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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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00:00:10,908 --> 00:00:12,239
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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00:00:23,821 --> 00:00:28,918
But they rule the universe.
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They are center-stage.
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00:00:31,962 --> 00:00:33,725
We now know they dominate
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00:00:33,797 --> 00:00:36,925
the evolution
of the universe itself.
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00:00:58,022 --> 00:01:00,752
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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00:02:15,065 --> 00:02:18,091
Eventually,
over the next million years,
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00:02:18,168 --> 00:02:22,969
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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00:03:30,641 --> 00:03:32,871
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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00:04:03,707 --> 00:04:09,202
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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00:04:41,245 --> 00:04:44,681
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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00:06:03,627 --> 00:06:05,788
throughout
the Milky Way galaxy...
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vagabonds throughout the galaxy,
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00:06:08,966 --> 00:06:12,094
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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00:08:02,946 --> 00:08:05,312
is nothing to a black hole.
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00:08:05,382 --> 00:08:10,285
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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00:08:34,811 --> 00:08:39,043
When the Earth crushes down
to just 2 inches across,
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00:08:39,116 --> 00:08:42,017
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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00:09:04,307 --> 00:09:07,003
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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00:09:09,112 --> 00:09:12,912
There is only
one place in the universe
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that generates
that much gravity.
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00:09:15,786 --> 00:09:18,516
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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00:09:39,776 --> 00:09:45,112
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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00:10:32,929 --> 00:10:37,161
Others go out
in spectacular explosions.
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00:10:37,234 --> 00:10:42,638
And some give birth
to black holes.
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00:10:42,706 --> 00:10:44,571
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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00:11:07,030 --> 00:11:11,899
This is the dying star
V.Y. Canis Majoris.
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It's more than
a billion miles 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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00:11:26,583 --> 00:11:32,021
At the same time, the star's
extreme gravity crushes inward.
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00:11:32,088 --> 00:11:34,056
For a few million years,
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fusion and gravity
are locked in standoff.
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00:11:38,228 --> 00:11:41,220
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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00:11:49,973 --> 00:11:51,565
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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00:12:04,621 --> 00:12:07,988
As matter swirls into the black
hole, it gets incredibly hot.
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00:12:08,058 --> 00:12:10,526
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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00:12:33,216 --> 00:12:36,344
They basically
eat their way out from the star.
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This happens in milliseconds.
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00:12:38,255 --> 00:12:41,019
It happens before
the rest of the star even knows
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00:12:41,091 --> 00:12:42,524
the core is gone.
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00:12:42,592 --> 00:12:47,029
And so basically, the star is
dead before it hits the ground.
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00:12:50,700 --> 00:12:54,500
Finally, the star explodes.
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00:12:57,240 --> 00:13:02,439
In one second, it blasts out
100 times more energy
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00:13:02,512 --> 00:13:06,710
than our sun will produce
over its entire life.
196
00:13:09,185 --> 00:13:13,918
What's left is a new black hole
and two jets of energy
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00:13:13,990 --> 00:13:18,586
hurtling through the universe
at the speed of light.
198
00:13:18,662 --> 00:13:22,291
These jets are called
"gamma-ray bursts."
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00:13:27,737 --> 00:13:30,797
They're
incredibly energetic events.
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00:13:30,874 --> 00:13:33,138
In terms
of raw energy and power,
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00:13:33,209 --> 00:13:36,440
gamma ray bursts are second
only to the Big Bang itself.
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00:13:38,081 --> 00:13:41,016
Most of them last
only a few seconds.
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00:13:41,084 --> 00:13:44,520
And they fry
anything in their way.
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00:13:48,425 --> 00:13:51,724
They're so intense that
if there was a gamma-ray burster
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00:13:51,795 --> 00:13:54,764
in the region of our galaxy
near our solar system,
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00:13:54,831 --> 00:13:58,164
it could literally vaporize
the entire planet.
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00:13:58,234 --> 00:14:03,262
Fortunately, most gamma-ray
bursts occur outside our galaxy.
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00:14:10,280 --> 00:14:13,181
But they tell us
something important
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00:14:13,249 --> 00:14:18,209
about black holes
and how our universe works.
210
00:14:18,288 --> 00:14:21,587
What we were seeing every time
a gamma-ray burst went off
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00:14:21,658 --> 00:14:24,286
was basically
the birth cry of a black hole.
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00:14:24,361 --> 00:14:29,492
By counting gamma-ray
bursts, astronomers can figure out
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00:14:29,566 --> 00:14:32,194
how many black holes
are being created.
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00:14:32,268 --> 00:14:36,466
In 2004, NASA launched
the Swift probe
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00:14:36,539 --> 00:14:39,940
to scan the universe
for gamma-ray bursts.
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00:14:40,009 --> 00:14:40,941
Five...
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00:14:41,010 --> 00:14:41,977
four...
218
00:14:42,045 --> 00:14:43,012
three...
219
00:14:43,079 --> 00:14:44,137
two...
220
00:14:44,214 --> 00:14:46,273
one...
We have ignition.
221
00:14:46,349 --> 00:14:49,682
And we have lift-off
of NASA's Swift spacecraft,
222
00:14:49,753 --> 00:14:52,984
on a mission to study
and understand gamma-ray bursts
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00:14:53,056 --> 00:14:54,523
throughout the universe.
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00:15:00,930 --> 00:15:03,956
This is the most
powerful gamma-ray burst
225
00:15:04,033 --> 00:15:06,126
Swift has detected so far.
226
00:15:06,202 --> 00:15:10,104
The flash of light announces
the birth of a new black hole
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00:15:10,173 --> 00:15:12,641
on the other side
of the universe.
228
00:15:16,913 --> 00:15:21,680
Swift can only look at
a fraction of what's out there.
229
00:15:26,022 --> 00:15:30,823
Still, it detects at least
one gamma-ray burst every day.
230
00:15:32,796 --> 00:15:37,392
That discovery rocked astronomy
to its foundations.
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00:15:39,836 --> 00:15:42,600
We once thought
that black holes, like unicorns,
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00:15:42,672 --> 00:15:45,232
could never be found.
233
00:15:45,308 --> 00:15:48,641
We now believe that there are
perhaps billions of black holes
234
00:15:48,711 --> 00:15:49,939
in the night sky.
235
00:15:50,013 --> 00:15:52,641
When we look around our galaxy
and other galaxies,
236
00:15:52,715 --> 00:15:57,516
it's clear that the universe
is full of powerful black holes.
237
00:15:57,587 --> 00:16:00,078
Finding black holes
is one thing.
238
00:16:00,156 --> 00:16:01,748
Figuring out how they work...
239
00:16:01,825 --> 00:16:03,918
that's a whole different
ball game.
240
00:16:03,993 --> 00:16:06,689
The only way to find out
is to visit one.
241
00:16:06,763 --> 00:16:11,097
You'd have to take a spacecraft
across the vastness of space
242
00:16:11,167 --> 00:16:12,930
just to get close to it.
243
00:16:13,002 --> 00:16:17,166
Then you'd have to go
inside the black hole.
244
00:16:17,240 --> 00:16:19,071
There, you'd find a place
245
00:16:19,142 --> 00:16:23,272
where reality breaks down
and time stands still.
246
00:16:26,950 --> 00:16:30,249
There are billions
of black holes in the universe.
247
00:16:30,320 --> 00:16:33,619
We can detect them
with telescopes and satellites.
248
00:16:33,690 --> 00:16:38,286
But we don't actually know
what they're like up-close.
249
00:16:38,361 --> 00:16:39,692
It's a long way off,
250
00:16:39,762 --> 00:16:42,322
but scientists
are already speculating
251
00:16:42,398 --> 00:16:45,697
about a mission
to a black hole...
252
00:16:45,768 --> 00:16:50,501
A one-way trip to the most
dangerous place in the universe.
253
00:16:54,244 --> 00:16:55,677
Originally,
254
00:16:55,745 --> 00:17:00,580
physicists were horrified
at the idea of black holes.
255
00:17:00,650 --> 00:17:02,174
They wanted to banish them,
256
00:17:02,252 --> 00:17:04,914
because the laws of physics,
as we know them,
257
00:17:04,988 --> 00:17:07,889
seem to break down
at the instant of a black hole.
258
00:17:07,957 --> 00:17:09,515
Time stops.
259
00:17:10,960 --> 00:17:13,724
Gravity becomes infinite.
260
00:17:13,796 --> 00:17:17,163
This is a nightmare.
261
00:17:17,233 --> 00:17:20,532
Obviously, we can't send
humans anywhere near a black hole.
262
00:17:20,603 --> 00:17:23,265
But a robot?
Well, sure.
263
00:17:23,339 --> 00:17:26,399
A robotic probe
could transmit data back
264
00:17:26,476 --> 00:17:29,138
just before
it goes over the edge.
265
00:17:29,212 --> 00:17:34,149
That edge of a black hole
is called the "event horizon."
266
00:17:34,217 --> 00:17:36,344
It's the edge
of time and space...
267
00:17:36,419 --> 00:17:39,980
at least,
in the universe we know.
268
00:17:40,056 --> 00:17:42,047
We call the event horizon
"event horizon"
269
00:17:42,125 --> 00:17:43,114
quite simply because
270
00:17:43,192 --> 00:17:44,955
it separates space
into two regions.
271
00:17:47,764 --> 00:17:49,163
It's not a physical surface.
272
00:17:49,232 --> 00:17:52,531
You might not even notice it
if you were falling through it,
273
00:17:52,602 --> 00:17:55,799
but ultimately, once you're
inside of it, you're doomed.
274
00:17:55,872 --> 00:17:57,999
As you approach
the event horizon,
275
00:17:58,074 --> 00:17:59,769
gravity gets stronger
276
00:17:59,842 --> 00:18:03,869
and very strange things
start to happen.
277
00:18:03,947 --> 00:18:07,075
As you fall
into a black hole feet-first,
278
00:18:07,150 --> 00:18:09,618
your feet are closer
to the black hole.
279
00:18:09,686 --> 00:18:13,315
And so the gravity they feel
is stronger.
280
00:18:13,389 --> 00:18:15,118
Your head is not quite as close,
281
00:18:15,191 --> 00:18:17,318
and so the gravity it feels
is less.
282
00:18:17,393 --> 00:18:20,089
And basically, what happens is,
you get stretched out.
283
00:18:20,163 --> 00:18:22,461
Your feet are being pulled
much harder than your head,
284
00:18:22,532 --> 00:18:23,829
and you're like a piece of taffy
285
00:18:23,900 --> 00:18:25,629
being pulled
between two strong people.
286
00:18:28,104 --> 00:18:30,163
As you get thinner
and thinner and thinner,
287
00:18:30,239 --> 00:18:32,207
as you get closer
and closer and closer,
288
00:18:32,275 --> 00:18:35,767
you're undergoing a process
we call "spaghettification"
289
00:18:35,845 --> 00:18:39,804
because you're basically turned
into a long, thin tube of pasta.
290
00:18:43,753 --> 00:18:47,211
Gravity would stretch
our robotic probe to the limit,
291
00:18:47,290 --> 00:18:48,985
then rip it apart.
292
00:18:57,634 --> 00:19:00,068
But imagine
if the probe was strong enough
293
00:19:00,136 --> 00:19:02,570
to survive and keep going.
294
00:19:05,508 --> 00:19:10,878
As it gets close to the event
horizon, everything goes crazy.
295
00:19:10,947 --> 00:19:16,442
Gravity is so extreme,
it stops time.
296
00:19:16,519 --> 00:19:18,783
We think of time
as being endless.
297
00:19:18,855 --> 00:19:22,018
However, in a black hole,
in some sense, time stops.
298
00:19:26,295 --> 00:19:29,264
This sounds like it's
nuts, but that's the way it works.
299
00:19:29,332 --> 00:19:30,697
It's in the math.
300
00:19:30,767 --> 00:19:35,101
It's actually woven into the
fabric of the universe itself.
301
00:19:35,171 --> 00:19:37,867
If you were to watch
from a distance,
302
00:19:37,940 --> 00:19:40,272
the robot probe
would seem to slow down
303
00:19:40,343 --> 00:19:42,811
as it gets closer
to the black hole.
304
00:19:42,879 --> 00:19:46,610
Then it would appear to stop
completely.
305
00:19:46,683 --> 00:19:49,743
The whole process
might just take a brief moment.
306
00:19:49,819 --> 00:19:51,150
But from the outside,
307
00:19:51,220 --> 00:19:55,350
you appear to freeze
and fall ever more slowly.
308
00:19:55,425 --> 00:19:58,053
You actually can never observe
an object fall
309
00:19:58,127 --> 00:20:00,425
all the way
through the event horizon.
310
00:20:00,496 --> 00:20:02,862
It literally freezes
at the surface
311
00:20:02,932 --> 00:20:06,026
because its clock
is going infinitely slowly
312
00:20:06,102 --> 00:20:07,535
compared to yours.
313
00:20:07,603 --> 00:20:12,438
In reality,
the probe hasn't stopped at all.
314
00:20:12,508 --> 00:20:16,706
It keeps going
and crosses the event horizon.
315
00:20:18,614 --> 00:20:21,515
If the probe
points its cameras backwards,
316
00:20:21,584 --> 00:20:23,984
towards the entrance
of the black hole,
317
00:20:24,053 --> 00:20:29,650
it will see light
being sucked in.
318
00:20:29,726 --> 00:20:34,720
If it points the camera forward,
at first it sees only black,
319
00:20:34,797 --> 00:20:38,130
but as it moves toward the heart
of the black hole,
320
00:20:38,201 --> 00:20:42,968
it encounters the most bizarre
place in the universe.
321
00:20:44,607 --> 00:20:48,543
The black hole's immense gravity
pulls everything down
322
00:20:48,611 --> 00:20:51,944
to an unimaginably small point
at its center.
323
00:20:52,014 --> 00:20:56,542
Scientists call it
the "singularity."
324
00:20:56,619 --> 00:20:59,110
We really just don't know
325
00:20:59,188 --> 00:21:01,315
what happens
at the center of a black hole.
326
00:21:01,390 --> 00:21:02,618
The densities are so great
327
00:21:02,692 --> 00:21:05,217
that the laws of physics
break down, as we know them.
328
00:21:05,294 --> 00:21:09,993
A singularity is a point
of infinite gravity,
329
00:21:10,066 --> 00:21:13,194
where space and time
become meaningless.
330
00:21:13,269 --> 00:21:15,100
Now, that is ridiculous.
331
00:21:15,171 --> 00:21:19,972
A singularity is basically a
word for saying "I don't know."
332
00:21:20,042 --> 00:21:22,306
It's a word for saying
"I'm clueless."
333
00:21:26,582 --> 00:21:27,708
Even now,
334
00:21:27,784 --> 00:21:30,275
scientists can't really answer
the question,
335
00:21:30,353 --> 00:21:31,650
"What is a black hole?"
336
00:21:31,721 --> 00:21:33,245
It's upsetting, a little bit,
337
00:21:33,322 --> 00:21:34,846
to think that there are objects
out there
338
00:21:34,924 --> 00:21:37,256
that are breaking
the laws of physics.
339
00:21:37,326 --> 00:21:39,658
There must be bigger laws
340
00:21:39,729 --> 00:21:41,560
that are being used
by these black holes,
341
00:21:41,631 --> 00:21:43,496
that are being obeyed
by these black holes,
342
00:21:43,566 --> 00:21:45,124
that we just
don't understand yet.
343
00:21:48,638 --> 00:21:51,732
Okay, so,
the one thing we do understand
344
00:21:51,808 --> 00:21:55,244
is that black holes are born
from dying stars.
345
00:21:57,380 --> 00:22:00,838
And most are small...
around 20 miles across.
346
00:22:04,187 --> 00:22:07,156
But now
scientists have discovered
347
00:22:07,223 --> 00:22:10,454
that some black holes
are much bigger.
348
00:22:10,526 --> 00:22:13,654
They're called
"supermassive black holes."
349
00:22:13,729 --> 00:22:17,995
They're the same size
as our entire solar system.
350
00:22:18,067 --> 00:22:23,562
And one of these monsters lies
at the heart of our own galaxy.
351
00:22:28,110 --> 00:22:32,479
Our solar system lies
in the Milky Way galaxy.
352
00:22:32,548 --> 00:22:37,144
It's made up of billions
of stars, including our sun...
353
00:22:39,455 --> 00:22:42,515
...all revolving
around a mysterious region
354
00:22:42,592 --> 00:22:45,186
right at the center.
355
00:22:45,261 --> 00:22:48,492
Children ask the question...
356
00:22:48,564 --> 00:22:50,191
if the Moon goes
around the Earth,
357
00:22:50,266 --> 00:22:51,563
the Earth goes around the Sun,
358
00:22:51,634 --> 00:22:53,295
then what does the Sun
go around?
359
00:22:53,369 --> 00:22:54,768
It's a good question.
360
00:22:54,837 --> 00:22:57,135
And astronomers ask
the same thing.
361
00:22:57,206 --> 00:22:59,231
Maybe there was something
going on
362
00:22:59,308 --> 00:23:01,003
at the heart of the Milky Way...
363
00:23:01,077 --> 00:23:06,447
perhaps a black hole
at the very center.
364
00:23:06,515 --> 00:23:10,576
But because we can't
actually see a black hole,
365
00:23:10,653 --> 00:23:15,750
the best they could do
was look for telltale signs.
366
00:23:15,825 --> 00:23:17,486
Using infrared telescopes,
367
00:23:17,560 --> 00:23:20,188
they looked
at the middle of the galaxy
368
00:23:20,263 --> 00:23:23,562
and discovered
a densely packed swarm
369
00:23:23,633 --> 00:23:25,464
of millions of stars.
370
00:23:25,534 --> 00:23:29,402
But they couldn't see
what was at the center.
371
00:23:34,577 --> 00:23:39,071
One team has spent 15 years
looking for clues.
372
00:23:43,753 --> 00:23:46,984
High above the clouds
on Mauna Kea, in Hawaii,
373
00:23:47,056 --> 00:23:50,355
the giant Keck telescope
has the power
374
00:23:50,426 --> 00:23:54,863
to see right through
to the center of the Milky Way.
375
00:24:01,637 --> 00:24:04,265
The region
which we have to study
376
00:24:04,340 --> 00:24:07,639
to prove that there's a
black hole is incredibly small.
377
00:24:07,710 --> 00:24:09,302
It is absolutely the case
378
00:24:09,378 --> 00:24:11,903
of looking
for a needle in a haystack,
379
00:24:11,981 --> 00:24:14,814
except we know
exactly where the needle is.
380
00:24:16,686 --> 00:24:19,746
Andrea Ghez
has spent countless nights
381
00:24:19,822 --> 00:24:22,086
scanning
the center of the galaxy
382
00:24:22,158 --> 00:24:24,490
for signs of a black hole.
383
00:24:24,560 --> 00:24:26,357
To be able
to do this experiment,
384
00:24:26,429 --> 00:24:27,794
one has to be able to see
385
00:24:27,863 --> 00:24:30,627
the stars that are very close
to the center of the galaxy
386
00:24:30,700 --> 00:24:33,464
and to position them
incredibly accurately.
387
00:24:33,536 --> 00:24:35,265
And this would be equivalent
388
00:24:35,338 --> 00:24:38,330
to me in Los Angeles
looking at you in New York
389
00:24:38,407 --> 00:24:42,468
and seeing you be able to move
your finger like this.
390
00:24:56,325 --> 00:24:58,190
As the Keck kicks into action,
391
00:24:58,260 --> 00:25:02,287
a laser beam detects tiny
disturbances in the atmosphere
392
00:25:02,365 --> 00:25:04,731
that would distort the image.
393
00:25:07,470 --> 00:25:13,340
Motors then adjust the huge
30-foot mirror to compensate.
394
00:25:13,409 --> 00:25:15,570
The image is clear enough
395
00:25:15,644 --> 00:25:19,671
to track the stars
at the heart of our galaxy.
396
00:25:22,018 --> 00:25:26,478
Ghez has taken thousands of
images over the last 15 years.
397
00:25:26,555 --> 00:25:32,084
And what they reveal is amazing.
398
00:25:32,161 --> 00:25:34,823
The stars
at the center of the galaxy
399
00:25:34,897 --> 00:25:37,764
are moving
at millions of miles an hour.
400
00:25:44,240 --> 00:25:48,609
The center of the galaxy
is a very extreme environment.
401
00:25:48,677 --> 00:25:50,577
The speeds with which stars move
402
00:25:50,646 --> 00:25:53,615
is much higher than
anywhere else in our galaxy.
403
00:25:53,682 --> 00:25:56,446
And that is absolutely
the signpost of the black hole.
404
00:26:01,791 --> 00:26:07,627
They look like tiny planets
racing around an invisible sun.
405
00:26:07,696 --> 00:26:11,154
But they're not planets.
They're stars.
406
00:26:11,233 --> 00:26:13,224
It takes a lot of gravity
407
00:26:13,302 --> 00:26:17,568
to swing huge stars around
in such fast, tight orbits.
408
00:26:17,640 --> 00:26:22,600
There's only one thing in the
universe with that much pull...
409
00:26:22,678 --> 00:26:27,672
a supermassive black hole.
410
00:26:27,750 --> 00:26:29,945
Watching these things
shows the presence
411
00:26:30,019 --> 00:26:32,817
of a 4-million-times-
the-mass-of-our-sun black hole,
412
00:26:32,888 --> 00:26:35,152
located right at the heart
of our galaxy.
413
00:26:36,826 --> 00:26:38,987
It is a huge discovery.
414
00:26:39,061 --> 00:26:42,827
Everything in our galaxy,
including our own solar system,
415
00:26:42,898 --> 00:26:47,562
orbits around
a supermassive black hole.
416
00:26:47,636 --> 00:26:50,662
But the Milky Way
isn't the only galaxy
417
00:26:50,739 --> 00:26:53,037
with a black hole in the middle.
418
00:26:53,109 --> 00:26:55,270
There are
supermassive black holes
419
00:26:55,344 --> 00:26:58,745
at the heart of most galaxies
in the universe.
420
00:26:58,814 --> 00:27:02,306
The Andromeda galaxy
is our closest neighbor.
421
00:27:02,384 --> 00:27:05,820
It circles around
a supermassive black hole
422
00:27:05,888 --> 00:27:10,587
weighing 140 million times
more than our sun.
423
00:27:10,659 --> 00:27:14,026
Other galaxies,
like this one, M87,
424
00:27:14,096 --> 00:27:20,035
have black holes weighing
as much as 20 billion suns.
425
00:27:20,102 --> 00:27:22,662
How do black holes get so big,
426
00:27:22,738 --> 00:27:27,107
and what are they doing
at the center of galaxies?
427
00:27:27,176 --> 00:27:32,580
For answers, we have to go back
nearly 14 billion years
428
00:27:32,648 --> 00:27:36,584
to the beginning
of the universe.
429
00:27:36,652 --> 00:27:38,313
Back then,
430
00:27:38,387 --> 00:27:42,949
the universe was filled with
clouds of gas from the Big Bang.
431
00:27:43,025 --> 00:27:44,549
In some places,
432
00:27:44,627 --> 00:27:48,461
the gas was thick enough
for millions of stars to form.
433
00:27:53,369 --> 00:27:56,532
Most of these new stars
were supermassive.
434
00:27:56,605 --> 00:27:58,596
They burned hot and fast
435
00:27:58,674 --> 00:28:02,701
and then exploded,
creating lots of black holes.
436
00:28:13,289 --> 00:28:16,053
The early universe
was a wild-and-crazy place
437
00:28:16,125 --> 00:28:18,320
where huge regions of mass
438
00:28:18,394 --> 00:28:19,691
were collapsing
catastrophically,
439
00:28:19,762 --> 00:28:21,024
producing black holes.
440
00:28:21,096 --> 00:28:23,792
And, in fact, the early universe
might have been
441
00:28:23,866 --> 00:28:26,232
full of emerging black holes
everywhere.
442
00:28:28,938 --> 00:28:31,634
Gravity pulled
many of them together.
443
00:28:31,707 --> 00:28:33,971
All over the early universe,
444
00:28:34,043 --> 00:28:38,241
they merged, creating
larger and larger black holes.
445
00:28:41,250 --> 00:28:44,981
Over hundreds of millions
of years, each black hole grew,
446
00:28:45,054 --> 00:28:49,423
producing stronger gravity and
pulling in more and more gas.
447
00:28:49,491 --> 00:28:54,087
New stars were born from the
gas, forming primitive galaxies.
448
00:28:56,165 --> 00:28:59,965
But the black hole
kept on sucking in gas,
449
00:29:00,035 --> 00:29:01,832
until it could take no more,
450
00:29:01,904 --> 00:29:05,965
igniting the most powerful
flamethrower in the universe.
451
00:29:19,989 --> 00:29:23,356
A young galaxy
is a vast cluster of stars,
452
00:29:23,425 --> 00:29:26,451
stars that formed
from clouds of gas.
453
00:29:31,400 --> 00:29:33,868
At the center of the new galaxy
454
00:29:33,936 --> 00:29:38,339
is a young, supermassive
black hole feeding on the gas,
455
00:29:38,407 --> 00:29:40,341
getting bigger and bigger.
456
00:29:40,409 --> 00:29:41,603
If you can imagine,
457
00:29:41,677 --> 00:29:44,544
when a galaxy is very young
and still forming,
458
00:29:44,613 --> 00:29:47,377
there's a supermassive
black hole forming at the core,
459
00:29:47,449 --> 00:29:49,383
and the gas
is still falling into it
460
00:29:49,451 --> 00:29:50,918
and still forming the galaxy.
461
00:29:50,986 --> 00:29:53,284
Well,
near that central black hole,
462
00:29:53,355 --> 00:29:54,982
things are getting very hot.
463
00:29:55,057 --> 00:29:56,684
That material is heating up.
464
00:29:56,759 --> 00:30:00,320
Gas is speeding
into the black hole.
465
00:30:00,396 --> 00:30:02,830
But it overloads,
466
00:30:02,898 --> 00:30:07,562
and there is no room
for all that excess hot gas.
467
00:30:07,636 --> 00:30:11,970
It has nowhere to go but out.
468
00:30:12,041 --> 00:30:17,104
It's blasted into space
in huge jets of energy.
469
00:30:21,750 --> 00:30:25,208
Each jet is 20 times wider
than our solar system
470
00:30:25,287 --> 00:30:29,451
and shoots
clear through the galaxy.
471
00:30:29,525 --> 00:30:35,430
The supermassive black hole
has ignited a quasar.
472
00:30:35,497 --> 00:30:37,192
Quasars are literally
473
00:30:37,266 --> 00:30:39,359
the brightest objects
in the universe.
474
00:30:39,435 --> 00:30:42,427
They're so intense, they can
outshine an entire galaxy.
475
00:30:42,504 --> 00:30:45,268
This is a real photograph
476
00:30:45,341 --> 00:30:49,141
of a real quasar
in the galaxy M87,
477
00:30:49,211 --> 00:30:52,806
50 million light-years away.
478
00:30:56,285 --> 00:30:59,880
Quasars blast away
huge quantities of gas
479
00:30:59,955 --> 00:31:01,889
from the surrounding galaxy...
480
00:31:04,593 --> 00:31:09,121
...the equivalent
of 10 Earths every minute.
481
00:31:12,568 --> 00:31:14,695
When you heat up a gas,
482
00:31:14,770 --> 00:31:16,863
it tends to expand
and it blows outward.
483
00:31:16,939 --> 00:31:19,567
And it's sort of like a wind,
but on a huge scale.
484
00:31:19,641 --> 00:31:21,609
And you get a black-hole wind,
485
00:31:21,677 --> 00:31:24,202
gas blowing out
from the black hole.
486
00:31:24,279 --> 00:31:28,978
Black holes suck gas in.
Quasars blow it out.
487
00:31:29,051 --> 00:31:33,613
But eventually there's no gas
left to make stars,
488
00:31:33,689 --> 00:31:35,384
and the galaxy stops growing.
489
00:31:35,457 --> 00:31:38,187
So we think
that the eventual size
490
00:31:38,260 --> 00:31:39,750
that a galaxy can achieve
491
00:31:39,828 --> 00:31:42,319
depends on the black hole
in its center.
492
00:31:42,398 --> 00:31:43,922
The two are tied together.
493
00:31:45,901 --> 00:31:50,702
With no gas left to feed
on, the quasar jets shrink and die.
494
00:31:52,174 --> 00:31:55,200
What's left
is a supermassive black hole
495
00:31:55,277 --> 00:31:59,680
at the center of the galaxy,
with a whole lot of young stars,
496
00:31:59,748 --> 00:32:03,684
just like our Milky Way
back when it was young.
497
00:32:03,752 --> 00:32:06,414
Early on
in the history of the Milky Way,
498
00:32:06,488 --> 00:32:09,821
when it was a young galaxy,
we were probably a quasar.
499
00:32:09,892 --> 00:32:13,328
Probably every big galaxy
was a quasar when it was young.
500
00:32:13,395 --> 00:32:14,885
But right now we're old enough
501
00:32:14,963 --> 00:32:16,931
that the galaxy
has quieted down.
502
00:32:18,700 --> 00:32:22,568
Now astronomers
are looking for quasars,
503
00:32:22,638 --> 00:32:25,971
the secret
to finding more black holes
504
00:32:26,041 --> 00:32:28,601
and figuring out how they work.
505
00:32:28,677 --> 00:32:32,044
The Chandra observatory
is a space telescope
506
00:32:32,114 --> 00:32:37,814
that can detect the powerful
x-rays quasars send out.
507
00:32:37,886 --> 00:32:40,719
It's found thousands.
508
00:32:40,789 --> 00:32:43,257
These remarkable images show
509
00:32:43,325 --> 00:32:48,228
quasars of all shapes and sizes
firing out into space.
510
00:32:52,301 --> 00:32:54,428
Each one is a signpost
511
00:32:54,503 --> 00:32:58,530
for a young galaxy with
a new black hole at its center.
512
00:33:02,377 --> 00:33:05,369
These quasars
will eventually calm down
513
00:33:05,447 --> 00:33:10,714
as their galaxy matures
and takes its final shape.
514
00:33:10,786 --> 00:33:12,651
I guess the universe
is a lot like people...
515
00:33:12,721 --> 00:33:14,086
active when they're young,
516
00:33:14,156 --> 00:33:16,488
a little bit quieter and more
relaxed when they get older.
517
00:33:18,694 --> 00:33:21,663
We now know
that supermassive black holes
518
00:33:21,730 --> 00:33:25,723
and the quasars they create
control galaxies.
519
00:33:25,801 --> 00:33:29,760
Black holes are central
to understanding how galaxies form.
520
00:33:29,838 --> 00:33:32,807
They're a key to understanding
how they evolve with time.
521
00:33:32,875 --> 00:33:35,207
So, in fact,
rather than being obscura,
522
00:33:35,277 --> 00:33:37,268
they're fundamental
to our understanding
523
00:33:37,346 --> 00:33:39,075
of our galaxies
and our universe.
524
00:33:39,147 --> 00:33:43,345
The only way to
find out more about black holes
525
00:33:43,418 --> 00:33:45,386
is to get a good look at one.
526
00:33:45,454 --> 00:33:49,185
And since an up-close visit
is, well, not a good idea,
527
00:33:49,258 --> 00:33:52,159
astronomers are trying to devise
a way to take a picture
528
00:33:52,227 --> 00:33:56,027
of the supermassive black hole
at the heart of our own galaxy.
529
00:33:56,098 --> 00:33:57,531
To get it,
530
00:33:57,599 --> 00:34:01,729
they'll need a telescope
as large as Earth itself.
531
00:34:15,817 --> 00:34:17,751
There's
a supermassive black hole
532
00:34:17,819 --> 00:34:21,311
at the center of the Milky Way.
533
00:34:23,659 --> 00:34:26,560
It's hidden
by a dense cluster of stars
534
00:34:26,628 --> 00:34:29,119
circling
the heart of the galaxy.
535
00:34:31,967 --> 00:34:36,404
But soon,
we hope we'll be able to see it.
536
00:34:36,471 --> 00:34:39,838
Seeing is believing.
537
00:34:39,908 --> 00:34:43,071
It would be spectacular
if we can go right up there,
538
00:34:43,145 --> 00:34:45,978
nose-to-nose
with the event horizon
539
00:34:46,048 --> 00:34:49,381
of the black hole at the center
of the Milky Way galaxy.
540
00:34:49,451 --> 00:34:52,682
And that's the Holy Grail.
541
00:34:52,754 --> 00:34:55,985
A supermassive
black hole lies hidden
542
00:34:56,058 --> 00:34:58,083
at the center of most galaxies.
543
00:34:58,160 --> 00:34:59,889
We only know they're there
544
00:34:59,962 --> 00:35:02,863
because the stars around them
are drawn in
545
00:35:02,931 --> 00:35:05,092
at millions of miles per hour.
546
00:35:05,167 --> 00:35:06,794
But there might still be a way
547
00:35:06,868 --> 00:35:10,360
to take a picture of the
very edge of the black hole...
548
00:35:10,439 --> 00:35:12,600
the event horizon.
549
00:35:12,674 --> 00:35:16,405
Shep Doeleman and his team
are trying to capture an image
550
00:35:16,478 --> 00:35:18,469
that shows its outline.
551
00:35:18,547 --> 00:35:20,742
We're essentially looking
for the shadow,
552
00:35:20,816 --> 00:35:22,807
or the silhouette,
of the black hole,
553
00:35:22,884 --> 00:35:26,320
within this cloud of gas
that's swirling around it.
554
00:35:26,388 --> 00:35:30,051
This technique
that we're exploiting
555
00:35:30,125 --> 00:35:33,094
is the best hope I think we have
556
00:35:33,161 --> 00:35:35,891
to actually image
a region of the universe
557
00:35:35,964 --> 00:35:39,297
which has hitherto been
completely invisible to us.
558
00:35:39,368 --> 00:35:41,598
Optical telescopes
559
00:35:41,670 --> 00:35:45,128
can't see the black hole
directly.
560
00:35:45,207 --> 00:35:49,007
But the glowing, super-heated
gas surrounding the black hole
561
00:35:49,077 --> 00:35:52,535
sends out radio waves that can
be used to make an image.
562
00:35:54,616 --> 00:35:59,883
Huge radio telescopes pick up
these signals from space.
563
00:35:59,955 --> 00:36:02,389
The antenna will move
in azimuth and elevation.
564
00:36:09,031 --> 00:36:12,728
This one, at the
M.I.T. Observatory near Boston,
565
00:36:12,801 --> 00:36:15,463
is more than 100 feet wide.
566
00:36:15,537 --> 00:36:19,598
It's big enough to detect
very faint radio emissions
567
00:36:19,675 --> 00:36:24,578
from the black hole in our own
galaxy, 25,000 light-years away.
568
00:36:24,646 --> 00:36:28,878
But it's not nearly big enough
to capture an image.
569
00:36:28,950 --> 00:36:32,408
We need to take multiple copies
of these telescopes,
570
00:36:32,487 --> 00:36:34,284
place them around the world
571
00:36:34,356 --> 00:36:38,884
to create a virtual telescope
as large as the Earth itself.
572
00:36:38,960 --> 00:36:41,861
Doeleman's team
will link up radio telescopes
573
00:36:41,930 --> 00:36:46,094
around the globe,
from Hawaii to Chile to Africa.
574
00:36:52,307 --> 00:36:54,901
When the whole network
is connected,
575
00:36:54,976 --> 00:36:59,072
they'll have a virtual dish
over 10,000 miles across,
576
00:36:59,147 --> 00:37:03,641
with 500 times the power
of a single telescope.
577
00:37:07,089 --> 00:37:09,580
They think
it will be powerful enough
578
00:37:09,658 --> 00:37:12,218
to take a picture
of the event horizon
579
00:37:12,294 --> 00:37:17,732
of the supermassive black hole
at the center of the Milky Way.
580
00:37:17,799 --> 00:37:20,199
They're already picking up
signals
581
00:37:20,268 --> 00:37:22,736
from the dark heart
of our galaxy.
582
00:37:22,804 --> 00:37:25,295
When we saw the first detection,
583
00:37:25,373 --> 00:37:28,035
it was a moment where I just
looked at the computer screen
584
00:37:28,110 --> 00:37:30,806
and said to myself,
"My God, we've done it.
585
00:37:30,879 --> 00:37:33,746
We've actually seen something
that's so small
586
00:37:33,815 --> 00:37:36,306
that it has to be coming from
right around the event horizon."
587
00:37:37,886 --> 00:37:41,344
The signals are still too
weak to give a complete picture,
588
00:37:41,423 --> 00:37:45,052
but Doeleman expects
the images to improve
589
00:37:45,127 --> 00:37:50,030
as more telescopes come online
over the next few years.
590
00:37:50,098 --> 00:37:55,331
Eventually, the outline of the
black hole itself should emerge.
591
00:37:57,973 --> 00:38:03,138
But even a picture can't compare
to witnessing it for yourself.
592
00:38:05,447 --> 00:38:08,780
In the distant future,
we may have the technology
593
00:38:08,850 --> 00:38:13,253
to actually enter
and pass through a black hole
594
00:38:13,321 --> 00:38:16,381
and maybe even
survive the journey.
595
00:38:21,997 --> 00:38:25,296
Then we might finally answer
the question...
596
00:38:25,367 --> 00:38:29,326
what lies
at the heart of a black hole?
597
00:38:31,506 --> 00:38:32,871
Some scientists believe
598
00:38:32,941 --> 00:38:35,637
we could use black holes
as a kind of portal,
599
00:38:35,710 --> 00:38:38,941
with the potential
for travel across the universe.
600
00:38:39,014 --> 00:38:41,744
This is still very speculative,
601
00:38:41,817 --> 00:38:44,251
but the mathematics
seem to indicate
602
00:38:44,319 --> 00:38:46,583
that as you fall
through a black hole
603
00:38:46,655 --> 00:38:48,247
that you don't simply die...
604
00:38:48,323 --> 00:38:50,951
you fall
right through a wormhole,
605
00:38:51,026 --> 00:38:55,656
which is a gateway, a shortcut
through space and time.
606
00:38:55,730 --> 00:38:59,393
Perhaps we could simply
rocket across the universe
607
00:38:59,467 --> 00:39:04,666
through a subway system
that we call a black hole.
608
00:39:04,739 --> 00:39:08,971
If black holes are
shortcuts through space and time,
609
00:39:09,044 --> 00:39:13,003
it could turn one of the coolest
ideas from science fiction
610
00:39:13,081 --> 00:39:16,744
into reality.
611
00:39:16,818 --> 00:39:20,310
Time travel is possible,
but not very practical.
612
00:39:20,388 --> 00:39:23,880
You see, the energy source,
the material that you need
613
00:39:23,959 --> 00:39:26,427
to keep the throat
of a wormhole open
614
00:39:26,494 --> 00:39:27,893
is something so ex otic
615
00:39:27,963 --> 00:39:30,796
that we cannot produce it
in the laboratory.
616
00:39:30,866 --> 00:39:33,767
But if you could,
it might be possible
617
00:39:33,835 --> 00:39:37,965
to exploit the power of
black holes to visit yesterday.
618
00:39:39,608 --> 00:39:42,304
Perhaps our descendants
in the future
619
00:39:42,377 --> 00:39:45,141
have already mastered
this technology.
620
00:39:45,213 --> 00:39:47,340
So one day,
if somebody knocks on your door
621
00:39:47,415 --> 00:39:48,746
and claims to be
622
00:39:48,817 --> 00:39:51,183
your great-great-great-great-
great-great granddaughter,
623
00:39:51,253 --> 00:39:52,242
don't slam the door.
624
00:39:56,291 --> 00:40:00,591
Black holes might even
be gateways to other universes.
625
00:40:00,662 --> 00:40:03,153
On the other side
of a black hole,
626
00:40:03,231 --> 00:40:06,223
there could even be...
a Big Bang.
627
00:40:09,537 --> 00:40:13,132
As a black hole collapses
and matter falls into it,
628
00:40:13,208 --> 00:40:16,609
perhaps the matter is blown out
the other side in a white hole.
629
00:40:16,678 --> 00:40:18,839
Doesn't that sound
like the Big Bang?
630
00:40:24,519 --> 00:40:28,114
If a Big Bang is just
the flip side of a black hole,
631
00:40:28,189 --> 00:40:32,182
this could be
how our own universe was born.
632
00:40:33,995 --> 00:40:36,463
If you look at the equations
for a black hole
633
00:40:36,531 --> 00:40:38,362
and put in the parameters
of the universe...
634
00:40:38,433 --> 00:40:40,594
the mass of the universe,
the size of the universe...
635
00:40:40,669 --> 00:40:41,658
bingo!
636
00:40:41,736 --> 00:40:43,101
You find that our universe
637
00:40:43,171 --> 00:40:45,731
actually solves the equations
for a black hole.
638
00:40:45,807 --> 00:40:48,970
In other words, we could be
inside an event horizon.
639
00:40:49,044 --> 00:40:54,482
Perhaps we are actually living
inside a black hole.
640
00:40:54,549 --> 00:40:57,950
Every black hole
might be the origin
641
00:40:58,019 --> 00:41:00,817
of an entirely separate
universe.
642
00:41:00,889 --> 00:41:02,186
If that's true,
643
00:41:02,257 --> 00:41:06,853
there could be billions
of universes out there...
644
00:41:10,332 --> 00:41:15,531
...each one
full of stars, planets, life.
645
00:41:15,603 --> 00:41:18,071
Whatever we figure out later,
646
00:41:18,139 --> 00:41:22,041
we know now
that black holes are everywhere.
647
00:41:22,110 --> 00:41:23,270
They're bigger in size
648
00:41:23,345 --> 00:41:26,007
and more critical
to the evolution of the universe
649
00:41:26,081 --> 00:41:28,208
than we ever imagined.
650
00:41:39,594 --> 00:41:41,459
Literally, our understanding
651
00:41:41,529 --> 00:41:43,520
of the universe
that's important around us,
652
00:41:43,598 --> 00:41:45,930
the universe
that's visible to telescopes,
653
00:41:46,001 --> 00:41:47,798
has been profoundly affected
654
00:41:47,869 --> 00:41:51,236
by our realization
that black holes are everywhere.
655
00:41:54,209 --> 00:41:55,403
Once upon a time,
656
00:41:55,477 --> 00:41:57,069
people thought
that black-hole physics
657
00:41:57,145 --> 00:42:00,239
was too fantastic to be true.
658
00:42:00,315 --> 00:42:02,875
And now they are center-stage.
659
00:42:02,951 --> 00:42:04,350
We now know they dominate
660
00:42:04,419 --> 00:42:06,614
the evolution
of the universe itself.
661
00:42:08,590 --> 00:42:09,887
When I was a kid,
662
00:42:09,958 --> 00:42:12,188
black holes basically played
a part in science fiction.
663
00:42:12,260 --> 00:42:13,727
It was always
something to avoid.
664
00:42:13,795 --> 00:42:14,955
Your spaceship...
665
00:42:15,030 --> 00:42:16,930
you try to get around them
before you get drawn in.
666
00:42:16,998 --> 00:42:18,989
But what we've learned
since then
667
00:42:19,067 --> 00:42:21,228
is that black holes
play a huge role
668
00:42:21,302 --> 00:42:23,793
and a huge number of roles
in the universe.
669
00:42:26,741 --> 00:42:29,005
It's not an exaggeration to say
670
00:42:29,077 --> 00:42:32,774
that if black holes did not
exist, we wouldn't be here.
671
00:42:32,847 --> 00:42:35,577
We literally owe
our existence to black holes.
672
00:42:39,754 --> 00:42:43,121
The story's not over yet.
673
00:42:43,191 --> 00:42:45,751
There's still
much more to be discovered
674
00:42:45,827 --> 00:42:50,696
about the mysterious objects
called black holes...
675
00:42:50,765 --> 00:42:53,962
The masters of the universe.
676
00:42:54,012 --> 00:42:58,562
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