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Humans are natural born explorers.
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We charge into uncharted territory
and seek out the unknown.
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We've mapped nearly every
inch of Mother Earth..
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..and left tracks on the Moon.
But to set foot on another planet,
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to travel beyond our solar system,
that is a dream for the future.
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A dream that comes to life in
the feature film Interstellar.
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We must think not as
individuals, but as a species.
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We must confront the reality
of interstellar travel.
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The film Interstellar deals with the quest
for new worlds and the faith of humanity.
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Sound like the stuff of science fiction?
Maybe.
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But the foundations of this film
are rooted in real science,
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thanks to the involvement of a
renowned astrophysicist Kip Thorne.
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In Interstellar, one of the
most important features is
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the way that science is
totally embedded in the film.
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There is some wild things in here.
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Beyond fantasy and fiction, this
is the real science of Interstellar.
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Space travel has been a staple of
the movies from the very beginning,
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but the feature film Interstellar has
a unique pedigree.
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It was inspired in part by
the work of Kip Thorne,
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an authority on astrophysics,
gravitational waves
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and the warping of spacetime,
he is also an executive producer on the film.
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In Interstellar, real science was built into
the fabric of the film from the outset.
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The other major players in this film,
they all respected the science
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and they worked with me to see if
the science was well incorporated.
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Can you tell me what the... the easiest
definition of what a singularity is?
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Kip and myself meshed well in terms of trying
to use current thinking,
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current scientific understanding
to drive the narrative
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-It lies in between, this
is a place where curvature
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of space and time gets infinitely high.
So we're good, okay.
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And we just hope that the
research that we've done
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and the conversations that
I'd had over the years
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with Kip and that Chris had
had with Kip informed the
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narrative, and that the
audience would feel that.
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Why simply imagine,
fantasize about things that
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might happen in space or
an interstellar journey?
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Why not actually look at
the real science there?
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-It's an Indian surveillance drone!
Interstellar takes place in the future
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where living conditions on Earth threaten
the survival of humanity.
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Now you need to tell me
what your plan it is to
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save the world. -We're not
meant to save the world,
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we're meant to leave it.
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One of the things that the
film explores is do we
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belong on Earth and should
we be staying on Earth,
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and if there is anything else that there
should we be exploring there. - Here we go.
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In the film the crew seeks
a new place to call home.
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A planet that can sustain life.
Human life.
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-We're not gonna to make it!
Yes you are.
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Sounds like a job for the
explorers of tomorrow. But
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the search for another Earth
is happening right now.
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Astrophysicist Natalie Bataglia is
a passionate planet hunter.
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you think the only way
that we're really going
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to really understand our
place in the galaxy
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is by looking at this broad picture and
understanding the diversity of all planets.
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20 or 30 years ago we
didn't know of any other
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planets orbiting normal
stars like our own Sun.
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Natalie has helped rewrite
that story as a misison
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scientist for NASA's
Kepler space telescope
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Kepler's objective is very
simple: it's to determine
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the fraction of stars in
our galaxy that harbour
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potentially habitable oversized planets.
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And what makes a planet
potentially habitable?
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The one ingredient that
we think is common to all
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life forms is this
requirement of liquid water.
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So that's why we look for
planets that have rocky
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surfaces where water can
pool and that are receiving
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the right amount of energy from the star
where the water wouldn't be locked up in a
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frozen state because the
planet is so cold, nor would
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it be evaporated away because
the planet is too hot.
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We call it the Goldilocks zone,
where liquid water could potentially exist.
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Launched in 2009, Kepler
stared at one small
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patch of the Milky Way
for four years straight.
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Compared to stars, planets are too tiny
for Kepler to spot...
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but it can detect their shadows.
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Every planet orbiting an illuminous object
is casting a shadow out into space
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and the Kepler spacecraft
makes use of that fact.
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Waiting for a planet in
it's orbit about the star
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to pass directly between
the disc of the star and
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the spacecraft, and the
telescope perceives that
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as a dimming of light.
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This simple method has
revealed 1000's of exoplanets.
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Planets orbiting other
stars in our galaxy.
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What we've learned so far
is that literally every
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star in our galaxy has
at least one planet.
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There is an amazing diversity of exoplanets
out there and we've found very exotic worlds.
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200 lightyears away there is a Saturn sized
planet orbiting not one, but two stars.
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So if you were living
on a world like
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Kepler-16b, you would see
in the sky two stars
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rising in the east setting
in the west, continuously
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changing position as
they orbit one another.
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This is an artist rendition
of the planet Kepler-10b,
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it's orbiting 23 times
closer to its parent star
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than Mercury is to our own Sun.
So this star-facing
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side is just being blasted
by this stellar radiation.
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Creating temperatures in excess of
that required to melt iron.
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The planet has an entire hemisphere larger
than the Pacific Ocean, which is an ocean,
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but it's not an ocean of water.
It's an ocean of molten lava.
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Not an attractive destination. But Kepler
recently found as a possible second home.
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This is an artist concept of the Kepler-186
planetary system.
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Five planets orbiting this M-type star
and the outermost planet is Kepler-186f.
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Our first discovery of an Earth-sized planet
in the habitable zone of a normal star.
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When I think about Kepler-186f,
I try to imagine it as a real place
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because it is a real place.
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We know that it could be rocky, same size
as Earth so I do imagine a rocky surface...
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We don't know that it has a liquid ocean,
but we can certainly imagine one.
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And then, all of a sudden
in your imagination you
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eternalize the existence
of this world out there,
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that there is a place that could
be very, very much like Earth.
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So, when do we set sail for these
distant shores? Reality check.
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Kepler-186f is nearly three quadrillion miles
(~4.8 quadrillion km) from Earth.
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Otherwise put five hundred
light years away.
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That's a journey 500 years
at the speed of light.
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But no thing can travel as fast as light.
At best, our spacecrafts are
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thousands of times slower. Even the
spaceships in Insterstellar don't come close.
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So how do they reach new worlds
beyond our solar system?
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They take a walk on the warp side
of space and time.
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The science of Interstellar
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-You have no idea when you're coming back.
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Couldn't you have told her you were
going to save the world? -No.
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I'm coming back.
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When we journey to a far off place we travel
not just in space but also in time,
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as we move into the future.
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Until about a century ago scientists believed
that space and time were entirely separate.
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Theoretical physicist Sean Caroll explains
how Albert Einstein overturned that idea.
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One of Einsten's great insights was that
space and time were related to each other,
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where you had space and you had time, Einsten
says: "Actually, there's only one thing
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which we call spacetime."
-And then he says
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"this spacetime thing,
it's not just the stage
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on which all the action plays out.
It's an act for itself."
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Spacetime can change, it can move,
it can bend and it can warp.
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Einstein's theory of relativity states
that spacetime is like a flexible fabric.
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The objects embedded in it: the Sun, planets,
even us, warp that fabric.
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And the consequence of that warping is what
we call gravity.
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The more massive the object,
the more spacetime is warped
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and the greater the gravity.
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We feel gravity. The flexibility of
spacetime is harder to grasp on a gut level
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but it's effects are measurable.
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As Sean demonstrates, the greater the
gravity, the more slowly time flows.
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For example, if I were on the ground floor
with a clock, a super accurate atomic clock,
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and a twin of mine was up
on the top floor of the
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building with an equally
accurate atomic clock,
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if we later on compared them, mine would've
ticked off fewer seconds.
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On the gorund floor, Sean
experiences slightly
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more gravity than his
twin on the top floor.
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He also experiences slightly
less time than his twin.
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The difference is tiny, but real.
And there are practical applications.
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For example, the GPS system
is a very, very precise set
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of clocks on satellites
orbiting around the Earth.
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and that orbit is in a slightly different
gravitational field than we are in down here
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so the fact that time moves
differently here on the
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surface of the Earth than
in the satellite orbit,
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is very very important to getting
the GPS to work correctly.
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Time on a GPS satellite
clock advances faster
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than the clock on Earth
by about 38ms per day,
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so the system's computers correct for that.
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Motion also affects our
experience of spacetime.
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-The best way to say
this just staying still
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means that you experience
the most time that you can.
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Moving around and doing things
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means you experience less time.
-Let's revisit Sean
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at the wheel of his car and
his twin on a park bench.
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If you move out of your
car, and then you come
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back, compared to the
person who stayed behind
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your clock that you took
with you on that journey
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will have experienced a
little bit less time
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than the one who stayed behind.
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We normally move too slowly
to notice the effect.
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But if Sean could drive
near the speed of light,
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he could race across the
USA and back again a
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million times and experience
less than a second
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of time, while the twin he left behind would
endure hours of waiting for Sean's return.
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In other words, Sean would've travelled into
the future compared to his twin.
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This means things may get tricky in years
to come, as we build faster spaceships.
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The closer we get to the
speed of light, the more out
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of sync we'll become with
those we leave behind.
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But the warping of
spacetime may also provide
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shortcuts that could make
interstellar travel a snap.
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Wormholes: they're a staple of science
fiction, but they're based on real science.
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Einstein's relativistic
laws govern the warping
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of space and time and
they say that wormholes
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might exist, they could exist.
So this dates all the way back to 1916.
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The wormhole's a particular way that
space and time can be curved.
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It's like adding a little tube that
connects two parts of space.
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The basic idea is that if you're an ant, and
you live on the surface of the apple,
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the surface of the apple
is your entire universe.
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You can go around the outside
through the universe
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itself, or you can go
through the wormhole.
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But Einstein's equations also predict that if
wormholes do form in nature, they may be
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sub-atomic in size and exist for only
fractions of a second before closing off.
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Theoretically, what
would it take to keep a
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wormhole open and make it
big enough to acommodate
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a spaceship. -It turns
out that in order to
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pull the wormhole open
so it doesn't crunch off
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and kill you when you try to go through,
then you have to have the wormhole threaded
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by a negative mass or negative energy,
Einstein says mass and energy are equivalent.
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Almost all the forms of matter we know have
positive mass and exert gravity.
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Negative mass would
exert anti-gravity and
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repel the walls of a
wormhole to keep it open.
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Strangely, it is true
that negative energy can
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exist, and it's been
created in the laboratory
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but only in very tiny amounts.
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It would take vast quantities to prop open
a wormhole big enough for a spaceship,
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But just maybe, in the
future, engineers will
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devise advanced technologies
to do just that.
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Today's it's an educated
guess, maybe I should say a
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half-educated guess, that
wormholes can not exist
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in our universe, but we're
far from sure of that.
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- The truth is, we just
don't know right now.
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We don't understand the
laws of physics well enough
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to say for sure wether or
not wormholes are possible.
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But since they're not impossible,
they're fair game for a filmmaker.
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I was very excited about the idea of focusing
on a family who would be the pioneers,
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who would experience some
of the extraordinary
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features of astrophysics,
particularly the idea
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of a wormhole that would allow us
to travel to distant stars.
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To create a wormhole based
on real science, visual
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effects supervisor Paul
Franklin turned to Kip Thorne.
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The topolar image of what a wormhole might
look like is literally just a hole in space.
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Generally it sits on an invisible surface,
you can see stuff sliding down the sides
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and disappearing down the
drain as it were. And
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right in that first
conversation Kip showed me
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an image of that kind of
classical fantasy image
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of these things and said
"This is all wrong!"
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"This is not how it is."
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Kip worked out the scientific
equations that define the
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wormhole and sent it to
Paul's animators in London.
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And so for the movie I
built a mathematical model
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wormhole based on Einstein's
relativity equations.
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Paul, Kip and myself, we
discussed "Okay, we'll
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visualize the hole, we'll
simulate it exactly
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as your calculations say."
-And Paul Franklin and
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his team, they were
thrilled to get algorithms
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that were the latest, most interesting and up
to the minute. -Now we go to the other one.
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The wormhole is a three-dimensional hole
in space, and what do you get if you take
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a circle, sweep it out in three dimensions?
You get a sphere.
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So the wormhole almost feels like
a crystal ball hanging in space.
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I don't think anybody ever
really done this kind
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of visualization before.
This is really unique.
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First time for me, as well
as for you and the audience.
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- Absolutely, yes.
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In Interstellar, crew
members take a giant
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leap of faith when they
plunge into a wormhole
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You can't just think about your family, now
you have to think bigger than that.
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-I am thinking about my family and
millions of other families.
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Beyond that wormhole, the
crew will enter the realm
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of the most extreme
objects in the universe:
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black holes.
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From Earth, the starry sky may seem
a realm of timeless calm.
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But when we aim our most advanced
tools at the universe, they capture displays
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of monstruous power and violence.
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Galaxies collide, cosmic clouds of gas and
dust spew radiation. Stars explode and die.
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For a filmmaker, space is full of dramatic
possibilities. When you venture out into
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a story about a man against the elements,
when that journey is interstellar,
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the possibilities for visualizing the threat
against our protagonist
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become very much more exotic. Deep, deep
space gives you a very fresh approach.
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- Exactly.
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One of the greatest challenges for a crew
on an interstellar voyage
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will be to nagivate the
dangers of black holes.
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Black holes were predicted
by Einstein's equations, but
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physicists question wether
they could really exist.
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The black hole is a strange beast.
If this were
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a black hole, then instead
of a rubber surface
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it would have a surface
that is made of
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absolutely nothing except
warped space and time.
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It's a place where gravity is so strong that
if anything falls into the black hole,
265
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it can never get back out. If you fall in,
you can't send signals back out,
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light can't get out from the interior.
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See, you might ask: how
did that ever happen? In
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outer space you can get
so much mass together
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like in a super-massive
star, that the gravity
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does become stronger and
stronger and stronger,
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and eventually the pressure that matter
exerts on itself can't keep up.
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And everything collapses,
there's a big explosion, some
273
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of the stuff is blown away
but the rest of it collapses
274
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into a black hole.
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A black hole that spins on its axis drags the
very space around it into a whilring motion
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that pulls stars and planets into orbit.
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Closer in, gravity increases like a riptide.
At a boundary called the event horizon
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the gravity becomes so
extreme that nothing can
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escape being pulled into
the heart of the beast
280
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and lost forever.
281
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Black holes are simple, and yet
they have a lot of character.
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It's almost like they can
take on personalities, umm,
283
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they can be picky eaters,
they can be energetic.
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And what you're seeing and
describing is really how
285
00:19:55,308 --> 00:19:57,800
the black hole interacts
with the environment.
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00:19:58,200 --> 00:20:04,050
UCLA astronomer Andrea Ghez is an
expert on black hole detection.
287
00:20:06,300 --> 00:20:10,050
She played a key role investigating what
had long been a scientific hunch.
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00:20:10,500 --> 00:20:14,750
That a huge black hole lives at the centre
of the Milky Way. -It's looking good.
289
00:20:15,500 --> 00:20:18,195
Astronomers knew the
heart of our galaxy was
290
00:20:18,220 --> 00:20:21,000
buzzing with gas, dust
and millions of stars.
291
00:20:21,800 --> 00:20:25,531
Some powerful force appeared
to be driving this hubbub.
292
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Could it be a black hole?
293
00:20:28,000 --> 00:20:31,600
Ground telescopes just couldn't produce
sharp images of the region,
294
00:20:32,300 --> 00:20:37,550
when the technique called adaptive optics
vastly improved the view.
295
00:20:37,600 --> 00:20:42,750
So this is what it looks like before you use
the advanced technology, it's a blurry mess
296
00:20:42,800 --> 00:20:46,600
and now you can see the individual stars
with the adaptive optics turned on.
297
00:20:46,650 --> 00:20:51,100
So each point of light here is associated
with an individual star.
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00:20:52,400 --> 00:20:56,400
Andrea put that technique to work at
the Keck observatory in Hawaii.
299
00:20:58,500 --> 00:20:59,850
This is a roadmap.
300
00:20:59,900 --> 00:21:03,400
- And she and her team began to track the
stars at the centre of the Milky way.
301
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And that's the centre of our galaxy.
302
00:21:05,750 --> 00:21:09,735
The very first year that we
took the data was in 1995.
303
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Then we go back to the
telescope in '96,
304
00:21:12,800 --> 00:21:17,050
and then we take our second image, and you
have two pictures. We can compare them,
305
00:21:18,000 --> 00:21:22,300
- Andrea wanted to see if the stars were
orbiting a single source of gravity, but
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00:21:22,450 --> 00:21:25,450
stars can take years to complete an orbit.
307
00:21:25,550 --> 00:21:29,239
So it was really important
that we kept going, and
308
00:21:29,264 --> 00:21:33,050
by 2000 we finally started
to see the star's curve.
309
00:21:33,300 --> 00:21:39,300
In other words, the gravitational influence
of the black hole had made those stars
310
00:21:39,350 --> 00:21:41,600
go from straight lines to starting to bend.
311
00:21:41,650 --> 00:21:45,150
The measurements were precise enough
to see that curvature. -Year by year,
312
00:21:45,300 --> 00:21:52,600
Andrea and her team built their case.
This animation represents 20 years of work
313
00:21:52,650 --> 00:21:59,400
and it tells you that it is a black hole, and
exactly how massive it is.
314
00:21:59,500 --> 00:22:02,515
Andrea's painstaking
project revealed a monster
315
00:22:02,540 --> 00:22:05,200
with more than 400
million times the mass
316
00:22:05,250 --> 00:22:09,650
of our Sun at the centre of our Milky Way.
317
00:22:09,700 --> 00:22:13,700
Today, scientists are hunting
black holes with new tools.
318
00:22:13,750 --> 00:22:19,350
CalTech astrophysicist Fiona Harrison
scans the skies with New Star,
319
00:22:19,500 --> 00:22:23,250
a telescope that looks at the universe
in high energy X-rays.
320
00:22:24,500 --> 00:22:29,500
The black hole itself doesn't emit light, but
dust and gas falls onto the black holes
321
00:22:29,950 --> 00:22:35,250
and in doing so heats up,
and it emits X-rays.
322
00:22:36,600 --> 00:22:40,600
New Star captures black holes in
a process of feasting on matter,
323
00:22:40,900 --> 00:22:44,690
and the telescope is spotting
it all over the place.
324
00:22:44,715 --> 00:22:47,450
- It's really only
10 or 20 years ago
325
00:22:47,500 --> 00:22:52,600
that we thought black holes were rare. We now
know that every galaxy, like our Milky way,
326
00:22:53,000 --> 00:22:55,600
has a massive black hole at its heart.
327
00:22:56,600 --> 00:23:01,400
so rather than being just curiosities
they're actually fundamentally important to
328
00:23:01,450 --> 00:23:03,800
why the universe is the way it is.
329
00:23:04,650 --> 00:23:07,950
So, is the Earth at risk of getting swallowed
by a black hole?
330
00:23:08,500 --> 00:23:11,235
Even though we have black
holes sprinkled throughout
331
00:23:11,260 --> 00:23:13,500
the galaxy, we're at
absolutely no danger.
332
00:23:13,550 --> 00:23:16,175
It's a common misconception
that black holes might
333
00:23:16,200 --> 00:23:18,850
suck the Earth. Well, there's
no sucking going on,
334
00:23:18,900 --> 00:23:23,550
it's just normal gravity.
It's just when you get very close to it
335
00:23:23,600 --> 00:23:26,555
that there's a region from
which even light can't
336
00:23:26,580 --> 00:23:29,500
even escape, and the Earth
is not gonna do that.
337
00:23:31,000 --> 00:23:33,913
But what if a spaceship
had a close encounter?
338
00:23:33,938 --> 00:23:36,500
What if an astronaut
dove in feet first?
339
00:23:36,650 --> 00:23:39,178
-In the simplest
descriptions of this, the
340
00:23:39,203 --> 00:23:42,350
descriptions you'll find in
most books that you read
341
00:23:42,400 --> 00:23:47,400
you're simply stretched from head to foot,
and squeezed from the sides by tidal forces
342
00:23:47,450 --> 00:23:53,400
'spaghettified' as it's well often said,
you're spaghettified if you fall in
343
00:23:53,450 --> 00:23:56,900
and you're destroyed.
That's the standard story.
344
00:24:01,200 --> 00:24:03,622
The truth is, all the
laws of physics that we
345
00:24:03,647 --> 00:24:06,200
know break down in the
heart of the black hole.
346
00:24:07,900 --> 00:24:11,100
Physicists are still working on exactly
what happens there.
347
00:24:13,150 --> 00:24:18,150
That's the gravity where there is no...
When we talk to a physicist,
348
00:24:18,200 --> 00:24:21,900
we will often say 'it's the gravity' lie.
-So you've been lying to us all these years.
349
00:24:22,500 --> 00:24:27,000
-You know how these things go: there are lies
and there are 'lies'. - I know, but now...
350
00:24:27,400 --> 00:24:30,870
The movie Interstellar deals
with physics that is well
351
00:24:30,895 --> 00:24:34,200
understood, well established,
it deals with physics
352
00:24:34,250 --> 00:24:36,625
where we make educated
guesses and we're almost
353
00:24:36,650 --> 00:24:38,700
sure but not a 100%
sure of our guesses.
354
00:24:39,000 --> 00:24:41,893
And it deals with physics
at the frontiers of
355
00:24:41,918 --> 00:24:44,900
human understanding where
we have to speculate
356
00:24:45,700 --> 00:24:50,950
and when you get beyond those frontiers,
Interstellar works hard to align itself with
357
00:24:51,500 --> 00:24:54,500
the best speculations our
scientists can imagine.
358
00:24:54,550 --> 00:24:58,200
Interstellar mines that gray area
where new ideas percolate
359
00:24:59,500 --> 00:25:03,800
and taps deep into questions
about the nature of the universe.
360
00:25:17,500 --> 00:25:22,750
In Interstellar, telescopes on Earth first
detect the presence of a wormhole
361
00:25:22,800 --> 00:25:28,000
it shows up as a gravitational anomaly
that distorts the view of space.
362
00:25:28,200 --> 00:25:33,700
We made the wormholes have all that
strong gravity. -But what then?
363
00:25:33,750 --> 00:25:35,985
Cuz then you have a
reason for your...
364
00:25:36,010 --> 00:25:38,850
- I just, I feel uncomfortable
with the wormhole
365
00:25:38,900 --> 00:25:40,000
having that much gravity.
366
00:25:40,100 --> 00:25:42,749
-When I first began working
with Christopher Nolan, he
367
00:25:42,774 --> 00:25:45,350
wanted the wormhole to have
a rather gentle gravity,
368
00:25:45,500 --> 00:25:48,425
so we discussed how big the
wormhole should be and
369
00:25:48,450 --> 00:25:51,400
we agreed that it should
be just barely big enough
370
00:25:51,450 --> 00:25:54,788
that it could be seen from
Earth through the bending
371
00:25:54,813 --> 00:25:58,050
of light around the wormhole
by it's warped space.
372
00:25:58,250 --> 00:26:02,650
-Kip Thorne worked out just the right gravity
for Interstellar's wormhole.
373
00:26:02,700 --> 00:26:06,750
Using equations based on Einstein's
theory of general relativity.
374
00:26:06,800 --> 00:26:09,355
-As we've learned, that
theory states that
375
00:26:09,380 --> 00:26:12,200
objects warp space and
time, creating gravity.
376
00:26:14,450 --> 00:26:16,769
It also predicts that
when objects move they
377
00:26:16,794 --> 00:26:19,450
generate a pulse that
propagates through spacetime
378
00:26:19,500 --> 00:26:21,100
a bit like waves through the water.
379
00:26:25,200 --> 00:26:28,745
These gravitational waves
have never been directly
380
00:26:28,770 --> 00:26:32,200
observed. They would be
small and hard to detect
381
00:26:32,250 --> 00:26:36,750
unless they were generated by
a massively violent motion.
382
00:26:38,500 --> 00:26:41,500
Like the birth of the universe.
383
00:26:44,500 --> 00:26:49,400
Physicists developed their Big Bang theory
in part by observing that today
384
00:26:49,400 --> 00:26:52,150
the universe is expanding.
385
00:26:53,000 --> 00:26:58,000
Galaxies are moving away from each other
like raisins in a rising loaf of bread
386
00:26:59,400 --> 00:27:04,500
which suggests that in the distant past,
the universe must've been much smaller.
387
00:27:04,600 --> 00:27:08,850
-If you wind the movie backwards, in the past
everything was closer together
388
00:27:08,900 --> 00:27:13,400
and you plug that idea into the equations
that Einstein gives us.
389
00:27:14,650 --> 00:27:18,300
And there's a moment which we now know
was about 14 billion years ago,
390
00:27:18,350 --> 00:27:20,550
when everything was on
top of everything else,
391
00:27:20,600 --> 00:27:24,600
when the density of stuff in the universe
was apparently infinitely big.
392
00:27:28,000 --> 00:27:32,000
Then a powerful force triggered
an expansion of space itself.
393
00:27:32,050 --> 00:27:37,050
Faster than the speed of light,
a theory called Cosmic Inflation.
394
00:27:37,100 --> 00:27:40,254
And the theory said that
this Inflation should've
395
00:27:40,279 --> 00:27:42,950
taken fluctuation from
the shape of space
396
00:27:43,000 --> 00:27:46,500
and amplify them, so they got much stronger.
397
00:27:48,100 --> 00:27:51,336
And they've become
gravitational waves, producing
398
00:27:51,361 --> 00:27:54,100
ripple from the fabric
of space and time.
399
00:27:55,400 --> 00:27:58,212
If we could detect those
ripples today, it would
400
00:27:58,237 --> 00:28:00,900
help us understand how
the Big Bang - banged.
401
00:28:00,950 --> 00:28:03,550
-The trick was always how were we going to
measure such a thing.
402
00:28:03,600 --> 00:28:08,600
And that led us to propose and develop this
very specialized experiment
403
00:28:08,650 --> 00:28:13,350
which one of my colleagues refered to
gleefully as a wild goose chase.
404
00:28:14,500 --> 00:28:18,700
CalTech physicist Jamie Bock works
in experimental cosmology.
405
00:28:18,750 --> 00:28:21,725
Experimental cosmology
is building experiments,
406
00:28:21,750 --> 00:28:24,250
trying to get back
to the dawn of time.
407
00:28:24,300 --> 00:28:27,263
-You need a hand with that?
-The focus of his latest
408
00:28:27,288 --> 00:28:30,050
experiment was the oldest
light in the universe.
409
00:28:30,100 --> 00:28:33,026
The faint afterglow of the Big Bang.
410
00:28:34,150 --> 00:28:39,550
Physicists have mapped this cosmic microwave
bacground across the universe.
411
00:28:41,200 --> 00:28:44,132
If the birth of the universe
produced gravitational
412
00:28:44,157 --> 00:28:47,000
waves, they would've warped
this primordial light
413
00:28:47,050 --> 00:28:51,306
and cause it to be polarized or curled in
a specific direction.
414
00:28:51,600 --> 00:28:54,001
-If one could measure the
polarization and then
415
00:28:54,026 --> 00:28:56,200
not only measure, but
look at its pattern,
416
00:28:56,250 --> 00:28:58,895
there might be kind of
a swirly pattern that
417
00:28:58,920 --> 00:29:01,650
would be an indicator
of gravitational waves.
418
00:29:02,800 --> 00:29:07,600
Jamie and his team designed a series
of small super-sensitive telescopes
419
00:29:07,650 --> 00:29:13,350
that they installed where the skies
are crystal clear. At the South Pole.
420
00:29:14,000 --> 00:29:19,000
The South Pole is the closest that we can get
to outer space to make our measurements.
421
00:29:20,700 --> 00:29:23,325
For eight years the team's
telescope scanned a
422
00:29:23,350 --> 00:29:26,000
patch in the sky, measuring
minute differences
423
00:29:26,050 --> 00:29:30,950
in the temperature of the cosmic
microwave background, and a pattern emerged.
424
00:29:31,000 --> 00:29:34,858
-Our results reported
that we see this swirly
425
00:29:34,883 --> 00:29:38,850
pattern of polarization
that's consistent with
426
00:29:38,900 --> 00:29:41,650
what you expect from gravitational waves.
427
00:29:41,700 --> 00:29:45,609
So they didn't really see the gravitational
waves from the early universe,
428
00:29:45,659 --> 00:29:49,409
they saw this polarization pattern that was
precisely what was predicted,
429
00:29:49,459 --> 00:29:51,459
except they were stronger than expected.
430
00:29:52,451 --> 00:29:56,701
Ok, this is like, going on immediately after
the Big Bang when the universe was a
431
00:29:56,751 --> 00:29:59,651
trillionth of a trillionth of
a trillionth of a second old.
432
00:29:59,701 --> 00:30:03,701
So it's seeing almost the
creation of the universe.
433
00:30:04,500 --> 00:30:08,300
-The finding must be confirmed
by other experiments.
434
00:30:08,600 --> 00:30:11,191
If it holds up, this will
be the first evidence
435
00:30:11,216 --> 00:30:13,450
for detection of the
gravitational waves
436
00:30:13,500 --> 00:30:16,000
predicted by Einstein.
437
00:30:17,000 --> 00:30:20,900
To contemplate the mysteries of space,
time and the universe
438
00:30:20,950 --> 00:30:23,250
can make a person feel mighty small.
439
00:30:23,300 --> 00:30:29,000
Maybe it's best to lower our sights,
hunger down and focus on planet Earth.
440
00:30:29,050 --> 00:30:33,550
But that's not really an option for you,
namely in the long run.
441
00:30:35,450 --> 00:30:39,650
Interstellar depicts a future where
living conditions on Earth are grim.
442
00:30:41,000 --> 00:30:43,000
There's only one solution.
443
00:30:44,500 --> 00:30:46,998
-Now you need to tell me
what your plan it is to
444
00:30:47,023 --> 00:30:49,700
save the world. -We're not
meant to save the world,
445
00:30:49,750 --> 00:30:51,750
we're meant to leave it.
446
00:31:08,000 --> 00:31:13,000
This blue oasis is the only place we know
that supports life.
447
00:31:20,500 --> 00:31:23,000
But that could change in a flash.
448
00:31:26,400 --> 00:31:29,400
February 15th, 2013
449
00:31:31,100 --> 00:31:35,600
A meteor shining brighter than the Sun
shrieks across Siberia.
450
00:31:35,650 --> 00:31:40,500
It's a rock 65 feet in diameter,
and when it explodes in mid-air
451
00:31:40,550 --> 00:31:46,550
it releases more than 20 times the energy
of the bomb dropped on Hiroshima.
452
00:31:51,500 --> 00:31:55,500
No one was killed, but more than
a thousand people were injured.
453
00:31:58,000 --> 00:32:02,500
Asteroids have struck Earth before.
Some 65 million years ago,
454
00:32:02,550 --> 00:32:07,300
a monster 6 miles wide may have wiped out
half the species on Earth.
455
00:32:07,350 --> 00:32:13,350
Remember the dinosaurs? A similar
impact, or worse, could happen anytime
456
00:32:13,400 --> 00:32:18,041
and turn our Blue Marble
into a lifeless rock. In the
457
00:32:18,066 --> 00:32:22,300
meantime, perhaps a greater
threat to the planet
458
00:32:22,350 --> 00:32:24,350
is us.
459
00:32:27,000 --> 00:32:31,000
And the bottom line? Earth
can not sustain us forever.
460
00:32:31,000 --> 00:32:37,000
In a few billion years, our Sun will expand
as it begins to die.
461
00:32:38,300 --> 00:32:40,800
And our planet will be toast.
462
00:32:44,150 --> 00:32:50,500
But there's good news. Unlike the dinosaurs,
we can leave Earth.
463
00:32:51,150 --> 00:33:02,150
T minus 10, 9... Ignition sequence start!
6, 5, 4, 3, 2, 1... Zero!
464
00:33:07,350 --> 00:33:10,752
Zero left. lift off of
space shuttle Atlantis.
465
00:33:10,777 --> 00:33:14,350
-Today nearly 600 people
have traveled to space.
466
00:33:16,000 --> 00:33:20,400
During the shuttle era, Marsha Ivins
made the trip five times.
467
00:33:20,450 --> 00:33:26,100
-In order to record all of this, we have
created this wiring nightmare here.
468
00:33:26,150 --> 00:33:31,150
-At Kennedy Space Center Visitor Complex
she checks in on an old friend.
469
00:33:32,800 --> 00:33:37,400
Looking at Atlantis hanging here, it's a
surreal kind of experience to think...
470
00:33:37,450 --> 00:33:42,450
I flew that into outer space. It's still
something that I have a hard time believing.
471
00:33:45,500 --> 00:33:53,250
And it makes me feel good that people still
have a wonder and an amazement and a pure joy
472
00:33:53,300 --> 00:33:57,300
for the fact that we did fly
this vehicle into space.
473
00:33:57,350 --> 00:34:01,850
-For Marsha, each mission was as
breathtaking as her first.
474
00:34:02,500 --> 00:34:08,100
-I looked up overhead, and
here was this black sky
475
00:34:08,150 --> 00:34:15,150
and this blue Earth. It all hits you at that
point: "I am not on the planet anymore."
476
00:34:15,700 --> 00:34:19,700
And every astronaut who has flewn has
come back and said the same thing.
477
00:34:19,750 --> 00:34:23,325
As you circle the Earth,
you do not see natural
478
00:34:23,350 --> 00:34:27,250
borders and boundaries that
separate the countries.
479
00:34:27,300 --> 00:34:31,950
And all of the wars, and the angst and
the strife that tear this planet apart
480
00:34:32,000 --> 00:34:35,500
seem so insignificant from that view.
481
00:34:36,700 --> 00:34:44,200
-To me space travel, space exploration has
always represented the ultimate frontier.
482
00:34:44,250 --> 00:34:48,900
It's of the absolute extremities of what
human experience is, and it's all about
483
00:34:48,950 --> 00:34:52,200
trying to in some way define
our place in the universe.
484
00:34:52,250 --> 00:34:57,400
-40 sec away from the Apollo 11 lift off.
-I remember growing up as a kid
485
00:34:57,450 --> 00:35:00,900
and we were both fascinated by
this impulse to fly.
486
00:35:01,400 --> 00:35:08,100
This impulse to build unimaginable machines
and use them to blast off into.. into space.
487
00:35:08,750 --> 00:35:11,877
-Having fired the imagination
of a generation,
488
00:35:11,902 --> 00:35:14,250
pulls into port for
the last time.
489
00:35:14,300 --> 00:35:17,444
-The space shuttles were
retired in 2011 after
490
00:35:17,469 --> 00:35:20,300
traveling more than a
half billion miles.
491
00:35:23,500 --> 00:35:26,300
Space exploration demands enormous resources.
492
00:35:26,350 --> 00:35:30,850
The kind that government agencies
like NASA can marshal.
493
00:35:30,900 --> 00:35:34,400
Recently, some new players entered the fray
494
00:35:34,450 --> 00:35:38,550
I really think we're at a dawn of a new
space era, and it's one where
495
00:35:38,600 --> 00:35:41,000
commercial companies play
a much stronger role.
496
00:35:41,050 --> 00:35:44,875
NASA's not out of the
picture, they're very much in
497
00:35:44,900 --> 00:35:48,750
the picture, but it's not
all a NASA design system.
498
00:35:48,800 --> 00:35:53,592
In 2002, Elon Musk started
his own rocket company.
499
00:35:53,617 --> 00:35:57,300
A decade later, under
contract of NASA
500
00:35:57,350 --> 00:36:00,669
SpaceX became the first
private company in
501
00:36:00,694 --> 00:36:04,350
history to carry supplies
to and from the ISS.
502
00:36:08,000 --> 00:36:11,100
Now SpaceX is tackling an
even greater challenge.
503
00:36:11,150 --> 00:36:16,150
-I started SpaceX with the idea of
trying to revolutionize space transport.
504
00:36:16,200 --> 00:36:20,000
And critical to that is
full and rapid reusability
505
00:36:20,025 --> 00:36:23,700
of the rocket. The big
issue with rocketry today
506
00:36:23,750 --> 00:36:27,450
is that you get one use out of the rocket,
and then it smashes down into the ocean
507
00:36:27,500 --> 00:36:32,500
or warms the plains of Siberia,
and you can't use it again.
508
00:36:33,500 --> 00:36:36,325
If you can, in fact,
land a rocket safely and
509
00:36:36,350 --> 00:36:39,200
then reuse it with a
minimal amount of effort
510
00:36:39,500 --> 00:36:44,500
then you can dramatically reduce the cost
of both for space transport.
511
00:36:45,000 --> 00:36:49,800
SpaceX is currently developing a fully
and rapidly reusable launch system.
512
00:36:49,850 --> 00:36:53,200
And that will take Elon closer to
a more ambitious goal:
513
00:36:54,000 --> 00:36:58,500
to help send crews to establish
a colony on Mars.
514
00:36:59,500 --> 00:37:01,800
Not an issue for the faint-hearted.
515
00:37:01,850 --> 00:37:06,600
If anybody wants to go to Mars,
their desire for adventure
516
00:37:06,700 --> 00:37:10,700
would have to overcome the desire
for comfort and safety.
517
00:37:10,750 --> 00:37:15,350
-The colony on Mars could be the next
giant leap for human kind.
518
00:37:15,400 --> 00:37:18,300
-It's such a fundamental idea
when you think about it,
519
00:37:18,350 --> 00:37:22,250
it's just the decision that has to be made
in terms of how you view the...
520
00:37:23,850 --> 00:37:26,850
the human race's place in the universe.
We are to stay here on Earth,
521
00:37:27,000 --> 00:37:30,500
or we leave and we journey
through the galaxy?
522
00:37:34,500 --> 00:37:38,500
-We'll find a way, we always have.
523
00:37:49,200 --> 00:37:51,995
To create the look and
the space technology of
524
00:37:52,020 --> 00:37:55,200
Interstellar, Christopher
Nolan took a clean design.
525
00:37:55,250 --> 00:37:59,750
-We didn't want to have anything that felt
purely decorative.
526
00:37:59,800 --> 00:38:03,300
We wanted to approach it from a much,
much more functional point of view,
527
00:38:03,350 --> 00:38:08,450
just be as convincing as possible, looking at
NASA technology that already exists today
528
00:38:08,500 --> 00:38:11,500
and the ISS, these kind of things
were our influences.
529
00:38:12,500 --> 00:38:16,000
-There's no telling how space technology
will evolve in the years to come,
530
00:38:18,000 --> 00:38:23,000
we may be decades away or longer
from establishing a colony on Mars.
531
00:38:23,750 --> 00:38:26,550
or a permanent habitat in
orbit around the Earth.
532
00:38:27,000 --> 00:38:30,000
But people around the world are
dreaming of that next step.
533
00:38:32,600 --> 00:38:37,700
At a recent space conference, NASA
and the International Space Society
534
00:38:37,750 --> 00:38:41,750
hands out awards to dozens
of forward-looking designs.
535
00:38:43,900 --> 00:38:47,900
So, a sustaining settlement
for 20,000 people.
536
00:38:49,200 --> 00:38:52,850
A moon base that mines
minerals from lunar soil.
537
00:38:53,600 --> 00:38:56,600
A fleet of robots that clean up space junk.
538
00:38:56,650 --> 00:38:59,050
-But of course this is really hard,
because we're burning fuel...
539
00:38:59,100 --> 00:39:02,900
-There's not a single PhD among
the prize-winning designers.
540
00:39:06,415 --> 00:39:10,115
These are middle and high school students
from around the world.
541
00:39:11,200 --> 00:39:14,225
One of these kids may
stand on Mars some day,
542
00:39:14,250 --> 00:39:17,300
or make a breakthrough
in propulsion systems.
543
00:39:17,350 --> 00:39:20,350
Or start a revolution in astrophysics.
544
00:39:20,700 --> 00:39:25,700
To inspire their kind of enthusiasm
is the hope of the Interstellar team.
545
00:39:26,000 --> 00:39:29,575
-I would love the kids to
watch and get excited about
546
00:39:29,600 --> 00:39:33,000
the possibilities of space
travel and exploration.
547
00:39:33,050 --> 00:39:37,700
-I would hope that this
film introduces many people
548
00:39:37,800 --> 00:39:40,166
to science that might have
not have gotten curious
549
00:39:40,191 --> 00:39:42,300
about this kind of science
in any other way.
550
00:39:42,350 --> 00:39:46,850
-I think it would be really thrilling if
people got some sense from this film,
551
00:39:46,950 --> 00:39:50,950
these ideas are worth thinking about.
552
00:39:51,700 --> 00:39:57,700
-The interplay between science and sci-fi
springs from a deep-seeded creative drive.
553
00:40:00,500 --> 00:40:04,300
To make sense of the unknown...
554
00:40:10,300 --> 00:40:14,800
to engineer new worlds...
555
00:40:17,400 --> 00:40:22,400
to dream up a better future...
we'll find answers where we always have.
556
00:40:24,000 --> 00:40:26,300
Just beyond the next horizon. (thanks vvb)
50944
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