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The universe was born to die.
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00:00:04,569 --> 00:00:08,972
But how and when
will it all end?
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00:00:08,973 --> 00:00:10,806
That's the reason
i became a cosmologist.
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I wanted to be the first person
that would know
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how the universe would end.
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00:00:14,512 --> 00:00:18,282
Two cosmic heavyweights
wrestle for control.
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The winner seals our fate.
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00:00:20,784 --> 00:00:23,587
The tug of war is gravity,
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which is trying
to shrink it down,
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00:00:25,257 --> 00:00:28,058
and the expansion of space
and time itself.
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00:00:28,059 --> 00:00:30,393
Will gravity triumph?
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00:00:30,394 --> 00:00:33,563
The universe will get smaller
and smaller, hotter and hotter.
13
00:00:33,564 --> 00:00:36,566
Or will expansion
get the upper hand?
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00:00:36,567 --> 00:00:40,538
Even the electrons around
your atoms will be ripped apart.
15
00:00:40,539 --> 00:00:42,005
The end is coming,
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and it could be
sooner than you think.
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The universe is everything
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all space, all time, all matter.
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The earth is a speck
by comparison,
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a grain of rock orbiting just
one of the 200 billion stars
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in our home galaxy,
the milky way.
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In turn, this enormous structure
is just a drop
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in an ocean of galaxies
that stretch
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for 90 billion light years.
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And all of this,
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from the biggest galaxy
to the smallest atom,
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will one day die.
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We don't see evidence
of anything being eternal.
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Eternity doesn't exist.
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Even space and time
will come to an end.
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The universe has been
expanding since its birth,
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gradually burning through
the fuel that lights its stars.
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But what happens
when the fuel runs out?
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00:02:02,055 --> 00:02:04,556
Will it all just fade away?
35
00:02:04,557 --> 00:02:06,960
Stars die out,
use up their nuclear fuel.
36
00:02:06,961 --> 00:02:09,563
We have an empty, cold,
desolate universe.
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00:02:09,564 --> 00:02:11,632
Just dead remnants of stars
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00:02:11,633 --> 00:02:13,734
black holes, neutron stars.
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00:02:13,735 --> 00:02:15,268
Eventually, they decay away,
40
00:02:15,269 --> 00:02:18,204
and you're left with a thin haze
of very low energy light.
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00:02:18,205 --> 00:02:19,539
That's it.
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00:02:19,540 --> 00:02:21,306
We used to think the universe
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00:02:21,307 --> 00:02:24,077
would cruise gently
into old age.
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00:02:24,078 --> 00:02:26,179
But over the past few decades,
45
00:02:26,180 --> 00:02:29,649
astronomers have
revealed a very different
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00:02:29,650 --> 00:02:31,418
and disturbing picture.
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The universe isn't cruising.
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It's fighting for its life.
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00:02:36,189 --> 00:02:38,458
It may seem peaceful here
on earth on a nice, sunny day,
50
00:02:38,459 --> 00:02:40,293
but in fact, above us
and all around us,
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00:02:40,294 --> 00:02:43,429
throughout the universe,
a battle is raging,
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00:02:43,430 --> 00:02:45,467
and it has raged
since the beginning of time.
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00:02:46,335 --> 00:02:49,904
Two deadly forces
grapple for control.
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00:02:49,905 --> 00:02:54,441
The first, expansion,
pulls galaxies apart,
55
00:02:54,442 --> 00:02:57,477
cooling the universe
and threatening it
56
00:02:57,478 --> 00:03:00,548
with a frozen extinction.
57
00:03:00,549 --> 00:03:05,085
The second, gravity, tries to
crush everything back together,
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00:03:05,086 --> 00:03:08,924
annihilating the universe
in a dense ball of fire.
59
00:03:11,492 --> 00:03:15,096
Will gravity or expansion win?
60
00:03:15,097 --> 00:03:17,131
Or will it end in a tie?
61
00:03:17,132 --> 00:03:20,937
These two colossal forces
yield three endgames.
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One is the big freeze.
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Expansion wins, and the universe
just expands forever.
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00:03:26,574 --> 00:03:29,176
The second is that there is
a delicate balance
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between the expansion
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00:03:30,445 --> 00:03:32,114
and the amount of gravitational
attraction,
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and the universe gets
to a particular size,
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00:03:34,216 --> 00:03:35,684
and it pretty much stays there.
69
00:03:35,685 --> 00:03:37,353
And the third outcome is that
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the gravitational
attraction wins,
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and the expansion stops,
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and the universe
begins to get smaller
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until, eventually,
it goes back to a big crunch.
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00:03:47,931 --> 00:03:50,265
So far,
the universe seems balanced
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00:03:50,266 --> 00:03:54,203
on a tightrope between
expansion and contraction.
76
00:03:54,204 --> 00:03:57,607
But will it keep its equilibrium
until it runs out of steam,
77
00:03:57,608 --> 00:04:00,411
or will something
tip the balance?
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00:04:02,446 --> 00:04:05,382
I don't think there's
any bigger question than,
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00:04:05,383 --> 00:04:07,616
where is the universe going?
80
00:04:07,617 --> 00:04:11,154
To predict the future,
cosmologists have always looked
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00:04:11,155 --> 00:04:15,358
to the past, back to
the beginning of expansion,
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the beginning of gravity,
the beginning of everything.
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00:04:22,732 --> 00:04:27,702
13.8 billion years ago,
An infinitely dense,
84
00:04:27,703 --> 00:04:32,408
hot speck ignites
and suddenly expands outward
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the big bang.
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00:04:35,946 --> 00:04:39,516
All energy, all space,
and all matter...
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...the building blocks of
The universe we see today,
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are created and set in motion.
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Think of it.
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00:04:49,995 --> 00:04:52,297
Everything you see around us
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concentrated into a primordial
fireball that exploded,
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00:04:56,935 --> 00:04:59,738
sending all the galaxies
into motion.
93
00:05:03,809 --> 00:05:07,477
That outward blast,
the birth of expansion,
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00:05:07,478 --> 00:05:10,147
is still going on today.
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00:05:10,148 --> 00:05:13,551
Without it, we wouldn't have
a universe big enough
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00:05:13,552 --> 00:05:16,354
for stars
and galaxies to exist in.
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00:05:16,355 --> 00:05:19,623
Expansion is an astonishing
force of nature.
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00:05:19,624 --> 00:05:23,927
It works by inflating
the fabric of space-time.
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00:05:23,928 --> 00:05:27,599
Space between galaxies expands,
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00:05:27,600 --> 00:05:29,902
and it pushes
the galaxies apart.
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00:05:29,903 --> 00:05:35,006
Space carries objects with it
like a surfer on a wave.
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00:05:35,007 --> 00:05:37,409
It's going on
in every part of space.
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00:05:37,410 --> 00:05:39,078
Even inside your body right now,
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there's a pressure
for space to expand.
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Expansion generated
the vast, moving stage
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00:05:44,918 --> 00:05:47,552
on which today's universe
plays out.
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00:05:47,553 --> 00:05:50,456
But left unchecked,
it could have been a force
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00:05:50,457 --> 00:05:52,590
for utter annihilation.
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00:05:52,591 --> 00:05:54,826
If the universe had
been expanding much faster,
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00:05:54,827 --> 00:05:56,595
it would have emptied out
so fast,
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00:05:56,596 --> 00:05:58,864
you wouldn't have had time
to make galaxies,
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00:05:58,865 --> 00:06:00,000
planets, people.
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The fact
that we're here
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00:06:04,271 --> 00:06:06,840
means that something must have
put on the brakes.
115
00:06:06,841 --> 00:06:11,443
It was, of course,
our universal glue -- gravity.
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Gravity and matter
go hand in hand.
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00:06:14,914 --> 00:06:17,816
The more massive the object,
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00:06:17,817 --> 00:06:20,919
the more pull it exerts
on everything around it.
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00:06:20,920 --> 00:06:26,526
It draws atom to atom,
particle to particle...
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...building stars, nebulas,
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00:06:32,533 --> 00:06:34,868
Galaxies
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00:06:34,869 --> 00:06:39,006
the hardware of the universe
we see today.
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00:06:39,007 --> 00:06:41,840
But gravity
is a double-edged sword.
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00:06:41,841 --> 00:06:44,744
Too much, and the early universe
would never have gotten
125
00:06:44,745 --> 00:06:46,912
out of the starting blocks.
126
00:06:46,913 --> 00:06:48,948
If it had been
expanding more slowly,
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00:06:48,949 --> 00:06:51,217
it would have re-collapsed
into another singularity.
128
00:06:51,218 --> 00:06:53,986
And again, you wouldn't have had
the time to make galaxies,
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00:06:53,987 --> 00:06:55,789
planets, or people.
130
00:06:55,790 --> 00:06:57,424
So we live in the goldilocks
universe.
131
00:06:57,425 --> 00:06:59,559
We live in the universe
that lasts long enough
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00:06:59,560 --> 00:07:02,061
that we can be here,
but expands gently enough
133
00:07:02,062 --> 00:07:03,997
that we have time to form.
134
00:07:06,767 --> 00:07:10,569
The universe has
lasted for 13.8 billion years,
135
00:07:10,570 --> 00:07:14,542
thanks to the opposing forces
of gravity and expansion.
136
00:07:14,543 --> 00:07:18,612
But just how stable
is this balancing act?
137
00:07:18,613 --> 00:07:22,115
Does our universe have just
the right amount of stuff in it
138
00:07:22,116 --> 00:07:24,216
to keep it from
runaway expansion
139
00:07:24,217 --> 00:07:26,287
or catastrophic collapse?
140
00:07:26,888 --> 00:07:29,757
In the 1920s,
scientists did the math,
141
00:07:29,758 --> 00:07:33,594
and the results were
anything but reassuring.
142
00:07:33,595 --> 00:07:36,831
The more matter you have,
the more gravity you have.
143
00:07:36,832 --> 00:07:40,168
If you have lots of matter
in a very dense universe,
144
00:07:40,169 --> 00:07:43,238
perhaps the universe
begins to re-collapse.
145
00:07:43,239 --> 00:07:45,339
Or, if you have
very little matter,
146
00:07:45,340 --> 00:07:47,709
the universe would
freeze to death.
147
00:07:47,710 --> 00:07:51,879
So what is the critical density,
the border between the two?
148
00:07:51,880 --> 00:07:56,416
It's approximately five hydrogen
atoms per cubic meter.
149
00:07:56,417 --> 00:08:01,822
So think of a cubic yard,
and put just five hydrogen atoms
150
00:08:01,823 --> 00:08:04,659
inside,
and that is the tipping point.
151
00:08:04,660 --> 00:08:06,793
If you put more than five atoms,
152
00:08:06,794 --> 00:08:08,796
then the universe will
begin to collapse.
153
00:08:08,797 --> 00:08:10,331
If you have
less than five atoms,
154
00:08:10,332 --> 00:08:11,934
then the universe
just keeps on going.
155
00:08:12,935 --> 00:08:15,135
If we thought
the universe was balanced
156
00:08:15,136 --> 00:08:18,306
on a tightrope before,
the critical density question
157
00:08:18,307 --> 00:08:22,579
showed us that the rope
was more like a razor blade.
158
00:08:22,946 --> 00:08:25,882
Yet, when astronomers took
additional measurements,
159
00:08:25,883 --> 00:08:28,316
they liked what they saw.
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00:08:28,317 --> 00:08:31,720
The universe appeared to contain
just the right amount
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00:08:31,721 --> 00:08:34,658
of matter to stay
at the critical density.
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00:08:35,793 --> 00:08:37,893
More and more,
the indirect evidence
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00:08:37,894 --> 00:08:40,729
and the theoretical
arguments suggested
164
00:08:40,730 --> 00:08:43,432
that the universe must be
exactly at the boundary
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between a universe
that would collapse
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and one that
would expand forever,
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00:08:47,571 --> 00:08:51,206
that we were teetering
on the hairy edge of expansion.
168
00:08:51,207 --> 00:08:55,478
The universe seemed
so perfectly balanced
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00:08:55,479 --> 00:08:59,380
that it would head quietly
into old age.
170
00:08:59,381 --> 00:09:02,918
Then, in the 1970s, astronomers
made an observation
171
00:09:02,919 --> 00:09:04,921
that shocked them.
172
00:09:04,922 --> 00:09:08,825
The cosmos was filled
with invisible stuff,
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00:09:08,826 --> 00:09:13,531
and its gravity could cause
a catastrophic collapse.
174
00:09:23,943 --> 00:09:27,078
The universe
is balanced on a tightrope.
175
00:09:27,079 --> 00:09:31,215
On each side of the drop
lies an early death
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00:09:31,216 --> 00:09:34,954
a big freeze, fueled by
the runaway stretching of space,
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00:09:34,955 --> 00:09:40,858
or a big crunch, the result of
gravity overcoming expansion.
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00:09:40,859 --> 00:09:44,328
40 years ago, scientists
Believed we'd stay balanced
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00:09:44,329 --> 00:09:47,899
between these fates
for eternity.
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00:09:47,900 --> 00:09:50,135
Now things have changed
tremendously,
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00:09:50,136 --> 00:09:52,871
because we've discovered
something we never knew about
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00:09:52,872 --> 00:09:53,672
40 years ago.
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00:09:54,273 --> 00:09:58,944
In the 1970s,
astronomers are stunned.
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00:09:58,945 --> 00:10:02,647
Some unknown form of matter,
invisible to telescopes,
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dwarfs what we thought was
out there,
186
00:10:05,350 --> 00:10:09,121
not a fraction more,
but five times more.
187
00:10:09,122 --> 00:10:12,290
We used to think
that gravity came from stars
188
00:10:12,291 --> 00:10:15,294
and objects you can see
end of story.
189
00:10:15,295 --> 00:10:18,665
Now, we realize that that naive
picture is actually wrong.
190
00:10:19,700 --> 00:10:22,001
Astronomers make
the discovery,
191
00:10:22,002 --> 00:10:25,373
studying the clockwork
nature of our universe.
192
00:10:26,775 --> 00:10:29,442
The huge gravity of the sun
holds the earth
193
00:10:29,443 --> 00:10:33,582
and all the other planets
in a delicate circular dance.
194
00:10:37,451 --> 00:10:40,987
The sun's mass controls
the speed of these orbits.
195
00:10:40,988 --> 00:10:44,157
If it were more massive,
the planets would orbit
196
00:10:44,158 --> 00:10:45,825
much more quickly.
197
00:10:45,826 --> 00:10:48,395
And if it were smaller,
it would take much longer
198
00:10:48,396 --> 00:10:51,032
for a planet to complete
an orbit.
199
00:10:53,233 --> 00:10:56,502
Galaxies run
like clockwork, too.
200
00:10:56,503 --> 00:10:59,772
The vast mass at the center
pulls the outer stars
201
00:10:59,773 --> 00:11:03,176
into circular,
planet-like orbits.
202
00:11:03,177 --> 00:11:05,679
Astronomers make
precise measurements
203
00:11:05,680 --> 00:11:09,348
of these galactic
orbits in the 1970s.
204
00:11:09,349 --> 00:11:12,521
The results change everything.
205
00:11:13,422 --> 00:11:15,989
The galaxies
were spinning too fast.
206
00:11:15,990 --> 00:11:17,525
Way too fast.
207
00:11:20,596 --> 00:11:23,465
Even accounting for
the supermassive black holes
208
00:11:23,466 --> 00:11:27,768
at their center, nine-tenths
of their mass was missing.
209
00:11:27,769 --> 00:11:30,605
By rights,
the galaxy should fly apart.
210
00:11:30,606 --> 00:11:32,774
By rights, the earth
should have been flung
211
00:11:32,775 --> 00:11:35,744
into intergalactic space
billions of years ago.
212
00:11:35,745 --> 00:11:38,946
We should have no
milky way galaxy, and yet,
213
00:11:38,947 --> 00:11:40,683
our universe is
full of galaxies.
214
00:11:44,753 --> 00:11:47,688
An immense
additional source of gravity
215
00:11:47,689 --> 00:11:50,591
must be holding galaxies
together.
216
00:11:50,592 --> 00:11:53,827
But no matter where astronomers
point their telescopes,
217
00:11:53,828 --> 00:11:55,764
they see nothing.
218
00:11:55,765 --> 00:11:59,299
Not a glimmer, not a shadow.
219
00:11:59,300 --> 00:12:04,172
Whatever this new stuff is,
it doesn't emit light,
220
00:12:04,173 --> 00:12:07,808
reflect light,
or even block light.
221
00:12:07,809 --> 00:12:10,713
They call it dark matter.
222
00:12:10,746 --> 00:12:14,084
What we've learned is that most
of the matter in the universe
223
00:12:14,085 --> 00:12:16,720
is not ordinary stuff.
it's not atoms.
224
00:12:16,721 --> 00:12:19,522
It's not particles we've yet
detected in any experiment
225
00:12:19,523 --> 00:12:21,224
done here on earth.
226
00:12:21,225 --> 00:12:23,860
It's some new kind of particle
that we call the dark matter.
227
00:12:26,996 --> 00:12:28,898
Dark matter fills the universe,
228
00:12:28,899 --> 00:12:32,002
outstripping normal matter
by 5-to-1.
229
00:12:35,605 --> 00:12:40,109
Vast filaments spread out
throughout the cosmos,
230
00:12:40,110 --> 00:12:44,581
and bright galaxies cluster
where dark matter is thickest.
231
00:12:46,917 --> 00:12:51,253
Dark matter provides
the scaffolding that underlies
232
00:12:51,254 --> 00:12:54,123
how the matter in the universe
structures itself,
233
00:12:54,124 --> 00:12:56,027
where it goes,
and what it does.
234
00:12:56,894 --> 00:12:58,829
So,
dark matter dictated
235
00:12:58,830 --> 00:13:02,396
how the universe unfolded.
236
00:13:02,397 --> 00:13:04,535
It seems as if
out of the hot big bang,
237
00:13:04,536 --> 00:13:08,171
dark matter condensed first,
before atoms,
238
00:13:08,172 --> 00:13:11,141
and dark matter began
to become clumpy.
239
00:13:11,142 --> 00:13:14,344
The clumpiness then began
to attract atoms
240
00:13:14,345 --> 00:13:18,047
as they were formed later,
and that formed galaxies.
241
00:13:18,048 --> 00:13:20,084
And in some sense,
the dark matter therefore
242
00:13:20,085 --> 00:13:23,689
provides kind of a womb that
allows the birth of our galaxy.
243
00:13:26,925 --> 00:13:30,094
Dark matter holds
the universe together,
244
00:13:30,095 --> 00:13:32,564
but it also threatens
to destroy it.
245
00:13:35,397 --> 00:13:36,098
One of the most
amazing discoveries
246
00:13:36,099 --> 00:13:38,536
of the past few decades
is dark matter,
247
00:13:38,537 --> 00:13:40,502
the fact that there's much more
matter in the universe
248
00:13:40,503 --> 00:13:41,972
than we were aware of.
249
00:13:41,973 --> 00:13:44,476
And all of that matter
has a lot of gravity.
250
00:13:44,477 --> 00:13:46,609
So all this new matter,
all this new gravity
251
00:13:46,610 --> 00:13:49,013
must be slowing down
the expansion of the universe.
252
00:13:49,781 --> 00:13:52,717
Dark matter may even
tip the cosmic scales
253
00:13:52,718 --> 00:13:54,718
in favor of gravity,
254
00:13:54,719 --> 00:13:58,488
defeating expansion
and pulling the entire universe
255
00:13:58,489 --> 00:14:01,093
towards a death by fire.
256
00:14:01,094 --> 00:14:03,895
It's called the big crunch,
257
00:14:03,896 --> 00:14:06,265
and this is how
it would play out.
258
00:14:07,967 --> 00:14:12,303
For a fraction of a second,
the universe stalls,
259
00:14:12,304 --> 00:14:16,040
poised between
expansion and contraction.
260
00:14:16,041 --> 00:14:20,144
Then, gravity kicks off
a cataclysm.
261
00:14:20,145 --> 00:14:22,613
When you looked out,
the very first things
262
00:14:22,614 --> 00:14:24,549
as it began to turn around
that you began to see
263
00:14:24,550 --> 00:14:27,184
is that galaxies, instead of
moving away from us on average,
264
00:14:27,185 --> 00:14:29,689
would begin to be moving towards
us on average.
265
00:14:30,823 --> 00:14:33,794
The whole universe would look
like it was coming to get us.
266
00:14:35,596 --> 00:14:38,197
As space
contracts further,
267
00:14:38,198 --> 00:14:42,033
the density of matter increases,
gravity gets stronger,
268
00:14:42,034 --> 00:14:47,206
temperatures soar
as the crunch gathers momentum.
269
00:14:47,207 --> 00:14:49,542
Galaxies begin to collide,
270
00:14:49,543 --> 00:14:52,512
gas clouds begin to collide,
271
00:14:52,513 --> 00:14:55,616
planets slam into the earth.
272
00:14:59,385 --> 00:15:02,955
Black holes will execute a death
dance around each other.
273
00:15:02,956 --> 00:15:06,392
Temperatures, of course,
will continue to skyrocket.
274
00:15:06,393 --> 00:15:10,230
Matter, space,
and time implode
275
00:15:10,231 --> 00:15:13,164
until everything in the universe
is compressed
276
00:15:13,165 --> 00:15:19,004
into a tiny speck of infinite
mass, heat, and pressure.
277
00:15:19,005 --> 00:15:21,773
For the last stages
of the big crunch,
278
00:15:21,774 --> 00:15:24,976
galaxies will collide
and form a primordial atom.
279
00:15:24,977 --> 00:15:29,349
And then, life as we know it
will be impossible.
280
00:15:29,350 --> 00:15:31,783
We're back
to where it all began,
281
00:15:31,784 --> 00:15:32,921
back at the big bang.
282
00:15:33,722 --> 00:15:37,459
The universe that we live in
will cease to exist.
283
00:15:41,028 --> 00:15:46,766
But some believe a big crunch
could herald a new beginning.
284
00:15:46,767 --> 00:15:49,102
We don't know what the end point
of a big crunch would be,
285
00:15:49,103 --> 00:15:51,838
because the laws of physics
break down.
286
00:15:51,839 --> 00:15:55,309
It's possible, and indeed,
philosophically very pleasant,
287
00:15:55,310 --> 00:15:59,545
to imagine that that crunch
would somehow end up evolving
288
00:15:59,546 --> 00:16:02,848
into an expansion again, and you
could have a cyclic universe
289
00:16:02,849 --> 00:16:04,383
which goes on forever.
290
00:16:04,384 --> 00:16:08,123
Perhaps at that point, we will
recreate another big bang.
291
00:16:12,060 --> 00:16:14,428
It's conceivable that as
everything comes together
292
00:16:14,429 --> 00:16:17,963
in the crunch, something sort of
keeps it from just continuing
293
00:16:17,964 --> 00:16:21,635
and pushes out in a hot,
dense, smooth state,
294
00:16:21,636 --> 00:16:24,338
and from the other side,
it looks like a big bang,
295
00:16:24,339 --> 00:16:26,073
and a new universe has been
created.
296
00:16:26,074 --> 00:16:28,942
Our big bang might have been
someone else's big crunch.
297
00:16:28,943 --> 00:16:31,245
But just when
scientists came to terms
298
00:16:31,246 --> 00:16:34,716
with dark matter's big crunch,
the universe threw them
299
00:16:34,717 --> 00:16:37,118
another, even bigger curve.
300
00:16:37,119 --> 00:16:41,656
Some ghostly force seemed to be
sending us hurtling toward
301
00:16:41,657 --> 00:16:43,757
a completely different death.
302
00:16:43,758 --> 00:16:46,561
My postdoctoral
scholar showed me the results.
303
00:16:46,562 --> 00:16:47,730
I nearly fell off my chair.
304
00:16:57,874 --> 00:17:00,210
Gravity and expansion
battle for control
305
00:17:00,211 --> 00:17:03,681
of our universe
for 14 billion years...
306
00:17:07,852 --> 00:17:12,287
...expansion
Pushing it outwards,
307
00:17:12,288 --> 00:17:14,893
gravity pulling it in.
308
00:17:16,394 --> 00:17:18,495
With dark matter in its corner,
309
00:17:18,496 --> 00:17:20,997
gravity seems to be
the inevitable winner.
310
00:17:20,998 --> 00:17:25,568
The extra mass will drag
the universe into a big crunch,
311
00:17:25,569 --> 00:17:27,604
until a stunning discovery
312
00:17:27,605 --> 00:17:32,110
revolutionizes our understanding
of the universe.
313
00:17:34,444 --> 00:17:39,383
Around 1990, two teams of
researchers decided to measure
314
00:17:39,384 --> 00:17:41,450
the expansion history
of the universe
315
00:17:41,451 --> 00:17:44,554
to determine whether
it's been slowing down so much
316
00:17:44,555 --> 00:17:46,791
that it'll eventually have
a big crunch,
317
00:17:46,792 --> 00:17:49,325
or whether it hasn't been
slowing down much
318
00:17:49,326 --> 00:17:51,295
and will eternally expand.
319
00:17:51,296 --> 00:17:55,798
Astronomer alex filippenko
was on one team.
320
00:17:55,799 --> 00:17:58,401
Saul perlmutter led the other.
321
00:17:58,402 --> 00:18:01,438
We realized that it was possible
for the first time
322
00:18:01,439 --> 00:18:05,108
to go and actually make
a direct measurement
323
00:18:05,109 --> 00:18:07,611
of how much the universe had
been slowing down in the past.
324
00:18:07,813 --> 00:18:09,347
Both teams want
to measure
325
00:18:09,348 --> 00:18:11,648
the speed of distant galaxies.
326
00:18:11,649 --> 00:18:15,520
But because the galaxies are
too dim and too far away,
327
00:18:15,521 --> 00:18:17,557
they look for something
brighter.
328
00:18:22,461 --> 00:18:26,931
Billions of light years
from earth, a star detonates.
329
00:18:26,932 --> 00:18:29,600
This is a supernova,
330
00:18:29,601 --> 00:18:33,605
a dying star's
brilliant final gasp.
331
00:18:33,606 --> 00:18:37,541
It burns brightly, 5 billion
times brighter than the sun,
332
00:18:37,542 --> 00:18:40,212
but briefly.
333
00:18:40,213 --> 00:18:42,379
Perlmutter and filippenko
have a window
334
00:18:42,380 --> 00:18:44,948
of just one or two weeks
to measure
335
00:18:44,949 --> 00:18:48,252
how much the galaxy it sits in
is slowing down
336
00:18:48,253 --> 00:18:50,523
as it moves away from us.
337
00:18:54,628 --> 00:18:57,864
The teams look for supernovas
for eight years.
338
00:18:57,865 --> 00:19:03,670
They measure 42, and the results
seem impossible.
339
00:19:03,671 --> 00:19:06,271
We plotted the points
on the graphs,
340
00:19:06,272 --> 00:19:09,008
and...it didn't make any sense.
341
00:19:09,009 --> 00:19:10,876
They were not slowing down
at all.
342
00:19:10,877 --> 00:19:12,813
They were actually speeding up.
343
00:19:13,980 --> 00:19:17,584
What both groups found
stunned the world.
344
00:19:17,585 --> 00:19:20,420
In the last 4 or 5 billion
years,
345
00:19:20,421 --> 00:19:24,589
the universe has actually been
speeding up in its expansion.
346
00:19:24,590 --> 00:19:26,425
An accelerating universe,
347
00:19:26,426 --> 00:19:30,396
propelled by something
mysterious.
348
00:19:30,397 --> 00:19:32,865
For so long, we've been arguing
whether the universe would
349
00:19:32,866 --> 00:19:35,701
expand forever or collapse
back in on itself,
350
00:19:35,702 --> 00:19:38,070
but nobody thought
the answer was going to be
351
00:19:38,071 --> 00:19:40,373
that the universe was
accelerating,
352
00:19:40,374 --> 00:19:42,175
going faster and faster
all the time.
353
00:19:43,745 --> 00:19:47,115
The acceleration
bewilders the scientists.
354
00:19:47,116 --> 00:19:50,218
It seems to defy
the laws of physics.
355
00:19:50,219 --> 00:19:52,487
Imagine i've got a baseball
356
00:19:52,488 --> 00:19:54,154
and i throw it straight up.
357
00:19:54,155 --> 00:19:56,958
And instead of slowing down
once it leaves my hand,
358
00:19:56,959 --> 00:19:58,792
which is what
normally it will do,
359
00:19:58,793 --> 00:20:00,661
it begins to slow down at first,
360
00:20:00,662 --> 00:20:02,564
but then it starts
speeding away.
361
00:20:02,565 --> 00:20:04,199
Somehow, it's getting energy.
362
00:20:04,200 --> 00:20:09,670
The new energy seemed
to be coming from nothing,
363
00:20:09,671 --> 00:20:11,905
the vacuum of space.
364
00:20:11,906 --> 00:20:15,676
The word "vacuum" to a scientist
means completely empty space,
365
00:20:15,677 --> 00:20:18,278
no particles there at all,
no temperature,
366
00:20:18,279 --> 00:20:19,879
no energy to speak of.
367
00:20:19,880 --> 00:20:23,183
But there's an intrinsic energy
in space and time.
368
00:20:23,184 --> 00:20:26,886
Empty space has energy,
and that energy produces
369
00:20:26,887 --> 00:20:30,023
a gravitational repulsion,
a kind of anti-gravity.
370
00:20:30,024 --> 00:20:34,462
Without a clue what
this force is or how it works,
371
00:20:34,463 --> 00:20:40,034
all scientists can do is give it
a name -- dark energy.
372
00:20:40,403 --> 00:20:42,804
We could have called it
we-don't-know energy.
373
00:20:42,805 --> 00:20:44,273
We could have called it
anything.
374
00:20:44,274 --> 00:20:46,676
But we don't know what it is,
and dark or not,
375
00:20:46,677 --> 00:20:48,811
it's the biggest mystery
in physics.
376
00:20:51,980 --> 00:20:55,016
Nasa calibrates
its finest space telescopes
377
00:20:55,017 --> 00:20:58,152
to measure how much dark energy
is out there,
378
00:20:58,153 --> 00:21:01,489
and the result is mind-blowing.
379
00:21:01,490 --> 00:21:06,295
It dominates the mass of
the universe by nearly 3-to-1.
380
00:21:06,296 --> 00:21:07,962
And the more space expands,
381
00:21:07,963 --> 00:21:11,132
the more dark energy
there seems to be.
382
00:21:11,133 --> 00:21:14,068
Dark energy is the energy
of nothing,
383
00:21:14,069 --> 00:21:15,604
and it's repulsive.
384
00:21:15,605 --> 00:21:19,408
Therefore, as this dark energy
repels galaxies,
385
00:21:19,409 --> 00:21:21,343
there's more of it,
there's more vacuum.
386
00:21:21,344 --> 00:21:23,446
And so there's more repulsion,
387
00:21:23,447 --> 00:21:26,381
and perhaps that's the reason
why the universe is accelerating
388
00:21:26,382 --> 00:21:29,718
right now
rather than slowing down.
389
00:21:29,719 --> 00:21:33,189
Dark energy seems to
kill the big crunch theory,
390
00:21:33,190 --> 00:21:36,257
but scientists aren't yet sure
how dark energy,
391
00:21:36,258 --> 00:21:39,795
expansion, and space
are connected.
392
00:21:39,796 --> 00:21:43,131
If a volume of space doubles
in size,
393
00:21:43,132 --> 00:21:46,034
does the dark energy
inside it double, too?
394
00:21:46,035 --> 00:21:48,137
Or does it increase more?
395
00:21:48,138 --> 00:21:51,673
A 1-to-1 relationship leads
to a steady expansion.
396
00:21:51,674 --> 00:21:54,810
The universe ends
in a big freeze.
397
00:21:54,811 --> 00:21:59,381
But if dark energy increases
above and beyond expansion,
398
00:21:59,382 --> 00:22:03,955
a new, even more terrifying end
awaits the universe -- a big rip.
399
00:22:04,756 --> 00:22:08,791
In a big rip scenario,
the expansion is so great
400
00:22:08,792 --> 00:22:12,996
that even the galaxies begin
to expand internally,
401
00:22:12,997 --> 00:22:14,331
which means that literally
402
00:22:14,332 --> 00:22:16,268
our bodies
are going to be ripped apart.
403
00:22:17,567 --> 00:22:19,068
Scientists calculate
404
00:22:19,069 --> 00:22:21,405
just how the big rip
will play out.
405
00:22:23,740 --> 00:22:27,810
One by one, the galaxies in
the night sky will blink out
406
00:22:27,811 --> 00:22:30,779
as space pulls them away
from the earth
407
00:22:30,780 --> 00:22:32,582
faster than the speed of light.
408
00:22:34,286 --> 00:22:38,689
60 million years before the end,
Dark energy overcomes gravity
409
00:22:38,690 --> 00:22:41,624
on smaller and smaller scales.
410
00:22:41,625 --> 00:22:44,928
First galaxies start
to rip apart,
411
00:22:44,929 --> 00:22:48,798
then insides of galaxies
will begin to rip apart,
412
00:22:48,799 --> 00:22:51,469
and then solar systems will
begin to rip apart...
413
00:22:53,739 --> 00:22:56,708
Then planets...
414
00:22:56,709 --> 00:23:02,114
And then rocks, people, atoms.
415
00:23:02,115 --> 00:23:05,418
The end will
be mercifully quick.
416
00:23:06,719 --> 00:23:08,987
In the space of a few minutes,
417
00:23:08,988 --> 00:23:13,158
all the stars and planets in the
universe will be destroyed,
418
00:23:13,159 --> 00:23:17,929
their remains pulled apart
into ever-smaller pieces
419
00:23:17,930 --> 00:23:20,599
until finally,
when the universe has
420
00:23:20,600 --> 00:23:22,333
less than a second to live,
421
00:23:22,334 --> 00:23:25,804
the subatomic particles
that made all matter
422
00:23:25,805 --> 00:23:27,471
will be destroyed,
423
00:23:27,472 --> 00:23:30,775
and all that remains will be
individual photons
424
00:23:30,776 --> 00:23:33,077
becoming scarcer and scarcer
425
00:23:33,078 --> 00:23:35,814
as the space between them
expands.
426
00:23:35,815 --> 00:23:38,283
All you're left with is very low
energy light
427
00:23:38,284 --> 00:23:39,752
that gets stretched
and stretched
428
00:23:39,753 --> 00:23:41,854
until it might as well
not exist at all.
429
00:23:41,855 --> 00:23:43,854
The last thing to go --
430
00:23:43,855 --> 00:23:47,359
the empty vacuum
of space itself.
431
00:23:48,896 --> 00:23:51,397
It'll be pulling on the universe
so hard,
432
00:23:51,398 --> 00:23:54,300
it could tear the fabric
of the universe apart.
433
00:23:54,301 --> 00:23:57,703
Reality could dissolve.
434
00:23:57,704 --> 00:24:01,040
Will the universe end
with a big rip,
435
00:24:01,041 --> 00:24:03,375
or a big freeze?
436
00:24:03,376 --> 00:24:07,847
The answer is locked inside
the mystery of dark energy.
437
00:24:07,848 --> 00:24:12,619
Solve that, and the fate
of the universe becomes clear.
438
00:24:24,500 --> 00:24:26,866
The end
of the universe is coming.
439
00:24:26,867 --> 00:24:29,037
But how will it play out?
440
00:24:29,038 --> 00:24:32,906
For a time, a big crunch
was the likely answer.
441
00:24:32,907 --> 00:24:36,677
Dark matter, the invisible bulk
of the universe,
442
00:24:36,678 --> 00:24:39,982
causes space
to fall in on itself.
443
00:24:41,250 --> 00:24:45,619
Galaxies collide.
Planet merges with planet.
444
00:24:45,620 --> 00:24:50,392
Everything becomes hotter
and hotter, denser and denser.
445
00:24:50,393 --> 00:24:52,962
The universe is like
one giant star.
446
00:24:56,732 --> 00:25:00,768
Dark energy kills
the big crunch theory.
447
00:25:00,769 --> 00:25:03,904
It acts like rocket fuel
for the expansion of space
448
00:25:03,905 --> 00:25:06,141
between galaxies.
449
00:25:06,142 --> 00:25:09,379
They're not just coasting.
They're getting pushed outward.
450
00:25:12,713 --> 00:25:14,915
Only two possible fates
remain --
451
00:25:14,916 --> 00:25:17,618
a big rip or a big freeze.
452
00:25:17,619 --> 00:25:20,520
Both scenarios rely
on dark energy.
453
00:25:20,521 --> 00:25:23,458
For the universe to be torn
to shreds in a big rip,
454
00:25:23,459 --> 00:25:27,162
dark energy must increase
exponentially in the future.
455
00:25:27,163 --> 00:25:30,498
But a big freeze requires
a steady increase
456
00:25:30,499 --> 00:25:32,000
in dark energy,
457
00:25:32,001 --> 00:25:33,902
pushing galaxies away
from each other.
458
00:25:34,003 --> 00:25:36,972
We can't write the last chapter
of our universe
459
00:25:36,973 --> 00:25:40,444
until we understand the nature
of dark energy.
460
00:25:42,045 --> 00:25:44,914
May 2009.
461
00:25:44,915 --> 00:25:48,519
The european space agency
launches the planck satellite
462
00:25:48,520 --> 00:25:52,421
to search for the birth
of dark energy.
463
00:25:52,422 --> 00:25:56,892
Its ultra-sensitive telescope
peers through space and time
464
00:25:56,893 --> 00:25:59,428
back through billions of years,
465
00:25:59,429 --> 00:26:04,000
towards the beginning of
everything, to capture this.
466
00:26:04,001 --> 00:26:06,503
This is our universe
as it appeared
467
00:26:06,504 --> 00:26:09,438
over 13 billion years ago,
468
00:26:09,439 --> 00:26:13,477
380,000 years
after the big bang.
469
00:26:15,045 --> 00:26:17,647
So what planck has done
is take a picture
470
00:26:17,648 --> 00:26:19,916
of the early universe
471
00:26:19,917 --> 00:26:23,052
and told us about what
the early universe is like
472
00:26:23,053 --> 00:26:25,488
and given us our most detailed
and accurate picture
473
00:26:25,489 --> 00:26:26,822
of that moment in time.
474
00:26:26,823 --> 00:26:29,257
The universe in this picture
475
00:26:29,258 --> 00:26:33,764
is a hot soup of protons,
electrons, and photons.
476
00:26:33,765 --> 00:26:36,832
Hydrogen atoms have just started
to form,
477
00:26:36,833 --> 00:26:39,569
and it's the light from this
genesis of matter
478
00:26:39,570 --> 00:26:41,438
that we see here.
479
00:26:43,507 --> 00:26:46,744
Blue areas are colder.
Reds are warm.
480
00:26:46,878 --> 00:26:48,980
Eventually, those hot spots,
481
00:26:48,981 --> 00:26:51,182
those red spots you see
in the map,
482
00:26:51,183 --> 00:26:53,818
are going to form large
superclusters
483
00:26:53,819 --> 00:26:58,290
made up of hundreds or thousands
of galaxies.
484
00:26:58,291 --> 00:27:02,427
Each one of those galaxies will
contain billions of stars.
485
00:27:04,061 --> 00:27:06,364
Gravity
and expansion alone
486
00:27:06,365 --> 00:27:11,068
appear to drive the formation
of these embryonic galaxies.
487
00:27:11,069 --> 00:27:15,339
Dark energy doesn't seem
to have switched on yet.
488
00:27:15,340 --> 00:27:20,178
So, when did dark energy take
control of the universe?
489
00:27:26,685 --> 00:27:29,887
Astronomer brenda frye
is part of a team
490
00:27:29,888 --> 00:27:32,491
using massive
ground-based telescopes
491
00:27:32,492 --> 00:27:35,292
like this one at kitt peak,
arizona.
492
00:27:35,293 --> 00:27:39,664
She peers back in time
to capture the universe
493
00:27:39,665 --> 00:27:42,569
through its childhood
as it was growing.
494
00:27:44,604 --> 00:27:47,172
Right.
So this is an aluminum plate,
495
00:27:47,173 --> 00:27:51,375
and into this plate are
drilled 640 individual holes.
496
00:27:51,376 --> 00:27:54,445
Each one is put at a very
specific place on the mask
497
00:27:54,446 --> 00:27:58,517
which will correspond to one
particular galaxy in the sky.
498
00:28:00,886 --> 00:28:02,619
During each observation,
499
00:28:02,620 --> 00:28:07,125
the light from 640 individual
galaxies is collected
500
00:28:07,126 --> 00:28:10,529
using fiber optic cables.
501
00:28:10,530 --> 00:28:13,999
The speed and relative position
of each galaxy is measured
502
00:28:14,000 --> 00:28:17,871
to pinpoint exactly where it is
in space.
503
00:28:17,972 --> 00:28:20,607
So far, the team
has accurately mapped
504
00:28:20,608 --> 00:28:23,443
around a million galaxies
in 3d,
505
00:28:23,444 --> 00:28:25,312
and this is what they look like.
506
00:28:26,546 --> 00:28:29,182
Each one of these fuzzy patches
507
00:28:29,183 --> 00:28:31,016
is a fully grown galaxy
508
00:28:31,017 --> 00:28:35,053
containing around
200 billion stars.
509
00:28:35,054 --> 00:28:36,723
This is a very basic
measurement,
510
00:28:36,724 --> 00:28:38,890
and we think that
this will be able to help us
511
00:28:38,891 --> 00:28:41,895
to get a grasp into the nature
of dark energy.
512
00:28:41,896 --> 00:28:46,197
Scientists compare
this adolescent universe
513
00:28:46,198 --> 00:28:48,067
to its baby pictures.
514
00:28:48,068 --> 00:28:50,302
It shows dark energy emerging
515
00:28:50,303 --> 00:28:53,508
when the universe is
half as old as it is today.
516
00:28:54,776 --> 00:28:57,511
About 8 billion years
after the big bang,
517
00:28:57,512 --> 00:29:01,748
this expansion of the universe
begins to accelerate,
518
00:29:01,749 --> 00:29:04,384
and we're in the middle
of this acceleration.
519
00:29:04,385 --> 00:29:09,089
The data also shows
that as space expands,
520
00:29:09,090 --> 00:29:13,726
dark energy
increases in lockstep with it.
521
00:29:13,727 --> 00:29:16,062
If you had a box and you put
some dark energy in it,
522
00:29:16,063 --> 00:29:18,398
and then you went and you
weighed that box...
523
00:29:18,399 --> 00:29:20,300
Now you take the box,
you make it twice as big.
524
00:29:20,301 --> 00:29:22,168
You don't open it.
You don't put anything in it.
525
00:29:22,169 --> 00:29:24,705
You weigh it again, it's gonna
weigh twice as much.
526
00:29:24,706 --> 00:29:27,041
This remarkable
observation means
527
00:29:27,042 --> 00:29:30,511
that we should be safe
from a big rip.
528
00:29:30,512 --> 00:29:33,947
Dark energy will continue
to increase gradually.
529
00:29:33,948 --> 00:29:37,516
The universe is heading
for a big freeze,
530
00:29:37,517 --> 00:29:41,554
and scientists can finally
calculate a timeline
531
00:29:41,555 --> 00:29:44,425
for the end of everything.
532
00:29:53,602 --> 00:29:55,137
It now seems
that we live
533
00:29:55,138 --> 00:29:57,772
in an almost perfect universe,
534
00:29:57,773 --> 00:30:01,342
with just enough gravity
to hold the galaxies together
535
00:30:01,343 --> 00:30:05,248
and just enough dark energy
that it will expand forever
536
00:30:05,249 --> 00:30:07,885
without ripping itself
to shreds.
537
00:30:09,820 --> 00:30:14,492
Cosmologists can finally
envision the end of it all.
538
00:30:15,826 --> 00:30:18,394
30 years ago,
It was debatable.
539
00:30:18,395 --> 00:30:21,262
But now, it appears
that the universe most likely
540
00:30:21,263 --> 00:30:22,831
will suffer a deep freeze.
541
00:30:22,832 --> 00:30:26,137
If you look at the data,
it stares out at you.
542
00:30:27,303 --> 00:30:28,870
In a big freeze,
543
00:30:28,871 --> 00:30:33,009
dark energy pushes galaxies
further and further apart,
544
00:30:33,010 --> 00:30:35,880
but they remain intact.
545
00:30:35,913 --> 00:30:39,583
The stars inside them
fade away.
546
00:30:39,584 --> 00:30:42,119
Every star you see in the sky,
including our sun,
547
00:30:42,120 --> 00:30:44,222
is burning through
its nuclear fuel.
548
00:30:44,223 --> 00:30:47,423
The gas will run out,
stars will stop being made,
549
00:30:47,424 --> 00:30:51,062
and the ones that exist are it.
those are the last ones.
550
00:30:55,467 --> 00:30:57,767
A hundred trillion
years from now,
551
00:30:57,768 --> 00:31:02,073
the biggest stars will be
the first to go extinct.
552
00:31:02,074 --> 00:31:05,208
Big stars burn bright
and die hard.
553
00:31:05,209 --> 00:31:09,647
The star's core collapses,
554
00:31:09,648 --> 00:31:11,784
unleashing a supernova.
555
00:31:13,084 --> 00:31:16,420
Then gravity crushes
the dead star down
556
00:31:16,421 --> 00:31:19,090
to a single dense spot.
557
00:31:19,091 --> 00:31:22,527
The bright star
is now a black hole.
558
00:31:24,897 --> 00:31:27,467
Sun-like stars go next.
559
00:31:28,934 --> 00:31:31,535
As their supply of hydrogen
runs out,
560
00:31:31,536 --> 00:31:33,905
they swell to a bloated fireball
561
00:31:33,906 --> 00:31:36,842
over 200 times
their current size.
562
00:31:42,715 --> 00:31:44,950
And when the core
has no more hydrogen,
563
00:31:44,951 --> 00:31:48,220
it's going to bloat up
into a red giant star.
564
00:31:48,221 --> 00:31:50,589
Now, red giant stars are so big,
they will actually
565
00:31:50,590 --> 00:31:52,590
eat up their own planets.
566
00:31:52,591 --> 00:31:54,425
We know of examples
of red giants
567
00:31:54,426 --> 00:31:56,494
that go all the way out
to where the orbit of jupiter is
568
00:31:56,495 --> 00:31:58,429
in our solar system.
569
00:31:58,430 --> 00:32:01,399
Its fuel exhausted,
570
00:32:01,400 --> 00:32:04,102
the sun-like star
gives in to gravity
571
00:32:04,103 --> 00:32:06,204
and shrinks to a white dwarf,
572
00:32:06,205 --> 00:32:07,973
a dense ball of matter
573
00:32:07,974 --> 00:32:11,108
just a few thousand miles
in diameter.
574
00:32:11,109 --> 00:32:15,147
It will glow with heat
for a further 10 billion years
575
00:32:15,148 --> 00:32:17,715
before cooling to a black dwarf,
576
00:32:17,716 --> 00:32:22,755
a ball of compressed carbon,
perhaps even diamond.
577
00:32:25,459 --> 00:32:27,793
As the biggest stars die,
578
00:32:27,794 --> 00:32:31,330
the universe
will slowly turn red.
579
00:32:31,331 --> 00:32:33,098
The blue stars
will blow up,
580
00:32:33,099 --> 00:32:35,267
and then the slightly less blue
stars will blow up,
581
00:32:35,268 --> 00:32:37,636
and then stars like the sun
will fade away and die,
582
00:32:37,637 --> 00:32:40,308
leaving just the red stars
to exist.
583
00:32:41,876 --> 00:32:43,711
Red stars
are the smallest
584
00:32:43,712 --> 00:32:45,613
and coolest in the universe.
585
00:32:45,614 --> 00:32:47,882
They burn their fuel slowly.
586
00:32:47,883 --> 00:32:50,616
But, after another
10 trillion years,
587
00:32:50,617 --> 00:32:53,020
even these smallest
of dwarf stars
588
00:32:53,021 --> 00:32:55,289
will use up their fuel.
589
00:32:55,290 --> 00:32:58,858
Stars as we know them
will cease to burn energy,
590
00:32:58,859 --> 00:33:01,328
and the night sky
will turn black.
591
00:33:01,329 --> 00:33:05,199
Black holes,
the corpses of dead stars,
592
00:33:05,200 --> 00:33:09,838
and cold clouds of gas and dust
are all that remains.
593
00:33:11,640 --> 00:33:14,409
The age of stars is over.
594
00:33:14,410 --> 00:33:18,145
The age of black holes begins.
595
00:33:18,146 --> 00:33:20,348
Black holes become
the fundamental building block
596
00:33:20,349 --> 00:33:22,015
of the universe.
597
00:33:22,016 --> 00:33:24,384
A galaxy will basically be
a supermassive black hole
598
00:33:24,385 --> 00:33:26,419
in the center, with smaller
black holes orbiting it.
599
00:33:26,420 --> 00:33:28,955
In some ways, it's kind of
a ghost universe.
600
00:33:28,956 --> 00:33:30,792
It's the corpses,
the zombie stars,
601
00:33:30,793 --> 00:33:32,493
that will take us
into the future.
602
00:33:32,494 --> 00:33:35,663
Zombie galaxies
filled with black holes
603
00:33:35,664 --> 00:33:37,464
continue to evolve.
604
00:33:37,465 --> 00:33:40,835
They sweep up the dead remains
of stars.
605
00:33:40,836 --> 00:33:44,939
Black hole merges
with black hole.
606
00:33:44,940 --> 00:33:47,040
They'll eat each other
and they'll get bigger,
607
00:33:47,041 --> 00:33:48,875
and maybe they'll fall into
the supermassive black hole
608
00:33:48,876 --> 00:33:50,344
and it'll get bigger.
609
00:33:50,345 --> 00:33:53,346
The universe will still be
an exciting, dynamic place,
610
00:33:53,347 --> 00:33:55,649
it's just that the time scales
you're talking about
611
00:33:55,650 --> 00:33:57,218
are now trillions of years
612
00:33:57,219 --> 00:33:59,920
instead of thousands
or millions of years.
613
00:33:59,921 --> 00:34:04,091
Any material that
evades the pull of a black hole
614
00:34:04,092 --> 00:34:09,362
eventually dies away
as its protons disintegrate.
615
00:34:09,363 --> 00:34:12,500
A proton, one of the fundamental
building blocks
616
00:34:12,501 --> 00:34:15,335
of atomic matter,
of what makes us up,
617
00:34:15,336 --> 00:34:17,837
can just spontaneously
fall apart,
618
00:34:17,838 --> 00:34:21,710
and it turns out this takes
a tremendously long time.
619
00:34:21,711 --> 00:34:23,810
but even that will go away.
620
00:34:23,811 --> 00:34:28,882
All that will be left
is a sea of black holes.
621
00:34:28,883 --> 00:34:32,152
Scientists used to think
black holes were immortal,
622
00:34:32,153 --> 00:34:33,823
but even these will one day die.
623
00:34:33,924 --> 00:34:36,625
Now we're talking about
time scales
624
00:34:36,626 --> 00:34:38,294
of unimaginable length --
625
00:34:38,295 --> 00:34:40,831
quadrillions of years
into the future.
626
00:34:40,932 --> 00:34:42,398
But on that time scale,
627
00:34:42,399 --> 00:34:46,501
even the black holes
begin to evaporate.
628
00:34:46,502 --> 00:34:48,738
They'll get smaller and smaller
and smaller,
629
00:34:48,739 --> 00:34:50,673
and then, poof, they'll be gone.
630
00:34:50,674 --> 00:34:53,142
The universe will end
631
00:34:53,143 --> 00:34:55,977
when the last remaining
black hole dies.
632
00:34:55,978 --> 00:34:58,780
As it gets smaller,
the evaporation rate
633
00:34:58,781 --> 00:35:00,816
increases exponentially.
634
00:35:00,817 --> 00:35:03,017
Before long,
it reaches a size
635
00:35:03,018 --> 00:35:08,023
a billionth of a trillionth
of a trillionth of an inch.
636
00:35:08,024 --> 00:35:11,427
At that instant,
the laws of physics break down,
637
00:35:11,428 --> 00:35:15,597
and the last black hole explodes
in a flash of gamma rays,
638
00:35:15,598 --> 00:35:18,367
leaving nothing.
639
00:35:18,368 --> 00:35:21,970
And it will die
in a sudden burst of light,
640
00:35:21,971 --> 00:35:23,639
the last burst of light
641
00:35:23,640 --> 00:35:25,975
in the entire history
of the universe.
642
00:35:26,611 --> 00:35:28,612
The big freeze is coming.
643
00:35:28,613 --> 00:35:32,916
The universe will suffer a cold,
slow, dark death
644
00:35:32,917 --> 00:35:34,284
which will play out
645
00:35:34,285 --> 00:35:38,021
over trillions upon trillions
of years.
646
00:35:38,022 --> 00:35:41,425
But quantum physics leaves
the door open
647
00:35:41,426 --> 00:35:43,193
for an alternative end,
648
00:35:43,194 --> 00:35:46,630
an event so powerful,
so destructive,
649
00:35:46,631 --> 00:35:52,336
that it could destroy everything
we see in the blink of an eye.
650
00:35:52,337 --> 00:35:55,507
And it could happen tomorrow.
651
00:36:04,751 --> 00:36:06,585
The end of the universe --
652
00:36:06,586 --> 00:36:08,118
it's coming.
653
00:36:08,119 --> 00:36:11,522
Dark energy accelerates
the space between galaxies,
654
00:36:11,523 --> 00:36:15,093
pushing everything we see
to a long, cold,
655
00:36:15,094 --> 00:36:17,830
and very slow death.
656
00:36:17,831 --> 00:36:21,699
Unless, that is, something
bizarre happens first.
657
00:36:21,700 --> 00:36:25,504
A monster called
phase transition
658
00:36:25,505 --> 00:36:27,138
is lurking in the shadows,
659
00:36:27,139 --> 00:36:31,076
and it could annihilate
the fabric of space and time
660
00:36:31,077 --> 00:36:34,178
at any moment.
661
00:36:34,179 --> 00:36:37,949
When we cool down water,
it turns into ice.
662
00:36:37,950 --> 00:36:39,451
The properties change.
663
00:36:39,452 --> 00:36:41,654
If you lived in the water,
when it changed to ice,
664
00:36:41,655 --> 00:36:43,489
your world
would be very different.
665
00:36:43,490 --> 00:36:48,694
Water phase changes
into ice when it loses energy.
666
00:36:48,695 --> 00:36:51,730
I once left a water
bottle in my car overnight.
667
00:36:51,731 --> 00:36:54,632
It was still liquid,
but the moment i touched it,
668
00:36:54,633 --> 00:36:56,033
the slight imperfection,
669
00:36:56,034 --> 00:36:57,902
the little bit of ice
that it formed, spread,
670
00:36:57,903 --> 00:36:59,770
poof, and filled up
the whole bottle.
671
00:36:59,771 --> 00:37:02,974
That rapid change
to something new
672
00:37:02,975 --> 00:37:05,144
is called a phase transition,
673
00:37:05,145 --> 00:37:10,548
and bizarrely, the same thing
could happen to empty space.
674
00:37:10,549 --> 00:37:13,253
We've really come to understand
675
00:37:13,254 --> 00:37:16,456
that we shouldn't take
for granted that...vacuum,
676
00:37:16,457 --> 00:37:19,191
what we call nothing,
is actually stable.
677
00:37:19,192 --> 00:37:22,094
It could be that the energy
stored in empty space
678
00:37:22,095 --> 00:37:24,898
is just waiting to be released
in a phase transition.
679
00:37:24,899 --> 00:37:28,035
If it is, the laws of physics
will change.
680
00:37:29,904 --> 00:37:33,606
A spontaneous glitch
in the fabric of space-time
681
00:37:33,607 --> 00:37:37,510
could trigger
a phase transition of space,
682
00:37:37,511 --> 00:37:41,914
a tiny bubble of new universe
that spreads out,
683
00:37:41,915 --> 00:37:44,215
overwriting the old.
684
00:37:44,216 --> 00:37:47,887
We know it can happen,
because it's happened before.
685
00:37:51,692 --> 00:37:53,693
At the moment of the big bang,
686
00:37:53,694 --> 00:37:55,762
the universe
that's first created
687
00:37:55,763 --> 00:37:59,132
is completely different
to the one we see today.
688
00:37:59,133 --> 00:38:02,068
Hot and without form,
689
00:38:02,069 --> 00:38:04,670
there's no matter, no time.
690
00:38:04,671 --> 00:38:08,240
The laws of physics
are different.
691
00:38:08,241 --> 00:38:11,945
Suddenly, less than a trillionth
of a second later,
692
00:38:11,946 --> 00:38:15,014
a glitch triggers
a phase transition.
693
00:38:15,015 --> 00:38:18,652
A tiny bubble of the universe
we live in today forms,
694
00:38:18,653 --> 00:38:20,887
and it races outward,
695
00:38:20,888 --> 00:38:22,856
destroying everything it touches
696
00:38:22,857 --> 00:38:26,025
like ice
spreading through water.
697
00:38:26,026 --> 00:38:29,762
The energy that spills out
creates the space and time
698
00:38:29,763 --> 00:38:31,398
that we exist in,
699
00:38:31,399 --> 00:38:36,003
the building blocks of matter
and the forces that govern them.
700
00:38:36,004 --> 00:38:38,739
All that energy was released,
producing all the matter
701
00:38:38,740 --> 00:38:40,675
and radiation we observe
in the universe today.
702
00:38:40,875 --> 00:38:43,711
The old universe
gives up its energy
703
00:38:43,712 --> 00:38:45,347
to create the new.
704
00:38:45,348 --> 00:38:47,482
But it holds some back.
705
00:38:47,483 --> 00:38:51,919
The vacuum of space
still has energy bound to it.
706
00:38:51,920 --> 00:38:56,457
Perhaps this is the dark energy
we see today.
707
00:38:56,458 --> 00:38:59,761
Physicists believe
that someday in the future,
708
00:38:59,762 --> 00:39:03,263
a brand new glitch in the fabric
of space-time
709
00:39:03,264 --> 00:39:05,800
may trigger another
phase transition,
710
00:39:05,801 --> 00:39:09,370
one that wipes us
and everything we see
711
00:39:09,371 --> 00:39:11,305
out of existence.
712
00:39:11,306 --> 00:39:14,809
This is a way to destroy
an entire universe,
713
00:39:14,810 --> 00:39:16,577
because within your universe
714
00:39:16,578 --> 00:39:19,079
are the seeds
of its own destruction.
715
00:39:19,080 --> 00:39:22,050
It would spread out at the speed
of light in a death bubble,
716
00:39:22,051 --> 00:39:25,019
ruining all the galaxies
as it passes through,
717
00:39:25,020 --> 00:39:28,322
and ultimately completely
destroying our universe.
718
00:39:28,323 --> 00:39:31,827
Nothing can survive
the expanding phase transition.
719
00:39:31,828 --> 00:39:36,632
Planets, nebulas, galaxies --
all are ripped apart
720
00:39:36,633 --> 00:39:38,934
as the boundary
of the bubble reaches them.
721
00:39:38,935 --> 00:39:42,170
Inside this bubble,
protons are unstable,
722
00:39:42,171 --> 00:39:46,007
atoms begin to rearrange
in a new form of matter.
723
00:39:46,008 --> 00:39:48,043
As these bubbles
begin to expand,
724
00:39:48,044 --> 00:39:50,679
a new universe is being born
725
00:39:50,680 --> 00:39:53,347
in the corpse
of the old universe,
726
00:39:53,348 --> 00:39:56,686
and the beginning
of a new law of physics.
727
00:39:56,887 --> 00:40:00,522
And so, the expanding universe
we now see
728
00:40:00,523 --> 00:40:03,960
may end in a phase transition,
but we won't know what hit us,
729
00:40:03,961 --> 00:40:05,895
'cause the laws of physics
will change,
730
00:40:05,896 --> 00:40:08,631
and we will essentially most
likely disappear
731
00:40:08,632 --> 00:40:10,399
at the instant it happens.
732
00:40:10,400 --> 00:40:14,069
This bubble will expand
at the speed of light,
733
00:40:14,070 --> 00:40:15,939
and as the bubble passes you,
734
00:40:15,940 --> 00:40:18,975
all the atoms of your body
rearrange themselves,
735
00:40:18,976 --> 00:40:20,678
and you would never know it.
736
00:40:20,679 --> 00:40:23,379
You would have no warning,
because the bubble itself
737
00:40:23,380 --> 00:40:24,948
is expanding
at the speed of light.
738
00:40:24,949 --> 00:40:27,552
You can't predict precisely
when it could happen.
739
00:40:27,553 --> 00:40:29,184
You only have a probability.
740
00:40:29,185 --> 00:40:31,421
So what you really
are predicting is a rate.
741
00:40:31,422 --> 00:40:34,592
Does it happen once a year?
Once every 10 billion years?
742
00:40:34,593 --> 00:40:36,825
Once every googol years?
Or whatever.
743
00:40:36,826 --> 00:40:40,128
It's very possible that
these bubbles get nucleated
744
00:40:40,129 --> 00:40:43,767
and grow about once every
10 or 20 billion years.
745
00:40:43,768 --> 00:40:46,403
So it hasn't happened yet
because we got lucky.
746
00:40:46,404 --> 00:40:49,340
It's unlikely it would happen
the next year or the next day,
747
00:40:49,341 --> 00:40:51,408
but the laws of physics
absolutely allow it.
748
00:40:54,745 --> 00:40:59,016
A phase change
may happen, or it may not.
749
00:41:00,150 --> 00:41:04,290
The universe plays its cards
close to its chest.
750
00:41:08,125 --> 00:41:11,329
And, like dark energy
and dark matter,
751
00:41:11,330 --> 00:41:13,299
there may be more surprises
to come...
752
00:41:15,100 --> 00:41:19,970
...surprises that will only
Add to the mystery and wonder
753
00:41:19,971 --> 00:41:22,608
our universe holds for us.
754
00:41:25,978 --> 00:41:27,613
Whatever the universe
is up to,
755
00:41:27,614 --> 00:41:28,979
we still don't know enough.
756
00:41:28,980 --> 00:41:31,082
We're in an age of discovery
right now.
757
00:41:31,083 --> 00:41:32,983
Perhaps there is something else
out there
758
00:41:32,984 --> 00:41:34,352
that we don't know about.
759
00:41:34,353 --> 00:41:36,755
So, i'm not going to draw
any conclusions
760
00:41:36,756 --> 00:41:38,457
until things are conclusive.
761
00:41:41,159 --> 00:41:43,660
We don't understand
the nature of dark energy.
762
00:41:43,661 --> 00:41:47,265
And without that understanding,
virtually anything is possible.
763
00:41:47,266 --> 00:41:49,300
The future is still uncertain,
764
00:41:49,301 --> 00:41:51,635
and that means
there's still a mystery.
765
00:41:51,636 --> 00:41:55,007
And for me, that's the most
exciting possibility of all.
766
00:41:55,057 --> 00:41:59,607
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