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              ¶ ¶

2
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        (sail rustling)

3
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     NEIL DEGRASSE TYSON:
    <i> The dream of becoming</i>
   <i> a citizen of the cosmos</i>

4
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        <i> was born here,</i>
 <i> more than two millennia ago,</i>

5
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  <i> in the city of Alexandria,</i>

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 <i> named after and conceived by</i>
     <i> its dead conqueror,</i>

7
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     <i> Alexander the Great.</i>

8
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 The Ptolemys, the Greek kings

9
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  who inherited the Egyptian
portion of Alexander's empire,

10
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      <i> built this library</i>

11
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      <i> and its associated</i>
    <i> research institution.</i>

12
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       Rarely, if ever,

13
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       before or since,

14
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  has there been a government
   that was willing to spend

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        so much of its
    gross national product

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on the acquisition of knowledge.

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       And it paid off.

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           Big time.

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      Every ship entering
      Alexandria's harbor

20
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        was searched--
      not for contraband,

21
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  but for books that might be
    copied and stored here,

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       in what was then
the greatest library on Earth.

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      Here, Eratosthenes,
 one of the chief librarians,

24
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     accurately calculated
     the size of the Earth

25
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    and invented geography.

26
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          Pythagoras.

27
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           Hypatia.

28
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Euclid.

29
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       Euclid set forth
   the precepts of geometry

30
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  in a textbook that remained
    in use for 2,300 years.

31
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    The Old Testament Bible
       comes down to us

32
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     mainly from the Greek
    translations made here.

33
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   The original manuscripts
      of the masterpieces

34
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           of Greek
   comedy and drama, poetry,

35
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     science, engineering,

36
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    medicine and history--

37
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    the total work product

38
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  of the awakening of ancient
civilization-- were kept here.

39
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        Estimates vary
on the total number of scrolls.

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    They range from 500,000

41
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     to nearly a million.

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       And all of it...

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         <i> all</i> of this

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    is but a tiny fraction
      of the information

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that you have at your fingertips
     at this very moment.

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   <i> The collective knowledge</i>
       <i> of our species,</i>

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      <i> our own electronic</i>
    <i> Library of Alexandria,</i>

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  <i> may be accessed by anyone</i>
       <i> who has a device</i>

49
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       <i> and the interest</i>
  <i> and the freedom to do so.</i>

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      <i> This was not true</i>
        <i> in Alexandria,</i>

51
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   <i> where knowledge belonged</i>
        <i> to the elite.</i>

52
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 <i> So in the fourth century AD,</i>

53
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      <i> when the mob came</i>
    <i> to destroy the library</i>

54
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        <i> and the genius</i>
  <i> of classical civilization,</i>

55
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 <i> there were not enough people</i>
        <i> to defend it.</i>

56
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<i> What will happen the next time</i>
        <i> the mob comes?</i>

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              ¶ ¶

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              ¶ ¶

59
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              ¶ ¶

60
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              ¶ ¶

61
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        DEGRASSE TYSON:
<i> We've come a long way together,</i>

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  <i> traveling from deep inside</i>
     <i> the heart of an atom</i>

63
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          <i> clear out</i>
    <i> to the cosmic horizon,</i>

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and from the beginning of time
    to the distant future.

65
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      I think we're ready
   to perform an experiment.

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It's not the kind of experiment
  that requires a laboratory.

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  You can do it in your head.

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          It's called
    a "thought experiment."

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        <i> Pick a star--</i>

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   <i> any one of the hundreds</i>
     <i> of billions of stars</i>

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   <i> in our Milky Way Galaxy,</i>

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   which is just one galaxy

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  out of the hundred billion
    in the known universe.

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     <i> How about that star?</i>

75
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         <i> Or that one?</i>

76
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       <i> Okay, this one.</i>

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    <i> It's orbited by dozens</i>
    <i> of planets and moons.</i>

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   <i> Suppose, on one of them,</i>

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         <i> there lives</i>
   <i> an intelligent species,</i>

80
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<i> one the ten million life-forms</i>
       <i> on that planet,</i>

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    and there's a subgroup
        of that species

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   who believe they have it
       all figured out--

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  <i> their world is the center</i>
       <i> of the universe,</i>

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  <i> a universe made for them,</i>

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<i> and that they know everything</i>
 <i> they need to know about it--</i>

86
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 <i> their knowledge is complete.</i>

87
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        <i> How seriously</i>
 <i> would you take their claim?</i>

88
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    <i> Our ancestors believed</i>

89
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<i> the universe was made for them.</i>

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   It was natural to assume
  that we were at the center.

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          After all,
it looks like the Sun and stars

92
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    all revolve around us.

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        We still speak
     of the Sun "rising."

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      The architecture of
our language, myths and dreams

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          comes from
    that prescientific age.

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      This is our planet
     as it was known then,

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just before Columbus set sail.

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 This first globe of the Earth
       was cutting-edge

99
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      when Martin Behaim
       made it in 1492.

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Like everyone else, he believed

101
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    that the jigsaw puzzle
  of geography was complete.

102
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 There were three continents:

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   Europe, Africa and Asia,

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and only the great world ocean
          in between.

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 Behaim had no clue that North
and South America even existed.

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It's easy to feel smug, right?

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Well, the fact is Martin Behaim
     knew infinitely more

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  about his world, the Earth,

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   than we know about ours,
         the universe.

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  A recent lesson in humility

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  <i> will serve to illustrate.</i>

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     <i> In 1912, Victor Hess</i>
   <i> made a series of voyages</i>

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 <i> into the sky above Austria,</i>

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     <i> and found the thing</i>
 <i> that scientists love best...</i>

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         <i> ...a mystery</i>
  <i> that defied understanding</i>

116
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   <i> in terms of conventional</i>
      <i> scientific wisdom.</i>

117
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       <i> And even today,</i>

118
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       <i> a century later,</i>
    <i> we are still searching</i>

119
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  <i> for a complete explanation</i>
     <i> of what Hess found.</i>

120
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     <i> A new kind of energy</i>
<i> had recently been discovered:</i>

121
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        <i> radioactivity.</i>

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       <i> It was given off</i>

123
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     <i> by certain elements,</i>
         <i> like radium.</i>

124
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       <i> But it was also</i>
      <i> found in the air,</i>

125
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        <i> even far away</i>
   <i> from radioactive rocks.</i>

126
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      <i> It was everywhere.</i>

127
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        <i> Where did this</i>
  <i> strange energy come from?</i>

128
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         <i> No one knew.</i>

129
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 <i> Hess suspected that it might</i>
  <i> come from above the Earth.</i>

130
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   <i> To test his hypothesis,</i>
<i> he carried radiation detectors</i>

131
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      <i> high into the sky.</i>

132
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    <i> During a risky ascent</i>
    <i> in a hydrogen balloon,</i>

133
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   <i> he attained an altitude</i>
  <i> of more than three miles.</i>

134
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<i> When he reached the thin, cold,</i>

135
00:08:56,185 --> 00:08:58,186
<i> upper half of the atmosphere...</i>

136
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        (wind whistles)

137
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<i> ...he found that the radiation</i>

138
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     <i> was more than twice</i>
 <i> as strong as on the ground.</i>

139
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        <i> The radiation</i>
  <i> must be coming from above.</i>

140
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   <i> That's why its intensity</i>
  <i> was weaker on the ground--</i>

141
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    <i> the Earth's atmosphere</i>
  <i> was absorbing most of it.</i>

142
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<i> Some thought that the radiation</i>
   <i> might come from the Sun.</i>

143
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      <i> To test that idea,</i>
<i> Hess timed one of his ascents</i>

144
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         <i> to coincide</i>
    <i> with a solar eclipse.</i>

145
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     <i> But the eclipse had</i>
 <i> no effect on the radiation.</i>

146
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       <i> Hess also found</i>
      <i> that the radiation</i>

147
00:09:47,003 --> 00:09:50,438
 <i> was just as strong at night</i>
       <i> as in daylight.</i>

148
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  <i> It was coming from above,</i>
    <i> but not from the Sun.</i>

149
00:09:53,142 --> 00:09:55,977
    <i> What Hess did not know</i>

150
00:09:56,012 --> 00:09:59,147
   <i> was that the solar wind</i>
  <i> doesn't move that quickly.</i>

151
00:09:59,181 --> 00:10:01,449
<i> And so, for the wrong reason,</i>

152
00:10:01,484 --> 00:10:04,653
           <i> he came</i>
   <i> to the right conclusion.</i>

153
00:10:04,687 --> 00:10:07,722
      Hess had discovered
         cosmic rays--

154
00:10:07,757 --> 00:10:11,559
showers of subatomic particles
 that crisscross the universe

155
00:10:11,594 --> 00:10:13,962
at literally the speed of light.

156
00:10:13,996 --> 00:10:16,564
 Without the shielding effect
  of the Earth's atmosphere,

157
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     they would be lethal.

158
00:10:18,601 --> 00:10:21,336
       Some cosmic rays
   can carry as much energy

159
00:10:21,370 --> 00:10:23,705
as a bullet fired from a rifle.

160
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     It would take decades
  to trace those cosmic rays

161
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        back to a death
   of unimaginable violence.

162
00:10:41,090 --> 00:10:43,124
DEGRASSE TYSON:<i> The cosmic rays</i>
  <i> that Victor Hess detected</i>

163
00:10:43,126 --> 00:10:46,928
  <i> in the skies above Austria</i>
<i> posed a mystery to scientists.</i>

164
00:10:48,331 --> 00:10:50,598
        <i> Radioactivity</i>
    <i> in minerals on Earth--</i>

165
00:10:50,616 --> 00:10:52,967
      <i> like uranium ore--</i>

166
00:10:53,002 --> 00:10:55,503
<i> comes from the disintegration</i>
          <i> of atoms.</i>

167
00:10:55,538 --> 00:10:58,673
     <i> But cosmic rays were</i>
    <i> of a different nature.</i>

168
00:10:58,708 --> 00:11:01,142
  They were far more powerful

169
00:11:01,177 --> 00:11:03,645
      than anything known
       in Hess's world.

170
00:11:03,679 --> 00:11:05,814
      Scientists wondered
        for two decades

171
00:11:05,831 --> 00:11:08,483
  what could possibly produce
         cosmic rays.

172
00:11:08,517 --> 00:11:12,087
Enter Fritz Zwicky,

173
00:11:12,154 --> 00:11:16,191
the most brilliant man
you've never heard of.

174
00:11:16,225 --> 00:11:19,260
           <i> In 1933,</i>
<i> he and a colleague discovered</i>

175
00:11:19,295 --> 00:11:22,030
   <i> that some stars flare up</i>
     <i> to become as bright</i>

176
00:11:22,064 --> 00:11:24,265
    <i> as their entire galaxy</i>
       <i> for a few weeks,</i>

177
00:11:24,300 --> 00:11:26,701
   <i> before fading out again.</i>

178
00:11:26,736 --> 00:11:28,203
Fritz Zwicky was
the first person

179
00:11:28,237 --> 00:11:30,772
to understand
what just happened.

180
00:11:30,806 --> 00:11:33,775
     He correctly surmised
     that this is the way

181
00:11:33,809 --> 00:11:35,977
     a massive star dies--
           it blows

182
00:11:36,011 --> 00:11:38,046
   <i> its guts out into space.</i>

183
00:11:38,080 --> 00:11:41,850
    <i> He called this kind of</i>
<i> stellar death a "supernova"...</i>

184
00:11:47,056 --> 00:11:49,724
       ...and predicted
that the dying star would shrink

185
00:11:49,759 --> 00:11:52,527
  <i> from about a million miles</i>
     <i> across to only ten.</i>

186
00:11:54,196 --> 00:11:56,131
<i> This corpse would be so dense</i>

187
00:11:56,198 --> 00:11:58,633
   that a single grain of it
      would weigh as much

188
00:11:58,635 --> 00:12:00,368
as the Great Pyramid in Egypt.

189
00:12:00,386 --> 00:12:02,470
It would consist almost entirely

190
00:12:02,505 --> 00:12:04,806
    of subatomic particles
       called neutrons,

191
00:12:04,840 --> 00:12:08,176
  <i> so he named these bizarre</i>
   <i> objects "neutron stars."</i>

192
00:12:08,210 --> 00:12:11,513
  <i> And 35 years after Zwicky</i>
  <i> predicted their existence,</i>

193
00:12:11,547 --> 00:12:13,415
astronomers began to find them.

194
00:12:13,449 --> 00:12:15,350
    We call them "pulsars"

195
00:12:15,384 --> 00:12:18,987
<i> when they spin rapidly and emit</i>
<i> regular pulses of radio energy.</i>

196
00:12:19,021 --> 00:12:21,823
 Supernovas and neutron stars
         could account

197
00:12:21,857 --> 00:12:23,992
for a wide range of cosmic rays,

198
00:12:24,026 --> 00:12:26,528
           <i> but not</i>
   <i> the most energetic ones.</i>

199
00:12:26,562 --> 00:12:28,229
 <i> Nothing yet known to science</i>

200
00:12:28,264 --> 00:12:30,832
       can explain them,
   and we're fine with that.

201
00:12:30,866 --> 00:12:33,201
    It's one of the things
     I love about science,

202
00:12:33,235 --> 00:12:35,837
   we don't have to pretend
   we have all the answers.

203
00:12:35,871 --> 00:12:38,406
     <i> Zwicky also came up</i>
        <i> with the idea</i>

204
00:12:38,441 --> 00:12:41,376
 <i> that the gravity of a galaxy</i>
       <i> warps the fabric</i>

205
00:12:41,443 --> 00:12:43,511
     <i> of space around it,</i>
     <i> to act like a lens.</i>

206
00:12:43,546 --> 00:12:45,780
        <i> This distorts</i>
     <i> and magnifies light</i>

207
00:12:45,815 --> 00:12:48,216
 <i> from any other galaxy lying</i>
     <i> directly behind it.</i>

208
00:12:48,250 --> 00:12:51,853
   <i> So, astronomers on Earth</i>
  <i> would see multiple images</i>

209
00:12:51,887 --> 00:12:54,122
 <i> of that same distant galaxy,</i>

210
00:12:54,156 --> 00:12:57,125
          <i> deformed,</i>
   <i> as in a funhouse mirror.</i>

211
00:12:57,159 --> 00:13:02,831
<i> 40 years after this prediction,</i>
<i> we started finding them, too.</i>

212
00:13:04,600 --> 00:13:08,603
And Zwicky made yet another
discovery back in the 1930s.

213
00:13:08,637 --> 00:13:12,140
        <i> While studying</i>
<i> the Coma Cluster of galaxies,</i>

214
00:13:12,174 --> 00:13:16,644
  <i> he noticed something funny</i>
  <i> about the way they moved.</i>

215
00:13:16,679 --> 00:13:19,881
    The galaxies were going
         way too fast,

216
00:13:19,915 --> 00:13:23,051
so fast that they should've been
 flying apart from each other,

217
00:13:23,085 --> 00:13:25,470
     because all the stars
     in all those galaxies

218
00:13:25,521 --> 00:13:28,923
  had far too little gravity
 to hold the cluster together.

219
00:13:28,958 --> 00:13:30,725
        Zwicky thought

220
00:13:30,792 --> 00:13:33,328
  that something else must be
  binding them to each other.

221
00:13:33,362 --> 00:13:36,164
        That mysterious
       missing component

222
00:13:36,198 --> 00:13:39,467
 would have to weigh something
     like 50 times as much

223
00:13:39,502 --> 00:13:41,102
   as the stars themselves.

224
00:13:41,136 --> 00:13:44,405
But no one paid much attention
     to this wild notion.

225
00:13:44,440 --> 00:13:47,609
       Just another one
   of Zwicky's crazy ideas.

226
00:13:47,643 --> 00:13:49,277
     In our solar system,

227
00:13:49,311 --> 00:13:51,846
the innermost planet, Mercury,
       moves much faster

228
00:13:51,848 --> 00:13:53,848
than the outermost one, Neptune.

229
00:13:53,883 --> 00:13:55,683
 And that makes sense, right?

230
00:13:55,718 --> 00:13:59,087
The harder you push or pull on
something, the faster it goes.

231
00:13:59,121 --> 00:14:02,423
   The Sun's gravity weakens
   with increasing distance,

232
00:14:02,458 --> 00:14:06,828
so, the planets that are farther
from the Sun move more slowly.

233
00:14:06,862 --> 00:14:10,532
  Everyone expected that the
  outermost stars in a galaxy

234
00:14:10,566 --> 00:14:13,201
    would act the same way.

235
00:14:13,235 --> 00:14:16,704
     Most of the stars are
concentrated towards the center,

236
00:14:16,739 --> 00:14:20,008
 so, their collective gravity
   pulls on the other stars

237
00:14:20,042 --> 00:14:23,211
         the same way
 the Sun pulls on the planets.

238
00:14:23,245 --> 00:14:25,647
      <i> But in the 1970s,</i>
       <i> when astronomer</i>

239
00:14:25,681 --> 00:14:28,049
      <i> Vera Rubin studied</i>
    <i> the Andromeda Galaxy,</i>

240
00:14:28,083 --> 00:14:32,620
<i> she discovered that the outer</i>
  <i> stars obeyed no such rule.</i>

241
00:14:32,655 --> 00:14:35,223
   Unlike the outer planets
     of the solar system,

242
00:14:35,257 --> 00:14:38,960
 the outer stars in the galaxy
were all going at the same speed

243
00:14:38,994 --> 00:14:41,296
         as the stars
     that were closer in,

244
00:14:41,330 --> 00:14:43,965
and they were moving way faster
        than expected.

245
00:14:43,999 --> 00:14:46,367
 "That's funny," Vera thought.

246
00:14:46,402 --> 00:14:50,505
"There must be something weird
 about the Andromeda Galaxy."

247
00:14:50,539 --> 00:14:51,806
So she looked at another galaxy.

248
00:14:51,873 --> 00:14:54,042
          Same story.

249
00:14:54,059 --> 00:14:55,410
         And another.

250
00:14:55,444 --> 00:14:57,912
   Vera studied 60 galaxies

251
00:14:57,947 --> 00:14:59,914
  and found that all of them

252
00:14:59,949 --> 00:15:01,649
    seemed to be violating
      the Law of Gravity,

253
00:15:01,684 --> 00:15:03,651
 a core principle of physics.

254
00:15:03,686 --> 00:15:07,021
      After some initial
      healthy skepticism,

255
00:15:07,056 --> 00:15:09,057
     her colleagues looked
        for themselves,

256
00:15:09,091 --> 00:15:12,360
and found that Vera was right.

257
00:15:12,394 --> 00:15:15,530
It's not that Isaac Newton had
gotten the Law of Gravity wrong;

258
00:15:15,564 --> 00:15:18,099
   Vera Rubin had discovered
       that the gravity

259
00:15:18,133 --> 00:15:20,201
     of something massive
         and invisible

260
00:15:20,235 --> 00:15:24,439
     was forcing the stars
          to go fast.

261
00:15:24,473 --> 00:15:29,944
   And then, someone remembered
        crazy old Fritz Zwicky,

262
00:15:29,979 --> 00:15:32,914
    and the unknown source
          of gravity

263
00:15:32,948 --> 00:15:34,449
    in the galaxy clusters

264
00:15:34,483 --> 00:15:38,553
 that he called "dark matter,"
         back in 1933.

265
00:15:44,793 --> 00:15:47,028
    Vera Rubin had verified
         the existence

266
00:15:47,062 --> 00:15:49,697
 of a new, much larger cosmos.

267
00:15:49,732 --> 00:15:51,966
     And just like the one
      we thought we knew,

268
00:15:52,001 --> 00:15:54,035
  it was filled with mystery.

269
00:15:54,069 --> 00:15:57,538
          Dark matter
  is completely unobservable,

270
00:15:57,573 --> 00:15:59,340
            except
 for its gravitational effect,

271
00:15:59,342 --> 00:16:04,045
   which makes visible stars
   and galaxies move faster.

272
00:16:04,079 --> 00:16:07,782
     Its nature is another
         deep mystery.

273
00:16:07,816 --> 00:16:10,918
Rubin had provided the evidence
   for an invisible universe

274
00:16:10,953 --> 00:16:15,723
 nearly ten times more massive
than the one we thought we knew.

275
00:16:15,758 --> 00:16:17,792
   It was as if we had been
   standing on the seashore

276
00:16:17,859 --> 00:16:19,894
at night, mistakenly believing

277
00:16:19,928 --> 00:16:23,164
that the froth on the waves was
  all there was to the ocean.

278
00:16:23,198 --> 00:16:26,801
Vera Rubin looked at the stars
         and realized

279
00:16:26,835 --> 00:16:29,404
   they were merely the foam
         on the waves,

280
00:16:29,438 --> 00:16:34,575
  and that the greatest part
of the ocean remained unknown.

281
00:16:34,610 --> 00:16:35,927
           But wait.

282
00:16:35,929 --> 00:16:37,945
       It gets crazier.

283
00:16:39,581 --> 00:16:41,566
laxy,

284
00:16:41,617 --> 00:16:43,718
 <i> a few hundred billion stars,</i>

285
00:16:43,752 --> 00:16:46,220
       <i> plus the clouds</i>
       <i> of gas and dust,</i>

286
00:16:46,255 --> 00:16:49,257
      <i> the stuff of once</i>
      <i> and future stars--</i>

287
00:16:49,274 --> 00:16:54,228
 <i> and about a hundred billion</i>
<i> other galaxies-- all of that,</i>

288
00:16:54,263 --> 00:16:57,498
  <i> including those uncounted</i>
    <i> billions of trillions</i>

289
00:16:57,533 --> 00:17:00,568
<i> of planets, moons, and comets--</i>

290
00:17:00,602 --> 00:17:04,672
 <i> amounts to only five percent</i>
  <i> of what is actually there.</i>

291
00:17:04,707 --> 00:17:06,841
   <i> Because there's a bigger</i>
       <i> unsolved mystery</i>

292
00:17:06,875 --> 00:17:08,876
      <i> than dark matter--</i>

293
00:17:08,911 --> 00:17:13,047
 <i> dark energy, which makes up</i>
   <i> even more of the cosmos</i>

294
00:17:13,082 --> 00:17:15,183
  <i> and drives its expansion.</i>

295
00:17:15,217 --> 00:17:17,885
  <i> And it was Fritz Zwicky's</i>
          <i> supernovas</i>

296
00:17:17,920 --> 00:17:21,489
   <i> that lit the way to the</i>
 <i> revelation of its existence.</i>

297
00:17:23,926 --> 00:17:28,496
In one scenario, a star consumes
  all of its nuclear fuel...

298
00:17:32,067 --> 00:17:33,534
        <i> ...then cools,</i>

299
00:17:33,569 --> 00:17:36,270
    <i> and suddenly collapses</i>
    <i> under its own gravity.</i>

300
00:17:36,305 --> 00:17:39,974
      <i> The star rebounds</i>
   <i> in a massive explosion,</i>

301
00:17:40,008 --> 00:17:43,911
<i> leaving behind a neutron star</i>
       <i> or a black hole.</i>

302
00:17:45,514 --> 00:17:47,949
        Since the mass
     of the original star

303
00:17:47,983 --> 00:17:49,751
 can fall within a wide range,

304
00:17:49,785 --> 00:17:51,319
      its peak brightness
        as a supernova

305
00:17:51,353 --> 00:17:53,154
     can also vary widely.

306
00:17:53,188 --> 00:17:55,890
      So, you can't tell
      how far away it is

307
00:17:55,892 --> 00:17:57,792
just from how bright it looks.

308
00:17:57,826 --> 00:18:01,295
 A relatively nearby supernova
  might appear just as bright

309
00:18:01,330 --> 00:18:04,465
as one that was more powerful,
       but farther away.

310
00:18:04,500 --> 00:18:07,401
   But there's another kind
         of supernova

311
00:18:07,436 --> 00:18:09,470
          <i> that comes</i>
    <i> in only one strength.</i>

312
00:18:09,505 --> 00:18:11,806
     <i> It marks the violent</i>
         <i> grand finale</i>

313
00:18:11,840 --> 00:18:16,477
      <i> of a tango danced</i>
 <i> by a giant star and a dwarf.</i>

314
00:18:18,347 --> 00:18:21,149
    <i> As the two stars orbit</i>
  <i> closely around each other,</i>

315
00:18:21,183 --> 00:18:23,618
       <i> the giant sheds</i>
   <i> its outer layers of gas</i>

316
00:18:23,652 --> 00:18:25,620
       <i> onto the dwarf.</i>

317
00:18:25,654 --> 00:18:28,122
    <i> When the added weight</i>
       <i> becomes too much</i>

318
00:18:28,157 --> 00:18:29,957
       <i> for it to bear,</i>

319
00:18:29,992 --> 00:18:34,529
  <i> the dwarf detonates like a</i>
<i> stupendous thermonuclear bomb.</i>

320
00:18:34,563 --> 00:18:36,631
       <i> For a few weeks,</i>

321
00:18:36,665 --> 00:18:39,267
        <i> the brilliance</i>
  <i> of such a supernova rivals</i>

322
00:18:39,301 --> 00:18:42,603
      <i> the combined light</i>
<i> of all the stars in its galaxy.</i>

323
00:18:42,638 --> 00:18:44,438
    <i> This kind of supernova</i>

324
00:18:44,473 --> 00:18:46,974
     <i> always has the same</i>
    <i> maximum power output,</i>

325
00:18:47,009 --> 00:18:50,744
   <i> about five billion times</i>
    <i> brighter than our Sun.</i>

326
00:18:50,813 --> 00:18:52,547
     <i> With big telescopes,</i>

327
00:18:52,581 --> 00:18:54,982
       <i> we can see them</i>
  <i> in galaxies very far away,</i>

328
00:18:55,017 --> 00:18:58,519
     <i> out toward the edge</i>
 <i> of the observable universe.</i>

329
00:19:07,262 --> 00:19:10,364
 <i> Because all such supernovas</i>
    <i> have the same wattage,</i>

330
00:19:10,399 --> 00:19:13,334
     <i> they're ideal tools</i>
   <i> for measuring distances</i>

331
00:19:13,368 --> 00:19:15,570
   <i> to the farthest reaches</i>
       <i> of the universe.</i>

332
00:19:15,604 --> 00:19:18,506
         <i> We call them</i>
     <i> "standard candles."</i>

333
00:19:23,178 --> 00:19:28,816
In 1929, Edwin Hubble discovered
that the universe is expanding.

334
00:19:28,851 --> 00:19:32,086
   The distant galaxies are
drifting away from one another.

335
00:19:32,120 --> 00:19:33,738
       Later, we learned

336
00:19:33,789 --> 00:19:36,724
   that the expansion began
   some 14 billion years ago

337
00:19:36,758 --> 00:19:41,229
   with the explosive birth
of the universe-- the big bang.

338
00:19:42,898 --> 00:19:44,932
      <i> Everybody assumed</i>

339
00:19:44,967 --> 00:19:47,335
  <i> that the rate of expansion</i>
    <i> would be slowing down,</i>

340
00:19:47,369 --> 00:19:49,103
    <i> due to the mutual pull</i>
          <i> of gravity</i>

341
00:19:49,137 --> 00:19:50,872
    <i> between all the parts</i>
       <i> of the universe.</i>

342
00:19:50,906 --> 00:19:52,740
If there is enough dark matter,

343
00:19:52,774 --> 00:19:56,060
 its gravity would eventually
bring the expansion to a stop,

344
00:19:56,111 --> 00:19:58,913
    and the universe would
   then fall back on itself.

345
00:19:58,947 --> 00:20:02,116
   In that case, everything
   would eventually collapse

346
00:20:02,150 --> 00:20:03,918
       in a big crunch.

347
00:20:03,952 --> 00:20:07,288
   On the other hand, if the
universe had less dark matter,

348
00:20:07,322 --> 00:20:09,390
         the expansion
    would continue forever,

349
00:20:09,424 --> 00:20:12,293
      just getting slower
          and slower.

350
00:20:12,327 --> 00:20:14,896
      Two competing teams
        of astronomers

351
00:20:14,930 --> 00:20:18,199
were observing those supernovas
     in distant galaxies.

352
00:20:18,233 --> 00:20:19,867
It turned out to be another one

353
00:20:19,902 --> 00:20:22,303
           of those
    "that's funny" moments.

354
00:20:22,337 --> 00:20:25,640
      In 1998, both teams
      independently came

355
00:20:25,674 --> 00:20:27,308
    to the same conclusion:

356
00:20:27,342 --> 00:20:29,710
      The expansion isn't
    slowing down at all...

357
00:20:29,761 --> 00:20:31,479
       it's speeding up.

358
00:20:31,513 --> 00:20:35,116
 This means the universe will
  continue to expand forever.

359
00:20:35,150 --> 00:20:38,920
There seems to be a mysterious
    force in the universe,

360
00:20:38,954 --> 00:20:41,923
  one that overwhelms gravity
     on the grandest scale

361
00:20:41,957 --> 00:20:44,492
   to push the cosmos apart.

362
00:20:44,526 --> 00:20:47,228
      Most of the energy
  of the universe is bound up

363
00:20:47,262 --> 00:20:48,729
    in this unknown force.

364
00:20:48,764 --> 00:20:51,132
   We call it "dark energy,"

365
00:20:51,166 --> 00:20:53,834
        but that name,
      like "dark matter,"

366
00:20:53,869 --> 00:20:57,305
     is merely a code word
      for our ignorance.

367
00:20:57,339 --> 00:20:59,674
         It's okay not
   to know all the answers.

368
00:20:59,708 --> 00:21:01,676
          It's better
    to admit our ignorance

369
00:21:01,710 --> 00:21:04,078
    than to believe answers
     that might be wrong.

370
00:21:04,112 --> 00:21:07,581
 Pretending to know everything
        closes the door

371
00:21:07,616 --> 00:21:09,617
        to finding out
     what's really there.

372
00:21:10,652 --> 00:21:13,154
   <i> Tonight, our ships sail</i>

373
00:21:13,188 --> 00:21:16,624
<i> into even more exotic waters.</i>

374
00:21:16,658 --> 00:21:18,659
        <i> Come with me.</i>

375
00:21:25,984 --> 00:21:28,252
  DEGRASSE TYSON:<i> Only two of</i>
   <i> our ships have ventured</i>

376
00:21:28,287 --> 00:21:31,756
  <i> into the great dark ocean</i>
    <i> of interstellar space.</i>

377
00:21:31,790 --> 00:21:35,626
     <i> The longest odyssey</i>
      <i> in all of history</i>

378
00:21:35,661 --> 00:21:38,929
 <i> was launched back in 1977--</i>

379
00:21:38,964 --> 00:21:42,667
   <i> NASA's</i> Voyager 1<i> and</i> 2.

380
00:21:42,701 --> 00:21:47,004
      <i> The</i> Voyagers<i> move</i>
 <i> about 40,000 miles an hour.</i>

381
00:21:47,039 --> 00:21:49,824
         <i> They gave us</i>
   <i> our first close-up look</i>

382
00:21:49,875 --> 00:21:51,909
 <i> at Jupiter's Great Red Spot,</i>

383
00:21:51,943 --> 00:21:55,813
   <i> a hurricane three times</i>
      <i> the size of Earth</i>

384
00:21:55,847 --> 00:21:59,784
  <i> and one that's been raging</i>
     <i> since at least 1644,</i>

385
00:21:59,818 --> 00:22:01,519
 <i> when it was first observed.</i>

386
00:22:01,553 --> 00:22:05,323
 <i> For all we know, it could be</i>
   <i> thousands of years old.</i>

387
00:22:05,357 --> 00:22:08,659
   <i> The</i> Voyagers<i> discovered</i>
   <i> the first active volcano</i>

388
00:22:08,694 --> 00:22:12,630
      <i> on another world,</i>
   <i> on Jupiter's moon Io...</i>

389
00:22:14,199 --> 00:22:16,334
       <i> ...and an ocean</i>
   <i> beneath the icy surface</i>

390
00:22:16,368 --> 00:22:17,968
    <i> of the moon Europa...</i>

391
00:22:21,673 --> 00:22:25,209
<i> ...with at least twice as much</i>
<i> water as we have here on Earth.</i>

392
00:22:28,313 --> 00:22:31,682
  <i> The</i> Voyagers<i> dared to fly</i>
    <i> across Saturn's rings</i>

393
00:22:31,717 --> 00:22:36,053
 <i> and revealed that they were</i>
<i> made of hundreds of thin bands</i>

394
00:22:36,088 --> 00:22:37,888
    <i> of orbiting snowballs.</i>

395
00:22:41,259 --> 00:22:43,894
<i> On Saturn's giant moon Titan,</i>

396
00:22:43,929 --> 00:22:48,065
Voyager<i> detected an atmosphere</i>
<i> four times denser than Earth's.</i>

397
00:22:48,100 --> 00:22:52,837
 <i> That hinted at the existence</i>
<i> of hydrocarbon seas on Titan,</i>

398
00:22:52,871 --> 00:22:54,538
  <i> which we later confirmed.</i>

399
00:22:56,508 --> 00:22:58,476
       Voyager 2<i> gave us</i>
      <i> our first portrait</i>

400
00:22:58,510 --> 00:23:02,313
   <i> of the outermost planet,</i>
          <i> Neptune...</i>

401
00:23:02,347 --> 00:23:06,217
     <i> where the winds roar</i>
  <i> at 1,000 miles per hour...</i>

402
00:23:08,053 --> 00:23:10,921
   <i> ...and its moon Triton,</i>
        <i> where geysers</i>

403
00:23:10,956 --> 00:23:15,459
     <i> of boiling nitrogen</i>
    <i> shoot five miles high.</i>

404
00:23:18,597 --> 00:23:21,399
Voyager<i> successfully completed</i>
   <i> its mission of discovery</i>

405
00:23:21,433 --> 00:23:23,234
    <i> to the outer planets,</i>

406
00:23:23,268 --> 00:23:25,236
       <i> but its odyssey</i>
      <i> into the darkness</i>

407
00:23:25,270 --> 00:23:27,271
     <i> was just beginning.</i>

408
00:23:29,574 --> 00:23:31,275
  35 years after its launch,

409
00:23:31,309 --> 00:23:33,944
  <i> Voyager 1</i> became the first
       of our spacecraft

410
00:23:33,979 --> 00:23:36,847
 to enter an uncharted realm.

411
00:23:36,882 --> 00:23:40,084
    <i> The Sun is constantly</i>
     <i> shooting out streams</i>

412
00:23:40,118 --> 00:23:42,420
     <i> of charged particles</i>
      <i> in all directions,</i>

413
00:23:42,454 --> 00:23:44,755
  <i> moving at a million miles</i>
           <i> an hour.</i>

414
00:23:44,790 --> 00:23:49,460
    <i> This solar wind blows</i>
   <i> a vast magnetic bubble,</i>

415
00:23:49,561 --> 00:23:53,464
<i> our heliosphere, that extends</i>
  <i> beyond the outer planets.</i>

416
00:23:53,466 --> 00:23:58,803
  <i> It pushes out against the</i>
<i> thin gas of interstellar space.</i>

417
00:23:58,837 --> 00:24:03,407
    <i> There's a border where</i>
<i> one ends and the other begins.</i>

418
00:24:03,442 --> 00:24:05,576
    Voyager 1<i> reported back</i>
           <i> to Earth</i>

419
00:24:05,610 --> 00:24:08,112
      <i> that its detectors</i>
     <i> were being pummeled</i>

420
00:24:08,146 --> 00:24:09,647
<i> by more and more cosmic rays.</i>

421
00:24:09,664 --> 00:24:12,082
  <i> Until then, we didn't know</i>

422
00:24:12,117 --> 00:24:14,385
    <i> where the interstellar</i>
         <i> ocean began.</i>

423
00:24:14,419 --> 00:24:16,654
     Voyager 1<i> pressed on</i>

424
00:24:16,688 --> 00:24:19,874
       <i> past a boundary</i>
 <i> we had never crossed before.</i>

425
00:24:19,925 --> 00:24:23,694
<i> The heliosphere shields us from</i>
<i> most of the deadly cosmic rays.</i>

426
00:24:23,795 --> 00:24:25,930
<i> When stormy solar winds blow,</i>

427
00:24:25,964 --> 00:24:28,165
<i> this zone of protection grows;</i>

428
00:24:28,200 --> 00:24:30,301
    <i> in calm solar weather,</i>
         <i> it shrinks.</i>

429
00:24:30,335 --> 00:24:33,604
  <i> When a star goes supernova</i>
<i> in our galactic neighborhood...</i>

430
00:24:35,440 --> 00:24:37,675
        <i> ...the debris</i>
    <i> from the exploded star</i>

431
00:24:37,709 --> 00:24:40,678
    pushes the heliosphere
     back towards the Sun.

432
00:24:40,712 --> 00:24:42,313
     If it's strong enough
          to push it

433
00:24:42,347 --> 00:24:44,248
       all the way back
       to Earth's orbit,

434
00:24:44,282 --> 00:24:49,320
<i> our planet gets a radioactive</i>
  <i> bath of supernova debris.</i>

435
00:24:49,354 --> 00:24:52,156
           Luckily,
this doesn't happen very often.

436
00:24:52,190 --> 00:24:55,593
   The last one was perhaps
    two million years ago.

437
00:24:55,627 --> 00:24:58,762
  A neighboring star explodes
        a million years

438
00:24:58,797 --> 00:25:02,433
before there's even such a thing
     as the human species.

439
00:25:02,467 --> 00:25:04,935
How can we possibly know this?

440
00:25:04,970 --> 00:25:07,771
    Because the dying star
        left its traces

441
00:25:07,806 --> 00:25:10,274
    miles below the surface
         of the ocean.

442
00:25:10,308 --> 00:25:15,012
      Manganese nodules,
  small rocks like this one,

443
00:25:15,046 --> 00:25:19,517
    are scattered over much
    of the deep sea floor.

444
00:25:19,551 --> 00:25:22,353
    They grow very slowly.

445
00:25:22,387 --> 00:25:27,124
   I'm talking a millimeter
      in a million years,

446
00:25:27,158 --> 00:25:31,128
      <i> layer upon layer.</i>

447
00:25:31,162 --> 00:25:34,198
      <i> These nodules grow</i>
 <i> in partnership with bacteria</i>

448
00:25:34,232 --> 00:25:39,069
<i> by taking up minerals dissolved</i>
       <i> in the seawater.</i>

449
00:25:39,104 --> 00:25:43,073
     <i> A supernova produces</i>
 <i> a radioactive form of iron,</i>

450
00:25:43,108 --> 00:25:47,144
     <i> unlike anything made</i>
<i> by natural processes on Earth.</i>

451
00:25:47,178 --> 00:25:49,547
       Researchers found
 telltale traces of this iron

452
00:25:49,581 --> 00:25:51,549
        in a thin layer
       below the surface

453
00:25:51,583 --> 00:25:53,551
   of the manganese nodules.

454
00:25:53,585 --> 00:25:56,387
   They used the known rate
   of growth of the nodules

455
00:25:56,421 --> 00:25:58,722
      to date that layer
       and to connect it

456
00:25:58,757 --> 00:26:02,760
     to the fate of a star
    that perished eons ago.

457
00:26:04,396 --> 00:26:07,264
    The difference between
  seeing nothing but a pebble

458
00:26:07,299 --> 00:26:11,702
  and reading the history of
the cosmos inscribed inside it

459
00:26:11,736 --> 00:26:14,138
          is science.

460
00:26:16,291 --> 00:26:20,277
    The interstellar ocean
       is dark and deep.

461
00:26:20,312 --> 00:26:24,281
   Out here, the Sun is just
the brightest star in the sky.

462
00:26:24,299 --> 00:26:27,718
   Yet the<i> Voyagers</i> maintain
 their regular communications

463
00:26:27,752 --> 00:26:29,820
          with NASA's
  Jet Propulsion Laboratory,

464
00:26:29,921 --> 00:26:32,523
    talking back and forth
    across the light-hours

465
00:26:32,557 --> 00:26:35,426
   that separate these ships
     from their home port.

466
00:26:35,460 --> 00:26:39,263
   No other objects touched
        by human hands

467
00:26:39,297 --> 00:26:42,616
      have ever ventured
      this far from home.

468
00:26:48,940 --> 00:26:50,407
     Even after they lose
         their ability

469
00:26:50,442 --> 00:26:52,476
  to respond to our command,

470
00:26:52,510 --> 00:26:54,712
         the last and,
   by far, the longest phase

471
00:26:54,746 --> 00:26:56,747
    of the<i> Voyager</i> mission
          will begin.

472
00:27:04,089 --> 00:27:07,257
h<i> Voyagers</i>
        rounded Jupiter,

473
00:27:07,292 --> 00:27:09,693
   its massive gravity acted
        as a slingshot,

474
00:27:09,728 --> 00:27:11,695
       flinging them out
      of the solar system

475
00:27:11,730 --> 00:27:13,897
   to travel among the stars
         of our galaxy

476
00:27:13,932 --> 00:27:16,350
     for a billion years.

477
00:27:16,401 --> 00:27:18,969
     Carl Sagan recognized
   that the<i> Voyager</i> mission

478
00:27:19,070 --> 00:27:23,107
  offered two free tickets to
something approaching eternity.

479
00:27:23,141 --> 00:27:26,110
   He assembled a small team
      to create a message

480
00:27:26,177 --> 00:27:29,113
      to any civilization
     that might, one day,

481
00:27:29,147 --> 00:27:32,483
           encounter
   the derelict spacecraft.

482
00:27:35,453 --> 00:27:37,621
      <i> 26 centuries ago,</i>

483
00:27:37,656 --> 00:27:40,490
 <i> the Assyrian king Esarhaddon</i>
            <i> wrote:</i>

484
00:27:40,492 --> 00:27:43,227
<i> "I had monuments made of bronze</i>

485
00:27:43,261 --> 00:27:45,896
      <i> "and inscriptions</i>
        <i> of baked clay.</i>

486
00:27:45,930 --> 00:27:49,299
<i> I left them in the foundations</i>
      <i> for future times."</i>

487
00:27:49,334 --> 00:27:53,637
 <i> These hieroglyphics continue</i>
   <i> that ancient tradition.</i>

488
00:27:53,705 --> 00:27:56,640
<i> They are inscribed on the cover</i>
    <i> of a message designed</i>

489
00:27:56,675 --> 00:28:01,145
   <i> to be read by the beings</i>
  <i> of other worlds and times.</i>

490
00:28:02,814 --> 00:28:04,348
    What could we possibly
        have in common

491
00:28:04,382 --> 00:28:05,816
  with an alien civilization

492
00:28:05,850 --> 00:28:08,519
     with its own separate
     evolutionary history

493
00:28:08,553 --> 00:28:10,788
    and one so far advanced
           beyond us

494
00:28:10,822 --> 00:28:15,025
     that they can patrol
      interstellar space?

495
00:28:15,060 --> 00:28:16,593
      One thing at least:

496
00:28:16,628 --> 00:28:18,362
    a universal language...

497
00:28:18,396 --> 00:28:20,197
           science.

498
00:28:20,215 --> 00:28:23,200
 <i> It's hard to break the bonds</i>
         <i> of gravity.</i>

499
00:28:23,218 --> 00:28:25,469
      <i> You can only sail</i>
       <i> the cosmic seas</i>

500
00:28:25,503 --> 00:28:28,839
   <i> if you speak mathematics</i>
         <i> and physics.</i>

501
00:28:28,873 --> 00:28:31,942
  Hydrogen is the most common
   element in the universe.

502
00:28:31,976 --> 00:28:33,944
The electron in a hydrogen atom

503
00:28:33,978 --> 00:28:35,779
flips the direction of its spin

504
00:28:35,814 --> 00:28:37,781
      at a constant rate,
         or frequency.

505
00:28:37,816 --> 00:28:41,785
      <i> Hydrogen atoms are</i>
  <i> like tiny natural clocks--</i>

506
00:28:41,787 --> 00:28:44,621
        <i> tick... tock.</i>

507
00:28:44,656 --> 00:28:46,757
  <i> Now we have a unit of time</i>
          <i> in common</i>

508
00:28:46,858 --> 00:28:48,442
 <i> with the extraterrestrials.</i>

509
00:28:48,493 --> 00:28:50,360
    This will come in handy
 when we get to the next level

510
00:28:50,395 --> 00:28:51,962
        of the message.

511
00:28:51,996 --> 00:28:54,565
  <i> Here's our return address</i>
          <i> in space.</i>

512
00:28:54,599 --> 00:28:57,401
 <i> Pulsars are rapidly-spinning</i>
        <i> neutron stars</i>

513
00:28:57,435 --> 00:29:00,537
 <i> that give off regular bursts</i>
       <i> of radio waves.</i>

514
00:29:00,555 --> 00:29:03,240
<i> You can set your clock by them.</i>

515
00:29:03,258 --> 00:29:05,776
   The Sun is at the center
       of this diagram,

516
00:29:05,860 --> 00:29:09,513
      and the lines point
  to the 14 nearest pulsars.

517
00:29:09,515 --> 00:29:13,350
A simple code labels each pulsar
  with its unique frequency,

518
00:29:13,384 --> 00:29:15,519
      using the ticktock
     of the hydrogen atom

519
00:29:15,586 --> 00:29:17,254
     as the unit of time.

520
00:29:17,288 --> 00:29:20,090
So alien astronomers could use
         this diagram

521
00:29:20,125 --> 00:29:22,693
    to locate the home star
   of the<i> Voyager</i> spacecraft

522
00:29:22,727 --> 00:29:24,328
        in our galaxy.

523
00:29:24,362 --> 00:29:25,929
     <i> They could also tell</i>

524
00:29:25,964 --> 00:29:27,998
 <i> how long ago the spacecraft</i>
        <i> was launched.</i>

525
00:29:28,032 --> 00:29:30,200
     <i> And that's important</i>
  <i> because the</i> Voyager<i> record</i>

526
00:29:30,235 --> 00:29:34,238
  <i> has a projected shelf life</i>
   <i> of 1,000 million years.</i>

527
00:29:37,275 --> 00:29:38,876
  <i> Become an extraterrestrial</i>
        <i> archaeologist</i>

528
00:29:38,910 --> 00:29:40,878
      <i> for a few moments.</i>

529
00:29:40,912 --> 00:29:44,081
<i> An artifact has been fished out</i>
  <i> of the interstellar ocean.</i>

530
00:29:44,115 --> 00:29:45,215
   (classical music playing)

531
00:29:45,250 --> 00:29:46,750
    <i> It was made by beings</i>

532
00:29:46,785 --> 00:29:48,919
          <i> that lived</i>
  <i> about a billion years ago.</i>

533
00:29:48,953 --> 00:29:51,121
 <i> What would you make of them</i>
       <i> and their world?</i>

534
00:29:51,156 --> 00:29:52,289
    (guitar playing blues)

535
00:29:52,323 --> 00:29:56,026
 <i> They've sent us their music</i>

536
00:29:56,060 --> 00:30:00,130
         and greetings
    in 59 human languages.

537
00:30:00,165 --> 00:30:03,033
  (various languages overlap,
      speaking greetings)

538
00:30:03,035 --> 00:30:06,203
  NICK SAGAN: Hello from the
   children of planet Earth.

539
00:30:06,205 --> 00:30:07,304
        DEGRASSE TYSON:
   <i> And one whale language.</i>

540
00:30:07,306 --> 00:30:09,306
       (whales singing)

541
00:30:09,308 --> 00:30:12,676
<i> And a sound essay that includes</i>
   <i> a</i> Saturn V<i> rocket launch.</i>

542
00:30:12,678 --> 00:30:14,511
     (jet engine whooshes)

543
00:30:14,513 --> 00:30:17,347
    <i> A mother's first words</i>
     <i> to her newborn baby.</i>

544
00:30:17,349 --> 00:30:18,849
         (baby crying)

545
00:30:18,851 --> 00:30:20,150
    WOMAN: Oh, come on now.

546
00:30:20,152 --> 00:30:22,319
Be a good boy... be a good boy.

547
00:30:22,321 --> 00:30:25,122
  <i> The brain waves of a young</i>
 <i> woman newly fallen in love.</i>

548
00:30:25,124 --> 00:30:28,125
     (staticky crackling)

549
00:30:28,127 --> 00:30:31,662
  And the sound of a pulsar.

550
00:30:31,696 --> 00:30:33,664
 (steady, rhythmic crackling)

551
00:30:33,698 --> 00:30:35,766
    (Blind Willie Johnson's
"Dark Was the Night..." playing)

552
00:30:35,800 --> 00:30:40,804
    <i> All of that will live</i>
     <i> for a billion years.</i>

553
00:30:40,839 --> 00:30:45,642
     ("Dark Was the Night"
    continues, then fades)

554
00:30:53,184 --> 00:30:56,620
 How long is a billion years?

555
00:31:02,360 --> 00:31:05,329
press all the time
      since the big bang,

556
00:31:05,363 --> 00:31:07,331
      the explosive birth
       of the universe,

557
00:31:07,365 --> 00:31:09,333
   into a single Earth year,

558
00:31:09,367 --> 00:31:12,669
      a billion years is
 about one month of that year.

559
00:31:12,704 --> 00:31:17,040
  What was happening on Earth
     a billion years ago?

560
00:31:20,078 --> 00:31:23,080
Most of Earth's land was amassed
     into a supercontinent

561
00:31:23,114 --> 00:31:24,781
        called Rodinia.

562
00:31:24,816 --> 00:31:28,452
   It was a barren desert--
    no animals, no plants.

563
00:31:28,486 --> 00:31:30,420
     A billion years ago,
  there wasn't enough oxygen

564
00:31:30,455 --> 00:31:32,856
       in our atmosphere
    to form an ozone layer,

565
00:31:32,891 --> 00:31:35,525
        and without it,
     ultraviolet radiation

566
00:31:35,527 --> 00:31:38,262
        prevented life
   from colonizing the land.

567
00:31:38,296 --> 00:31:40,797
    Rodinia probably looked
        more like Mars

568
00:31:40,832 --> 00:31:43,533
    than present-day Earth.

569
00:31:43,568 --> 00:31:46,270
    <i> The giant world ocean</i>
   <i> produced huge rainstorms</i>

570
00:31:46,304 --> 00:31:48,805
<i> causing flooding and erosion.</i>

571
00:31:48,840 --> 00:31:51,942
  <i> Glaciers formed, and their</i>
<i> slow but relentless movements</i>

572
00:31:51,976 --> 00:31:55,145
       <i> carved the land</i>
       <i> into new shapes.</i>

573
00:31:55,179 --> 00:31:58,548
   <i> Single-celled organisms</i>
    <i> dominated the oceans,</i>

574
00:31:58,583 --> 00:32:02,152
 <i> but some existed in colonies</i>
   <i> called "microbial mats,"</i>

575
00:32:02,186 --> 00:32:06,890
 <i> and the first multicellular</i>
 <i> organisms would soon evolve.</i>

576
00:32:06,925 --> 00:32:08,892
 And a billion years from now,

577
00:32:08,927 --> 00:32:10,894
  what will Earth be like...

578
00:32:10,929 --> 00:32:13,563
    long after our cities,
    the Egyptian pyramids,

579
00:32:13,598 --> 00:32:16,733
      the Rocky Mountains
 have all been eroded to dust?

580
00:32:16,768 --> 00:32:19,336
     There are few things
  we can say with confidence

581
00:32:19,370 --> 00:32:22,372
about such a far distant time.

582
00:32:26,044 --> 00:32:28,545
        <i> The only thing</i>
     <i> we can say for sure</i>

583
00:32:28,547 --> 00:32:32,349
  is that Earth as we know it
      will be so changed

584
00:32:32,383 --> 00:32:35,686
         that we would
scarcely recognize it as home.

585
00:32:35,720 --> 00:32:39,256
      But even a thousand
    million years from now,

586
00:32:39,290 --> 00:32:42,793
   something of who we were
  and the music that we made

587
00:32:42,827 --> 00:32:45,095
  in that long-ago spring...

588
00:32:45,129 --> 00:32:47,130
         will live on.

589
00:32:52,003 --> 00:32:55,172
   <i> In that distant future,</i>
 <i> our Sun will have completed</i>

590
00:32:55,206 --> 00:32:58,542
  <i> another four orbits around</i>
 <i> the center of the galaxy...</i>

591
00:33:06,784 --> 00:33:11,355
<i> ...and the</i> Voyagers<i> will have</i>
  <i> ventured far from the Sun.</i>

592
00:33:14,692 --> 00:33:17,394
    Carl Sagan was a member
  of<i> Voyager's</i> imaging team,

593
00:33:17,428 --> 00:33:21,631
and it was his idea that<i> Voyager</i>
     take one last picture.

594
00:33:21,666 --> 00:33:23,600
     A generation before,

595
00:33:23,701 --> 00:33:26,536
   an astronaut on the last
   Apollo flight to the Moon

596
00:33:26,571 --> 00:33:29,206
      had taken a picture
     of the whole Earth--

597
00:33:29,240 --> 00:33:32,409
          the planet
  as a world without borders.

598
00:33:32,443 --> 00:33:35,812
       It became an icon
    of a new consciousness.

599
00:33:35,847 --> 00:33:39,983
  Carl realized the next step
       in this process.

600
00:33:40,018 --> 00:33:43,053
   He convinced NASA to turn
     the<i> Voyager 1</i> camera

601
00:33:43,120 --> 00:33:46,857
  back towards Earth when the
spacecraft went beyond Neptune

602
00:33:46,924 --> 00:33:50,527
  for one last look homeward
     at what he called...

603
00:33:50,561 --> 00:33:53,563
      the pale blue dot.

604
00:33:59,370 --> 00:34:00,937
          CARL SAGAN:
         <i> That's here.</i>

605
00:34:00,972 --> 00:34:02,506
         <i> That's home.</i>

606
00:34:02,540 --> 00:34:04,107
          <i> That's us.</i>

607
00:34:04,142 --> 00:34:06,843
  <i> On it, everyone you love,</i>

608
00:34:06,878 --> 00:34:08,879
      <i> everyone you know,</i>

609
00:34:08,913 --> 00:34:10,881
 <i> everyone you ever heard of,</i>

610
00:34:10,915 --> 00:34:13,550
<i> every human being who ever was,</i>

611
00:34:13,584 --> 00:34:15,952
    <i> lived out their lives.</i>

612
00:34:15,987 --> 00:34:19,723
        <i> The aggregate</i>
  <i> of our joy and suffering,</i>

613
00:34:19,757 --> 00:34:22,559
    <i> thousands of confident</i>
    <i> religions, ideologies,</i>

614
00:34:22,593 --> 00:34:24,561
   <i> and economic doctrines,</i>

615
00:34:24,595 --> 00:34:26,730
  <i> every hunter and forager,</i>

616
00:34:26,764 --> 00:34:28,732
    <i> every hero and coward,</i>

617
00:34:28,766 --> 00:34:32,202
 <i> every creator and destroyer</i>
       <i> of civilization,</i>

618
00:34:32,236 --> 00:34:34,204
   <i> every king and peasant,</i>

619
00:34:34,238 --> 00:34:36,239
 <i> every young couple in love,</i>

620
00:34:36,274 --> 00:34:39,543
   <i> every mother and father,</i>
        <i> hopeful child,</i>

621
00:34:39,577 --> 00:34:41,812
    <i> inventor and explorer,</i>

622
00:34:41,846 --> 00:34:45,482
   <i> every teacher of morals,</i>
  <i> every corrupt politician,</i>

623
00:34:45,516 --> 00:34:49,586
       <i> every superstar,</i>
    <i> every supreme leader,</i>

624
00:34:49,620 --> 00:34:53,457
    <i> every saint and sinner</i>
<i> in the history of our species,</i>

625
00:34:53,491 --> 00:34:55,492
        <i> lived there...</i>

626
00:34:55,494 --> 00:34:57,294
      <i> on a mote of dust</i>

627
00:34:57,328 --> 00:35:00,597
  <i> suspended... in a sunbeam.</i>

628
00:35:00,599 --> 00:35:04,801
         <i> The Earth is</i>
      <i> a very small stage</i>

629
00:35:04,836 --> 00:35:08,638
   <i> in a vast, cosmic arena.</i>

630
00:35:08,673 --> 00:35:11,908
 <i> Think of the rivers of blood</i>

631
00:35:11,943 --> 00:35:15,645
     <i> spilled by all those</i>
    <i> generals and emperors</i>

632
00:35:15,680 --> 00:35:18,115
 <i> so that in glory and triumph</i>

633
00:35:18,149 --> 00:35:21,017
      <i> they could become</i>
    <i> the momentary masters</i>

634
00:35:21,119 --> 00:35:24,354
  <i> of a fraction... of a dot.</i>

635
00:35:24,388 --> 00:35:27,491
     <i> Think of the endless</i>
      <i> cruelties visited</i>

636
00:35:27,508 --> 00:35:30,927
      <i> by the inhabitants</i>
 <i> of</i> one<i> corner of this pixel</i>

637
00:35:31,028 --> 00:35:33,930
       <i> on the scarcely</i>
 <i> distinguishable inhabitants</i>

638
00:35:33,965 --> 00:35:36,016
    <i> of some other corner.</i>

639
00:35:36,067 --> 00:35:39,035
         <i> How frequent</i>
   <i> their misunderstandings,</i>

640
00:35:39,137 --> 00:35:42,105
      <i> how eager they are</i>
     <i> to kill one another,</i>

641
00:35:42,140 --> 00:35:45,442
  <i> how fervent their hatreds.</i>

642
00:35:45,476 --> 00:35:47,978
       <i> Our posturings,</i>

643
00:35:48,012 --> 00:35:51,047
<i> our imagined self-importance,</i>

644
00:35:51,082 --> 00:35:53,650
  <i> the delusion that we have</i>
   <i> some privileged position</i>

645
00:35:53,684 --> 00:35:55,285
       <i> in the universe,</i>

646
00:35:55,319 --> 00:35:59,990
        <i> are challenged</i>
 <i> by this point of pale light.</i>

647
00:36:00,024 --> 00:36:02,025
        <i> Our planet...</i>

648
00:36:02,059 --> 00:36:05,061
<i> is a lonely speck in the great,</i>

649
00:36:05,096 --> 00:36:08,165
   <i> enveloping cosmic dark.</i>

650
00:36:08,199 --> 00:36:11,001
      <i> In our obscurity,</i>

651
00:36:11,035 --> 00:36:13,803
    <i> in all this vastness,</i>

652
00:36:13,838 --> 00:36:17,541
  <i> there is no hint that help</i>
   <i> will come from elsewhere</i>

653
00:36:17,575 --> 00:36:20,510
  <i> to save us from ourselves.</i>

654
00:36:20,545 --> 00:36:24,748
 <i> The Earth is the only world</i>
 <i> known so far to harbor life.</i>

655
00:36:24,765 --> 00:36:26,750
    <i> There is nowhere else,</i>

656
00:36:26,784 --> 00:36:28,752
 <i> at least in the near future,</i>

657
00:36:28,786 --> 00:36:31,588
     <i> to which our species</i>
        <i> could migrate.</i>

658
00:36:31,622 --> 00:36:34,390
         <i> Visit, yes.</i>

659
00:36:34,392 --> 00:36:36,593
       <i> Settle, not yet.</i>

660
00:36:36,627 --> 00:36:38,662
       <i> Like it or not,</i>

661
00:36:38,696 --> 00:36:43,233
  <i> for the moment, the Earth</i>
 <i> is where we make our stand.</i>

662
00:36:43,267 --> 00:36:46,570
    <i> It has been said that</i>
   <i> astronomy is a humbling</i>

663
00:36:46,587 --> 00:36:50,707
    <i> and character-building</i>
         <i> experience.</i>

664
00:36:50,741 --> 00:36:53,210
       <i> There is perhaps</i>
   <i> no better demonstration</i>

665
00:36:53,244 --> 00:36:56,112
<i> of the folly of human conceits</i>

666
00:36:56,114 --> 00:36:59,616
   <i> than this distant image.</i>

667
00:36:59,650 --> 00:37:03,220
    <i> To me, it underscores</i>
      <i> our responsibility</i>

668
00:37:03,254 --> 00:37:05,922
     <i> to deal more kindly</i>
       <i> with one another</i>

669
00:37:05,957 --> 00:37:08,425
 <i> and to preserve and cherish</i>

670
00:37:08,459 --> 00:37:10,627
      <i> the pale blue dot,</i>

671
00:37:10,629 --> 00:37:13,763
<i> the only home we've ever known.</i>

672
00:37:20,671 --> 00:37:22,639
        DEGRASSE TYSON:
         <i> How did we,</i>

673
00:37:22,673 --> 00:37:25,025
    <i> tiny creatures living</i>
    <i> on that speck of dust,</i>

674
00:37:25,076 --> 00:37:28,378
  <i> ever manage to figure out</i>
    <i> how to send spacecraft</i>

675
00:37:28,380 --> 00:37:31,247
     <i> out among the stars</i>
      <i> of the Milky Way?</i>

676
00:37:31,249 --> 00:37:35,619
  <i> Only a few centuries ago,</i>
<i> a mere second of cosmic time,</i>

677
00:37:35,653 --> 00:37:38,255
       <i> we knew nothing</i>
   <i> of where or who we were.</i>

678
00:37:38,289 --> 00:37:41,057
    <i> Oblivious to the rest</i>
        <i> of the cosmos,</i>

679
00:37:41,092 --> 00:37:43,660
<i> we inhabited a kind of prison--</i>

680
00:37:43,694 --> 00:37:45,645
       <i> a tiny universe</i>

681
00:37:45,696 --> 00:37:49,199
    <i> bounded by a nutshell.</i>

682
00:37:51,302 --> 00:37:55,572
      <i> How did we escape</i>
       <i> from the prison?</i>

683
00:37:55,606 --> 00:37:59,509
       <i> It was the work</i>
 <i> of generations of searchers</i>

684
00:37:59,543 --> 00:38:03,380
        <i> who took five</i>
    <i> simple rules to heart.</i>

685
00:38:07,285 --> 00:38:09,252
     <i> Question authority.</i>

686
00:38:09,287 --> 00:38:12,589
       <i> No idea is true</i>
<i> just because someone says so,</i>

687
00:38:12,623 --> 00:38:14,291
        <i> including me.</i>

688
00:38:15,276 --> 00:38:17,127
     <i> Think for yourself.</i>

689
00:38:20,564 --> 00:38:22,532
      <i> Question yourself.</i>

690
00:38:24,885 --> 00:38:27,537
    <i> Don't believe anything</i>
  <i> just because you want to.</i>

691
00:38:27,571 --> 00:38:32,342
     <i> Believing something</i>
     <i> doesn't make it so.</i>

692
00:38:32,376 --> 00:38:34,344
          <i> Test ideas</i>
    <i> by the evidence gained</i>

693
00:38:34,378 --> 00:38:38,048
       <i> from observation</i>
       <i> and experiment.</i>

694
00:38:38,082 --> 00:38:41,451
   <i> If a favorite idea fails</i>
    <i> a well-designed test,</i>

695
00:38:41,485 --> 00:38:43,653
         <i> it's wrong!</i>

696
00:38:43,688 --> 00:38:45,221
         <i> Get over it.</i>

697
00:38:45,323 --> 00:38:50,160
     <i> Follow the evidence,</i>
      <i> wherever it leads.</i>

698
00:38:51,762 --> 00:38:55,165
   <i> If you have no evidence,</i>
      <i> reserve judgment.</i>

699
00:38:55,232 --> 00:38:58,218
     <i> And perhaps the most</i>
    <i> important rule of all:</i>

700
00:38:58,269 --> 00:39:00,036
          <i> Remember,</i>
     <i> you could be wrong.</i>

701
00:39:00,038 --> 00:39:02,739
   <i> Even the best scientists</i>

702
00:39:02,773 --> 00:39:04,674
       <i> have been wrong</i>
      <i> about some things.</i>

703
00:39:04,742 --> 00:39:07,410
      <i> Newton, Einstein,</i>

704
00:39:07,428 --> 00:39:10,180
<i> and every other great scientist</i>
         <i> in history,</i>

705
00:39:10,214 --> 00:39:12,682
   <i> they all made mistakes.</i>

706
00:39:12,717 --> 00:39:15,885
     <i> Of course they did--</i>
       <i> they were human.</i>

707
00:39:15,920 --> 00:39:20,223
   <i> Science is a way to keep</i>
  <i> from fooling ourselves...</i>

708
00:39:20,257 --> 00:39:23,026
       <i> and each other.</i>

709
00:39:23,060 --> 00:39:25,395
  <i> Have scientists known sin?</i>

710
00:39:28,566 --> 00:39:30,033
          <i> Of course.</i>

711
00:39:30,051 --> 00:39:32,402
   <i> We have misused science,</i>
       <i> just as we have</i>

712
00:39:32,436 --> 00:39:35,672
       <i> every other tool</i>
       <i> at our disposal,</i>

713
00:39:35,706 --> 00:39:37,874
<i> and that's why we can't afford</i>

714
00:39:37,908 --> 00:39:41,845
   <i> to leave it in the hands</i>
      <i> of a powerful few.</i>

715
00:39:41,879 --> 00:39:44,781
       <i> The more science</i>
    <i> belongs to all of us,</i>

716
00:39:44,815 --> 00:39:47,884
       <i> the less likely</i>
     <i> it is to be misused.</i>

717
00:39:50,121 --> 00:39:52,756
         <i> These values</i>
    <i> undermine the appeals</i>

718
00:39:52,790 --> 00:39:55,058
 <i> of fanaticism and ignorance</i>

719
00:39:55,092 --> 00:39:56,960
       <i> and, after all,</i>

720
00:39:56,994 --> 00:39:59,429
 <i> the universe is mostly dark,</i>

721
00:39:59,463 --> 00:40:02,699
 <i> dotted by islands of light.</i>

722
00:40:02,733 --> 00:40:06,369
<i> Learning the age of the Earth</i>
 <i> or the distance to the stars</i>

723
00:40:06,404 --> 00:40:08,371
    <i> or how life evolves--</i>

724
00:40:08,406 --> 00:40:10,640
<i> what difference does that make?</i>

725
00:40:10,674 --> 00:40:13,376
   Well, part of it depends
     on how big a universe

726
00:40:13,411 --> 00:40:15,278
  you're willing to live in.

727
00:40:15,312 --> 00:40:17,280
   Some of us like it small.

728
00:40:17,314 --> 00:40:18,915
         That's fine.

729
00:40:18,949 --> 00:40:20,316
        Understandable.

730
00:40:20,351 --> 00:40:22,051
      But I like it big.

731
00:40:22,086 --> 00:40:25,221
  And when I take all of this
  into my heart and my mind,

732
00:40:25,256 --> 00:40:27,157
      I'm uplifted by it.

733
00:40:27,191 --> 00:40:30,960
 And when I have that feeling,
I want to know that it's real,

734
00:40:30,995 --> 00:40:34,464
 that it's not just something
 happening inside my own head,

735
00:40:34,498 --> 00:40:36,633
because it matters what's true,

736
00:40:36,667 --> 00:40:39,102
and our imagination is nothing

737
00:40:39,136 --> 00:40:42,505
         compared with
   Nature's awesome reality.

738
00:40:46,644 --> 00:40:50,647
        <i> I want to know</i>
 <i> what's in those dark places,</i>

739
00:40:50,681 --> 00:40:54,384
      <i> and what happened</i>
     <i> before the big bang.</i>

740
00:40:56,454 --> 00:40:59,289
   <i> I want to know what lies</i>
  <i> beyond the cosmic horizon,</i>

741
00:40:59,323 --> 00:41:02,192
     <i> and how life began.</i>

742
00:41:02,226 --> 00:41:04,694
    <i> Are there other places</i>
        <i> in the cosmos</i>

743
00:41:04,728 --> 00:41:08,698
   <i> where matter and energy</i>
     <i> have become alive...</i>

744
00:41:08,732 --> 00:41:11,167
          <i> and aware?</i>

745
00:41:18,509 --> 00:41:20,677
<i> I want to know my ancestors--</i>

746
00:41:20,711 --> 00:41:22,178
         <i> all of them.</i>

747
00:41:22,213 --> 00:41:24,447
         <i> I want to be</i>
     <i> a good, strong link</i>

748
00:41:24,482 --> 00:41:26,349
 <i> in the chain of generations.</i>

749
00:41:26,383 --> 00:41:28,184
<i> I want to protect my children</i>

750
00:41:28,219 --> 00:41:31,354
       <i> and the children</i>
       <i> of ages to come.</i>

751
00:41:31,388 --> 00:41:34,557
        We, who embody
    the local eyes and ears

752
00:41:34,592 --> 00:41:37,293
   and thoughts and feelings
        of the cosmos,

753
00:41:37,328 --> 00:41:40,563
we've begun to learn the story
       of our origins--

754
00:41:40,598 --> 00:41:44,467
   star stuff contemplating
   the evolution of matter,

755
00:41:44,502 --> 00:41:48,171
tracing that long path by which
 it arrived at consciousness.

756
00:41:48,205 --> 00:41:51,174
We and the other living things
        on this planet

757
00:41:51,208 --> 00:41:53,376
        carry a legacy
      of cosmic evolution

758
00:41:53,410 --> 00:41:55,812
  spanning billions of years.

759
00:41:55,846 --> 00:41:58,047
   If we take that knowledge
           to heart,

760
00:41:58,082 --> 00:42:01,584
  if we come to know and love
    nature as it really is,

761
00:42:01,619 --> 00:42:04,654
    then we will surely be
 remembered by our descendants

762
00:42:04,688 --> 00:42:07,757
     as good, strong links
     in the chain of life.

763
00:42:07,791 --> 00:42:11,094
And our children will continue
    this sacred searching,

764
00:42:11,128 --> 00:42:14,864
 seeing for us as we have seen
  for those who came before,

765
00:42:14,899 --> 00:42:18,167
      discovering wonders
      yet undreamt of...

766
00:42:18,202 --> 00:42:20,403
        in the cosmos.

767
00:42:20,437 --> 00:42:22,805
              ¶ ¶

768
00:42:45,262 --> 00:42:47,630
              ¶ ¶

769
00:43:00,244 --> 00:42:47,630
         Captioned by
  <font color="#00ffff"> Media Access Group at WGBH</font>
        access.wgbh.org

