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1
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The universe was born to die.
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00:00:05,069 --> 00:00:09,472
But how and when
will it all end?
3
00:00:09,473 --> 00:00:11,306
That's the reason
i became a cosmologist.
4
00:00:11,307 --> 00:00:13,043
I wanted to be the first person
that would know
5
00:00:13,044 --> 00:00:15,011
How the universe would end.
6
00:00:15,012 --> 00:00:18,782
Two cosmic heavyweights
wrestle for control.
7
00:00:18,783 --> 00:00:21,283
The winner seals our fate.
8
00:00:21,284 --> 00:00:24,087
The tug of war is gravity,
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00:00:24,088 --> 00:00:25,756
Which is trying
to shrink it down,
10
00:00:25,757 --> 00:00:28,558
And the expansion of space
and time itself.
11
00:00:28,559 --> 00:00:30,893
Will gravity triumph?
12
00:00:30,894 --> 00:00:34,063
The universe will get smaller
and smaller, hotter and hotter.
13
00:00:34,064 --> 00:00:37,066
Or will expansion
get the upper hand?
14
00:00:37,067 --> 00:00:41,038
Even the electrons around
your atoms will be ripped apart.
15
00:00:41,039 --> 00:00:42,505
The end is coming,
16
00:00:42,506 --> 00:00:46,043
And it could be
sooner than you think.
17
00:00:59,425 --> 00:01:02,494
The universe is everything
18
00:01:02,495 --> 00:01:06,198
All space, all time, all matter.
19
00:01:08,467 --> 00:01:11,436
The earth is a speck
by comparison,
20
00:01:11,437 --> 00:01:16,007
A grain of rock orbiting just
one of the 200 billion stars
21
00:01:16,008 --> 00:01:19,079
In our home galaxy,
the milky way.
22
00:01:22,381 --> 00:01:26,184
In turn, this enormous structure
is just a drop
23
00:01:26,185 --> 00:01:28,787
In an ocean of galaxies
that stretch
24
00:01:28,788 --> 00:01:31,324
For 90 billion light years.
25
00:01:33,425 --> 00:01:35,526
And all of this,
26
00:01:35,527 --> 00:01:39,698
From the biggest galaxy
to the smallest atom,
27
00:01:39,699 --> 00:01:41,902
Will one day die.
28
00:01:43,737 --> 00:01:46,138
We don't see evidence
of anything being eternal.
29
00:01:46,139 --> 00:01:47,838
Eternity doesn't exist.
30
00:01:47,839 --> 00:01:50,109
Even space and time
will come to an end.
31
00:01:51,445 --> 00:01:55,381
The universe has been
expanding since its birth,
32
00:01:55,382 --> 00:01:59,551
Gradually burning through
the fuel that lights its stars.
33
00:01:59,552 --> 00:02:02,554
But what happens
when the fuel runs out?
34
00:02:02,555 --> 00:02:05,056
Will it all just fade away?
35
00:02:05,057 --> 00:02:07,460
Stars die out,
use up their nuclear fuel.
36
00:02:07,461 --> 00:02:10,063
We have an empty, cold,
desolate universe.
37
00:02:10,064 --> 00:02:12,132
Just dead remnants of stars --
38
00:02:12,133 --> 00:02:14,234
Black holes, neutron stars.
39
00:02:14,235 --> 00:02:15,768
Eventually, they decay away,
40
00:02:15,769 --> 00:02:18,704
And you're left with a thin haze
of very low energy light.
41
00:02:18,705 --> 00:02:20,039
That's it.
42
00:02:20,040 --> 00:02:21,806
We used to think the universe
43
00:02:21,807 --> 00:02:24,577
Would cruise gently
into old age.
44
00:02:24,578 --> 00:02:26,679
But over the past few decades,
45
00:02:26,680 --> 00:02:30,149
Astronomers have
revealed a very different
46
00:02:30,150 --> 00:02:31,918
And disturbing picture.
47
00:02:31,919 --> 00:02:34,853
The universe isn't cruising.
48
00:02:34,854 --> 00:02:36,688
It's fighting for its life.
49
00:02:36,689 --> 00:02:38,958
It may seem peaceful here
on earth on a nice, sunny day,
50
00:02:38,959 --> 00:02:40,793
But in fact, above us
and all around us,
51
00:02:40,794 --> 00:02:43,929
Throughout the universe,
a battle is raging,
52
00:02:43,930 --> 00:02:45,967
And it has raged
since the beginning of time.
53
00:02:46,835 --> 00:02:50,404
Two deadly forces
grapple for control.
54
00:02:50,405 --> 00:02:54,941
The first, expansion,
pulls galaxies apart,
55
00:02:54,942 --> 00:02:57,977
Cooling the universe
and threatening it
56
00:02:57,978 --> 00:03:01,048
With a frozen extinction.
57
00:03:01,049 --> 00:03:05,585
The second, gravity, tries to
crush everything back together,
58
00:03:05,586 --> 00:03:09,424
Annihilating the universe
in a dense ball of fire.
59
00:03:11,992 --> 00:03:15,596
Will gravity or expansion win?
60
00:03:15,597 --> 00:03:17,631
Or will it end in a tie?
61
00:03:17,632 --> 00:03:21,437
These two colossal forces
yield three endgames.
62
00:03:22,037 --> 00:03:24,104
One is the big freeze.
63
00:03:24,105 --> 00:03:27,073
Expansion wins, and the universe
just expands forever.
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00:03:27,074 --> 00:03:29,676
The second is that there is
a delicate balance
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00:03:29,677 --> 00:03:30,944
Between the expansion
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00:03:30,945 --> 00:03:32,614
And the amount of gravitational
attraction,
67
00:03:32,615 --> 00:03:34,715
And the universe gets
to a particular size,
68
00:03:34,716 --> 00:03:36,184
And it pretty much stays there.
69
00:03:36,185 --> 00:03:37,853
And the third outcome is that
70
00:03:37,854 --> 00:03:39,688
The gravitational
attraction wins,
71
00:03:39,689 --> 00:03:41,322
And the expansion stops,
72
00:03:41,323 --> 00:03:43,057
And the universe
begins to get smaller
73
00:03:43,058 --> 00:03:46,228
Until, eventually,
it goes back to a big crunch.
74
00:03:48,431 --> 00:03:50,765
So far,
the universe seems balanced
75
00:03:50,766 --> 00:03:54,703
On a tightrope between
expansion and contraction.
76
00:03:54,704 --> 00:03:58,107
But will it keep its equilibrium
until it runs out of steam,
77
00:03:58,108 --> 00:04:00,911
Or will something
tip the balance?
78
00:04:02,946 --> 00:04:05,882
I don't think there's
any bigger question than,
79
00:04:05,883 --> 00:04:08,116
Where is the universe going?
80
00:04:08,117 --> 00:04:11,654
To predict the future,
cosmologists have always looked
81
00:04:11,655 --> 00:04:15,858
To the past, back to
the beginning of expansion,
82
00:04:15,859 --> 00:04:20,631
The beginning of gravity,
the beginning of everything.
83
00:04:23,232 --> 00:04:28,202
13.8 billion years ago,
an infinitely dense,
84
00:04:28,203 --> 00:04:32,908
Hot speck ignites
and suddenly expands outward --
85
00:04:32,909 --> 00:04:34,912
The big bang.
86
00:04:36,446 --> 00:04:40,016
All energy, all space,
and all matter...
87
00:04:41,751 --> 00:04:44,786
...the building blocks of
the universe we see today,
88
00:04:44,787 --> 00:04:47,258
Are created and set in motion.
89
00:04:48,259 --> 00:04:50,494
Think of it.
90
00:04:50,495 --> 00:04:52,797
Everything you see around us
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00:04:52,798 --> 00:04:57,434
Concentrated into a primordial
fireball that exploded,
92
00:04:57,435 --> 00:05:00,238
Sending all the galaxies
into motion.
93
00:05:04,309 --> 00:05:07,977
That outward blast,
the birth of expansion,
94
00:05:07,978 --> 00:05:10,647
Is still going on today.
95
00:05:10,648 --> 00:05:14,051
Without it, we wouldn't have
a universe big enough
96
00:05:14,052 --> 00:05:16,854
For stars
and galaxies to exist in.
97
00:05:16,855 --> 00:05:20,123
Expansion is an astonishing
force of nature.
98
00:05:20,124 --> 00:05:24,427
It works by inflating
the fabric of space-Time.
99
00:05:24,428 --> 00:05:28,099
Space between galaxies expands,
100
00:05:28,100 --> 00:05:30,402
And it pushes
the galaxies apart.
101
00:05:30,403 --> 00:05:35,506
Space carries objects with it
like a surfer on a wave.
102
00:05:35,507 --> 00:05:37,909
It's going on
in every part of space.
103
00:05:37,910 --> 00:05:39,578
Even inside your body right now,
104
00:05:39,579 --> 00:05:41,513
There's a pressure
for space to expand.
105
00:05:42,380 --> 00:05:45,417
Expansion generated
the vast, moving stage
106
00:05:45,418 --> 00:05:48,052
On which today's universe
plays out.
107
00:05:48,053 --> 00:05:50,956
But left unchecked,
it could have been a force
108
00:05:50,957 --> 00:05:53,090
For utter annihilation.
109
00:05:53,091 --> 00:05:55,326
If the universe had
been expanding much faster,
110
00:05:55,327 --> 00:05:57,095
It would have emptied out
so fast,
111
00:05:57,096 --> 00:05:59,364
You wouldn't have had time
to make galaxies,
112
00:05:59,365 --> 00:06:00,500
Planets, people.
113
00:06:03,168 --> 00:06:04,770
The fact
that we're here
114
00:06:04,771 --> 00:06:07,340
Means that something must have
put on the brakes.
115
00:06:07,341 --> 00:06:11,943
It was, of course,
our universal glue -- Gravity.
116
00:06:11,944 --> 00:06:15,413
Gravity and matter
go hand in hand.
117
00:06:15,414 --> 00:06:18,316
The more massive the object,
118
00:06:18,317 --> 00:06:21,419
The more pull it exerts
on everything around it.
119
00:06:21,420 --> 00:06:27,026
It draws atom to atom,
particle to particle...
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00:06:27,728 --> 00:06:33,032
...building stars, nebulas,
121
00:06:33,033 --> 00:06:35,368
Galaxies --
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00:06:35,369 --> 00:06:39,506
The hardware of the universe
we see today.
123
00:06:39,507 --> 00:06:42,340
But gravity
is a double-Edged sword.
124
00:06:42,341 --> 00:06:45,244
Too much, and the early universe
would never have gotten
125
00:06:45,245 --> 00:06:47,412
Out of the starting blocks.
126
00:06:47,413 --> 00:06:49,448
If it had been
expanding more slowly,
127
00:06:49,449 --> 00:06:51,717
It would have re-Collapsed
into another singularity.
128
00:06:51,718 --> 00:06:54,486
And again, you wouldn't have had
the time to make galaxies,
129
00:06:54,487 --> 00:06:56,289
Planets, or people.
130
00:06:56,290 --> 00:06:57,924
So we live in the goldilocks
universe.
131
00:06:57,925 --> 00:07:00,059
We live in the universe
that lasts long enough
132
00:07:00,060 --> 00:07:02,561
That we can be here,
but expands gently enough
133
00:07:02,562 --> 00:07:04,497
That we have time to form.
134
00:07:07,267 --> 00:07:11,069
The universe has
lasted for 13.8 billion years,
135
00:07:11,070 --> 00:07:15,042
Thanks to the opposing forces
of gravity and expansion.
136
00:07:15,043 --> 00:07:19,112
But just how stable
is this balancing act?
137
00:07:19,113 --> 00:07:22,615
Does our universe have just
the right amount of stuff in it
138
00:07:22,616 --> 00:07:24,716
To keep it from
runaway expansion
139
00:07:24,717 --> 00:07:26,787
Or catastrophic collapse?
140
00:07:27,388 --> 00:07:30,257
In the 1920s,
scientists did the math,
141
00:07:30,258 --> 00:07:34,094
And the results were
anything but reassuring.
142
00:07:34,095 --> 00:07:37,331
The more matter you have,
the more gravity you have.
143
00:07:37,332 --> 00:07:40,668
If you have lots of matter
in a very dense universe,
144
00:07:40,669 --> 00:07:43,738
Perhaps the universe
begins to re-Collapse.
145
00:07:43,739 --> 00:07:45,839
Or, if you have
very little matter,
146
00:07:45,840 --> 00:07:48,209
The universe would
freeze to death.
147
00:07:48,210 --> 00:07:52,379
So what is the critical density,
the border between the two?
148
00:07:52,380 --> 00:07:56,916
It's approximately five hydrogen
atoms per cubic meter.
149
00:07:56,917 --> 00:08:02,322
So think of a cubic yard,
and put just five hydrogen atoms
150
00:08:02,323 --> 00:08:05,159
Inside,
and that is the tipping point.
151
00:08:05,160 --> 00:08:07,293
If you put more than five atoms,
152
00:08:07,294 --> 00:08:09,296
Then the universe will
begin to collapse.
153
00:08:09,297 --> 00:08:10,831
If you have
less than five atoms,
154
00:08:10,832 --> 00:08:12,434
Then the universe
just keeps on going.
155
00:08:13,435 --> 00:08:15,635
If we thought
the universe was balanced
156
00:08:15,636 --> 00:08:18,806
On a tightrope before,
the critical density question
157
00:08:18,807 --> 00:08:23,079
Showed us that the rope
was more like a razor blade.
158
00:08:23,446 --> 00:08:26,382
Yet, when astronomers took
additional measurements,
159
00:08:26,383 --> 00:08:28,816
They liked what they saw.
160
00:08:28,817 --> 00:08:32,220
The universe appeared to contain
just the right amount
161
00:08:32,221 --> 00:08:35,158
Of matter to stay
at the critical density.
162
00:08:36,293 --> 00:08:38,393
More and more,
the indirect evidence
163
00:08:38,394 --> 00:08:41,229
And the theoretical
arguments suggested
164
00:08:41,230 --> 00:08:43,932
That the universe must be
exactly at the boundary
165
00:08:43,933 --> 00:08:45,768
Between a universe
that would collapse
166
00:08:45,769 --> 00:08:48,070
And one that
would expand forever,
167
00:08:48,071 --> 00:08:51,706
That we were teetering
on the hairy edge of expansion.
168
00:08:51,707 --> 00:08:55,978
The universe seemed
so perfectly balanced
169
00:08:55,979 --> 00:08:59,880
That it would head quietly
into old age.
170
00:08:59,881 --> 00:09:03,418
Then, in the 1970s, astronomers
made an observation
171
00:09:03,419 --> 00:09:05,421
That shocked them.
172
00:09:05,422 --> 00:09:09,325
The cosmos was filled
with invisible stuff,
173
00:09:09,326 --> 00:09:14,031
And its gravity could cause
a catastrophic collapse.
174
00:09:24,443 --> 00:09:27,578
The universe
is balanced on a tightrope.
175
00:09:27,579 --> 00:09:31,715
On each side of the drop
lies an early death --
176
00:09:31,716 --> 00:09:35,454
A big freeze, fueled by
the runaway stretching of space,
177
00:09:35,455 --> 00:09:41,358
Or a big crunch, the result of
gravity overcoming expansion.
178
00:09:41,359 --> 00:09:44,828
40 years ago, scientists
believed we'd stay balanced
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00:09:44,829 --> 00:09:48,399
Between these fates
for eternity.
180
00:09:48,400 --> 00:09:50,635
Now things have changed
tremendously,
181
00:09:50,636 --> 00:09:53,371
Because we've discovered
something we never knew about
182
00:09:53,372 --> 00:09:54,172
40 years ago.
183
00:09:54,773 --> 00:09:59,444
In the 1970s,
astronomers are stunned.
184
00:09:59,445 --> 00:10:03,147
Some unknown form of matter,
invisible to telescopes,
185
00:10:03,148 --> 00:10:05,849
Dwarfs what we thought was
out there,
186
00:10:05,850 --> 00:10:09,621
Not a fraction more,
but five times more.
187
00:10:09,622 --> 00:10:12,790
We used to think
that gravity came from stars
188
00:10:12,791 --> 00:10:15,794
And objects you can see --
End of story.
189
00:10:15,795 --> 00:10:19,165
Now, we realize that that naive
picture is actually wrong.
190
00:10:20,200 --> 00:10:22,501
Astronomers make
the discovery,
191
00:10:22,502 --> 00:10:25,873
Studying the clockwork
nature of our universe.
192
00:10:27,275 --> 00:10:29,942
The huge gravity of the sun
holds the earth
193
00:10:29,943 --> 00:10:34,082
And all the other planets
in a delicate circular dance.
194
00:10:37,951 --> 00:10:41,487
The sun's mass controls
the speed of these orbits.
195
00:10:41,488 --> 00:10:44,657
If it were more massive,
the planets would orbit
196
00:10:44,658 --> 00:10:46,325
Much more quickly.
197
00:10:46,326 --> 00:10:48,895
And if it were smaller,
it would take much longer
198
00:10:48,896 --> 00:10:51,532
For a planet to complete
an orbit.
199
00:10:53,733 --> 00:10:57,002
Galaxies run
like clockwork, too.
200
00:10:57,003 --> 00:11:00,272
The vast mass at the center
pulls the outer stars
201
00:11:00,273 --> 00:11:03,676
Into circular,
planet-Like orbits.
202
00:11:03,677 --> 00:11:06,179
Astronomers make
precise measurements
203
00:11:06,180 --> 00:11:09,848
Of these galactic
orbits in the 1970s.
204
00:11:09,849 --> 00:11:13,021
The results change everything.
205
00:11:13,922 --> 00:11:16,489
The galaxies
were spinning too fast.
206
00:11:16,490 --> 00:11:18,025
Way too fast.
207
00:11:21,096 --> 00:11:23,965
Even accounting for
the supermassive black holes
208
00:11:23,966 --> 00:11:28,268
At their center, nine-Tenths
of their mass was missing.
209
00:11:28,269 --> 00:11:31,105
By rights,
the galaxy should fly apart.
210
00:11:31,106 --> 00:11:33,274
By rights, the earth
should have been flung
211
00:11:33,275 --> 00:11:36,244
Into intergalactic space
billions of years ago.
212
00:11:36,245 --> 00:11:39,446
We should have no
milky way galaxy, and yet,
213
00:11:39,447 --> 00:11:41,183
Our universe is
full of galaxies.
214
00:11:45,253 --> 00:11:48,188
An immense
additional source of gravity
215
00:11:48,189 --> 00:11:51,091
Must be holding galaxies
together.
216
00:11:51,092 --> 00:11:54,327
But no matter where astronomers
point their telescopes,
217
00:11:54,328 --> 00:11:56,264
They see nothing.
218
00:11:56,265 --> 00:11:59,799
Not a glimmer, not a shadow.
219
00:11:59,800 --> 00:12:04,672
Whatever this new stuff is,
it doesn't emit light,
220
00:12:04,673 --> 00:12:08,308
Reflect light,
or even block light.
221
00:12:08,309 --> 00:12:11,213
They call it dark matter.
222
00:12:11,246 --> 00:12:14,584
What we've learned is that most
of the matter in the universe
223
00:12:14,585 --> 00:12:17,220
Is not ordinary stuff.
It's not atoms.
224
00:12:17,221 --> 00:12:20,022
It's not particles we've yet
detected in any experiment
225
00:12:20,023 --> 00:12:21,724
Done here on earth.
226
00:12:21,725 --> 00:12:24,360
It's some new kind of particle
that we call the dark matter.
227
00:12:27,496 --> 00:12:29,398
Dark matter fills the universe,
228
00:12:29,399 --> 00:12:32,502
Outstripping normal matter
by 5-To-1.
229
00:12:36,105 --> 00:12:40,609
Vast filaments spread out
throughout the cosmos,
230
00:12:40,610 --> 00:12:45,081
And bright galaxies cluster
where dark matter is thickest.
231
00:12:47,417 --> 00:12:51,753
Dark matter provides
the scaffolding that underlies
232
00:12:51,754 --> 00:12:54,623
How the matter in the universe
structures itself,
233
00:12:54,624 --> 00:12:56,527
Where it goes,
and what it does.
234
00:12:57,394 --> 00:12:59,329
So,
dark matter dictated
235
00:12:59,330 --> 00:13:02,896
How the universe unfolded.
236
00:13:02,897 --> 00:13:05,035
It seems as if
out of the hot big bang,
237
00:13:05,036 --> 00:13:08,671
Dark matter condensed first,
before atoms,
238
00:13:08,672 --> 00:13:11,641
And dark matter began
to become clumpy.
239
00:13:11,642 --> 00:13:14,844
The clumpiness then began
to attract atoms
240
00:13:14,845 --> 00:13:18,547
As they were formed later,
and that formed galaxies.
241
00:13:18,548 --> 00:13:20,584
And in some sense,
the dark matter therefore
242
00:13:20,585 --> 00:13:24,189
Provides kind of a womb that
allows the birth of our galaxy.
243
00:13:27,425 --> 00:13:30,594
Dark matter holds
the universe together,
244
00:13:30,595 --> 00:13:33,064
But it also threatens
to destroy it.
245
00:13:35,897 --> 00:13:36,598
One of the most
amazing discoveries
246
00:13:36,599 --> 00:13:39,036
Of the past few decades
is dark matter,
247
00:13:39,037 --> 00:13:41,002
The fact that there's much more
matter in the universe
248
00:13:41,003 --> 00:13:42,472
Than we were aware of.
249
00:13:42,473 --> 00:13:44,976
And all of that matter
has a lot of gravity.
250
00:13:44,977 --> 00:13:47,109
So all this new matter,
all this new gravity
251
00:13:47,110 --> 00:13:49,513
Must be slowing down
the expansion of the universe.
252
00:13:50,281 --> 00:13:53,217
Dark matter may even
tip the cosmic scales
253
00:13:53,218 --> 00:13:55,218
In favor of gravity,
254
00:13:55,219 --> 00:13:58,988
Defeating expansion
and pulling the entire universe
255
00:13:58,989 --> 00:14:01,593
Towards a death by fire.
256
00:14:01,594 --> 00:14:04,395
It's called the big crunch,
257
00:14:04,396 --> 00:14:06,765
And this is how
it would play out.
258
00:14:08,467 --> 00:14:12,803
For a fraction of a second,
the universe stalls,
259
00:14:12,804 --> 00:14:16,540
Poised between
expansion and contraction.
260
00:14:16,541 --> 00:14:20,644
Then, gravity kicks off
a cataclysm.
261
00:14:20,645 --> 00:14:23,113
When you looked out,
the very first things
262
00:14:23,114 --> 00:14:25,049
As it began to turn around
that you began to see
263
00:14:25,050 --> 00:14:27,684
Is that galaxies, instead of
moving away from us on average,
264
00:14:27,685 --> 00:14:30,189
Would begin to be moving towards
us on average.
265
00:14:31,323 --> 00:14:34,294
The whole universe would look
like it was coming to get us.
266
00:14:36,096 --> 00:14:38,697
As space
contracts further,
267
00:14:38,698 --> 00:14:42,533
The density of matter increases,
gravity gets stronger,
268
00:14:42,534 --> 00:14:47,706
Temperatures soar
as the crunch gathers momentum.
269
00:14:47,707 --> 00:14:50,042
Galaxies begin to collide,
270
00:14:50,043 --> 00:14:53,012
Gas clouds begin to collide,
271
00:14:53,013 --> 00:14:56,116
Planets slam into the earth.
272
00:14:59,885 --> 00:15:03,455
Black holes will execute a death
dance around each other.
273
00:15:03,456 --> 00:15:06,892
Temperatures, of course,
will continue to skyrocket.
274
00:15:06,893 --> 00:15:10,730
Matter, space,
and time implode
275
00:15:10,731 --> 00:15:13,664
Until everything in the universe
is compressed
276
00:15:13,665 --> 00:15:19,504
Into a tiny speck of infinite
mass, heat, and pressure.
277
00:15:19,505 --> 00:15:22,273
For the last stages
of the big crunch,
278
00:15:22,274 --> 00:15:25,476
Galaxies will collide
and form a primordial atom.
279
00:15:25,477 --> 00:15:29,849
And then, life as we know it
will be impossible.
280
00:15:29,850 --> 00:15:32,283
We're back
to where it all began,
281
00:15:32,284 --> 00:15:33,421
Back at the big bang.
282
00:15:34,222 --> 00:15:37,959
The universe that we live in
will cease to exist.
283
00:15:41,528 --> 00:15:47,266
But some believe a big crunch
could herald a new beginning.
284
00:15:47,267 --> 00:15:49,602
We don't know what the end point
of a big crunch would be,
285
00:15:49,603 --> 00:15:52,338
Because the laws of physics
break down.
286
00:15:52,339 --> 00:15:55,809
It's possible, and indeed,
philosophically very pleasant,
287
00:15:55,810 --> 00:16:00,045
To imagine that that crunch
would somehow end up evolving
288
00:16:00,046 --> 00:16:03,348
Into an expansion again, and you
could have a cyclic universe
289
00:16:03,349 --> 00:16:04,883
Which goes on forever.
290
00:16:04,884 --> 00:16:08,623
Perhaps at that point, we will
recreate another big bang.
291
00:16:12,560 --> 00:16:14,928
It's conceivable that as
everything comes together
292
00:16:14,929 --> 00:16:18,463
In the crunch, something sort of
keeps it from just continuing
293
00:16:18,464 --> 00:16:22,135
And pushes out in a hot,
dense, smooth state,
294
00:16:22,136 --> 00:16:24,838
And from the other side,
it looks like a big bang,
295
00:16:24,839 --> 00:16:26,573
And a new universe has been
created.
296
00:16:26,574 --> 00:16:29,442
Our big bang might have been
someone else's big crunch.
297
00:16:29,443 --> 00:16:31,745
But just when
scientists came to terms
298
00:16:31,746 --> 00:16:35,216
With dark matter's big crunch,
the universe threw them
299
00:16:35,217 --> 00:16:37,618
Another, even bigger curve.
300
00:16:37,619 --> 00:16:42,156
Some ghostly force seemed to be
sending us hurtling toward
301
00:16:42,157 --> 00:16:44,257
A completely different death.
302
00:16:44,258 --> 00:16:47,061
My postdoctoral
scholar showed me the results.
303
00:16:47,062 --> 00:16:48,230
I nearly fell off my chair.
304
00:16:58,374 --> 00:17:00,710
Gravity and expansion
battle for control
305
00:17:00,711 --> 00:17:04,181
Of our universe
for 14 billion years...
306
00:17:08,352 --> 00:17:12,787
...expansion
pushing it outwards,
307
00:17:12,788 --> 00:17:15,393
Gravity pulling it in.
308
00:17:16,894 --> 00:17:18,995
With dark matter in its corner,
309
00:17:18,996 --> 00:17:21,497
Gravity seems to be
the inevitable winner.
310
00:17:21,498 --> 00:17:26,068
The extra mass will drag
the universe into a big crunch,
311
00:17:26,069 --> 00:17:28,104
Until a stunning discovery
312
00:17:28,105 --> 00:17:32,610
Revolutionizes our understanding
of the universe.
313
00:17:34,944 --> 00:17:39,883
Around 1990, two teams of
researchers decided to measure
314
00:17:39,884 --> 00:17:41,950
The expansion history
of the universe
315
00:17:41,951 --> 00:17:45,054
To determine whether
it's been slowing down so much
316
00:17:45,055 --> 00:17:47,291
That it'll eventually have
a big crunch,
317
00:17:47,292 --> 00:17:49,825
Or whether it hasn't been
slowing down much
318
00:17:49,826 --> 00:17:51,795
And will eternally expand.
319
00:17:51,796 --> 00:17:56,298
Astronomer alex filippenko
was on one team.
320
00:17:56,299 --> 00:17:58,901
Saul perlmutter led the other.
321
00:17:58,902 --> 00:18:01,938
We realized that it was possible
for the first time
322
00:18:01,939 --> 00:18:05,608
To go and actually make
a direct measurement
323
00:18:05,609 --> 00:18:08,111
Of how much the universe had
been slowing down in the past.
324
00:18:08,313 --> 00:18:09,847
Both teams want
to measure
325
00:18:09,848 --> 00:18:12,148
The speed of distant galaxies.
326
00:18:12,149 --> 00:18:16,020
But because the galaxies are
too dim and too far away,
327
00:18:16,021 --> 00:18:18,057
They look for something
brighter.
328
00:18:22,961 --> 00:18:27,431
Billions of light years
from earth, a star detonates.
329
00:18:27,432 --> 00:18:30,100
This is a supernova,
330
00:18:30,101 --> 00:18:34,105
A dying star's
brilliant final gasp.
331
00:18:34,106 --> 00:18:38,041
It burns brightly, 5 billion
times brighter than the sun,
332
00:18:38,042 --> 00:18:40,712
But briefly.
333
00:18:40,713 --> 00:18:42,879
Perlmutter and filippenko
have a window
334
00:18:42,880 --> 00:18:45,448
Of just one or two weeks
to measure
335
00:18:45,449 --> 00:18:48,752
How much the galaxy it sits in
is slowing down
336
00:18:48,753 --> 00:18:51,023
As it moves away from us.
337
00:18:55,128 --> 00:18:58,364
The teams look for supernovas
for eight years.
338
00:18:58,365 --> 00:19:04,170
They measure 42, and the results
seem impossible.
339
00:19:04,171 --> 00:19:06,771
We plotted the points
on the graphs,
340
00:19:06,772 --> 00:19:09,508
And...it didn't make any sense.
341
00:19:09,509 --> 00:19:11,376
They were not slowing down
at all.
342
00:19:11,377 --> 00:19:13,313
They were actually speeding up.
343
00:19:14,480 --> 00:19:18,084
What both groups found
stunned the world.
344
00:19:18,085 --> 00:19:20,920
In the last 4 or 5 billion
years,
345
00:19:20,921 --> 00:19:25,089
The universe has actually been
speeding up in its expansion.
346
00:19:25,090 --> 00:19:26,925
An accelerating universe,
347
00:19:26,926 --> 00:19:30,896
Propelled by something
mysterious.
348
00:19:30,897 --> 00:19:33,365
For so long, we've been arguing
whether the universe would
349
00:19:33,366 --> 00:19:36,201
Expand forever or collapse
back in on itself,
350
00:19:36,202 --> 00:19:38,570
But nobody thought
the answer was going to be
351
00:19:38,571 --> 00:19:40,873
That the universe was
accelerating,
352
00:19:40,874 --> 00:19:42,675
Going faster and faster
all the time.
353
00:19:44,245 --> 00:19:47,615
The acceleration
bewilders the scientists.
354
00:19:47,616 --> 00:19:50,718
It seems to defy
the laws of physics.
355
00:19:50,719 --> 00:19:52,987
Imagine i've got a baseball
356
00:19:52,988 --> 00:19:54,654
And i throw it straight up.
357
00:19:54,655 --> 00:19:57,458
And instead of slowing down
once it leaves my hand,
358
00:19:57,459 --> 00:19:59,292
Which is what
normally it will do,
359
00:19:59,293 --> 00:20:01,161
It begins to slow down at first,
360
00:20:01,162 --> 00:20:03,064
But then it starts
speeding away.
361
00:20:03,065 --> 00:20:04,699
Somehow, it's getting energy.
362
00:20:04,700 --> 00:20:10,170
The new energy seemed
to be coming from nothing,
363
00:20:10,171 --> 00:20:12,405
The vacuum of space.
364
00:20:12,406 --> 00:20:16,176
The word "vacuum" to a scientist
means completely empty space,
365
00:20:16,177 --> 00:20:18,778
No particles there at all,
no temperature,
366
00:20:18,779 --> 00:20:20,379
No energy to speak of.
367
00:20:20,380 --> 00:20:23,683
But there's an intrinsic energy
in space and time.
368
00:20:23,684 --> 00:20:27,386
Empty space has energy,
and that energy produces
369
00:20:27,387 --> 00:20:30,523
A gravitational repulsion,
a kind of anti-Gravity.
370
00:20:30,524 --> 00:20:34,962
Without a clue what
this force is or how it works,
371
00:20:34,963 --> 00:20:40,534
All scientists can do is give it
a name -- Dark energy.
372
00:20:40,903 --> 00:20:43,304
We could have called it
we-Don't-Know energy.
373
00:20:43,305 --> 00:20:44,773
We could have called it
anything.
374
00:20:44,774 --> 00:20:47,176
But we don't know what it is,
and dark or not,
375
00:20:47,177 --> 00:20:49,311
It's the biggest mystery
in physics.
376
00:20:52,480 --> 00:20:55,516
Nasa calibrates
its finest space telescopes
377
00:20:55,517 --> 00:20:58,652
To measure how much dark energy
is out there,
378
00:20:58,653 --> 00:21:01,989
And the result is mind-Blowing.
379
00:21:01,990 --> 00:21:06,795
It dominates the mass of
the universe by nearly 3-To-1.
380
00:21:06,796 --> 00:21:08,462
And the more space expands,
381
00:21:08,463 --> 00:21:11,632
The more dark energy
there seems to be.
382
00:21:11,633 --> 00:21:14,568
Dark energy is the energy
of nothing,
383
00:21:14,569 --> 00:21:16,104
And it's repulsive.
384
00:21:16,105 --> 00:21:19,908
Therefore, as this dark energy
repels galaxies,
385
00:21:19,909 --> 00:21:21,843
There's more of it,
there's more vacuum.
386
00:21:21,844 --> 00:21:23,946
And so there's more repulsion,
387
00:21:23,947 --> 00:21:26,881
And perhaps that's the reason
why the universe is accelerating
388
00:21:26,882 --> 00:21:30,218
Right now
rather than slowing down.
389
00:21:30,219 --> 00:21:33,689
Dark energy seems to
kill the big crunch theory,
390
00:21:33,690 --> 00:21:36,757
But scientists aren't yet sure
how dark energy,
391
00:21:36,758 --> 00:21:40,295
Expansion, and space
are connected.
392
00:21:40,296 --> 00:21:43,631
If a volume of space doubles
in size,
393
00:21:43,632 --> 00:21:46,534
Does the dark energy
inside it double, too?
394
00:21:46,535 --> 00:21:48,637
Or does it increase more?
395
00:21:48,638 --> 00:21:52,173
A 1-To-1 relationship leads
to a steady expansion.
396
00:21:52,174 --> 00:21:55,310
The universe ends
in a big freeze.
397
00:21:55,311 --> 00:21:59,881
But if dark energy increases
above and beyond expansion,
398
00:21:59,882 --> 00:22:04,455
A new, even more terrifying end
awaits the universe -- A big rip.
399
00:22:05,256 --> 00:22:09,291
In a big rip scenario,
the expansion is so great
400
00:22:09,292 --> 00:22:13,496
That even the galaxies begin
to expand internally,
401
00:22:13,497 --> 00:22:14,831
Which means that literally
402
00:22:14,832 --> 00:22:16,768
Our bodies
are going to be ripped apart.
403
00:22:18,067 --> 00:22:19,568
Scientists calculate
404
00:22:19,569 --> 00:22:21,905
Just how the big rip
will play out.
405
00:22:24,240 --> 00:22:28,310
One by one, the galaxies in
the night sky will blink out
406
00:22:28,311 --> 00:22:31,279
As space pulls them away
from the earth
407
00:22:31,280 --> 00:22:33,082
Faster than the speed of light.
408
00:22:34,786 --> 00:22:39,189
60 million years before the end,
dark energy overcomes gravity
409
00:22:39,190 --> 00:22:42,124
On smaller and smaller scales.
410
00:22:42,125 --> 00:22:45,428
First galaxies start
to rip apart,
411
00:22:45,429 --> 00:22:49,298
Then insides of galaxies
will begin to rip apart,
412
00:22:49,299 --> 00:22:51,969
And then solar systems will
begin to rip apart...
413
00:22:54,239 --> 00:22:57,208
then planets...
414
00:22:57,209 --> 00:23:02,614
and then rocks, people, atoms.
415
00:23:02,615 --> 00:23:05,918
The end will
be mercifully quick.
416
00:23:07,219 --> 00:23:09,487
In the space of a few minutes,
417
00:23:09,488 --> 00:23:13,658
All the stars and planets in the
universe will be destroyed,
418
00:23:13,659 --> 00:23:18,429
Their remains pulled apart
into ever-Smaller pieces
419
00:23:18,430 --> 00:23:21,099
Until finally,
when the universe has
420
00:23:21,100 --> 00:23:22,833
Less than a second to live,
421
00:23:22,834 --> 00:23:26,304
The subatomic particles
that made all matter
422
00:23:26,305 --> 00:23:27,971
Will be destroyed,
423
00:23:27,972 --> 00:23:31,275
And all that remains will be
individual photons
424
00:23:31,276 --> 00:23:33,577
Becoming scarcer and scarcer
425
00:23:33,578 --> 00:23:36,314
As the space between them
expands.
426
00:23:36,315 --> 00:23:38,783
All you're left with is very low
energy light
427
00:23:38,784 --> 00:23:40,252
That gets stretched
and stretched
428
00:23:40,253 --> 00:23:42,354
Until it might as well
not exist at all.
429
00:23:42,355 --> 00:23:44,354
The last thing to go --
430
00:23:44,355 --> 00:23:47,859
The empty vacuum
of space itself.
431
00:23:49,396 --> 00:23:51,897
It'll be pulling on the universe
so hard,
432
00:23:51,898 --> 00:23:54,800
It could tear the fabric
of the universe apart.
433
00:23:54,801 --> 00:23:58,203
Reality could dissolve.
434
00:23:58,204 --> 00:24:01,540
Will the universe end
with a big rip,
435
00:24:01,541 --> 00:24:03,875
Or a big freeze?
436
00:24:03,876 --> 00:24:08,347
The answer is locked inside
the mystery of dark energy.
437
00:24:08,348 --> 00:24:13,119
Solve that, and the fate
of the universe becomes clear.
438
00:24:26,000 --> 00:24:28,366
The end
of the universe is coming.
439
00:24:28,367 --> 00:24:30,537
But how will it play out?
440
00:24:30,538 --> 00:24:34,406
For a time, a big crunch
was the likely answer.
441
00:24:34,407 --> 00:24:38,177
Dark matter, the invisible bulk
of the universe,
442
00:24:38,178 --> 00:24:41,482
Causes space
to fall in on itself.
443
00:24:42,750 --> 00:24:47,119
Galaxies collide.
Planet merges with planet.
444
00:24:47,120 --> 00:24:51,892
Everything becomes hotter
and hotter, denser and denser.
445
00:24:51,893 --> 00:24:54,462
The universe is like
one giant star.
446
00:24:58,232 --> 00:25:02,268
Dark energy kills
the big crunch theory.
447
00:25:02,269 --> 00:25:05,404
It acts like rocket fuel
for the expansion of space
448
00:25:05,405 --> 00:25:07,641
Between galaxies.
449
00:25:07,642 --> 00:25:10,879
They're not just coasting.
They're getting pushed outward.
450
00:25:14,213 --> 00:25:16,415
Only two possible fates
remain --
451
00:25:16,416 --> 00:25:19,118
A big rip or a big freeze.
452
00:25:19,119 --> 00:25:22,020
Both scenarios rely
on dark energy.
453
00:25:22,021 --> 00:25:24,958
For the universe to be torn
to shreds in a big rip,
454
00:25:24,959 --> 00:25:28,662
Dark energy must increase
exponentially in the future.
455
00:25:28,663 --> 00:25:31,998
But a big freeze requires
a steady increase
456
00:25:31,999 --> 00:25:33,500
In dark energy,
457
00:25:33,501 --> 00:25:35,402
Pushing galaxies away
from each other.
458
00:25:35,503 --> 00:25:38,472
We can't write the last chapter
of our universe
459
00:25:38,473 --> 00:25:41,944
Until we understand the nature
of dark energy.
460
00:25:43,545 --> 00:25:46,414
May 2009.
461
00:25:46,415 --> 00:25:50,019
The european space agency
launches the planck satellite
462
00:25:50,020 --> 00:25:53,921
To search for the birth
of dark energy.
463
00:25:53,922 --> 00:25:58,392
Its ultra-Sensitive telescope
peers through space and time
464
00:25:58,393 --> 00:26:00,928
Back through billions of years,
465
00:26:00,929 --> 00:26:05,500
Towards the beginning of
everything, to capture this.
466
00:26:05,501 --> 00:26:08,003
This is our universe
as it appeared
467
00:26:08,004 --> 00:26:10,938
Over 13 billion years ago,
468
00:26:10,939 --> 00:26:14,977
380,000 years
after the big bang.
469
00:26:16,545 --> 00:26:19,147
So what planck has done
is take a picture
470
00:26:19,148 --> 00:26:21,416
Of the early universe
471
00:26:21,417 --> 00:26:24,552
And told us about what
the early universe is like
472
00:26:24,553 --> 00:26:26,988
And given us our most detailed
and accurate picture
473
00:26:26,989 --> 00:26:28,322
Of that moment in time.
474
00:26:28,323 --> 00:26:30,757
The universe in this picture
475
00:26:30,758 --> 00:26:35,264
Is a hot soup of protons,
electrons, and photons.
476
00:26:35,265 --> 00:26:38,332
Hydrogen atoms have just started
to form,
477
00:26:38,333 --> 00:26:41,069
And it's the light from this
genesis of matter
478
00:26:41,070 --> 00:26:42,938
That we see here.
479
00:26:45,007 --> 00:26:48,244
Blue areas are colder.
Reds are warm.
480
00:26:48,378 --> 00:26:50,480
Eventually, those hot spots,
481
00:26:50,481 --> 00:26:52,682
Those red spots you see
in the map,
482
00:26:52,683 --> 00:26:55,318
Are going to form large
superclusters
483
00:26:55,319 --> 00:26:59,790
Made up of hundreds or thousands
of galaxies.
484
00:26:59,791 --> 00:27:03,927
Each one of those galaxies will
contain billions of stars.
485
00:27:05,561 --> 00:27:07,864
Gravity
and expansion alone
486
00:27:07,865 --> 00:27:12,568
Appear to drive the formation
of these embryonic galaxies.
487
00:27:12,569 --> 00:27:16,839
Dark energy doesn't seem
to have switched on yet.
488
00:27:16,840 --> 00:27:21,678
So, when did dark energy take
control of the universe?
489
00:27:28,185 --> 00:27:31,387
Astronomer brenda frye
is part of a team
490
00:27:31,388 --> 00:27:33,991
Using massive
ground-Based telescopes
491
00:27:33,992 --> 00:27:36,792
Like this one at kitt peak,
arizona.
492
00:27:36,793 --> 00:27:41,164
She peers back in time
to capture the universe
493
00:27:41,165 --> 00:27:44,069
Through its childhood
as it was growing.
494
00:27:46,104 --> 00:27:48,672
Right.
So this is an aluminum plate,
495
00:27:48,673 --> 00:27:52,875
And into this plate are
drilled 640 individual holes.
496
00:27:52,876 --> 00:27:55,945
Each one is put at a very
specific place on the mask
497
00:27:55,946 --> 00:28:00,017
Which will correspond to one
particular galaxy in the sky.
498
00:28:02,386 --> 00:28:04,119
During each observation,
499
00:28:04,120 --> 00:28:08,625
The light from 640 individual
galaxies is collected
500
00:28:08,626 --> 00:28:12,029
Using fiber optic cables.
501
00:28:12,030 --> 00:28:15,499
The speed and relative position
of each galaxy is measured
502
00:28:15,500 --> 00:28:19,371
To pinpoint exactly where it is
in space.
503
00:28:19,472 --> 00:28:22,107
So far, the team
has accurately mapped
504
00:28:22,108 --> 00:28:24,943
Around a million galaxies
in 3d,
505
00:28:24,944 --> 00:28:26,812
And this is what they look like.
506
00:28:28,046 --> 00:28:30,682
Each one of these fuzzy patches
507
00:28:30,683 --> 00:28:32,516
Is a fully grown galaxy
508
00:28:32,517 --> 00:28:36,553
Containing around
200 billion stars.
509
00:28:36,554 --> 00:28:38,223
This is a very basic
measurement,
510
00:28:38,224 --> 00:28:40,390
And we think that
this will be able to help us
511
00:28:40,391 --> 00:28:43,395
To get a grasp into the nature
of dark energy.
512
00:28:43,396 --> 00:28:47,697
Scientists compare
this adolescent universe
513
00:28:47,698 --> 00:28:49,567
To its baby pictures.
514
00:28:49,568 --> 00:28:51,802
It shows dark energy emerging
515
00:28:51,803 --> 00:28:55,008
When the universe is
half as old as it is today.
516
00:28:56,276 --> 00:28:59,011
About 8 billion years
after the big bang,
517
00:28:59,012 --> 00:29:03,248
This expansion of the universe
begins to accelerate,
518
00:29:03,249 --> 00:29:05,884
And we're in the middle
of this acceleration.
519
00:29:05,885 --> 00:29:10,589
The data also shows
that as space expands,
520
00:29:10,590 --> 00:29:15,226
Dark energy
increases in lockstep with it.
521
00:29:15,227 --> 00:29:17,562
If you had a box and you put
some dark energy in it,
522
00:29:17,563 --> 00:29:19,898
And then you went and you
weighed that box...
523
00:29:19,899 --> 00:29:21,800
now you take the box,
you make it twice as big.
524
00:29:21,801 --> 00:29:23,668
You don't open it.
You don't put anything in it.
525
00:29:23,669 --> 00:29:26,205
You weigh it again, it's gonna
weigh twice as much.
526
00:29:26,206 --> 00:29:28,541
This remarkable
observation means
527
00:29:28,542 --> 00:29:32,011
That we should be safe
from a big rip.
528
00:29:32,012 --> 00:29:35,447
Dark energy will continue
to increase gradually.
529
00:29:35,448 --> 00:29:39,016
The universe is heading
for a big freeze,
530
00:29:39,017 --> 00:29:43,054
And scientists can finally
calculate a timeline
531
00:29:43,055 --> 00:29:45,925
For the end of everything.
532
00:29:55,102 --> 00:29:56,637
It now seems
that we live
533
00:29:56,638 --> 00:29:59,272
In an almost perfect universe,
534
00:29:59,273 --> 00:30:02,842
With just enough gravity
to hold the galaxies together
535
00:30:02,843 --> 00:30:06,748
And just enough dark energy
that it will expand forever
536
00:30:06,749 --> 00:30:09,385
Without ripping itself
to shreds.
537
00:30:11,320 --> 00:30:15,992
Cosmologists can finally
envision the end of it all.
538
00:30:17,326 --> 00:30:19,894
30 years ago,
it was debatable.
539
00:30:19,895 --> 00:30:22,762
But now, it appears
that the universe most likely
540
00:30:22,763 --> 00:30:24,331
Will suffer a deep freeze.
541
00:30:24,332 --> 00:30:27,637
If you look at the data,
it stares out at you.
542
00:30:28,803 --> 00:30:30,370
In a big freeze,
543
00:30:30,371 --> 00:30:34,509
Dark energy pushes galaxies
further and further apart,
544
00:30:34,510 --> 00:30:37,380
But they remain intact.
545
00:30:37,413 --> 00:30:41,083
The stars inside them
fade away.
546
00:30:41,084 --> 00:30:43,619
Every star you see in the sky,
including our sun,
547
00:30:43,620 --> 00:30:45,722
Is burning through
its nuclear fuel.
548
00:30:45,723 --> 00:30:48,923
The gas will run out,
stars will stop being made,
549
00:30:48,924 --> 00:30:52,562
And the ones that exist are it.
Those are the last ones.
550
00:30:56,967 --> 00:30:59,267
A hundred trillion
years from now,
551
00:30:59,268 --> 00:31:03,573
The biggest stars will be
the first to go extinct.
552
00:31:03,574 --> 00:31:06,708
Big stars burn bright
and die hard.
553
00:31:06,709 --> 00:31:11,147
The star's core collapses,
554
00:31:11,148 --> 00:31:13,284
Unleashing a supernova.
555
00:31:14,584 --> 00:31:17,920
Then gravity crushes
the dead star down
556
00:31:17,921 --> 00:31:20,590
To a single dense spot.
557
00:31:20,591 --> 00:31:24,027
The bright star
is now a black hole.
558
00:31:26,397 --> 00:31:28,967
Sun-Like stars go next.
559
00:31:30,434 --> 00:31:33,035
As their supply of hydrogen
runs out,
560
00:31:33,036 --> 00:31:35,405
They swell to a bloated fireball
561
00:31:35,406 --> 00:31:38,342
Over 200 times
their current size.
562
00:31:44,215 --> 00:31:46,450
And when the core
has no more hydrogen,
563
00:31:46,451 --> 00:31:49,720
It's going to bloat up
into a red giant star.
564
00:31:49,721 --> 00:31:52,089
Now, red giant stars are so big,
they will actually
565
00:31:52,090 --> 00:31:54,090
Eat up their own planets.
566
00:31:54,091 --> 00:31:55,925
We know of examples
of red giants
567
00:31:55,926 --> 00:31:57,994
That go all the way out
to where the orbit of jupiter is
568
00:31:57,995 --> 00:31:59,929
In our solar system.
569
00:31:59,930 --> 00:32:02,899
Its fuel exhausted,
570
00:32:02,900 --> 00:32:05,602
The sun-Like star
gives in to gravity
571
00:32:05,603 --> 00:32:07,704
And shrinks to a white dwarf,
572
00:32:07,705 --> 00:32:09,473
A dense ball of matter
573
00:32:09,474 --> 00:32:12,608
Just a few thousand miles
in diameter.
574
00:32:12,609 --> 00:32:16,647
It will glow with heat
for a further 10 billion years
575
00:32:16,648 --> 00:32:19,215
Before cooling to a black dwarf,
576
00:32:19,216 --> 00:32:24,255
A ball of compressed carbon,
perhaps even diamond.
577
00:32:26,959 --> 00:32:29,293
As the biggest stars die,
578
00:32:29,294 --> 00:32:32,830
The universe
will slowly turn red.
579
00:32:32,831 --> 00:32:34,598
The blue stars
will blow up,
580
00:32:34,599 --> 00:32:36,767
And then the slightly less blue
stars will blow up,
581
00:32:36,768 --> 00:32:39,136
And then stars like the sun
will fade away and die,
582
00:32:39,137 --> 00:32:41,808
Leaving just the red stars
to exist.
583
00:32:43,376 --> 00:32:45,211
Red stars
are the smallest
584
00:32:45,212 --> 00:32:47,113
And coolest in the universe.
585
00:32:47,114 --> 00:32:49,382
They burn their fuel slowly.
586
00:32:49,383 --> 00:32:52,116
But, after another
10 trillion years,
587
00:32:52,117 --> 00:32:54,520
Even these smallest
of dwarf stars
588
00:32:54,521 --> 00:32:56,789
Will use up their fuel.
589
00:32:56,790 --> 00:33:00,358
Stars as we know them
will cease to burn energy,
590
00:33:00,359 --> 00:33:02,828
And the night sky
will turn black.
591
00:33:02,829 --> 00:33:06,699
Black holes,
the corpses of dead stars,
592
00:33:06,700 --> 00:33:11,338
And cold clouds of gas and dust
are all that remains.
593
00:33:13,140 --> 00:33:15,909
The age of stars is over.
594
00:33:15,910 --> 00:33:19,645
The age of black holes begins.
595
00:33:19,646 --> 00:33:21,848
Black holes become
the fundamental building block
596
00:33:21,849 --> 00:33:23,515
Of the universe.
597
00:33:23,516 --> 00:33:25,884
A galaxy will basically be
a supermassive black hole
598
00:33:25,885 --> 00:33:27,919
In the center, with smaller
black holes orbiting it.
599
00:33:27,920 --> 00:33:30,455
In some ways, it's kind of
a ghost universe.
600
00:33:30,456 --> 00:33:32,292
It's the corpses,
the zombie stars,
601
00:33:32,293 --> 00:33:33,993
That will take us
into the future.
602
00:33:33,994 --> 00:33:37,163
Zombie galaxies
filled with black holes
603
00:33:37,164 --> 00:33:38,964
Continue to evolve.
604
00:33:38,965 --> 00:33:42,335
They sweep up the dead remains
of stars.
605
00:33:42,336 --> 00:33:46,439
Black hole merges
with black hole.
606
00:33:46,440 --> 00:33:48,540
They'll eat each other
and they'll get bigger,
607
00:33:48,541 --> 00:33:50,375
And maybe they'll fall into
the supermassive black hole
608
00:33:50,376 --> 00:33:51,844
And it'll get bigger.
609
00:33:51,845 --> 00:33:54,846
The universe will still be
an exciting, dynamic place,
610
00:33:54,847 --> 00:33:57,149
It's just that the time scales
you're talking about
611
00:33:57,150 --> 00:33:58,718
Are now trillions of years
612
00:33:58,719 --> 00:34:01,420
Instead of thousands
or millions of years.
613
00:34:01,421 --> 00:34:05,591
Any material that
evades the pull of a black hole
614
00:34:05,592 --> 00:34:10,862
Eventually dies away
as its protons disintegrate.
615
00:34:10,863 --> 00:34:14,000
A proton, one of the fundamental
building blocks
616
00:34:14,001 --> 00:34:16,835
Of atomic matter,
of what makes us up,
617
00:34:16,836 --> 00:34:19,337
Can just spontaneously
fall apart,
618
00:34:19,338 --> 00:34:23,210
And it turns out this takes
a tremendously long time.
619
00:34:23,211 --> 00:34:25,310
But even that will go away.
620
00:34:25,311 --> 00:34:30,382
All that will be left
is a sea of black holes.
621
00:34:30,383 --> 00:34:33,652
Scientists used to think
black holes were immortal,
622
00:34:33,653 --> 00:34:35,323
But even these will one day die.
623
00:34:35,424 --> 00:34:38,125
Now we're talking about
time scales
624
00:34:38,126 --> 00:34:39,794
Of unimaginable length --
625
00:34:39,795 --> 00:34:42,331
Quadrillions of years
into the future.
626
00:34:42,432 --> 00:34:43,898
But on that time scale,
627
00:34:43,899 --> 00:34:48,001
Even the black holes
begin to evaporate.
628
00:34:48,002 --> 00:34:50,238
They'll get smaller and smaller
and smaller,
629
00:34:50,239 --> 00:34:52,173
And then, poof, they'll be gone.
630
00:34:52,174 --> 00:34:54,642
The universe will end
631
00:34:54,643 --> 00:34:57,477
When the last remaining
black hole dies.
632
00:34:57,478 --> 00:35:00,280
As it gets smaller,
the evaporation rate
633
00:35:00,281 --> 00:35:02,316
Increases exponentially.
634
00:35:02,317 --> 00:35:04,517
Before long,
it reaches a size
635
00:35:04,518 --> 00:35:09,523
A billionth of a trillionth
of a trillionth of an inch.
636
00:35:09,524 --> 00:35:12,927
At that instant,
the laws of physics break down,
637
00:35:12,928 --> 00:35:17,097
And the last black hole explodes
in a flash of gamma rays,
638
00:35:17,098 --> 00:35:19,867
Leaving nothing.
639
00:35:19,868 --> 00:35:23,470
And it will die
in a sudden burst of light,
640
00:35:23,471 --> 00:35:25,139
The last burst of light
641
00:35:25,140 --> 00:35:27,475
In the entire history
of the universe.
642
00:35:28,111 --> 00:35:30,112
The big freeze is coming.
643
00:35:30,113 --> 00:35:34,416
The universe will suffer a cold,
slow, dark death
644
00:35:34,417 --> 00:35:35,784
Which will play out
645
00:35:35,785 --> 00:35:39,521
Over trillions upon trillions
of years.
646
00:35:39,522 --> 00:35:42,925
But quantum physics leaves
the door open
647
00:35:42,926 --> 00:35:44,693
For an alternative end,
648
00:35:44,694 --> 00:35:48,130
An event so powerful,
so destructive,
649
00:35:48,131 --> 00:35:53,836
That it could destroy everything
we see in the blink of an eye.
650
00:35:53,837 --> 00:35:57,007
And it could happen tomorrow.
651
00:36:06,251 --> 00:36:08,085
The end of the universe --
652
00:36:08,086 --> 00:36:09,618
It's coming.
653
00:36:09,619 --> 00:36:13,022
Dark energy accelerates
the space between galaxies,
654
00:36:13,023 --> 00:36:16,593
Pushing everything we see
to a long, cold,
655
00:36:16,594 --> 00:36:19,330
And very slow death.
656
00:36:19,331 --> 00:36:23,199
Unless, that is, something
bizarre happens first.
657
00:36:23,200 --> 00:36:27,004
A monster called
phase transition
658
00:36:27,005 --> 00:36:28,638
Is lurking in the shadows,
659
00:36:28,639 --> 00:36:32,576
And it could annihilate
the fabric of space and time
660
00:36:32,577 --> 00:36:35,678
At any moment.
661
00:36:35,679 --> 00:36:39,449
When we cool down water,
it turns into ice.
662
00:36:39,450 --> 00:36:40,951
The properties change.
663
00:36:40,952 --> 00:36:43,154
If you lived in the water,
when it changed to ice,
664
00:36:43,155 --> 00:36:44,989
Your world
would be very different.
665
00:36:44,990 --> 00:36:50,194
Water phase changes
into ice when it loses energy.
666
00:36:50,195 --> 00:36:53,230
I once left a water
bottle in my car overnight.
667
00:36:53,231 --> 00:36:56,132
It was still liquid,
but the moment i touched it,
668
00:36:56,133 --> 00:36:57,533
The slight imperfection,
669
00:36:57,534 --> 00:36:59,402
The little bit of ice
that it formed, spread,
670
00:36:59,403 --> 00:37:01,270
Poof, and filled up
the whole bottle.
671
00:37:01,271 --> 00:37:04,474
That rapid change
to something new
672
00:37:04,475 --> 00:37:06,644
Is called a phase transition,
673
00:37:06,645 --> 00:37:12,048
And bizarrely, the same thing
could happen to empty space.
674
00:37:12,049 --> 00:37:14,753
We've really come to understand
675
00:37:14,754 --> 00:37:17,956
That we shouldn't take
for granted that...vacuum,
676
00:37:17,957 --> 00:37:20,691
What we call nothing,
is actually stable.
677
00:37:20,692 --> 00:37:23,594
It could be that the energy
stored in empty space
678
00:37:23,595 --> 00:37:26,398
Is just waiting to be released
in a phase transition.
679
00:37:26,399 --> 00:37:29,535
If it is, the laws of physics
will change.
680
00:37:31,404 --> 00:37:35,106
A spontaneous glitch
in the fabric of space-Time
681
00:37:35,107 --> 00:37:39,010
Could trigger
a phase transition of space,
682
00:37:39,011 --> 00:37:43,414
A tiny bubble of new universe
that spreads out,
683
00:37:43,415 --> 00:37:45,715
Overwriting the old.
684
00:37:45,716 --> 00:37:49,387
We know it can happen,
because it's happened before.
685
00:37:53,192 --> 00:37:55,193
At the moment of the big bang,
686
00:37:55,194 --> 00:37:57,262
The universe
that's first created
687
00:37:57,263 --> 00:38:00,632
Is completely different
to the one we see today.
688
00:38:00,633 --> 00:38:03,568
Hot and without form,
689
00:38:03,569 --> 00:38:06,170
There's no matter, no time.
690
00:38:06,171 --> 00:38:09,740
The laws of physics
are different.
691
00:38:09,741 --> 00:38:13,445
Suddenly, less than a trillionth
of a second later,
692
00:38:13,446 --> 00:38:16,514
A glitch triggers
a phase transition.
693
00:38:16,515 --> 00:38:20,152
A tiny bubble of the universe
we live in today forms,
694
00:38:20,153 --> 00:38:22,387
And it races outward,
695
00:38:22,388 --> 00:38:24,356
Destroying everything it touches
696
00:38:24,357 --> 00:38:27,525
Like ice
spreading through water.
697
00:38:27,526 --> 00:38:31,262
The energy that spills out
creates the space and time
698
00:38:31,263 --> 00:38:32,898
That we exist in,
699
00:38:32,899 --> 00:38:37,503
The building blocks of matter
and the forces that govern them.
700
00:38:37,504 --> 00:38:40,239
All that energy was released,
producing all the matter
701
00:38:40,240 --> 00:38:42,175
And radiation we observe
in the universe today.
702
00:38:42,375 --> 00:38:45,211
The old universe
gives up its energy
703
00:38:45,212 --> 00:38:46,847
To create the new.
704
00:38:46,848 --> 00:38:48,982
But it holds some back.
705
00:38:48,983 --> 00:38:53,419
The vacuum of space
still has energy bound to it.
706
00:38:53,420 --> 00:38:57,957
Perhaps this is the dark energy
we see today.
707
00:38:57,958 --> 00:39:01,261
Physicists believe
that someday in the future,
708
00:39:01,262 --> 00:39:04,763
A brand new glitch in the fabric
of space-Time
709
00:39:04,764 --> 00:39:07,300
May trigger another
phase transition,
710
00:39:07,301 --> 00:39:10,870
One that wipes us
and everything we see
711
00:39:10,871 --> 00:39:12,805
Out of existence.
712
00:39:12,806 --> 00:39:16,309
This is a way to destroy
an entire universe,
713
00:39:16,310 --> 00:39:18,077
Because within your universe
714
00:39:18,078 --> 00:39:20,579
Are the seeds
of its own destruction.
715
00:39:20,580 --> 00:39:23,550
It would spread out at the speed
of light in a death bubble,
716
00:39:23,551 --> 00:39:26,519
Ruining all the galaxies
as it passes through,
717
00:39:26,520 --> 00:39:29,822
And ultimately completely
destroying our universe.
718
00:39:29,823 --> 00:39:33,327
Nothing can survive
the expanding phase transition.
719
00:39:33,328 --> 00:39:38,132
Planets, nebulas, galaxies --
All are ripped apart
720
00:39:38,133 --> 00:39:40,434
As the boundary
of the bubble reaches them.
721
00:39:40,435 --> 00:39:43,670
Inside this bubble,
protons are unstable,
722
00:39:43,671 --> 00:39:47,507
Atoms begin to rearrange
in a new form of matter.
723
00:39:47,508 --> 00:39:49,543
As these bubbles
begin to expand,
724
00:39:49,544 --> 00:39:52,179
A new universe is being born
725
00:39:52,180 --> 00:39:54,847
In the corpse
of the old universe,
726
00:39:54,848 --> 00:39:58,186
And the beginning
of a new law of physics.
727
00:39:58,387 --> 00:40:02,022
And so, the expanding universe
we now see
728
00:40:02,023 --> 00:40:05,460
May end in a phase transition,
but we won't know what hit us,
729
00:40:05,461 --> 00:40:07,395
'Cause the laws of physics
will change,
730
00:40:07,396 --> 00:40:10,131
And we will essentially most
likely disappear
731
00:40:10,132 --> 00:40:11,899
At the instant it happens.
732
00:40:11,900 --> 00:40:15,569
This bubble will expand
at the speed of light,
733
00:40:15,570 --> 00:40:17,439
And as the bubble passes you,
734
00:40:17,440 --> 00:40:20,475
All the atoms of your body
rearrange themselves,
735
00:40:20,476 --> 00:40:22,178
And you would never know it.
736
00:40:22,179 --> 00:40:24,879
You would have no warning,
because the bubble itself
737
00:40:24,880 --> 00:40:26,448
Is expanding
at the speed of light.
738
00:40:26,449 --> 00:40:29,052
You can't predict precisely
when it could happen.
739
00:40:29,053 --> 00:40:30,684
You only have a probability.
740
00:40:30,685 --> 00:40:32,921
So what you really
are predicting is a rate.
741
00:40:32,922 --> 00:40:36,092
Does it happen once a year?
Once every 10 billion years?
742
00:40:36,093 --> 00:40:38,325
Once every googol years?
Or whatever.
743
00:40:38,326 --> 00:40:41,628
It's very possible that
these bubbles get nucleated
744
00:40:41,629 --> 00:40:45,267
And grow about once every
10 or 20 billion years.
745
00:40:45,268 --> 00:40:47,903
So it hasn't happened yet
because we got lucky.
746
00:40:47,904 --> 00:40:50,840
It's unlikely it would happen
the next year or the next day,
747
00:40:50,841 --> 00:40:52,908
But the laws of physics
absolutely allow it.
748
00:40:56,245 --> 00:41:00,516
A phase change
may happen, or it may not.
749
00:41:01,650 --> 00:41:05,790
The universe plays its cards
close to its chest.
750
00:41:09,625 --> 00:41:12,829
And, like dark energy
and dark matter,
751
00:41:12,830 --> 00:41:14,799
There may be more surprises
to come...
752
00:41:16,600 --> 00:41:21,470
...surprises that will only
add to the mystery and wonder
753
00:41:21,471 --> 00:41:24,108
Our universe holds for us.
754
00:41:27,478 --> 00:41:29,113
Whatever the universe
is up to,
755
00:41:29,114 --> 00:41:30,479
We still don't know enough.
756
00:41:30,480 --> 00:41:32,582
We're in an age of discovery
right now.
757
00:41:32,583 --> 00:41:34,483
Perhaps there is something else
out there
758
00:41:34,484 --> 00:41:35,852
That we don't know about.
759
00:41:35,853 --> 00:41:38,255
So, i'm not going to draw
any conclusions
760
00:41:38,256 --> 00:41:39,957
Until things are conclusive.
761
00:41:42,659 --> 00:41:45,160
We don't understand
the nature of dark energy.
762
00:41:45,161 --> 00:41:48,765
And without that understanding,
virtually anything is possible.
763
00:41:48,766 --> 00:41:50,800
The future is still uncertain,
764
00:41:50,801 --> 00:41:53,135
And that means
there's still a mystery.
765
00:41:53,136 --> 00:41:56,507
And for me, that's the most
exciting possibility of all.
61288
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