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A large object suddenly
about to strike our planet.
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The fear and panic that this can inspire
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is the stuff of science fiction movies.
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But scientists say that
this sort of impact event
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could actually happen.
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December, 2006.
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NASA submitted a detailed 270-page report
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to the U.S. Congress.
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This study assessed the risk of an impact
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by what are called near-Earth objects.
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It found that the number
of small space objects
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posing a threat, such as
comets and asteroids,
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came to about 20,000.
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These objects have the potential to
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take out civilization as we know it.
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So we really owe it ourselves
to monitor the skies,
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and find and track all
of the fairly large ones
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that could cause
civilization-ending events.
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It's not a matter of if they will hit.
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It's a matter of when.
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Astronomers around the world have
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joined forces to identify
potentially hazardous objects
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in space with the goal of
protecting Earth from this danger.
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In the course of their surveys
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they have discovered new threats.
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For example, an asteroid that
might collide with Earth
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in the year 2029.
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There would be
extensive damage at the very
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location of the impact,
sort of ground zero.
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When will an object next impact our Earth?
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How are scientists addressing this threat
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from outer space?
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The Sonoma Valley in California.
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This valley has long boasted
prime agricultural land,
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including world famous vineyards.
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But there's someone here
who's thoughts have turned
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from terroir to terror,
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the threat of a potential
asteroid collision.
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Russell Schweickart, nicknamed Rusty.
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Nice to see you.
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He's a former astronaut who flew on
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Apollo Nine, and has circled
the globe 151 times.
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Would you come in?
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Schweickart's space flight
took place in 1969.
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The mission was designed to
check out systems in advance
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of the moon landing scheduled
for later that year.
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The primary objective was to
test fly the Lunar Module,
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piloted by Schweickart, in
the zero gravity of space.
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And Schweickart undertook
the first ever space walk
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without an umbilical cable.
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Separated from his comrades,
he faced all alone
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the blackness of space.
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He was brought face-to-face
with planet Earth's
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exposure to catastrophe.
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The three of us were
looking down at the Earth,
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which is spectacular at
night because of lightning
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and weather fronts and
things, cities lit up.
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It's really beautiful, but
everyone once in a while
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you would see a little flash.
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Earth is constantly exposed to collisions
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with objects from space.
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But Schweickart was the first to experience
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this vulnerability on
such a personal level.
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Shooting stars are meteors,
space objects as small
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as pebbles, or even grains
of sand, whose entry into
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Earth's atmosphere is a
frequently observed phenomenon.
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In 1992, a fireball appeared
suddenly over Pennsylvania
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in the United States, traveling
toward the northeast
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before breaking up.
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Its descent was captured on
camera thanks to the filming
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of a local football game.
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Over Spain in 2004, a shooting
star blazed so brightly
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it could be seen in the middle of the day.
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However, shooting stars are
created by objects so small
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that they almost always
burn up before they can
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cause injury or damage.
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Tunguska, Siberia.
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Here on June 30th, 1908
occurred a catastrophic event.
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A gigantic explosion.
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Scientists from the Soviet
Academy of Sciences
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who reached the remote
location were astounded at
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the spectacle that confronted them,
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millions of felled trees.
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The area of leveled forest measured some
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2,000 square kilometers, the size of Tokyo.
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The fallen trees radiated
away from one spot.
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It was hypothesized that
this was the epicenter
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of an asteroid impact.
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But there was a mystery.
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Not a single fragment of
meteorite, that is to say,
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no asteroid remnant was to
be found on the ground.
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Was the Tunguska event the
work of an asteroid, or not?
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Recently, as research into
this question continues,
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a new fact has come to the fore.
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Physicist Giuseppe Longo has
been investigating Tunguska
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onsite for two decades.
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His colleague in this
research is Luca Gasperini.
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Their first expedition was in 1991.
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They began searching the Tunguska area for
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meteorite fragments that would prove that
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the 1908 explosion was an impact event.
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First they had to contend with
the huge number of mosquitos
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that breed in the Tunguska wetlands.
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They split up into small teams and searched
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the center of the blast area.
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They took core samples from
trees in the hope that
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such a large explosion
would have left traces.
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Looking for meteorite fragments as well,
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they also collected soil samples.
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All their samples were
transported back to Bologna
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and stored in a warehouse.
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During their first two
research trips, 1991 and '99,
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they collected soil samples
from a total of 300 locations.
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They're going to show us a
soil sample taken in 1999.
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Radio isotope analysis
identifies the stratum
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corresponding to the blast year, 1908.
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X-ray examination of that
stratum reveals something else.
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OK.
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Ordinarily in this region humus and
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other debris form horizontal
layers, but the tremendous
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momentary force of the explosion
compressed this area.
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It also slanted the
disposition of the layers.
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However, no actual meteorite
fragments were found.
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If they were, that would
prove the theory of
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an asteroid impact.
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They really wanted that physical proof,
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so the two colleagues prepared for a third
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research expedition.
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This time they focused their
attention on a small lake
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eight kilometers north from
the presumed epicenter.
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The two colleagues were now
hypothesizing that an asteroid
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streaking in from the southeast
exploded in mid air.
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A portion then traveled another
eight kilometers before
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striking Earth and excavating the lake bed.
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00:13:20,019 --> 00:13:23,838
In 2008 the team made their
third research trip.
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They measured the depth of Lake Cheko
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and took samples of the lake floor.
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The results were as you see here.
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The lake floor in cross
section reveals a deep
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angular depression.
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It's markedly different from
the lake bed structures
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of other lakes nearby.
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Furthermore, acoustic
measurement of the lake floor
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showed striations consistent
with sudden external pressure.
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A whole series of new discoveries
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has by now fairly well established
that the Tunguska event
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was due to collision with a space object.
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Yet not the smallest fragment
of the impacting object
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has ever been recovered,
crucial evidence missing.
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We've come to Sandia National Laboratories
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In New Mexico, U.S.A.
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As a nuclear weapons research facility,
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entry is strictly regulated.
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Mark Boslough is a physicist here,
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studying large blast phenomena.
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To address this question of the
absence of object fragments
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at Tunguska, he's using a supercomputer.
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We knew from the old Russian expeditions
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and photographs and
mapping, we knew the area
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over which trees had been blown down,
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and we knew the pattern.
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So we could match that with
the size of the asteroid
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that would blow those down.
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After several months of computing,
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Boslough concluded that the
Tunguska explosion was caused
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by the intrusion of a
50-meter diameter asteroid.
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This is Boslough's simulation
of the Tunguska event
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created on the supercomputer.
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The asteroid, 50 meters across, as wide as
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an 18-story building is tall,
blazed into Earth's atmosphere
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as a meteor at 15 kilometers per second.
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At an altitude of 8500 meters, it exploded.
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At that moment its core temperature hit
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24,700 degrees celsius.
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It vaporized in an instant.
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The energy released by the
explosion propagated a shock wave
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toward the Earth's surface,
flattening forests and causing
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widespread destruction.
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To summarize, when the asteroid
exploded, it vaporized.
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That's the reason no fragments
descended to Earth.
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In this case, because
it's coming in at an angle,
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when it explodes the momentum
carries that energy downward,
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still very powerful.
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But because that energy
was directed downward,
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the effects on the ground at
ground zero, at Tunguska,
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the effects we observe
could have been caused by
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a smaller asteroid.
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Even a 50 meter wide asteroid
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would have the impact of a hydrogen bomb.
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What causes asteroids to approach Earth?
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Between Mars and Jupiter lies a
region called the main belt,
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that is, the main asteroid belt.
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The so-called minor planets,
asteroids and other such
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objects that populate it,
number in the hundreds
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of thousands, perhaps even the millions.
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But since most lie outside
the orbit of Mars,
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they rarely approach Earth.
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Sometimes, however, affected
by the gravitational pull
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00:18:26,400 --> 00:18:29,859
of Jupiter or Mars, these
objects are flung toward
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00:18:29,860 --> 00:18:32,471
the inner solar system.
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If an asteroid approaches our planet,
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there may well be a collision.
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These are potentially hazardous objects.
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And indeed, many asteroids
have left their imprint
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on the Earth's surface.
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Gosses Bluff Crater in central Australia.
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It has a diameter of 22 kilometers.
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It is thought that this crater
was created 140 million
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years ago by the impact of
an object from outer space.
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00:19:26,006 --> 00:19:29,765
The Barringer Crater, or
Meteor Crater in Arizona
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00:19:29,766 --> 00:19:32,625
measures one point two kilometers across,
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and dates back 50,000 years.
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In the long history of the
world there have been
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quite a few such impacts.
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00:19:48,248 --> 00:19:53,248
By 2011 the number of confirmed
craters reached 176.
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00:20:05,608 --> 00:20:08,307
The impact that caused
the greatest devastation
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was at the site shown here.
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Mexico's Yucatan Peninsula.
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A gigantic crater was gouged
into the terrain here,
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170 kilometers in diameter.
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The impact took place 65 million years ago
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during the cretaceous period,
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when the dinosaur population
was at its zenith.
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What caused the impact was
an asteroid as large as
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10 kilometers across.
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00:20:52,890 --> 00:20:56,149
The dinosaurs were assailed
by a gigantic blast
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and subsequent inferno.
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00:21:05,311 --> 00:21:08,770
Dirt and ash then filled the
atmosphere, blocking out
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00:21:08,771 --> 00:21:11,770
the sun's rays, yielding an extended period
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00:21:11,771 --> 00:21:13,531
of cold temperatures.
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00:21:13,532 --> 00:21:16,922
That led to the dinosaurs extinction.
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It's estimated that an
object large enough to cause
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a global extinction of
life, that is one that's
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10 kilometers wide or more,
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strikes Earth once every 100 million years.
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Even something one-tenth
that size would cause damage
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tantamount to a nuclear holocaust.
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Civilization as we know
it would be imperiled.
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00:21:45,277 --> 00:21:48,616
Objects that size strike
once every few hundred
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00:21:48,617 --> 00:21:50,347
thousand years.
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00:21:53,597 --> 00:21:56,676
Even an object in the 100
meter class would have
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00:21:56,677 --> 00:21:58,916
a catastrophic impact.
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00:21:58,917 --> 00:22:01,648
It could take out a large city.
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00:22:03,118 --> 00:22:05,857
Scientists estimate the
frequency of strikes by these
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smaller objects to be on the order of once
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00:22:08,658 --> 00:22:10,888
every few centuries.
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00:22:14,438 --> 00:22:17,517
Any substantial asteroid
impact would cause destruction
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on a scale that humanity
has never experienced.
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00:22:25,408 --> 00:22:30,408
Three, two, one.
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00:22:32,409 --> 00:22:35,188
Christmas time, 2004.
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00:22:35,189 --> 00:22:38,468
In this happy season,
shocking news made its way
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00:22:38,469 --> 00:22:40,219
around the globe.
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00:23:06,760 --> 00:23:09,359
Now the threat posed by
an asteroid collision
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was a reality reported by the media.
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Let's pay a visit to the person
who discovered this danger.
256
00:23:28,957 --> 00:23:32,616
David Tholen, an astronomer
at the University of Hawaii.
257
00:23:32,617 --> 00:23:33,576
Hi, nice to meet you.
258
00:23:33,577 --> 00:23:34,656
How are you today?
259
00:23:34,657 --> 00:23:35,729
Doing well.
260
00:23:37,559 --> 00:23:39,378
Tholen has already discovered
261
00:23:39,379 --> 00:23:41,670
over a thousand asteroids.
262
00:23:45,160 --> 00:23:49,120
This screen is telling us the
status of the telescope.
263
00:23:49,121 --> 00:23:52,480
Then on June 19th, 2004,
264
00:23:52,481 --> 00:23:55,560
he spotted an object of
particular interest.
265
00:23:55,561 --> 00:23:59,021
The slit is closed,
the wind screens are parked.
266
00:24:00,581 --> 00:24:02,953
Here are photographs of it.
267
00:24:04,303 --> 00:24:08,254
These are interval shots of
the same sector of space.
268
00:24:11,704 --> 00:24:14,203
When they are superimposed,
you can see that
269
00:24:14,204 --> 00:24:16,094
something has moved.
270
00:24:19,984 --> 00:24:21,934
A nearby asteroid.
271
00:24:30,504 --> 00:24:32,663
Two days after this sighting, however,
272
00:24:32,664 --> 00:24:34,935
Tholen lost track of it.
273
00:24:42,325 --> 00:24:44,495
He looked for it for months.
274
00:24:52,565 --> 00:24:56,705
Then on December 18th he spotted it again.
275
00:24:56,706 --> 00:24:59,625
Based on its previous
and current positions,
276
00:24:59,626 --> 00:25:02,185
he was able to calculate its orbit.
277
00:25:02,186 --> 00:25:03,945
That is when he concluded that there was a
278
00:25:03,946 --> 00:25:08,946
one in 300 probability that it
would impact Earth in 2029.
279
00:25:14,186 --> 00:25:18,145
Well, we were very excited
because this was the
280
00:25:18,146 --> 00:25:23,146
sort of thing that people looking
for asteroids that could
281
00:25:23,766 --> 00:25:25,865
potentially collide with the Earth...
282
00:25:25,866 --> 00:25:29,085
Here we were talking about
something that was just
283
00:25:29,086 --> 00:25:30,851
25 years away.
284
00:25:33,141 --> 00:25:34,760
The asteroid was estimated to be
285
00:25:34,761 --> 00:25:39,761
400 meters in diameter, and
to weigh 72 million tons.
286
00:25:40,097 --> 00:25:42,807
Tholen chose a name for it.
287
00:25:48,697 --> 00:25:50,176
Apophis.
288
00:25:50,177 --> 00:25:52,476
That is the Greek name
of the ancient Egyptian
289
00:25:52,477 --> 00:25:57,477
god of destruction, a deification
of darkness and chaos.
290
00:26:01,137 --> 00:26:03,696
Astronomers all over the
world began their own
291
00:26:03,697 --> 00:26:06,587
observations of Apophis.
292
00:26:11,017 --> 00:26:14,816
All of this news was breaking
right around the time
293
00:26:14,817 --> 00:26:17,176
of the Christmas season.
294
00:26:17,177 --> 00:26:21,376
And so many astronomers,
rather than spending the time,
295
00:26:21,377 --> 00:26:23,716
the holidays with their families,
296
00:26:23,717 --> 00:26:26,276
they were instead spending
time with a telescope
297
00:26:26,277 --> 00:26:28,516
measuring the position of this asteroid.
298
00:26:28,517 --> 00:26:30,156
One of my colleagues called it the Grinch
299
00:26:30,157 --> 00:26:32,087
that stole Christmas.
300
00:26:34,293 --> 00:26:36,192
The telescopes of the world were trained
301
00:26:36,193 --> 00:26:40,703
upon Apophis, and its orbit
was carefully calculated.
302
00:26:45,693 --> 00:26:48,412
In just three days the
probability of a collision
303
00:26:48,413 --> 00:26:51,823
was upgraded to one in 37.
304
00:26:59,633 --> 00:27:02,452
The asteroid could actually
collide with Earth
305
00:27:02,453 --> 00:27:04,668
and wreak tremendous havoc.
306
00:27:04,669 --> 00:27:07,929
It was starting to sound all too real.
307
00:27:17,749 --> 00:27:19,568
If Apophis were to hit Manhattan Island,
308
00:27:19,569 --> 00:27:22,855
you could probably say
goodbye to Manhattan Island.
309
00:27:27,025 --> 00:27:29,935
That's about similar dimensions.
310
00:27:32,385 --> 00:27:34,684
If it reached Earth, Apophis would create
311
00:27:34,685 --> 00:27:37,800
a four kilometer wide crater on impact.
312
00:27:37,801 --> 00:27:40,180
Shock waves would further
devastate thousands of
313
00:27:40,181 --> 00:27:43,210
square kilometers all around.
314
00:27:43,211 --> 00:27:46,262
Not just Manhattan, but
all of New York City
315
00:27:46,263 --> 00:27:48,173
would be destroyed.
316
00:27:58,863 --> 00:28:01,642
Destruction would not be limited
to the immediate vicinity
317
00:28:01,643 --> 00:28:03,502
of the impact site.
318
00:28:03,503 --> 00:28:05,482
One scientist has raised concerns that
319
00:28:05,483 --> 00:28:07,633
it would be widespread.
320
00:28:17,203 --> 00:28:20,722
Professor Seiji Sugita of
the University of Toyko
321
00:28:20,723 --> 00:28:24,209
studies the impact of space objects.
322
00:28:26,979 --> 00:28:30,098
His team will simulate
impact scenarios for Apophis
323
00:28:30,099 --> 00:28:32,569
inside this special chamber.
324
00:28:47,359 --> 00:28:50,484
They'll fire an eight-millimeter
projectile into a basin
325
00:28:50,485 --> 00:28:55,485
of sand at an effective speed
of 1200 kilometers per hour.
326
00:29:11,271 --> 00:29:13,786
The first simulation models the impact
327
00:29:13,787 --> 00:29:16,526
on a planet without an atmosphere.
328
00:29:16,527 --> 00:29:19,766
The ejecta curtain, the sheet
of displaced material,
329
00:29:19,767 --> 00:29:22,557
makes a perfect inverted cone.
330
00:29:29,587 --> 00:29:32,306
Next the effect on a
planet with an atmosphere,
331
00:29:32,307 --> 00:29:34,946
like Earth, is simulated.
332
00:29:34,947 --> 00:29:38,946
The ejecta curtain here forms,
not a smooth inverted cone,
333
00:29:38,947 --> 00:29:41,217
but a swirling vortex.
334
00:29:49,627 --> 00:29:51,966
A closer look reveals a great difference
335
00:29:51,967 --> 00:29:54,282
in elapsed time also.
336
00:29:54,283 --> 00:29:57,142
In the no atmosphere simulation on the left
337
00:29:57,143 --> 00:30:01,405
the sand subsided in point
zero three seconds.
338
00:30:05,595 --> 00:30:08,634
But in the atmospheric case
simulated on the right
339
00:30:08,635 --> 00:30:11,334
the sand stays aloft much longer.
340
00:30:11,335 --> 00:30:14,134
Sugita estimates that the
displaced dirt and dust would
341
00:30:14,135 --> 00:30:17,254
stay aloft 100 thousand
times longer on an actual
342
00:30:17,255 --> 00:30:21,785
Earth-sized planet with
atmosphere than one without.
343
00:30:50,891 --> 00:30:52,770
Based on such simulations,
344
00:30:52,771 --> 00:30:55,835
Sugita predicts that if
Apophis collides with Earth,
345
00:30:55,836 --> 00:30:58,655
it will project as much as
three billion tons of dirt
346
00:30:58,656 --> 00:31:01,635
and dust up into the stratosphere.
347
00:31:01,636 --> 00:31:03,855
Some of it will remain in the atmosphere,
348
00:31:03,856 --> 00:31:06,915
where for the next three
months it will stay suspended,
349
00:31:06,916 --> 00:31:11,486
blocking sunlight and
cooling the entire planet.
350
00:31:18,516 --> 00:31:21,355
There have been actual cases
where enough particulates
351
00:31:21,356 --> 00:31:25,326
have swirled up into the
stratosphere to lower temperatures.
352
00:31:27,450 --> 00:31:31,509
The eruption of Mount Pinatubo
in 1991, for example,
353
00:31:31,510 --> 00:31:34,149
spewed 300 million tons of dust and ash
354
00:31:34,150 --> 00:31:36,495
into the stratosphere.
355
00:31:37,265 --> 00:31:39,484
As a result, the amount
of sunlight reaching
356
00:31:39,485 --> 00:31:43,004
the Earth's surface was
reduced by five percent.
357
00:31:43,005 --> 00:31:45,604
And in the northern hemisphere
the average temperature
358
00:31:45,605 --> 00:31:49,030
dropped by point six degrees celsius.
359
00:31:53,560 --> 00:31:56,619
If Apophis collides with
Earth, it will send up into
360
00:31:56,620 --> 00:31:59,839
the stratosphere ten times
as much particulate matter
361
00:31:59,840 --> 00:32:02,579
as the Mount Pinatubo eruption.
362
00:32:02,580 --> 00:32:05,710
The damage would be incalculable.
363
00:32:09,220 --> 00:32:11,219
The world's clearing house
for information about
364
00:32:11,220 --> 00:32:16,220
asteroid and comet discoveries
is the Minor Planet Center.
365
00:32:22,660 --> 00:32:25,559
Gareth Williams is in
charge of compiling data on
366
00:32:25,560 --> 00:32:28,965
more than 200,000 space objects.
367
00:32:31,895 --> 00:32:34,974
When astronomers around the
world observed Apophis,
368
00:32:34,975 --> 00:32:37,545
they sent their information here.
369
00:32:41,555 --> 00:32:44,434
It was Williams whose task it
was to collect and correlate
370
00:32:44,435 --> 00:32:47,474
all this data, and to
publicize it to the global
371
00:32:47,475 --> 00:32:49,565
research community.
372
00:32:56,855 --> 00:32:59,994
As soon as Apophis was discovered,
the Minor Planet Center
373
00:32:59,995 --> 00:33:02,788
sent out requests to astronomers worldwide
374
00:33:02,789 --> 00:33:05,108
for follow up observations.
375
00:33:05,109 --> 00:33:07,748
Ascertaining whether Apophis
would strike Earth or not
376
00:33:07,749 --> 00:33:12,299
required extremely accurate
data about its trajectory.
377
00:33:14,849 --> 00:33:16,888
We need to find them, and
we need to follow them
378
00:33:16,889 --> 00:33:18,588
long enough that we can predict
where they're gonna be
379
00:33:18,589 --> 00:33:20,748
with accuracy years in the future.
380
00:33:20,749 --> 00:33:24,639
And in order to do that you
need long arcs of observation.
381
00:33:25,489 --> 00:33:27,188
Responding to the requests by the Minor
382
00:33:27,189 --> 00:33:30,728
Planet Center, observatories
around the world trained
383
00:33:30,729 --> 00:33:33,859
their telescopes on Apophis.
384
00:33:36,869 --> 00:33:39,968
The astronomers then pooled
their observational data,
385
00:33:39,969 --> 00:33:43,539
and the asteroid's orbit was
more accurately plotted.
386
00:33:44,309 --> 00:33:45,619
The result?
387
00:33:49,249 --> 00:33:54,249
In 2029, Apothos will approach
Earth, but finally whiz by it
388
00:33:54,649 --> 00:33:59,168
at an altitude of 32,500 kilometers.
389
00:33:59,169 --> 00:34:03,949
That's closer than the orbit
of a geosynchronous satellite.
390
00:34:04,839 --> 00:34:07,238
Earth will have escaped
an asteroid impact by
391
00:34:07,239 --> 00:34:09,769
the slimmest of margins.
392
00:34:13,719 --> 00:34:16,378
But Apophis is not the
only near-Earth object
393
00:34:16,379 --> 00:34:18,024
heading our way.
394
00:34:28,844 --> 00:34:33,844
Calculating asteroid orbits is
Makoto Yoshikawa's specialty.
395
00:34:36,209 --> 00:34:38,387
He is sounding the alarm.
396
00:34:38,388 --> 00:34:42,239
These objects pose an all
too imminent threat.
397
00:34:43,209 --> 00:34:46,328
Yoshikawa has calculated the
trajectories of space objects
398
00:34:46,329 --> 00:34:49,169
whose orbits take them close to Earth.
399
00:34:50,819 --> 00:34:52,870
Here is what he's found.
400
00:34:55,040 --> 00:34:58,299
The yellow circle is the
orbit of the Earth.
401
00:34:58,300 --> 00:35:02,720
Around it are clustered 5,700 asteroids.
402
00:35:02,721 --> 00:35:06,360
Let's put them all in motion
based on actual observation
403
00:35:06,361 --> 00:35:09,092
and assessment of their orbits.
404
00:35:12,082 --> 00:35:15,081
The red flashes show where
the orbits of asteroids
405
00:35:15,082 --> 00:35:17,593
intersect Earth's orbit.
406
00:35:19,863 --> 00:35:22,202
Yoshikawa calculates
that among the asteroids
407
00:35:22,203 --> 00:35:25,662
approaching Earth, 205
have the potential to
408
00:35:25,663 --> 00:35:27,922
collide with our planet.
409
00:35:27,923 --> 00:35:30,062
Since others have yet to be discovered,
410
00:35:30,063 --> 00:35:33,993
an Earth impact could occur at any time.
411
00:35:39,883 --> 00:35:42,482
To discover any unknown
objects that could collide
412
00:35:42,483 --> 00:35:45,022
with Earth, an international organization
413
00:35:45,023 --> 00:35:47,342
has been established in Italy.
414
00:35:47,343 --> 00:35:50,673
It's called the Spaceguard Foundation.
415
00:35:51,823 --> 00:35:54,902
It has been joined by
observatories in seven countries,
416
00:35:54,903 --> 00:35:58,462
including Japan, the United
States, the United Kingdom
417
00:35:58,463 --> 00:36:00,033
and Australia.
418
00:36:02,723 --> 00:36:07,133
Participating in Japan is the
Bisei Spaceguard Center.
419
00:36:15,593 --> 00:36:19,394
Here the Japanese observatory
is using two telescopes
420
00:36:19,395 --> 00:36:23,525
to track and photograph space
objects approaching the Earth.
421
00:36:33,115 --> 00:36:35,474
Members of a six-person team take turns
422
00:36:35,475 --> 00:36:37,686
monitoring the equipment.
423
00:36:41,356 --> 00:36:43,855
They're looking for any
movement that stands out
424
00:36:43,856 --> 00:36:46,666
from the background array of stars.
425
00:36:54,636 --> 00:36:59,327
In one evening they'll take
300 or 400 photographs,
426
00:37:01,857 --> 00:37:06,587
and so far they've discovered
over 1,000 asteroids.
427
00:37:18,917 --> 00:37:21,616
When Rusty Schweickart
observed Earth from space on
428
00:37:21,617 --> 00:37:26,617
Apollo Nine, he felt keenly the
danger posed by asteroids.
429
00:37:28,917 --> 00:37:31,576
Motivated by his heightened
sense of the threat posed
430
00:37:31,577 --> 00:37:35,787
by such space objects,
Schweickart is taking action.
431
00:37:36,257 --> 00:37:37,357
His message.
432
00:37:37,358 --> 00:37:40,697
An asteroid collision is inevitable.
433
00:37:40,698 --> 00:37:45,698
However, humankind working
together can defend against it.
434
00:37:45,855 --> 00:37:48,674
So the question is, do we care
435
00:37:48,675 --> 00:37:50,574
about future generations?
436
00:37:50,575 --> 00:37:52,294
How much do we care?
437
00:37:52,295 --> 00:37:56,673
Should we take action today
to protect our grandchildren?
438
00:37:56,674 --> 00:37:59,505
This is survival of the species.
439
00:38:03,235 --> 00:38:05,194
The American government is now also
440
00:38:05,195 --> 00:38:09,825
getting involved in plans to
avoid an asteroid collision.
441
00:38:12,375 --> 00:38:16,694
The summit of Haleakala on
the Hawaiian island of Maui
442
00:38:16,695 --> 00:38:20,474
has an elevation of 3,000
meters above sea level.
443
00:38:20,475 --> 00:38:23,174
In 2008, the American government built a
444
00:38:23,175 --> 00:38:25,745
new observatory here.
445
00:38:29,674 --> 00:38:32,341
It's called Pan-STARRS.
446
00:38:40,487 --> 00:38:45,487
The Director of Pan-STARRS
Telescope One is Ken Chambers.
447
00:38:48,617 --> 00:38:51,482
The Pan-STARRS One telescope
was purpose built
448
00:38:51,483 --> 00:38:53,728
to spot space objects.
449
00:39:02,999 --> 00:39:07,378
Its field of view emcompasses
36 full moons at one time,
450
00:39:07,379 --> 00:39:09,718
a large sector the sky.
451
00:39:09,719 --> 00:39:13,058
It takes just one week to
complete a full survey of space
452
00:39:13,059 --> 00:39:15,609
as visible from this location.
453
00:39:22,319 --> 00:39:27,319
Pan-STARRS is a small
telescope, but in some ways
454
00:39:27,379 --> 00:39:29,698
it's the biggest telescope in the world,
455
00:39:29,699 --> 00:39:32,379
and that's because of its camera.
456
00:39:33,259 --> 00:39:35,364
The camera is the largest
camera in the world.
457
00:39:35,365 --> 00:39:40,365
It's actually a CCD camera,
about 40 centimeters across.
458
00:39:43,476 --> 00:39:46,175
Thanks to this CCD camera exclusively
459
00:39:46,176 --> 00:39:49,415
developed for Pan-STARRS,
the telescope can spot
460
00:39:49,416 --> 00:39:52,895
space objects 100 times fainter
than could the telescope
461
00:39:52,896 --> 00:39:55,586
used to discover Apophis.
462
00:40:04,176 --> 00:40:08,795
We know many of the largest
ones, but as you get to
463
00:40:08,796 --> 00:40:12,095
the smaller and smaller ones
that are still dangerous enough
464
00:40:12,096 --> 00:40:16,642
to be a threat to life on Earth,
465
00:40:17,835 --> 00:40:19,898
we still haven't found them all.
466
00:40:20,948 --> 00:40:23,287
The plan for the Pan-STARRS observatory
467
00:40:23,288 --> 00:40:26,487
is to identify several hundred
thousand space objects
468
00:40:26,488 --> 00:40:28,934
in three and a half years.
469
00:40:30,084 --> 00:40:32,803
If an asteroid or a comet were
to be found that was really
470
00:40:32,804 --> 00:40:37,406
going to collide with Earth,
how could we respond?
471
00:40:38,944 --> 00:40:42,734
The United States has begun
to formulate a strategy.
472
00:40:44,504 --> 00:40:47,159
Three, two, one.
473
00:40:47,160 --> 00:40:51,039
We have ignition and lift
off of a Delta Two rocket
474
00:40:51,040 --> 00:40:52,735
carrying Deep Impact.
475
00:40:52,736 --> 00:40:56,595
In 2005, NASA conducted a grand experiment
476
00:40:56,596 --> 00:40:58,595
in outer space.
477
00:40:58,596 --> 00:41:00,746
The Deep Impact Mission.
478
00:41:03,876 --> 00:41:06,335
The goal, to intercept a comet moving at
479
00:41:06,336 --> 00:41:08,295
10 kilometers per second,
480
00:41:08,296 --> 00:41:12,613
and strike it with a
projectile called an impactor.
481
00:41:14,742 --> 00:41:17,542
The ambitious plan called for
the impactor to be launched
482
00:41:17,543 --> 00:41:22,241
at the target from a distance
of 880,000 kilometers.
483
00:41:22,242 --> 00:41:25,172
That was one tough shot to make.
484
00:41:29,802 --> 00:41:33,482
Moreover, the targeted
comet was 133 million
485
00:41:33,483 --> 00:41:35,442
kilometers from Earth.
486
00:41:35,443 --> 00:41:39,521
Radio transmissions took seven
minutes to travel each way.
487
00:41:39,522 --> 00:41:43,032
Remote control from Earth was impossible.
488
00:41:50,262 --> 00:41:53,421
To overcome these constraints,
the impactor was outfitted
489
00:41:53,422 --> 00:41:54,881
with a camera.
490
00:41:54,882 --> 00:41:58,192
It could thus guide itself to the target.
491
00:42:06,822 --> 00:42:10,562
Starting two hours prior to
impact, the impactor received
492
00:42:10,563 --> 00:42:13,061
no instructions from Earth.
493
00:42:13,062 --> 00:42:15,932
It was a self-guided missile.
494
00:42:18,322 --> 00:42:21,161
This is an image taken
by the impactor itself
495
00:42:21,162 --> 00:42:23,302
on its way to the comet.
496
00:42:23,303 --> 00:42:27,912
It has fixed its sights on this
bright spot in deep space.
497
00:42:34,712 --> 00:42:37,742
Then it adjusts its own trajectory.
498
00:42:51,662 --> 00:42:54,721
It makes three mid-course
corrections in all,
499
00:42:54,722 --> 00:42:58,153
and finally hits right on target.
500
00:43:00,342 --> 00:43:03,801
This was proof that an
extremely remote space object
501
00:43:03,802 --> 00:43:08,802
traveling extremely fast
could indeed be impacted.
502
00:43:09,062 --> 00:43:12,383
The Deep Impact Mission did
demonstrate rather effectively
503
00:43:12,384 --> 00:43:15,683
that we have the technology to
run into a near-Earth object,
504
00:43:15,684 --> 00:43:17,422
should we choose to do so.
505
00:43:17,423 --> 00:43:20,783
If you have enough time,
10, 20, 30 years prior to
506
00:43:20,784 --> 00:43:24,482
a predicted impact, you can
run into it and slow it down
507
00:43:24,483 --> 00:43:27,733
just a bit so in 10 or
20 years it will miss.
508
00:43:28,883 --> 00:43:31,962
In 2006, Yeomans and his colleagues were
509
00:43:31,963 --> 00:43:35,242
largely responsible for
producing a report for NASA
510
00:43:35,243 --> 00:43:38,393
on the subject of space object impacts.
511
00:43:40,343 --> 00:43:43,502
The report specified concrete
measures that could be taken
512
00:43:43,503 --> 00:43:46,453
to alter such objects' orbits.
513
00:43:51,443 --> 00:43:54,582
This 15-ton spacecraft
would land a solar-powered
514
00:43:54,583 --> 00:43:58,393
plasma engine onto a threatening asteroid.
515
00:43:59,283 --> 00:44:02,263
Over time it would literally
push the asteroid
516
00:44:02,264 --> 00:44:04,613
off its collision course.
517
00:44:08,203 --> 00:44:11,462
Yeomans and the other NASA
scientists alike felt that
518
00:44:11,463 --> 00:44:14,822
given sufficient time, this
could prevent an asteroid
519
00:44:14,823 --> 00:44:16,854
from colliding with Earth.
520
00:44:35,783 --> 00:44:39,042
The American government has
committed $100 million dollars
521
00:44:39,043 --> 00:44:41,922
to the Pan-STARRS project, and in fact,
522
00:44:41,923 --> 00:44:45,933
plans to expand its
observational capabilities.
523
00:44:49,063 --> 00:44:52,393
So here's Pan-STARRS One
where we just were.
524
00:44:53,044 --> 00:44:57,282
We're building Pan-STARRS
Two, the second one,
525
00:44:57,283 --> 00:44:59,433
in this dome here.
526
00:45:02,003 --> 00:45:06,102
Pan-STARRS One has been
in operation since 2008.
527
00:45:06,103 --> 00:45:11,103
Pan-STARRS Two is scheduled
to come online by 2014,
528
00:45:12,244 --> 00:45:14,243
and there are plans for a third and fourth
529
00:45:14,244 --> 00:45:18,683
telescope as well, all to
look for objects that might
530
00:45:18,684 --> 00:45:21,255
collide with our planet.
531
00:45:23,165 --> 00:45:28,165
Then if you find one, and there
is one headed for Earth,
532
00:45:28,344 --> 00:45:30,994
you want to find it...
533
00:45:30,995 --> 00:45:33,384
If you find it a hundred
years ahead of time,
534
00:45:33,385 --> 00:45:35,584
and it's not gonna hit the
Earth for a hundred years,
535
00:45:35,585 --> 00:45:39,583
then we have time to do
something about it, yes.
536
00:45:39,584 --> 00:45:43,983
If it's headed for Earth, and
it's gonna hit in 10 years,
537
00:45:43,984 --> 00:45:46,543
we still have time to do something about it
538
00:45:46,544 --> 00:45:49,415
if we all work together.
539
00:45:50,204 --> 00:45:51,583
With the number of telescopes
540
00:45:51,584 --> 00:45:55,044
increasing to four, the
survey of near-Earth objects
541
00:45:55,045 --> 00:45:57,103
can be greatly speeded up,
542
00:45:57,104 --> 00:46:01,554
hopefully giving sufficient
time to ward off disaster.
543
00:46:08,784 --> 00:46:11,203
The Earth exists in space.
544
00:46:11,204 --> 00:46:14,163
The threat of a collision
with another space object
545
00:46:14,164 --> 00:46:16,115
is ever present.
546
00:46:17,285 --> 00:46:19,984
Even one such impact has the potential to
547
00:46:19,985 --> 00:46:22,635
wipe out civilization.
548
00:46:23,946 --> 00:46:28,045
But now humankind has
awakened to this threat.
549
00:46:28,046 --> 00:46:31,884
We are devising early warning
systems and ways to mitigate
550
00:46:31,885 --> 00:46:35,077
or avoid a major impact.
551
00:46:36,787 --> 00:46:40,245
Observatories around the
world are on the alert,
552
00:46:40,246 --> 00:46:43,005
peering into the heavens every night,
553
00:46:43,006 --> 00:46:47,216
keeping watch on those starry skies.
44878
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