocks all around us that night.
434
00:29:43,640 --> 00:29:46,127
It was bright enough to burn
out cameras on the ground
435
00:29:46,152 --> 00:29:48,840
from NASA that were
watching for fireballs.
436
00:29:49,940 --> 00:29:53,134
The asteroid is just
seconds away from impact
437
00:29:53,159 --> 00:29:56,540
and major damage seems inevitable.
438
00:29:59,240 --> 00:30:05,734
But the asteroid never
makes it to the ground, why?
439
00:30:05,759 --> 00:30:10,930
We do have a natural barrier
against at least small asteroid impacts.
440
00:30:11,010 --> 00:30:12,880
And let me give you a
hint about what that is.
441
00:30:18,650 --> 00:30:20,811
The air around us
seems too tenuous
442
00:30:20,836 --> 00:30:23,126
to actually defend
against a threat from space.
443
00:30:23,150 --> 00:30:28,526
But in fact, the atmosphere is sort of
the last line of defense against asteroids.
444
00:30:29,450 --> 00:30:35,926
One day our planetary protectors will
be ready to save us from asteroid strikes.
445
00:30:35,950 --> 00:30:42,126
Until then, we'll have to rely on
the Earth's built in defense system,
446
00:30:42,150 --> 00:30:45,226
the atmosphere.
447
00:30:45,250 --> 00:30:48,230
We know for a fact that our
atmosphere acts like a shield.
448
00:30:48,260 --> 00:30:52,613
Because space rocks
come the earth every day.
449
00:30:52,637 --> 00:30:54,835
Some of them are tiny,
some of them are a bit larger.
450
00:30:54,860 --> 00:30:58,463
But what's happening is that as they
enter the atmosphere at high speed
451
00:30:58,488 --> 00:31:01,160
the friction burns them up.
452
00:31:01,960 --> 00:31:05,736
Even though the top layers
of the atmosphere are very thin,
453
00:31:05,760 --> 00:31:12,336
compared to the vacuum of space,
they're extremely dense.
454
00:31:12,360 --> 00:31:15,242
As rocky asteroids hurtle
through the atmosphere,
455
00:31:15,267 --> 00:31:21,836
friction and air pressure can heat them
to over 3 thousand degrees Fahrenheit.
456
00:31:21,860 --> 00:31:25,536
The larger the asteroid,
the longer it takes to burn up.
457
00:31:25,560 --> 00:31:31,936
And for these larger rocks,
the effects can be dramatic.
458
00:31:31,960 --> 00:31:35,216
If there's a rock that's big enough
that it doesn't burn out very quickly.
459
00:31:35,240 --> 00:31:38,879
We call that a bolide, and as the
bolide falls through the atmosphere,
460
00:31:38,904 --> 00:31:42,858
it creates a spectacular show,
called a fireball.
461
00:31:44,160 --> 00:31:50,336
In February 2013, the town of Chelyabinsk
in Russia had it's own fireball
462
00:31:50,360 --> 00:31:55,036
when a 60 ft wide space
rock barreled through the sky.
463
00:31:58,460 --> 00:32:03,436
This asteroid was
bigger than a school bus
464
00:32:03,460 --> 00:32:07,250
and it traveled at 11 miles per second.
465
00:32:07,290 --> 00:32:10,389
It got super hot,
broke up into small pieces,
466
00:32:10,414 --> 00:32:13,566
those pieces then rammed
through the atmosphere.
467
00:32:13,590 --> 00:32:16,676
When all of that vast
energy of motion of this rock
468
00:32:16,700 --> 00:32:21,154
was converted into light
and heat, it exploded.
469
00:32:23,270 --> 00:32:27,346
The Chelyabinsk meteor is
the largest natural object seen
470
00:32:27,371 --> 00:32:31,146
entering the atmosphere
in over a hundred years.
471
00:32:33,370 --> 00:32:37,055
It explodes 12 miles
above the Earth's surface
472
00:32:37,080 --> 00:32:40,146
with the power of
30 nuclear bombs.
473
00:32:43,970 --> 00:32:51,646
The blast causes over 15 hundred injuries
and damages seven thousand buildings.
474
00:32:51,670 --> 00:32:54,846
But if it wasn't for the protective
shielding of our atmosphere,
475
00:32:54,870 --> 00:32:59,046
the results would have been far worse.
476
00:33:01,270 --> 00:33:02,364
The problem is,
477
00:33:02,389 --> 00:33:06,750
the atmosphere can only protect us
from rocky and rubble pile asteroids
478
00:33:06,775 --> 00:33:09,494
up to around 100 ft wide.
479
00:33:11,270 --> 00:33:15,246
And there is something else
much more dangerous to consider,
480
00:33:15,270 --> 00:33:18,046
metallic asteroids.
481
00:33:18,070 --> 00:33:20,412
If you had a rocky asteroid hitting,
482
00:33:20,437 --> 00:33:22,724
or a rubbly rocky asteroid hitting,
483
00:33:22,800 --> 00:33:24,237
It wouldn't make it to the ground.
484
00:33:24,262 --> 00:33:26,555
An asteroid that's
around a 100 ft across
485
00:33:26,580 --> 00:33:28,924
would actually blow up in the sky.
486
00:33:30,500 --> 00:33:33,030
But if a 100 ft metallic
asteroid were to hit,
487
00:33:33,070 --> 00:33:34,800
First of all you wouldn't
have much warning
488
00:33:34,825 --> 00:33:36,594
it would hit the top
of the atmosphere
489
00:33:36,790 --> 00:33:39,907
and then would hit the
ground about a second later.
490
00:33:39,932 --> 00:33:42,923
Causing an enormous
explosion that would
491
00:33:42,948 --> 00:33:46,514
open up a crater that
would be about a mile across.
492
00:33:46,560 --> 00:33:51,516
You'd have a flattened ruin
of remnants of buildings.
493
00:33:51,540 --> 00:33:58,216
Millions dead from the shockwave
that would be radiating out
494
00:33:58,240 --> 00:34:04,216
and layer of dust falling back down
over the next minutes and hours.
495
00:34:05,640 --> 00:34:08,560
The metallic asteroid punches
through the atmosphere
496
00:34:08,585 --> 00:34:13,916
because it's too hard for friction and
air pressure to break up completely.
497
00:34:13,940 --> 00:34:20,316
So it slams into the ground
in a catastrophic explosion.
498
00:34:20,340 --> 00:34:26,316
Metallic asteroids could be our
planetary protectors greatest foe.
499
00:34:28,440 --> 00:34:34,416
But turns out the Earth could
have another built in defense.
500
00:34:35,540 --> 00:34:41,916
We know an asteroid punched through the
atmosphere and killed off the dinosaurs.
501
00:34:41,940 --> 00:34:46,716
But research is showing our
planet could have saved them.
502
00:34:46,740 --> 00:34:49,416
The dinosaurs were incredibly unlucky.
503
00:34:49,440 --> 00:34:51,855
Even if the object does
make it past our atmosphere
504
00:34:51,880 --> 00:34:55,540
we still have another
line of defense.
505
00:34:55,640 --> 00:35:02,616
It's not always what an asteroid is
made of that makes the difference.
506
00:35:02,640 --> 00:35:08,030
Sometimes, it's all about where it is.
507
00:35:25,850 --> 00:35:30,092
Our planetary protectors
are creating technologies
508
00:35:30,417 --> 00:35:34,850
to divert a potentially
catastrophic asteroid.
509
00:35:37,150 --> 00:35:40,026
But until their armory is complete,
510
00:35:40,050 --> 00:35:44,126
the Earth has its own defensive strategy.
511
00:35:45,950 --> 00:35:50,326
One of the things that is sure, is that we
will be hit by an asteroid or comet again.
512
00:35:50,350 --> 00:35:53,090
It may not happen for millions
of years, but it will happen.
513
00:35:53,130 --> 00:35:55,728
And on that day
the thing that will differentiate
514
00:35:55,753 --> 00:35:59,545
between a just being a very bad day
and it being a global catastrophe,
515
00:35:59,580 --> 00:36:02,160
is location, location, location.
516
00:36:04,990 --> 00:36:06,966
Some regions of the Earth
517
00:36:06,990 --> 00:36:12,566
could actually reduce the
damage done by a killer asteroid.
518
00:36:12,590 --> 00:36:15,445
How do we know that?
519
00:36:15,470 --> 00:36:16,866
Dinosaurs.
520
00:36:16,890 --> 00:36:21,860
65 million years ago,
the dinosaurs had a very bad day.
521
00:36:21,884 --> 00:36:26,986
They had the bad luck
to be wiped out by an asteroid impact.
522
00:36:29,510 --> 00:36:32,588
We thought we
knew the full story.
523
00:36:32,613 --> 00:36:37,886
But researchers have
revealed something astonishing.
524
00:36:37,910 --> 00:36:43,186
If the asteroid had hit
the earth just minutes later.
525
00:36:43,210 --> 00:36:50,420
Dinosaurs may still roam
the planet today, but how?
526
00:36:50,470 --> 00:36:52,997
This object hit right at
the Yucatan Peninsula.
527
00:36:53,022 --> 00:36:56,354
It caused an incredible tsunami
that flooded North America
528
00:36:56,379 --> 00:36:59,670
but it also threw a lot
of sulfates into the air.
529
00:37:02,970 --> 00:37:06,521
The six mile wide asteroid
landed in shallow seas
530
00:37:06,546 --> 00:37:09,846
in what is now
the Gulf of Mexico.
531
00:37:12,370 --> 00:37:17,446
It vaporized rocks in the
sea floor of the continental shelf.
532
00:37:17,470 --> 00:37:23,546
The impact blasted out trillions of
tons of gases into the atmosphere.
533
00:37:23,570 --> 00:37:26,792
Triggering catastrophic climate change.
534
00:37:26,817 --> 00:37:32,246
70% of all life on Earth became extinct.
535
00:37:32,270 --> 00:37:35,146
Including the dinosaurs.
536
00:37:35,170 --> 00:37:36,840
The thing that's kind of tragic
537
00:37:36,870 --> 00:37:39,433
is that the Earth had
rotated just a little bit more,
538
00:37:39,458 --> 00:37:42,490
when that impact hit,
it would have been in deeper ocean.
539
00:37:42,520 --> 00:37:46,596
And there wouldn't have been all
that vaporized rock and sulphur.
540
00:37:50,520 --> 00:37:54,796
Our planet spins at a
thousand miles an hour.
541
00:37:54,820 --> 00:38:01,196
70% of the earth's
surface is covered by ocean.
542
00:38:01,220 --> 00:38:07,196
With a little luck, the dinosaur destroyer
could have struck in deeper water.
543
00:38:07,420 --> 00:38:08,944
There's no good place on the earth
544
00:38:08,969 --> 00:38:13,514
to take a five mile wide asteroid strike,
there's just no good place.
545
00:38:13,539 --> 00:38:15,855
Some places are
worse than others and
546
00:38:15,880 --> 00:38:20,896
the Yucatan Peninsula with that much
sulfur was one of the worst possible.
547
00:38:20,920 --> 00:38:23,890
So it's just not going to be a good day.
548
00:38:25,990 --> 00:38:32,666
The asteroid that killed the dinosaurs,
allowed us mammals to take over the Earth.
549
00:38:32,690 --> 00:38:39,466
Fortunately, these giant asteroids
only strike once every few million years.
550
00:38:39,790 --> 00:38:44,163
But every two thousand years or so,
551
00:38:44,188 --> 00:38:50,066
a rock about the size of
a football field hits Earth.
552
00:38:50,090 --> 00:38:52,784
What would happen
if one of these smaller,
553
00:38:52,809 --> 00:38:56,666
more common asteroids,
were to hit the ocean?
554
00:38:56,690 --> 00:38:58,346
Think of something
like the Pacific Ocean,
555
00:38:58,371 --> 00:39:00,052
there's a lot of
coastline there.
556
00:39:00,076 --> 00:39:02,866
And so you have many,
many people that are at risk.
557
00:39:02,965 --> 00:39:05,465
Most of the Earth's surface is ocean.
558
00:39:05,490 --> 00:39:08,137
So it's a much
more likely scenario,
559
00:39:08,162 --> 00:39:10,066
for an asteroid to hit the ocean.
560
00:39:10,090 --> 00:39:13,896
And so the question is,
how much of a tsunami risk is there?
561
00:39:16,620 --> 00:39:19,496
Scientist have modeled
what would happen.
562
00:39:19,520 --> 00:39:24,796
If an asteroid strikes
different places in the ocean.
563
00:39:24,820 --> 00:39:26,863
It was studied in
three dimensions
564
00:39:26,888 --> 00:39:30,275
with different types of
compositions, different ocean depths,
565
00:39:30,300 --> 00:39:32,220
different entry angles
566
00:39:32,320 --> 00:39:39,396
and found out that the
continental shelf actually saves us.
567
00:39:39,420 --> 00:39:43,496
The continental shelf is an
underwater landmass that extends
568
00:39:43,520 --> 00:39:47,496
around 50 miles beyond the coast.
569
00:39:47,520 --> 00:39:50,917
So when an asteroid
hundreds of feet across
570
00:39:50,942 --> 00:39:53,596
slams into the deep ocean,
571
00:39:53,620 --> 00:39:57,219
the shallow sea created
by the continental shelf
572
00:39:57,244 --> 00:40:02,296
could force a tsunami
to collapse before it hits land.
573
00:40:02,320 --> 00:40:07,296
It seems, the ocean has our back.
574
00:40:07,320 --> 00:40:11,802
For the deep ocean we think that
asteroids smaller than 400 ft across,
575
00:40:11,827 --> 00:40:15,096
which is quite large,
are not a tsunami risk
576
00:40:15,120 --> 00:40:19,996
and so we don't need to worry as
much as we thought we did, about it.
577
00:40:20,020 --> 00:40:22,012
That shallow part of the water
578
00:40:22,037 --> 00:40:26,020
actually buffers any tsunami
wave that might be coming in.
579
00:40:32,720 --> 00:40:35,896
So our planet has defense mechanisms
580
00:40:35,920 --> 00:40:41,896
and our scientists are devising plans
that will take the fight to the asteroids.
581
00:40:43,620 --> 00:40:46,696
What they need is time.
582
00:40:48,320 --> 00:40:52,385
Astronomy very well can save the world,
because we're on the lookout
583
00:40:52,410 --> 00:40:55,596
for all the asteroids that may
someday collide with Earth
584
00:40:55,620 --> 00:41:00,696
and if we find them we could
avoid a civilization ending event.
585
00:41:00,720 --> 00:41:03,820
If we have warning time,
we then have the advantage of
586
00:41:03,845 --> 00:41:06,802
being able to think about
the problem, plan for it
587
00:41:06,827 --> 00:41:10,220
and actually build up the technologies
practice the techniques that it's gonna
588
00:41:10,244 --> 00:41:15,396
take to push that asteroid out of the way,
time is definitely an ally for us.
589
00:41:15,420 --> 00:41:20,196
We're not ready to cancel
the apocalypse just yet.
590
00:41:20,220 --> 00:41:24,896
But with the planetary
protection team on the case,
591
00:41:24,920 --> 00:41:27,535
soon, we'll have a fighting chance.
592
00:41:29,060 --> 00:41:32,296
If you want to know what, like an
astronomer's sweatiest nightmare is.
593
00:41:32,320 --> 00:41:37,196
It's an asteroid impact.
It's kinda personal, right?
594
00:41:37,220 --> 00:41:40,228
This is happening right here on Earth.
595
00:41:40,253 --> 00:41:45,196
It's a challenge to us and that's
why we want to prevent them.
596
00:41:45,820 --> 00:41:50,496
The good news is, we actually are on
the cusp of being able to deflect them.
597
00:41:50,520 --> 00:41:55,996
We're almost there we
just have to push it through.
598
00:41:56,020 --> 00:41:58,164
The planet is incredibly resilient.
599
00:41:58,189 --> 00:42:02,824
Even if one specific species or
one specific individual is very fragile,
600
00:42:02,849 --> 00:42:07,596
as a whole, the Earth
is actually quite tough.
601
00:42:07,620 --> 00:42:09,903
It really comes back to,
as human beings:
602
00:42:09,928 --> 00:42:14,096
What is our will to discover, to explore
and understand the solar system?
603
00:42:14,120 --> 00:42:17,247
It becomes very important
when you think about asteroids.
604
00:42:17,272 --> 00:42:19,596
We need to keep scanning the skies.
605
00:42:19,620 --> 00:42:23,696
We need to keep being
scientists to defend the Earth.
606
00:42:26,700 --> 00:42:28,900
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