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[narrator] Scientists believ
there is a hidden substance
deep in space
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00:00:04,772 --> 00:00:07,106
that keeps the cosmos runnin
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00:00:08,175 --> 00:00:11,043
But is that substance real?
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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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and yet it is all around us
it affects everything
that we do.
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[narrator] After searching
for decades,
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00:00:27,728 --> 00:00:32,131
we still don't understand
this inexplicable substance
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[de Rham] We know dark matte
is there because we feel
its strong gravitational pul
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00:00:36,837 --> 00:00:39,671
but it just doesn't
want to talk to us.
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[narrator] There's evidence
that dark matter
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makes up 85%
of all the matter
in the universe.
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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] But if you can't
see dark matter
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and if you can't touch it,
does it really exist?
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[narrator] The Hyades
star cluster.
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This family of 700 stars
is 150 light years from Eart
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At the scale of the universe
it's in our backyard.
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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] For most
of its 650-million-year
lifetime,
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the Hyades enjoyed
a peaceful existence.
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But something
is breaking the calm.
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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] Two star tails
extend from the cluster
center,
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they should be roughly equal
but one tail
is hemorrhaging stars.
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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] Something
with immense
gravitational pull
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has passed by the cluster
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and robbed it of stars.
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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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as much as 10 million times
the mass of the sun.
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[narrator] This monstrous
cosmic mugger
should still be visible,
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but when we point
our telescopes
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to where it should be,
that region is empty.
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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] We know somethin
is out there,
invisible and powerful.
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And whenever we witness
these unseen assaults,
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a prime suspect
gets called in,
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a phantom of physics,
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dark matter.
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So what can we confidently s
about this mysterious
cosmic substance?
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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] We may not be abl
to see or touch dark matter
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but we are very good
at finding its fingerprints
all over the universe.
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We can see dark matter's
use of gravity to break
and bind structures
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and we've been spotting
its handiwork for decades.
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Let's rewind back to 1933.
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Swiss-American physicist,
Fritz Zwicky tracks
strange movements
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in a far off collection
of galaxies called
the Coma cluster.
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He knows he's not
seeing the whole picture.
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Some galaxies are speeding
around the cluster
at inexplicably fast rates.
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[Bullock] Zwicky is looking
at these galaxies
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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]
At these velocities,
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galaxies should be flying of
the cluster like sparks
from fireworks.
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Zwicky realized there had
to be extra stuff,
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in his words, Dunkle Materie
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Dark matter.
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Dark matter.
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Dark matter.
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[narrator] It becomes clear
that Zwicky's Coma cluster
isn't an isolated case.
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Astronomers begin seeing
the same dynamics
within galaxies themselves.
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In systems governed
exclusively by gravity,
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objects farthest away
from the center
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would take the longest
to complete an orbit.
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But in many galaxies,
stars on the outside
are orbiting
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at almost the same rate
as those in the core.
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[Thaller] It's almost like
a photograph record.
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Every part of that record
spins around
like a solid disc.
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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] Physicists come u
with an explanation.
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Galaxies sit in a giant hal
or ball of invisible
dark matter.
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And it's that extra mass
that allows the stars
to turn fast
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all the way out
to the galactic rim.
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[Thaller] Think about actual
taking a disc of dough
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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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that's what would happen
to a galaxy if it weren't
for dark matter.
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Uh, as you spin pizza dough
and you spin it faster
and faster,
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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] By calculating
the mass needed to bind
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those speeding outer stars
to the galaxy,
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physicists are able
to estimate
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how much visible matter
there is compared
to dark matter.
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The results are staggering.
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[Tegmark] All the stuff
we thought existed was just
maybe 15% of our universe.
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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] We may not
be able to see it,
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but dark matter makes up
some 85% of all matter.
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Wherever we look, we can se
its gravity having effects.
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It glues galaxies
like our Milky Way together
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And a close look
reveals dark matter
can also bend light itself.
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It's called
gravitational lensing.
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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.
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[narrator] Gigantic clumps
of any matter create
a gravitational lens.
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Dark matter showed
its space-warping power
in a trick it played
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with a gigantic explosion
in a far off galaxy cluster
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Supernova Refsdal was first
detected in November of 2014
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Supernova Refsdal
is actually one of my favorite
recent results
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00:08:04,985 --> 00:08:07,419
in all of the astronomical
literature.
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That result blew me away.
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So a star explodes,
light is emitted
in all directions,
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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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and then,
another flash appears.
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We see it again,
and again, and again.
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[Mingarelli] We see
the explosion go off
in four parts of the sky.
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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.
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What's going on?
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[narrator] Analysis proves
that these multiple explosio
are the same supernova.
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-[explosion]
-But between this one
dying star and our telescope
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sits a giant mass
of dark matter,
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a huge gravitational lens.
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What that means is that some
of these rays of light
will take much longer,
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more complicated paths
through this region
of space time.
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[narrator] The dark matter
lens turns one supernova
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into a fireworks display
lasting an entire year.
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Dark matter affected
the trajectory of light
from this supernova so much
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that for some
of those trajectories,
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it added a whole light year,
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it took a whole extra year
for light to reach us.
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[narrator] Something is ver
definitely out there
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distorting our view
of the cosmos.
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It's a potent clue
that dark matter is real.
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Now, new evidence suggests
that without it,
we might not exist at all.
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[narrator] The cosmos
is filled with an unseen
substance,
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its mass even bends starligh
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Gravitational lensing sugges
dark matter holds our entir
universe together.
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For decades, this specter
of space has haunted us.
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We've never been able
to pin it down.
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00:10:17,784 --> 00:10:23,922
In 2021, an international te
ran a virtual experiment
to try to predict
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00:10:23,924 --> 00:10:27,626
where dark matter should
be by letting computers
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map out
where we think it lives.
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[Bullock] Because we think
we know how it behaves,
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we can model what it should
be doing in supercomputer
simulations.
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[narrator] The team taught
the computer how dark matte
bends light,
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then applied computational
power to 17,000
unexplored galaxies.
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The model created
a dark matter map.
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I think a lot of people,
when they imagine the universe
on the larger scales,
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think it's sort of boring,
everything's uniform.
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But that's not what we see.
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What's amazing is that
on the larger scales
of the universe,
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we see a very
particular pattern.
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00:11:09,102 --> 00:11:12,470
When we zoom out,
we see this magnificent
structure,
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this cosmic web
that's created by dark matter.
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[narrator]
The interweaving tendrils
of dark matter stretch
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00:11:19,279 --> 00:11:23,882
for thousands of light year
across the cosmos.
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00:11:23,917 --> 00:11:30,088
At the junctions where matte
is concentrated,
we find galaxies form,
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00:11:30,090 --> 00:11:32,457
illuminating
the dark scaffold.
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00:11:34,061 --> 00:11:36,728
If dark matter exists,
scientists believe
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00:11:36,730 --> 00:11:40,932
it makes up 85% of the matte
in the universe,
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00:11:41,000 --> 00:11:45,570
and also controls
the remaining
15% regular matter,
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00:11:45,638 --> 00:11:49,174
like stars, planets, us.
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00:11:50,477 --> 00:11:54,245
If they're right, dark matte
played a critical role
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00:11:54,247 --> 00:11:58,383
in actually building
the universe we see today.
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00:12:03,056 --> 00:12:04,489
2021.
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00:12:04,491 --> 00:12:08,226
Astronomers using
the SkyMapper observatory
in Australia
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00:12:08,228 --> 00:12:14,733
trains specialist optics
on a dwarf galaxy
called Tucana II.
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00:12:14,735 --> 00:12:20,472
The SkyMapper's filters
split up the starlight
into a spectrum of wavelengt
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00:12:20,474 --> 00:12:24,342
revealing some
very ancient light.
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00:12:25,746 --> 00:12:30,181
[Tremblay] One of the best
clocks that we can put
on the universe
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00:12:30,250 --> 00:12:32,283
is the progress of chemistry.
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00:12:32,385 --> 00:12:33,451
Right?
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00:12:33,453 --> 00:12:37,522
The build-up of more complex
elements over time.
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00:12:37,524 --> 00:12:41,893
Stars are nothing
if not factories
of chemical complexity.
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00:12:41,895 --> 00:12:45,597
They slam, uh, particles
together and create
heavier elements,
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00:12:45,665 --> 00:12:48,233
right, through a process
called fusion.
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00:12:48,268 --> 00:12:52,470
The later the generation
of star, the more chemicall
complex it is.
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00:12:52,472 --> 00:12:56,608
[narrator] Tucana II's
spectral signature
reveals its stars contain
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00:12:56,676 --> 00:13:00,512
very few of these heavy
complex elements.
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00:13:00,514 --> 00:13:05,817
A clue that lets
astrophysicists calculate
the age of the galaxy.
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00:13:05,885 --> 00:13:10,688
These are very, very old stars
from the very early days
of the universe
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00:13:10,690 --> 00:13:15,260
when the gas
in the universe was not
that chemically complex.
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00:13:15,962 --> 00:13:19,931
Tucana II might be one
of the oldest known structur
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00:13:19,999 --> 00:13:21,900
that we can see
in our local universe.
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00:13:21,968 --> 00:13:25,336
It could be as old
as 13 billion years.
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00:13:25,338 --> 00:13:28,106
You know, almost as old
as the universe itself.
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00:13:29,843 --> 00:13:33,278
[narrator] This grand old la
of a galaxy is a tiny thing
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00:13:33,313 --> 00:13:35,380
Barely 3,000 stars.
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00:13:37,083 --> 00:13:39,584
And yet, way out
on her galactic rim,
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stars hurdle around
at breakneck speed.
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00:13:43,990 --> 00:13:47,492
[Plait] When you look
at the mass of this
ultra-faint dwarf galaxy,
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00:13:47,494 --> 00:13:50,695
it only has a few thousand
times the mass of the sun.
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00:13:50,697 --> 00:13:52,263
That's really small.
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00:13:52,265 --> 00:13:54,899
And at the speed it's moving,
it should fly apart.
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00:13:54,901 --> 00:14:00,004
[narrator] Tucana II doesn'
break up because
it's glued together,
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00:14:00,006 --> 00:14:04,576
apparently by an incredible
amount of dark matter.
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00:14:04,578 --> 00:14:06,644
When you look at a galaxy
like our Milky Way,
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00:14:06,646 --> 00:14:10,048
it's about 85% dark matter,
which is a lot.
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00:14:10,050 --> 00:14:14,085
But with Tucana II,
it's more like 99%.
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00:14:14,087 --> 00:14:18,356
[narrator] Tucana II is old
among the oldest galaxies
in the universe
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00:14:18,358 --> 00:14:22,360
and it is packed full
of dark matter.
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00:14:22,362 --> 00:14:27,432
Simulations suggest
this dark matter played a ke
role in shaping Tucana II
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00:14:27,434 --> 00:14:31,569
and other very early galaxie
right from the beginning,
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00:14:31,571 --> 00:14:38,843
gathering regular matter
into clumps and building
the first galaxies.
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00:14:38,845 --> 00:14:41,012
[Thaller] The importance
of dark matter
really can't be overstated.
225
00:14:41,014 --> 00:14:44,449
It has actually controlled
the way matter has evolved
226
00:14:44,517 --> 00:14:45,483
since the beginning
of the universe.
227
00:14:45,551 --> 00:14:47,352
It brings matter together.
228
00:14:47,354 --> 00:14:53,091
You need this underlying
structure of dark matter
to make it all happen.
229
00:14:53,093 --> 00:14:58,463
[narrator] Scientists think
that for billions of years
as the early universe grew,
230
00:14:58,465 --> 00:15:00,665
dark matter called the shots
231
00:15:00,667 --> 00:15:06,104
Without its gravity,
structures like the Milky Wa
wouldn't have formed.
232
00:15:07,807 --> 00:15:11,142
We've seen dark matter's
light-bending effects.
233
00:15:11,144 --> 00:15:14,445
We've even deduced
where it should be.
234
00:15:14,447 --> 00:15:18,449
Dark matter really does
appear to exist,
235
00:15:18,451 --> 00:15:22,287
but this evidence
is indirect, circumstantial
236
00:15:23,156 --> 00:15:27,492
To get conclusive proof
that dark matter exists,
237
00:15:27,494 --> 00:15:29,227
don't we need to find some?
238
00:15:29,663 --> 00:15:33,898
If we could find a lump
of dark matter [laughs],
239
00:15:33,967 --> 00:15:37,101
um, that would be one
of the greatest discoveries
in all of nature,
240
00:15:37,103 --> 00:15:38,536
in all of our history, right?
241
00:15:38,538 --> 00:15:40,037
Because we would understand
242
00:15:40,273 --> 00:15:44,275
one of the most fundamental
components for how
our universe works.
243
00:15:44,811 --> 00:15:47,011
Dropping the title,
they love that.
244
00:15:48,148 --> 00:15:52,216
[narrator] It's time to hun
for dark matter itself.
245
00:15:52,218 --> 00:15:56,454
Could it be hiding
in the darkest place of all
246
00:15:57,791 --> 00:15:59,424
Black holes.
247
00:16:09,569 --> 00:16:11,869
[narrator] Scientists believ
an invisible substance
248
00:16:11,938 --> 00:16:15,873
is pulling the strings
in our universe.
249
00:16:15,942 --> 00:16:19,877
But until we see it, sense i
perhaps even touch it,
250
00:16:19,946 --> 00:16:22,447
dark matter is just a theory
251
00:16:23,850 --> 00:16:26,017
Sometimes though,
ideas dreamed up
252
00:16:26,019 --> 00:16:28,319
by scientists come true
253
00:16:28,822 --> 00:16:31,956
like black holes.
254
00:16:31,958 --> 00:16:35,960
Once the stuff
of science fiction
and children's nightmares,
255
00:16:35,962 --> 00:16:40,765
black holes today
are confirmed reality.
256
00:16:40,767 --> 00:16:43,935
So black holes
and dark matter have a ton
of similarities, right?
257
00:16:43,937 --> 00:16:46,471
You know,
an unseen collection of matter
258
00:16:46,473 --> 00:16:48,873
that creates an enormous
gravitational field, check.
259
00:16:48,908 --> 00:16:52,877
It bends light
and causes gravitational
lensing, check.
260
00:16:52,912 --> 00:16:56,347
Tests the boundaries
of known physics, check.
261
00:16:57,617 --> 00:16:59,951
[narrator] It seems crazy
to even ask,
262
00:16:59,953 --> 00:17:01,853
but could our search
for dark matter
263
00:17:01,855 --> 00:17:06,591
end in an idea more
than 100 years old?
264
00:17:06,593 --> 00:17:10,094
Could dark matter
be black holes?
265
00:17:11,664 --> 00:17:14,565
Black holes appear
when stars explode.
266
00:17:14,567 --> 00:17:17,769
And their remaining mass
crunches down into a sphere
267
00:17:17,837 --> 00:17:22,840
so dense even light
can't escape its gravity.
268
00:17:22,842 --> 00:17:27,345
But that's where
the black hole dark matter
theory stumbles.
269
00:17:27,347 --> 00:17:29,614
We know
that black holes happen.
We know how they form.
270
00:17:29,682 --> 00:17:34,919
And we also know that there's
nowhere near enough of them
to be dark matter.
271
00:17:34,921 --> 00:17:38,723
[narrator] Not enough stars
have lived and died
in the history of the univer
272
00:17:38,725 --> 00:17:42,927
to create 85%
of the matter in it.
273
00:17:42,962 --> 00:17:46,230
If dark matter is made up
of black holes,
274
00:17:46,232 --> 00:17:50,668
they would have
to be an entirely new type.
275
00:17:50,670 --> 00:17:55,673
It's possible that these black
holes are of a type
that we've never seen before.
276
00:17:55,741 --> 00:17:59,143
They could be
primordial black holes.
277
00:18:00,580 --> 00:18:03,681
[Hopkins] Primordial black
holes are an idea.
278
00:18:03,683 --> 00:18:05,483
A theoretical concept
at this point
279
00:18:05,485 --> 00:18:10,154
that we've never seen,
but they could exist.
280
00:18:10,189 --> 00:18:15,760
If primordial black holes
are real then the universe
is flooded with black holes.
281
00:18:15,762 --> 00:18:18,362
[Hopkins] The smallest coul
have the mass of Mount Evere
282
00:18:18,397 --> 00:18:20,431
packed into the size
of one atom.
283
00:18:20,433 --> 00:18:27,438
The biggest could be hundreds
of thousands or millions
of times the mass of the sun.
284
00:18:27,507 --> 00:18:30,775
[narrator] Stephen Hawking
first suggested
that primordial black holes
285
00:18:30,777 --> 00:18:35,713
could be dark matter back
in the 1970s.
286
00:18:35,715 --> 00:18:40,384
The idea centers
on what happened
during that intangible momen
287
00:18:40,386 --> 00:18:45,890
13.8 billion years ago,
the big-bang.
288
00:18:45,958 --> 00:18:50,461
Theory says
that primordial black holes
formed in the first fraction
289
00:18:50,463 --> 00:18:52,396
of a second
of the early universe.
290
00:18:52,398 --> 00:18:55,099
It's that time
between when the universe
291
00:18:55,101 --> 00:19:00,571
goes from a pinprick
to this giant inflating
ball of gas.
292
00:19:00,573 --> 00:19:03,741
[narrator] In these first
moments of the universe's
existence,
293
00:19:03,743 --> 00:19:07,145
matter is packed
incredibly tightly.
294
00:19:07,180 --> 00:19:10,515
But it's not quite
evenly spread.
295
00:19:10,517 --> 00:19:16,220
Even the tiniest fluctuation
in density could trigger
gravitational collapses.
296
00:19:17,490 --> 00:19:21,325
In other words,
black holes would
be forming everywhere,
297
00:19:21,861 --> 00:19:24,962
theoretically,
in huge numbers.
298
00:19:25,732 --> 00:19:30,501
By the time one second
has passed in our universe,
299
00:19:30,503 --> 00:19:33,271
you're already making
black holes
300
00:19:33,339 --> 00:19:37,942
thousands, hundreds
of thousands of times
more massive than our sun.
301
00:19:37,944 --> 00:19:41,512
[narrator] The collective ma
of these objects could be va
302
00:19:41,581 --> 00:19:46,617
but could they be 85%
of the universe's matter?
303
00:19:46,619 --> 00:19:48,586
[Sutter] If primordial
black holes really do exist
304
00:19:48,588 --> 00:19:53,658
there might be enough
to explain the dark matter.
305
00:19:53,726 --> 00:20:00,765
[narrator] It's a tantalizin
possibility, but there's on
pretty big problem.
306
00:20:00,767 --> 00:20:03,734
For most scientists,
the physics
of the very early universe
307
00:20:03,736 --> 00:20:06,871
is incomplete
and hard to trust.
308
00:20:06,873 --> 00:20:11,676
Generations of physicists
dismissed primordial
black holes
309
00:20:11,744 --> 00:20:17,014
as myths, fantasies,
astrophysical unicorns,
310
00:20:17,016 --> 00:20:21,219
until that is, an earthshaki
crash in space.
311
00:20:21,788 --> 00:20:24,422
May, 2019.
312
00:20:24,457 --> 00:20:27,458
A violent cosmic
event rocks the USA.
313
00:20:27,460 --> 00:20:29,193
How violent?
314
00:20:29,195 --> 00:20:33,231
Well, the physical distance
between Louisiana
and Washington state
315
00:20:33,266 --> 00:20:39,570
is stretched by nearly
the width of an atom which
is bigger than it sounds.
316
00:20:39,572 --> 00:20:42,573
The Laser Interferometer
Gravitational-Wave Observato
317
00:20:42,575 --> 00:20:45,977
detects this wobble
in space time.
318
00:20:46,479 --> 00:20:51,582
This is the biggest
gravitational wave event
that LIGO has seen.
319
00:20:51,584 --> 00:20:56,554
[narrator] This cosmic
disturbance seems to come
from colliding black holes
320
00:20:56,556 --> 00:21:02,193
but crucially not the ordina
dead star type.
321
00:21:02,228 --> 00:21:06,831
In this LIGO detection,
one of the black holes
is 85 solar masses.
322
00:21:06,833 --> 00:21:12,370
There's no way that a star
could've made that black hole.
323
00:21:12,372 --> 00:21:15,406
[narrator] Physicists believ
there's a range of masses
324
00:21:15,408 --> 00:21:20,878
where dying stars
can't collapse
into black holes.
325
00:21:20,880 --> 00:21:26,817
Instead, stars in this zone
become insanely hot
and rip themselves apart
326
00:21:26,819 --> 00:21:31,289
leaving nothing to crunch do
into a black hole.
327
00:21:32,659 --> 00:21:35,726
Eighty-five solar masses
sits right in the middle
328
00:21:35,795 --> 00:21:39,897
of this so called forbidden
mass range.
329
00:21:39,899 --> 00:21:43,467
The black hole
that LIGO detected
can't be a dead star,
330
00:21:43,469 --> 00:21:47,638
but in theory
it could be primordial.
331
00:21:47,640 --> 00:21:52,476
Could this discarded theory
of dark matter
be back in fashion?
332
00:21:52,478 --> 00:21:55,212
The LIGO detections come up
and everyone says,
333
00:21:55,281 --> 00:21:57,748
"Oh, right,
primordial black holes.
334
00:21:57,750 --> 00:22:00,618
Maybe we should pay
more attention to that."
335
00:22:00,686 --> 00:22:03,054
Primordial black holes can
be really appealing
336
00:22:03,056 --> 00:22:05,956
because they would solve
the dark matter problem.
337
00:22:06,526 --> 00:22:09,694
But unfortunately,
it's not that simple.
338
00:22:09,762 --> 00:22:13,798
The thing with flooding
the universe with primordial
black holes
339
00:22:13,800 --> 00:22:16,334
is that you expect
a lot of collisions.
340
00:22:16,336 --> 00:22:18,636
And so LIGO shouldn't
have seen one,
341
00:22:18,704 --> 00:22:23,040
it should have seen a thousand
of these collisions
and we don't.
342
00:22:24,110 --> 00:22:29,313
[narrator] Many scientists
doubt what LIGO saw
was a primordial black hole
343
00:22:30,283 --> 00:22:34,452
To them, these beasts remai
fairytales of physics,
344
00:22:34,454 --> 00:22:38,489
red herrings in the quest
for solid evidence
of dark matter.
345
00:22:41,828 --> 00:22:43,861
Does dark matter exist?
346
00:22:43,863 --> 00:22:46,630
Or are we chasing shadows?
347
00:22:46,632 --> 00:22:49,467
Some scientists think
it's not only real,
348
00:22:49,469 --> 00:22:52,770
but the dark matter
is within our grasp,
349
00:22:52,772 --> 00:22:57,274
and that it's flying
through our bodies right now
350
00:23:07,120 --> 00:23:11,389
[narrator] We think 85%
of the universe's matter
is dark.
351
00:23:12,558 --> 00:23:15,693
And yet, we've never found
a speck of it.
352
00:23:15,695 --> 00:23:19,797
We can't prove
dark matter exists.
353
00:23:19,832 --> 00:23:25,035
Regular matter is made up
of everyday particles,
like electrons and protons.
354
00:23:26,472 --> 00:23:31,409
Scientists wonder
if dark matter is also
a type of particle.
355
00:23:32,512 --> 00:23:34,712
One of the leading candidates
for dark matter
356
00:23:34,714 --> 00:23:38,449
are these things called
Weakly Interacting
Massive Particles.
357
00:23:38,517 --> 00:23:41,652
They're massive particles
like protons and electrons
and things like that.
358
00:23:41,720 --> 00:23:44,922
But they don't interact well
with normal matters,
so they're weakly interacting.
359
00:23:44,924 --> 00:23:48,092
And they just have this name
because it's awesome
to call them WIMPs.
360
00:23:49,595 --> 00:23:51,962
[narrator] For decades,
scientists have struggled
361
00:23:51,964 --> 00:23:55,966
to find these shy
theoretical particles.
362
00:23:55,968 --> 00:23:59,069
[Oluseyi] The very first
physics research I ever did
in my life
363
00:23:59,071 --> 00:24:04,475
was about actually
measuring directly
dark matter particles,
364
00:24:04,477 --> 00:24:06,143
these so called WIMPs.
365
00:24:06,145 --> 00:24:10,681
And if they exist,
then there will be a flux
of millions of them
366
00:24:10,683 --> 00:24:13,851
through my hand right now,
just by holding out
right here.
367
00:24:13,853 --> 00:24:17,455
If dark matter is actually
made of WIMPs,
if these particles exist,
368
00:24:17,457 --> 00:24:21,525
then we're actually living
basically in a sea of them.
369
00:24:21,527 --> 00:24:25,496
It surrounds
and penetrates us and it bin
the galaxy together.
370
00:24:26,732 --> 00:24:30,768
[narrator] WIMPs don't play
by our rules.
371
00:24:30,770 --> 00:24:33,804
They barely interact
with the world
of regular matter,
372
00:24:33,806 --> 00:24:36,006
so they're hard to detect.
373
00:24:36,509 --> 00:24:38,776
But when they play
with each other,
374
00:24:38,844 --> 00:24:45,216
sparks fly, intense flashes
that we just might
be able to see.
375
00:24:45,952 --> 00:24:49,887
[Plait] As the theory goes,
WIMPs will self-annihilate.
376
00:24:49,889 --> 00:24:53,023
WIMP A and WIMP B
get too close together, poof,
377
00:24:53,025 --> 00:24:55,326
they explode
and they create gamma rays.
378
00:24:56,362 --> 00:25:01,098
[narrator] Gamma rays
are high energy light,
making them easy to spot.
379
00:25:03,536 --> 00:25:07,705
Scientists point
their detectors at the cente
of the Milky Way,
380
00:25:07,707 --> 00:25:12,943
where they believe the WIMP
collision rate should
be especially high.
381
00:25:13,012 --> 00:25:15,212
[Plait] We have a 4 million
solar mass black hole there
382
00:25:15,214 --> 00:25:16,480
There are billions
of stars there.
383
00:25:16,548 --> 00:25:20,751
That's where most of the mass
of the galaxies is densest.
384
00:25:20,819 --> 00:25:24,455
So any WIMPs orbiting
the galaxy will feel
this natural attraction
385
00:25:24,457 --> 00:25:26,891
towards the center
and fall toward it.
386
00:25:26,893 --> 00:25:29,793
[narrator] The Fermi Large
Area Telescope scoured
387
00:25:29,862 --> 00:25:33,264
the center of our galaxy
for more than 10 years.
388
00:25:33,666 --> 00:25:36,333
It detected lots
of gamma rays,
389
00:25:36,335 --> 00:25:41,405
but scientists couldn't tel
if they came
from colliding WIMPs.
390
00:25:41,407 --> 00:25:45,009
The Galactic Center is a mess.
It's like downtown
of a city, right?
391
00:25:45,011 --> 00:25:47,478
That's where everything is,
where all the hustle
and bustle is.
392
00:25:47,480 --> 00:25:49,446
There are stars
exploding there,
393
00:25:49,515 --> 00:25:51,882
just tons of stars, gas,
magnetic fields, a black hole,
394
00:25:51,884 --> 00:25:53,651
a lot of sources
of gamma rays,
395
00:25:53,653 --> 00:25:56,453
so it's very difficult
to tease out the signal.
396
00:25:56,455 --> 00:25:59,056
[narrator] Downtown Milky Wa
was a washout.
397
00:25:59,058 --> 00:26:01,725
So the scientists turned
their attention to planets
398
00:26:01,794 --> 00:26:03,861
living in less noisy
ZIP codes,
399
00:26:03,863 --> 00:26:07,965
where WIMP collisions
should be easier to spot.
400
00:26:07,967 --> 00:26:10,634
One place where you might see
evidence for WIMP collisions
401
00:26:10,636 --> 00:26:12,903
is actually the cores
of exoplanets.
402
00:26:12,905 --> 00:26:19,143
Turns out exoplanets might
be the best dark matter
detector we have.
403
00:26:20,012 --> 00:26:22,880
You can use giant planets
orbiting distant stars
404
00:26:22,882 --> 00:26:26,150
as laboratories
to understand dark matter.
405
00:26:26,886 --> 00:26:30,521
[narrator] We know gravity
should attract WIMPs.
406
00:26:30,589 --> 00:26:35,759
The more gravity,
the more dark matter particl
come together.
407
00:26:35,761 --> 00:26:39,964
Scientists suggest that WIMP
congregate inside the cores
408
00:26:40,032 --> 00:26:42,800
of the Milky Way's
largest gas planets.
409
00:26:42,802 --> 00:26:45,669
In these super-sized
gas giants,
410
00:26:45,671 --> 00:26:51,408
WIMPs could collide,
annihilate, and release
gamma rays.
411
00:26:51,410 --> 00:26:53,477
If there are these WIMPs
that are collecting
the centers
412
00:26:53,479 --> 00:26:56,013
of mass of exoplanets,
the annihilation
of that dark matter
413
00:26:56,015 --> 00:26:57,881
can heat those exoplanets up.
414
00:26:57,883 --> 00:27:02,286
If you have a WIMP-heated
exoplanet, and that's just fun
to say,
415
00:27:02,354 --> 00:27:03,854
this thing is going
to be warm,
416
00:27:03,856 --> 00:27:06,824
it's gonna be warmer
than the heat of space,
which is very cold.
417
00:27:06,826 --> 00:27:09,159
So what you need
is an infrared telescope,
418
00:27:09,161 --> 00:27:11,695
something that sees
an infrared light
and is sensitive enough
419
00:27:11,697 --> 00:27:14,798
to be able to measure
the temperatures
of these things.
420
00:27:14,867 --> 00:27:20,037
[narrator] But a dedicated
telescope like this
won't launch until 2028.
421
00:27:21,741 --> 00:27:25,542
For some dark matter hunters
that's too long to wait.
422
00:27:25,544 --> 00:27:29,480
They argue that WIMPs
do have one characteristic
423
00:27:29,482 --> 00:27:33,150
that should allow us
to detect them
right here on Earth.
424
00:27:33,886 --> 00:27:37,821
The key to detecting WIMPs
is in their name,
it's the W-I.
425
00:27:37,823 --> 00:27:40,824
They're weakly interacting.
They're not not interacting.
426
00:27:40,826 --> 00:27:43,594
They do interact,
it's just very weak
with matter.
427
00:27:43,629 --> 00:27:46,497
And that means that
there are the rare occasions
428
00:27:46,499 --> 00:27:48,766
where it will smack
into a particle
of normal matter
429
00:27:48,834 --> 00:27:51,268
and then there are effects
that we can observe.
430
00:27:52,772 --> 00:27:58,409
[narrator] Scientists in
Gran Sasso in Central Italy
watch for a spark of energy
431
00:27:58,444 --> 00:28:02,680
generated when a WIMP hits
an atom of regular matter.
432
00:28:02,715 --> 00:28:06,517
Their detector, a tank
of super cooled xenon
433
00:28:06,519 --> 00:28:11,488
built thousands of feet
beneath the Earth's surface
434
00:28:11,490 --> 00:28:14,992
The beauty of putting
this detector under a mountain
is that you've got all of this
435
00:28:14,994 --> 00:28:16,727
rock and soil
and everything else
436
00:28:16,729 --> 00:28:18,796
which is blocking
a lot of background noise.
437
00:28:18,831 --> 00:28:20,931
When you're looking
for a WIMP interaction,
438
00:28:20,933 --> 00:28:24,568
you're looking for something
that's very rare
and something very subtle,
439
00:28:24,570 --> 00:28:27,004
so you don't want
other things going on.
440
00:28:27,039 --> 00:28:29,406
You don't want other particles
coming in and messing up
your experiment.
441
00:28:29,475 --> 00:28:33,844
These Weakly Interacting
Massive Particles will pass
right through that mountain,
442
00:28:33,912 --> 00:28:36,413
and then if they smack
into a xenon atom,
we can look at it and go,
443
00:28:36,415 --> 00:28:39,383
"Ah, that was
a dark matter particle."
444
00:28:39,385 --> 00:28:44,922
[narrator] Detecting a WIMP
could be definitive proof
that dark matter exists.
445
00:28:44,990 --> 00:28:49,893
In 2020, the scientists
spotted something
in the results.
446
00:28:49,895 --> 00:28:52,296
But was it
the elusive evidence
447
00:28:52,998 --> 00:28:56,200
or a ghost among the stars?
448
00:29:03,609 --> 00:29:06,744
[ambient music playing]
449
00:29:06,746 --> 00:29:09,279
[narrator] Scientists believ
they can prove
dark matter is real
450
00:29:09,315 --> 00:29:12,616
by detecting WIMPs.
451
00:29:12,618 --> 00:29:16,787
An experiment buried
deep beneath
an Italian mountain
452
00:29:16,789 --> 00:29:21,091
spotted unusual activity
in a tank of regular matter
453
00:29:21,093 --> 00:29:22,893
pure liquid xenon.
454
00:29:22,895 --> 00:29:24,995
[popping]
455
00:29:26,465 --> 00:29:29,967
So a WIMP detector,
like the XENON1T,
456
00:29:30,002 --> 00:29:33,904
waits for a little WIMP,
tiny, tiny little particle
457
00:29:33,972 --> 00:29:36,740
to hit an atom
of normal matter,
458
00:29:36,742 --> 00:29:38,742
and that creates a vibration.
459
00:29:38,744 --> 00:29:42,713
And we can see this entire
block of xenon shake
460
00:29:42,781 --> 00:29:46,250
just a little bit
from that little,
subatomic collision.
461
00:29:47,453 --> 00:29:49,186
[narrator] The intensity
of the vibration
462
00:29:49,188 --> 00:29:52,122
from the particle collision
is critical.
463
00:29:52,124 --> 00:29:58,529
In theory, a WIMP striking
a xenon atom should generat
a powerful shock.
464
00:29:58,531 --> 00:30:03,400
The vibrations XENON1T
detected were too weak.
465
00:30:05,037 --> 00:30:08,005
When a WIMP comes through,
it smashes into the atom.
466
00:30:08,007 --> 00:30:11,508
It seemed like here
something was just sort of
rattling the electrons
467
00:30:11,510 --> 00:30:13,243
on the outside of the atom.
468
00:30:13,278 --> 00:30:15,579
So whatever is causing
these detections was likely
469
00:30:15,581 --> 00:30:18,482
something much smaller
than a WIMP.
470
00:30:18,484 --> 00:30:21,285
[Sutter] Let's take
these results at face value
471
00:30:21,353 --> 00:30:23,921
It... If they're correct,
it's telling us
472
00:30:23,989 --> 00:30:26,423
that the dark matter
isn't a WIMP,
473
00:30:26,458 --> 00:30:28,392
but something
much, much smaller
474
00:30:28,394 --> 00:30:30,327
and something
much, much lighter.
475
00:30:31,363 --> 00:30:34,464
[narrator] The results sugge
that what hit the xenon
476
00:30:34,466 --> 00:30:40,771
was actually a much
smaller theoretical particl
called an axion.
477
00:30:40,839 --> 00:30:44,141
[Bullock] Axions are really
weird particles,
incredibly light.
478
00:30:44,143 --> 00:30:47,911
In fact, almost zero mass
is possible for an axion.
479
00:30:47,913 --> 00:30:50,514
An axion is no bigger
480
00:30:50,582 --> 00:30:55,452
than 150 billionth
the size of an electron.
481
00:30:55,454 --> 00:31:02,726
Compared to a WIMP,
an axion is like a soccer ball
compared to our sun.
482
00:31:02,728 --> 00:31:05,529
[narrator] The sheer tinines
of axions makes them seem
483
00:31:05,531 --> 00:31:08,065
like an unlikely candidate
for dark matter.
484
00:31:09,735 --> 00:31:14,972
If dark matter is real,
it makes up 85% of the matte
in the universe.
485
00:31:18,010 --> 00:31:24,147
To account for all that mass
we would need an almost
unfathomable number of axion
486
00:31:24,950 --> 00:31:28,585
142 trigintillion of them,
in fact.
487
00:31:28,587 --> 00:31:32,022
That's 140
with 93 zeros after it.
488
00:31:33,359 --> 00:31:37,828
If axions exist, space must
swimming with them.
489
00:31:37,830 --> 00:31:42,432
They must be packed
into every corner
of the cosmos.
490
00:31:42,501 --> 00:31:46,003
When regular matter
clumps together,
it forms stars.
491
00:31:46,639 --> 00:31:49,606
So, to prove
dark matter exists,
492
00:31:49,608 --> 00:31:52,442
maybe we should be
looking for dark stars.
493
00:31:53,979 --> 00:31:56,213
There's no reason
they can't exist.
494
00:31:56,215 --> 00:31:58,048
There's even a name for them
495
00:31:58,918 --> 00:32:00,384
Ghost stars.
496
00:32:01,553 --> 00:32:03,820
[Bullock] They're very
weird objects.
497
00:32:03,822 --> 00:32:07,925
These ghost stars are like
nothing we would ever see
in the night sky.
498
00:32:07,927 --> 00:32:09,426
[narrator] We've never seen
a ghost star.
499
00:32:09,428 --> 00:32:14,865
They are theoretical object
made of hypothetical axions
500
00:32:14,867 --> 00:32:20,203
But in theory,
ghost stars should form
like any other star,
501
00:32:20,238 --> 00:32:22,539
pulled together by gravity.
502
00:32:22,541 --> 00:32:28,412
They would be gigantic,
super dense objects
floating through space.
503
00:32:28,414 --> 00:32:32,316
They could reach the mass
of tens of millions of suns
504
00:32:32,818 --> 00:32:35,886
But because they are made
of dark matter,
505
00:32:35,921 --> 00:32:40,691
ghost stars would produce
no energy and emit no light
506
00:32:40,693 --> 00:32:45,662
They would be transparent
to both light and matter.
507
00:32:45,664 --> 00:32:48,865
If you were right next to it,
you wouldn't
even notice it, right?
508
00:32:48,900 --> 00:32:52,469
If we sent a probe through it,
it'd sail right through it
509
00:32:52,471 --> 00:32:55,906
uh, and once it passed
through, it would be
pulled back by its gravity.
510
00:32:55,941 --> 00:33:02,579
[narrator] 85% of the matte
in our universe could consis
of transparent orbs
511
00:33:02,581 --> 00:33:07,317
made of infinitesimally
small, dark matter particles
512
00:33:08,053 --> 00:33:11,221
But do these
invisible stars exist?
513
00:33:11,289 --> 00:33:13,457
The evidence is thin, but..
514
00:33:13,459 --> 00:33:14,758
[tape rewinding]
515
00:33:14,760 --> 00:33:18,428
[narrator] Rewind back to th
LIGO detection in 2019.
516
00:33:21,900 --> 00:33:25,168
The gravitational wave
detector picked up the signa
517
00:33:25,170 --> 00:33:28,372
of two massive
objects colliding.
518
00:33:28,941 --> 00:33:30,374
[pulsating explosion]
519
00:33:31,377 --> 00:33:34,978
We call the event GW190521.
520
00:33:34,980 --> 00:33:38,849
Most scientists agree this w
a black hole collision.
521
00:33:38,851 --> 00:33:43,053
But could it have been
clashing ghost stars?
522
00:33:43,789 --> 00:33:45,989
[Plait] If there are
ghost stars out there
523
00:33:45,991 --> 00:33:47,724
and they can interact with
each other gravitationally,
524
00:33:47,726 --> 00:33:49,893
they may collide.
525
00:33:49,895 --> 00:33:51,828
And when they do,
they would emit
gravitational waves
526
00:33:51,864 --> 00:33:54,931
and it would look
a lot like
two black holes colliding.
527
00:33:54,933 --> 00:34:00,337
In fact, it would look
theoretically very much
like GW190521.
528
00:34:01,673 --> 00:34:04,341
[narrator] One collision,
two explanations.
529
00:34:05,911 --> 00:34:09,379
Primordial black holes
or ghost stars,
530
00:34:10,816 --> 00:34:13,483
LIGO can't tell them apart.
531
00:34:13,485 --> 00:34:18,989
Do these ideas bring us
closer to proving
the existence of dark matter
532
00:34:18,991 --> 00:34:25,128
Or are we just hurtling
further down
a weird physics rabbit hole
533
00:34:25,130 --> 00:34:29,566
[Chiara Mingarelli]
Primordial black holes,
ghost stars, axions,
534
00:34:29,634 --> 00:34:32,135
this is all very
exotic physics.
535
00:34:32,171 --> 00:34:36,740
We can't take for granted
that any of this is real
or that it's not real.
536
00:34:36,742 --> 00:34:37,607
We just don't know.
537
00:34:37,609 --> 00:34:40,544
Dark matter is irritating.
538
00:34:40,546 --> 00:34:43,747
[groans] We know
it's out there.
We see its effects, right?
539
00:34:43,782 --> 00:34:48,919
But we can't see
the dark matter
and that's frustrating.
540
00:34:48,987 --> 00:34:51,888
And it's like a lot
of young fields in astronomy.
541
00:34:51,924 --> 00:34:56,259
We have way more ideas
than we do hard observations.
542
00:34:57,463 --> 00:35:00,397
[narrator] We have ideas,
we have theories,
543
00:35:00,399 --> 00:35:05,435
but without direct
observations, we just can't
back them up with solid proo
544
00:35:06,839 --> 00:35:11,308
The more we look,
the harder it is
to find dark matter.
545
00:35:12,544 --> 00:35:16,813
Maybe it's primordial
black holes
from the early universe.
546
00:35:16,815 --> 00:35:22,285
Maybe it's a sea of particle
that flow right through us
every day.
547
00:35:22,621 --> 00:35:28,625
Or maybe it's gigantic,
transparent ghost stars.
548
00:35:28,627 --> 00:35:34,197
Perhaps it's the combined ma
of Santa's sleigh
and the Easter Bunny's baske
549
00:35:34,199 --> 00:35:39,436
Or maybe all our physics
is based on questionable mat
550
00:35:49,548 --> 00:35:54,851
[narrator] 85% of the stuff
in the universe
is missing in action.
551
00:35:54,853 --> 00:35:58,221
The search for this
dark matter looks hopeless.
552
00:35:59,691 --> 00:36:03,059
This problem of dark matter
is really a tough one.
553
00:36:03,061 --> 00:36:04,160
Everything that
we've predicted
554
00:36:04,162 --> 00:36:07,164
and then gone and looked for,
we're not finding.
555
00:36:07,166 --> 00:36:09,699
It's starting to become
a huge embarrassment.
556
00:36:09,701 --> 00:36:11,902
Surely something
so fundamental
557
00:36:11,904 --> 00:36:13,803
to our cosmology
should be detectable.
558
00:36:13,805 --> 00:36:15,572
And yet, it remains elusive.
559
00:36:17,976 --> 00:36:22,579
[narrator] We're stumbling
blindly around the limits
of our understanding.
560
00:36:22,581 --> 00:36:26,283
As of right now, there are
zero direct observations.
561
00:36:27,619 --> 00:36:31,054
Maybe dark matter
doesn't exist after all.
562
00:36:31,056 --> 00:36:33,890
Instead of searching
for an invisible substance
563
00:36:33,892 --> 00:36:36,760
affecting the universe
with its gravity,
564
00:36:36,762 --> 00:36:41,731
maybe it's gravity
we don't quite understand.
565
00:36:41,733 --> 00:36:45,936
If you're looking in a galaxy
and it's spinning
way too quickly,
566
00:36:45,938 --> 00:36:50,040
either there's a new
ingredient in the galaxy,
567
00:36:50,042 --> 00:36:52,576
like dark matter,
that holds it all together.
568
00:36:52,578 --> 00:36:56,813
Or you're misunderstanding
the laws of physics.
569
00:36:56,815 --> 00:36:58,715
[narrator] To describe
the effects of gravity,
570
00:36:58,717 --> 00:37:04,321
we use the nearly 350-year-o
math of Sir Isaac Newton.
571
00:37:05,924 --> 00:37:10,460
Maybe to explain
the excess gravity
we see in the universe,
572
00:37:10,462 --> 00:37:13,163
it's not extra matter we nee
573
00:37:13,465 --> 00:37:15,498
It's better math.
574
00:37:15,500 --> 00:37:17,601
Although we understand
very well how gravity works
575
00:37:17,603 --> 00:37:19,869
here on Earth
and in our Solar System,
576
00:37:19,871 --> 00:37:22,739
perhaps when you get up
to galactic scales,
577
00:37:22,741 --> 00:37:25,575
it actually behaves
just slightly differently.
578
00:37:25,577 --> 00:37:29,079
And if that were the case,
you can kind of
tweak that idea
579
00:37:29,081 --> 00:37:33,149
until it fits the data we see
of how galaxies
are spinning around
580
00:37:33,151 --> 00:37:36,019
without needing dark matter.
581
00:37:36,922 --> 00:37:38,388
[narrator] Questioning
the math of a legend
582
00:37:38,390 --> 00:37:41,358
of physics might sound
like sacrilege,
583
00:37:41,360 --> 00:37:45,595
but to solve
the dark matter conundrum,
it has been done.
584
00:37:45,597 --> 00:37:50,800
It's called Modified
Newtonian Dynamics
or MOND.
585
00:37:50,802 --> 00:37:56,306
Modeling galaxies
with this math produces
very different results.
586
00:37:57,743 --> 00:38:01,845
On its surface,
MOND is not a bad idea.
587
00:38:01,847 --> 00:38:04,748
In the same way that we would
normally program a computer
588
00:38:04,750 --> 00:38:07,584
to include dark matter
in our simulations,
589
00:38:07,586 --> 00:38:10,487
you can take that out,
and instead program it
590
00:38:10,489 --> 00:38:12,922
with a different law
of gravity with MOND.
591
00:38:12,924 --> 00:38:16,826
And then, you can set up
a kind of spinning mass of gas
592
00:38:16,828 --> 00:38:19,562
and it does seem
to be possible with MOND
593
00:38:19,564 --> 00:38:23,166
to get things settled down
and look a bit
like a real galaxy.
594
00:38:25,971 --> 00:38:29,472
[narrator] Changing the law
of gravity
accurately recreates
595
00:38:29,474 --> 00:38:34,010
the super-fast spin
astronomers see
through their telescopes.
596
00:38:34,012 --> 00:38:37,480
No need for dark matter.
It doesn't exist.
597
00:38:37,916 --> 00:38:39,149
Case closed?
598
00:38:39,584 --> 00:38:40,884
Not by a long shot.
599
00:38:40,886 --> 00:38:43,453
With anything bigger
than a galaxy,
600
00:38:43,455 --> 00:38:46,990
this artificial physics
breaks down.
601
00:38:47,793 --> 00:38:50,994
MOND does really well
on galaxy scales,
602
00:38:50,996 --> 00:38:52,796
but when you zoom out
and you go to larger
603
00:38:52,798 --> 00:38:55,098
and larger structures
in our universe,
604
00:38:55,100 --> 00:38:59,169
like clusters of galaxies,
big, big structure,
605
00:38:59,171 --> 00:39:03,273
you see that MOND by itself
can't reproduce
all of our observations.
606
00:39:03,275 --> 00:39:04,774
There's something missing.
607
00:39:04,776 --> 00:39:05,675
Dark matter.
608
00:39:05,944 --> 00:39:07,377
Dark matter,
dark matter, dark matter.
609
00:39:07,379 --> 00:39:09,012
Dark matter.
610
00:39:09,014 --> 00:39:13,350
In MOND, you still have
to invoke the existence
of material you can't see.
611
00:39:13,985 --> 00:39:15,652
[Andrew Pontzen]
It basically introduces
612
00:39:15,654 --> 00:39:17,854
some of its own
dark matter as well,
613
00:39:17,856 --> 00:39:21,358
which kind of negates
the point of having MOND
in the first place.
614
00:39:24,429 --> 00:39:28,064
[narrator] MOND doesn't
replace dark matter.
615
00:39:28,066 --> 00:39:31,935
The universe still needs
something to hold it togethe
616
00:39:31,937 --> 00:39:33,837
We just don't know what it i
617
00:39:33,839 --> 00:39:37,240
But there are plenty
of new ideas flying around.
618
00:39:38,510 --> 00:39:41,411
In my theory, the dark matter
is a super fluid.
619
00:39:42,848 --> 00:39:45,915
[narrator] It's a radical
new theory of dark matter,
620
00:39:45,984 --> 00:39:48,785
particles not
acting individually,
621
00:39:48,787 --> 00:39:54,023
but flowing as one invisibl
mass around the galaxies.
622
00:39:54,726 --> 00:39:58,628
A super fluid is like
an ordinary fluid that flows,
623
00:39:58,630 --> 00:40:02,132
but in this case,
it flows without
any resistance or viscosity.
624
00:40:02,134 --> 00:40:05,435
If I pour honey,
it will flow very slowly.
625
00:40:05,437 --> 00:40:06,736
It has high viscosity.
626
00:40:06,738 --> 00:40:10,740
A super fluid will just flo
and never stop flowing.
627
00:40:10,742 --> 00:40:14,844
[narrator] As the super flui
dark matter flows
around the universe,
628
00:40:14,846 --> 00:40:21,117
eddies and waves form
large enough to engulf
entire galaxies.
629
00:40:21,119 --> 00:40:24,954
The gravity of the fluid
holds the stars together.
630
00:40:25,991 --> 00:40:31,694
But like most theories
on dark matter,
there's no direct evidence.
631
00:40:31,696 --> 00:40:35,131
If these waves are on the size
of galaxies,
632
00:40:35,133 --> 00:40:39,769
then we have to find
detectors that can detect
those types of huge waves.
633
00:40:39,771 --> 00:40:41,971
They don't exist
at the moment.
634
00:40:42,908 --> 00:40:45,675
[narrator] Which brings us
back to square one.
635
00:40:45,677 --> 00:40:48,611
We just can't prove
that dark matter is real.
636
00:40:48,613 --> 00:40:51,714
Primordial black holes,
ghost stars, WIMPs,
637
00:40:51,716 --> 00:40:55,985
a super fluid sloshing
about the cosmos,
638
00:40:55,987 --> 00:40:59,055
or maybe we're just using
the wrong math.
639
00:41:00,625 --> 00:41:02,859
What's your money on?
640
00:41:02,861 --> 00:41:07,363
If I had to wager $20
on what dark matter is.
641
00:41:07,699 --> 00:41:08,865
Hmm.
642
00:41:08,934 --> 00:41:12,702
I would never place money
on what dark matter is.
643
00:41:12,704 --> 00:41:14,437
I just think we have no idea.
644
00:41:15,173 --> 00:41:20,109
My money is on
dark matter itself is real,
645
00:41:20,111 --> 00:41:22,212
but it's not
the whole picture.
646
00:41:22,214 --> 00:41:26,249
I would say
left socks in dryers.
647
00:41:26,251 --> 00:41:30,720
I would say remote controls
that fall into sofa cushions
and disappear.
648
00:41:30,722 --> 00:41:32,088
I would love there to be
649
00:41:32,090 --> 00:41:35,792
dark matter,
ghost stars, planets,
even dark matter people.
650
00:41:35,794 --> 00:41:37,460
I'm going all black.
651
00:41:37,963 --> 00:41:43,032
I think no current
ideas are correct.
652
00:41:43,034 --> 00:41:47,337
I think dark matter
is something that
we haven't thought of yet.
653
00:41:48,974 --> 00:41:50,507
[narrator]
Does dark matter exist?
654
00:41:51,309 --> 00:41:52,942
Watch the space.