All language subtitles for Universe (1960) Roman Kroitor, Colin Low
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1
00:01:01,420 --> 00:01:06,320
The ground beneath our feet is the
surface of a planet whirling at
2
00:01:06,320 --> 00:01:08,780
miles an hour around a distant sun.
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00:01:11,020 --> 00:01:16,560
Our life is possible only because of the
light and warmth of that sun, a star.
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00:01:17,620 --> 00:01:22,880
Yet the sun which shines on us is only
one out of billions of such stars in the
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00:01:22,880 --> 00:01:23,880
universe.
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00:01:40,720 --> 00:01:45,760
This is one of the world's major
observatories, the David Dunlap
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00:01:45,760 --> 00:01:46,940
miles north of Toronto.
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00:01:48,460 --> 00:01:52,360
Dr. Donald McRae is a professor of
astronomy at the University of Toronto.
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00:01:58,240 --> 00:02:02,620
Observatory. At any moment scattered
throughout the world, there are hundreds
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00:02:02,620 --> 00:02:06,900
men and women observing the heavens with
optical and radio telescopes, gathering
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00:02:06,900 --> 00:02:09,660
data for the solution of many questions
about the universe.
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00:02:10,979 --> 00:02:12,420
routine work for the most part.
13
00:02:13,800 --> 00:02:18,040
McRae's job tonight, if the sky remains
clear, will be to take photographs of
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00:02:18,040 --> 00:02:19,440
six stars with the telescope.
15
00:02:43,400 --> 00:02:47,880
A mirror over six feet in diameter, with
its surface shape to within one
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00:02:47,880 --> 00:02:51,240
millionth of an inch, will catch the
light from a star.
17
00:02:56,580 --> 00:03:01,440
This light will be reflected from the
large mirror onto a smaller one, which
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00:03:01,440 --> 00:03:04,420
turn will focus it back into a camera at
the base of the telescope.
19
00:03:27,820 --> 00:03:32,240
Out of the study of hundreds of
thousands of observations, astronomers
20
00:03:32,240 --> 00:03:34,460
pieced together an accurate picture of
the universe.
21
00:03:57,160 --> 00:04:03,260
Beyond the appearance of starshine and
moonbeam, what will the first men to
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00:04:03,260 --> 00:04:04,260
leave the earth find?
23
00:04:06,200 --> 00:04:10,820
Enough is now known that we can, in
imagination, journey into these spaces.
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00:04:26,730 --> 00:04:29,850
250 ,000 miles away, the moon.
25
00:04:31,330 --> 00:04:35,890
This is the moon that men have
worshipped as a goddess, that countless
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00:04:35,890 --> 00:04:37,790
have sighed over and sworn by.
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00:04:46,130 --> 00:04:51,550
It will take immense courage to journey
to this place, for on this pitted and
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00:04:51,550 --> 00:04:54,990
pocked ball of pumice and stone there is
no atmosphere.
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00:04:56,620 --> 00:04:59,660
No air to breathe, no sound to hear.
30
00:05:07,760 --> 00:05:12,520
By day, the sun's heat would boil water,
if there were water.
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00:05:15,700 --> 00:05:19,480
At night, 240 degrees below zero.
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00:05:29,330 --> 00:05:31,370
Unshielded, a man couldn't live here for
two minutes.
33
00:05:32,190 --> 00:05:37,290
But if he were to die, his body would
lie unchanged through thousands of
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00:05:37,510 --> 00:05:42,030
for nothing grows and nothing decays.
35
00:05:47,970 --> 00:05:53,350
If you were to hover in space beyond the
moon, speeding up in imagination its
36
00:05:53,350 --> 00:05:56,890
movement, you would see a majestic
procession in the sky.
37
00:05:58,600 --> 00:06:03,420
As the moon circles the earth, so the
earth itself circles the sun.
38
00:06:17,720 --> 00:06:23,440
The sun is the center of a system of
nine heavenly bodies, called planets,
39
00:06:23,440 --> 00:06:27,360
wheel around it in vast orbits trapped
by its gravitational pull.
40
00:06:29,060 --> 00:06:31,820
closest to it, the tiny planet, Mercury.
41
00:06:36,800 --> 00:06:41,600
On the surface of Mercury, the
temperature is hot enough to melt lead,
42
00:06:41,600 --> 00:06:45,620
face of it is turned perpetually to the
sun, only 36 million miles away.
43
00:06:57,230 --> 00:07:01,630
If we looked outward from Mercury, we
would see the second closest planet,
44
00:07:01,810 --> 00:07:05,610
Venus, shining brighter than the much
more distant stars.
45
00:07:06,890 --> 00:07:13,610
Venus, in orbit 31 million miles further
out from the Sun, is a mystery, for its
46
00:07:13,610 --> 00:07:18,030
face is veiled by dust storms, or
perhaps dense cloud.
47
00:07:22,350 --> 00:07:23,990
Looking outward from Venus,
48
00:07:24,700 --> 00:07:29,020
The most brilliant and beautiful object
in the sky would be a planet in orbit 25
49
00:07:29,020 --> 00:07:31,040
million miles still further out.
50
00:07:31,940 --> 00:07:32,940
Earth.
51
00:07:47,760 --> 00:07:51,800
Beyond Earth, shining redly in the
night, Mars.
52
00:07:53,420 --> 00:07:58,860
Colder than Earth and smaller, this is
the planet men have looked on and
53
00:07:58,860 --> 00:08:01,140
wondered whether they are alone in the
heavens.
54
00:08:05,060 --> 00:08:10,020
It is reasonably certain that the
markings on its surface, bluish green in
55
00:08:10,020 --> 00:08:14,560
Martian summer turning rusty brown in
the autumn, indicate vegetation.
56
00:08:20,300 --> 00:08:25,740
Here, however, the atmosphere has almost
no oxygen, and no creatures like men
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00:08:25,740 --> 00:08:29,400
could live here, 140 million miles from
the sun.
58
00:08:43,940 --> 00:08:49,090
In the place past Mars, where there
should theoretically be a planet, There
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00:08:49,090 --> 00:08:55,810
only the asteroids, small bodies ranging
from boulders to chunks 300 miles
60
00:08:55,810 --> 00:09:00,010
across, hundreds of them swinging in
orbit about the sun.
61
00:09:23,850 --> 00:09:29,710
500 million miles out from the Sun, the
giant planet Jupiter, ruling 12 moons.
62
00:09:36,830 --> 00:09:42,310
Jupiter, seen here from one of its
moons, is larger than all the other
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00:09:42,310 --> 00:09:43,310
put together.
64
00:09:43,490 --> 00:09:49,310
Its atmosphere is a thousand miles deep,
a poisonous mixture of methane gas,
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00:09:49,650 --> 00:09:51,090
ammonia and hydrogen.
66
00:09:51,870 --> 00:09:54,330
which at the bottom must have the
density of water.
67
00:10:01,050 --> 00:10:06,030
Here, under the enormous pressure of the
atmosphere, a human being would be
68
00:10:06,030 --> 00:10:07,070
crushed beyond recognition.
69
00:10:16,790 --> 00:10:18,670
These are the rings of Saturn.
70
00:10:19,720 --> 00:10:25,940
Bands 10 ,000 miles wide, composed of
almost an infinity of meteoric particles
71
00:10:25,940 --> 00:10:29,420
of gravel and ice circling the sixth
planet.
72
00:10:34,460 --> 00:10:39,860
Saturn, with its nine moons, is so far
from the sun that it takes 30 Earth
73
00:10:39,860 --> 00:10:40,860
to circle it.
74
00:10:41,420 --> 00:10:45,920
And here the temperature never rises
above 240 degrees below zero.
75
00:10:51,720 --> 00:10:57,640
And if we were to plunge still further
out, hundreds of millions of miles, past
76
00:10:57,640 --> 00:11:04,340
the planet Uranus, beyond Neptune, we
would finally come to the last of the
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00:11:04,340 --> 00:11:10,580
known planets, to the dwarf Pluto, named
for the god of the underworld.
78
00:11:14,260 --> 00:11:19,180
Its surface moves in perpetual darkness
and unimaginable cold.
79
00:11:20,270 --> 00:11:25,650
For the sun is four billion miles away,
only a starry speck in the sky.
80
00:11:54,589 --> 00:11:58,950
Sometimes a strange apparition appears
in the sky, a comet.
81
00:12:03,070 --> 00:12:09,610
Like a planet, a comet orbits the sun,
but it is only a loose conglomeration of
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00:12:09,610 --> 00:12:16,050
ice and dust, invisible, until its head
comes close enough to the sun, whose
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00:12:16,050 --> 00:12:20,890
rays then excite it into fluorescence,
and push away from the head a vaporous
84
00:12:20,890 --> 00:12:23,730
tail, which may become a million miles
long.
85
00:12:37,420 --> 00:12:43,600
For a few weeks, a comet blossoms, and
then, passing the sun, it will fade and
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00:12:43,600 --> 00:12:50,000
coast again, unseen, billions of miles
into the darkness, perhaps not to return
87
00:12:50,000 --> 00:12:53,280
for a century to the blazing star, which
is its master.
88
00:13:05,680 --> 00:13:12,180
The sun is an unimaginable inferno, a
thermonuclear furnace churning with the
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00:13:12,180 --> 00:13:17,600
storms we see as sunspots, heaving from
its surface columns of gas that arch 300
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00:13:17,600 --> 00:13:23,180
,000 miles into space, pulled and
twisted by enormous electrical and
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00:13:23,180 --> 00:13:24,180
fields.
92
00:13:40,330 --> 00:13:46,150
The sun produces the energy of a million
hydrogen bombs exploding every second.
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So it has raged for five billion years,
and so it will rage for perhaps another
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00:13:54,690 --> 00:13:59,030
five billion years, flooding its planets
with radiant energy.
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00:14:14,890 --> 00:14:18,630
Too near or too far from this furnace,
instant death for men.
96
00:14:19,770 --> 00:14:25,190
Between 91 and 93 million miles from
this star, filtered through a blanket of
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00:14:25,190 --> 00:14:28,730
atmosphere, its energies sustain human
life.
98
00:14:54,930 --> 00:14:55,930
Hey,
99
00:14:56,550 --> 00:14:58,610
what's the matter? You're a striker.
100
00:15:30,700 --> 00:15:35,200
When a particular star is to be
photographed, it is located by its
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00:15:35,200 --> 00:15:36,320
on a star chart.
102
00:15:38,620 --> 00:15:41,800
On such a chart, every black speck is a
star.
103
00:15:44,400 --> 00:15:47,500
146 .7 plus 1349.
104
00:15:52,860 --> 00:15:56,180
Forty -five tons of steel and glass must
be aimed precisely.
105
00:15:57,070 --> 00:16:00,910
at a spot perhaps 200 million billion
miles away.
106
00:16:20,510 --> 00:16:24,350
Many of the stars astronomers study are
invisible to the naked eye.
107
00:16:26,670 --> 00:16:31,690
Even the nearest ones, apart from our
sun, are so far away that their light is
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00:16:31,690 --> 00:16:32,690
very dim.
109
00:16:33,770 --> 00:16:38,010
The mirror in the base of the telescope
gathers and focuses hundreds of
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00:16:38,010 --> 00:16:41,190
thousands of times the amount of light
seen by the naked eye.
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00:17:02,830 --> 00:17:05,050
Almost nothing of a star can be known
directly.
112
00:17:05,730 --> 00:17:07,690
It is a photograph that is studied.
113
00:17:08,010 --> 00:17:12,849
Not a portrait of a star, but a
photograph of its light, split into a
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00:17:12,849 --> 00:17:14,930
in which each band has its meaning.
115
00:17:15,410 --> 00:17:20,490
The presence in that distant star of
elements like iron, calcium, carbon.
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00:17:21,270 --> 00:17:25,410
From a spectroscopic photograph,
astronomers can tell whether a star is
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00:17:25,410 --> 00:17:26,690
towards us or away.
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By exposing on the same plate the
spectrum of the star, and the spectrum
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00:17:32,610 --> 00:17:36,090
iron arc, and measuring the displacement
between the two.
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00:17:48,990 --> 00:17:52,390
To photograph the spectrum of the arc
takes ten seconds.
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To catch enough of the light from the
star may take up to two hours.
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During the exposure, machinery in the
base of the telescope automatically
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00:18:06,490 --> 00:18:11,050
compensates for the rotation of the
Earth, keeping the star centered.
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00:18:28,790 --> 00:18:31,310
If we looked more deeply into space,
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leaving behind us the Earth and the
whole of our solar system, and traveled
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00:18:37,960 --> 00:18:43,280
the speed of light, it would take four
years before we came to even the closest
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00:18:43,280 --> 00:18:46,460
of the billions of suns scattered
through stellar space.
128
00:18:54,020 --> 00:18:58,360
Although the stars are suns, many of
them are unlike our sun.
129
00:19:02,760 --> 00:19:08,300
Some, like Beta in the constellation
Lyra, instead of planets, have a second
130
00:19:08,300 --> 00:19:09,320
swinging around them.
131
00:19:18,840 --> 00:19:22,580
There are multiple suns, like Castor in
the constellation Gemini.
132
00:19:31,400 --> 00:19:37,200
There are giant suns 5 ,000 times as
large as ours, and dwarfs, in which one
133
00:19:37,200 --> 00:19:39,280
cubic inch of matter weighs 40 ton.
134
00:19:45,320 --> 00:19:50,720
Suns rotating so rapidly that pinwheels
of gas are thrown off, weighing more
135
00:19:50,720 --> 00:19:52,300
than our whole system of planets.
136
00:20:05,680 --> 00:20:10,600
Suns that over a period of days or hours
pulse as their internal nuclear
137
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processes change.
138
00:20:14,300 --> 00:20:19,720
Rare suns in which the temperature
reaches 5 billion degrees, where nuclear
139
00:20:19,720 --> 00:20:25,120
fusion makes elements as heavy as iron
and results in the enormous explosion of
140
00:20:25,120 --> 00:20:27,320
a nova or supernova.
141
00:20:49,160 --> 00:20:53,440
The brilliant light from such explosions
floods through the gaseous clouds of
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space for billions on billions of miles.
143
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And the remains of a supernova recorded
ten centuries ago can still be seen as
144
00:21:02,000 --> 00:21:04,860
the Crab Nebula in the constellation
Taurus.
145
00:21:11,100 --> 00:21:15,780
As well as stars, in stellar space there
is gas and dust.
146
00:21:16,810 --> 00:21:22,410
sometimes glowing in starlight,
sometimes dark, obscuring what is behind
147
00:21:27,790 --> 00:21:34,170
Stars, gas, dust, all moving in apparent
chaos.
148
00:21:35,330 --> 00:21:38,530
Until a generation ago, it seemed
indecipherable.
149
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The only suggestion of form was their
grouping in the band we know as the
150
00:21:43,690 --> 00:21:44,690
Way.
151
00:21:55,690 --> 00:21:59,510
Now years of patient work have revealed
a pattern in the universe.
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A pattern beyond anything we could have
imagined looking at the heavens with the
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00:22:04,570 --> 00:22:05,570
naked eye.
154
00:22:06,950 --> 00:22:12,890
With data sifted from countless
painstaking observations, astronomers
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00:22:12,890 --> 00:22:18,350
filling in the details of a pattern so
vast that everyday ideas of distance and
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time cannot encompass it.
157
00:22:26,670 --> 00:22:32,050
If we could move with the freedom of a
god, so that a million years pass in a
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00:22:32,050 --> 00:22:38,810
second, and if we went far enough, past
the nearest suns, beyond the star
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clouds and nebulae, in time they would
end, and as if moving out from behind a
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00:22:45,770 --> 00:22:49,950
curtain, we would come to an endless sea
of night.
161
00:22:59,920 --> 00:23:06,900
In that sea are islands, continents of
stars, that we have named the galaxies.
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00:23:08,720 --> 00:23:14,600
The largest known forms in the universe,
hundreds of billions of suns bound
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together by gravity, rotating around
their common center once in 200 million
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00:23:20,040 --> 00:23:21,040
years.
165
00:23:26,820 --> 00:23:27,980
Our sun.
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with its planets, is near the edge of
one such galaxy, the rim of which we see
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dimly as the Milky Way.
168
00:23:43,130 --> 00:23:47,050
The galaxies are the birthplace and
graveyard of the stars.
169
00:23:47,910 --> 00:23:54,470
Here, gas contracts into knots, becomes
hot, and flares into the life of a sun,
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sometimes forming with it planets.
171
00:23:58,760 --> 00:24:01,360
sometimes planets which must be suitable
for life.
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00:24:03,100 --> 00:24:09,300
And here, too, the stars finally consume
themselves and collapse into cold, dark
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00:24:09,300 --> 00:24:10,300
dwarfs.
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00:24:22,400 --> 00:24:29,010
A hundred billion suns, yet formed so
enormous, that they have been observed
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00:24:29,010 --> 00:24:34,430
slipping through one another like
phantoms, their stars light years apart,
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continuing undisturbed in their courses.
177
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At the very limit of our most powerful
instruments, galaxies still are flung
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00:24:50,010 --> 00:24:54,730
across space, themselves as numerous as
stars in the night sky.
179
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But when we look this deeply into space,
we are looking at a ghostly image of
180
00:25:11,260 --> 00:25:17,000
the distant past, for the light by which
we see these regions started traveling
181
00:25:17,000 --> 00:25:20,380
towards us long before the dawn of life
on earth.
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00:25:30,400 --> 00:25:31,860
In all of time,
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on all the planets of all the galaxies
in space, what civilizations have risen,
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looked into the night, seen what we see,
185
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asked the questions that we ask?
17052
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