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Our universe is at war.
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The universe is a very violent
and deadly place.
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Entire galaxies fight to the death.
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Talk about clash of the titans.
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It doesn't get more titanic
than this.
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It's a slaughter.
It's a massacre.
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Only the strongest survive.
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If a galaxy wants to stay alive,
it has to feed on other galaxies.
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Our own galaxy
also fights for survival.
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We are facing
the ultimate destruction
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of the Milky Way galaxy.
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These battles are how galaxies live,
grow and die.
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These collisions got us
to where we are today,
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and they're gonna determine
the future of the universe.
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In 2018, astronomers used
the Gaia space telescope
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to map our Milky Way galaxy.
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They tracked the movements of
a billion stars.
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And they found that some behave
very strangely.
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When astronomers were mapping stars
in our galaxy,
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they found a whole bunch that were
on similar but very strange orbits.
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Most stars in the Milky Way
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are orbiting in a sort of
regular pattern,
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but these stars at the centre,
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they're in these highly
elongated orbits.
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Coming in from very far,
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swinging around the centre of
our galaxy,
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and then going back out again,
a little bit like a comet does.
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This group of stars plunges wildly
through the centre of our galaxy.
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When you track their direction
and speed on a chart,
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you get a shape
that looks a bit like a sausage.
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This doesn't sound very sciency,
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but this sausage is really
what the stars look like
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if you look at the shapes of
their orbits
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in a certain configuration.
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What sent so many stars
on such a strange path?
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It must have been a huge event.
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We think these stars are the result
of a past cosmic collision.
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They are casualties
from an enormous battle
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between the Milky Way
and a foreign galactic army.
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They don't move like stars
in the Milky Way
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because they're not from
the Milky Way.
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These stars are actually
alien stars.
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They're invaders
from outer, outer space
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The attackers left their mark
on the Milky Way.
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We find similar battle scars
on galaxies across the universe.
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Our models of galaxy formation
are still pretty uncertain.
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We still don't really understand
how galaxies got to where they are,
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how we go from the Big Bang
to the Milky Way.
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Wars between galaxies
have profound consequences.
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For the winners, the losers
and for us.
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00:03:15,040 --> 00:03:17,840
What we're learning
is that these galactic battles
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have had a huge impact on what
the universe looks like today.
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Our understanding of galaxies
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has changed entirely
in the last few decades.
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We understand now that
every big galaxy like the Milky Way
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started from many smaller things
colliding,
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changing each other as they went.
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Nearly ten billion years ago,
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the sausage stars were part of
a foreign galaxy.
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It was on a collision course
with our home, the Milky Way.
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We call this invading army
the Sausage Galaxy,
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or Gaia-Enceladus.
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The galaxy that we fought
probably had about 50 billion stars,
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so we're talking about something
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that is a significant fraction of
the size of the Milky Way.
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Gaia-Enceladus was a tough opponent.
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But the Milky Way was 20 times
its mass,
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and that makes a huge difference.
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When galaxies interact
with each other,
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size definitely matters.
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The bigger galaxies are gonna
dominate over the smaller ones,
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ripping them apart
and essentially consuming them.
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Galaxy interactions
are all about bullies.
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The bigger you are,
the badder you are.
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When two galaxies collide,
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it's like two massive armies
marching towards each other.
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And these galaxies aren't fighting
with knives or spears or guns,
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or even nuclear bombs,
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they're fighting with something
much more powerful.
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Gravity itself.
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Each galaxy contains
billions of stars and planets.
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And a supermassive black hole,
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millions of times
the mass of the sun.
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00:05:06,520 --> 00:05:09,520
That's a lot of
gravitational firepower.
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As these galaxies approach
each other,
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you can get tidal effects.
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The same way that the moon
can raise tides
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on one side of the Earth
and the opposite side,
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one galaxy can stretch
another galaxy
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along a certain direction.
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As Gaia-Enceladus
advanced towards us,
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our galaxy's superior gravity
grabbed hold of the smaller galaxy.
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As it approached,
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the gravity from the Milky Way
would've stretched it out.
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Gaia-Enceladus was distorted,
but not defeated.
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The battle was just beginning.
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It would've passed through
our galaxy,
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maybe orbiting a couple of times,
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before being torn apart
by our gravity.
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The Milky Way's gravitational power
ripped Gaia-Enceladus apart
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and captured billions of its stars.
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And eventually most of those stars
would have then settled down
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into the disc of the Milky Way
and become a part of it.
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Little galaxy try to take on
the Milky Way,
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you gonna get what's coming to you.
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Despite winning the battle,
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the Milky Way suffered
serious damage.
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The collision with
the Sausage Galaxy
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left a scar on the Milky Way,
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and when we look
near the centre of our galaxy,
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we see a bulge just left over
from that collision.
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The Milky Way isn't the only galaxy
scarred by war.
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Across the universe, rival armies
made up of billions of stars
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slug it out,
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leaving behind distorted and damaged
casualties of war.
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There's a million different
subcategories of them.
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There's tadpole galaxies
that have long tails,
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longer than our own galaxy.
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There are things like
Arp-Madore 2026,
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where you see
this eerie glowing face,
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two big eyes looking right at you
from across the universe.
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There are galaxies that look like
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they might've collided
and blown holes through each other.
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These battle scars give us
important clues
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about one of the biggest mysteries
in astronomy.
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How galaxies develop and grow.
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But there's a problem.
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We can't watch these battles
in real time.
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The scale of galaxies is huge.
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They're hundreds of thousands of
light years across.
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It's going to take them millions or
billions of years to come together.
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So it's like looking at one frame
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from a really energetic fight scene
in a movie.
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By piecing these snapshots together,
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00:08:02,320 --> 00:08:05,720
astronomers can build up
a detailed picture
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of past conflicts,
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and discover how these battles
transformed galaxies
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over billions of years.
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We have pictures of
isolated galaxies,
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we have pictures of
interacting galaxies,
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and we have pictures of
aftermath galaxies.
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And that's helped us discover
something alarming.
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The Milky Way faces
yet another attack.
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From an enemy armed with
an enormous secret weapon.
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Will our solar system
survive the onslaught?
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Across the universe,
galaxies are at war.
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Their main weapon?
Gravity.
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It tears the combatants
into weird and wonderful shapes.
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Our galaxy didn't escape the mayhem.
It's peppered with battle scars.
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The overall shape of the Milky Way
is a flat disc of stars and gas.
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Except recently we have found out
that at the edges,
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it's actually warped a little bit
like the brim of a fedora.
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The stars actually dip down
below the plane on one side,
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and dip above it on the other.
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We think the attacker
was one of our satellites.
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A galaxy that orbits the Milky Way
like the moon orbits the Earth.
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It's called
the Sagittarius Dwarf Galaxy.
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From looking at how the stars move
in the Milky Way,
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we suspect that
the Sagittarius Dwarf Galaxy
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has actually crashed through
the Milky Way a few times
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on its course of its orbit
around the galaxy.
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It came in
about six billion years ago,
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hit the disc hard
about two billion years ago,
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and crashed again
about a billion years ago.
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And our gravity has pulled it out
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into a gigantic looping
stream of stars
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that is moving in and out of
our Milky Way.
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The war is not over.
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The insurgent galaxy will return.
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When galaxies interact,
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often they're caught in
this huge cosmic dance
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where they revolve around each other
a few times,
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or they even crash through
each other
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and then come back around.
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The Sagittarius Dwarf Galaxy
looks like it's crashing in
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with ever-increasing frequency.
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A new skirmish could take place
in the next 100 million years.
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So, should we be worried
about these attacks?
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Because the Sagittarius Dwarf Galaxy
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is so small
compared to the Milky Way,
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it will do some damage
at the beginning.
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But because we're so massive,
we can absorb the impact.
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I mean, this galaxy,
it's looking for a fight,
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but it's also 10,000 times
smaller than us,
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so this is gonna be no sweat at all.
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So far, the Milky Way
has been victorious.
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But the danger isn't over.
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We are surrounded by enemies.
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Our local neighbourhood of galaxies
has three major galaxies,
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but up to 50 smaller ones.
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All these galaxies
are potential troublemakers.
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Each one of these could be armies
that rise up against us.
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The two most famous galaxies
that orbit the Milky Way
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are the Large and Small
Magellanic Clouds.
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These are two independent
dwarf galaxies
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that you can see in the night sky
from the southern hemisphere.
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We thought
the Large Magellanic Cloud
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orbited our galaxy
at a safe distance
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00:11:51,520 --> 00:11:54,320
of 160,000 light years.
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00:11:55,400 --> 00:11:59,120
We thought it would stay that way
and we thought it was harmless.
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00:12:00,200 --> 00:12:05,000
Now a new discovery shows
we were wrong on all counts.
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00:12:06,400 --> 00:12:10,360
The new factor that changed our view
of the Magellanic Cloud
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is we found out it has
a lot more dark matter
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than we thought.
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Dark matter.
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00:12:17,720 --> 00:12:21,280
The most mysterious stuff
in the universe.
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Dark matter is literally
what it sounds like.
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It's matter that we cannot see.
209
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But it has gravity
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and can affect objects
that we can see.
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00:12:33,440 --> 00:12:38,320
Adding in this extra dark matter
makes the Large Magellanic Cloud
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at least twice as massive
as predicted,
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00:12:41,560 --> 00:12:45,200
so its gravity is double
what we thought.
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00:12:46,800 --> 00:12:49,720
And it's secretly been gathering
allies,
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has been gathering dark matter
on its side,
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and now it's a much bigger threat
than we thought before.
217
00:12:58,280 --> 00:13:00,120
So it's not just going to orbit us,
218
00:13:00,200 --> 00:13:02,160
it's gonna collide with
the Milky Way.
219
00:13:03,480 --> 00:13:06,560
Moving at nearly
a million miles an hour,
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00:13:06,640 --> 00:13:11,120
the Large Magellanic Cloud
will not swing past us,
221
00:13:11,200 --> 00:13:12,360
it will attack.
222
00:13:13,560 --> 00:13:15,400
The Large Magellanic Cloud
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00:13:15,480 --> 00:13:19,280
is one tenth the mass of
the Milky Way.
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00:13:19,360 --> 00:13:22,080
That's enough to make
a pretty big punch.
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00:13:24,000 --> 00:13:26,480
In about two-and-a-half billion
years,
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it will smash into our galaxy.
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00:13:32,000 --> 00:13:35,320
It's gonna plough through the disc
of the Milky Way.
228
00:13:35,400 --> 00:13:36,880
It's gonna blow a cavity.
229
00:13:36,960 --> 00:13:39,960
It might even damage
our spiral arms.
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Earth sits in one of
those spiral arms.
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Could our planet become
collateral damage?
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If the Large Magellanic Cloud
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00:13:53,440 --> 00:13:55,600
passes through
the plane of our galaxy
234
00:13:55,680 --> 00:13:59,680
near our location,
that could have dire consequences.
235
00:14:01,000 --> 00:14:03,960
The gravitational clash
between the invader
236
00:14:04,040 --> 00:14:05,280
and the Milky Way
237
00:14:05,360 --> 00:14:08,560
could hurl stars and planets
out of our galaxy.
238
00:14:10,000 --> 00:14:12,480
Earth could be one of them.
239
00:14:13,640 --> 00:14:16,640
Our planet's very close to
its own star,
240
00:14:16,720 --> 00:14:21,200
so the odds are that you'll just get
ripped out along with your star,
241
00:14:21,280 --> 00:14:23,200
so we'd be moving along
with the sun
242
00:14:23,280 --> 00:14:26,840
even as the sun gets jettisoned
from our galaxy.
243
00:14:26,920 --> 00:14:29,920
And it'll move off
out into intergalactic space.
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00:14:30,000 --> 00:14:33,120
And that's not terrible, I mean,
it's not gonna get destroyed,
245
00:14:33,200 --> 00:14:34,800
but it's a little lonely.
246
00:14:37,880 --> 00:14:41,960
Our view of the night sky
would radically change.
247
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We'd be able to see
much more of the Milky Way,
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00:14:46,560 --> 00:14:50,120
especially if we got kicked up
above the plane of the galaxy.
249
00:14:50,200 --> 00:14:52,680
We'd be able to see
the whole shebang.
250
00:14:52,760 --> 00:14:56,640
Just look at any image of
a spiral galaxy,
251
00:14:56,720 --> 00:14:57,880
they're gorgeous.
252
00:14:57,960 --> 00:15:00,200
Now, imagine seeing your night sky
253
00:15:00,280 --> 00:15:03,080
filled with
the face-on spiral galaxy.
254
00:15:04,200 --> 00:15:07,440
That would be like waking up
to my face every morning.
255
00:15:07,520 --> 00:15:08,760
Spectacular.
256
00:15:09,880 --> 00:15:11,440
(LAUGHS)
257
00:15:14,000 --> 00:15:16,160
If we were unlucky,
258
00:15:16,240 --> 00:15:18,720
our home planet could have
a close encounter
259
00:15:18,800 --> 00:15:20,440
with an invading star.
260
00:15:21,520 --> 00:15:23,680
The odds are very low
261
00:15:23,760 --> 00:15:26,840
that another star
will pass close by the sun.
262
00:15:26,920 --> 00:15:28,720
But those odds aren't zero.
263
00:15:28,800 --> 00:15:31,520
It could happen that another star
passes close enough
264
00:15:31,600 --> 00:15:32,840
to affect the planets.
265
00:15:32,920 --> 00:15:34,480
And if that were to happen,
266
00:15:34,560 --> 00:15:39,280
it could upset the delicate balance
in the solar system.
267
00:15:40,320 --> 00:15:42,640
We don't know where the Earth
could end up.
268
00:15:43,880 --> 00:15:47,080
It might find its way into the sun.
You just don't know.
269
00:15:47,160 --> 00:15:49,400
Or there might just be
a rain of comets
270
00:15:49,480 --> 00:15:51,280
into our inner solar system.
271
00:15:51,360 --> 00:15:53,920
Our own planet might be flung out,
272
00:15:54,000 --> 00:15:58,400
in which case this would be
a death knell for all life on Earth.
273
00:15:58,480 --> 00:16:01,280
I'm not someone who's like
a doom and gloom person,
274
00:16:01,360 --> 00:16:03,000
but, like, that would be insane.
275
00:16:04,400 --> 00:16:09,400
You don't know what's gonna happen,
but most of the options are bad.
276
00:16:10,480 --> 00:16:14,280
All these nightmare scenarios
will extinguish life.
277
00:16:18,000 --> 00:16:20,080
Earth might survive,
278
00:16:20,160 --> 00:16:23,720
but our cosmic zipcode
will take a severe beating.
279
00:16:25,040 --> 00:16:28,600
The Milky Way galaxy is bigger than
the Large Magellanic Cloud,
280
00:16:28,680 --> 00:16:31,000
so we are gonna win,
281
00:16:31,080 --> 00:16:33,480
but it's gonna hurt us
for a long time.
282
00:16:34,880 --> 00:16:38,600
The Large Magellanic Cloud
will leave our galaxy battered,
283
00:16:38,680 --> 00:16:41,680
bruised,
but ultimately undefeated.
284
00:16:42,720 --> 00:16:47,680
But there's a far bigger threat
looming over the Milky Way.
285
00:16:47,760 --> 00:16:50,960
It's gonna face an opponent
that it can't defeat.
286
00:16:52,000 --> 00:16:56,560
Will this mega-collision
be the Milky Way's last stand?
287
00:16:59,600 --> 00:17:03,480
In the not-too-distant future,
galactically speaking,
288
00:17:03,560 --> 00:17:07,560
a much, much larger battle
is due for the Milky Way.
289
00:17:09,000 --> 00:17:14,080
A battle with a local superpower,
the Andromeda Galaxy.
290
00:17:15,480 --> 00:17:19,360
We thought this huge galaxy
might wound us in the future.
291
00:17:20,680 --> 00:17:23,160
Now recent evidence reveals
292
00:17:23,240 --> 00:17:26,400
it's going to make
a full-scale assault.
293
00:17:27,720 --> 00:17:29,200
We've known for a long time
294
00:17:29,280 --> 00:17:32,880
that Andromeda is heading
more or less toward us,
295
00:17:32,960 --> 00:17:35,440
but we didn't know exactly
in what direction.
296
00:17:35,520 --> 00:17:39,240
But in recent years, we've been able
to pinpoint this a lot better,
297
00:17:39,320 --> 00:17:43,160
and, uh, yeah, it's heading
right for us.
298
00:17:45,400 --> 00:17:47,400
Data from the Hubble Space Telescope
299
00:17:47,480 --> 00:17:52,880
shows the two galaxies will collide
in about four billion years.
300
00:17:55,120 --> 00:17:58,520
And it will be a monumental battle.
301
00:17:59,560 --> 00:18:02,680
This collision that is coming,
and it is coming,
302
00:18:02,760 --> 00:18:05,920
is not gonna be anything like
the Milky Way has experienced before
303
00:18:06,000 --> 00:18:08,000
in its 10 or 12-billion-year
history.
304
00:18:08,080 --> 00:18:10,880
This is galaxy of comparable size.
305
00:18:10,960 --> 00:18:14,520
This is two heavyweight
prizefighters coming at it.
306
00:18:14,600 --> 00:18:19,240
Warriors with the same
gravitational firepower.
307
00:18:19,320 --> 00:18:23,280
Simulations suggest
a clash of the titans.
308
00:18:23,360 --> 00:18:26,000
Each of them
with half a trillion stars in them.
309
00:18:26,080 --> 00:18:28,600
Well, that sounds like
a pretty spectacular collision.
310
00:18:30,240 --> 00:18:34,400
Fights between
equally-matched galaxies are rare
311
00:18:34,480 --> 00:18:35,480
and messy.
312
00:18:36,720 --> 00:18:38,200
When the battle kicks off,
313
00:18:38,280 --> 00:18:41,360
there will be no good news
for either side.
314
00:18:43,240 --> 00:18:46,040
When the Andromeda Galaxy
and the Milky Way galaxy
315
00:18:46,120 --> 00:18:47,440
start to get close,
316
00:18:47,520 --> 00:18:50,080
they're gonna start
affecting each other profoundly.
317
00:18:50,160 --> 00:18:52,480
Tendrils of stars
are gonna be thrown out.
318
00:18:52,560 --> 00:18:54,800
Gas is gonna be thrown out.
319
00:18:56,320 --> 00:18:59,000
It won't be a single impact.
320
00:19:00,040 --> 00:19:05,120
Gravity will send the two opponents
into a spiralling dance of death.
321
00:19:06,800 --> 00:19:09,400
The first pass is actually
not a direct hit.
322
00:19:09,480 --> 00:19:12,480
They're gonna swing past each other,
in fact.
323
00:19:12,560 --> 00:19:13,720
And at this point,
324
00:19:13,800 --> 00:19:16,440
their gravitational interaction
is gonna slow 'em down,
325
00:19:16,520 --> 00:19:18,680
and they're gonna come back
toward each other.
326
00:19:18,760 --> 00:19:22,320
The galaxies will collide
and fly apart again,
327
00:19:22,400 --> 00:19:25,960
inflicting more and more damage
with each clash.
328
00:19:27,160 --> 00:19:29,240
If you were to go outside
and look up,
329
00:19:29,320 --> 00:19:32,640
you could see the disc of our galaxy
getting ripped apart
330
00:19:32,720 --> 00:19:35,120
by tidal interactions
with Andromeda.
331
00:19:38,320 --> 00:19:43,720
The two beautiful spiral galaxies
will tear each other apart,
332
00:19:45,000 --> 00:19:48,880
leaving one vast, elliptical galaxy.
333
00:19:50,720 --> 00:19:54,720
The fate of
- the Andromeda/
- Milky Way battle
334
00:19:54,800 --> 00:19:57,200
is that they will merge.
335
00:19:57,280 --> 00:20:01,080
This is going to be
one gigantic galaxy.
336
00:20:03,840 --> 00:20:05,240
And that presents a problem.
337
00:20:05,320 --> 00:20:07,120
What are we gonna call
this new galaxy?
338
00:20:07,200 --> 00:20:10,640
Of course, my nerd colleagues
have come up with names
339
00:20:10,720 --> 00:20:13,520
like Milkomeda, Andromoway,
whatever.
340
00:20:13,600 --> 00:20:14,960
Those are corny.
341
00:20:15,040 --> 00:20:17,600
We should just call it Hakeem.
342
00:20:23,240 --> 00:20:25,200
With a trillion stars,
343
00:20:25,280 --> 00:20:29,160
it will be one of the biggest
galaxies in the universe.
344
00:20:31,320 --> 00:20:34,880
In the Hakeem galaxy,
things gonna be completely new.
345
00:20:34,960 --> 00:20:38,120
First off, it's gonna be
a really good-looking galaxy,
346
00:20:38,200 --> 00:20:40,200
let's get that straight
from the get-go.
347
00:20:40,280 --> 00:20:42,840
Second, it's gonna be powerful.
348
00:20:42,920 --> 00:20:44,960
And I'm talking powerful.
349
00:20:45,040 --> 00:20:47,440
This may be
the most remarkable galaxy
350
00:20:47,520 --> 00:20:49,240
in the history of the universe.
351
00:20:51,560 --> 00:20:55,520
Milkomeda,
or Hakeem if you prefer,
352
00:20:55,600 --> 00:20:59,040
will become the undisputed boss of
our cosmic neighbourhood.
353
00:21:00,400 --> 00:21:04,480
Its calm appearance concealing
a history of violence.
354
00:21:07,000 --> 00:21:09,960
It's the result of
a complete war zone of mergers
355
00:21:10,040 --> 00:21:11,840
over the course of
billions of years.
356
00:21:11,920 --> 00:21:15,720
Many galaxies crashing together,
fully reconfiguring each time.
357
00:21:15,800 --> 00:21:20,520
And slowly you grow this smooth,
placid, big blob of stars.
358
00:21:23,000 --> 00:21:29,000
After billions of years of warfare,
our galaxy will finally be peaceful.
359
00:21:30,920 --> 00:21:34,160
But before its honourable discharge,
360
00:21:34,240 --> 00:21:39,480
Milkomeda may produce
one final devastating act of war.
361
00:21:40,640 --> 00:21:43,120
Imagine World War Two,
362
00:21:43,200 --> 00:21:44,440
and then all of a sudden
363
00:21:44,520 --> 00:21:47,400
one of the sides comes up with
the Death Star.
364
00:21:47,480 --> 00:21:49,560
That's what we're talking about
here.
365
00:21:51,480 --> 00:21:54,280
A weapon of cosmic destruction.
366
00:22:06,560 --> 00:22:08,600
When giant galaxies clash,
367
00:22:08,680 --> 00:22:11,920
the battles are spectacular
and destructive.
368
00:22:15,320 --> 00:22:18,400
The victors steal
huge numbers of stars
369
00:22:18,480 --> 00:22:20,120
and vast amounts of gas
370
00:22:20,200 --> 00:22:24,200
as fuel for
the ultimate super weapon.
371
00:22:26,400 --> 00:22:29,800
This special weapon
that these monster galaxies have
372
00:22:29,880 --> 00:22:32,280
is a giant death ray,
373
00:22:32,360 --> 00:22:37,160
a jet of material racing across
thousands of light years.
374
00:22:39,480 --> 00:22:41,800
These huge outbursts of energy
375
00:22:41,880 --> 00:22:45,440
blast out of the centre of
the colliding galaxies.
376
00:22:45,520 --> 00:22:48,520
They produce more energy
in one second
377
00:22:48,600 --> 00:22:53,120
than the sun will in its entire
ten-billion-year lifetime.
378
00:22:54,160 --> 00:22:56,320
We call them jets.
379
00:22:57,880 --> 00:23:01,960
These incredibly powerful jets
aren't just brief features.
380
00:23:02,040 --> 00:23:05,280
They can be sustained
for millions of years.
381
00:23:05,360 --> 00:23:07,480
And they can maintain
their structure
382
00:23:07,560 --> 00:23:09,360
for thousands of light years.
383
00:23:10,560 --> 00:23:13,440
It's like turning on a garden hose
in Chicago
384
00:23:13,520 --> 00:23:16,640
and using it to water a garden
in London.
385
00:23:18,240 --> 00:23:21,240
Exactly what triggered these jets
was a mystery.
386
00:23:21,320 --> 00:23:23,960
Then, in June 2018,
387
00:23:24,040 --> 00:23:27,880
astronomers in Hawaii
captured something stunning,
388
00:23:27,960 --> 00:23:31,840
a jet forming
during a galactic collision.
389
00:23:34,000 --> 00:23:36,520
The team found something
really incredible.
390
00:23:36,600 --> 00:23:39,920
They found two galaxies
that were in a cosmic collision,
391
00:23:40,000 --> 00:23:43,200
and actually found an active jet
in one of these galaxies.
392
00:23:43,280 --> 00:23:46,440
It was the first time anything
like this has been discovered.
393
00:23:48,640 --> 00:23:50,280
When galaxies collide,
394
00:23:50,360 --> 00:23:54,160
the clash drives huge clouds of gas
and dust
395
00:23:54,240 --> 00:23:56,240
towards their centres.
396
00:23:56,320 --> 00:24:00,560
The supermassive black holes
start to feed.
397
00:24:02,080 --> 00:24:04,080
The gas that was in those galaxies
398
00:24:04,160 --> 00:24:06,040
starts to funnel toward
the black hole
399
00:24:06,120 --> 00:24:07,600
and will fall upon it.
400
00:24:08,640 --> 00:24:12,960
Not all this gas ends up inside
the supermassive black hole,
401
00:24:13,040 --> 00:24:16,200
powerful magnetic fields
carry some of this matter
402
00:24:16,280 --> 00:24:17,280
to the poles,
403
00:24:18,400 --> 00:24:21,800
and blast it out
in tight, narrow jets.
404
00:24:21,880 --> 00:24:23,680
A super weapon is born.
405
00:24:24,720 --> 00:24:29,640
This discovery helps us understand
how giant elliptical galaxies form.
406
00:24:30,800 --> 00:24:35,000
Knowing that mergers of
spiral galaxies can cause these jets
407
00:24:35,080 --> 00:24:37,280
helps us put together
a complete picture
408
00:24:37,360 --> 00:24:40,360
of how these huge
elliptical galaxies might be formed.
409
00:24:43,160 --> 00:24:46,880
The discovery doesn't answer
all our questions.
410
00:24:46,960 --> 00:24:48,400
There's another mystery.
411
00:24:48,480 --> 00:24:53,560
How did the super giant galaxies
that dwarf the Milky Way get so big?
412
00:24:54,600 --> 00:25:00,120
Our Milky Way galaxy is big-ish.
It's slightly bigger than average.
413
00:25:00,200 --> 00:25:02,760
But IC 1101, for example,
414
00:25:02,840 --> 00:25:06,000
is more than 50 times larger than
our home galaxy,
415
00:25:06,080 --> 00:25:09,160
and has more than a trillion,
with a T,
416
00:25:09,240 --> 00:25:11,240
a trillion stars in it.
417
00:25:11,320 --> 00:25:15,120
The biggest galaxies
make the Milky Way look like an ant.
418
00:25:16,160 --> 00:25:19,800
These galactic giants
pose a problem.
419
00:25:19,880 --> 00:25:23,280
There hasn't been enough time
since the birth of the universe
420
00:25:23,360 --> 00:25:25,800
for them to become so large.
421
00:25:26,840 --> 00:25:29,960
Even by conquering smaller galaxies.
422
00:25:30,040 --> 00:25:32,040
When we look into
the distant universe,
423
00:25:32,120 --> 00:25:35,520
we see something very strange
that we don't quite understand.
424
00:25:35,600 --> 00:25:37,480
We see enormous galaxies
425
00:25:37,560 --> 00:25:40,440
that existed just a billion years
after the Big Bang.
426
00:25:40,520 --> 00:25:42,600
And even though
these cosmic collisions
427
00:25:42,680 --> 00:25:44,920
help explain
how galaxies get bigger,
428
00:25:45,000 --> 00:25:48,800
they don't quite explain everything
about how galaxies grow over time.
429
00:25:48,880 --> 00:25:51,160
So we still have a big mystery
on our hands here.
430
00:25:54,880 --> 00:25:57,200
So, in 2019,
431
00:25:57,280 --> 00:26:01,160
an international team investigated
a very large galaxy
432
00:26:01,240 --> 00:26:03,640
over 300 million light years away.
433
00:26:03,720 --> 00:26:07,880
We call it NGC 6240.
434
00:26:09,000 --> 00:26:11,800
NGC 6240 was being steadied
435
00:26:11,880 --> 00:26:14,440
because it had two supermassive
black holes in it.
436
00:26:14,520 --> 00:26:17,800
Now, the galaxy itself
looked like it had been disturbed,
437
00:26:17,880 --> 00:26:19,280
like something had happened,
438
00:26:19,360 --> 00:26:22,840
so they thought that potentially
it had had a recent merger.
439
00:26:28,080 --> 00:26:32,080
They were expecting to see
two supermassive black holes
440
00:26:32,160 --> 00:26:33,960
in the galaxy's heart.
441
00:26:34,040 --> 00:26:38,200
As the researchers peered through
the layers of gas and dust,
442
00:26:38,280 --> 00:26:41,160
they discovered something
surprising.
443
00:26:41,240 --> 00:26:43,640
What we found was staggering.
444
00:26:43,720 --> 00:26:47,720
We found not two, but three
supermassive black holes
445
00:26:47,800 --> 00:26:49,280
lurking in the centre.
446
00:26:55,240 --> 00:26:57,600
It's the first time
we've found a galaxy
447
00:26:57,680 --> 00:27:00,240
with three supermassive black holes.
448
00:27:01,280 --> 00:27:04,280
Evidence of a three galaxy pile up.
449
00:27:05,520 --> 00:27:10,240
This galaxy is an active battlefield
of not two,
450
00:27:10,320 --> 00:27:14,560
but three armies colliding at once.
451
00:27:14,640 --> 00:27:16,800
And because there are three armies
involved,
452
00:27:16,880 --> 00:27:20,760
there are three galaxies involved
with three times as much mass,
453
00:27:20,840 --> 00:27:24,160
three times as many stars,
three times as much material,
454
00:27:24,240 --> 00:27:26,400
and three times as much violence.
455
00:27:27,440 --> 00:27:31,840
This three-way battle may explain
how the largest galaxies
456
00:27:31,920 --> 00:27:34,080
got so big so fast.
457
00:27:35,120 --> 00:27:38,080
It could be that galaxy mergers
are more frequent
458
00:27:38,160 --> 00:27:39,880
than what we thought previously.
459
00:27:39,960 --> 00:27:43,600
And therefore,
galaxies become more massive
460
00:27:43,680 --> 00:27:45,400
faster than previously expected.
461
00:27:47,480 --> 00:27:48,560
In the past,
462
00:27:48,640 --> 00:27:52,640
galaxies may have battled
and collided more often than today.
463
00:27:52,720 --> 00:27:57,280
Back then, galaxies were
more densely packed together.
464
00:27:58,560 --> 00:28:01,440
Our universe is expanding
as it ages,
465
00:28:01,520 --> 00:28:05,000
which means in the past
all the galaxies in the universe
466
00:28:05,080 --> 00:28:06,920
were closer together.
467
00:28:07,000 --> 00:28:08,720
That means they've had
greater chance
468
00:28:08,800 --> 00:28:10,560
for their gravitational interactions
469
00:28:10,640 --> 00:28:12,960
to pull them together
and smash them together.
470
00:28:15,960 --> 00:28:18,960
When galaxies fight,
the big get bigger.
471
00:28:20,000 --> 00:28:24,160
More mass means more gravity.
The vital ingredient for victory.
472
00:28:26,400 --> 00:28:30,320
But galactic conflict
doesn't always result in growth.
473
00:28:31,360 --> 00:28:36,000
A strange new astronomical object
had scientists confused.
474
00:28:38,640 --> 00:28:41,640
They just look like stars
from the ground.
475
00:28:41,720 --> 00:28:43,880
However, with the advent of Hubble
476
00:28:43,960 --> 00:28:46,600
and beautiful
space-based telescopes,
477
00:28:46,680 --> 00:28:50,160
it was possible to look at
these "stars" again
478
00:28:50,240 --> 00:28:52,560
and actually discover that
they were galaxies.
479
00:28:58,000 --> 00:29:02,640
They're kind of crazy.
They're a huge number of stars,
480
00:29:02,720 --> 00:29:05,360
but crammed into
an incredibly tiny space
481
00:29:05,440 --> 00:29:06,760
on an astrophysical scale,
482
00:29:06,840 --> 00:29:10,320
something 500 times smaller than
our Milky Way galaxy.
483
00:29:11,560 --> 00:29:15,200
We call them
ultra-compact dwarf galaxies,
484
00:29:15,280 --> 00:29:16,520
or UCDs.
485
00:29:17,800 --> 00:29:20,760
You might imagine
the difference between
486
00:29:20,840 --> 00:29:23,720
the Milky Way galaxy and a UCD
487
00:29:23,800 --> 00:29:27,960
as the difference between a cloud
and a rock,
488
00:29:28,040 --> 00:29:31,520
where the rock is just
the same kind of material,
489
00:29:31,600 --> 00:29:34,000
but compressed to just
incredibly high densities
490
00:29:34,080 --> 00:29:36,320
compared to some fluffy,
gaseous thing.
491
00:29:39,400 --> 00:29:43,960
What are these strange galaxies?
They seem to break all the rules.
492
00:29:45,000 --> 00:29:47,480
To find out, astronomers zoomed in
493
00:29:47,560 --> 00:29:51,640
to a particularly dense
ultra-compact dwarf galaxy
494
00:29:51,720 --> 00:29:55,440
called M60-UCD1.
495
00:29:56,720 --> 00:30:00,520
M60-UCD1 is 300 light years across.
496
00:30:00,600 --> 00:30:04,080
It's tiny. It's a pinpoint
compared to our enormous galaxy.
497
00:30:04,160 --> 00:30:08,040
Our galaxy has 200 or more
billion stars in it.
498
00:30:08,120 --> 00:30:11,000
M60-UCD1 only has 140 million,
499
00:30:11,080 --> 00:30:14,880
but they're packed into
this incredibly tight volume.
500
00:30:14,960 --> 00:30:17,440
The night sky inside the galaxy
501
00:30:17,520 --> 00:30:19,760
would look very different
from our own.
502
00:30:20,840 --> 00:30:22,800
On Earth,
when you look at the night sky,
503
00:30:22,880 --> 00:30:24,880
you see a few thousand stars.
504
00:30:24,960 --> 00:30:27,440
But if you were in M60-UCD1,
505
00:30:27,520 --> 00:30:29,920
you wouldn't just see
a few thousand stars,
506
00:30:30,000 --> 00:30:34,160
you would see hundreds of thousands
of stars in the night sky.
507
00:30:34,240 --> 00:30:35,880
That would be amazing.
508
00:30:41,920 --> 00:30:46,320
As the astronomers looked deeper
into the heart of this tiny galaxy,
509
00:30:47,560 --> 00:30:50,040
things got even weirder.
510
00:30:50,120 --> 00:30:54,560
They found a supermassive black hole
much bigger than expected.
511
00:30:56,800 --> 00:31:00,600
It actually has a black hole
that's bigger, five times bigger,
512
00:31:00,680 --> 00:31:03,840
than the black hole at the centre of
our Milky Way galaxy.
513
00:31:03,920 --> 00:31:07,400
When we see supermassive
black holes inside of galaxies,
514
00:31:07,480 --> 00:31:10,880
they tend to scale with the size of
the galaxy itself.
515
00:31:10,960 --> 00:31:14,640
A bigger galaxy has a bigger
supermassive black hole.
516
00:31:14,720 --> 00:31:16,880
Why does such a tiny little object
517
00:31:16,960 --> 00:31:19,880
have such an oversized
central black hole?
518
00:31:19,960 --> 00:31:22,520
The only possible explanation?
519
00:31:22,600 --> 00:31:26,400
This tiny galaxy was once
much larger.
520
00:31:27,440 --> 00:31:29,880
These galaxies might have begun
their lives
521
00:31:29,960 --> 00:31:32,360
as, in fact, much bigger galaxies.
522
00:31:32,440 --> 00:31:36,240
And that what we see today is really
just the very central densest part
523
00:31:36,320 --> 00:31:37,960
of a much larger galaxy.
524
00:31:39,560 --> 00:31:42,880
Based on the size of
its supermassive black hole,
525
00:31:42,960 --> 00:31:49,600
M60-UCD1 may once have contained
many billions of stars.
526
00:31:49,680 --> 00:31:52,320
Something captured them,
527
00:31:52,400 --> 00:31:55,720
and we don't have to look far
to find the aggressor.
528
00:31:55,800 --> 00:31:57,440
A nearby super galaxy
529
00:31:57,520 --> 00:32:01,680
with lots of gravitational
firepower, M60.
530
00:32:02,800 --> 00:32:06,120
M60's a monster.
It has a trillion stars in it.
531
00:32:06,200 --> 00:32:09,000
It's bigger than the Milky Way
and we're pretty big.
532
00:32:09,080 --> 00:32:12,400
The battle was not
a full-on frontal assault.
533
00:32:12,480 --> 00:32:17,960
M60 raided its smaller opponent,
capturing its troops.
534
00:32:18,040 --> 00:32:21,520
This is more of a stealthy,
guerrilla hit and run,
535
00:32:21,600 --> 00:32:24,400
where we're gonna move in,
pick off some of your troops
536
00:32:24,480 --> 00:32:27,200
and then get out
before you even notice.
537
00:32:28,320 --> 00:32:32,640
All that's left from one of
these drive-by galaxy interactions
538
00:32:32,720 --> 00:32:35,040
is this supermassive black hole
539
00:32:35,120 --> 00:32:37,400
with a fraction of
its original stars.
540
00:32:38,560 --> 00:32:42,560
The conflict devastated M60-UCD1.
541
00:32:42,640 --> 00:32:46,640
Over 98% of its stellar army
were captured
542
00:32:46,720 --> 00:32:48,840
and became prisoners of war.
543
00:32:48,920 --> 00:32:52,480
It used to be a big galaxy,
544
00:32:52,560 --> 00:32:57,320
but it suffered one too many defeats
and now it's a fallen empire.
545
00:32:58,360 --> 00:33:02,440
We can frame this battle
between M60 and M60-UCD1
546
00:33:02,520 --> 00:33:03,760
as just a battle,
547
00:33:03,840 --> 00:33:07,080
but, in fact, it's a slaughter,
it's a massacre.
548
00:33:08,120 --> 00:33:12,360
These small galaxies
get all their troops removed,
549
00:33:12,440 --> 00:33:13,920
but the HQ,
550
00:33:14,000 --> 00:33:16,000
the supermassive black hole,
remains,
551
00:33:16,080 --> 00:33:17,840
but it doesn't have any troops left.
552
00:33:19,000 --> 00:33:22,880
Eventually, M60 will conquer
its battered opponent,
553
00:33:22,960 --> 00:33:26,120
destroying what's left of
the compact galaxy.
554
00:33:27,200 --> 00:33:28,920
It'll get ripped apart
even further,
555
00:33:29,000 --> 00:33:31,000
and more and more stars
will be consumed
556
00:33:31,080 --> 00:33:32,280
by the bigger galaxy.
557
00:33:32,360 --> 00:33:37,080
So chances are this little dwarf is
eventually going to be pulled apart
558
00:33:37,160 --> 00:33:39,520
and become a part of M60.
559
00:33:42,080 --> 00:33:44,560
But while this little galaxy
is down,
560
00:33:44,640 --> 00:33:47,640
it is most certainly not yet out.
561
00:33:47,720 --> 00:33:49,960
It's likely to stage
a counterattack.
562
00:33:51,080 --> 00:33:56,960
Its final mission? A kamikaze charge
that will leave M60 reeling.
563
00:34:01,240 --> 00:34:04,400
It's absolutely chaotic.
564
00:34:04,480 --> 00:34:08,360
Stars are sent off flying
in every direction,
565
00:34:08,440 --> 00:34:11,440
and they're moving
at really high velocities.
566
00:34:12,560 --> 00:34:15,200
And when stars are stripped
out of galaxies,
567
00:34:15,280 --> 00:34:17,280
they become what we call
rogue stars.
568
00:34:19,880 --> 00:34:23,600
These ejected, runaway stars
will leave the galaxy
569
00:34:23,680 --> 00:34:25,400
at two million miles an hour.
570
00:34:27,720 --> 00:34:30,360
They'll hurtle through
the emptiness of space,
571
00:34:30,440 --> 00:34:32,440
never to be seen again.
572
00:34:35,720 --> 00:34:40,960
But even this dramatic assault
can't change the inevitable outcome.
573
00:34:41,040 --> 00:34:45,120
M60-UCD1 is doomed.
574
00:34:50,640 --> 00:34:52,960
In the great game of
galactic warfare,
575
00:34:53,040 --> 00:34:55,040
losing can be catastrophic.
576
00:34:55,120 --> 00:35:00,000
For weak and small galaxies,
resistance is futile.
577
00:35:01,480 --> 00:35:04,880
Pillaged for resources
by their more powerful opponents,
578
00:35:04,960 --> 00:35:07,680
they slowly become burnt-out wrecks.
579
00:35:10,000 --> 00:35:14,880
But some peaceful galaxies
face an equally terrible fate.
580
00:35:15,920 --> 00:35:17,320
They starve to death.
581
00:35:24,320 --> 00:35:29,200
Cosmic wars are vicious.
They destroy many galaxies.
582
00:35:30,240 --> 00:35:34,080
But violent conflicts
can also give galaxies new life.
583
00:35:35,640 --> 00:35:41,640
Case in point, galaxy NGC 4485.
584
00:35:41,720 --> 00:35:44,880
NGC 4485 has a nickname of
the Two-Face galaxy,
585
00:35:44,960 --> 00:35:46,280
like the Batman villain,
586
00:35:46,360 --> 00:35:48,840
because it has two different halves
of the galaxy
587
00:35:48,920 --> 00:35:50,600
doing completely different things.
588
00:35:50,680 --> 00:35:55,080
Half of the galaxy is sort of old
and calm and relatively quiescent,
589
00:35:55,160 --> 00:35:57,560
whereas half of it
appears to be undergoing
590
00:35:57,640 --> 00:36:00,880
a sort of fireworks display of
new star formation.
591
00:36:02,000 --> 00:36:06,640
Why are new stars only born
in one half of this galaxy?
592
00:36:08,080 --> 00:36:10,720
We found a clue
on the edge of a photo
593
00:36:10,800 --> 00:36:12,960
taken by the Hubble Space Telescope.
594
00:36:15,120 --> 00:36:18,680
It was evidence of an attack
by another galaxy.
595
00:36:18,760 --> 00:36:23,080
We think that another galaxy
passed through it just off centre
596
00:36:23,160 --> 00:36:25,960
in a way that strongly perturbed
the gas
597
00:36:26,040 --> 00:36:28,040
on one half of the galaxy.
598
00:36:30,000 --> 00:36:34,400
The Two-Face galaxy skirmish
gave it a gravitational jolt,
599
00:36:34,480 --> 00:36:37,120
forcing clouds of gas together.
600
00:36:38,240 --> 00:36:40,480
When we think of galaxies,
we think of stars,
601
00:36:40,560 --> 00:36:42,520
and of course
galaxies are made of stars,
602
00:36:42,600 --> 00:36:46,400
but of course gas is the stuff
that stars are made of.
603
00:36:48,320 --> 00:36:50,280
When two galaxies collide,
604
00:36:50,360 --> 00:36:54,520
the gravitational duel can trigger
a huge burst of star formation.
605
00:36:58,720 --> 00:37:01,200
You need something to give a galaxy
a push,
606
00:37:01,280 --> 00:37:03,760
and that's exactly
what a galaxy collision does.
607
00:37:03,840 --> 00:37:07,000
And when gas clouds collide,
they compress.
608
00:37:07,080 --> 00:37:09,880
And when they compress,
you get knots in them
609
00:37:09,960 --> 00:37:12,960
that can compress more
and form stars.
610
00:37:15,000 --> 00:37:18,000
So you can think of these collisions
as very violent events,
611
00:37:18,080 --> 00:37:21,080
but ultimately it can breathe
new life into a galaxy.
612
00:37:22,120 --> 00:37:25,520
But the spoils of war
don't last long.
613
00:37:25,600 --> 00:37:30,000
In the short term, the victor galaxy
can come out glorious
614
00:37:30,080 --> 00:37:32,640
with so many new stars.
615
00:37:32,720 --> 00:37:36,760
But this celebration is short lived
because that round of star formation
616
00:37:36,840 --> 00:37:40,560
quickly uses up
the material available.
617
00:37:40,640 --> 00:37:45,480
If a galaxy wants to stay alive,
it has to feed on other galaxies.
618
00:37:49,560 --> 00:37:52,480
But what happens when opponents
are closely matched
619
00:37:52,560 --> 00:37:54,200
in gravitational firepower?
620
00:37:56,960 --> 00:38:02,920
When two equal mass galaxies meet,
when two armies of equal size meet,
621
00:38:03,000 --> 00:38:07,800
they can exhaust all their fuel,
they can kill all their troops,
622
00:38:07,880 --> 00:38:10,680
so at the end of it
there's nobody left to fight.
623
00:38:10,760 --> 00:38:14,240
The galaxies themselves
can be stripped of gas and dust,
624
00:38:14,320 --> 00:38:17,800
all the things you need to actually
make star formation happen.
625
00:38:21,880 --> 00:38:23,840
Once the gas is used up,
626
00:38:23,920 --> 00:38:26,240
the galaxy can't create
any new stars.
627
00:38:27,320 --> 00:38:31,320
It can only get more gas
by looting other galaxies.
628
00:38:32,400 --> 00:38:36,400
We can sometimes see a gas stream
coming from one galaxy
629
00:38:36,480 --> 00:38:37,880
and joining to the other,
630
00:38:37,960 --> 00:38:40,360
and then the gas from that galaxy
is now free
631
00:38:40,440 --> 00:38:42,600
and it starts to make stars again.
632
00:38:44,000 --> 00:38:46,880
You're bringing in new ingredients
to form stars,
633
00:38:46,960 --> 00:38:50,440
new gas, new dust to become part of
this larger galaxy.
634
00:38:50,520 --> 00:38:54,360
All sorts of weird and wonderful
things can happen in galaxy mergers.
635
00:38:58,320 --> 00:38:59,560
A star is born
636
00:38:59,640 --> 00:39:02,960
when a huge cloud of gas
collapses under gravity,
637
00:39:03,040 --> 00:39:05,040
triggering nuclear fusion.
638
00:39:06,080 --> 00:39:08,640
The star ignites
and begins to shine.
639
00:39:09,800 --> 00:39:11,040
It's a glorious sight
640
00:39:11,120 --> 00:39:15,200
and often a sign
that the war is finally ending.
641
00:39:17,240 --> 00:39:20,040
When two galaxies come together,
boom,
642
00:39:20,120 --> 00:39:22,840
all of a sudden, stars light up
all over the place.
643
00:39:23,880 --> 00:39:27,160
In this moment, as you catch
this system getting excited,
644
00:39:27,240 --> 00:39:28,960
the star formation rate's ramping up
645
00:39:29,040 --> 00:39:31,040
and it's sort of
a cosmic fireworks display,
646
00:39:31,120 --> 00:39:34,280
as if they're celebrating
the end of this hostile encounter
647
00:39:34,360 --> 00:39:36,160
with the other galaxy,
this war.
648
00:39:38,480 --> 00:39:41,720
But it's also a sign
that the victorious galaxy
649
00:39:41,800 --> 00:39:43,800
is using up its gas supply.
650
00:39:46,160 --> 00:39:50,320
So galaxies constantly need to raid
new targets
651
00:39:50,400 --> 00:39:53,200
and that raises
an important question.
652
00:39:53,280 --> 00:39:55,680
What happens if there's a galaxy
just alone in space,
653
00:39:55,760 --> 00:39:59,160
nothing else is colliding with it,
sort of a pacifist galaxy.
654
00:40:00,200 --> 00:40:03,440
The poster child
for these peace-loving galaxies
655
00:40:03,520 --> 00:40:06,400
is NGC 1277.
656
00:40:07,640 --> 00:40:11,440
NGC 1277 is a very peculiar galaxy.
657
00:40:11,520 --> 00:40:15,920
It's pretty big
and its stars are extremely old.
658
00:40:16,000 --> 00:40:20,200
It basically hasn't formed new stars
in the last ten billion years,
659
00:40:20,280 --> 00:40:23,280
so it's kind of the veterans home
of galaxies.
660
00:40:24,320 --> 00:40:27,880
NGC 1277 lives in a rough part of
the cosmos
661
00:40:27,960 --> 00:40:29,600
called the Perseus Cluster.
662
00:40:30,680 --> 00:40:35,000
Thousands of other galaxies
surround NGC 1277
663
00:40:35,080 --> 00:40:37,400
and they are all ready for a fight.
664
00:40:38,560 --> 00:40:41,720
So, you might ask why hasn't it had
encounters with other galaxies
665
00:40:41,800 --> 00:40:43,440
that might rejuvenate it?
666
00:40:44,480 --> 00:40:47,280
The answer, once again, is gravity.
667
00:40:48,480 --> 00:40:53,440
NGC 1277 sits inside
this massive galaxy cluster
668
00:40:53,520 --> 00:40:54,600
that has a ton of mass.
669
00:40:54,680 --> 00:40:56,160
And if you look at its position,
670
00:40:56,240 --> 00:40:58,280
it's fairly near the centre of
the cluster.
671
00:41:00,640 --> 00:41:03,600
The combined gravity of
thousands of galaxies
672
00:41:03,680 --> 00:41:06,400
pulls on NGC 1277,
673
00:41:06,480 --> 00:41:10,200
accelerating it
to two million miles an hour.
674
00:41:12,880 --> 00:41:16,040
And so it has spent
the last few billion years
675
00:41:16,120 --> 00:41:17,680
travelling faster and faster,
676
00:41:17,760 --> 00:41:20,400
until now it's almost at
its fastest pace.
677
00:41:22,640 --> 00:41:25,440
It's very hard for gravity
to catch it,
678
00:41:25,520 --> 00:41:26,920
or catch one of its neighbours,
679
00:41:27,000 --> 00:41:29,680
and bring them together
to merge with each other.
680
00:41:31,080 --> 00:41:37,480
NGC 1277 has no chance of grabbing
new gas to make new stars.
681
00:41:37,560 --> 00:41:38,800
It's dying.
682
00:41:38,880 --> 00:41:42,120
All it has left are old red stars.
683
00:41:43,320 --> 00:41:46,880
When it comes to galaxies,
red is dead.
684
00:41:46,960 --> 00:41:50,360
No new stars means no big stars,
no blue stars,
685
00:41:50,440 --> 00:41:52,920
just small, dim, red dwarfs.
686
00:41:57,400 --> 00:42:00,400
Galaxies that don't fight
just fade away.
687
00:42:01,560 --> 00:42:02,720
At that point,
688
00:42:02,800 --> 00:42:05,680
the history of the universe
becomes really kind of boring.
689
00:42:05,760 --> 00:42:08,080
All the stars
will simply start to die out.
690
00:42:08,160 --> 00:42:09,960
Eventually there will be
the last star
691
00:42:10,040 --> 00:42:11,280
formed in the Milky Way,
692
00:42:11,360 --> 00:42:13,760
with no new galaxy
bringing fresh material.
693
00:42:13,840 --> 00:42:17,400
Without galaxy collisions,
the universe dies.
694
00:42:24,000 --> 00:42:29,080
Galactic battles mix things up
and replenish gas supplies.
695
00:42:30,360 --> 00:42:33,000
And our own galaxy
has reaped the benefits.
696
00:42:34,240 --> 00:42:38,200
Our Milky Way galaxy
fought a massive battle,
697
00:42:38,280 --> 00:42:40,800
but that battle
may have been necessary
698
00:42:40,880 --> 00:42:45,040
to build solar systems
like the one we live in right now.
699
00:42:48,240 --> 00:42:51,400
Clashes with
the Sagittarius Dwarf Galaxy
700
00:42:51,480 --> 00:42:54,200
occurred at the same time
the sun formed.
701
00:42:56,160 --> 00:42:59,040
It's possible that we owe
our very existence
702
00:42:59,120 --> 00:43:01,920
to the collision with
the Sagittarius Dwarf Galaxy.
703
00:43:03,000 --> 00:43:04,160
Maybe the gas
704
00:43:04,240 --> 00:43:07,400
that ultimately gave rise to
the birth of our solar system
705
00:43:07,480 --> 00:43:10,000
once came from another galaxy
entirely.
706
00:43:12,400 --> 00:43:16,280
So, galactic wars are both creative
and destructive.
707
00:43:17,320 --> 00:43:20,960
Galaxies are built from collisions.
708
00:43:21,040 --> 00:43:24,440
Galaxies survive from collisions.
709
00:43:24,520 --> 00:43:27,840
And galaxies can also die
from collisions.
710
00:43:29,240 --> 00:43:30,880
Far from being destructive events,
711
00:43:30,960 --> 00:43:33,920
colliding galaxies may be the reason
that you and I are here.
712
00:43:36,760 --> 00:43:38,760
Intergalactic warfare
713
00:43:38,840 --> 00:43:44,080
has revolutionised our understanding
of how galaxies live and die.
714
00:43:45,120 --> 00:43:46,920
Ultimately,
it's these galaxy mergers
715
00:43:47,000 --> 00:43:48,800
that are one of the great engines
716
00:43:48,880 --> 00:43:51,200
of all structured growth
in the universe.
717
00:43:52,240 --> 00:43:55,040
These collisions got us
to where we are today,
718
00:43:55,120 --> 00:43:58,440
and they're gonna determine
the future of all the universe.
719
00:43:58,520 --> 00:44:00,520
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