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The universe is home
to real monsters.
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We can't see them,
but we know they're out there.
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You really can't get anything
bigger or stronger or scarier
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00:00:11,411 --> 00:00:12,742
than a black hole.
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Black holes consume
planets and stars...
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anything that gets too close.
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Black holes give physicists
no end of headaches,
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'cause they break all the rules.
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But they rule the universe.
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They are center-stage.
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We now know they dominate
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the evolution
of the universe itself.
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00:00:59,020 --> 00:01:01,750
Black holes
are the most mysterious objects
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in our universe.
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Their gravity is absolute.
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Nothing can escape.
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They can suck in whole galaxies.
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Black holes
used to be science fiction.
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Now we know they're real.
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When I was a PhD student,
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people used to giggle when
you'd hear about black holes.
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They're like unicorns,
mythical creatures.
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We called this
the "giggle factor."
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People would say,
"Beam me up, Scotty."
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Well, no one is
laughing anymore.
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So, they're not science fiction.
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Even though
we've never landed in one,
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we have enough evidence to know
that they're really out there.
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This image might not
look like much to you and me,
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but to a scientist, it's proof
that black holes exist.
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It's an actual movie
of a black hole devouring a star
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in the constellation of Aquila.
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Black holes are messy eaters.
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The red spots you see are gas
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that's being spit
out of the hole, into space.
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00:02:16,060 --> 00:02:19,090
Eventually,
over the next million years,
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this star will be eaten alive
and disappear.
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A black hole is pretty much
the end point of everything.
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It's the end point of a star.
It's the end point of matter.
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It's the end point of energy.
It's the end point of gravity.
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I mean, that's really it.
That's the top of the scale.
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Although
they have the power to destroy
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like nothing else
in the universe,
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black holes also help build
galaxies...
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a vital part
of the great cosmic machine.
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Some astronomers think
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they could even be gateways
to parallel universes.
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We are now entering
the golden age of research
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in black-hole physics.
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They could be the key
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to understanding
the birth of the universe,
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its formation,
and then its death.
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Black holes really represent,
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00:03:31,590 --> 00:03:33,820
in one sense, the frontier
of modern astronomy.
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And they're changing our ideas
about how galaxies form
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and, indeed,
how the universe works.
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Their power comes
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from one of the primary forces
in nature... gravity.
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I teach astronomy.
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And we teach our students
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that the fundamental principle
of gravity is, "gravity sucks."
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Gravity keeps our feet
on the ground
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and our planet
orbiting around the Sun.
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But in a black hole, the force
of gravity is off the charts...
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so strong,
it sucks in anything nearby.
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It can even bend
the light from distant stars.
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And if that light
gets too close,
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the black hole swallows it.
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Think of it like this.
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Imagine a black hole
as a waterfall.
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Gravity is the river
flowing toward the falls,
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and a beam of light...
the kayak.
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Upriver from the waterfall,
the current is weak.
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The kayaker can paddle
against it and get away.
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But closer to the waterfall,
the current is stronger,
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and the kayaker struggles
to escape.
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The edge of the waterfall is
like the edge of a black hole.
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No matter how strong
the kayaker is, he's going down.
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It's the same in space.
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The way black holes
are really devastating
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is because
when you get close to them,
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the gravity gets super-strong.
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So strong that they eat light.
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That's why black holes
are black.
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A black hole
is like a roach motel.
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Everything checks in.
Nothing checks out.
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Anything
that gets too close is doomed...
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planets, stars,
even whole solar systems.
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And don't think this is
some faraway phenomenon.
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Black holes are on the loose
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right here in our own
cosmic neighborhood.
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We now know there
are wandering nomads
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throughout
the Milky Way galaxy...
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vagabonds throughout the galaxy,
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where black holes can
come up right behind you
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and perhaps gobble you up,
and they won't even burp.
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If one ever comes close,
watch out.
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If a black hole found
its way into our solar system,
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it would rip us apart.
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Any kind of black hole
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that could pass
through the solar system
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would be pulling
on all the planets
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harder than the Sun does.
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And so it's just
gonna totally disrupt
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the gravitational balance
of the solar system.
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The black hole would literally
tear planets from their orbits
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and smash them into each other.
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It's just an epic disaster.
It's a bull in a china shop.
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If it got close enough
to, say, Jupiter,
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it could actually pull
the moons of Jupiter
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away from the planet itself.
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It would just be flinging
planets left and right
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everywhere as it whipped
through the solar system,
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leaving disaster in its wake.
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If a black hole
approached Earth,
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all that gravity would rip
asteroids from their orbits
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and hurl them toward our planet.
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The Earth's surface
would become an inferno.
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It would be
the beginning of the end.
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First, it would swallow up
the atmosphere,
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then the planet itself.
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Destroying
an entire solar system
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is nothing to a black hole.
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00:08:05,830 --> 00:08:10,730
But it's more than just a big,
empty, sucking piece of space.
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It's incredibly heavy.
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To get an idea just how heavy
and dense a black hole is,
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imagine the Earth.
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Now start to crush it...
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...and keep crushing
until it's packed so tight
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even the atoms themselves
collapse.
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When the Earth crushes down
to just 2 inches across,
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that's the density
of a black hole.
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It would be
the size of a golf ball,
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yet weigh the same as the Earth,
with the same amount of gravity.
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What can make
something that small,
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that dense, and that powerful?
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We don't have external forces,
large pistons in the universe,
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to create black holes.
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00:09:04,760 --> 00:09:07,450
So the only way the real
black holes of the universe form
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is if gravity
can do the job itself.
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00:09:09,560 --> 00:09:13,360
There is only
one place in the universe
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that generates
that much gravity.
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And it's
inside the largest stars.
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When massive stars 10 times
heavier than our sun die,
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gravity crushes them,
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creating a huge explosion,
a supernova.
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00:09:40,220 --> 00:09:45,560
But some stars
are even bigger than that.
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These supermassive stars weigh
100 times more than our sun
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and have 100 times more gravity.
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When one of these stars dies,
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it sets off the biggest
explosion in the universe...
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A hypernova.
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This is the birth
of a black hole.
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Our universe is full of stars.
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At the end of their lives,
some die quietly.
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Others go out
in spectacular explosions.
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And some give birth
to black holes.
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If you have a star,
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a supermassive star that's
100 times the mass of the Sun,
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at the end of its life,
the core runs out of fuel.
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There's nothing left
to hold it up,
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and the core collapses
down into a black hole.
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When that happens,
the enormous gravity
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generated at the heart
of supermassive stars runs wild.
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This is the dying star
V.Y. Canis Majoris.
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It's more than
a billion kilometers across.
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Like all stars, it's a giant
nuclear-fusion reactor,
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pumping energy outward.
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At the same time, the star's
extreme gravity crushes inward.
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For a few million years,
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fusion and gravity
are locked in standoff.
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But when the star
runs out of fuel,
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fusion stops
and the stalemate ends.
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Gravity wins.
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In a millisecond,
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the core shrinks to a fraction
of its original size
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and a baby black hole is born.
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Immediately,
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it starts to cannibalize
what's left of the star.
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00:12:05,070 --> 00:12:08,440
As matter swirls into the black
hole, it gets incredibly hot.
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And there are magnetic forces
and frictional forces,
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and it's just a witch's brew,
a nightmare,
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what's going on right above
the surface of the black hole.
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The new black hole in the middle
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keeps feeding on the body
of the star around it.
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It eats the gas so fast,
it chokes and coughs,
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blasting out
huge beams of energy.
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They basically
eat their way out from the star.
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This happens in milliseconds.
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It happens before
the rest of the star even knows
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the core is gone.
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00:12:43,040 --> 00:12:47,480
And so basically, the star is
dead before it hits the ground.
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00:12:51,150 --> 00:12:54,950
Finally, the star explodes.
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00:12:57,690 --> 00:13:02,890
In one second, it blasts out
100 times more energy
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00:13:02,960 --> 00:13:07,160
than our sun will produce
over its entire life.
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00:13:09,630 --> 00:13:14,370
What's left is a new black hole
and two jets of energy
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00:13:14,440 --> 00:13:19,030
hurtling through the universe
at the speed of light.
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00:13:19,110 --> 00:13:22,740
These jets are called
"gamma-ray bursts."
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00:13:28,190 --> 00:13:31,250
They're
incredibly energetic events.
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00:13:31,320 --> 00:13:33,590
In terms
of raw energy and power,
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00:13:33,660 --> 00:13:36,890
gamma ray bursts are second
only to the Big Bang itself.
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Most of them last
only a few seconds.
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00:13:41,530 --> 00:13:44,970
And they fry
anything in their way.
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00:13:48,870 --> 00:13:52,170
They're so intense that
if there was a gamma-ray burster
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00:13:52,240 --> 00:13:55,210
in the region of our galaxy
near our solar system,
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00:13:55,280 --> 00:13:58,610
it could literally vaporize
the entire planet.
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00:13:58,680 --> 00:14:03,710
Fortunately, most gamma-ray
bursts occur outside our galaxy.
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00:14:10,730 --> 00:14:13,630
But they tell us
something important
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about black holes
and how our universe works.
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00:14:18,740 --> 00:14:22,040
What we were seeing every time
a gamma-ray burst went off
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was basically
the birth cry of a black hole.
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00:14:24,810 --> 00:14:29,940
By counting gamma-ray
bursts, astronomers can figure out
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00:14:30,010 --> 00:14:32,640
how many black holes
are being created.
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00:14:32,720 --> 00:14:36,910
In 2004, NASA launched
the Swift probe
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00:14:36,990 --> 00:14:40,390
to scan the universe
for gamma-ray bursts.
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00:14:40,460 --> 00:14:41,390
Five...
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00:14:41,460 --> 00:14:42,430
four...
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00:14:42,490 --> 00:14:43,460
three...
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00:14:43,530 --> 00:14:44,590
two...
220
00:14:44,660 --> 00:14:46,720
one...
We have ignition.
221
00:14:46,800 --> 00:14:50,130
And we have lift-off
of NASA's Swift spacecraft,
222
00:14:50,200 --> 00:14:53,430
on a mission to study
and understand gamma-ray bursts
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00:14:53,500 --> 00:14:54,970
throughout the universe.
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00:15:02,380 --> 00:15:05,400
This is the most
powerful gamma-ray burst
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00:15:05,480 --> 00:15:07,570
Swift has detected so far.
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00:15:07,650 --> 00:15:11,550
The flash of light announces
the birth of a new black hole
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00:15:11,620 --> 00:15:14,090
on the other side
of the universe.
228
00:15:18,360 --> 00:15:23,130
Swift can only look at
a fraction of what's out there.
229
00:15:26,470 --> 00:15:31,270
Still, it detects at least
one gamma-ray burst every day.
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00:15:33,240 --> 00:15:37,840
That discovery rocked astronomy
to its foundations.
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00:15:40,280 --> 00:15:43,050
We once thought
that black holes, like unicorns,
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00:15:43,120 --> 00:15:45,680
could never be found.
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00:15:45,760 --> 00:15:49,090
We now believe that there are
perhaps billions of black holes
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00:15:49,160 --> 00:15:50,390
in the night sky.
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00:15:50,460 --> 00:15:53,090
When we look around our galaxy
and other galaxies,
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00:15:53,160 --> 00:15:57,960
it's clear that the universe
is full of powerful black holes.
237
00:15:58,040 --> 00:16:00,530
Finding black holes
is one thing.
238
00:16:00,600 --> 00:16:02,200
Figuring out how they work...
239
00:16:02,270 --> 00:16:04,370
that's a whole different
ball game.
240
00:16:04,440 --> 00:16:07,140
The only way to find out
is to visit one.
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00:16:07,210 --> 00:16:11,550
You'd have to take a spacecraft
across the vastness of space
242
00:16:11,620 --> 00:16:13,380
just to get close to it.
243
00:16:13,450 --> 00:16:17,610
Then you'd have to go
inside the black hole.
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00:16:17,690 --> 00:16:19,520
There, you'd find a place
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00:16:19,590 --> 00:16:23,720
where reality breaks down
and time stands still.
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00:16:27,400 --> 00:16:30,700
There are billions
of black holes in the universe.
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00:16:30,770 --> 00:16:34,070
We can detect them
with telescopes and satellites.
248
00:16:34,140 --> 00:16:38,730
But we don't actually know
what they're like up-close.
249
00:16:38,810 --> 00:16:40,140
It's a long way off,
250
00:16:40,210 --> 00:16:42,770
but scientists
are already speculating
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00:16:42,850 --> 00:16:46,150
about a mission
to a black hole...
252
00:16:46,220 --> 00:16:50,950
A one-way trip to the most
dangerous place in the universe.
253
00:16:54,690 --> 00:16:56,130
Originally,
254
00:16:56,190 --> 00:17:01,030
physicists were horrified
at the idea of black holes.
255
00:17:01,100 --> 00:17:02,620
They wanted to banish them,
256
00:17:02,700 --> 00:17:05,360
because the laws of physics,
as we know them,
257
00:17:05,440 --> 00:17:08,340
seem to break down
at the instant of a black hole.
258
00:17:08,410 --> 00:17:09,960
Time stops.
259
00:17:11,410 --> 00:17:14,170
Gravity becomes infinite.
260
00:17:14,240 --> 00:17:17,610
This is a nightmare.
261
00:17:17,680 --> 00:17:20,980
Obviously, we can't send
humans anywhere near a black hole.
262
00:17:21,050 --> 00:17:23,710
But a robot?
Well, sure.
263
00:17:23,790 --> 00:17:26,850
A robotic probe
could transmit data back
264
00:17:26,920 --> 00:17:29,590
just before
it goes over the edge.
265
00:17:29,660 --> 00:17:34,600
That edge of a black hole
is called the "event horizon."
266
00:17:34,670 --> 00:17:36,790
It's the edge
of time and space...
267
00:17:36,870 --> 00:17:40,430
at least,
in the universe we know.
268
00:17:40,500 --> 00:17:42,500
We call the event horizon
"event horizon"
269
00:17:42,570 --> 00:17:43,560
quite simply because
270
00:17:43,640 --> 00:17:45,400
it separates space
into two regions.
271
00:17:48,210 --> 00:17:49,610
It's not a physical surface.
272
00:17:49,680 --> 00:17:52,980
You might not even notice it
if you were falling through it,
273
00:17:53,050 --> 00:17:56,250
but ultimately, once you're
inside of it, you're doomed.
274
00:17:56,320 --> 00:17:58,450
As you approach
the event horizon,
275
00:17:58,520 --> 00:18:00,220
gravity gets stronger
276
00:18:00,290 --> 00:18:04,320
and very strange things
start to happen.
277
00:18:04,400 --> 00:18:07,520
As you fall
into a black hole feet-first,
278
00:18:07,600 --> 00:18:10,070
your feet are closer
to the black hole.
279
00:18:10,130 --> 00:18:13,760
And so the gravity they feel
is stronger.
280
00:18:13,840 --> 00:18:15,570
Your head is not quite as close,
281
00:18:15,640 --> 00:18:17,770
and so the gravity it feels
is less.
282
00:18:17,840 --> 00:18:20,540
And basically, what happens is,
you get stretched out.
283
00:18:20,610 --> 00:18:22,910
Your feet are being pulled
much harder than your head,
284
00:18:22,980 --> 00:18:24,280
and you're like a piece of taffy
285
00:18:24,350 --> 00:18:26,080
being pulled
between two strong people.
286
00:18:28,550 --> 00:18:30,610
As you get thinner
and thinner and thinner,
287
00:18:30,690 --> 00:18:32,660
as you get closer
and closer and closer,
288
00:18:32,720 --> 00:18:36,220
you're undergoing a process
we call "spaghettification"
289
00:18:36,290 --> 00:18:40,250
because you're basically turned
into a long, thin tube of pasta.
290
00:18:44,200 --> 00:18:47,660
Gravity would stretch
our robotic probe to the limit,
291
00:18:47,740 --> 00:18:49,430
then rip it apart.
292
00:18:58,080 --> 00:19:00,520
But imagine
if the probe was strong enough
293
00:19:00,580 --> 00:19:03,020
to survive and keep going.
294
00:19:05,960 --> 00:19:11,330
As it gets close to the event
horizon, everything goes crazy.
295
00:19:11,400 --> 00:19:16,890
Gravity is so extreme,
it stops time.
296
00:19:16,970 --> 00:19:19,230
We think of time
as being endless.
297
00:19:19,300 --> 00:19:22,470
However, in a black hole,
in some sense, time stops.
298
00:19:26,740 --> 00:19:29,710
This sounds like it's
nuts, but that's the way it works.
299
00:19:29,780 --> 00:19:31,150
It's in the math.
300
00:19:31,220 --> 00:19:35,550
It's actually woven into the
fabric of the universe itself.
301
00:19:35,620 --> 00:19:38,320
If you were to watch
from a distance,
302
00:19:38,390 --> 00:19:40,720
the robot probe
would seem to slow down
303
00:19:40,790 --> 00:19:43,260
as it gets closer
to the black hole.
304
00:19:43,330 --> 00:19:47,060
Then it would appear to stop
completely.
305
00:19:47,130 --> 00:19:50,190
The whole process
might just take a brief moment.
306
00:19:50,270 --> 00:19:51,600
But from the outside,
307
00:19:51,670 --> 00:19:55,800
you appear to freeze
and fall ever more slowly.
308
00:19:55,870 --> 00:19:58,500
You actually can never observe
an object fall
309
00:19:58,580 --> 00:20:00,870
all the way
through the event horizon.
310
00:20:00,940 --> 00:20:03,310
It literally freezes
at the surface
311
00:20:03,380 --> 00:20:06,470
because its clock
is going infinitely slowly
312
00:20:06,550 --> 00:20:07,980
compared to yours.
313
00:20:08,050 --> 00:20:12,890
In reality,
the probe hasn't stopped at all.
314
00:20:12,960 --> 00:20:17,150
It keeps going
and crosses the event horizon.
315
00:20:19,060 --> 00:20:21,960
If the probe
points its cameras backwards,
316
00:20:22,030 --> 00:20:24,430
towards the entrance
of the black hole,
317
00:20:24,500 --> 00:20:30,100
it will see light
being sucked in.
318
00:20:30,170 --> 00:20:35,170
If it points the camera forward,
at first it sees only black,
319
00:20:35,250 --> 00:20:38,580
but as it moves toward the heart
of the black hole,
320
00:20:38,650 --> 00:20:43,420
it encounters the most bizarre
place in the universe.
321
00:20:45,060 --> 00:20:48,990
The black hole's immense gravity
pulls everything down
322
00:20:49,060 --> 00:20:52,390
to an unimaginably small point
at its center.
323
00:20:52,460 --> 00:20:56,990
Scientists call it
the "singularity."
324
00:20:57,070 --> 00:20:59,560
We really just don't know
325
00:20:59,640 --> 00:21:01,760
what happens
at the center of a black hole.
326
00:21:01,840 --> 00:21:03,070
The densities are so great
327
00:21:03,140 --> 00:21:05,670
that the laws of physics
break down, as we know them.
328
00:21:07,740 --> 00:21:10,440
A singularity is a point
of infinite gravity,
329
00:21:10,510 --> 00:21:13,640
where space and time
become meaningless.
330
00:21:13,720 --> 00:21:15,550
Now, that is ridiculous.
331
00:21:15,620 --> 00:21:20,420
A singularity is basically a
word for saying "I don't know."
332
00:21:20,490 --> 00:21:22,750
It's a word for saying
"I'm clueless."
333
00:21:27,030 --> 00:21:28,160
Even now,
334
00:21:28,230 --> 00:21:30,720
scientists can't really answer
the question,
335
00:21:30,800 --> 00:21:32,100
"What is a black hole?"
336
00:21:32,170 --> 00:21:33,690
It's upsetting, a little bit,
337
00:21:33,770 --> 00:21:35,290
to think that there are objects
out there
338
00:21:35,370 --> 00:21:37,700
that are breaking
the laws of physics.
339
00:21:37,770 --> 00:21:40,110
There must be bigger laws
340
00:21:40,180 --> 00:21:42,010
that are being used
by these black holes,
341
00:21:42,080 --> 00:21:43,940
that are being obeyed
by these black holes,
342
00:21:44,010 --> 00:21:45,570
that we just
don't understand yet.
343
00:21:48,090 --> 00:21:51,180
Okay, so,
the one thing we do understand
344
00:21:51,260 --> 00:21:54,690
is that black holes are born
from dying stars.
345
00:21:56,830 --> 00:22:00,290
And most are small...
around 20 kilometers across.
346
00:22:03,640 --> 00:22:06,600
But now
scientists have discovered
347
00:22:06,670 --> 00:22:09,900
that some black holes
are much bigger.
348
00:22:09,970 --> 00:22:13,100
They're called
"supermassive black holes."
349
00:22:13,180 --> 00:22:17,440
They're the same size
as our entire solar system.
350
00:22:17,520 --> 00:22:23,010
And one of these monsters lies
at the heart of our own galaxy.
351
00:22:28,560 --> 00:22:32,930
Our solar system lies
in the Milky Way galaxy.
352
00:22:33,000 --> 00:22:37,590
It's made up of billions
of stars, including our sun...
353
00:22:39,900 --> 00:22:42,960
...all revolving
around a mysterious region
354
00:22:43,040 --> 00:22:45,630
right at the center.
355
00:22:45,710 --> 00:22:48,940
Children ask the question...
356
00:22:49,010 --> 00:22:50,640
if the Moon goes
around the Earth,
357
00:22:50,710 --> 00:22:52,010
the Earth goes around the Sun,
358
00:22:52,080 --> 00:22:53,740
then what does the Sun
go around?
359
00:22:53,820 --> 00:22:55,220
It's a good question.
360
00:22:55,290 --> 00:22:57,580
And astronomers ask
the same thing.
361
00:22:57,650 --> 00:22:59,680
Maybe there was something
going on
362
00:22:59,760 --> 00:23:01,450
at the heart of the Milky Way...
363
00:23:01,530 --> 00:23:06,900
perhaps a black hole
at the very center.
364
00:23:06,960 --> 00:23:11,020
But because we can't
actually see a black hole,
365
00:23:11,100 --> 00:23:16,200
the best they could do
was look for telltale signs.
366
00:23:16,270 --> 00:23:17,930
Using infrared telescopes,
367
00:23:18,010 --> 00:23:20,640
they looked
at the middle of the galaxy
368
00:23:20,710 --> 00:23:24,010
and discovered
a densely packed swarm
369
00:23:24,080 --> 00:23:25,910
of millions of stars.
370
00:23:25,980 --> 00:23:29,850
But they couldn't see
what was at the center.
371
00:23:35,030 --> 00:23:39,520
One team has spent 15 years
looking for clues.
372
00:23:44,200 --> 00:23:47,430
High above the clouds
on Mauna Kea, in Hawaii,
373
00:23:47,500 --> 00:23:50,800
the giant Keck telescope
has the power
374
00:23:50,870 --> 00:23:55,310
to see right through
to the center of the Milky Way.
375
00:24:02,090 --> 00:24:04,710
The region
which we have to study
376
00:24:04,790 --> 00:24:08,090
to prove that there's a
black hole is incredibly small.
377
00:24:08,160 --> 00:24:09,750
It is absolutely the case
378
00:24:09,830 --> 00:24:12,350
of looking
for a needle in a haystack,
379
00:24:12,430 --> 00:24:15,260
except we know
exactly where the needle is.
380
00:24:17,130 --> 00:24:20,190
Andrea Ghez
has spent countless nights
381
00:24:20,270 --> 00:24:22,530
scanning
the center of the galaxy
382
00:24:22,610 --> 00:24:24,940
for signs of a black hole.
383
00:24:25,010 --> 00:24:26,810
To be able
to do this experiment,
384
00:24:26,880 --> 00:24:28,240
one has to be able to see
385
00:24:28,310 --> 00:24:31,080
the stars that are very close
to the center of the galaxy
386
00:24:31,150 --> 00:24:33,910
and to position them
incredibly accurately.
387
00:24:33,980 --> 00:24:35,710
And this would be equivalent
388
00:24:35,790 --> 00:24:38,780
to me in Los Angeles
looking at you in New York
389
00:24:38,860 --> 00:24:42,920
and seeing you be able to move
your finger like this.
390
00:24:56,770 --> 00:24:58,640
As the Keck kicks into action,
391
00:24:58,710 --> 00:25:02,740
a laser beam detects tiny
disturbances in the atmosphere
392
00:25:02,810 --> 00:25:05,180
that would distort the image.
393
00:25:07,920 --> 00:25:13,790
Motors then adjust the huge
30-foot mirror to compensate.
394
00:25:13,860 --> 00:25:16,020
The image is clear enough
395
00:25:16,090 --> 00:25:20,120
to track the stars
at the heart of our galaxy.
396
00:25:22,470 --> 00:25:26,930
Ghez has taken thousands of
images over the last 15 years.
397
00:25:27,000 --> 00:25:32,530
And what they reveal is amazing.
398
00:25:32,610 --> 00:25:35,270
The stars
at the center of the galaxy
399
00:25:35,350 --> 00:25:38,210
are moving
at millions of kilometers an hour.
400
00:25:44,690 --> 00:25:49,060
The center of the galaxy
is a very extreme environment.
401
00:25:49,130 --> 00:25:51,030
The speeds with which stars move
402
00:25:51,090 --> 00:25:54,060
is much higher than
anywhere else in our galaxy.
403
00:25:54,130 --> 00:25:56,890
And that is absolutely
the signpost of the black hole.
404
00:26:02,240 --> 00:26:08,080
They look like tiny planets
racing around an invisible sun.
405
00:26:08,140 --> 00:26:11,600
But they're not planets.
They're stars.
406
00:26:11,680 --> 00:26:13,670
It takes a lot of gravity
407
00:26:13,750 --> 00:26:18,020
to swing huge stars around
in such fast, tight orbits.
408
00:26:18,090 --> 00:26:23,050
There's only one thing in the
universe with that much pull...
409
00:26:23,130 --> 00:26:28,120
a supermassive black hole.
410
00:26:28,200 --> 00:26:30,390
Watching these things
shows the presence
411
00:26:30,470 --> 00:26:33,270
of a 4-million-times-
the-mass-of-our-sun black hole,
412
00:26:33,340 --> 00:26:35,600
located right at the heart
of our galaxy.
413
00:26:37,270 --> 00:26:39,440
It is a huge discovery.
414
00:26:39,510 --> 00:26:43,280
Everything in our galaxy,
including our own solar system,
415
00:26:43,350 --> 00:26:48,010
orbits around
a supermassive black hole.
416
00:26:48,080 --> 00:26:51,110
But the Milky Way
isn't the only galaxy
417
00:26:51,190 --> 00:26:53,490
with a black hole in the middle.
418
00:26:53,560 --> 00:26:55,720
There are
supermassive black holes
419
00:26:55,790 --> 00:26:59,190
at the heart of most galaxies
in the universe.
420
00:26:59,260 --> 00:27:02,750
The Andromeda galaxy
is our closest neighbor.
421
00:27:02,830 --> 00:27:06,270
It circles around
a supermassive black hole
422
00:27:06,340 --> 00:27:11,040
weighing 140 million times
more than our sun.
423
00:27:11,110 --> 00:27:14,470
Other galaxies,
like this one, M87,
424
00:27:14,540 --> 00:27:20,480
have black holes weighing
as much as 20 billion suns.
425
00:27:20,550 --> 00:27:23,110
How do black holes get so big,
426
00:27:23,190 --> 00:27:27,560
and what are they doing
at the center of galaxies?
427
00:27:27,620 --> 00:27:33,030
For answers, we have to go back
nearly 14 billion years
428
00:27:33,100 --> 00:27:37,030
to the beginning
of the universe.
429
00:27:37,100 --> 00:27:38,760
Back then,
430
00:27:38,840 --> 00:27:43,400
the universe was filled with
clouds of gas from the Big Bang.
431
00:27:44,970 --> 00:27:46,500
In some places,
432
00:27:46,580 --> 00:27:50,410
the gas was thick enough
for millions of stars to form.
433
00:27:55,320 --> 00:27:58,480
Most of these new stars
were supermassive.
434
00:27:58,550 --> 00:28:00,540
They burned hot and fast
435
00:28:00,620 --> 00:28:04,650
and then exploded,
creating lots of black holes.
436
00:28:14,240 --> 00:28:17,000
The early universe
was a wild-and-crazy place
437
00:28:17,070 --> 00:28:19,270
where huge regions of mass
438
00:28:19,340 --> 00:28:20,640
were collapsing
catastrophically,
439
00:28:20,710 --> 00:28:21,970
producing black holes.
440
00:28:22,040 --> 00:28:24,740
And, in fact, the early universe
might have been
441
00:28:24,810 --> 00:28:27,180
full of emerging black holes
everywhere.
442
00:28:29,890 --> 00:28:32,580
Gravity pulled
many of them together.
443
00:28:32,660 --> 00:28:34,920
All over the early universe,
444
00:28:34,990 --> 00:28:39,190
they merged, creating
larger and larger black holes.
445
00:28:42,200 --> 00:28:45,930
Over hundreds of millions
of years, each black hole grew,
446
00:28:46,000 --> 00:28:50,370
producing stronger gravity and
pulling in more and more gas.
447
00:28:50,440 --> 00:28:55,040
New stars were born from the
gas, forming primitive galaxies.
448
00:28:57,110 --> 00:29:00,910
But the black hole
kept on sucking in gas,
449
00:29:00,980 --> 00:29:02,780
until it could take no more,
450
00:29:02,850 --> 00:29:06,910
igniting the most powerful
flamethrower in the universe.
451
00:29:20,940 --> 00:29:24,300
A young galaxy
is a vast cluster of stars,
452
00:29:24,370 --> 00:29:27,400
stars that formed
from clouds of gas.
453
00:29:32,350 --> 00:29:34,820
At the center of the new galaxy
454
00:29:34,880 --> 00:29:39,290
is a young, supermassive
black hole feeding on the gas,
455
00:29:39,360 --> 00:29:41,290
getting bigger and bigger.
456
00:29:41,360 --> 00:29:42,550
If you can imagine,
457
00:29:42,630 --> 00:29:45,490
when a galaxy is very young
and still forming,
458
00:29:45,560 --> 00:29:48,330
there's a supermassive
black hole forming at the core,
459
00:29:48,400 --> 00:29:50,330
and the gas
is still falling into it
460
00:29:50,400 --> 00:29:51,870
and still forming the galaxy.
461
00:29:51,930 --> 00:29:54,230
Well,
near that central black hole,
462
00:29:54,300 --> 00:29:55,930
things are getting very hot.
463
00:29:56,010 --> 00:29:57,630
That material is heating up.
464
00:29:57,710 --> 00:30:01,270
Gas is speeding
into the black hole.
465
00:30:01,340 --> 00:30:03,780
But it overloads,
466
00:30:03,850 --> 00:30:08,510
and there is no room
for all that excess hot gas.
467
00:30:08,580 --> 00:30:12,920
It has nowhere to go but out.
468
00:30:12,990 --> 00:30:18,050
It's blasted into space
in huge jets of energy.
469
00:30:22,700 --> 00:30:26,160
Each jet is 20 times wider
than our solar system
470
00:30:26,240 --> 00:30:30,400
and shoots
clear through the galaxy.
471
00:30:30,470 --> 00:30:36,380
The supermassive black hole
has ignited a quasar.
472
00:30:36,450 --> 00:30:38,140
Quasars are literally
473
00:30:38,210 --> 00:30:40,310
the brightest objects
in the universe.
474
00:30:40,380 --> 00:30:43,380
They're so intense, they can
outshine an entire galaxy.
475
00:30:43,450 --> 00:30:46,220
This is a real photograph
476
00:30:46,290 --> 00:30:50,090
of a real quasar
in the galaxy M87,
477
00:30:50,160 --> 00:30:53,750
50 million light-years away.
478
00:30:57,230 --> 00:31:00,830
Quasars blast away
huge quantities of gas
479
00:31:00,900 --> 00:31:02,840
from the surrounding galaxy...
480
00:31:05,540 --> 00:31:10,070
...the equivalent
of 10 Earths every minute.
481
00:31:13,520 --> 00:31:15,640
When you heat up a gas,
482
00:31:15,720 --> 00:31:17,810
it tends to expand
and it blows outward.
483
00:31:17,890 --> 00:31:20,520
And it's sort of like a wind,
but on a huge scale.
484
00:31:20,590 --> 00:31:22,560
And you get a black-hole wind,
485
00:31:22,630 --> 00:31:25,150
gas blowing out
from the black hole.
486
00:31:25,230 --> 00:31:29,930
Black holes suck gas in.
Quasars blow it out.
487
00:31:30,000 --> 00:31:34,560
But eventually there's no gas
left to make stars,
488
00:31:34,640 --> 00:31:36,330
and the galaxy stops growing.
489
00:31:36,410 --> 00:31:39,140
So we think
that the eventual size
490
00:31:39,210 --> 00:31:40,700
that a galaxy can achieve
491
00:31:40,780 --> 00:31:43,270
depends on the black hole
in its center.
492
00:31:43,350 --> 00:31:44,870
The two are tied together.
493
00:31:46,850 --> 00:31:51,650
With no gas left to feed
on, the quasar jets shrink and die.
494
00:31:53,120 --> 00:31:56,150
What's left
is a supermassive black hole
495
00:31:56,230 --> 00:32:00,630
at the center of the galaxy,
with a whole lot of young stars,
496
00:32:00,700 --> 00:32:04,630
just like our Milky Way
back when it was young.
497
00:32:04,700 --> 00:32:07,360
Early on
in the history of the Milky Way,
498
00:32:07,440 --> 00:32:10,770
when it was a young galaxy,
we were probably a quasar.
499
00:32:10,840 --> 00:32:14,280
Probably every big galaxy
was a quasar when it was young.
500
00:32:14,340 --> 00:32:15,830
But right now we're old enough
501
00:32:15,910 --> 00:32:17,880
that the galaxy
has quieted down.
502
00:32:19,650 --> 00:32:23,520
Now astronomers
are looking for quasars,
503
00:32:23,590 --> 00:32:26,920
the secret
to finding more black holes
504
00:32:26,990 --> 00:32:29,550
and figuring out how they work.
505
00:32:29,630 --> 00:32:32,990
The Chandra observatory
is a space telescope
506
00:32:33,060 --> 00:32:38,760
that can detect the powerful
x-rays quasars send out.
507
00:32:38,830 --> 00:32:41,670
It's found thousands.
508
00:32:41,740 --> 00:32:44,210
These remarkable images show
509
00:32:44,270 --> 00:32:49,180
quasars of all shapes and sizes
firing out into space.
510
00:32:53,250 --> 00:32:55,380
Each one is a signpost
511
00:32:55,450 --> 00:32:59,480
for a young galaxy with
a new black hole at its center.
512
00:33:03,330 --> 00:33:06,320
These quasars
will eventually calm down
513
00:33:06,400 --> 00:33:11,660
as their galaxy matures
and takes its final shape.
514
00:33:11,730 --> 00:33:13,600
I guess the universe
is a lot like people...
515
00:33:13,670 --> 00:33:15,030
active when they're young,
516
00:33:15,100 --> 00:33:17,440
a little bit quieter and more
relaxed when they get older.
517
00:33:19,640 --> 00:33:22,610
We now know
that supermassive black holes
518
00:33:22,680 --> 00:33:26,670
and the quasars they create
control galaxies.
519
00:33:26,750 --> 00:33:30,710
Black holes are central
to understanding how galaxies form.
520
00:33:30,790 --> 00:33:33,760
They're a key to understanding
how they evolve with time.
521
00:33:33,820 --> 00:33:36,160
So, in fact,
rather than being obscura,
522
00:33:36,230 --> 00:33:38,220
they're fundamental
to our understanding
523
00:33:38,290 --> 00:33:40,020
of our galaxies
and our universe.
524
00:33:40,600 --> 00:33:44,790
The only way to
find out more about black holes
525
00:33:44,870 --> 00:33:46,830
is to get a good look at one.
526
00:33:46,900 --> 00:33:50,630
And since an up-close visit
is, well, not a good idea,
527
00:33:50,710 --> 00:33:53,610
astronomers are trying to devise
a way to take a picture
528
00:33:53,680 --> 00:33:57,480
of the supermassive black hole
at the heart of our own galaxy.
529
00:33:57,550 --> 00:33:58,980
To get it,
530
00:33:59,050 --> 00:34:03,180
they'll need a telescope
as large as Earth itself.
531
00:34:16,770 --> 00:34:18,700
There's
a supermassive black hole
532
00:34:18,770 --> 00:34:22,260
at the center of the Milky Way.
533
00:34:24,610 --> 00:34:27,510
It's hidden
by a dense cluster of stars
534
00:34:27,580 --> 00:34:30,070
circling
the heart of the galaxy.
535
00:34:32,920 --> 00:34:37,350
But soon,
we hope we'll be able to see it.
536
00:34:37,420 --> 00:34:40,790
Seeing is believing.
537
00:34:40,860 --> 00:34:44,020
It would be spectacular
if we can go right up there,
538
00:34:44,090 --> 00:34:46,930
nose-to-nose
with the event horizon
539
00:34:47,000 --> 00:34:50,330
of the black hole at the center
of the Milky Way galaxy.
540
00:34:50,400 --> 00:34:53,630
And that's the Holy Grail.
541
00:34:53,700 --> 00:34:56,930
A supermassive
black hole lies hidden
542
00:34:57,010 --> 00:34:59,030
at the center of most galaxies.
543
00:34:59,110 --> 00:35:00,840
We only know they're there
544
00:35:00,910 --> 00:35:03,810
because the stars around them
are drawn in
545
00:35:03,880 --> 00:35:06,040
at millions of kilometers per hour.
546
00:35:06,120 --> 00:35:07,740
But there might still be a way
547
00:35:07,820 --> 00:35:11,310
to take a picture of the
very edge of the black hole...
548
00:35:11,390 --> 00:35:13,550
the event horizon.
549
00:35:13,620 --> 00:35:17,350
Shep Doeleman and his team
are trying to capture an image
550
00:35:17,430 --> 00:35:19,420
that shows its outline.
551
00:35:19,500 --> 00:35:21,690
We're essentially looking
for the shadow,
552
00:35:21,760 --> 00:35:23,760
or the silhouette,
of the black hole,
553
00:35:23,830 --> 00:35:27,270
within this cloud of gas
that's swirling around it.
554
00:35:27,340 --> 00:35:31,000
This technique
that we're exploiting
555
00:35:31,070 --> 00:35:34,040
is the best hope I think we have
556
00:35:34,110 --> 00:35:36,840
to actually image
a region of the universe
557
00:35:36,910 --> 00:35:40,250
which has hitherto been
completely invisible to us.
558
00:35:40,320 --> 00:35:42,550
Optical telescopes
559
00:35:42,620 --> 00:35:46,080
can't see the black hole
directly.
560
00:35:46,160 --> 00:35:49,960
But the glowing, super-heated
gas surrounding the black hole
561
00:35:50,030 --> 00:35:53,480
sends out radio waves that can
be used to make an image.
562
00:35:55,560 --> 00:36:00,830
Huge radio telescopes pick up
these signals from space.
563
00:36:00,900 --> 00:36:03,340
The antenna will move
in azimuth and elevation.
564
00:36:09,980 --> 00:36:13,680
This one, at the
M.I.T. Observatory near Boston,
565
00:36:13,750 --> 00:36:16,410
is more than 100 feet wide.
566
00:36:16,490 --> 00:36:20,550
It's big enough to detect
very faint radio emissions
567
00:36:20,620 --> 00:36:25,530
from the black hole in our own
galaxy, 25,000 light-years away.
568
00:36:25,590 --> 00:36:29,830
But it's not nearly big enough
to capture an image.
569
00:36:29,900 --> 00:36:33,360
We need to take multiple copies
of these telescopes,
570
00:36:33,440 --> 00:36:35,230
place them around the world
571
00:36:35,300 --> 00:36:39,830
to create a virtual telescope
as large as the Earth itself.
572
00:36:39,910 --> 00:36:42,810
Doeleman's team
will link up radio telescopes
573
00:36:42,880 --> 00:36:47,040
around the globe,
from Hawaii to Chile to Africa.
574
00:36:53,260 --> 00:36:55,850
When the whole network
is connected,
575
00:36:55,920 --> 00:37:00,020
they'll have a virtual dish
over 10,000 kilometers across,
576
00:37:00,100 --> 00:37:04,590
with 500 times the power
of a single telescope.
577
00:37:08,040 --> 00:37:10,530
They think
it will be powerful enough
578
00:37:10,610 --> 00:37:13,170
to take a picture
of the event horizon
579
00:37:13,240 --> 00:37:18,680
of the supermassive black hole
at the center of the Milky Way.
580
00:37:18,750 --> 00:37:21,150
They're already picking up
signals
581
00:37:21,220 --> 00:37:23,680
from the dark heart
of our galaxy.
582
00:37:23,750 --> 00:37:26,240
When we saw the first detection,
583
00:37:26,320 --> 00:37:28,980
it was a moment where I just
looked at the computer screen
584
00:37:29,060 --> 00:37:31,750
and said to myself,
"My God, we've done it.
585
00:37:31,830 --> 00:37:34,690
We've actually seen something
that's so small
586
00:37:34,760 --> 00:37:37,250
that it has to be coming from
right around the event horizon."
587
00:37:38,830 --> 00:37:42,290
The signals are still too
weak to give a complete picture,
588
00:37:42,370 --> 00:37:46,000
but Doeleman expects
the images to improve
589
00:37:46,080 --> 00:37:50,980
as more telescopes come online
over the next few years.
590
00:37:51,050 --> 00:37:56,280
Eventually, the outline of the
black hole itself should emerge.
591
00:37:58,920 --> 00:38:04,090
But even a picture can't compare
to witnessing it for yourself.
592
00:38:06,400 --> 00:38:09,730
In the distant future,
we may have the technology
593
00:38:09,800 --> 00:38:14,200
to actually enter
and pass through a black hole
594
00:38:14,270 --> 00:38:17,330
and maybe even
survive the journey.
595
00:38:22,950 --> 00:38:26,240
Then we might finally answer
the question...
596
00:38:26,320 --> 00:38:30,270
what lies
at the heart of a black hole?
597
00:38:32,450 --> 00:38:33,820
Some scientists believe
598
00:38:33,890 --> 00:38:36,590
we could use black holes
as a kind of portal,
599
00:38:36,660 --> 00:38:39,890
with the potential
for travel across the universe.
600
00:38:39,960 --> 00:38:42,690
This is still very speculative,
601
00:38:42,770 --> 00:38:45,200
but the mathematics
seem to indicate
602
00:38:45,270 --> 00:38:47,530
that as you fall
through a black hole
603
00:38:47,600 --> 00:38:49,200
that you don't simply die...
604
00:38:49,270 --> 00:38:51,900
you fall
right through a wormhole,
605
00:38:51,970 --> 00:38:56,600
which is a gateway, a shortcut
through space and time.
606
00:38:56,680 --> 00:39:00,340
Perhaps we could simply
rocket across the universe
607
00:39:00,420 --> 00:39:05,610
through a subway system
that we call a black hole.
608
00:39:05,690 --> 00:39:09,920
If black holes are
shortcuts through space and time,
609
00:39:09,990 --> 00:39:13,950
it could turn one of the coolest
ideas from science fiction
610
00:39:14,030 --> 00:39:17,690
into reality.
611
00:39:17,770 --> 00:39:21,260
Time travel is possible,
but not very practical.
612
00:39:21,340 --> 00:39:24,830
You see, the energy source,
the material that you need
613
00:39:24,910 --> 00:39:27,380
to keep the throat
of a wormhole open
614
00:39:27,440 --> 00:39:28,840
is something so exotic
615
00:39:28,910 --> 00:39:31,740
that we cannot produce it
in the laboratory.
616
00:39:31,810 --> 00:39:34,720
But if you could,
it might be possible
617
00:39:34,780 --> 00:39:38,910
to exploit the power of
black holes to visit yesterday.
618
00:39:40,560 --> 00:39:43,250
Perhaps our descendants
in the future
619
00:39:43,330 --> 00:39:46,090
have already mastered
this technology.
620
00:39:46,160 --> 00:39:48,290
So one day,
if somebody knocks on your door
621
00:39:48,360 --> 00:39:49,690
and claims to be
622
00:39:49,770 --> 00:39:52,130
your great-great-great-great-
great-great granddaughter,
623
00:39:52,200 --> 00:39:53,190
don't slam the door.
624
00:39:57,240 --> 00:40:01,540
Black holes might even
be gateways to other universes.
625
00:40:01,610 --> 00:40:04,100
On the other side
of a black hole,
626
00:40:04,180 --> 00:40:07,170
there could even be...
a Big Bang.
627
00:40:10,490 --> 00:40:14,080
As a black hole collapses
and matter falls into it,
628
00:40:14,160 --> 00:40:17,560
perhaps the matter is blown out
the other side in a white hole.
629
00:40:17,630 --> 00:40:19,790
Doesn't that sound
like the Big Bang?
630
00:40:25,470 --> 00:40:29,060
If a Big Bang is just
the flip side of a black hole,
631
00:40:29,140 --> 00:40:33,130
this could be
how our own universe was born.
632
00:40:34,940 --> 00:40:37,410
If you look at the equations
for a black hole
633
00:40:37,480 --> 00:40:39,310
and put in the parameters
of the universe...
634
00:40:39,380 --> 00:40:41,540
the mass of the universe,
the size of the universe...
635
00:40:41,620 --> 00:40:42,610
bingo!
636
00:40:42,680 --> 00:40:44,050
You find that our universe
637
00:40:44,120 --> 00:40:46,680
actually solves the equations
for a black hole.
638
00:40:46,760 --> 00:40:49,920
In other words, we could be
inside an event horizon.
639
00:40:49,990 --> 00:40:55,430
Perhaps we are actually living
inside a black hole.
640
00:40:55,500 --> 00:40:58,900
Every black hole
might be the origin
641
00:40:58,970 --> 00:41:01,770
of an entirely separate
universe.
642
00:41:01,840 --> 00:41:03,130
If that's true,
643
00:41:03,210 --> 00:41:07,800
there could be billions
of universes out there...
644
00:41:11,280 --> 00:41:16,480
...each one
full of stars, planets, life.
645
00:41:16,550 --> 00:41:19,020
Whatever we figure out later,
646
00:41:19,090 --> 00:41:22,990
we know now
that black holes are everywhere.
647
00:41:23,060 --> 00:41:24,220
They're bigger in size
648
00:41:24,290 --> 00:41:26,960
and more critical
to the evolution of the universe
649
00:41:27,030 --> 00:41:29,160
than we ever imagined.
650
00:41:40,540 --> 00:41:42,410
Literally, our understanding
651
00:41:42,480 --> 00:41:44,470
of the universe
that's important around us,
652
00:41:44,550 --> 00:41:46,880
the universe
that's visible to telescopes,
653
00:41:46,950 --> 00:41:48,750
has been profoundly affected
654
00:41:48,820 --> 00:41:52,180
by our realization
that black holes are everywhere.
655
00:41:55,160 --> 00:41:56,350
Once upon a time,
656
00:41:56,430 --> 00:41:58,020
people thought
that black-hole physics
657
00:41:58,090 --> 00:42:01,190
was too fantastic to be true.
658
00:42:01,260 --> 00:42:03,820
And now they are center-stage.
659
00:42:03,900 --> 00:42:05,300
We now know they dominate
660
00:42:05,370 --> 00:42:07,560
the evolution
of the universe itself.
661
00:42:09,540 --> 00:42:10,840
When I was a kid,
662
00:42:10,910 --> 00:42:13,140
black holes basically played
a part in science fiction.
663
00:42:13,210 --> 00:42:14,680
It was always
something to avoid.
664
00:42:14,740 --> 00:42:15,900
Your spaceship...
665
00:42:15,980 --> 00:42:17,880
you try to get around them
before you get drawn in.
666
00:42:17,950 --> 00:42:19,940
But what we've learned
since then
667
00:42:20,020 --> 00:42:22,180
is that black holes
play a huge role
668
00:42:22,250 --> 00:42:24,740
and a huge number of roles
in the universe.
669
00:42:27,690 --> 00:42:29,950
It's not an exaggeration to say
670
00:42:30,030 --> 00:42:33,720
that if black holes did not
exist, we wouldn't be here.
671
00:42:33,800 --> 00:42:36,530
We literally owe
our existence to black holes.
672
00:42:40,700 --> 00:42:44,070
The story's not over yet.
673
00:42:44,140 --> 00:42:46,700
There's still
much more to be discovered
674
00:42:46,780 --> 00:42:51,640
about the mysterious objects
called black holes...
675
00:42:51,710 --> 00:42:54,910
The masters of the universe.54220
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