Would you like to inspect the original subtitles? These are the user uploaded subtitles that are being translated:
1
00:00:02,567 --> 00:00:06,266
You might have seen
a boxing match on TV.
2
00:00:06,367 --> 00:00:08,900
Maybe you've even seen one live.
3
00:00:09,000 --> 00:00:12,867
But you have never seen
a contest like this.
4
00:00:12,967 --> 00:00:18,466
Take your ringside seat to
the fight of the cosmos.
5
00:00:18,567 --> 00:00:20,899
This is gonna be a wonderful
fight to witness.
6
00:00:21,000 --> 00:00:23,343
But you'll want to be a few
7
00:00:23,367 --> 00:00:25,100
million billion
light-years away.
8
00:00:25,166 --> 00:00:28,567
It's like being punched by
the ghost of Muhammad Ali.
9
00:00:28,667 --> 00:00:29,975
You don't even see it coming.
10
00:00:30,000 --> 00:00:30,100
You don't even see it coming.
11
00:00:30,166 --> 00:00:34,366
Our fighters don't float
like a butterfly or sting like
12
00:00:34,466 --> 00:00:39,343
a bee, but they can deliver
the ultimate knockout blow.
13
00:00:39,366 --> 00:00:45,200
It is a soul-chilling,
mind-crushing amount of energy.
14
00:00:45,265 --> 00:00:47,165
It's just unbelievable.
15
00:00:47,265 --> 00:00:50,700
It's a fight between
two supermassive black holes.
16
00:00:50,767 --> 00:00:53,466
Forget about the world
heavyweight championships.
17
00:00:53,567 --> 00:00:56,567
This is the universe's
heavyweight championships.
18
00:00:57,600 --> 00:00:59,767
Get ready for the heavyweight
19
00:00:59,866 --> 00:00:59,976
championship of the universe.
20
00:01:00,000 --> 00:01:01,700
Championship of the universe.
21
00:01:17,966 --> 00:01:21,099
2021, scientists detect
22
00:01:21,165 --> 00:01:24,099
a gigantic rumble deep in space,
23
00:01:24,165 --> 00:01:27,099
a tsunami of
gravitational waves,
24
00:01:27,165 --> 00:01:29,975
giant ripples racing
across the universe.
25
00:01:30,000 --> 00:01:30,667
Giant ripples racing
across the universe.
26
00:01:30,766 --> 00:01:33,799
Gravitational waves
that big have to
27
00:01:33,866 --> 00:01:37,643
come from a giant,
cataclysmic event.
28
00:01:37,667 --> 00:01:41,299
The universe is immense
and full of very
29
00:01:41,366 --> 00:01:44,442
violent events that are
happening every single day.
30
00:01:44,466 --> 00:01:47,700
The universe is a scary place.
31
00:01:47,766 --> 00:01:50,766
There is violence
everywhere we look.
32
00:01:52,000 --> 00:01:55,099
The growls and roars
are clues about
33
00:01:55,165 --> 00:01:58,643
the ultimate cosmic brawl,
34
00:01:58,667 --> 00:01:59,975
the most violent event in
the universe.
35
00:02:00,000 --> 00:02:01,867
The most violent event in
the universe.
36
00:02:04,165 --> 00:02:07,900
But we don't know
where they're coming from.
37
00:02:08,000 --> 00:02:09,599
Imagine a storm is coming
38
00:02:09,667 --> 00:02:10,644
in the middle of the night.
39
00:02:10,668 --> 00:02:12,000
You can't see the storm,
40
00:02:12,066 --> 00:02:15,265
you can't see the lightning,
but you can hear that rumble of
41
00:02:15,366 --> 00:02:19,900
the distant thunder,
and you know that it's coming.
42
00:02:20,000 --> 00:02:23,567
This distant rumble
of gravitational waves
43
00:02:23,667 --> 00:02:26,099
is like the footwork
of heavyweights
44
00:02:26,165 --> 00:02:28,667
pounding the canvas
of the boxing ring.
45
00:02:29,866 --> 00:02:29,977
The waves are caused
by something massive
46
00:02:30,001 --> 00:02:32,643
The waves are caused
by something massive
47
00:02:32,667 --> 00:02:34,265
throwing its weight around.
48
00:02:36,066 --> 00:02:39,766
It's not the first time we've
detected gravitational waves.
49
00:02:43,000 --> 00:02:44,300
Our experiments have picked up
50
00:02:44,366 --> 00:02:47,241
the signal of
two small stellar mass
51
00:02:47,265 --> 00:02:49,366
black holes colliding.
52
00:02:49,466 --> 00:02:54,099
These waves are high-pitched
and ring like a boxing bell.
53
00:02:54,165 --> 00:02:58,343
The deep space growl
is a much lower frequency,
54
00:02:58,366 --> 00:02:59,975
like the roar of a crowd.
55
00:03:00,000 --> 00:03:01,000
Like the roar of a crowd.
56
00:03:02,667 --> 00:03:04,300
The difference in frequencies
57
00:03:04,366 --> 00:03:07,099
would be even more exaggerated
than the difference
58
00:03:07,165 --> 00:03:10,567
between a sparrow chirping
and the sound coming from
59
00:03:10,667 --> 00:03:12,400
a blue whale underwater.
60
00:03:12,467 --> 00:03:16,599
It would be orders of magnitude
more different than that.
61
00:03:18,866 --> 00:03:21,400
The low frequency
of the deep space rumble
62
00:03:21,466 --> 00:03:24,199
tells us that
the waves are colossal.
63
00:03:25,466 --> 00:03:28,366
Imagine throwing
a stone in the water
64
00:03:28,466 --> 00:03:29,975
and watching the little
ripples come out.
65
00:03:30,000 --> 00:03:30,300
And watching the little
ripples come out.
66
00:03:30,366 --> 00:03:33,543
Now imagine throwing
in a boulder a billion times
67
00:03:33,567 --> 00:03:34,667
more massive
68
00:03:34,766 --> 00:03:37,543
and watching the huge waves
that come from that.
69
00:03:37,567 --> 00:03:39,800
Those are the waves
that we're looking at.
70
00:03:41,400 --> 00:03:43,099
These are more
difficult to detect,
71
00:03:43,165 --> 00:03:45,766
because the waves are so big.
72
00:03:45,866 --> 00:03:49,942
One of their wavelengths is
about 15 light-years.
73
00:03:49,966 --> 00:03:51,766
You could wait for 15 years
74
00:03:51,866 --> 00:03:54,766
and only have one wavelength
go by the Earth.
75
00:03:55,966 --> 00:03:58,699
The waves are too big
for an earthbound detector
76
00:03:58,766 --> 00:03:59,975
to pick up.
77
00:04:00,000 --> 00:04:00,300
To pick up.
78
00:04:00,366 --> 00:04:03,800
So, to search for the source
of these giant waves,
79
00:04:03,866 --> 00:04:06,199
Chiara Mingarelli and her team
80
00:04:06,265 --> 00:04:10,300
use a detector already in space,
81
00:04:10,366 --> 00:04:12,042
something large enough
to pick up
82
00:04:12,066 --> 00:04:14,866
these galactic heavyweights,
83
00:04:14,967 --> 00:04:18,800
spinning dead stars
called pulsars.
84
00:04:18,867 --> 00:04:23,367
Our galaxy
is awash with pulsars.
85
00:04:23,466 --> 00:04:26,100
Now, they're called pulsars
because they pulsate
86
00:04:26,165 --> 00:04:29,165
very regularly... they're
like cosmic lighthouses.
87
00:04:29,266 --> 00:04:29,976
The lighthouse beams
are so regular,
88
00:04:30,000 --> 00:04:31,667
The lighthouse beams
are so regular,
89
00:04:31,766 --> 00:04:33,300
you can set your watch by them.
90
00:04:34,667 --> 00:04:38,266
But when a huge gravitational
wave hits them,
91
00:04:38,367 --> 00:04:41,165
the timing gets knocked out
of whack.
92
00:04:41,266 --> 00:04:44,867
That pulsar is going to
basically rock back and forth
93
00:04:44,966 --> 00:04:46,843
and that's going
to change the timing
94
00:04:46,867 --> 00:04:50,165
of the pulses that
we measure from that object.
95
00:04:50,266 --> 00:04:53,843
To identify the source
of the gravitational waves,
96
00:04:53,867 --> 00:04:58,843
Chiara and her team measure
the wobbles of 100 pulsars,
97
00:04:58,867 --> 00:04:59,975
spread across light-years
of space.
98
00:05:00,000 --> 00:05:02,141
Spread across light-years
of space.
99
00:05:02,165 --> 00:05:06,165
It's like a tsunami,
and the pulsars are
100
00:05:06,266 --> 00:05:08,600
like the buoys on the surface
of the ocean.
101
00:05:08,666 --> 00:05:10,643
And as the tsunami passes by,
102
00:05:10,666 --> 00:05:12,543
we can watch all of them moving
103
00:05:12,567 --> 00:05:14,199
and shifting up and down.
104
00:05:14,266 --> 00:05:16,100
So our pulsar timing array
105
00:05:16,165 --> 00:05:18,667
is a gravitational wave
warning system.
106
00:05:20,000 --> 00:05:22,266
The pulsar array has identified
107
00:05:22,367 --> 00:05:25,600
the source of the tsunami
of gravitational waves.
108
00:05:27,266 --> 00:05:29,367
The only thing we know
of that can make these
109
00:05:29,466 --> 00:05:29,976
very long wavelength,
very low pitch
110
00:05:30,000 --> 00:05:32,042
very long wavelength,
very low pitch
111
00:05:32,066 --> 00:05:34,800
gravitational waves
would be the collisions
112
00:05:34,867 --> 00:05:36,643
of supermassive black holes.
113
00:05:36,667 --> 00:05:38,742
They're massive, they're huge,
114
00:05:38,766 --> 00:05:40,942
and they know how
to throw their weight around.
115
00:05:40,966 --> 00:05:44,343
Supermassive black hole
binaries produce the loudest
116
00:05:44,367 --> 00:05:46,500
gravitational waves in
the universe.
117
00:05:48,100 --> 00:05:50,667
The gravitational wave
signal revealed
118
00:05:50,766 --> 00:05:52,543
something extraordinary.
119
00:05:52,567 --> 00:05:55,141
It's not just
gravitational waves coming
120
00:05:55,165 --> 00:05:57,843
from one black hole binary pair.
121
00:05:57,867 --> 00:05:59,399
It's actually from the cosmic
122
00:05:59,466 --> 00:05:59,976
population of supermassive
black hole binaries.
123
00:06:00,000 --> 00:06:03,199
Population of supermassive
black hole binaries.
124
00:06:04,500 --> 00:06:06,800
Chiara and her team
think there may be
125
00:06:06,867 --> 00:06:11,266
tens of thousands of
heavyweight bouts going on.
126
00:06:11,367 --> 00:06:14,867
Now, the scientists want to
pick out the sound of one
127
00:06:14,966 --> 00:06:19,899
single collision between two
supermassive black holes from
128
00:06:20,000 --> 00:06:21,667
the background roar.
129
00:06:24,165 --> 00:06:26,100
If we were to hear
130
00:06:26,165 --> 00:06:28,000
a supermassive
black hole merger,
131
00:06:28,100 --> 00:06:29,975
it would sound like a very
low frequency growl.
132
00:06:30,000 --> 00:06:30,699
It would sound like a very
low frequency growl.
133
00:06:30,766 --> 00:06:33,399
This "ooooooh"
134
00:06:33,466 --> 00:06:36,199
that would last
about 25 million years.
135
00:06:36,266 --> 00:06:39,100
To date, we haven't
witnessed two supermassive
136
00:06:39,165 --> 00:06:41,942
black holes trading blows
in real time.
137
00:06:41,966 --> 00:06:45,343
But we have seen events
leading up
138
00:06:45,367 --> 00:06:47,100
to the championship bout.
139
00:06:47,165 --> 00:06:50,000
We've watched galaxies merge.
140
00:06:50,100 --> 00:06:51,500
We've seen stars explode.
141
00:06:51,567 --> 00:06:54,567
We've seen so many violent
events in the universe.
142
00:06:54,667 --> 00:06:56,367
But we haven't seen this one.
143
00:06:56,466 --> 00:06:58,667
It's odd if you think about it.
144
00:06:58,766 --> 00:06:59,975
We haven't seen the biggest one.
145
00:07:00,000 --> 00:07:00,500
We haven't seen the biggest one.
146
00:07:00,567 --> 00:07:03,942
We haven't seen mergers between
supermassive black holes.
147
00:07:03,966 --> 00:07:06,567
But that may be about to change.
148
00:07:08,600 --> 00:07:12,442
Chiara predicts there are
112 fighters who are
149
00:07:12,466 --> 00:07:15,567
pumped up and ready
to enter the ring.
150
00:07:18,266 --> 00:07:19,600
In the next five years,
151
00:07:19,667 --> 00:07:22,300
we should be able to detect
at least one
152
00:07:22,367 --> 00:07:24,141
supermassive black hole merger.
153
00:07:24,165 --> 00:07:29,975
It'll be the most violent
event in the cosmos.
154
00:07:30,000 --> 00:07:30,600
It'll be the most violent
event in the cosmos.
155
00:07:30,667 --> 00:07:32,699
Let's put that in context.
156
00:07:32,766 --> 00:07:37,165
We talk about how supernova
are some of the most explosive,
157
00:07:37,266 --> 00:07:39,466
energetic things in
our universe.
158
00:07:39,567 --> 00:07:42,543
Well, colliding supermassive
black holes
159
00:07:42,567 --> 00:07:45,000
are a billion, billion, billion,
160
00:07:45,066 --> 00:07:48,800
billion times more energetic
than a supernova.
161
00:07:48,867 --> 00:07:52,100
Think about all of the light
being emitted by everything in
162
00:07:52,165 --> 00:07:55,367
the universe,
every star, every galaxy.
163
00:07:55,466 --> 00:07:58,199
In one instant,
two supermassive black holes
164
00:07:58,266 --> 00:07:59,975
colliding could release
100 million times that energy.
165
00:08:00,000 --> 00:08:02,543
Colliding could release
100 million times that energy.
166
00:08:02,567 --> 00:08:05,942
Imagine being
punched in the face by
167
00:08:05,966 --> 00:08:08,899
the biggest, baddest
heavyweight of all time.
168
00:08:09,000 --> 00:08:11,742
Ouch.
169
00:08:11,766 --> 00:08:13,843
This is way bigger than that.
170
00:08:13,867 --> 00:08:17,543
Where does
all this energy come from?
171
00:08:17,567 --> 00:08:19,867
Surprisingly, it originates in
172
00:08:19,966 --> 00:08:22,667
the smallest atoms in
the cosmos,
173
00:08:22,766 --> 00:08:26,199
in a story that dates back
billions of years,
174
00:08:26,266 --> 00:08:29,667
all the way to the birth of
the universe.
175
00:08:38,866 --> 00:08:40,000
We're taking our seats for
176
00:08:40,100 --> 00:08:43,000
the most violent event
in the universe,
177
00:08:43,100 --> 00:08:47,265
the collision of two
supermassive black holes.
178
00:08:47,366 --> 00:08:49,100
We've never witnessed
this cosmic
179
00:08:49,165 --> 00:08:50,799
heavyweight championship,
180
00:08:50,866 --> 00:08:54,342
but we can build up a picture
of this epic fight by studying
181
00:08:54,366 --> 00:08:56,767
other weight classes
with lighter fighters.
182
00:09:01,399 --> 00:09:03,054
2020... the earthbound
gravitational wave detector,
183
00:09:03,078 --> 00:09:05,767
2020... the earthbound
gravitational wave detector,
184
00:09:05,866 --> 00:09:07,366
LIGO, picks up
185
00:09:07,466 --> 00:09:10,366
the distinctive signal of
a stellar mass
186
00:09:10,466 --> 00:09:11,700
black hole merger.
187
00:09:12,899 --> 00:09:17,842
What we saw was a black hole
of 85 times the mass of our sun,
188
00:09:17,866 --> 00:09:21,142
and another black hole of
66 times the mass of our sun,
189
00:09:21,166 --> 00:09:25,142
smashing together to create
a combined black hole.
190
00:09:25,166 --> 00:09:29,000
As someone who
studies black hole mergers,
191
00:09:29,100 --> 00:09:31,000
this was a really
exciting event.
192
00:09:31,066 --> 00:09:32,142
We're talking about
193
00:09:32,165 --> 00:09:33,056
the largest, the heaviest,
the most massive
194
00:09:33,080 --> 00:09:34,643
the largest, the heaviest,
the most massive
195
00:09:34,667 --> 00:09:37,399
black holes we have seen
collide to date.
196
00:09:39,165 --> 00:09:41,241
It may be the largest detection,
197
00:09:41,265 --> 00:09:43,265
but on a universal scale,
198
00:09:43,366 --> 00:09:46,866
it's still a small fry...
Like lightweight boxers,
199
00:09:46,966 --> 00:09:49,700
the two black holes
circle each other
200
00:09:49,767 --> 00:09:53,899
and emit low energy
gravitational waves.
201
00:09:54,000 --> 00:09:56,466
This energy loss causes
the black holes
202
00:09:56,567 --> 00:09:59,000
to spiral in together.
203
00:09:59,066 --> 00:10:02,899
Finally, they collide in
a cosmos-shattering event,
204
00:10:04,667 --> 00:10:07,100
forming a single black hole
205
00:10:07,166 --> 00:10:11,265
and releasing a huge blast
of gravitational waves.
206
00:10:11,366 --> 00:10:16,241
But when astronomers examine
the single merged black hole,
207
00:10:16,265 --> 00:10:18,567
something doesn't add up.
208
00:10:18,667 --> 00:10:20,667
If you take the combined mass of
209
00:10:20,767 --> 00:10:24,042
the two black holes,
you get to 150 times
210
00:10:24,066 --> 00:10:25,466
the mass of our sun.
211
00:10:25,567 --> 00:10:28,799
But actually, the black hole
that's left only has
212
00:10:28,866 --> 00:10:33,054
a mass of 142 times
the mass of our sun.
213
00:10:33,078 --> 00:10:33,500
A mass of 142 times
the mass of our sun.
214
00:10:33,567 --> 00:10:36,399
So the mass you have
before the event does
215
00:10:36,466 --> 00:10:39,643
not equal the mass you have
after the event.
216
00:10:39,667 --> 00:10:44,042
What happened to that missing
eight solar masses?
217
00:10:44,066 --> 00:10:48,000
The way these black hole mergers
work is very roughly 5 percent
218
00:10:48,100 --> 00:10:50,866
of the total mass of
the system gets converted
219
00:10:50,966 --> 00:10:52,342
into energy.
220
00:10:52,366 --> 00:10:56,799
It all comes down to
E equals MC squared.
221
00:10:58,000 --> 00:11:00,466
This is that beautiful
equation that Einstein
222
00:11:00,567 --> 00:11:02,942
told us... E equals MC squared.
223
00:11:02,966 --> 00:11:03,056
E is the energy,
and M is the mass.
224
00:11:03,080 --> 00:11:06,000
E is the energy,
and M is the mass.
225
00:11:06,066 --> 00:11:09,342
Einstein taught us that mass
and energy are related.
226
00:11:09,366 --> 00:11:13,466
In fact, much of what we call
mass is actually energy.
227
00:11:13,567 --> 00:11:16,543
In this case,
the violence of the collision
228
00:11:16,567 --> 00:11:21,265
transforms 18,000 trillion
trillion tons
229
00:11:21,366 --> 00:11:25,366
of matter into an explosion
of gravitational waves.
230
00:11:25,466 --> 00:11:28,166
In just a fraction of a second,
231
00:11:28,265 --> 00:11:33,054
eight suns worth of matter is
converted into pure
232
00:11:33,078 --> 00:11:33,866
eight suns worth of matter is
converted into pure
233
00:11:33,966 --> 00:11:35,866
unadulterated energy.
234
00:11:35,966 --> 00:11:38,942
The amount of energy released
was so great, that if you add
235
00:11:38,966 --> 00:11:41,899
up all the energy of all
the stars burning in
236
00:11:42,000 --> 00:11:43,643
the universe,
237
00:11:43,667 --> 00:11:45,643
it was bigger than that.
238
00:11:45,667 --> 00:11:50,743
This event was a collision
between relative lightweights,
239
00:11:50,767 --> 00:11:54,000
two stellar mass black holes.
240
00:11:56,100 --> 00:11:58,399
To understand heavyweight bouts,
241
00:11:58,466 --> 00:12:03,054
we need to scale up to
supermassive black holes.
242
00:12:03,078 --> 00:12:04,958
We need to scale up to
supermassive black holes.
243
00:12:06,100 --> 00:12:07,899
In the universe of sports,
244
00:12:08,000 --> 00:12:11,500
supermassive black holes are
the heavyweight contenders.
245
00:12:11,567 --> 00:12:14,767
With these big black holes,
size matters.
246
00:12:14,866 --> 00:12:16,299
The bigger the better.
247
00:12:16,366 --> 00:12:18,442
More mass means more energy,
248
00:12:18,466 --> 00:12:21,265
which means more
destructive power.
249
00:12:21,366 --> 00:12:23,942
We don't need to look
too far to find
250
00:12:23,966 --> 00:12:26,000
this devastating muscle.
251
00:12:26,066 --> 00:12:28,942
This is M87 star,
252
00:12:28,966 --> 00:12:32,299
one of the largest
supermassive black holes
253
00:12:32,366 --> 00:12:33,054
in our cosmic zip code.
254
00:12:33,078 --> 00:12:34,078
In our cosmic zip code.
255
00:12:34,966 --> 00:12:37,442
M87 star is huge.
256
00:12:37,466 --> 00:12:40,466
It weighs about six billion
solar masses,
257
00:12:40,567 --> 00:12:42,000
about six billion suns,
258
00:12:42,066 --> 00:12:44,466
and it's the size
of our solar system.
259
00:12:44,567 --> 00:12:48,142
A collision between two
6-billion solar mass
260
00:12:48,165 --> 00:12:51,299
supermassive black holes would
release around five
261
00:12:51,366 --> 00:12:55,399
times 10 to the power of
56 joules.
262
00:12:55,466 --> 00:12:59,299
So what's that mean
in real world terms?
263
00:12:59,366 --> 00:13:02,743
It's hard to use words to
express how much energy this is,
264
00:13:02,767 --> 00:13:03,056
and the numbers are so huge,
they are almost meaningless.
265
00:13:03,080 --> 00:13:05,500
And the numbers are so huge,
they are almost meaningless.
266
00:13:05,567 --> 00:13:07,966
The only way I can really
explain this is...
267
00:13:11,767 --> 00:13:14,442
In physics,
we have these comparisons
268
00:13:14,466 --> 00:13:15,706
so we can get a mental picture,
269
00:13:15,767 --> 00:13:18,500
but for something like this,
there is no mental picture.
270
00:13:18,567 --> 00:13:21,100
That is so freaking big.
271
00:13:24,166 --> 00:13:26,241
So where does this destructive
272
00:13:26,265 --> 00:13:29,100
mass and energy come from?
273
00:13:32,366 --> 00:13:33,056
It starts with
the simplest ingredient...
274
00:13:33,080 --> 00:13:35,466
It starts with
the simplest ingredient...
275
00:13:35,567 --> 00:13:37,000
Hydrogen.
276
00:13:39,667 --> 00:13:44,165
Hydrogen is the basic
building block of the universe.
277
00:13:44,265 --> 00:13:49,667
Each atom is tiny, but it
contains a lot of energy.
278
00:13:49,767 --> 00:13:52,667
Hydrogen atoms contain a huge
amount of energy,
279
00:13:52,767 --> 00:13:54,265
just like all matter does.
280
00:13:54,366 --> 00:13:56,000
And if it's unlocked in
281
00:13:56,066 --> 00:13:58,866
a certain way,
there can be huge explosions.
282
00:14:01,767 --> 00:14:03,054
I mean, you take the mass
contained simply in my hand,
283
00:14:03,078 --> 00:14:04,842
I mean, you take the mass
contained simply in my hand,
284
00:14:04,866 --> 00:14:07,000
and you could blow up
pretty much the entire Earth.
285
00:14:07,066 --> 00:14:11,166
Matter has energy
because it formed from
286
00:14:11,265 --> 00:14:13,667
energy in the early moments
of the universe.
287
00:14:14,767 --> 00:14:17,466
In many ways,
atoms are reservoirs
288
00:14:17,567 --> 00:14:20,700
of stored energy
from the Big Bang.
289
00:14:20,767 --> 00:14:24,200
13.8 billion years ago,
290
00:14:24,265 --> 00:14:26,667
the universe ignites
291
00:14:26,767 --> 00:14:30,366
in a super hot ball of
intense energy.
292
00:14:30,466 --> 00:14:33,054
Right after the Big Bang,
there's a tremendous
293
00:14:33,078 --> 00:14:33,243
Right after the Big Bang,
there's a tremendous
294
00:14:33,267 --> 00:14:34,700
amount of energy...
So much energy,
295
00:14:34,767 --> 00:14:36,899
in fact, that normal atoms
can't exist.
296
00:14:39,366 --> 00:14:42,366
As that early energy
starts to cool,
297
00:14:42,466 --> 00:14:45,265
it can start to form
primitive matter.
298
00:14:47,866 --> 00:14:51,042
The universe takes
that first matter and energy
299
00:14:51,066 --> 00:14:53,366
in the form of hydrogen atoms
300
00:14:53,466 --> 00:14:55,842
and starts
the process of creating
301
00:14:55,866 --> 00:14:58,241
a supermassive black hole.
302
00:14:58,265 --> 00:15:01,600
Step one... build giant stars.
303
00:15:01,667 --> 00:15:03,054
So gravity brings
together gas, dust, hydrogen,
304
00:15:03,078 --> 00:15:06,366
So gravity brings
together gas, dust, hydrogen,
305
00:15:06,466 --> 00:15:07,466
all of that stuff,
306
00:15:07,567 --> 00:15:09,700
and as the clouds
become more dense,
307
00:15:09,767 --> 00:15:12,500
they attract even more material.
308
00:15:12,567 --> 00:15:16,442
As they spin, they get
hotter and hotter, and as that
309
00:15:16,466 --> 00:15:18,399
temperature
and pressure increase,
310
00:15:18,466 --> 00:15:21,842
finally, it ignites
nuclear fusion within the core
311
00:15:21,866 --> 00:15:23,700
and creates an actual star.
312
00:15:26,200 --> 00:15:29,942
These huge stars
are like cosmic rock stars.
313
00:15:29,966 --> 00:15:32,200
They live fast and die young.
314
00:15:33,767 --> 00:15:38,567
When they die, they flame out
in a huge explosion,
315
00:15:38,667 --> 00:15:40,466
a supernova.
316
00:15:40,567 --> 00:15:44,842
The entire star
turns itself inside out
317
00:15:44,866 --> 00:15:48,142
and releases a shockwave
going a good
318
00:15:48,165 --> 00:15:52,100
fraction of the speed of light
and releases enough energy to
319
00:15:52,165 --> 00:15:54,100
just obliterate you.
320
00:15:54,165 --> 00:15:57,342
If the dying star is more
321
00:15:57,366 --> 00:15:59,567
than 15 stellar masses,
322
00:15:59,667 --> 00:16:02,842
its core collapses
into a black hole.
323
00:16:02,866 --> 00:16:03,056
It's kind of astounding
what the universe is doing.
324
00:16:03,080 --> 00:16:06,100
It's kind of astounding
what the universe is doing.
325
00:16:06,166 --> 00:16:09,142
It's taking incredibly simple
things, like hydrogen atoms,
326
00:16:09,166 --> 00:16:11,643
and using gravity to ultimately
327
00:16:11,667 --> 00:16:13,427
bring all this stuff together
and make things
328
00:16:13,466 --> 00:16:15,567
like black holes.
329
00:16:15,667 --> 00:16:18,842
I find it quite beautiful
how our whole
330
00:16:18,866 --> 00:16:21,399
cosmic history is the story of
331
00:16:21,466 --> 00:16:24,600
little things coming together
into bigger things.
332
00:16:24,667 --> 00:16:27,466
But these stellar mass
black holes are tiny
333
00:16:27,567 --> 00:16:31,042
flyweights... to step up to
the heavyweight division,
334
00:16:31,066 --> 00:16:33,054
they have to grow billions of
times more massive.
335
00:16:33,078 --> 00:16:35,000
They have to grow billions of
times more massive.
336
00:16:35,066 --> 00:16:36,899
But how?
337
00:16:37,000 --> 00:16:39,700
How do black holes
become supermassive?
338
00:16:40,866 --> 00:16:43,100
This is the age-old question.
339
00:16:43,165 --> 00:16:44,799
We're not really sure.
340
00:16:44,866 --> 00:16:47,700
The current state
of our understanding
341
00:16:47,767 --> 00:16:50,743
of how black holes become
supermassive is like,
342
00:16:50,767 --> 00:16:52,442
uhhh, we're confused.
343
00:16:52,466 --> 00:16:53,866
We really don't know.
344
00:16:53,966 --> 00:16:57,466
We still don't know exactly
how they become so big.
345
00:16:59,399 --> 00:17:00,667
But we do know that
346
00:17:00,767 --> 00:17:03,054
the process involves
ultraviolence,
347
00:17:03,078 --> 00:17:03,500
the process involves
ultraviolence,
348
00:17:03,567 --> 00:17:05,366
death, and destruction.
349
00:17:14,165 --> 00:17:18,299
How do supermassive
black holes grow so big?
350
00:17:18,366 --> 00:17:22,200
That's a question that
continues to baffle scientists.
351
00:17:22,266 --> 00:17:26,299
In June of 2018,
we spotted a clue,
352
00:17:26,366 --> 00:17:28,599
an enormous flash of light.
353
00:17:28,666 --> 00:17:32,041
AT2018cow,
354
00:17:32,066 --> 00:17:33,366
nicknamed "the cow,"
355
00:17:33,467 --> 00:17:36,900
was the brightest explosion
ever recorded.
356
00:17:37,000 --> 00:17:38,068
A huge amount of energy
was released,
357
00:17:38,093 --> 00:17:39,142
A huge amount of energy
was released,
358
00:17:39,165 --> 00:17:41,000
and then all of a sudden,
everything was gone.
359
00:17:42,266 --> 00:17:45,142
This explosion
was incredibly violent.
360
00:17:45,165 --> 00:17:46,099
At first, it was thought
361
00:17:46,165 --> 00:17:48,400
to just be a supernova,
a flash of light.
362
00:17:48,467 --> 00:17:50,000
But over time, it became clear
363
00:17:50,066 --> 00:17:52,442
that this was something much
more powerful.
364
00:17:52,467 --> 00:17:55,742
It was too bright, basically,
to be a supernova.
365
00:17:55,767 --> 00:17:59,142
It was extremely bright,
and it didn't fit into
366
00:17:59,165 --> 00:18:01,299
any of our theoretical
understandings
367
00:18:01,366 --> 00:18:03,567
of how bright
supernova should be.
368
00:18:04,599 --> 00:18:07,542
One explanation is that
the light may have come from
369
00:18:07,567 --> 00:18:08,069
a black hole feeding
370
00:18:08,094 --> 00:18:09,299
a black hole feeding
371
00:18:09,366 --> 00:18:13,742
on a small white dwarf star
weighing less than the sun.
372
00:18:13,767 --> 00:18:18,099
What really seemed to fit that
model was a star getting
373
00:18:18,165 --> 00:18:19,343
too close to a black hole
374
00:18:19,366 --> 00:18:20,700
and getting ripped apart,
and then
375
00:18:20,767 --> 00:18:22,567
everything going right down
the black hole.
376
00:18:24,165 --> 00:18:27,366
A black hole gains mass
every time it eats something.
377
00:18:27,467 --> 00:18:28,643
That's how they grow.
378
00:18:28,666 --> 00:18:31,542
Whether it's a gas cloud
or a star or another black hole,
379
00:18:31,567 --> 00:18:34,799
once it gains that mass,
it's gained that mass.
380
00:18:37,366 --> 00:18:38,069
People often ask me,
what happens to
381
00:18:38,094 --> 00:18:39,241
People often ask me,
what happens to
382
00:18:39,266 --> 00:18:41,099
the mass that falls
into a black hole?
383
00:18:41,165 --> 00:18:42,666
Does it go to another dimension?
384
00:18:42,767 --> 00:18:45,200
And the answer is no,
it's still there.
385
00:18:45,266 --> 00:18:50,000
It's inside the black hole...
They get bigger, they grow.
386
00:18:50,066 --> 00:18:53,666
Could this be how weak
flyweight black holes
387
00:18:53,767 --> 00:18:55,700
turn into mean and powerful
388
00:18:55,767 --> 00:18:57,599
supermassive heavyweights?
389
00:18:57,666 --> 00:18:59,599
The star is like protein,
390
00:18:59,666 --> 00:19:04,142
and the black hole
is like a boxer.
391
00:19:04,165 --> 00:19:07,000
And so the more protein
they get, the more stars
392
00:19:07,066 --> 00:19:08,068
they consume,
the stronger they get,
393
00:19:08,093 --> 00:19:08,567
they consume,
the stronger they get,
394
00:19:08,666 --> 00:19:10,266
the more destructive
they can be.
395
00:19:13,700 --> 00:19:15,200
But there's a problem with
396
00:19:15,266 --> 00:19:16,866
the training program
explanation.
397
00:19:18,400 --> 00:19:20,467
Eating small stars
398
00:19:20,567 --> 00:19:24,165
one at a time just doesn't
add enough mass fast enough
399
00:19:24,266 --> 00:19:26,241
to grow
the supermassive black holes
400
00:19:26,266 --> 00:19:27,599
that we see today.
401
00:19:27,666 --> 00:19:32,500
That's like boxers eating just
one egg per day.
402
00:19:32,567 --> 00:19:37,599
Like them, black holes
need much bigger meals,
403
00:19:37,666 --> 00:19:38,069
and in 2020, we detected one,
404
00:19:38,094 --> 00:19:41,599
and in 2020, we detected one,
405
00:19:41,666 --> 00:19:44,742
a sudden burst of
gravitational waves from
406
00:19:44,767 --> 00:19:46,700
a black hole gorging on
407
00:19:46,767 --> 00:19:49,142
the remains of a dead star
408
00:19:49,165 --> 00:19:53,165
called a neutron star.
409
00:19:54,165 --> 00:19:58,400
For scientists, January 2020
was exciting, because it was
410
00:19:58,467 --> 00:20:02,400
the first time LIGO observed
the very first black hole
411
00:20:02,467 --> 00:20:04,241
neutron star merger.
412
00:20:04,266 --> 00:20:07,099
Neutron stars may be small,
413
00:20:07,165 --> 00:20:08,069
but they are
inconceivably dense.
414
00:20:08,094 --> 00:20:10,467
But they are
inconceivably dense.
415
00:20:10,567 --> 00:20:12,343
Now, you want to talk about
an enormous amount of mass,
416
00:20:12,366 --> 00:20:13,542
let's talk about a neutron star.
417
00:20:13,567 --> 00:20:15,165
That's... that's one heck of
a snack.
418
00:20:16,266 --> 00:20:20,266
The black hole swallowed
the neutron star in one gulp.
419
00:20:21,567 --> 00:20:25,366
So this black hole
ate a whole neutron star,
420
00:20:25,467 --> 00:20:28,866
which means it gained just
over 10 percent of its entire
421
00:20:28,967 --> 00:20:31,366
body weight in one shot.
422
00:20:31,467 --> 00:20:34,099
10 percent doesn't
sound like a lot,
423
00:20:34,165 --> 00:20:36,099
but then we detected another
424
00:20:36,165 --> 00:20:38,068
black hole swallowing a neutron
star just 10 days later,
425
00:20:38,093 --> 00:20:40,142
black hole swallowing a neutron
star just 10 days later,
426
00:20:40,165 --> 00:20:44,099
suggesting that there are lots
of black holes bulking up
427
00:20:44,165 --> 00:20:45,266
across the universe.
428
00:20:45,366 --> 00:20:48,442
But even with this extreme
weight gain,
429
00:20:48,467 --> 00:20:52,400
it's probably not enough to
get supermassive.
430
00:20:52,467 --> 00:20:54,366
They need to eat even more.
431
00:20:55,567 --> 00:20:57,700
If you're a black hole,
and you want to get bigger,
432
00:20:57,767 --> 00:21:01,266
your best bet is to merge
with another black hole.
433
00:21:01,366 --> 00:21:03,442
But there's a catch.
434
00:21:03,467 --> 00:21:08,068
So if you're a flyweight black
hole, and you try to eat all of
435
00:21:08,093 --> 00:21:09,542
So if you're a flyweight black
hole, and you try to eat all of
436
00:21:09,567 --> 00:21:11,567
the other flyweight black holes,
437
00:21:11,666 --> 00:21:15,041
there's just not enough time
in the history of the universe
438
00:21:15,066 --> 00:21:17,799
for you to become
a supermassive black hole.
439
00:21:17,866 --> 00:21:20,266
But you can make it
to middleweight.
440
00:21:20,366 --> 00:21:24,400
So exactly how
supermassive black holes
441
00:21:24,467 --> 00:21:27,866
grow so large remains
an open question.
442
00:21:27,967 --> 00:21:31,366
We do know that the process
started in the very early
443
00:21:31,467 --> 00:21:33,099
universe with a journey
444
00:21:33,165 --> 00:21:35,165
from the lightest
element to the most
445
00:21:35,266 --> 00:21:38,068
intimidating object
in the cosmos.
446
00:21:38,093 --> 00:21:38,344
Intimidating object
in the cosmos.
447
00:21:38,367 --> 00:21:41,142
It's so interesting how
the cosmos can take something as
448
00:21:41,165 --> 00:21:44,843
simple as a hydrogen atom
and build stellar mass
449
00:21:44,866 --> 00:21:48,700
black holes and intermediate
mass black holes
450
00:21:48,767 --> 00:21:51,165
and even supermassive
black holes out of
451
00:21:51,266 --> 00:21:55,467
these really densely compressed
hydrogen atoms.
452
00:21:55,567 --> 00:21:58,165
It's really a wonder.
453
00:21:58,266 --> 00:22:01,142
Now, 13.8 billion years
454
00:22:01,165 --> 00:22:04,343
after the Big Bang,
supermassive black holes
455
00:22:04,366 --> 00:22:06,799
feed and flex their muscles,
456
00:22:06,866 --> 00:22:08,068
ready to fight
for the heavyweight
457
00:22:08,093 --> 00:22:08,743
ready to fight
for the heavyweight
458
00:22:08,768 --> 00:22:10,643
championship of the universe.
459
00:22:10,666 --> 00:22:13,942
These supermassive black holes
have been bulking up
460
00:22:13,967 --> 00:22:15,767
since the age of the universe.
461
00:22:15,866 --> 00:22:17,799
These black holes have been
462
00:22:17,866 --> 00:22:19,666
getting ready for the fight.
463
00:22:19,767 --> 00:22:21,165
They have been bulking up.
464
00:22:21,266 --> 00:22:24,942
They have been eating
entire stars as snacks
465
00:22:24,967 --> 00:22:27,099
to get the masks they need.
466
00:22:27,165 --> 00:22:29,000
So they are ready to rumble.
467
00:22:30,000 --> 00:22:32,266
It's not the rumble
in the jungle.
468
00:22:32,366 --> 00:22:36,266
This is the battle to be
the boss of the cosmos.
469
00:22:36,366 --> 00:22:38,068
Supermassive black hole
versus supermassive
470
00:22:38,093 --> 00:22:40,400
Supermassive black hole
versus supermassive
471
00:22:40,467 --> 00:22:44,542
black hole, fought in
the grandest arena.
472
00:22:44,567 --> 00:22:48,567
The fighter's entourage,
their host galaxies,
473
00:22:48,666 --> 00:22:50,599
escort them to the ring.
474
00:22:50,666 --> 00:22:52,866
But even this journey
is violent,
475
00:22:52,967 --> 00:22:56,866
triggering starbursts, jets,
and carnage.
476
00:23:05,767 --> 00:23:08,467
It's the build up before
the heavyweight fight
477
00:23:08,567 --> 00:23:10,165
of the cosmos.
478
00:23:10,266 --> 00:23:13,967
The fighters' entourages,
their galaxies, carry
479
00:23:14,032 --> 00:23:16,500
their supermassive black holes
to the ring.
480
00:23:17,767 --> 00:23:19,733
Things are about to get nasty.
481
00:23:20,866 --> 00:23:23,299
Galaxies can look calm
and serene,
482
00:23:23,366 --> 00:23:25,767
but they can get into
pretty big scraps.
483
00:23:28,266 --> 00:23:29,354
There's a lot of them
that are totally
484
00:23:29,377 --> 00:23:30,165
There's a lot of them
that are totally
485
00:23:30,232 --> 00:23:33,933
messed up and are clearly
merging with each other.
486
00:23:37,066 --> 00:23:40,710
When galaxies fight,
their gravity pulls on each
487
00:23:40,733 --> 00:23:43,767
other, twisting and distorting
their structures.
488
00:23:43,834 --> 00:23:49,099
The galaxy will be warped
and morphed into different ways
489
00:23:49,165 --> 00:23:52,767
that we can only imagine
how twisted it would be.
490
00:23:54,467 --> 00:23:56,467
This violent cosmic tango brings
491
00:23:56,567 --> 00:23:59,354
the two supermassive
black holes together.
492
00:23:59,377 --> 00:23:59,400
The two supermassive
black holes together.
493
00:23:59,467 --> 00:24:02,099
It's elegant, it's beautiful.
494
00:24:02,165 --> 00:24:06,666
It's this billion-year
choreographed dance
495
00:24:06,733 --> 00:24:09,299
that is entirely conducted
by gravity.
496
00:24:12,866 --> 00:24:15,933
The two heavyweight
fighters approach each other.
497
00:24:16,000 --> 00:24:18,066
Their feet beat out a rhythm
on the canvas,
498
00:24:18,133 --> 00:24:22,400
just like circling black holes
release low energy
499
00:24:22,467 --> 00:24:24,000
gravitational waves.
500
00:24:25,099 --> 00:24:29,165
You have these giant beasts
that are stalking
501
00:24:29,266 --> 00:24:29,355
around each other,
and as they do,
502
00:24:29,378 --> 00:24:31,266
around each other,
and as they do,
503
00:24:31,366 --> 00:24:34,133
they create these
gravitational waves.
504
00:24:36,366 --> 00:24:39,099
June 2021.
505
00:24:39,165 --> 00:24:42,066
Astronomers photograph
a galactic collision
506
00:24:42,133 --> 00:24:46,442
and witness a spectacular
pre-fight fireworks show.
507
00:24:46,467 --> 00:24:49,343
One of the amazing things
that can happen
508
00:24:49,366 --> 00:24:51,241
when galaxies collide
is they can create
509
00:24:51,266 --> 00:24:53,400
tremendous starbursts.
510
00:24:53,467 --> 00:24:56,108
There is a big inrush as all of
511
00:24:56,133 --> 00:24:59,354
the gas follows that gravity...
As the gas gets hotter
512
00:24:59,377 --> 00:25:00,076
the gas follows that gravity...
As the gas gets hotter
513
00:25:00,101 --> 00:25:03,165
and denser,
it creates shockwaves,
514
00:25:03,266 --> 00:25:05,866
and each shockwave actually
creates a new generation of
515
00:25:05,967 --> 00:25:09,209
stars going out around
the core of the galaxy.
516
00:25:09,232 --> 00:25:13,066
The sudden starburst
lights up the merging galaxies.
517
00:25:13,133 --> 00:25:16,467
The inrushing gas also fuels
the prize fighters,
518
00:25:17,467 --> 00:25:20,108
the supermassive
black holes spiraling
519
00:25:20,133 --> 00:25:24,400
towards the merging
galactic center.
520
00:25:24,467 --> 00:25:28,000
If there's a big
supermassive black hole,
521
00:25:28,066 --> 00:25:29,354
it suddenly finds it
surrounded by loads of gas
522
00:25:29,377 --> 00:25:31,442
it suddenly finds it
surrounded by loads of gas
523
00:25:31,467 --> 00:25:34,266
and other material it can eat.
524
00:25:34,366 --> 00:25:37,066
It goes on a kind of
feeding frenzy.
525
00:25:37,133 --> 00:25:39,467
If you're a hungry
supermassive black hole,
526
00:25:39,567 --> 00:25:42,666
then this is
your lunchtime buffet.
527
00:25:42,767 --> 00:25:46,767
Not all the gas falls into
the supermassive black hole.
528
00:25:46,834 --> 00:25:50,967
Other parts of the matter
actually gets caught up
529
00:25:51,032 --> 00:25:52,866
in what we call
an accretion disk
530
00:25:52,967 --> 00:25:56,366
rotating around the outside
of the black hole.
531
00:25:56,467 --> 00:25:59,354
This bright vortex spins
around the supermassive
532
00:25:59,377 --> 00:25:59,500
This bright vortex spins
around the supermassive
533
00:25:59,567 --> 00:26:03,500
black hole at over
two million miles an hour.
534
00:26:03,567 --> 00:26:06,866
The material in the disk
rubs against itself,
535
00:26:06,967 --> 00:26:09,000
creating friction.
536
00:26:09,066 --> 00:26:12,866
Friction generates heat...
If I rub my hands together,
537
00:26:12,933 --> 00:26:14,400
they get a little bit warm.
538
00:26:14,467 --> 00:26:18,500
If I rub my hands together at
hundreds of thousands of
539
00:26:18,567 --> 00:26:21,733
miles per hour, it's gonna get
very, very, very warm.
540
00:26:24,066 --> 00:26:26,000
The accretion disk heats up,
541
00:26:26,066 --> 00:26:28,467
blasting out intense light.
542
00:26:30,366 --> 00:26:31,467
In 2020,
543
00:26:31,500 --> 00:26:35,108
NASA's Hubble space
telescope saw two fueled-up
544
00:26:35,133 --> 00:26:38,500
supermassive black holes
lighting up for the fight.
545
00:26:40,266 --> 00:26:42,099
We call them quasars.
546
00:26:43,767 --> 00:26:49,066
Quasars are a subclass
of very bright black holes
547
00:26:49,133 --> 00:26:51,299
that are emitting huge
amounts of power.
548
00:26:51,366 --> 00:26:54,467
So these can be seen at
the far reaches of the universe.
549
00:26:57,133 --> 00:26:59,354
Black holes,
these so-called dark things,
550
00:26:59,377 --> 00:26:59,666
Black holes,
these so-called dark things,
551
00:26:59,767 --> 00:27:01,933
when they're growing
at a very high rate
552
00:27:02,000 --> 00:27:04,866
are some of the brightest
lights in the universe.
553
00:27:05,866 --> 00:27:09,099
To date,
we've detected over 100 pairs
554
00:27:09,165 --> 00:27:13,108
of quasars in the cores of
merging galaxies.
555
00:27:13,133 --> 00:27:17,299
We think they will all
eventually collide,
556
00:27:17,366 --> 00:27:21,366
but before they do,
they'll put on a spectacular
557
00:27:21,467 --> 00:27:24,241
and lethal light show.
558
00:27:24,266 --> 00:27:27,666
A common theme
in science fiction
559
00:27:27,767 --> 00:27:29,354
are different kind of jets
of energy or beams
560
00:27:29,377 --> 00:27:30,109
are different kind of jets
of energy or beams
561
00:27:30,134 --> 00:27:32,500
that people shoot out of
their eyes or their hands.
562
00:27:32,567 --> 00:27:35,933
Well, supermassive black holes
do that, too.
563
00:27:36,000 --> 00:27:38,567
Firing out relativistic jets.
564
00:27:39,866 --> 00:27:43,467
When those jets fire up,
565
00:27:43,567 --> 00:27:46,666
that's when you're talking
about superstar, really,
566
00:27:46,733 --> 00:27:49,767
really bright lights, and at
this point, the galaxy is lit up
567
00:27:49,866 --> 00:27:51,000
and ready to go.
568
00:27:52,834 --> 00:27:57,032
These are the spotlight's
on Madison Square Garden.
569
00:27:57,099 --> 00:27:59,354
This is telling you that
the event is going down.
570
00:27:59,377 --> 00:28:01,298
This is telling you that
the event is going down.
571
00:28:02,032 --> 00:28:04,467
A single supermassive
black hole jet
572
00:28:04,567 --> 00:28:07,442
will produce more energy
in a second
573
00:28:07,467 --> 00:28:09,099
than the sun will produce in
574
00:28:09,165 --> 00:28:11,599
its entire
10-billion-year lifetime.
575
00:28:16,567 --> 00:28:20,032
Imagine a laser of
radiation that
576
00:28:20,099 --> 00:28:22,266
is light-years
in length and across.
577
00:28:22,366 --> 00:28:23,666
That's what we're talking about.
578
00:28:23,767 --> 00:28:26,266
This thing would fry a planet.
579
00:28:27,366 --> 00:28:29,354
This is no pre-fight hype.
580
00:28:29,377 --> 00:28:30,109
This is no pre-fight hype.
581
00:28:30,134 --> 00:28:34,834
In February 2020,
we saw the impact of a jet.
582
00:28:36,099 --> 00:28:38,000
So in the Ophiuchus
galaxy cluster,
583
00:28:38,066 --> 00:28:41,209
there's an enormous void
that is 15 times wider than
584
00:28:41,232 --> 00:28:42,299
the Milky Way galaxy.
585
00:28:42,366 --> 00:28:44,500
And this has all been
sculpted, carved,
586
00:28:44,567 --> 00:28:48,442
by jets from
a supermassive black hole.
587
00:28:48,467 --> 00:28:50,442
It's like this scar
on the universe.
588
00:28:50,467 --> 00:28:52,299
It's a million
light-years across.
589
00:28:52,366 --> 00:28:54,442
It's huge.
590
00:28:54,467 --> 00:28:57,467
Scientists calculate
the impact of the jet hitting
591
00:28:57,567 --> 00:28:59,354
the cluster was equivalent to
592
00:28:59,377 --> 00:28:59,810
the cluster was equivalent to
593
00:28:59,835 --> 00:29:05,165
a 20-billion-billion megaton
TNT explosion every 1,000th of
594
00:29:05,232 --> 00:29:09,066
a second for 240 million years.
595
00:29:12,500 --> 00:29:15,343
The relativistic jets'
immense power may be
596
00:29:15,366 --> 00:29:16,366
a showstopper.
597
00:29:16,467 --> 00:29:18,866
But when it's time to land
the killer punch,
598
00:29:18,967 --> 00:29:23,933
supermassive black holes draw
on an even more powerful force,
599
00:29:24,000 --> 00:29:25,500
gravity.
600
00:29:25,567 --> 00:29:27,666
Jets are very
powerful, but really
601
00:29:27,767 --> 00:29:29,354
only on a relatively
small scale.
602
00:29:29,377 --> 00:29:29,767
Only on a relatively
small scale.
603
00:29:29,834 --> 00:29:32,209
When you're talking about
cosmic scale,
604
00:29:32,232 --> 00:29:33,866
gravity always wins.
605
00:29:33,933 --> 00:29:36,710
Nothing is as powerful
as gravity.
606
00:29:36,733 --> 00:29:38,467
The immense gravity
of the circling
607
00:29:38,567 --> 00:29:42,599
supermassive black holes
drags them ever closer,
608
00:29:42,666 --> 00:29:46,066
but will it ultimately
bring them together
609
00:29:46,133 --> 00:29:47,933
or blast them apart?
610
00:29:56,567 --> 00:29:58,567
Across the universe,
611
00:29:58,666 --> 00:30:02,032
supermassive black holes
duke it out
612
00:30:02,099 --> 00:30:06,567
in the cosmos's version of
heavyweight super fights.
613
00:30:06,666 --> 00:30:11,442
Supermassive black holes are
merging around us all the time.
614
00:30:11,467 --> 00:30:13,933
It's only our ability
to detect them
615
00:30:14,000 --> 00:30:15,866
that's preventing us
from seeing them.
616
00:30:18,165 --> 00:30:19,663
Scientists have
identified at least a dozen
617
00:30:19,686 --> 00:30:20,742
Scientists have
identified at least a dozen
618
00:30:20,767 --> 00:30:24,567
pairs of supermassive black
holes circling each other.
619
00:30:25,933 --> 00:30:28,266
We have some hints
of some galaxies
620
00:30:28,366 --> 00:30:29,666
where we think it might happen,
621
00:30:29,767 --> 00:30:32,542
where we see two glowing black
holes that are getting
622
00:30:32,567 --> 00:30:33,767
very close.
623
00:30:34,933 --> 00:30:37,567
But not all these matches
will end with a knockout.
624
00:30:38,834 --> 00:30:41,442
Black hole collisions
happen all the time.
625
00:30:41,467 --> 00:30:44,165
But they don't always
go according to plan.
626
00:30:44,232 --> 00:30:45,866
When black holes come together,
627
00:30:45,933 --> 00:30:48,333
really strange things
can happen.
628
00:30:49,666 --> 00:30:49,663
The Hubble space telescope
spots something strange in
629
00:30:49,688 --> 00:30:53,967
The Hubble space telescope
spots something strange in
630
00:30:54,032 --> 00:30:58,666
a distant galaxy called 3C186.
631
00:30:58,767 --> 00:31:02,666
It's a quasar, an active
supermassive black hole.
632
00:31:05,066 --> 00:31:06,366
But it's in the wrong place.
633
00:31:07,666 --> 00:31:11,032
In nearly every galaxy we see,
the supermassive black hole
634
00:31:11,099 --> 00:31:12,967
sits right at the center,
and that makes sense.
635
00:31:14,066 --> 00:31:15,226
Because that's the only place
636
00:31:15,266 --> 00:31:18,165
with enough material to
power them.
637
00:31:18,232 --> 00:31:19,663
But in 3C186,
that's not what we see.
638
00:31:19,686 --> 00:31:21,567
But in 3C186,
that's not what we see.
639
00:31:21,666 --> 00:31:24,000
The supermassive black hole is
displaced from
640
00:31:24,066 --> 00:31:25,666
the center,
and not a little bit.
641
00:31:25,733 --> 00:31:27,933
It's 35,000 light-years.
642
00:31:28,000 --> 00:31:30,866
So to see a quasar
35,000 light-years away from
643
00:31:30,967 --> 00:31:33,599
the core means something
really violent
644
00:31:33,666 --> 00:31:34,866
had to happen there.
645
00:31:34,933 --> 00:31:37,866
The quasar is racing
away from the center
646
00:31:37,967 --> 00:31:41,866
of the galaxy at over
four million miles an hour.
647
00:31:41,933 --> 00:31:44,266
That is insane.
648
00:31:44,366 --> 00:31:46,108
The magnitude of the energy
649
00:31:46,133 --> 00:31:49,663
and the forces required are
just something unimaginable.
650
00:31:49,686 --> 00:31:50,309
And the forces required are
just something unimaginable.
651
00:31:50,334 --> 00:31:55,542
So what can kick a giant
black hole out of a galaxy?
652
00:31:55,567 --> 00:31:58,767
What has that kind of power?
653
00:31:58,866 --> 00:32:03,666
The answer is a clash
that wasn't evenly matched.
654
00:32:03,767 --> 00:32:08,000
The two supermassive black
holes were different sizes...
655
00:32:08,066 --> 00:32:11,733
A middleweight boxer
taking on a heavyweight.
656
00:32:13,066 --> 00:32:15,767
When we humans set up a fight,
we like to make it fair,
657
00:32:15,866 --> 00:32:17,066
because it's sport.
658
00:32:17,133 --> 00:32:18,500
Nature doesn't care about sport.
659
00:32:18,567 --> 00:32:19,663
It's survival of the fittest.
660
00:32:19,686 --> 00:32:20,000
It's survival of the fittest.
661
00:32:20,066 --> 00:32:21,500
This is not a fair fight.
662
00:32:21,567 --> 00:32:24,467
It's over before it even begins.
663
00:32:24,567 --> 00:32:26,767
One punch, and it's a K.O.
664
00:32:29,467 --> 00:32:31,666
As these two black holes
are merging,
665
00:32:31,733 --> 00:32:33,767
there's one
really small black hole
666
00:32:33,866 --> 00:32:35,209
and one much bigger black hole.
667
00:32:35,232 --> 00:32:38,108
The whole system wobbles
around, and it can get more of
668
00:32:38,133 --> 00:32:40,000
a gravitational wave kick in one
669
00:32:40,066 --> 00:32:42,767
direction than the other.
- And that's momentum.
670
00:32:42,866 --> 00:32:46,165
That's a push,
that's enough energy to kick
671
00:32:46,232 --> 00:32:47,567
the black hole out.
672
00:32:49,500 --> 00:32:49,663
The lopsided gravitational punch
673
00:32:49,688 --> 00:32:51,767
The lopsided gravitational punch
674
00:32:51,866 --> 00:32:53,866
sends the merged supermassive
675
00:32:53,967 --> 00:32:56,733
black hole on a one-way trip
to oblivion.
676
00:32:58,467 --> 00:33:00,076
This tells us that gravitational
677
00:33:00,099 --> 00:33:02,666
waves can be
tremendously powerful.
678
00:33:02,767 --> 00:33:05,567
They can move a supermassive
black hole out from
679
00:33:05,666 --> 00:33:08,866
the center of a galaxy
and send it on its way.
680
00:33:08,967 --> 00:33:10,400
But it just carries on drifting.
681
00:33:10,467 --> 00:33:12,500
There's no way to stop it.
682
00:33:12,567 --> 00:33:14,467
And who knows, in a few
million years it could
683
00:33:14,567 --> 00:33:17,266
just drift entirely
out of its galaxy
684
00:33:17,333 --> 00:33:19,663
and go floating off
into deep space.
685
00:33:19,686 --> 00:33:21,086
And go floating off
into deep space.
686
00:33:22,165 --> 00:33:24,108
In some matches, the fighters
687
00:33:24,133 --> 00:33:25,767
don't even land a punch.
688
00:33:27,767 --> 00:33:30,809
Scientists spot
a supermassive black hole
689
00:33:30,834 --> 00:33:35,567
named B3 1715+425.
690
00:33:36,866 --> 00:33:39,000
This black hole is strange.
691
00:33:40,567 --> 00:33:42,266
Stripped of all its stars,
692
00:33:42,366 --> 00:33:46,809
it hurtles through empty space
at 4.5 million miles an hour.
693
00:33:46,834 --> 00:33:48,967
The first thing
that draws our attention is
694
00:33:49,032 --> 00:33:49,663
this faint trail of debris
across the sky.
695
00:33:49,688 --> 00:33:53,108
This faint trail of debris
across the sky.
696
00:33:53,133 --> 00:33:55,266
There is actually
a trail leading
697
00:33:55,366 --> 00:33:57,099
back to the center of
the galaxy.
698
00:33:57,165 --> 00:33:59,666
It's kind of like a dump truck,
right, that's filled with
699
00:33:59,767 --> 00:34:02,099
dirt driving down the highway,
and the dirt's flying off
700
00:34:02,165 --> 00:34:05,209
behind it...
This is a naked black hole.
701
00:34:05,232 --> 00:34:07,500
The exposed
super massive black hole
702
00:34:07,567 --> 00:34:09,809
has lost its stars and galaxy,
703
00:34:09,833 --> 00:34:14,467
a champion stripped of
its fans and entourage.
704
00:34:14,567 --> 00:34:17,766
So what event is powerful
enough to strip
705
00:34:17,867 --> 00:34:19,663
a supermassive black hole of
its entire host galaxy?
706
00:34:19,686 --> 00:34:22,467
A supermassive black hole of
its entire host galaxy?
707
00:34:22,567 --> 00:34:24,400
That has to be something
really big.
708
00:34:26,967 --> 00:34:29,032
B3 is a smallish galaxy, and it
709
00:34:29,099 --> 00:34:31,208
got into a scrap with a much
bigger one.
710
00:34:31,233 --> 00:34:33,266
The stronger gravity of
the bigger galaxy
711
00:34:33,333 --> 00:34:36,333
stripped the stars away from
that black hole and shot it out.
712
00:34:38,567 --> 00:34:40,166
Typically in the universe,
when something
713
00:34:40,233 --> 00:34:42,108
is bigger and more massive,
it wins.
714
00:34:42,132 --> 00:34:43,867
So this is true for galaxies.
715
00:34:43,967 --> 00:34:46,666
A big galaxy versus
a little galaxy...
716
00:34:46,766 --> 00:34:48,032
Put your money on the big one.
717
00:34:49,567 --> 00:34:49,664
But when two
evenly matched heavyweights
718
00:34:49,688 --> 00:34:52,266
But when two
evenly matched heavyweights
719
00:34:52,367 --> 00:34:53,367
enter the ring,
720
00:34:54,766 --> 00:34:57,367
it's time for the main event.
721
00:34:59,000 --> 00:35:01,500
A clash of the titans.
722
00:35:01,567 --> 00:35:04,099
I grew up watching boxing
with my dad.
723
00:35:04,166 --> 00:35:08,000
So I've always been a boxing
fan, and I love a great battle.
724
00:35:08,065 --> 00:35:10,166
And what's a bigger battle than
725
00:35:10,266 --> 00:35:14,266
a head-on collision between
two supermassive black holes?
726
00:35:14,333 --> 00:35:17,666
If you're a boxing fan,
this is the big one.
727
00:35:17,733 --> 00:35:18,867
We are ready.
728
00:35:18,967 --> 00:35:19,664
We are on the edge of our seats.
729
00:35:19,688 --> 00:35:21,467
We are on the edge of our seats.
730
00:35:21,567 --> 00:35:24,166
We've got two
supermassive black holes,
731
00:35:24,233 --> 00:35:26,967
each one is in their corner,
and they're getting ready for
732
00:35:27,032 --> 00:35:28,333
the fight of the century.
733
00:35:30,666 --> 00:35:33,467
I mean, they're just gonna
go at it like goosh, goosh.
734
00:35:33,567 --> 00:35:36,367
I would watch that.
I'd Pay-Per-View that.
735
00:35:36,467 --> 00:35:37,842
It doesn't get
any better than this.
736
00:35:37,867 --> 00:35:40,967
These are prize fighters
at the top of their game.
737
00:35:41,032 --> 00:35:42,543
They're trained to a T.
738
00:35:42,567 --> 00:35:43,934
They're beefed up.
739
00:35:44,000 --> 00:35:46,400
They are ready to rumble.
740
00:35:46,467 --> 00:35:49,663
We are just seconds away
from the fight of the cosmos.
741
00:35:49,686 --> 00:35:51,806
We are just seconds away
from the fight of the cosmos.
742
00:36:02,867 --> 00:36:05,108
Welcome to
the heavyweight championship
743
00:36:05,132 --> 00:36:06,500
of the universe.
744
00:36:06,567 --> 00:36:09,867
Weighing in at eight billion
solar masses,
745
00:36:09,934 --> 00:36:15,309
We have the galactic
destroyer, M101 star.
746
00:36:15,333 --> 00:36:16,967
And in the other corner,
747
00:36:17,032 --> 00:36:20,567
at a punishing 7.8 billion suns,
748
00:36:20,666 --> 00:36:23,960
the star crusher, NSC47 star.
749
00:36:23,985 --> 00:36:24,867
The star crusher, NSC47 star.
750
00:36:24,967 --> 00:36:28,099
They are pumped
and ready to rumble.
751
00:36:28,166 --> 00:36:31,367
So here it is,
we're finally here.
752
00:36:31,432 --> 00:36:34,032
The crowd is roaring.
753
00:36:34,099 --> 00:36:35,599
The bell has rung,
754
00:36:35,666 --> 00:36:37,867
and the fighters are
approaching each other.
755
00:36:37,934 --> 00:36:39,967
They are ready to go at it.
756
00:36:42,032 --> 00:36:43,766
Let's have
a clean fight, fellas.
757
00:36:43,833 --> 00:36:46,367
Touch hands,
and go back to your corners.
758
00:36:48,065 --> 00:36:51,099
Round one.
The two heavyweights circle,
759
00:36:51,166 --> 00:36:53,443
testing the other's defenses.
760
00:36:53,467 --> 00:36:53,961
The black hole's gonna do what
the boxes are gonna do.
761
00:36:53,985 --> 00:36:55,809
The black hole's gonna do what
the boxes are gonna do.
762
00:36:55,833 --> 00:36:57,467
They're gonna circle each other,
763
00:36:57,567 --> 00:36:59,000
and they're gonna orbit
each other,
764
00:36:59,065 --> 00:37:00,833
and they're gonna
size each other up.
765
00:37:02,567 --> 00:37:04,766
Once these two
supermassive black holes
766
00:37:04,833 --> 00:37:06,567
are close enough, their gravity,
767
00:37:06,666 --> 00:37:08,833
inexorably, is gonna
draw them together.
768
00:37:11,467 --> 00:37:14,443
As the two supermassive
black holes get closer,
769
00:37:14,467 --> 00:37:17,166
they throw a few
exploratory jabs,
770
00:37:20,833 --> 00:37:23,666
triggering bursts of
gravitational waves
771
00:37:23,733 --> 00:37:23,961
that warp everything
in their path.
772
00:37:23,985 --> 00:37:25,599
That warp everything
in their path.
773
00:37:27,065 --> 00:37:30,266
These enormous gravitational
waves are completely
774
00:37:30,367 --> 00:37:33,599
deforming the fabric of
spacetime around them.
775
00:37:33,666 --> 00:37:35,809
Not just a little bit,
but a lot.
776
00:37:35,833 --> 00:37:39,266
It's like feeling
the fighters approach in
777
00:37:39,333 --> 00:37:41,543
the boxing ring...
778
00:37:41,567 --> 00:37:44,367
from the next town over.
779
00:37:48,567 --> 00:37:52,309
Next, the supermassive
black hole's gravity throws in
780
00:37:52,333 --> 00:37:53,967
a couple of right hooks
781
00:37:54,032 --> 00:37:56,333
straight into
the accretion disks.
782
00:37:59,766 --> 00:38:02,367
What could happen is
that they start to form
783
00:38:02,432 --> 00:38:03,599
like an angle grinder.
784
00:38:03,666 --> 00:38:07,065
You'll see sparks flying as
they try to merge and form
785
00:38:07,132 --> 00:38:08,967
a new single accretion disk.
786
00:38:09,032 --> 00:38:11,367
When those accretion
disks collide,
787
00:38:11,467 --> 00:38:16,099
the whole thing is gonna light
up like the Fourth of July.
788
00:38:16,166 --> 00:38:19,766
Spiraling in at millions
of miles an hour,
789
00:38:19,867 --> 00:38:21,934
the heavyweight fighters
get close,
790
00:38:22,000 --> 00:38:23,960
delivering punishing body blows.
791
00:38:23,985 --> 00:38:25,264
Delivering punishing body blows.
792
00:38:28,666 --> 00:38:30,934
The event horizons,
the surface of
793
00:38:31,000 --> 00:38:34,166
the supermassive black holes,
are about to touch.
794
00:38:36,099 --> 00:38:37,409
In their final moments,
795
00:38:37,432 --> 00:38:40,309
these two supermassive black
holes are orbiting each other
796
00:38:40,333 --> 00:38:42,266
at a significant fraction
797
00:38:42,333 --> 00:38:44,666
of the speed of light,
and their event horizons
798
00:38:44,766 --> 00:38:45,766
will touch.
799
00:38:47,599 --> 00:38:49,967
And they'll eventually
merge into one new
800
00:38:50,032 --> 00:38:51,766
supermassive black hole.
801
00:38:51,867 --> 00:38:53,099
You might think,
802
00:38:53,166 --> 00:38:53,961
don't they bump into each
other like bowling balls?
803
00:38:53,985 --> 00:38:55,543
Don't they bump into each
other like bowling balls?
804
00:38:55,567 --> 00:38:56,733
No, they don't.
805
00:38:56,766 --> 00:38:58,710
Because what we're calling
the edge of a black hole is
806
00:38:58,733 --> 00:39:01,599
actually not a thing...
That's just
807
00:39:01,666 --> 00:39:03,500
the surface around
the black hole.
808
00:39:03,567 --> 00:39:06,409
Gravity is so strong
that nothing can come out.
809
00:39:06,432 --> 00:39:10,367
The two supermassive
black holes finally merge,
810
00:39:10,432 --> 00:39:14,367
releasing around 5 percent of
the mass they've gathered over
811
00:39:14,432 --> 00:39:16,367
billions of years in
812
00:39:16,467 --> 00:39:20,710
an enormous burst of
gravitational waves.
813
00:39:20,733 --> 00:39:22,733
The amount of energy
that we're talking about...
814
00:39:24,867 --> 00:39:27,666
there's nothing to compare it
to... it's mind-crushing.
815
00:39:27,766 --> 00:39:30,967
There's really almost no point
in thinking about it.
816
00:39:31,032 --> 00:39:33,367
It's just not something
I think that I can
817
00:39:33,432 --> 00:39:34,599
wrap my head around.
818
00:39:34,666 --> 00:39:36,666
Coming from where I come from,
819
00:39:36,766 --> 00:39:38,500
you know, you don't
show weakness,
820
00:39:38,567 --> 00:39:41,367
so I'm not gonna say that
the collision of two black holes
821
00:39:41,467 --> 00:39:44,166
is more powerful than one of
my punches, but...
822
00:39:45,500 --> 00:39:46,833
it's close.
823
00:39:48,233 --> 00:39:52,166
The gigantic and powerful
gravitational waves race out
824
00:39:52,233 --> 00:39:53,967
from the collision zone,
825
00:39:54,032 --> 00:39:57,766
leaving a single merged
black hole.
826
00:39:57,867 --> 00:40:02,108
The supermassive black hole,
after it merges, permanently
827
00:40:02,132 --> 00:40:05,766
deforms the fabric of spacetime
around it, and this deformation
828
00:40:05,833 --> 00:40:07,867
travels out at
the speed of light.
829
00:40:09,500 --> 00:40:13,367
The surviving 95 percent
of mass from the two colliding
830
00:40:13,467 --> 00:40:15,409
supermassive black holes
831
00:40:15,432 --> 00:40:20,266
is now locked in a single
ultramassive black hole,
832
00:40:20,333 --> 00:40:23,934
the undisputed super
heavyweight champion of
833
00:40:24,000 --> 00:40:26,567
the universe...
At least for now.
834
00:40:27,867 --> 00:40:30,166
It seems the universe is
always upping the ante.
835
00:40:30,233 --> 00:40:32,065
Could there be something
even more
836
00:40:32,132 --> 00:40:33,643
violent we haven't even
discovered yet?
837
00:40:33,666 --> 00:40:36,309
The universe
keeps wanting to give us
838
00:40:36,333 --> 00:40:38,567
something more violent
all the time.
839
00:40:38,666 --> 00:40:43,266
Energy locked in hydrogen
atoms formed at the birth of
840
00:40:43,333 --> 00:40:45,666
the universe is finally
841
00:40:45,766 --> 00:40:49,766
released in the violent
collision and builds
842
00:40:49,867 --> 00:40:51,867
an ultramassive black hole.
843
00:40:54,733 --> 00:40:57,567
This is one of the most
beautiful stories in
844
00:40:57,666 --> 00:41:00,599
our universe... you have
the most energetic collision,
845
00:41:00,666 --> 00:41:02,367
the most amount of
energy released,
846
00:41:02,467 --> 00:41:05,032
the most violent event,
can trace
847
00:41:05,099 --> 00:41:08,266
its origins to the humble
hydrogen atom.
848
00:41:11,132 --> 00:41:14,467
So we have our
champion... matter compressed
849
00:41:14,567 --> 00:41:17,766
and then smashed together
by supermassive black holes
850
00:41:17,833 --> 00:41:21,367
creates the most violent event
in the universe.
851
00:41:22,599 --> 00:41:23,960
I don't think there's a contest.
852
00:41:23,985 --> 00:41:24,367
I don't think there's a contest.
853
00:41:24,432 --> 00:41:26,543
The supermassive
black hole collisions
854
00:41:26,567 --> 00:41:28,208
are the most energetic,
855
00:41:28,233 --> 00:41:32,809
just, like, mind-numbingly
large amounts of energy in
856
00:41:32,833 --> 00:41:33,967
these collisions.
857
00:41:36,867 --> 00:41:39,710
A merger of two supermassive
black holes
858
00:41:39,733 --> 00:41:43,065
is at the absolute top end
extreme of that
859
00:41:43,132 --> 00:41:46,867
for all possible events
in the entire universe,
860
00:41:46,967 --> 00:41:49,867
A supermassive black hole
merger is the most
861
00:41:49,934 --> 00:41:53,000
violent thing that we can
observe in the universe.
67723
Can't find what you're looking for?
Get subtitles in any language from opensubtitles.com, and translate them here.