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Nothing can escape.
2
00:01:16,239 --> 00:01:20,843
They can suck in whole galaxies.
3
00:01:20,844 --> 00:01:24,113
Black holes
used to be science fiction.
4
00:01:24,114 --> 00:01:26,549
Now we know they're real.
5
00:01:26,550 --> 00:01:28,117
When I was a PhD student,
6
00:01:28,118 --> 00:01:31,554
People used to giggle when
you'd hear about black holes.
7
00:01:31,555 --> 00:01:34,223
They're like unicorns,
mythical creatures.
8
00:01:34,224 --> 00:01:35,991
We called this
the "giggle factor."
9
00:01:35,992 --> 00:01:37,927
People would say,
"beam me up, Scotty."
10
00:01:37,928 --> 00:01:40,796
Well,
no one is laughing anymore.
11
00:01:42,032 --> 00:01:44,433
Krauss:
So, they're not science fiction.
12
00:01:44,434 --> 00:01:46,569
Even though
we've never landed in one,
13
00:01:46,570 --> 00:01:48,938
We have enough evidence to know
that they're really out there.
14
00:01:54,778 --> 00:01:58,047
Narrator: This image might not
look like much to you and me,
15
00:01:58,048 --> 00:02:02,785
But to a scientist, it's proof
that black holes exist.
16
00:02:02,786 --> 00:02:07,356
It's an actual movie
of a black hole devouring a star
17
00:02:07,357 --> 00:02:09,992
In the constellation of Aquila.
18
00:02:09,993 --> 00:02:12,161
Black holes are messy eaters.
19
00:02:12,162 --> 00:02:14,296
The red spots you see are gas
20
00:02:14,297 --> 00:02:18,801
That's being spit
out of the hole, into space.
21
00:02:18,802 --> 00:02:21,904
Eventually,
over the next million years,
22
00:02:21,905 --> 00:02:26,775
This star will be eaten alive
and disappear.
23
00:02:34,851 --> 00:02:37,253
A black hole is pretty much
the end point of everything.
24
00:02:37,254 --> 00:02:39,755
It's the end point of a star.
It's the end point of matter.
25
00:02:39,756 --> 00:02:42,324
It's the end point of energy.
It's the end point of gravity.
26
00:02:42,325 --> 00:02:46,996
I mean, that's really it.
That's the top of the scale.
27
00:02:51,468 --> 00:02:53,903
Narrator: Although
they have the power to destroy
28
00:02:53,904 --> 00:02:55,704
Like nothing else
in the universe,
29
00:02:55,705 --> 00:02:59,742
Black holes also help build
galaxies --
30
00:02:59,743 --> 00:03:03,746
A vital part
of the great cosmic machine.
31
00:03:03,747 --> 00:03:05,648
Some astronomers think
32
00:03:05,649 --> 00:03:09,585
They could even be gateways
to parallel universes.
33
00:03:14,724 --> 00:03:17,793
Dr. Kaku: We are now entering
the golden age of research
34
00:03:17,794 --> 00:03:19,061
In black-hole physics.
35
00:03:19,062 --> 00:03:21,730
They could be the key
36
00:03:21,731 --> 00:03:24,533
To understanding
the birth of the universe,
37
00:03:24,534 --> 00:03:26,869
Its formation,
and then its death.
38
00:03:31,741 --> 00:03:33,776
Dr. Krauss:
Black holes really represent,
39
00:03:33,777 --> 00:03:36,045
In one sense, the frontier
of modern astronomy.
40
00:03:36,046 --> 00:03:38,781
And they're changing our ideas
about how galaxies form
41
00:03:38,782 --> 00:03:40,716
And, indeed,
how the universe works.
42
00:03:40,717 --> 00:03:43,585
Narrator:
Their power comes
43
00:03:43,586 --> 00:03:47,389
From one of the primary forces
in nature -- gravity.
44
00:03:50,126 --> 00:03:52,294
Dr. Kaku:
I teach astronomy.
45
00:03:52,295 --> 00:03:53,862
And we teach our students
46
00:03:53,863 --> 00:03:57,599
That the fundamental principle
of gravity is, "gravity sucks."
47
00:03:57,600 --> 00:04:01,170
Narrator: Gravity keeps our feet
on the ground
48
00:04:01,171 --> 00:04:04,273
And our planet
orbiting around the sun.
49
00:04:06,609 --> 00:04:12,181
But in a black hole, the force
of gravity is off the charts --
50
00:04:12,182 --> 00:04:15,918
So strong,
it sucks in anything nearby.
51
00:04:15,919 --> 00:04:21,457
It can even bend
the light from distant stars.
52
00:04:21,458 --> 00:04:24,460
And if that light
gets too close,
53
00:04:24,461 --> 00:04:26,729
The black hole swallows it.
54
00:04:26,730 --> 00:04:28,464
Think of it like this.
55
00:04:28,465 --> 00:04:31,333
Imagine a black hole
as a waterfall.
56
00:04:31,334 --> 00:04:34,636
Gravity is the river
flowing toward the falls,
57
00:04:34,637 --> 00:04:37,039
And a beam of light --
the kayak.
58
00:04:37,040 --> 00:04:40,275
Upriver from the waterfall,
the current is weak.
59
00:04:40,276 --> 00:04:43,846
The kayaker can paddle
against it and get away.
60
00:04:43,847 --> 00:04:47,349
But closer to the waterfall,
the current is stronger,
61
00:04:47,350 --> 00:04:52,321
And the kayaker struggles
to escape.
62
00:04:52,322 --> 00:04:58,260
The edge of the waterfall is
like the edge of a black hole.
63
00:04:58,261 --> 00:05:03,165
No matter how strong
the kayaker is, he's going down.
64
00:05:03,166 --> 00:05:04,900
It's the same in space.
65
00:05:04,901 --> 00:05:08,070
The way black holes
are really devastating
66
00:05:08,071 --> 00:05:10,406
Is because
when you get close to them,
67
00:05:10,407 --> 00:05:12,141
The gravity gets super-strong.
68
00:05:17,247 --> 00:05:20,249
Narrator:
So strong that they eat light.
69
00:05:20,250 --> 00:05:23,685
That's why black holes
are black.
70
00:05:28,391 --> 00:05:30,959
A black hole
is like a roach motel.
71
00:05:30,960 --> 00:05:33,896
Everything checks in.
Nothing checks out.
72
00:05:38,101 --> 00:05:41,203
Narrator: Anything
that gets too close is doomed --
73
00:05:41,204 --> 00:05:46,909
Planets, stars,
even whole solar systems.
74
00:05:53,683 --> 00:05:57,186
And don't think
this is some faraway phenomenon.
75
00:05:57,187 --> 00:05:59,521
Black holes are on the loose
76
00:05:59,522 --> 00:06:03,158
Right here
in our own cosmic neighborhood.
77
00:06:03,159 --> 00:06:05,627
We now know
there are wandering nomads
78
00:06:05,628 --> 00:06:07,863
Throughout
the milky way galaxy --
79
00:06:07,864 --> 00:06:10,966
Vagabonds throughout the galaxy,
80
00:06:10,967 --> 00:06:14,169
Where black holes can come up
right behind you
81
00:06:14,170 --> 00:06:16,939
And perhaps gobble you up,
and they won't even burp.
82
00:06:16,940 --> 00:06:20,576
If one ever comes close,
watch out.
83
00:06:20,577 --> 00:06:25,080
Narrator: If a black hole found
its way into our solar system,
84
00:06:25,081 --> 00:06:26,815
It would rip us apart.
85
00:06:26,816 --> 00:06:28,784
Dr. Plait:
Any kind of black hole
86
00:06:28,785 --> 00:06:31,053
That could pass
through the solar system
87
00:06:31,054 --> 00:06:32,788
Would be pulling
on all the planets
88
00:06:32,789 --> 00:06:34,189
Harder than the sun does.
89
00:06:34,190 --> 00:06:35,858
And so it's just
gonna totally disrupt
90
00:06:35,859 --> 00:06:38,026
The gravitational balance
of the solar system.
91
00:06:38,027 --> 00:06:43,499
Narrator: The black hole would literally
tear planets from their orbits
92
00:06:43,500 --> 00:06:45,701
And smash them into each other.
93
00:06:52,942 --> 00:06:56,945
It's just an epic disaster.
It's a bull in a china shop.
94
00:07:00,016 --> 00:07:03,418
If it got close enough
to, say, Jupiter,
95
00:07:03,419 --> 00:07:05,954
It could actually pull
the moons of Jupiter
96
00:07:05,955 --> 00:07:08,157
Away from the planet itself.
97
00:07:10,260 --> 00:07:12,594
It would just be flinging
planets left and right
98
00:07:12,595 --> 00:07:14,930
Everywhere as it whipped
through the solar system,
99
00:07:14,931 --> 00:07:17,332
Leaving disaster in its wake.
100
00:07:22,071 --> 00:07:25,107
Narrator: If a black hole
approached earth,
101
00:07:25,108 --> 00:07:28,810
All that gravity would rip
asteroids from their orbits
102
00:07:28,811 --> 00:07:30,979
And hurl them toward our planet.
103
00:07:39,622 --> 00:07:42,591
The earth's surface
would become an inferno.
104
00:07:42,592 --> 00:07:46,361
It would be
the beginning of the end.
105
00:07:50,967 --> 00:07:53,635
First, it would swallow up
the atmosphere,
106
00:07:53,636 --> 00:07:56,205
Then the planet itself.
107
00:08:01,511 --> 00:08:03,946
Destroying
an entire solar system
108
00:08:03,947 --> 00:08:06,381
Is nothing to a black hole.
109
00:08:06,382 --> 00:08:11,353
But it's more than just a big,
empty, sucking piece of space.
110
00:08:11,354 --> 00:08:14,156
It's incredibly heavy.
111
00:08:14,157 --> 00:08:18,627
To get an idea just how heavy
and Dee a black hole is,
112
00:08:18,628 --> 00:08:20,329
Imagine the earth.
113
00:08:20,330 --> 00:08:23,665
Now start to crush it...
114
00:08:26,269 --> 00:08:29,705
...And keep crushing
until it's packed so tight
115
00:08:29,706 --> 00:08:32,874
Even the atoms themselves
collapse.
116
00:08:35,712 --> 00:08:40,015
When the earth crushes down
to just 2 inches across,
117
00:08:40,016 --> 00:08:42,985
That's the density
of a black hole.
118
00:08:42,986 --> 00:08:45,754
It would be
the size of a golf ball,
119
00:08:45,755 --> 00:08:51,627
Yet weigh the same as e earth,
with the same amount of gravity.
120
00:08:51,628 --> 00:08:55,230
What can make
something that small,
121
00:08:55,231 --> 00:08:59,101
That dense, and that powerful?
122
00:08:59,102 --> 00:09:03,305
We don't have external forces,
large pistons in the universe,
123
00:09:03,306 --> 00:09:04,906
To create black holes.
124
00:09:04,907 --> 00:09:07,676
So the only way the real
black holes of the universe form
125
00:09:07,677 --> 00:09:09,544
Is if gravity
can do the job itself.
126
00:09:09,545 --> 00:09:13,415
Narrator: There is only
one place in the universe
127
00:09:13,416 --> 00:09:16,218
That generates
that much gravity.
128
00:09:16,219 --> 00:09:19,087
And it's
inside the largest stars.
129
00:09:19,088 --> 00:09:24,426
When massive stars 10 times
heavier than our sun die,
130
00:09:24,427 --> 00:09:26,295
Gravity crushes them,
131
00:09:26,296 --> 00:09:29,898
Creating a huge explosion,
a supernova.
132
00:09:40,109 --> 00:09:45,514
But some stars
are even bigger than that.
133
00:09:45,515 --> 00:09:50,552
These supermassive stars weigh
100 times more than our sun
134
00:09:50,553 --> 00:09:53,422
And have 100 times more gravity.
135
00:09:53,423 --> 00:09:55,824
When one of these stars dies,
136
00:09:55,825 --> 00:10:01,563
It sets off the biggest
explosion in the universe...
137
00:10:01,564 --> 00:10:03,565
A hypernova.
138
00:10:13,576 --> 00:10:17,946
This is the birth
of a black hole.
139
00:10:28,946 --> 00:10:33,483
Narrator:
Our universe is full of stars.
140
00:10:33,484 --> 00:10:37,854
At the end of their lives,
some die quietly.
141
00:10:37,855 --> 00:10:42,159
Others go out
in spectacular explosions.
142
00:10:42,160 --> 00:10:47,631
And some give birth
to black holes.
143
00:10:47,632 --> 00:10:49,566
Dr. Plait:
If you have a star,
144
00:10:49,567 --> 00:10:52,869
A supermassive star that's
100 times the mass of the sun,
145
00:10:52,870 --> 00:10:55,839
At the end of its life,
the core runs out of fuel.
146
00:10:55,840 --> 00:10:57,741
There's nothing left
to hold it up,
147
00:10:57,742 --> 00:11:00,110
And the core collapses
down into a black hole.
148
00:11:00,111 --> 00:11:03,847
Narrator: When that happens,
the enormous gravity
149
00:11:03,848 --> 00:11:08,919
Generated at the heart
of supermassive stars runs wild.
150
00:11:11,723 --> 00:11:16,593
This is the dying star
v.Y. Canis majoris.
151
00:11:16,594 --> 00:11:21,198
It's more than
a billion miles across.
152
00:11:24,369 --> 00:11:28,805
Like all stars, it's a giant
nuclear-fusion reactor,
153
00:11:28,806 --> 00:11:31,208
Pumping energy outward.
154
00:11:31,209 --> 00:11:36,713
At the same time, the star's
extreme gravity crushes inward.
155
00:11:36,714 --> 00:11:38,749
For a few million years,
156
00:11:38,750 --> 00:11:42,853
Fusion and gravity
are locked in standoff.
157
00:11:42,854 --> 00:11:45,922
But when the star
runs out of fuel,
158
00:11:45,923 --> 00:11:49,826
Fusion stops
and the stalemate ends.
159
00:11:49,827 --> 00:11:51,628
Gravity wins.
160
00:11:54,031 --> 00:11:56,099
In a millisecond,
161
00:11:56,100 --> 00:11:59,436
The core shrinks to a fraction
of its original size
162
00:11:59,437 --> 00:12:03,573
And a baby black hole is born.
163
00:12:03,574 --> 00:12:05,175
Immediately,
164
00:12:05,176 --> 00:12:09,012
It starts to cannibalize
what's left of the star.
165
00:12:09,013 --> 00:12:12,449
As matter swirls into the black
hole, it gets incredibly hot.
166
00:12:12,450 --> 00:12:14,985
And there are magnetic forces
and frictional forces,
167
00:12:14,986 --> 00:12:17,087
And it's just a witch's brew,
a nightmare,
168
00:12:17,088 --> 00:12:19,856
What's going on right above
the surface of the black hole.
169
00:12:19,857 --> 00:12:22,526
Narrator:
The new black hole in the middle
170
00:12:22,527 --> 00:12:25,495
Keeps feeding on the body
of the star around it.
171
00:12:25,496 --> 00:12:30,267
It eats the gas so fast,
it chokes and coughs,
172
00:12:30,268 --> 00:12:33,503
Blasting out
huge beams of energy.
173
00:12:37,608 --> 00:12:40,610
Dr. Plait: They basically
eat their way out from the star.
174
00:12:40,611 --> 00:12:42,446
This happens in milliseconds.
175
00:12:42,447 --> 00:12:45,282
It happens before
the rest of the star even knows
176
00:12:45,283 --> 00:12:46,783
The core is gone.
177
00:12:46,784 --> 00:12:51,288
And so basically, the star is
dead before it hits the ground.
178
00:12:54,892 --> 00:12:58,762
Narrator:
Finally, the star explodes.
179
00:13:01,432 --> 00:13:06,703
In one second, it blasts out
100 times more energy
180
00:13:06,704 --> 00:13:10,974
Than our sun will produce
over its entire life.
181
00:13:13,377 --> 00:13:18,181
What's left is a new black hole
and two jets of energy
182
00:13:18,182 --> 00:13:22,853
Hurtling through the universe
at the speed of light.
183
00:13:22,854 --> 00:13:26,556
These jets are called
"gamma-ray bursts."
184
00:13:31,929 --> 00:13:35,065
Dr. Plait: They're
incredibly energetic events.
185
00:13:35,066 --> 00:13:37,400
In terms
of raw energy and power,
186
00:13:37,401 --> 00:13:40,570
Gamma ray bursts are second
only to the big bang itself.
187
00:13:42,273 --> 00:13:45,275
Narrator: Most of them last
only a few seconds.
188
00:13:45,276 --> 00:13:48,778
And they fry
anything in their way.
189
00:13:52,617 --> 00:13:55,986
They're so intense that
if there was a gamma-ray burster
190
00:13:55,987 --> 00:13:59,022
In the region of our galaxy
near our solar system,
191
00:13:59,023 --> 00:14:02,425
It could literally vaporize
the entire planet.
192
00:14:02,426 --> 00:14:07,531
Narrator: Fortunately, most gamma-ray
bursts occur outside our galaxy.
193
00:14:14,472 --> 00:14:17,440
But they tell us
something important
194
00:14:17,441 --> 00:14:22,479
About black holes
and how our universe works.
195
00:14:22,480 --> 00:14:25,849
What we were seeing every time
a gamma-ray burst went off
196
00:14:25,850 --> 00:14:28,552
Was basically
the birth cry of a black hole.
197
00:14:28,553 --> 00:14:33,757
Narrator: By counting gamma-ray
bursts, astronomers can figure out
198
00:14:33,758 --> 00:14:36,459
How many black holes
are being created.
199
00:14:36,460 --> 00:14:40,730
In 2004, NASA launched
the swift probe
200
00:14:40,731 --> 00:14:43,867
To scan the universe
for gamma-ray bursts.
201
00:14:43,868 --> 00:14:44,868
Man: Five...
202
00:14:44,869 --> 00:14:45,902
Four...
203
00:14:45,903 --> 00:14:46,937
Three...
204
00:14:46,938 --> 00:14:48,071
Two...
205
00:14:48,072 --> 00:14:50,206
One...
We have ignition.
206
00:14:50,207 --> 00:14:53,610
And we have lift-off
of NASA's swift spacecraft,
207
00:14:53,611 --> 00:14:56,913
On a mission to study
and understand gamma-ray bursts
208
00:14:56,914 --> 00:14:58,448
Throughout the universe.
209
00:15:04,789 --> 00:15:07,891
Narrator: This is the most
powerful gamma-ray burst
210
00:15:07,892 --> 00:15:10,060
Swift has detected so far.
211
00:15:10,061 --> 00:15:14,030
The flash of light announces
the birth of a new black hole
212
00:15:14,031 --> 00:15:16,566
On the other side
of the universe.
213
00:15:20,771 --> 00:15:25,609
Swift can only look at
a fraction of what's out there.
214
00:15:29,714 --> 00:15:34,584
Still, it detects at least
one gamma-ray burst every day.
215
00:15:36,487 --> 00:15:41,157
That discovery rocked astronomy
to its foundations.
216
00:15:43,527 --> 00:15:46,363
Dr. Kaku: We once thought
that black holes, like unicorns,
217
00:15:46,364 --> 00:15:48,999
Could never be found.
218
00:15:49,000 --> 00:15:52,402
We now believe that there are
perhaps billions of black holes
219
00:15:52,403 --> 00:15:53,703
In the night sky.
220
00:15:53,704 --> 00:15:56,406
When we look around our galaxy
and other galaxies,
221
00:15:56,407 --> 00:16:01,277
It's clear that the universe
is full of powerful black holes.
222
00:16:01,278 --> 00:16:03,847
Narrator: Finding black holes
is one thing.
223
00:16:03,848 --> 00:16:05,515
Figuring out how they work --
224
00:16:05,516 --> 00:16:07,684
That's a whole different
ball game.
225
00:16:07,685 --> 00:16:10,453
The only way to find out
is to visit one.
226
00:16:10,454 --> 00:16:14,858
You'd have to take a spacecraft
across the vastness of space
227
00:16:14,859 --> 00:16:16,693
Just to get close to it.
228
00:16:16,694 --> 00:16:20,930
Then you'd have to go
inside the black hole.
229
00:16:20,931 --> 00:16:22,832
There, you'd find a place
230
00:16:22,833 --> 00:16:27,070
Where reality breaks down
and time stands still.
231
00:16:34,762 --> 00:16:38,532
Narrator: There are billions
of black holes in the universe.
232
00:16:38,533 --> 00:16:41,902
We can detect them
with telescopes and satellites.
233
00:16:41,903 --> 00:16:46,573
But we don't actually know
what they're like up-close.
234
00:16:46,574 --> 00:16:47,975
It's a long way off,
235
00:16:47,976 --> 00:16:50,611
But scientists
are already speculating
236
00:16:50,612 --> 00:16:53,981
About a mission
to a black hole...
237
00:16:53,982 --> 00:16:58,785
A one-way trip to the most
dangerous place in the universe.
238
00:17:02,457 --> 00:17:04,158
Dr. Kaku:
Originally,
239
00:17:04,159 --> 00:17:08,495
Physicists were horrified
at the idea of black holes.
240
00:17:08,496 --> 00:17:10,130
They wanted to banish them,
241
00:17:10,131 --> 00:17:12,900
Because the laws of physics,
as we know them,
242
00:17:12,901 --> 00:17:15,903
Seem to break down
at the instant of a black hole.
243
00:17:15,904 --> 00:17:17,404
Time stops.
244
00:17:18,806 --> 00:17:21,375
Gravity becomes infinite.
245
00:17:21,376 --> 00:17:24,978
This is a nightmare.
246
00:17:24,979 --> 00:17:28,815
Narrator: Obviously, we can't send
humans anywhere near a black hole.
247
00:17:28,816 --> 00:17:31,552
But a robot?
Well, sure.
248
00:17:31,553 --> 00:17:34,688
A robotic probe
could transmit data back
249
00:17:34,689 --> 00:17:37,424
Just before
it goes over the edge.
250
00:17:37,425 --> 00:17:41,929
That edge of a black hole
is called the "event horizon."
251
00:17:41,930 --> 00:17:44,631
It's the edge
of time and space --
252
00:17:44,632 --> 00:17:47,768
At least,
in the universe we know.
253
00:17:47,769 --> 00:17:49,870
We call the event horizon
"event horizon"
254
00:17:49,871 --> 00:17:51,238
Quite simply because
255
00:17:51,239 --> 00:17:52,806
It separates space
into two regions.
256
00:17:55,043 --> 00:17:56,877
It's not a physical surface.
257
00:17:56,878 --> 00:18:00,814
You might not even notice it
if you were falling through it,
258
00:18:00,815 --> 00:18:03,417
But ultimately, once you're
inside of it, you're doomed.
259
00:18:03,418 --> 00:18:06,286
Narrator: As you approach
the event horizon,
260
00:18:06,287 --> 00:18:08,055
Gravity gets stronger
261
00:18:08,056 --> 00:18:12,159
And very strange things
start to happen.
262
00:18:12,160 --> 00:18:14,828
Dr. Plait: As you fall
into a black hole feet-first,
263
00:18:14,829 --> 00:18:16,930
Your feet are closer
to the black hole.
264
00:18:16,931 --> 00:18:21,001
And so the gravity they feel
is stronger.
265
00:18:21,002 --> 00:18:22,536
Your head is not quite as close,
266
00:18:22,537 --> 00:18:24,371
And so the gravity it feels
is less.
267
00:18:24,372 --> 00:18:27,908
And basically, what happens is,
you get stretched out.
268
00:18:27,909 --> 00:18:30,143
Your feet are being pulled
much harder than your head,
269
00:18:30,144 --> 00:18:31,478
And you're like a piece of taffy
270
00:18:31,479 --> 00:18:33,180
Being pulled
between two strong people.
271
00:18:36,317 --> 00:18:38,452
As you get thinner
and thinner and thinner,
272
00:18:38,453 --> 00:18:40,487
As you get closer
and closer and closer,
273
00:18:40,488 --> 00:18:44,057
You're undergoing a process
we call "spaghettification"
274
00:18:44,058 --> 00:18:48,095
Because you're basically turned
into a long, thin tube of pasta.
275
00:18:51,966 --> 00:18:55,502
Narrator: Gravity would stretch
our robotic probe to the limit,
276
00:18:55,503 --> 00:18:57,271
Then rip it apart.
277
00:19:04,779 --> 00:19:07,648
But imagine
if the probe was strong enough
278
00:19:07,649 --> 00:19:10,484
To survive and keep going.
279
00:19:12,854 --> 00:19:18,825
As it gets close to the event
horizon, everything goes crazy.
280
00:19:18,826 --> 00:19:23,830
Gravity is so extreme,
it stops time.
281
00:19:23,831 --> 00:19:26,199
Dr. Kaku: We think of time
as being endless.
282
00:19:26,200 --> 00:19:29,403
However, in a black hole,
in some sense, time stops.
283
00:19:33,274 --> 00:19:37,544
Dr. Plait: This sounds like it's
nuts, but that's the way it works.
284
00:19:37,545 --> 00:19:38,979
It's in the math.
285
00:19:38,980 --> 00:19:42,449
It's actually woven into the
fabric of the universe itself.
286
00:19:42,450 --> 00:19:45,218
Narrator: If you were to watch
from a distance,
287
00:19:45,219 --> 00:19:47,587
The robot probe
would seem to slow down
288
00:19:47,588 --> 00:19:50,624
As it gets closer
to the black hole.
289
00:19:50,625 --> 00:19:53,927
Then it would appear to stop
completely.
290
00:19:53,928 --> 00:19:57,064
The whole process
might just take a brief moment.
291
00:19:57,065 --> 00:19:58,465
But from the outside,
292
00:19:58,466 --> 00:20:02,669
You appear to freeze
and fall ever more slowly.
293
00:20:02,670 --> 00:20:05,372
You actually can never observe
an object fall
294
00:20:05,373 --> 00:20:07,741
All the way
through the event horizon.
295
00:20:07,742 --> 00:20:10,077
It literally freezes
at the surface
296
00:20:10,078 --> 00:20:13,347
Because its clock
is going infinitely slowly
297
00:20:13,348 --> 00:20:14,748
Compared to yours.
298
00:20:14,749 --> 00:20:19,753
Narrator: In reality,
the probe hasn't stopped at all.
299
00:20:19,754 --> 00:20:24,024
It keeps going
and crosses the event horizon.
300
00:20:25,860 --> 00:20:28,829
If the probe
points its cameras backwards,
301
00:20:28,830 --> 00:20:31,298
Towards the entrance
of the black hole,
302
00:20:31,299 --> 00:20:36,970
It will see light
being sucked in.
303
00:20:36,971 --> 00:20:42,042
If it points the camera forward,
at first it sees only black,
304
00:20:42,043 --> 00:20:45,445
But as it moves toward the heart
of the black hole,
305
00:20:45,446 --> 00:20:50,283
It encounters the most bizarre
place in the universe.
306
00:20:51,853 --> 00:20:55,856
The black hole's immense gravity
pulls everything down
307
00:20:55,857 --> 00:20:59,259
To an unimaginably small point
at its center.
308
00:20:59,260 --> 00:21:03,864
Scientists call it
the "singularity."
309
00:21:03,865 --> 00:21:06,433
We really just don't know
310
00:21:06,434 --> 00:21:08,468
What happens
at the center of a black hole.
311
00:21:08,469 --> 00:21:09,936
The densities are so great
312
00:21:09,937 --> 00:21:12,205
That the laws of physics
break down, as we know them.
313
00:21:12,206 --> 00:21:17,043
A singularity is a point
of infinite gravity,
314
00:21:17,044 --> 00:21:20,213
Where space and time
become meaningless.
315
00:21:20,214 --> 00:21:22,082
Now, that is ridiculous.
316
00:21:22,083 --> 00:21:26,720
A singularity is basically a
word for saying "I don't know."
317
00:21:26,721 --> 00:21:29,189
It's a word for saying
"I'm clueless."
318
00:21:32,927 --> 00:21:34,127
Narrator: Even now,
319
00:21:34,128 --> 00:21:36,696
Scientists can't really answer
the question,
320
00:21:36,697 --> 00:21:38,064
"what is a black hole?"
321
00:21:38,065 --> 00:21:39,800
Dr. Plait:
It's upsetting, a little bit,
322
00:21:39,801 --> 00:21:41,568
To think that there are objects
out there
323
00:21:41,569 --> 00:21:44,171
That are breaking
the laws of physics.
324
00:21:44,172 --> 00:21:46,072
There must be bigger laws
325
00:21:46,073 --> 00:21:48,108
That are being used
by these black holes,
326
00:21:48,109 --> 00:21:50,243
That are being obeyed
by these black holes,
327
00:21:50,244 --> 00:21:51,978
That we just
don't understand yet.
328
00:21:54,982 --> 00:21:58,151
Narrator: Okay, so,
the one thing we do understand
329
00:21:58,152 --> 00:22:01,655
Is that black holes are born
from dying stars.
330
00:22:04,358 --> 00:22:07,894
And most are small --
around 20 miles across.
331
00:22:11,165 --> 00:22:14,201
But now
scientists have discovered
332
00:22:14,202 --> 00:22:17,504
That some black holes
are much bigger.
333
00:22:17,505 --> 00:22:20,707
They're called
"supermassive black holes."
334
00:22:20,708 --> 00:22:24,511
They're the same size
as our entire solar system.
335
00:22:24,512 --> 00:22:30,684
And one of these monsters lies
at the heart of our own galaxy.
336
00:22:38,827 --> 00:22:43,297
Narrator: Our solar system lies
in the milky way galaxy.
337
00:22:43,298 --> 00:22:47,969
It's made up of billions
of stars, including our sun...
338
00:22:49,972 --> 00:22:53,674
...All revolving
around a mysterious region
339
00:22:53,675 --> 00:22:56,344
Right at the center.
340
00:22:56,345 --> 00:22:59,213
Dr. Kaku:
Children ask the question --
341
00:22:59,214 --> 00:23:00,915
If the moon goes
around the earth,
342
00:23:00,916 --> 00:23:02,283
The earth goes around the sun,
343
00:23:02,284 --> 00:23:03,951
Then what does the sun
go around?
344
00:23:03,952 --> 00:23:06,087
Narrator:
It's a good question.
345
00:23:06,088 --> 00:23:08,456
And astronomers ask
the same thing.
346
00:23:08,457 --> 00:23:10,558
Maybe there was something
going on
347
00:23:10,559 --> 00:23:12,360
At the heart of the milky way --
348
00:23:12,361 --> 00:23:17,799
Perhaps a black hole
at the very center.
349
00:23:17,800 --> 00:23:21,269
But because we can't
actually see a black hole,
350
00:23:21,270 --> 00:23:26,441
The best they could do
was look for telltale signs.
351
00:23:26,442 --> 00:23:28,176
Using infrared telescopes,
352
00:23:28,177 --> 00:23:30,878
They looked
at the middle of the galaxy
353
00:23:30,879 --> 00:23:34,248
And discovered
a densely packed swarm
354
00:23:34,249 --> 00:23:36,150
Of millions of stars.
355
00:23:36,151 --> 00:23:40,087
But they couldn't see
what was at the center.
356
00:23:45,060 --> 00:23:49,630
One team has spent 15 years
looking for clues.
357
00:23:54,236 --> 00:23:57,538
High above the clouds
on Mauna Kea, in Hawaii,
358
00:23:57,539 --> 00:24:00,908
The giant Keck telescope
has the power
359
00:24:00,909 --> 00:24:05,313
To see right through
to the center of the milky way.
360
00:24:12,120 --> 00:24:14,822
The region
which we have to study
361
00:24:14,823 --> 00:24:18,192
To prove that there's a
black hole is incredibly small.
362
00:24:18,193 --> 00:24:19,827
It is absolutely the case
363
00:24:19,828 --> 00:24:22,363
Of looking
for a needle in a haystack,
364
00:24:22,364 --> 00:24:25,166
Except we know
exactly where the needle is.
365
00:24:27,169 --> 00:24:30,104
Narrator: Andrea Ghez
has spent countless nights
366
00:24:30,105 --> 00:24:32,240
Scanning
the center of the galaxy
367
00:24:32,241 --> 00:24:35,376
For signs of a black hole.
368
00:24:35,377 --> 00:24:37,245
To be able
to do this experiment,
369
00:24:37,246 --> 00:24:38,880
One has to be able to see
370
00:24:38,881 --> 00:24:41,516
The stars that are very close
to the center of the galaxy
371
00:24:41,517 --> 00:24:44,352
And to position them
incredibly accurately.
372
00:24:44,353 --> 00:24:46,153
And this would be equivalent
373
00:24:46,154 --> 00:24:49,223
To me in Los Angeles
looking at you in new York
374
00:24:49,224 --> 00:24:53,227
And seeing you be able to move
your finger like this.
375
00:24:56,932 --> 00:24:59,267
[ motors whirring ]
376
00:25:06,942 --> 00:25:08,943
Narrator:
As the Keck kicks into action,
377
00:25:08,944 --> 00:25:13,047
A laser beam detects tiny
disturbances in the atmosphere
378
00:25:13,048 --> 00:25:15,483
That would distort the image.
379
00:25:18,153 --> 00:25:24,091
Motors then adjust the huge
30-foot mirror to compensate.
380
00:25:24,092 --> 00:25:26,327
The image is clear enough
381
00:25:26,328 --> 00:25:30,431
To track the stars
at the heart of our galaxy.
382
00:25:32,701 --> 00:25:37,138
Ghez has taken thousands of
images over the last 15 years.
383
00:25:37,139 --> 00:25:42,677
And what they reveal is amazing.
384
00:25:42,678 --> 00:25:45,379
The stars
at the center of the galaxy
385
00:25:45,380 --> 00:25:48,316
Are moving
at millions of miles an hour.
386
00:25:54,723 --> 00:25:59,160
The center of the galaxy
is a very extreme environment.
387
00:25:59,161 --> 00:26:01,128
The speeds with which stars move
388
00:26:01,129 --> 00:26:04,165
Is much higher than
anywhere else in our galaxy.
389
00:26:04,166 --> 00:26:06,934
And that is absolutely
the signpost of the black hole.
390
00:26:12,274 --> 00:26:18,079
Narrator: They look like tiny planets
racing around an invisible sun.
391
00:26:18,080 --> 00:26:21,616
But they're not planets.
They're stars.
392
00:26:21,617 --> 00:26:23,684
It takes a lot of gravity
393
00:26:23,685 --> 00:26:28,022
To swing huge stars around
in such fast, tight orbits.
394
00:26:28,023 --> 00:26:33,060
There's only one thing in the
universe with that much pull...
395
00:26:33,061 --> 00:26:38,099
A supermassive black hole.
396
00:26:38,100 --> 00:26:40,368
Watching these things
shows the presence
397
00:26:40,369 --> 00:26:43,237
Of a 4-million-times-
the-mass-of-our-sun black hole,
398
00:26:43,238 --> 00:26:45,573
Located right at the heart
of our galaxy.
399
00:26:47,175 --> 00:26:49,377
Narrator:
It is a huge discovery.
400
00:26:49,378 --> 00:26:53,214
Everything in our galaxy,
including our own solar system,
401
00:26:53,215 --> 00:26:57,952
Orbits around
a supermassive black hole.
402
00:26:57,953 --> 00:27:01,055
But the milky way
isn't the only galaxy
403
00:27:01,056 --> 00:27:03,424
With a black hole in the middle.
404
00:27:03,425 --> 00:27:05,660
There are
supermassive black holes
405
00:27:05,661 --> 00:27:09,130
At the heart of most galaxies
in the universe.
406
00:27:09,131 --> 00:27:12,700
The Andromeda galaxy
is our closest neighbor.
407
00:27:12,701 --> 00:27:16,203
It circles around
a supermassive black hole
408
00:27:16,204 --> 00:27:20,808
Weighing 140 million times
more than our sun.
409
00:27:20,809 --> 00:27:24,178
Other galaxies,
like this one, m87,
410
00:27:24,179 --> 00:27:30,117
Have black holes weighing
as much as 20 billion suns.
411
00:27:30,118 --> 00:27:32,753
How do black holes get so big,
412
00:27:32,754 --> 00:27:37,191
And what are they doing
at the center of galaxies?
413
00:27:37,192 --> 00:27:42,663
For answers, we have to go back
nearly 14 billion years
414
00:27:42,664 --> 00:27:46,667
To the beginning
of the universe.
415
00:27:46,668 --> 00:27:48,402
Back then,
416
00:27:48,403 --> 00:27:53,040
The universe was filled with
clouds of gas from the big bang.
417
00:27:53,041 --> 00:27:54,642
In some places,
418
00:27:54,643 --> 00:27:58,546
The gas was thick enough
for millions of stars to form.
419
00:28:03,385 --> 00:28:06,520
Most of these new stars
were supermassive.
420
00:28:06,521 --> 00:28:08,589
They burned hot and fast
421
00:28:08,590 --> 00:28:12,693
And then exploded,
creating lots of black holes.
422
00:28:23,205 --> 00:28:26,040
The early universe
was a wild-and-crazy place
423
00:28:26,041 --> 00:28:29,677
Where huge regions of mass were
collapsing catastrophically,
424
00:28:29,678 --> 00:28:31,011
Producing black holes.
425
00:28:31,012 --> 00:28:33,781
And, in fact, the early universe
might have been
426
00:28:33,782 --> 00:28:36,217
Full of emerging black holes
everywhere.
427
00:28:38,854 --> 00:28:41,622
Narrator: Gravity pulled
many of them together.
428
00:28:41,623 --> 00:28:43,958
All over the early universe,
429
00:28:43,959 --> 00:28:48,229
They merged, creating
larger and larger black holes.
430
00:28:51,166 --> 00:28:54,969
Over hundreds of millions
of years, each black hole grew,
431
00:28:54,970 --> 00:28:59,406
Producing stronger gravity and
pulling in more and more gas.
432
00:28:59,407 --> 00:29:04,078
New stars were born from the
gas, forming primitive galaxies.
433
00:29:06,081 --> 00:29:09,950
But the black hole
kept on sucking in gas,
434
00:29:09,951 --> 00:29:11,819
Until it could take no more,
435
00:29:11,820 --> 00:29:15,990
Igniting the most powerful
flamethrower in the universe.
436
00:29:34,507 --> 00:29:38,343
Narrator: A young galaxy
is a vast cluster of stars,
437
00:29:38,344 --> 00:29:41,446
Stars that formed
from clouds of gas.
438
00:29:46,319 --> 00:29:48,854
At the center of the new galaxy
439
00:29:48,855 --> 00:29:53,325
Is a young, supermassive
black hole feeding on the gas,
440
00:29:53,326 --> 00:29:55,327
Getting bigger and bigger.
441
00:29:55,328 --> 00:29:57,129
Dr. Plait:
If you can imagine,
442
00:29:57,130 --> 00:29:59,665
When a galaxy is very young
and still forming,
443
00:29:59,666 --> 00:30:02,501
There's a supermassive
black hole forming at the core,
444
00:30:02,502 --> 00:30:04,503
And the gas
is still falling into it
445
00:30:04,504 --> 00:30:06,038
And still forming the galaxy.
446
00:30:06,039 --> 00:30:08,340
Well,
near that central black hole,
447
00:30:08,341 --> 00:30:10,042
Things are getting very hot.
448
00:30:10,043 --> 00:30:11,743
That material is heating up.
449
00:30:11,744 --> 00:30:15,380
Narrator: Gas is speeding
into the black hole.
450
00:30:15,381 --> 00:30:17,883
But it overloads,
451
00:30:17,884 --> 00:30:22,621
And there is no room
for all that excess hot gas.
452
00:30:22,622 --> 00:30:26,992
It has nowhere to go but out.
453
00:30:26,993 --> 00:30:32,130
It's blasted into space
in huge jets of energy.
454
00:30:36,669 --> 00:30:40,205
Each jet is 20 times wider
than our solar system
455
00:30:40,206 --> 00:30:44,443
And shoots
clear through the galaxy.
456
00:30:44,444 --> 00:30:50,349
The supermassive black hole
has ignited a quasar.
457
00:30:50,350 --> 00:30:52,117
Quasars are literally
458
00:30:52,118 --> 00:30:54,286
The brightest objects
in the universe.
459
00:30:54,287 --> 00:30:57,222
They're so intense, they can
outshine an entire galaxy.
460
00:30:57,223 --> 00:31:00,058
Narrator:
This is a real photograph
461
00:31:00,059 --> 00:31:03,929
Of a real quasar
in the galaxy m87,
462
00:31:03,930 --> 00:31:07,599
50 million light-years away.
463
00:31:11,003 --> 00:31:14,673
Quasars blast away
huge quantities of gas
464
00:31:14,674 --> 00:31:16,675
From the surrounding galaxy...
465
00:31:19,312 --> 00:31:23,915
...The equivalent
of 10 earths every minute.
466
00:31:27,286 --> 00:31:31,523
Dr. Plait: When you heat up a gas, it
tends to expand and it blows outward.
467
00:31:31,524 --> 00:31:34,359
And it's sort of like a wind,
but on a huge scale.
468
00:31:34,360 --> 00:31:36,395
And you get a black-hole wind,
469
00:31:36,396 --> 00:31:38,997
Gas blowing out
from the black hole.
470
00:31:38,998 --> 00:31:43,635
Narrator: Black holes suck gas in.
Quasars blow it out.
471
00:31:43,636 --> 00:31:48,273
But eventually there's no gas
left to make stars,
472
00:31:48,274 --> 00:31:50,041
And the galaxy stops growing.
473
00:31:50,042 --> 00:31:52,811
Dr. Plait: So we think
that the eventual size
474
00:31:52,812 --> 00:31:54,379
That a galaxy can achieve
475
00:31:54,380 --> 00:31:56,948
Depends on the black hole
in its center.
476
00:31:56,949 --> 00:31:58,550
The two are tied together.
477
00:32:00,453 --> 00:32:05,323
Narrator: With no gas left to feed
on, the quasar jets shrink and die.
478
00:32:06,726 --> 00:32:09,795
What's left
is a supermassive black hole
479
00:32:09,796 --> 00:32:14,266
At the center of the galaxy,
with a whole lot of young stars,
480
00:32:14,267 --> 00:32:18,270
Just like our milky way
back when it was young.
481
00:32:18,271 --> 00:32:21,006
Dr. Plait: Early on
in the history of the milky way,
482
00:32:21,007 --> 00:32:24,409
When it was a young galaxy,
we were probably a quasar.
483
00:32:24,410 --> 00:32:27,913
Probably every big galaxy
was a quasar when it was young.
484
00:32:27,914 --> 00:32:29,481
But right now we're old enough
485
00:32:29,482 --> 00:32:31,383
That the galaxy
has quieted down.
486
00:32:33,219 --> 00:32:37,155
Narrator: Now astronomers
are looking for quasars,
487
00:32:37,156 --> 00:32:40,559
The secret
to finding more black holes
488
00:32:40,560 --> 00:32:43,195
And figuring out how they work.
489
00:32:43,196 --> 00:32:46,264
The Chandra observatory
is a space telescope
490
00:32:46,265 --> 00:32:52,237
That can detect the powerful
x-rays quasars send out.
491
00:32:52,238 --> 00:32:55,140
It's found thousands.
492
00:32:55,141 --> 00:32:57,676
These remarkable images show
493
00:32:57,677 --> 00:33:02,647
Quasars of all shapes and sizes
firing out into space.
494
00:33:06,652 --> 00:33:08,854
Each one is a signpost
495
00:33:08,855 --> 00:33:12,958
For a young galaxy with
a new black hole at its center.
496
00:33:16,729 --> 00:33:19,798
These quasars
will eventually calm down
497
00:33:19,799 --> 00:33:25,136
As their galaxy matures
and takes its final shape.
498
00:33:25,137 --> 00:33:27,072
I guess the universe
is a lot like people --
499
00:33:27,073 --> 00:33:28,807
Active when they're young,
500
00:33:28,808 --> 00:33:30,675
A little bit quieter and more
relaxed when they get older.
501
00:33:33,045 --> 00:33:36,081
Narrator: We now know
that supermassive black holes
502
00:33:36,082 --> 00:33:40,151
And the quasars they create
control galaxies.
503
00:33:40,152 --> 00:33:44,189
Dr. Ghez: Black holes are central
to understanding how galaxies form.
504
00:33:44,190 --> 00:33:47,225
They're a key to understanding
how they evolve with time.
505
00:33:47,226 --> 00:33:49,394
So, in fact,
rather than being obscura,
506
00:33:49,395 --> 00:33:51,463
They're fundamental
to our understanding
507
00:33:51,464 --> 00:33:53,265
Of our galaxies
and our universe.
508
00:33:53,266 --> 00:33:57,536
Narrator: The only way to
find out more about black holes
509
00:33:57,537 --> 00:33:59,571
Is to get a good look at one.
510
00:33:59,572 --> 00:34:03,375
And since an up-close visit
is, well, not a good idea,
511
00:34:03,376 --> 00:34:06,344
Astronomers are trying to devise
a way to take a picture
512
00:34:06,345 --> 00:34:10,215
Of the supermassive black hole
at the heart of our own galaxy.
513
00:34:10,216 --> 00:34:11,917
To get it,
514
00:34:11,918 --> 00:34:15,887
They'll need a telescope
as large as earth itself.
515
00:34:33,316 --> 00:34:36,552
Narrator: There's
a supermassive black hole
516
00:34:36,553 --> 00:34:40,222
At the center of the milky way.
517
00:34:42,392 --> 00:34:45,361
It's hidden
by a dense cluster of stars
518
00:34:45,362 --> 00:34:47,930
Circling
the heart of the galaxy.
519
00:34:50,700 --> 00:34:55,204
But soon,
we hope we'll be able to see it.
520
00:34:55,205 --> 00:34:58,040
Dr. Kaku:
Seeing is believing.
521
00:34:58,041 --> 00:35:01,877
It would be spectacular
if we can go right up there,
522
00:35:01,878 --> 00:35:04,780
Nose-to-nose
with the event horizon
523
00:35:04,781 --> 00:35:08,250
Of the black hole at the center
of the milky way galaxy.
524
00:35:08,251 --> 00:35:11,553
And that's the holy grail.
525
00:35:11,554 --> 00:35:14,857
Narrator: A supermassive
black hole lies hidden
526
00:35:14,858 --> 00:35:16,959
At the center of most galaxies.
527
00:35:16,960 --> 00:35:18,761
We only know they're there
528
00:35:18,762 --> 00:35:21,730
Because the stars around them
are drawn in
529
00:35:21,731 --> 00:35:23,966
At millions of miles per hour.
530
00:35:23,967 --> 00:35:25,667
But there might still be a way
531
00:35:25,668 --> 00:35:29,238
To take a picture of the
very edge of the black hole --
532
00:35:29,239 --> 00:35:31,407
The event horizon.
533
00:35:31,408 --> 00:35:35,210
Shep Doeleman and his team
are trying to capture an image
534
00:35:35,211 --> 00:35:37,346
That shows its outline.
535
00:35:37,347 --> 00:35:39,615
We're essentially looking
for the shadow,
536
00:35:39,616 --> 00:35:41,650
Or the silhouette,
of the black hole,
537
00:35:41,651 --> 00:35:45,154
Within this cloud of gas
that's swirling around it.
538
00:35:45,155 --> 00:35:48,891
This technique
that we're exploiting
539
00:35:48,892 --> 00:35:51,960
Is the best hope I think we have
540
00:35:51,961 --> 00:35:54,763
To actually image
a region of the universe
541
00:35:54,764 --> 00:35:58,067
Which has hitherto been
completely invisible to us.
542
00:35:58,068 --> 00:36:00,369
Narrator:
Optical telescopes
543
00:36:00,370 --> 00:36:03,906
Can't see the black hole
directly.
544
00:36:03,907 --> 00:36:07,776
But the glowing, super-heated
gas surrounding the black hole
545
00:36:07,777 --> 00:36:11,447
Sends out radio waves that can
be used to make an image.
546
00:36:13,416 --> 00:36:18,687
Huge radio telescopes pick up
these signals from space.
547
00:36:18,688 --> 00:36:21,290
The antenna will move
in azimuth and elevation.
548
00:36:21,291 --> 00:36:23,625
[ beeping ]
549
00:36:23,626 --> 00:36:26,161
[ whirring ]
550
00:36:27,864 --> 00:36:31,633
Narrator: This one, at the
m.I.T. Observatory near Boston,
551
00:36:31,634 --> 00:36:34,369
Is more than 100 feet wide.
552
00:36:34,370 --> 00:36:38,474
It's big enough to detect
very faint radio emissions
553
00:36:38,475 --> 00:36:43,445
From the black hole in our own
galaxy, 25,000 light-years away.
554
00:36:43,446 --> 00:36:47,716
But it's not nearly big enough
to capture an image.
555
00:36:47,717 --> 00:36:51,253
We need to take multiple copies
of these telescopes,
556
00:36:51,254 --> 00:36:53,122
Place them around the world
557
00:36:53,123 --> 00:36:57,726
To create a virtual telescope
as large as the earth itself.
558
00:36:57,727 --> 00:37:00,696
Narrator: Doeleman's team
will link up radio telescopes
559
00:37:00,697 --> 00:37:04,933
Around the globe,
from Hawaii to Chile to Africa.
560
00:37:11,107 --> 00:37:13,775
When the whole network
is connected,
561
00:37:13,776 --> 00:37:17,946
They'll have a virtual dish
over 10,000 miles across,
562
00:37:17,947 --> 00:37:22,518
With 500 times the power
of a single telescope.
563
00:37:25,889 --> 00:37:28,457
They think
it will be powerful enough
564
00:37:28,458 --> 00:37:31,093
To take a picture
of the event horizon
565
00:37:31,094 --> 00:37:36,598
Of the supermassive black hole
at the center of the milky way.
566
00:37:36,599 --> 00:37:39,067
They're already picking up
signals
567
00:37:39,068 --> 00:37:41,570
From the dark heart
of our galaxy.
568
00:37:41,571 --> 00:37:44,206
Dr. Doeleman:
When we saw the first detection,
569
00:37:44,207 --> 00:37:46,942
It was a moment where I just
looked at the computer screen
570
00:37:46,943 --> 00:37:49,711
And said to myself,
"my god, we've done it.
571
00:37:49,712 --> 00:37:52,648
"we've actually seen something
that's so small
572
00:37:52,649 --> 00:37:56,718
That it has to be coming from
right around the event horizon."
573
00:37:56,719 --> 00:38:00,255
Narrator: The signals are still too
weak to give a complete picture,
574
00:38:00,256 --> 00:38:03,892
But doeleman expects the images
to improve
575
00:38:03,893 --> 00:38:08,864
As more telescopes come online
over the next few years.
576
00:38:08,865 --> 00:38:14,169
Eventually, the outline of the
black hole itself should emerge.
577
00:38:16,739 --> 00:38:21,977
But even a picture can't compare
to witnessing it for yourself.
578
00:38:24,214 --> 00:38:27,616
In the distant future,
we may have the technology
579
00:38:27,617 --> 00:38:32,087
To actually enter
and pass through a black hole
580
00:38:32,088 --> 00:38:35,224
And maybe even
survive the journey.
581
00:38:40,763 --> 00:38:44,132
Then we might finally answer
the question --
582
00:38:44,133 --> 00:38:48,170
What lies
at the heart of a black hole?
583
00:38:50,273 --> 00:38:51,707
Some scientists believe
584
00:38:51,708 --> 00:38:54,476
We could use black holes
as a kind of portal,
585
00:38:54,477 --> 00:38:57,779
With the potential
for travel across the universe.
586
00:38:57,780 --> 00:39:00,582
Dr. Kaku:
This is still very speculative,
587
00:39:00,583 --> 00:39:03,085
But the mathematics
seem to indicate
588
00:39:03,086 --> 00:39:05,420
That as you fall
through a black hole
589
00:39:05,421 --> 00:39:07,089
That you don't simply die --
590
00:39:07,090 --> 00:39:09,791
You fall
right through a wormhole,
591
00:39:09,792 --> 00:39:14,496
Which is a gateway, a shortcut
through space and time.
592
00:39:14,497 --> 00:39:18,233
Perhaps we could simply
rocket across the universe
593
00:39:18,234 --> 00:39:23,505
Through a subway system
that we call a black hole.
594
00:39:23,506 --> 00:39:27,809
Narrator: If black holes are
shortcuts through space and time,
595
00:39:27,810 --> 00:39:31,913
It could turn one of the coolest
ideas from science fiction
596
00:39:31,914 --> 00:39:35,651
Into reality.
597
00:39:35,652 --> 00:39:39,221
Time travel is possible,
but not very practical.
598
00:39:39,222 --> 00:39:42,791
You see, the energy source,
the material that you need
599
00:39:42,792 --> 00:39:45,327
To keep the throat
of a wormhole open
600
00:39:45,328 --> 00:39:46,795
Is something so exotic
601
00:39:46,796 --> 00:39:49,698
That we cannot produce it
in the laboratory.
602
00:39:49,699 --> 00:39:52,668
But if you could,
it might be possible
603
00:39:52,669 --> 00:39:56,738
To exploit the power of
black holes to visit yesterday.
604
00:39:58,441 --> 00:40:01,209
Perhaps our descendants
in the future
605
00:40:01,210 --> 00:40:04,012
Have already mastered
this technology.
606
00:40:04,013 --> 00:40:06,214
So one day,
if somebody knocks on your door
607
00:40:06,215 --> 00:40:07,816
And claims to be
608
00:40:07,817 --> 00:40:10,052
Your great-great-great-great-
great-great granddaughter,
609
00:40:10,053 --> 00:40:11,119
Don't slam the door.
610
00:40:15,091 --> 00:40:19,461
Narrator: Black holes might even
be gateways to other universes.
611
00:40:19,462 --> 00:40:22,030
On the other side
of a black hole,
612
00:40:22,031 --> 00:40:25,100
There could even be...
A big bang.
613
00:40:28,338 --> 00:40:32,007
As a black hole collapses
and matter falls into it,
614
00:40:32,008 --> 00:40:35,477
Perhaps the matter is blown out
the other side in a white hole.
615
00:40:35,478 --> 00:40:37,713
Doesn't that sound
like the big bang?
616
00:40:43,252 --> 00:40:46,922
Narrator: If a big bang is just
the flip side of a black hole,
617
00:40:46,923 --> 00:40:50,992
This could be
how our own universe was born.
618
00:40:52,729 --> 00:40:55,263
If you look at the equations
for a black hole
619
00:40:55,264 --> 00:40:57,165
And put in the parameters
of the universe --
620
00:40:57,166 --> 00:40:59,401
The mass of the universe,
the size of the universe --
621
00:40:59,402 --> 00:41:00,469
Bingo!
622
00:41:00,470 --> 00:41:01,903
You find that our universe
623
00:41:01,904 --> 00:41:04,539
Actually solves the equations
for a black hole.
624
00:41:04,540 --> 00:41:07,776
In other words, we could be
inside an event horizon.
625
00:41:07,777 --> 00:41:13,281
Perhaps we are actually living
inside a black hole.
626
00:41:13,282 --> 00:41:16,752
Narrator: Every black hole
might be the origin
627
00:41:16,753 --> 00:41:19,621
Of an entirely separate
universe.
628
00:41:19,622 --> 00:41:20,989
If that's true,
629
00:41:20,990 --> 00:41:25,660
There could be billions
of universes out there...
630
00:41:29,065 --> 00:41:34,436
...Each one
full of stars, planets, life.
631
00:41:34,437 --> 00:41:36,972
Whatever we figure out later,
632
00:41:36,973 --> 00:41:40,909
We know now
that black holes are everywhere.
633
00:41:40,910 --> 00:41:42,144
They're bigger in size
634
00:41:42,145 --> 00:41:44,880
And more critical
to the evolution of the universe
635
00:41:44,881 --> 00:41:47,082
Than we ever imagined.
636
00:41:58,394 --> 00:42:00,328
Dr. Krauss:
Literally, our understanding
637
00:42:00,329 --> 00:42:02,397
Of the universe
that's important around us,
638
00:42:02,398 --> 00:42:04,800
The universe
that's visible to telescopes,
639
00:42:04,801 --> 00:42:06,668
Has been profoundly affected
640
00:42:06,669 --> 00:42:10,105
By our realization
that black holes are everywhere.
641
00:42:13,009 --> 00:42:14,276
Dr. Kaku:
Once upon a time,
642
00:42:14,277 --> 00:42:15,944
People thought
that black-hole physics
643
00:42:15,945 --> 00:42:19,080
Was too fantastic to be true.
644
00:42:19,081 --> 00:42:21,650
And now they are center-stage.
645
00:42:21,651 --> 00:42:23,118
We now know they dominate
646
00:42:23,119 --> 00:42:25,387
The evolution
of the universe itself.
647
00:42:27,290 --> 00:42:28,857
Dr. Plait:
When I was a kid,
648
00:42:28,858 --> 00:42:30,959
Black holes basically played
a part in science fiction.
649
00:42:30,960 --> 00:42:32,494
It was always
something to avoid.
650
00:42:32,495 --> 00:42:34,029
Your spaceship --
651
00:42:34,030 --> 00:42:35,764
You try to get around them
before you get drawn in.
652
00:42:35,765 --> 00:42:37,833
But what we've learned
since then
653
00:42:37,834 --> 00:42:40,068
Is that black holes
play a huge role
654
00:42:40,069 --> 00:42:42,637
And a huge number of roles
in the universe.
655
00:42:45,508 --> 00:42:47,843
It's not an exaggeration to say
656
00:42:47,844 --> 00:42:51,613
That if black holes did not
exist, we wouldn't be here.
657
00:42:51,614 --> 00:42:54,416
We literally owe
our existence to black holes.
658
00:42:58,521 --> 00:43:01,957
Narrator:
The story's not over yet.
659
00:43:01,958 --> 00:43:04,593
There's still
much more to be discovered
660
00:43:04,594 --> 00:43:09,531
About the mysterious objects
called black holes...
661
00:43:09,532 --> 00:43:12,801
The masters of the universe.
662
00:43:12,849 --> 00:43:18,849
Sync by kuniva for MY-SUBS.com
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