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[narrator] <i> Scientists believ</i>
   <i> there is a hidden substance</i>
          <i> deep in space</i>

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  <i> that keeps the cosmos runnin</i>

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   <i> But is that substance real?</i>

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  We've never seen dark matter,
    it's completely invisible,

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           but we know
     that it has to be there.

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   Not only can you not see it,
   you couldn't really touch it
    or taste it, or smell it,

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   <i> and yet it is all around us</i>
      <i> it affects everything</i>
<i> that we do.</i>

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    [narrator] <i> After searching</i>
           <i> for decades,</i>

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    <i> we still don't understand</i>
   <i> this inexplicable substance</i>

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  [de Rham] <i> We know dark matte</i>
     <i> is there because we feel</i>
  <i> its strong gravitational pul</i>

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       but it just doesn't
       want to talk to us.

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   [narrator] <i> There's evidence</i>
         <i> that dark matter</i>

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           <i> makes up 85%</i>
<i> of all the matter</i>
         <i> in the universe.</i>

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      We can see dark matter
    holding galaxies together

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           and ripping
     other structures apart,
  we even see it bending light.

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   Dark matter itself has been
    around since the beginning
         of the universe.

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       Without dark matter,
       we wouldn't be here.

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   [narrator] <i> But if you can't</i>
         <i> see dark matter</i>

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    <i> and if you can't touch it,</i>
<i> does it really exist?</i>

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      [narrator] <i> The Hyades</i>
          <i> star cluster.</i>

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     <i> This family of 700 stars</i>
  <i> is 150 light years from Eart</i>

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  <i> At the scale of the universe</i>
      <i> it's in our backyard.</i>

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        Hyades is actually
      close enough to Earth

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      that you could see it
       with your naked eye.

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         When you look up
        at the night sky,

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    Hyades is in that V-shape
       in Taurus the Bull.

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[narrator] <i> For most</i>
     <i> of its 650-million-year</i>
            <i> lifetime,</i>

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        <i> the Hyades enjoyed</i>
      <i> a peaceful existence.</i>

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          <i> But something</i>
      <i> is breaking the calm.</i>

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        The Hyades cluster
        is one of the most
  well-studied clusters of stars

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    we have in the entire sky
    and yet there's something

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      very deeply mysterious
            going on.

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    [narrator] <i> Two star tails</i>
<i> extend from the cluster</i>
             <i> center,</i>

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  <i> they should be roughly equal</i>
           <i> but one tail</i>
      <i> is hemorrhaging stars.</i>

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   Something is disrupting it,
    there's something exerting
          a force on it

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       that's ripping stars
       out of their orbits.

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       [narrator] <i> Something</i>
           <i> with immense</i>
        <i> gravitational pull</i>

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    <i> has passed by the cluster</i>

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<i> and robbed it of stars.</i>

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  In order to be gravitationally
        pulling stars out
    of an object like Hyades,

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  you need to have an incredibly
        massive structure,

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   <i> as much as 10 million times</i>
       <i> the mass of the sun.</i>

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    [narrator] <i> This monstrous</i>
          <i> cosmic mugger</i>
     <i> should still be visible,</i>

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        <i> but when we point</i>
          <i> our telescopes</i>

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    <i> to where it should be,</i>
<i> that region is empty.</i>

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      There's nothing there
       and I mean nothing.

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       And not a little bit
        or something dark,
       or something small,

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      but there's literally
     nothing that we can see.

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   [narrator] <i> We know somethin</i>
          <i> is out there,</i>
     <i> invisible and powerful.</i>

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  <i> And whenever we witness</i>
  <i> these unseen assaults,</i>

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         <i> a prime suspect</i>
         <i> gets called in,</i>

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<i> a phantom of physics,</i>

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       <i> dark matter.</i>

54
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  <i> So what can we confidently s</i>
      <i> about this mysterious</i>
        <i> cosmic substance?</i>

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     It does not emit light,
    it does not reflect light,
    it does not absorb light.

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      The only thing we know
        about dark matter
     is that it has gravity.

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    We're not even really sure
       it's matter at all.

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  It's just that that's the only
          thing we know,
that it has gravity.

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  [narrator] <i> We may not be abl</i>
   <i> to see or touch dark matter</i>

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       <i> but we are very good</i>
   <i> at finding its fingerprints</i>
      <i> all over the universe.</i>

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     <i> We can see dark matter's</i>
     <i> use of gravity to break</i>
       <i> and bind structures</i>

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     <i> and we've been spotting</i>
    <i> its handiwork for decades.</i>

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    <i> Let's rewind back to 1933.</i>

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    <i> Swiss-American physicist,</i>
<i> Fritz Zwicky tracks</i>
        <i> strange movements</i>

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     <i> in a far off collection</i>
        <i> of galaxies called</i>
        <i> the Coma cluster.</i>

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        <i> He knows he's not</i>
    <i> seeing the whole picture.</i>

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    <i> Some galaxies are speeding</i>
        <i> around the cluster</i>
   <i> at inexplicably fast rates.</i>

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   [Bullock] <i> Zwicky is looking</i>
        <i> at these galaxies</i>

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       and if the only mass
that was there were the other
      galaxies you can see,

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         you would expect
   these galaxies to be moving
   at about 50 miles a second,

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    then they would stay bound
          to each other
        and not fly apart.

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   Instead, he sees them moving
     at 1,000 miles a second.

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            [narrator]
       <i> At these velocities,</i>

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  <i> galaxies should be flying of</i>
     <i> the cluster like sparks</i>
         <i> from fireworks.</i>

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<i> Zwicky realized there had</i>
        <i> to be extra stuff,</i>

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  <i> in his words, Dunkle Materie</i>

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           Dark matter.

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           Dark matter.

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           Dark matter.

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   [narrator] <i> It becomes clear</i>
    <i> that Zwicky's Coma cluster</i>
     <i> isn't an isolated case.</i>

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     <i> Astronomers begin seeing</i>
        <i> the same dynamics</i>
   <i> within galaxies themselves.</i>

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       <i> In systems governed</i>
     <i> exclusively by gravity,</i>

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<i> objects farthest away</i>
         <i> from the center</i>

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    <i> would take the longest</i>
     <i> to complete an orbit.</i>

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      <i> But in many galaxies,</i>
       <i> stars on the outside</i>
           <i> are orbiting</i>

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     <i> at almost the same rate</i>
      <i> as those in the core.</i>

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    [Thaller] <i> It's almost like</i>
       <i> a photograph record.</i>

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    <i> Every part of that record</i>
           <i> spins around</i>
<i> like a solid disc.</i>

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   The stars are going too fast
   to stay bound to the gravity
          of the galaxy.

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         They should just
    fly right off into space.

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  [narrator] <i> Physicists come u</i>
       <i> with an explanation.</i>

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   <i> Galaxies sit in a giant hal</i>
       <i> or ball of invisible</i>
           <i> dark matter.</i>

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     <i> And it's that extra mass</i>
      <i> that allows the stars</i>
           <i> to turn fast</i>

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<i> all the way out</i>
       <i> to the galactic rim.</i>

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  [Thaller] <i> Think about actual</i>
      <i> taking a disc of dough</i>

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         and spinning it
         to make a pizza.

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      The more you spin it,
   the more those outer regions
   go farther and farther away.

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      Eventually, the dough
   just goes flying everywhere,

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     <i> that's what would happen</i>
    <i> to a galaxy if it weren't</i>
         <i> for dark matter.</i>

100
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<i> Uh, as you spin pizza dough</i>
      <i> and you spin it faster</i>
           <i> and faster,</i>

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   it does hold itself together

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  because there's all this yummy
       gluten that's acting
            as a glue.

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    Dark matter is the gluten
         of our universe.

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    [narrator] <i> By calculating</i>
     <i> the mass needed to bind</i>

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    <i> those speeding outer stars</i>
          <i> to the galaxy,</i>

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       <i> physicists are able</i>
<i> to estimate</i>

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     <i> how much visible matter</i>
        <i> there is compared</i>
         <i> to dark matter.</i>

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   <i> The results are staggering.</i>

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     [Tegmark] <i> All the stuff</i>
   <i> we thought existed was just</i>
    <i> maybe 15% of our universe.</i>

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      That's like if you go
         to a restaurant

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    and leave like the measly
        15% tip, you know,
       that's what we are.

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         I mean, not even
     the majority substance.

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[narrator] <i> We may not</i>
    <i> be able to see it,</i>

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     <i> but dark matter makes up</i>
     <i> some 85% of all matter.</i>

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   <i> Wherever we look, we can se</i>
   <i> its gravity having effects.</i>

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        <i> It glues galaxies</i>
   <i> like our Milky Way together</i>

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         <i> And a close look</i>
       <i> reveals dark matter</i>
   <i> can also bend light itself.</i>

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           <i> It's called</i>
      <i> gravitational lensing.</i>

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A massive object
     can bend space and time,

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      and light must follow
     the curves of that space
            and time.

121
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    [narrator] <i> Gigantic clumps</i>
       <i> of any matter create</i>
      <i> a gravitational lens.</i>

122
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        <i> Dark matter showed</i>
     <i> its space-warping power</i>
       <i> in a trick it played</i>

123
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    <i> with a gigantic explosion</i>
   <i> in a far off galaxy cluster</i>

124
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   <i> Supernova Refsdal was first</i>
<i> detected in November of 2014</i>

125
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        Supernova Refsdal
  is actually one of my favorite
          recent results

126
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    in all of the astronomical
           literature.

127
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    That result blew me away.

128
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       So a star explodes,
         light is emitted
        in all directions,

129
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   and some of it makes its way
        towards the Earth.

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         So far so good.
      This is very standard.

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       So the flash appears

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            <i> and then,</i>
<i> another flash appears.</i>

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         We see it again,
      and again, and again.

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       [Mingarelli] <i> We see</i>
       <i> the explosion go off</i>
    <i> in four parts of the sky.</i>

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     And then, a year later,
    a fifth explosion goes off

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   in a totally different part
           of the sky.

137
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         What's going on?

138
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    [narrator] <i> Analysis proves</i>
  <i> that these multiple explosio</i>
     <i> are the same supernova.</i>

139
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           -[explosion]
<i> -But between this one</i>
  <i> dying star and our telescope</i>

140
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        <i> sits a giant mass</i>
         <i> of dark matter,</i>

141
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    <i> a huge gravitational lens.</i>

142
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   What that means is that some
      of these rays of light
      will take much longer,

143
00:09:01,580 --> 00:09:05,282
      more complicated paths
       through this region
          of space time.

144
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    [narrator] <i> The dark matter</i>
     <i> lens turns one supernova</i>

145
00:09:09,588 --> 00:09:14,224
     <i> into a fireworks display</i>
<i> lasting an entire year.</i>

146
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       Dark matter affected
     the trajectory of light
   from this supernova so much

147
00:09:19,831 --> 00:09:21,865
          that for some
      of those trajectories,

148
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   it added a whole light year,

149
00:09:24,536 --> 00:09:28,438
    <i> it took a whole extra year</i>
      <i> for light to reach us.</i>

150
00:09:29,608 --> 00:09:32,842
   [narrator] <i> Something is ver</i>
       <i> definitely out there</i>

151
00:09:32,911 --> 00:09:35,445
       <i> distorting our view</i>
          <i> of the cosmos.</i>

152
00:09:36,682 --> 00:09:41,117
        <i> It's a potent clue</i>
<i> that dark matter is real.</i>

153
00:09:41,119 --> 00:09:47,090
    <i> Now, new evidence suggests</i>
         <i> that without it,</i>
    <i> we might not exist at all.</i>

154
00:09:54,866 --> 00:09:58,268
      [narrator] <i> The cosmos</i>
     <i> is filled with an unseen</i>
            <i> substance,</i>

155
00:09:58,503 --> 00:10:02,739
  <i> its mass even bends starligh</i>

156
00:10:02,774 --> 00:10:09,212
  <i> Gravitational lensing sugges</i>
   <i> dark matter holds our entir</i>
        <i> universe together.</i>

157
00:10:10,515 --> 00:10:14,651
    <i> For decades, this specter</i>
     <i> of space has haunted us.</i>

158
00:10:14,719 --> 00:10:17,787
<i> We've never been able</i>
         <i> to pin it down.</i>

159
00:10:17,789 --> 00:10:23,927
  <i> In 2021, an international te</i>
     <i> ran a virtual experiment</i>
        <i> to try to predict</i>

160
00:10:23,929 --> 00:10:27,631
     <i> where dark matter should</i>
     <i> be by letting computers</i>

161
00:10:27,699 --> 00:10:30,400
             <i> map out</i>
     <i> where we think it lives.</i>

162
00:10:30,468 --> 00:10:33,003
    [Bullock] <i> Because we think</i>
     <i> we know how it behaves,</i>

163
00:10:33,071 --> 00:10:36,506
   we can model what it should
    be doing in supercomputer
           simulations.

164
00:10:37,676 --> 00:10:42,946
[narrator] <i> The team taught</i>
   <i> the computer how dark matte</i>
           <i> bends light,</i>

165
00:10:42,948 --> 00:10:49,986
    <i> then applied computational</i>
         <i> power to 17,000</i>
       <i> unexplored galaxies.</i>

166
00:10:50,656 --> 00:10:55,558
       <i> The model created</i>
      <i> a dark matter map.</i>

167
00:10:55,560 --> 00:10:58,728
     I think a lot of people,
  when they imagine the universe
      on the larger scales,

168
00:10:58,730 --> 00:11:01,031
    think it's sort of boring,
      everything's uniform.

169
00:11:01,033 --> 00:11:03,500
   But that's not what we see.

170
00:11:03,502 --> 00:11:06,436
What's amazing is that
       on the larger scales
         of the universe,

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00:11:06,438 --> 00:11:09,105
          we see a very
       particular pattern.

172
00:11:09,107 --> 00:11:12,475
        When we zoom out,
     we see this magnificent
            structure,

173
00:11:12,477 --> 00:11:15,378
         this cosmic web
  that's created by dark matter.

174
00:11:16,581 --> 00:11:19,282
            [narrator]
    <i> The interweaving tendrils</i>
      <i> of dark matter stretch</i>

175
00:11:19,284 --> 00:11:23,887
   <i> for thousands of light year</i>
        <i> across the cosmos.</i>

176
00:11:23,922 --> 00:11:30,093
  <i> At the junctions where matte</i>
<i> is concentrated,</i>
      <i> we find galaxies form,</i>

177
00:11:30,095 --> 00:11:32,462
           <i> illuminating</i>
        <i> the dark scaffold.</i>

178
00:11:34,066 --> 00:11:36,733
      <i> If dark matter exists,</i>
        <i> scientists believe</i>

179
00:11:36,735 --> 00:11:40,937
  <i> it makes up 85% of the matte</i>
         <i> in the universe,</i>

180
00:11:41,005 --> 00:11:45,575
        <i> and also controls</i>
          <i> the remaining</i>
       <i> 15% regular matter,</i>

181
00:11:45,643 --> 00:11:49,179
     <i> like stars, planets, us.</i>

182
00:11:50,482 --> 00:11:54,250
  <i> If they're right, dark matte</i>
<i> played a critical role</i>

183
00:11:54,252 --> 00:11:58,388
       <i> in actually building</i>
    <i> the universe we see today.</i>

184
00:12:03,061 --> 00:12:04,494
              <i> 2021.</i>

185
00:12:04,496 --> 00:12:08,231
        <i> Astronomers using</i>
    <i> the SkyMapper observatory</i>
           <i> in Australia</i>

186
00:12:08,233 --> 00:12:14,738
     <i> trains specialist optics</i>
        <i> on a dwarf galaxy</i>
        <i> called Tucana II.</i>

187
00:12:14,740 --> 00:12:20,477
     <i> The SkyMapper's filters</i>
      <i> split up the starlight</i>
  <i> into a spectrum of wavelengt</i>

188
00:12:20,479 --> 00:12:24,347
<i> revealing some</i>
       <i> very ancient light.</i>

189
00:12:25,751 --> 00:12:30,186
    [Tremblay] <i> One of the best</i>
      <i> clocks that we can put</i>
         <i> on the universe</i>

190
00:12:30,255 --> 00:12:32,288
  is the progress of chemistry.

191
00:12:32,390 --> 00:12:33,456
              Right?

192
00:12:33,458 --> 00:12:37,527
   The build-up of more complex
       elements over time.

193
00:12:37,529 --> 00:12:41,898
        <i> Stars are nothing</i>
         <i> if not factories</i>
     <i> of chemical complexity.</i>

194
00:12:41,900 --> 00:12:45,602
     They slam, uh, particles
       together and create
        heavier elements,

195
00:12:45,670 --> 00:12:48,238
right, through a process
          called fusion.

196
00:12:48,273 --> 00:12:52,475
     <i> The later the generation</i>
   <i> of star, the more chemicall</i>
          <i> complex it is.</i>

197
00:12:52,477 --> 00:12:56,613
      [narrator] <i> Tucana II's</i>
        <i> spectral signature</i>
    <i> reveals its stars contain</i>

198
00:12:56,681 --> 00:13:00,517
     <i> very few of these heavy</i>
        <i> complex elements.</i>

199
00:13:00,519 --> 00:13:05,822
         <i> A clue that lets</i>
    <i> astrophysicists calculate</i>
      <i> the age of the galaxy.</i>

200
00:13:05,890 --> 00:13:10,693
These are very, very old stars
     from the very early days
         of the universe

201
00:13:10,695 --> 00:13:15,265
           when the gas
     in the universe was not
     that chemically complex.

202
00:13:15,967 --> 00:13:19,936
      <i> Tucana II might be one</i>
  <i> of the oldest known structur</i>

203
00:13:20,004 --> 00:13:21,905
         <i> that we can see</i>
      <i> in our local universe.</i>

204
00:13:21,973 --> 00:13:25,341
        It could be as old
       as 13 billion years.

205
00:13:25,343 --> 00:13:28,111
     You know, almost as old
     as the universe itself.

206
00:13:29,848 --> 00:13:33,283
  [narrator] <i> This grand old la</i>
<i> of a galaxy is a tiny thing</i>

207
00:13:33,318 --> 00:13:35,385
       <i> Barely 3,000 stars.</i>

208
00:13:37,088 --> 00:13:39,589
         <i> And yet, way out</i>
       <i> on her galactic rim,</i>

209
00:13:39,657 --> 00:13:43,993
       <i> stars hurdle around</i>
       <i> at breakneck speed.</i>

210
00:13:43,995 --> 00:13:47,497
      [Plait] <i> When you look</i>
       <i> at the mass of this</i>
    <i> ultra-faint dwarf galaxy,</i>

211
00:13:47,499 --> 00:13:50,700
    it only has a few thousand
    times the mass of the sun.

212
00:13:50,702 --> 00:13:52,268
       That's really small.

213
00:13:52,270 --> 00:13:54,904
  And at the speed it's moving,
       it should fly apart.

214
00:13:54,906 --> 00:14:00,009
[narrator] <i> Tucana II doesn'</i>
         <i> break up because</i>
       <i> it's glued together,</i>

215
00:14:00,011 --> 00:14:04,581
   <i> apparently by an incredible</i>
      <i> amount of dark matter.</i>

216
00:14:04,583 --> 00:14:06,649
    When you look at a galaxy
       like our Milky Way,

217
00:14:06,651 --> 00:14:10,053
   it's about 85% dark matter,
         which is a lot.

218
00:14:10,055 --> 00:14:14,090
       But with Tucana II,
       it's more like 99%.

219
00:14:14,092 --> 00:14:18,361
   [narrator] <i> Tucana II is old</i>
    <i> among the oldest galaxies</i>
         <i> in the universe</i>

220
00:14:18,363 --> 00:14:22,365
<i> and it is packed full</i>
         <i> of dark matter.</i>

221
00:14:22,367 --> 00:14:27,437
       <i> Simulations suggest</i>
  <i> this dark matter played a ke</i>
    <i> role in shaping Tucana II</i>

222
00:14:27,439 --> 00:14:31,574
  <i> and other very early galaxie</i>
    <i> right from the beginning,</i>

223
00:14:31,576 --> 00:14:38,848
     <i> gathering regular matter</i>
     <i> into clumps and building</i>
       <i> the first galaxies.</i>

224
00:14:38,850 --> 00:14:41,017
     [Thaller] <i> The importance</i>
          <i> of dark matter</i>
   <i> really can't be overstated.</i>

225
00:14:41,019 --> 00:14:44,454
It has actually controlled
    the way matter has evolved

226
00:14:44,522 --> 00:14:45,488
       <i> since the beginning</i>
         <i> of the universe.</i>

227
00:14:45,556 --> 00:14:47,357
    <i> It brings matter together.</i>

228
00:14:47,359 --> 00:14:53,096
  <i> You need this underlying</i>
  <i> structure of dark matter</i>
  <i> to make it all happen.</i>

229
00:14:53,098 --> 00:14:58,468
   [narrator] <i> Scientists think</i>
    <i> that for billions of years</i>
   <i> as the early universe grew,</i>

230
00:14:58,470 --> 00:15:00,670
  <i> dark matter called the shots</i>

231
00:15:00,672 --> 00:15:06,109
       <i> Without its gravity,</i>
<i> structures like the Milky Wa</i>
      <i> wouldn't have formed.</i>

232
00:15:07,812 --> 00:15:11,147
  <i> We've seen dark matter's</i>
  <i> light-bending effects.</i>

233
00:15:11,149 --> 00:15:14,450
    <i> We've even deduced</i>
    <i> where it should be.</i>

234
00:15:14,452 --> 00:15:18,454
     <i> Dark matter really does</i>
         <i> appear to exist,</i>

235
00:15:18,456 --> 00:15:22,292
        <i> but this evidence</i>
   <i> is indirect, circumstantial</i>

236
00:15:23,161 --> 00:15:27,497
     <i> To get conclusive proof</i>
     <i> that dark matter exists,</i>

237
00:15:27,499 --> 00:15:29,232
   <i> don't we need to find some?</i>

238
00:15:29,668 --> 00:15:33,903
If we could find a lump
     of dark matter [laughs],

239
00:15:33,972 --> 00:15:37,106
      um, that would be one
   of the greatest discoveries
        in all of nature,

240
00:15:37,108 --> 00:15:38,541
  in all of our history, right?

241
00:15:38,543 --> 00:15:40,042
   Because we would understand

242
00:15:40,278 --> 00:15:44,280
   one of the most fundamental
        components for how
       our universe works.

243
00:15:44,816 --> 00:15:47,016
       Dropping the title,
         they love that.

244
00:15:48,153 --> 00:15:52,221
   [narrator] <i> It's time to hun</i>
     <i> for dark matter itself.</i>

245
00:15:52,223 --> 00:15:56,459
        <i> Could it be hiding</i>
<i> in the darkest place of all</i>

246
00:15:57,796 --> 00:15:59,429
       <i> Black holes.</i>

247
00:16:09,574 --> 00:16:11,874
  [narrator] <i> Scientists believ</i>
      <i> an invisible substance</i>

248
00:16:11,943 --> 00:16:15,878
      <i> is pulling the strings</i>
         <i> in our universe.</i>

249
00:16:15,947 --> 00:16:19,882
  <i> But until we see it, sense i</i>
      <i> perhaps even touch it,</i>

250
00:16:19,951 --> 00:16:22,452
  <i> dark matter is just a theory</i>

251
00:16:23,855 --> 00:16:26,022
     <i> Sometimes though,</i>
     <i> ideas dreamed up</i>

252
00:16:26,024 --> 00:16:28,324
     <i> by scientists come true</i>

253
00:16:28,827 --> 00:16:31,961
        <i> like black holes.</i>

254
00:16:31,963 --> 00:16:35,965
<i> Once the stuff</i>
        <i> of science fiction</i>
    <i> and children's nightmares,</i>

255
00:16:35,967 --> 00:16:40,770
        <i> black holes today</i>
      <i> are confirmed reality.</i>

256
00:16:40,772 --> 00:16:43,940
          So black holes
    and dark matter have a ton
     of similarities, right?

257
00:16:43,942 --> 00:16:46,476
            You know,
  an unseen collection of matter

258
00:16:46,478 --> 00:16:48,878
     that creates an enormous
   gravitational field, check.

259
00:16:48,913 --> 00:16:52,882
          It bends light
     and causes gravitational
         lensing, check.

260
00:16:52,917 --> 00:16:56,352
Tests the boundaries
     of known physics, check.

261
00:16:57,622 --> 00:16:59,956
    [narrator] <i> It seems crazy</i>
           <i> to even ask,</i>

262
00:16:59,958 --> 00:17:01,858
       <i> but could our search</i>
         <i> for dark matter</i>

263
00:17:01,860 --> 00:17:06,596
       <i> end in an idea more</i>
       <i> than 100 years old?</i>

264
00:17:06,598 --> 00:17:10,099
        <i> Could dark matter</i>
         <i> be black holes?</i>

265
00:17:11,669 --> 00:17:14,570
    <i> Black holes appear</i>
    <i> when stars explode.</i>

266
00:17:14,572 --> 00:17:17,774
     <i> And their remaining mass</i>
   <i> crunches down into a sphere</i>

267
00:17:17,842 --> 00:17:22,845
<i> so dense even light</i>
    <i> can't escape its gravity.</i>

268
00:17:22,847 --> 00:17:27,350
         <i> But that's where</i>
    <i> the black hole dark matter</i>
         <i> theory stumbles.</i>

269
00:17:27,352 --> 00:17:29,619
             We know
     that black holes happen.
      We know how they form.

270
00:17:29,687 --> 00:17:34,924
  And we also know that there's
   nowhere near enough of them
        to be dark matter.

271
00:17:34,926 --> 00:17:38,728
   [narrator] <i> Not enough stars</i>
       <i> have lived and died</i>
  <i> in the history of the univer</i>

272
00:17:38,730 --> 00:17:42,932
<i> to create 85%</i>
       <i> of the matter in it.</i>

273
00:17:42,967 --> 00:17:46,235
    <i> If dark matter is made up</i>
         <i> of black holes,</i>

274
00:17:46,237 --> 00:17:50,673
         <i> they would have</i>
   <i> to be an entirely new type.</i>

275
00:17:50,675 --> 00:17:55,678
  It's possible that these black
       holes are of a type
  that we've never seen before.

276
00:17:55,746 --> 00:17:59,148
          They could be
     primordial black holes.

277
00:18:00,585 --> 00:18:03,686
    [Hopkins] <i> Primordial black</i>
        <i> holes are an idea.</i>

278
00:18:03,688 --> 00:18:05,488
      <i> A theoretical concept</i>
<i> at this point</i>

279
00:18:05,490 --> 00:18:10,159
      that we've never seen,
      but they could exist.

280
00:18:10,194 --> 00:18:15,765
    If primordial black holes
    are real then the universe
   is flooded with black holes.

281
00:18:15,767 --> 00:18:18,367
   [Hopkins] <i> The smallest coul</i>
  <i> have the mass of Mount Evere</i>

282
00:18:18,402 --> 00:18:20,436
       <i> packed into the size</i>
           <i> of one atom.</i>

283
00:18:20,438 --> 00:18:27,443
  The biggest could be hundreds
     of thousands or millions
  of times the mass of the sun.

284
00:18:27,512 --> 00:18:30,780
    [narrator] <i> Stephen Hawking</i>
<i> first suggested</i>
   <i> that primordial black holes</i>

285
00:18:30,782 --> 00:18:35,718
    <i> could be dark matter back</i>
          <i> in the 1970s.</i>

286
00:18:35,720 --> 00:18:40,389
         <i> The idea centers</i>
         <i> on what happened</i>
  <i> during that intangible momen</i>

287
00:18:40,391 --> 00:18:45,895
     <i> 13.8 billion years ago,</i>
          <i> the big-bang.</i>

288
00:18:45,963 --> 00:18:50,466
           Theory says
   that primordial black holes
   formed in the first fraction

289
00:18:50,468 --> 00:18:52,401
           of a second
      of the early universe.

290
00:18:52,403 --> 00:18:55,104
          It's that time
between when the universe

291
00:18:55,106 --> 00:19:00,576
       goes from a pinprick
     to this giant inflating
           ball of gas.

292
00:19:00,578 --> 00:19:03,746
    [narrator] <i> In these first</i>
    <i> moments of the universe's</i>
            <i> existence,</i>

293
00:19:03,748 --> 00:19:07,150
         <i> matter is packed</i>
       <i> incredibly tightly.</i>

294
00:19:07,185 --> 00:19:10,520
        <i> But it's not quite</i>
          <i> evenly spread.</i>

295
00:19:10,522 --> 00:19:16,225
  <i> Even the tiniest fluctuation</i>
     <i> in density could trigger</i>
     <i> gravitational collapses.</i>

296
00:19:17,495 --> 00:19:21,330
<i> In other words,</i>
        <i> black holes would</i>
      <i> be forming everywhere,</i>

297
00:19:21,866 --> 00:19:24,967
          <i> theoretically,</i>
         <i> in huge numbers.</i>

298
00:19:25,737 --> 00:19:30,506
      By the time one second
   has passed in our universe,

299
00:19:30,508 --> 00:19:33,276
      you're already making
           black holes

300
00:19:33,344 --> 00:19:37,947
       thousands, hundreds
      of thousands of times
    more massive than our sun.

301
00:19:37,949 --> 00:19:41,517
  [narrator] <i> The collective ma</i>
  <i> of these objects could be va</i>

302
00:19:41,586 --> 00:19:46,622
      <i> but could they be 85%</i>
<i> of the universe's matter?</i>

303
00:19:46,624 --> 00:19:48,591
      [Sutter] <i> If primordial</i>
   <i> black holes really do exist</i>

304
00:19:48,593 --> 00:19:53,663
      there might be enough
   to explain the dark matter.

305
00:19:53,731 --> 00:20:00,770
  [narrator] <i> It's a tantalizin</i>
   <i> possibility, but there's on</i>
       <i> pretty big problem.</i>

306
00:20:00,772 --> 00:20:03,739
       <i> For most scientists,</i>
           <i> the physics</i>
    <i> of the very early universe</i>

307
00:20:03,741 --> 00:20:06,876
          <i> is incomplete</i>
        <i> and hard to trust.</i>

308
00:20:06,878 --> 00:20:11,681
<i> Generations of physicists</i>
       <i> dismissed primordial</i>
           <i> black holes</i>

309
00:20:11,749 --> 00:20:17,019
       <i> as myths, fantasies,</i>
     <i> astrophysical unicorns,</i>

310
00:20:17,021 --> 00:20:21,224
  <i> until that is, an earthshaki</i>
         <i> crash in space.</i>

311
00:20:21,793 --> 00:20:24,427
        <i> May, 2019.</i>

312
00:20:24,462 --> 00:20:27,463
         <i> A violent cosmic</i>
       <i> event rocks the USA.</i>

313
00:20:27,465 --> 00:20:29,198
       <i> How violent?</i>

314
00:20:29,200 --> 00:20:33,236
   <i> Well, the physical distance</i>
        <i> between Louisiana</i>
       <i> and Washington state</i>

315
00:20:33,271 --> 00:20:39,575
<i> is stretched by nearly</i>
    <i> the width of an atom which</i>
    <i> is bigger than it sounds.</i>

316
00:20:39,577 --> 00:20:42,578
     <i> The Laser Interferometer</i>
  <i> Gravitational-Wave Observato</i>

317
00:20:42,580 --> 00:20:45,982
       <i> detects this wobble</i>
          <i> in space time.</i>

318
00:20:46,484 --> 00:20:51,587
       This is the biggest
     gravitational wave event
       that LIGO has seen.

319
00:20:51,589 --> 00:20:56,559
      [narrator] <i> This cosmic</i>
    <i> disturbance seems to come</i>
    <i> from colliding black holes</i>

320
00:20:56,561 --> 00:21:02,198
<i> but crucially not the ordina</i>
         <i> dead star type.</i>

321
00:21:02,233 --> 00:21:06,836
     In this LIGO detection,
      one of the black holes
       is 85 solar masses.

322
00:21:06,838 --> 00:21:12,375
    There's no way that a star
  could've made that black hole.

323
00:21:12,377 --> 00:21:15,411
  [narrator] <i> Physicists believ</i>
    <i> there's a range of masses</i>

324
00:21:15,413 --> 00:21:20,883
        <i> where dying stars</i>
          <i> can't collapse</i>
        <i> into black holes.</i>

325
00:21:20,885 --> 00:21:26,822
   <i> Instead, stars in this zone</i>
       <i> become insanely hot</i>
<i> and rip themselves apart</i>

326
00:21:26,824 --> 00:21:31,294
  <i> leaving nothing to crunch do</i>
        <i> into a black hole.</i>

327
00:21:32,664 --> 00:21:35,731
     <i> Eighty-five solar masses</i>
     <i> sits right in the middle</i>

328
00:21:35,800 --> 00:21:39,902
   <i> of this so called forbidden</i>
           <i> mass range.</i>

329
00:21:39,904 --> 00:21:43,472
          <i> The black hole</i>
        <i> that LIGO detected</i>
      <i> can't be a dead star,</i>

330
00:21:43,474 --> 00:21:47,643
          <i> but in theory</i>
     <i> it could be primordial.</i>

331
00:21:47,645 --> 00:21:52,481
   <i> Could this discarded theory</i>
<i> of dark matter</i>
       <i> be back in fashion?</i>

332
00:21:52,483 --> 00:21:55,217
   The LIGO detections come up
        and everyone says,

333
00:21:55,286 --> 00:21:57,753
           "Oh, right,
     primordial black holes.

334
00:21:57,755 --> 00:22:00,623
       Maybe we should pay
     more attention to that."

335
00:22:00,691 --> 00:22:03,059
    Primordial black holes can
       be really appealing

336
00:22:03,061 --> 00:22:05,961
     <i> because they would solve</i>
     <i> the dark matter problem.</i>

337
00:22:06,531 --> 00:22:09,699
        But unfortunately,
      it's not that simple.

338
00:22:09,767 --> 00:22:13,803
     The thing with flooding
the universe with primordial
           black holes

339
00:22:13,805 --> 00:22:16,339
        is that you expect
       a lot of collisions.

340
00:22:16,341 --> 00:22:18,641
      And so LIGO shouldn't
          have seen one,

341
00:22:18,709 --> 00:22:23,045
  it should have seen a thousand
       of these collisions
          and we don't.

342
00:22:24,115 --> 00:22:29,318
    [narrator] <i> Many scientists</i>
       <i> doubt what LIGO saw</i>
   <i> was a primordial black hole</i>

343
00:22:30,288 --> 00:22:34,457
   <i> To them, these beasts remai</i>
      <i> fairytales of physics,</i>

344
00:22:34,459 --> 00:22:38,494
    <i> red herrings in the quest</i>
<i> for solid evidence</i>
         <i> of dark matter.</i>

345
00:22:41,833 --> 00:22:43,866
     <i> Does dark matter exist?</i>

346
00:22:43,868 --> 00:22:46,635
    <i> Or are we chasing shadows?</i>

347
00:22:46,637 --> 00:22:49,472
      <i> Some scientists think</i>
       <i> it's not only real,</i>

348
00:22:49,474 --> 00:22:52,775
      <i> but the dark matter</i>
     <i> is within our grasp,</i>

349
00:22:52,777 --> 00:22:57,279
       <i> and that it's flying</i>
  <i> through our bodies right now</i>

350
00:23:07,125 --> 00:23:11,394
     [narrator] <i> We think 85%</i>
     <i> of the universe's matter</i>
             <i> is dark.</i>

351
00:23:12,563 --> 00:23:15,698
<i> And yet, we've never found</i>
          <i> a speck of it.</i>

352
00:23:15,700 --> 00:23:19,802
          <i> We can't prove</i>
       <i> dark matter exists.</i>

353
00:23:19,837 --> 00:23:25,040
    <i> Regular matter is made up</i>
      <i> of everyday particles,</i>
   <i> like electrons and protons.</i>

354
00:23:26,477 --> 00:23:31,414
        <i> Scientists wonder</i>
      <i> if dark matter is also</i>
       <i> a type of particle.</i>

355
00:23:32,517 --> 00:23:34,717
  One of the leading candidates
         for dark matter

356
00:23:34,719 --> 00:23:38,454
     are these things called
        Weakly Interacting
Massive Particles.

357
00:23:38,522 --> 00:23:41,657
    They're massive particles
    like protons and electrons
      and things like that.

358
00:23:41,725 --> 00:23:44,927
   But they don't interact well
       with normal matters,
  so they're weakly interacting.

359
00:23:44,929 --> 00:23:48,097
   And they just have this name
       because it's awesome
       to call them WIMPs.

360
00:23:49,600 --> 00:23:51,967
     [narrator] <i> For decades,</i>
    <i> scientists have struggled</i>

361
00:23:51,969 --> 00:23:55,971
        <i> to find these shy</i>
      <i> theoretical particles.</i>

362
00:23:55,973 --> 00:23:59,074
     [Oluseyi] <i> The very first</i>
<i> physics research I ever did</i>
            <i> in my life</i>

363
00:23:59,076 --> 00:24:04,480
        was about actually
        measuring directly
      dark matter particles,

364
00:24:04,482 --> 00:24:06,148
      these so called WIMPs.

365
00:24:06,150 --> 00:24:10,686
        And if they exist,
    then there will be a flux
       of millions of them

366
00:24:10,688 --> 00:24:13,856
    through my hand right now,
       just by holding out
           right here.

367
00:24:13,858 --> 00:24:17,460
    If dark matter is actually
          made of WIMPs,
    if these particles exist,

368
00:24:17,462 --> 00:24:21,530
    then we're actually living
basically in a sea of them.

369
00:24:21,532 --> 00:24:25,501
           <i> It surrounds</i>
  <i> and penetrates us and it bin</i>
       <i> the galaxy together.</i>

370
00:24:26,737 --> 00:24:30,773
   [narrator] <i> WIMPs don't play</i>
          <i> by our rules.</i>

371
00:24:30,775 --> 00:24:33,809
       <i> They barely interact</i>
          <i> with the world</i>
        <i> of regular matter,</i>

372
00:24:33,811 --> 00:24:36,011
    <i> so they're hard to detect.</i>

373
00:24:36,514 --> 00:24:38,781
        <i> But when they play</i>
         <i> with each other,</i>

374
00:24:38,849 --> 00:24:45,221
   <i> sparks fly, intense flashes</i>
<i> that we just might</i>
         <i> be able to see.</i>

375
00:24:45,957 --> 00:24:49,892
   [Plait] <i> As the theory goes,</i>
   <i> WIMPs will self-annihilate.</i>

376
00:24:49,894 --> 00:24:53,028
        WIMP A and WIMP B
  get too close together, poof,

377
00:24:53,030 --> 00:24:55,331
           they explode
   and they create gamma rays.

378
00:24:56,367 --> 00:25:01,103
      [narrator] <i> Gamma rays</i>
      <i> are high energy light,</i>
    <i> making them easy to spot.</i>

379
00:25:03,541 --> 00:25:07,710
         <i> Scientists point</i>
  <i> their detectors at the cente</i>
        <i> of the Milky Way,</i>

380
00:25:07,712 --> 00:25:12,948
<i> where they believe the WIMP</i>
      <i> collision rate should</i>
       <i> be especially high.</i>

381
00:25:13,017 --> 00:25:15,217
   [Plait] <i> We have a 4 million</i>
   <i> solar mass black hole there</i>

382
00:25:15,219 --> 00:25:16,485
        <i> There are billions</i>
         <i> of stars there.</i>

383
00:25:16,553 --> 00:25:20,756
  That's where most of the mass
   of the galaxies is densest.

384
00:25:20,824 --> 00:25:24,460
      <i> So any WIMPs orbiting</i>
       <i> the galaxy will feel</i>
     <i> this natural attraction</i>

385
00:25:24,462 --> 00:25:26,896
    <i> towards the center</i>
<i> and fall toward it.</i>

386
00:25:26,898 --> 00:25:29,798
  [narrator] <i> The Fermi Large</i>
  <i> Area Telescope scoured</i>

387
00:25:29,867 --> 00:25:33,269
     <i> the center of our galaxy</i>
     <i> for more than 10 years.</i>

388
00:25:33,671 --> 00:25:36,338
         <i> It detected lots</i>
          <i> of gamma rays,</i>

389
00:25:36,340 --> 00:25:41,410
   <i> but scientists couldn't tel</i>
           <i> if they came</i>
      <i> from colliding WIMPs.</i>

390
00:25:41,412 --> 00:25:45,014
  The Galactic Center is a mess.
        It's like downtown
        of a city, right?

391
00:25:45,016 --> 00:25:47,483
   That's where everything is,
where all the hustle
          and bustle is.

392
00:25:47,485 --> 00:25:49,451
        <i> There are stars</i>
       <i> exploding there,</i>

393
00:25:49,520 --> 00:25:51,887
     just tons of stars, gas,
  magnetic fields, a black hole,

394
00:25:51,889 --> 00:25:53,656
         a lot of sources
          of gamma rays,

395
00:25:53,658 --> 00:25:56,458
      so it's very difficult
     to tease out the signal.

396
00:25:56,460 --> 00:25:59,061
  [narrator] <i> Downtown Milky Wa</i>
          <i> was a washout.</i>

397
00:25:59,063 --> 00:26:01,730
     <i> So the scientists turned</i>
    <i> their attention to planets</i>

398
00:26:01,799 --> 00:26:03,866
       <i> living in less noisy</i>
<i> ZIP codes,</i>

399
00:26:03,868 --> 00:26:07,970
      <i> where WIMP collisions</i>
    <i> should be easier to spot.</i>

400
00:26:07,972 --> 00:26:10,639
  One place where you might see
   evidence for WIMP collisions

401
00:26:10,641 --> 00:26:12,908
      is actually the cores
          of exoplanets.

402
00:26:12,910 --> 00:26:19,148
    Turns out exoplanets might
     be the best dark matter
        detector we have.

403
00:26:20,017 --> 00:26:22,885
    You can use giant planets
      orbiting distant stars

404
00:26:22,887 --> 00:26:26,155
         as laboratories
    to understand dark matter.

405
00:26:26,891 --> 00:26:30,526
    [narrator] <i> We know gravity</i>
<i> should attract WIMPs.</i>

406
00:26:30,594 --> 00:26:35,764
        <i> The more gravity,</i>
  <i> the more dark matter particl</i>
          <i> come together.</i>

407
00:26:35,766 --> 00:26:39,969
  <i> Scientists suggest that WIMP</i>
   <i> congregate inside the cores</i>

408
00:26:40,037 --> 00:26:42,805
        <i> of the Milky Way's</i>
       <i> largest gas planets.</i>

409
00:26:42,807 --> 00:26:45,674
       <i> In these super-sized</i>
           <i> gas giants,</i>

410
00:26:45,676 --> 00:26:51,413
       <i> WIMPs could collide,</i>
     <i> annihilate, and release</i>
           <i> gamma rays.</i>

411
00:26:51,415 --> 00:26:53,482
If there are these WIMPs
       that are collecting
           the centers

412
00:26:53,484 --> 00:26:56,018
      of mass of exoplanets,
         the annihilation
       of that dark matter

413
00:26:56,020 --> 00:26:57,886
  can heat those exoplanets up.

414
00:26:57,888 --> 00:27:02,291
    If you have a WIMP-heated
  exoplanet, and that's just fun
             to say,

415
00:27:02,359 --> 00:27:03,859
       this thing is going
           to be warm,

416
00:27:03,861 --> 00:27:06,829
       it's gonna be warmer
     than the heat of space,
       which is very cold.

417
00:27:06,831 --> 00:27:09,164
         So what you need
    is an infrared telescope,

418
00:27:09,166 --> 00:27:11,700
something that sees
        an infrared light
     and is sensitive enough

419
00:27:11,702 --> 00:27:14,803
      to be able to measure
         the temperatures
         of these things.

420
00:27:14,872 --> 00:27:20,042
    [narrator] <i> But a dedicated</i>
       <i> telescope like this</i>
     <i> won't launch until 2028.</i>

421
00:27:21,746 --> 00:27:25,547
  <i> For some dark matter hunters</i>
     <i> that's too long to wait.</i>

422
00:27:25,549 --> 00:27:29,485
      <i> They argue that WIMPs</i>
    <i> do have one characteristic</i>

423
00:27:29,487 --> 00:27:33,155
       <i> that should allow us</i>
<i> to detect them</i>
       <i> right here on Earth.</i>

424
00:27:33,891 --> 00:27:37,826
    The key to detecting WIMPs
        is in their name,
          it's the W-I.

425
00:27:37,828 --> 00:27:40,829
   They're weakly interacting.
   They're not not interacting.

426
00:27:40,831 --> 00:27:43,599
        They do interact,
       it's just very weak
           with matter.

427
00:27:43,634 --> 00:27:46,502
       And that means that
   there are the rare occasions

428
00:27:46,504 --> 00:27:48,771
       where it will smack
         into a particle
         of normal matter

429
00:27:48,839 --> 00:27:51,273
    and then there are effects
that we can observe.

430
00:27:52,777 --> 00:27:58,414
     [narrator] <i> Scientists in</i>
   <i> Gran Sasso in Central Italy</i>
   <i> watch for a spark of energy</i>

431
00:27:58,449 --> 00:28:02,685
    <i> generated when a WIMP hits</i>
    <i> an atom of regular matter.</i>

432
00:28:02,720 --> 00:28:06,522
    <i> Their detector, a tank</i>
     <i> of super cooled xenon</i>

433
00:28:06,524 --> 00:28:11,493
     <i> built thousands of feet</i>
   <i> beneath the Earth's surface</i>

434
00:28:11,495 --> 00:28:14,997
      The beauty of putting
  this detector under a mountain
  is that you've got all of this

435
00:28:14,999 --> 00:28:16,732
rock and soil
       and everything else

436
00:28:16,734 --> 00:28:18,801
        which is blocking
    a lot of background noise.

437
00:28:18,836 --> 00:28:20,936
       When you're looking
     for a WIMP interaction,

438
00:28:20,938 --> 00:28:24,573
   you're looking for something
         that's very rare
    and something very subtle,

439
00:28:24,575 --> 00:28:27,009
        so you don't want
      other things going on.

440
00:28:27,044 --> 00:28:29,411
  You don't want other particles
     coming in and messing up
         your experiment.

441
00:28:29,480 --> 00:28:33,849
     These Weakly Interacting
   Massive Particles will pass
right through that mountain,

442
00:28:33,917 --> 00:28:36,418
      <i> and then if they smack</i>
        <i> into a xenon atom,</i>
    <i> we can look at it and go,</i>

443
00:28:36,420 --> 00:28:39,388
          <i> "Ah, that was</i>
     <i> a dark matter particle."</i>

444
00:28:39,390 --> 00:28:44,927
   [narrator] <i> Detecting a WIMP</i>
    <i> could be definitive proof</i>
     <i> that dark matter exists.</i>

445
00:28:44,995 --> 00:28:49,898
     <i> In 2020, the scientists</i>
        <i> spotted something</i>
         <i> in the results.</i>

446
00:28:49,900 --> 00:28:52,301
            <i> But was it</i>
<i> the elusive evidence</i>

447
00:28:53,003 --> 00:28:56,205
   <i> or a ghost among the stars?</i>

448
00:29:03,614 --> 00:29:06,749
     [ambient music playing]

449
00:29:06,751 --> 00:29:09,284
  [narrator] <i> Scientists believ</i>
          <i> they can prove</i>
       <i> dark matter is real</i>

450
00:29:09,320 --> 00:29:12,621
       <i> by detecting WIMPs.</i>

451
00:29:12,623 --> 00:29:16,792
       <i> An experiment buried</i>
           <i> deep beneath</i>
       <i> an Italian mountain</i>

452
00:29:16,794 --> 00:29:21,096
     <i> spotted unusual activity</i>
   <i> in a tank of regular matter</i>

453
00:29:21,098 --> 00:29:22,898
    <i> pure liquid xenon.</i>

454
00:29:22,900 --> 00:29:25,000
            [popping]

455
00:29:26,470 --> 00:29:29,972
So a WIMP detector,
        like the XENON1T,

456
00:29:30,007 --> 00:29:33,909
     waits for a little WIMP,
    tiny, tiny little particle

457
00:29:33,977 --> 00:29:36,745
          to hit an atom
        of normal matter,

458
00:29:36,747 --> 00:29:38,747
  and that creates a vibration.

459
00:29:38,749 --> 00:29:42,718
    And we can see this entire
       block of xenon shake

460
00:29:42,786 --> 00:29:46,255
        just a little bit
        from that little,
       subatomic collision.

461
00:29:47,458 --> 00:29:49,191
     [narrator] <i> The intensity</i>
         <i> of the vibration</i>

462
00:29:49,193 --> 00:29:52,127
   <i> from the particle collision</i>
           <i> is critical.</i>

463
00:29:52,129 --> 00:29:58,534
<i> In theory, a WIMP striking</i>
   <i> a xenon atom should generat</i>
        <i> a powerful shock.</i>

464
00:29:58,536 --> 00:30:03,405
  <i> The vibrations XENON1T</i>
  <i> detected were too weak.</i>

465
00:30:05,042 --> 00:30:08,010
    When a WIMP comes through,
    it smashes into the atom.

466
00:30:08,012 --> 00:30:11,513
       It seemed like here
    something was just sort of
      rattling the electrons

467
00:30:11,515 --> 00:30:13,248
   on the outside of the atom.

468
00:30:13,283 --> 00:30:15,584
      So whatever is causing
   these detections was likely

469
00:30:15,586 --> 00:30:18,487
      something much smaller
           than a WIMP.

470
00:30:18,489 --> 00:30:21,290
[Sutter] <i> Let's take</i>
   <i> these results at face value</i>

471
00:30:21,358 --> 00:30:23,926
    It... If they're correct,
         it's telling us

472
00:30:23,994 --> 00:30:26,428
       that the dark matter
          isn't a WIMP,

473
00:30:26,463 --> 00:30:28,397
          but something
        much, much smaller

474
00:30:28,399 --> 00:30:30,332
          and something
       much, much lighter.

475
00:30:31,368 --> 00:30:34,469
  [narrator] <i> The results sugge</i>
     <i> that what hit the xenon</i>

476
00:30:34,471 --> 00:30:40,776
       <i> was actually a much</i>
   <i> smaller theoretical particl</i>
         <i> called an axion.</i>

477
00:30:40,844 --> 00:30:44,146
[Bullock] <i> Axions are really</i>
         <i> weird particles,</i>
        <i> incredibly light.</i>

478
00:30:44,148 --> 00:30:47,916
    In fact, almost zero mass
    is possible for an axion.

479
00:30:47,918 --> 00:30:50,519
      An axion is no bigger

480
00:30:50,587 --> 00:30:55,457
        than 150 billionth
     the size of an electron.

481
00:30:55,459 --> 00:31:02,731
       Compared to a WIMP,
  an axion is like a soccer ball
       compared to our sun.

482
00:31:02,733 --> 00:31:05,534
  [narrator] <i> The sheer tinines</i>
    <i> of axions makes them seem</i>

483
00:31:05,536 --> 00:31:08,070
    <i> like an unlikely candidate</i>
<i> for dark matter.</i>

484
00:31:09,740 --> 00:31:14,977
     <i> If dark matter is real,</i>
  <i> it makes up 85% of the matte</i>
         <i> in the universe.</i>

485
00:31:18,015 --> 00:31:24,152
  <i> To account for all that mass</i>
     <i> we would need an almost</i>
  <i> unfathomable number of axion</i>

486
00:31:24,955 --> 00:31:28,590
    <i> 142 trigintillion of them,</i>
             <i> in fact.</i>

487
00:31:28,592 --> 00:31:32,027
            <i> That's 140</i>
     <i> with 93 zeros after it.</i>

488
00:31:33,364 --> 00:31:37,833
  <i> If axions exist, space must </i>
       <i> swimming with them.</i>

489
00:31:37,835 --> 00:31:42,437
<i> They must be packed</i>
        <i> into every corner</i>
          <i> of the cosmos.</i>

490
00:31:42,506 --> 00:31:46,008
       <i> When regular matter</i>
         <i> clumps together,</i>
         <i> it forms stars.</i>

491
00:31:46,644 --> 00:31:49,611
           <i> So, to prove</i>
       <i> dark matter exists,</i>

492
00:31:49,613 --> 00:31:52,447
        <i> maybe we should be</i>
     <i> looking for dark stars.</i>

493
00:31:53,984 --> 00:31:56,218
        <i> There's no reason</i>
        <i> they can't exist.</i>

494
00:31:56,220 --> 00:31:58,053
  <i> There's even a name for them</i>

495
00:31:58,923 --> 00:32:00,389
       <i> Ghost stars.</i>

496
00:32:01,558 --> 00:32:03,825
[Bullock] <i> They're very</i>
          <i> weird objects.</i>

497
00:32:03,827 --> 00:32:07,930
    These ghost stars are like
    nothing we would ever see
        in the night sky.

498
00:32:07,932 --> 00:32:09,431
   [narrator] <i> We've never seen</i>
          <i> a ghost star.</i>

499
00:32:09,433 --> 00:32:14,870
   <i> They are theoretical object</i>
   <i> made of hypothetical axions</i>

500
00:32:14,872 --> 00:32:20,208
          <i> But in theory,</i>
     <i> ghost stars should form</i>
       <i> like any other star,</i>

501
00:32:20,243 --> 00:32:22,544
   <i> pulled together by gravity.</i>

502
00:32:22,546 --> 00:32:28,417
<i> They would be gigantic,</i>
       <i> super dense objects</i>
     <i> floating through space.</i>

503
00:32:28,419 --> 00:32:32,321
    <i> They could reach the mass</i>
   <i> of tens of millions of suns</i>

504
00:32:32,823 --> 00:32:35,891
    <i> But because they are made</i>
         <i> of dark matter,</i>

505
00:32:35,926 --> 00:32:40,696
    <i> ghost stars would produce</i>
   <i> no energy and emit no light</i>

506
00:32:40,698 --> 00:32:45,667
    <i> They would be transparent</i>
    <i> to both light and matter.</i>

507
00:32:45,669 --> 00:32:48,870
  If you were right next to it,
           you wouldn't
even notice it, right?

508
00:32:48,905 --> 00:32:52,474
  If we sent a probe through it,
    it'd sail right through it

509
00:32:52,476 --> 00:32:55,911
      uh, and once it passed
       through, it would be
   pulled back by its gravity.

510
00:32:55,946 --> 00:33:02,584
   [narrator] <i> 85% of the matte</i>
  <i> in our universe could consis</i>
       <i> of transparent orbs</i>

511
00:33:02,586 --> 00:33:07,322
     <i> made of infinitesimally</i>
  <i> small, dark matter particles</i>

512
00:33:08,058 --> 00:33:11,226
           <i> But do these</i>
      <i> invisible stars exist?</i>

513
00:33:11,294 --> 00:33:13,462
   <i> The evidence is thin, but..</i>

514
00:33:13,464 --> 00:33:14,763
[tape rewinding]

515
00:33:14,765 --> 00:33:18,433
  [narrator] <i> Rewind back to th</i>
     <i> LIGO detection in 2019.</i>

516
00:33:21,905 --> 00:33:25,173
      <i> The gravitational wave</i>
  <i> detector picked up the signa</i>

517
00:33:25,175 --> 00:33:28,377
          <i> of two massive</i>
        <i> objects colliding.</i>

518
00:33:28,946 --> 00:33:30,379
      [pulsating explosion]

519
00:33:31,382 --> 00:33:34,983
   <i> We call the event GW190521.</i>

520
00:33:34,985 --> 00:33:38,854
  <i> Most scientists agree this w</i>
     <i> a black hole collision.</i>

521
00:33:38,856 --> 00:33:43,058
    <i> But could it have been</i>
     <i> clashing ghost stars?</i>

522
00:33:43,794 --> 00:33:45,994
[Plait] <i> If there are</i>
      <i> ghost stars out there</i>

523
00:33:45,996 --> 00:33:47,729
    and they can interact with
   each other gravitationally,

524
00:33:47,731 --> 00:33:49,898
        they may collide.

525
00:33:49,900 --> 00:33:51,833
        And when they do,
         they would emit
       gravitational waves

526
00:33:51,869 --> 00:33:54,936
        and it would look
            a lot like
    two black holes colliding.

527
00:33:54,938 --> 00:34:00,342
      In fact, it would look
     theoretically very much
          like GW190521.

528
00:34:01,678 --> 00:34:04,346
    [narrator] <i> One collision,</i>
        <i> two explanations.</i>

529
00:34:05,916 --> 00:34:09,384
<i> Primordial black holes</i>
         <i> or ghost stars,</i>

530
00:34:10,821 --> 00:34:13,488
   <i> LIGO can't tell them apart.</i>

531
00:34:13,490 --> 00:34:18,994
     <i> Do these ideas bring us</i>
        <i> closer to proving</i>
  <i> the existence of dark matter</i>

532
00:34:18,996 --> 00:34:25,133
     <i> Or are we just hurtling</i>
           <i> further down</i>
   <i> a weird physics rabbit hole</i>

533
00:34:25,135 --> 00:34:29,571
       [Chiara Mingarelli]
     <i> Primordial black holes,</i>
       <i> ghost stars, axions,</i>

534
00:34:29,639 --> 00:34:32,140
         this is all very
         exotic physics.

535
00:34:32,176 --> 00:34:36,745
We can't take for granted
     that any of this is real
      or that it's not real.

536
00:34:36,747 --> 00:34:37,612
       We just don't know.

537
00:34:37,614 --> 00:34:40,549
    Dark matter is irritating.

538
00:34:40,551 --> 00:34:43,752
         [groans] We know
         it's out there.
    We see its effects, right?

539
00:34:43,787 --> 00:34:48,924
         But we can't see
         the dark matter
     and that's frustrating.

540
00:34:48,992 --> 00:34:51,893
       And it's like a lot
  of young fields in astronomy.

541
00:34:51,929 --> 00:34:56,264
      We have way more ideas
  than we do hard observations.

542
00:34:57,468 --> 00:35:00,402
    [narrator] <i> We have ideas,</i>
<i> we have theories,</i>

543
00:35:00,404 --> 00:35:05,440
        <i> but without direct</i>
   <i> observations, we just can't</i>
  <i> back them up with solid proo</i>

544
00:35:06,844 --> 00:35:11,313
        <i> The more we look,</i>
         <i> the harder it is</i>
       <i> to find dark matter.</i>

545
00:35:12,549 --> 00:35:16,818
      <i> Maybe it's primordial</i>
           <i> black holes</i>
     <i> from the early universe.</i>

546
00:35:16,820 --> 00:35:22,290
  <i> Maybe it's a sea of particle</i>
    <i> that flow right through us</i>
            <i> every day.</i>

547
00:35:22,626 --> 00:35:28,630
<i> Or maybe it's gigantic,</i>
     <i> transparent ghost stars.</i>

548
00:35:28,632 --> 00:35:34,202
  <i> Perhaps it's the combined ma</i>
        <i> of Santa's sleigh</i>
  <i> and the Easter Bunny's baske</i>

549
00:35:34,204 --> 00:35:39,441
     <i> Or maybe all our physics</i>
  <i> is based on questionable mat</i>

550
00:35:49,553 --> 00:35:54,856
   [narrator] <i> 85% of the stuff</i>
         <i> in the universe</i>
      <i> is missing in action.</i>

551
00:35:54,858 --> 00:35:58,226
       <i> The search for this</i>
   <i> dark matter looks hopeless.</i>

552
00:35:59,696 --> 00:36:03,064
   This problem of dark matter
is really a tough one.

553
00:36:03,066 --> 00:36:04,165
         Everything that
         we've predicted

554
00:36:04,167 --> 00:36:07,169
  and then gone and looked for,
        we're not finding.

555
00:36:07,171 --> 00:36:09,704
     It's starting to become
      a huge embarrassment.

556
00:36:09,706 --> 00:36:11,907
         Surely something
          so fundamental

557
00:36:11,909 --> 00:36:13,808
         to our cosmology
      should be detectable.

558
00:36:13,810 --> 00:36:15,577
   And yet, it remains elusive.

559
00:36:17,981 --> 00:36:22,584
    [narrator] <i> We're stumbling</i>
    <i> blindly around the limits</i>
      <i> of our understanding.</i>

560
00:36:22,586 --> 00:36:26,288
<i> As of right now, there are</i>
    <i> zero direct observations.</i>

561
00:36:27,624 --> 00:36:31,059
        <i> Maybe dark matter</i>
     <i> doesn't exist after all.</i>

562
00:36:31,061 --> 00:36:33,895
       <i> Instead of searching</i>
    <i> for an invisible substance</i>

563
00:36:33,897 --> 00:36:36,765
      <i> affecting the universe</i>
        <i> with its gravity,</i>

564
00:36:36,767 --> 00:36:41,736
        <i> maybe it's gravity</i>
    <i> we don't quite understand.</i>

565
00:36:41,738 --> 00:36:45,941
  If you're looking in a galaxy
        and it's spinning
         way too quickly,

566
00:36:45,943 --> 00:36:50,045
       either there's a new
ingredient in the galaxy,

567
00:36:50,047 --> 00:36:52,581
        like dark matter,
   that holds it all together.

568
00:36:52,583 --> 00:36:56,818
    Or you're misunderstanding
       the laws of physics.

569
00:36:56,820 --> 00:36:58,720
      [narrator] <i> To describe</i>
     <i> the effects of gravity,</i>

570
00:36:58,722 --> 00:37:04,326
  <i> we use the nearly 350-year-o</i>
    <i> math of Sir Isaac Newton.</i>

571
00:37:05,929 --> 00:37:10,465
         <i> Maybe to explain</i>
        <i> the excess gravity</i>
     <i> we see in the universe,</i>

572
00:37:10,467 --> 00:37:13,168
  <i> it's not extra matter we nee</i>

573
00:37:13,470 --> 00:37:15,503
        <i> It's better math.</i>

574
00:37:15,505 --> 00:37:17,606
Although we understand
   very well how gravity works

575
00:37:17,608 --> 00:37:19,874
          here on Earth
     and in our Solar System,

576
00:37:19,876 --> 00:37:22,744
     perhaps when you get up
       to galactic scales,

577
00:37:22,746 --> 00:37:25,580
       it actually behaves
    just slightly differently.

578
00:37:25,582 --> 00:37:29,084
    And if that were the case,
         you can kind of
         tweak that idea

579
00:37:29,086 --> 00:37:33,154
  until it fits the data we see
         of how galaxies
       are spinning around

580
00:37:33,156 --> 00:37:36,024
   without needing dark matter.

581
00:37:36,927 --> 00:37:38,393
   [narrator] <i> Questioning</i>
<i> the math of a legend</i>

582
00:37:38,395 --> 00:37:41,363
      <i> of physics might sound</i>
         <i> like sacrilege,</i>

583
00:37:41,365 --> 00:37:45,600
           <i> but to solve</i>
    <i> the dark matter conundrum,</i>
        <i> it has been done.</i>

584
00:37:45,602 --> 00:37:50,805
       <i> It's called Modified</i>
        <i> Newtonian Dynamics</i>
             <i> or MOND.</i>

585
00:37:50,807 --> 00:37:56,311
        <i> Modeling galaxies</i>
     <i> with this math produces</i>
     <i> very different results.</i>

586
00:37:57,748 --> 00:38:01,850
         On its surface,
     MOND is not a bad idea.

587
00:38:01,852 --> 00:38:04,753
In the same way that we would
   normally program a computer

588
00:38:04,755 --> 00:38:07,589
      to include dark matter
       in our simulations,

589
00:38:07,591 --> 00:38:10,492
      you can take that out,
      and instead program it

590
00:38:10,494 --> 00:38:12,927
   <i> with a different law</i>
   <i> of gravity with MOND.</i>

591
00:38:12,929 --> 00:38:16,831
     And then, you can set up
  a kind of spinning mass of gas

592
00:38:16,833 --> 00:38:19,567
         <i> and it does seem</i>
     <i> to be possible with MOND</i>

593
00:38:19,569 --> 00:38:23,171
    <i> to get things settled down</i>
          <i> and look a bit</i>
       <i> like a real galaxy.</i>

594
00:38:25,976 --> 00:38:29,477
[narrator] <i> Changing the law</i>
            <i> of gravity</i>
       <i> accurately recreates</i>

595
00:38:29,479 --> 00:38:34,015
       <i> the super-fast spin</i>
         <i> astronomers see</i>
    <i> through their telescopes.</i>

596
00:38:34,017 --> 00:38:37,485
     <i> No need for dark matter.</i>
        <i> It doesn't exist.</i>

597
00:38:37,921 --> 00:38:39,154
       <i> Case closed?</i>

598
00:38:39,589 --> 00:38:40,889
       <i> Not by a long shot.</i>

599
00:38:40,891 --> 00:38:43,458
       <i> With anything bigger</i>
          <i> than a galaxy,</i>

600
00:38:43,460 --> 00:38:46,995
     <i> this artificial physics</i>
           <i> breaks down.</i>

601
00:38:47,798 --> 00:38:50,999
MOND does really well
        on galaxy scales,

602
00:38:51,001 --> 00:38:52,801
      but when you zoom out
       and you go to larger

603
00:38:52,803 --> 00:38:55,103
      and larger structures
         in our universe,

604
00:38:55,105 --> 00:38:59,174
    <i> like clusters of galaxies,</i>
       <i> big, big structure,</i>

605
00:38:59,176 --> 00:39:03,278
   <i> you see that MOND by itself</i>
         <i> can't reproduce</i>
     <i> all of our observations.</i>

606
00:39:03,280 --> 00:39:04,779
    <i> There's something missing.</i>

607
00:39:04,781 --> 00:39:05,680
           Dark matter.

608
00:39:05,949 --> 00:39:07,382
           Dark matter,
    dark matter, dark matter.

609
00:39:07,384 --> 00:39:09,017
Dark matter.

610
00:39:09,019 --> 00:39:13,355
     In MOND, you still have
     to invoke the existence
    of material you can't see.

611
00:39:13,990 --> 00:39:15,657
         [Andrew Pontzen]
     <i> It basically introduces</i>

612
00:39:15,659 --> 00:39:17,859
         <i> some of its own</i>
       <i> dark matter as well,</i>

613
00:39:17,861 --> 00:39:21,363
      which kind of negates
     the point of having MOND
       in the first place.

614
00:39:24,434 --> 00:39:28,069
   [narrator] <i> MOND doesn't</i>
   <i> replace dark matter.</i>

615
00:39:28,071 --> 00:39:31,940
     <i> The universe still needs</i>
  <i> something to hold it togethe</i>

616
00:39:31,942 --> 00:39:33,842
<i> We just don't know what it i</i>

617
00:39:33,844 --> 00:39:37,245
       <i> But there are plenty</i>
   <i> of new ideas flying around.</i>

618
00:39:38,515 --> 00:39:41,416
  In my theory, the dark matter
        is a super fluid.

619
00:39:42,853 --> 00:39:45,920
    [narrator] <i> It's a radical</i>
    <i> new theory of dark matter,</i>

620
00:39:45,989 --> 00:39:48,790
          <i> particles not</i>
       <i> acting individually,</i>

621
00:39:48,792 --> 00:39:54,028
   <i> but flowing as one invisibl</i>
    <i> mass around the galaxies.</i>

622
00:39:54,731 --> 00:39:58,633
      A super fluid is like
  an ordinary fluid that flows,

623
00:39:58,635 --> 00:40:02,137
        but in this case,
it flows without
   any resistance or viscosity.

624
00:40:02,139 --> 00:40:05,440
         <i> If I pour honey,</i>
    <i> it will flow very slowly.</i>

625
00:40:05,442 --> 00:40:06,741
  <i> It has high viscosity.</i>

626
00:40:06,743 --> 00:40:10,745
   <i> A super fluid will just flo</i>
     <i> and never stop flowing.</i>

627
00:40:10,747 --> 00:40:14,849
  [narrator] <i> As the super flui</i>
        <i> dark matter flows</i>
       <i> around the universe,</i>

628
00:40:14,851 --> 00:40:21,122
      <i> eddies and waves form</i>
      <i> large enough to engulf</i>
         <i> entire galaxies.</i>

629
00:40:21,124 --> 00:40:24,959
<i> The gravity of the fluid</i>
    <i> holds the stars together.</i>

630
00:40:25,996 --> 00:40:31,699
      <i> But like most theories</i>
         <i> on dark matter,</i>
   <i> there's no direct evidence.</i>

631
00:40:31,701 --> 00:40:35,136
  If these waves are on the size
           of galaxies,

632
00:40:35,138 --> 00:40:39,774
       then we have to find
    detectors that can detect
    those types of huge waves.

633
00:40:39,776 --> 00:40:41,976
         They don't exist
          at the moment.

634
00:40:42,913 --> 00:40:45,680
    [narrator] <i> Which brings us</i>
       <i> back to square one.</i>

635
00:40:45,682 --> 00:40:48,616
<i> We just can't prove</i>
    <i> that dark matter is real.</i>

636
00:40:48,618 --> 00:40:51,719
     <i> Primordial black holes,</i>
       <i> ghost stars, WIMPs,</i>

637
00:40:51,721 --> 00:40:55,990
      <i> a super fluid sloshing</i>
        <i> about the cosmos,</i>

638
00:40:55,992 --> 00:40:59,060
    <i> or maybe we're just using</i>
         <i> the wrong math.</i>

639
00:41:00,630 --> 00:41:02,864
      <i> What's your money on?</i>

640
00:41:02,866 --> 00:41:07,368
      If I had to wager $20
     on what dark matter is.

641
00:41:07,704 --> 00:41:08,870
               Hmm.

642
00:41:08,939 --> 00:41:12,707
    I would never place money
     on what dark matter is.

643
00:41:12,709 --> 00:41:14,442
I just think we have no idea.

644
00:41:15,178 --> 00:41:20,114
          My money is on
   dark matter itself is real,

645
00:41:20,116 --> 00:41:22,217
           but it's not
        the whole picture.

646
00:41:22,219 --> 00:41:26,254
           I would say
      left socks in dryers.

647
00:41:26,256 --> 00:41:30,725
   I would say remote controls
   that fall into sofa cushions
          and disappear.

648
00:41:30,727 --> 00:41:32,093
     I would love there to be

649
00:41:32,095 --> 00:41:35,797
           dark matter,
      ghost stars, planets,
     even dark matter people.

650
00:41:35,799 --> 00:41:37,465
       I'm going all black.

651
00:41:37,968 --> 00:41:43,037
        I think no current
        ideas are correct.

652
00:41:43,039 --> 00:41:47,342
I think dark matter
        is something that
    we haven't thought of yet.

653
00:41:48,979 --> 00:41:50,512
            [narrator]
     <i> Does dark matter exist?</i>

654
00:41:51,314 --> 00:41:52,947
     <i> Watch the space.</i>


