The Universe's Secret Weapons and How They Affect Earth - How the Universe Works - Science Channel

Universe Unveiled
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Video Summary
AI GeneratedThe universe is a volatile environment filled with extreme phenomena. From the violent supernovae of massive stars like Betelgeuse and the predatory nature of \"vampire stars\" to the silent collapse of \"unnovas\" and the devastating potential of gamma-ray bursts, the cosmos contains numerous mechanisms capable of obliterating entire planetary systems and extinguishing all forms of life.
Say you've got a taste for adventure, a risk-taker extraordinaire used to laughing at danger and
death. Want to take on the worst the universe can throw at you? Better think twice. The cosmos
has it all. Havens for life and lethal hell holes. Our universe is both benevolent and violent.
There are little oasis pockets where things are very nice and calm and really good for
life like right around here. But there are definitely places and times where things get
violent and rough. But you don't have to venture to the wrong side of the tracks to encounter some
of the universe's scariest locations. Some are right in the neighborhood. Take Betelgeuse,
hidden amidst the beautiful Orion constellation.
A red star 640 light years away from Earth and ready to die. Now Betelgeuse is a huge red
supergiant star and it even looks kind of angry and red hanging up there in the sky. It's so big
that if you put it in our solar system it would expand all the way out to the planet Jupiter.
It's gigantic. When massive stars like Betelgeuse die they go out with an epic bang.
Now this star is just on the edge of going supernova and when it does we're in for quite a
show. Betelgeuse is running out of gas. The nuclear fire at its heart fights a constant battle against
the crushing gravity of its enormous mass. Once the gas is gone you better stand back.
No one can predict exactly when but soon the star will begin to collapse.
Imagine you're near the surface of this star just before it goes out, just before it goes supernova.
You're going to see the surface of that star just recede away from you incredibly rapidly.
Much like if you were at the beach and you saw the water just recede away from you really rapidly,
you know something bad is coming. The collapsing outer layers pummel the core making it denser and
denser. The core compresses as more of the star falls in. All that gas has to go somewhere and
so it bounces with an explosive force we can hardly imagine. When Betelgeuse goes supernova
we are talking about an epic catastrophe. An entire star is exploding. It's hard to describe
just how much energy that is. Imagine all the energy the sun puts out every second. Multiply
that times 31 million seconds in a year. Multiply that by 10 billion years in the sun's lifetime.
That is how much energy a supernova puts out. The energy unleashed is a shock wave of light,
heat and superheated gas racing out at thousands of miles a second destroying everything around it.
Life on any planet orbiting this exploding star would be completely eliminated.
You certainly wouldn't want to book a cruise to Betelgeuse anytime soon
or after it has gone supernova because when it finally dies it might leave a nasty surprise.
One of the most extreme objects in the universe, a neutron star.
Neutron stars are kind of like vampire zombies. They are the cores of massive stars that have
died but now these neutron stars have their own gruesome lives and you don't want to get
anywhere near this thing. Trillions and trillions of tons of matter are compressed into a sphere
roughly the size of Manhattan. A neutron star is the densest body we know of in astrophysics
besides a black hole. So if you somehow had a little stone-sized piece of neutron star matter
it would weigh 100 million metric tons and it would immediately fall right through your hand.
Because the neutron star is so dense it generates an intense gravitational field.
It is really hard to exaggerate how dramatic and dangerous a neutron star is.
The gravity is so intense it would actually bend light around it.
You would see all these kind of weird shimmering effects.
Dazzling but deadly. No astronaut will ever be able to approach a neutron star.
But if you're an armchair traveler and want to find out what would happen
let's send a galactic crash test dummy. We'll call him Chuck. Crash test dummies are a species
that are completely devoted to ensuring human safety and they sacrifice themselves to do it.
Everything he encounters is going to be going to be a pretty rough ride. Better him than me.
As Chuck nears the neutron star its gravitational grip is doing very bad things.
The gravity is pulling on him so hard that he is accelerating all the way down to the surface.
He'll be moving at very roughly one-half to two-thirds of the speed of light.
The neutron star's gravity is 200 billion times stronger than on earth.
Around 150 miles above the surface it starts to pull on Chuck's limbs in a distinctly unpleasant
way. As you get closer and closer to a neutron star we were told to think that it would be this
elegant spaghettification where you would get longer like a piece of spaghetti but in reality
you're going to get ripped shreds. Think about what you're really going to experience. Think
about first all your joints dislocated in your body, your skin getting ripped off your body,
your bones being pulled apart, your organs being pulled apart. Within a blink of an eye
our dummy is just a thin stream of atoms hurtling towards the star. Those atoms will eventually fall
down onto the neutron star and unfortunately the violence doesn't stop there. What's left of Chuck
hits the surface triggering a huge burst of energy. So we're talking about a hundred thousand
miles per second. That's an impact. He's going to hit so hard that the amount of energy released
is just huge. It would completely dwarf the entire arsenal of nuclear weapons on our planet.
Anything and anyone that ventures too close to a neutron star is destined for this catastrophic end.
A neutron star is one of the most dangerous objects you can meet in any phase of their
existence. If you're meeting a neutron star right when it's born that means you're very near a
supernova and that means death. If you meet a neutron star after the supernova has gone off
that would be death and then if you were lucky enough or unlucky enough to go falling onto a
neutron star you'd be destroyed very rapidly and torn apart. If I had one piece of advice
about neutron stars for future space travelers it would be no no stay away.
So you really don't want to be anywhere near one neutron star and its lethal gravity.
Try two neutron stars colliding and creating one of the strangest
and most lethal particles in the universe.
Some of the brightest lights in the universe are created by young blue stars
as they die in bright explosions. Super luminous supernovas are the ultimate example but other
types of stars can go supernova too. Yellow stars like the sun swell up as they age
transforming into oversized monsters known as red giants. The biggest of these bloated stars are
called red supergiants and astronomers often see them explode in bright violent supernovas.
The bigger the red giant the bigger the bang but there's a problem. Nobody has ever witnessed the
flash of the very biggest red supergiants in our galaxy. These most massive bloated old stars
have to be dying but if not in a flash of light then how? Now scientists have come up with an
extraordinary theory. Instead of exploding in a bright supernova the biggest of the red supergiants
are simply blinking out of existence. Scientists dubbed these weird disappearing deaths unnovas
and new evidence suggests these unnovas could be cold-blooded planet killers.
You're looking up into the sky the sun is shining and all of a sudden it just turns out. That's what
an unnova would look like. It would be the biggest catastrophe in the history of the planet. Life as
we know it would not be able to survive. Scientists believe the key to the biggest red
supergiants disappearing is a super efficient transformation from a giant burning ball of gas
to a tiny dense black hole. Everything has to be perfectly tuned to get an unnova. The star can't
be rotating very quickly and the outer layers can't expand much. When all the conditions are right it
just collapses into a black hole. They basically just become a black hole. It's not unusual for red
supergiant stars to form black holes when they die but most do it after they've released the
violent flash of light we see as a supernova. But the biggest supergiants have so much mass
and so much gravity in their cores that when they collapse not a single photon of light escapes
from the newly formed black hole. To an observer the star simply disappears. The death of a star
without the flash. An unnova. It's almost like the star has fallen in and has forgotten to come out
but more realistically what's going on is when it falls in it just can't come out. It's created so
much gravity around itself that even an explosion doesn't allow it to escape. It doesn't get to
explode. It just falls right into a black hole. So what makes unnovas planet killers?
The biggest red supergiants age relatively quickly dying after just 10 million years.
But astronomer David Kipping believes that just might be enough time for these giant stars to
create potentially habitable worlds. Planets can form pretty quickly. They can form in within a
million years around these stars so there should be time for these massive stars to form planets.
And in fact when we look at the remnants of massive stars we indeed find rocky planets
around them. So as far as we can tell these stars really should have worlds orbiting them.
Imagine a lone rocky world warmed by the far distant light of a red supergiant star.
Simple life clings to shallow rock pools on the young planet's surface
but their warm comfortable existence is doomed. High in the sky the far distant supergiant sun
is burning through the last of its hydrogen fuel. The force of gravity pushing in overcomes the
force of fusion pushing out and 20,000 trillion trillion tons of hot burning hydrogen gas
collapses down into a single point in space. A black hole. Surprisingly the black hole that
makes the unnova so dark doesn't put the planet in immediate danger. This is one of the biggest
misconceptions of movies is that suddenly if a star becomes a black hole then the planet is
going to be sucked into it. The gravity of the black hole is exactly the same as the gravity
of the star as long as it hasn't lost any mass. From a distance if you're orbiting this star
it's the same as orbiting the black hole. Nothing would change. As the supergiant star collapses
the view from the far distant planet would be surreal. What you're going to see is there's your
star in the sky and then a minute later it's gone. You will actually see it collapse forming a black
hole and the whole thing just falls into it and that's that. What would happen next would be a
long slow cold death. You're basically turning off your star. A fleeting moment but the beginning
of a winter that would never end. If you suddenly turned off the light from the sun life wouldn't
actually be immediately extinguished. It would just be like the night. We would be a little bit
cooler than normal but eventually over time over weeks over months over years the planet would
begin to freeze over. After a hundred years a global ice age engulfs the planet. First the land
then the oceans. The oceans would freeze over into a thick crust. Maybe a little bit of liquid water
would still be there at the bottom of the ocean warmed by volcanic vents. Eventually what you're
left with are things that don't depend on sunlight to live. Maybe there are tube worms living in
vents, cracks, hydrothermal vents in the bottoms of the oceans and that sort of thing.
But even those can't possibly live forever. The internal heat of the planet continues to radiate
out into space. The surface temperature drops below minus 350 degrees Fahrenheit and the atmosphere
collapses onto the surface as snow. The core of the planet can no longer support active geology.
All life is gone. The planet is dead. So these habitable worlds will eventually end up being
just these spheres of ice. Whether killed by the light of a supernova or by the darkness of an
un-nova, planets are in the firing line from killer stars. But research recently released
suggests that stars too can fall victim to murder and some of these killings are straight
out of a horror movie. How can an old star that's on the way to die get more mass so it can become
young again? Well it can do exactly what a vampire does. It can suck life from something else.
2012. The Hubble Space Telescope makes a gruesome discovery. It finds killer stars
sucking the life from their neighbors. These vampire killers are found lurking inside
tightly packed groups of stars known as clusters. Stars are born in giant clouds of dust and gas
and these clouds have enough material to make dozens or even hundreds of stars.
We call these family of stars star clusters and we think they're all roughly the same age.
Young clusters shine like jewels with an array of bright colors. Blues, yellows and reds.
But this starry rainbow changes over time. The blue stars disappear first. These are
the biggest stars in the cluster burning brightly and dying young after millions of years.
Next to go are the yellow stars. These medium-sized stars age over billions of years
gradually turning red like ripening fruit. After 10 billion years the entire cluster matures
to a deep red. This gradual shift in color is useful to astronomers because it allows them
to judge just how old a cluster is. When you look at a population of stars in one place
if you see a lot of blue stars you can be pretty confident that must have
young stars. They couldn't have been born too long ago because blue stars are massive and
massive stars go through their fuel quickly and live very short lives. But in the 1950s
astronomers spotted something seriously weird in an ancient cluster. Tucked amongst the old
red stars they found a handful of brightly shining young blue stars. New stars don't
usually form inside mature clusters so how did they get there? The only explanation? Somehow
the old stars were getting younger. Astronomers dubbed these age-defying stars blue stragglers.
In some clusters we see these blue stars that appear younger than they should. In some ways
they're kind of straggling behind the natural aging of the cluster. Something must be actively
rejuvenating a star but what could do that? If you imagine these blue straggler stars were people
in a crowd these stars would look like they had been given a facelift. They're masquerading as
younger stars when really they're just as old as everybody else in the room. Astrophysicist
Natalie Gosnell believed the blue stars were being rejuvenated by a fresh supply of hydrogen fuel
but where was it coming from? In 2015 Natalie took a closer look at the Hubble images of the blue
straggler cluster. She discovered that most of the young looking stars were in binary partnerships
with the corpses of dead stars that appear to have had their gas sucked away from them.
So in movies vampires are perpetually youthful because they are sucking blood from humans and
so in this case we have stars that are sucking gas and material from other stars keeping them
looking young. Right now somewhere in the universe a giant star is detonating
creating a huge cosmic explosion called a supernova. Supernovas are a big giant traumatic
end to a star's life. All stars die but only the biggest go out with a bang.
For a star to go supernova we think it has to be at least eight times more massive than our sun.
It's so easy to think of our sun as this incredibly gigantic thing
but our sun is absolutely tiny compared to some of the giant stars in the sky.
We can see some of these giant stars with the naked eye and the tenth brightest in the night
sky is a red super giant around 15 times the mass of the sun, Betelgeuse. Betelgeuse is so big that
if you were to place it in our own solar system it would stretch to the orbit of Jupiter. This is
one of the biggest beasts in the galaxy. It's a star also that is on the verge of death. Betelgeuse
is less than 10 million years old but this huge star's days are numbered. It's ready to blow
and when it does we'll see a region of sky brighten for 14 days until it's nearly as bright
as a full moon. It is going to be one of the most spectacular shows in history and it could happen
at any moment. I mean this is the thing. I often stand outside in my yard in the winter time.
I look up at Orion and I see Betelgeuse and I'm like explode. So what will make Betelgeuse go
supernova? To understand a giant star's death we need to understand its life. From the day it's
until the day it dies a star's life is a constant battle. Gravity is pulling in and energy pushing
out. The interior of a star is fusing countless atomic nuclei together. Atoms are ramming into
each other getting very very close. If they get close enough they'll actually stick and form a
Every second a giant star fuses seven and a half billion tons of hydrogen.
That amount of energy is roughly equivalent to about a hundred billion atomic bombs per second.
That's a big ass explosion. This explosive energy threatens to blow the star apart
but the star's own massive gravity keeps the lid on.
Everything in the universe is a fight between the inward force of gravity and the outward
force of pressure or energy. Every single star in the sky, even our own sun, is an incredibly
dynamic battleground. In many ways stars are an explosion that are actually too big to explode.
Gravity holds it together. This battle between these two opposing forces determines the life
and death of the star and this is where size matters. The more massive the star the more
gravity pushes inward and the harder the star has to push outward to keep itself alive.
Very massive stars are like stars on steroids. They have a lot of fuel to burn.
They're so powerful that they use up their fuel at a rapid rate.
Massive stars like Betelgeuse are giant factories fusing lighter elements into
heavier ones but the hard work doesn't start until their final years. For around 90 percent
of their life they fuse hydrogen into helium but eventually the hydrogen starts running out.
In the core of a supergiant star there's a sequence of fusion that goes from lighter
elements to heavier elements and it gets faster and faster every step of the way.
The countdown to death begins. The inward push from gravity takes over
raising the temperature in the core. Helium starts fusing into carbon. There's enough helium to last
about a million years but it too runs out and things start speeding up. Carbon gets fused into
neon. That takes about a thousand years. Neon fusing into silicon that takes about one year.
Once it starts fusing silicon into iron that takes one day. It gets more and more frantic. It's kind
of like a cooking contest show whereas the clock is running down. They're trying to do more and
more things and they get more and more frantic until ding! Time's up. The star is now in its
death throes. Once iron production has started the clock is ticking towards the cataclysmic end
of this star. A giant ball of incredibly dense iron forms in the middle of the dying star's core.
This iron sphere is several thousand miles across and unbelievably hot. It gets so hot there
the temperature almost becomes meaningless. I mean we're talking about a billion degrees in the
center of one of these stars. This extreme heat is caused by fusion reactions. More and more reactions
create heavier and heavier elements and with each step less and less energy is produced
until iron is created. When you try to fuse iron nuclei together that takes energy. It doesn't
generate energy. So once the core starts to fuse iron it's basically stealing its own energy.
The growing iron core sucks more and more energy from the star.
Gravity continues pulling in overwhelming the outward pressure from inside the star.
Everything gets crushed to unimaginable degrees. All of a sudden there's no
nuclear reaction to support the star against the crush of gravity.
With nothing left holding it up the star is doomed. Gravity wins. The edges of the iron core
collapse. Trillions of tons of dense iron fall inward at a quarter of the speed of light.
The star has now less than one second left to live. Things start to fall apart really quickly.
The core collapse is so fast that the outer layers of the star don't even have time to react.
They're just hanging there. It's kind of like Wile E. Coyote when a cliff collapses underneath
him and he doesn't even fall until he notices. The rest of the star collapses. A trillion trillion
trillion tons of gas hurtle inwards following the iron. Think about the entire mass of the star
that has been held up by nuclear reactions inside. All of a sudden those nuclear reactions go away
in a split second. Everything rushes into the middle and that sets off the most dramatic
explosion in the universe. The spectacular death blow can outshine all of the stars in the galaxy
but there's a problem. We still don't fully understand how a collapsing ball of iron
and tons of falling gas create a giant fireball. How this collapsing core triggers a massive
explosion is one of the biggest mysteries in astrophysics. For over four and a half billion
years the sun has bathed our home planet with light. Its bright stable glow helps life flourish
but hidden in the night sky other planetary systems haven't been so lucky. Hanging right
above your head every night we see up there these dead corpses of stars. 400 light years from earth
lies a system called SDSS J1228. A disk of debris orbits the faintly glowing leftovers of a dead
star. J1228 is a dead star. It is the core of a star that had aged blown off its outer layers
revealed the core which is about the size of the earth but has about half the mass of the star in
it and we call these white dwarfs. May 2018 astronomers investigated J1228 using the world's
largest optical telescope the Grand Telescopio Canarius. They discovered what appears to be
a ball of iron orbiting the white dwarf. The lump of metal less than 400 miles across
could be the exposed core of a destroyed planet. It's a clue to this system's past.
It's always a little poignant when you see evidence of a planet around a dead star
you know you think back when that star was shining and could there have been life in that
solar system. The J1228 system is a cosmic graveyard. It might look different than our
solar system but this is our future. This discovery of a dead planet orbiting a dead star is like
looking into a crystal ball and is it the future of our own solar system? For a glimpse into your
future you know all you need to do is look up. Just like J1228 our sun will die killing off earth
in the process. This terrifying fate will play out across the galaxy in a star apocalypse.
Our sun is a fairly common type of star in the Milky Way and so other stars in the Milky Way
will undergo the same sort of fate as the sun and will end up as white dwarfs and so any other
planets out there orbiting sun-like stars will undergo a similar fate. Once the stars like our
sun have died out what's going to happen? Could life still survive around white dwarfs? To understand
the fate of sun-like stars we have to look inside them. Buried within are clues to how they live
and why they die. The core the very center that's where the action is that's where the star
is fusing light elements into heavier elements that works like a like a hydrogen bomb that's
the same thing. If you compress hydrogen enough it gets very hot and the pressure gets very high and
it fuses into helium and generates energy heat and that's what's happening in the core of every star.
Because of their enormous mass stars have huge amounts of gravity.
This gravity pushes inwards trying to collapse the star
but fusion energy from the core stops that from happening. It's really this sort of very balanced
dance between gravity pushing in fusion energy pushing out. You can think of a star as losing
energy continuously to the outside world and gravity is saying yes I'm going to take over
but no the nuclear reactions inside a star replenish the energy that's lost and keep the
star hot and pressurized inside so that the pressure gravity balance can be maintained.
This balance keeps sun-like stars alive for up to 10 billion years until the star's gas tank
runs dry. It's going to run out of fuel and when that happens it's going to
die but what is that going to look like how is this going to happen?
100 million years ago things in the J1228 system started to get ugly. First the star grew large
really large. Once the center starts fusing heavier elements the outside will swell into
what will eventually be a red giant star. J1228 transformed into a red giant its outer layers
blew off extending out over 40 million miles. When stars like our sun die it's not a quiet
affair it's very violent and ugly and messy they turn into red giants and they turn themselves
inside out and vomit all over the solar system. When J1228 swelled into a red giant nearby planets
were stuck in a kill zone. The dying star engulfed them or fried them with temperatures
of over 1200 degrees Fahrenheit. Atmospheres disappeared oceans boiled away but one planet
survived J1228's death throes. Here's a case where a planet survived in some sense the death
of its own star and is still hanging around still hanging on hoping for something new.
The red giant's expanding outer layers separated from the star's core with no active fusion the
core collapsed into a white dwarf. The white dwarf's dense gravity then went to work on the
one surviving planet. A planet that might have been orbiting the normal star can gradually spiral in
toward the white dwarf and then eventually the gravity of the white dwarf pulls on the near side
of the planet more than on the far side and that tears it apart. What we're seeing here is a dead
star dining on its own solar system that's what is in the future for the sun. J1228 feasted on the
remains of its rocky worlds leaving behind a disk of debris and the planetary core. It's a glimpse
of earth's future. What happened here around this white dwarf is going to happen to earth
it's going to be stripped of its atmosphere its crust and its mantle and the only thing that will
remain will be the core. Fried and ripped apart by a dying star not a good way to go.
Fortunately for life on earth our own sun isn't dying just yet. The sun is middle-aged it's four
and a half billion years old and it's going to go on for another five or six billion years.
We've got a little bit of time before our sun pukes all over the solar system.
Our home planet may be safe for now but systems like J1228 show us that sun-like stars are
destined to die killing off any life orbiting them. But sun-like stars aren't the only stars
dying across the cosmos there are others out there and they're all doomed.
There's a wonderful rainbow of stars out there of all different shapes all different sizes and
all different colors. We're talking down to you know fractions of the mass of the sun
up to hundreds of times the mass of the sun. When it comes to the star apocalypse
size matters. The bigger and brighter the star the faster it dies. The Bering Sea asteroid blew
up in the atmosphere but the Beringer crater asteroid hit the ground intact with its full force.
Why do different asteroids behave differently and what will Apophis do when it heads our way?
Arecibo's radar may have the answer. When we bounce radar waves off of these objects we can get
effectively imagery of the surface of some of these small objects that we just cannot do with
optical telescopes. This is the radar image of Apophis. It's so far away that all they could
image were a few pixels. So this is our most recent radar image of asteroid Apophis and you
can see it's only a few pixels but it does give us information on what it actually is.
These few pixels are enough to work out how big Apophis is. From this image we can
constrain the size to be about 1 000 feet which is about the same size as the
Arecibo radio telescope. All of that from a weird bunch of pixels. Knowing the size and
mass of an asteroid is critical to understanding what an asteroid is made of. If we have the size
and the mass we get the density. If we have the density we know what it's made of. Rock has some
density. Metal has a different density. So we can determine a huge amount about the asteroid
simply by pinging it with radar. Arecibo's data reveals that not all asteroids are alike.
There's not just one kind of asteroid. There are actually several kinds and this is important to
understand because they behave differently. They behave differently if they impact us and they
behave differently if we're trying to prevent them from impacting us. We need to know what these
asteroids are made of if they're gonna hit the earth because that drastically alters the potential
effects. Asteroids come in different shapes, different sizes and different compositions
and we think that is because they are the leftovers of planet formation. To understand how
each asteroid formed and their threat level we have to go back 4.6 billion years to the start
of the solar system. The reason that there are all these asteroids floating around in our solar
system today is just because of the early violence of the solar system as it was forming. At the birth
of the solar system the sun ignites leaving a disk of gas and dust. Slowly over time planets
form. Lots of planets. The early solar system was a messy place. There were a lot more planets,
a lot more forming planets. They would crash into each other, they would merge, they would
disintegrate, they would reform. This process of accretion of building planetary worlds was
not just you know kind of gentle and happy it was it was violent. It was like a giant
cosmic game of pool. Planet smashing into planet. The leftovers from this violence
formed a ring of junk between Mars and Jupiter. And now we call that junk asteroids. They're just
basically rubble left over from the formation of the solar system. Rocky leftovers became C-type
or chondrite asteroids. They're quite dense so big ones can punch through the atmosphere
and hit the ground. Radar reveals a rarer type of asteroid. Some of them really stand out because
their density is so much higher than the rest of the other asteroids. These asteroids are M-type
or metal. Because their mass is great they carry more kinetic energy during a strike.
By far the worst one is this iron meteorite. This is really heavy so the difference if you
were being hit by this would be the difference between being hit by a rock and being hit by
a metal hammer. We think that both the Beringer and the KPG dinosaur killer were caused by metal
asteroids. But there's another more mysterious type floating through space. December 2018 NASA's
spacecraft OSIRIS-REx approached the near-earth asteroid Bennu. Over time it drifted out of the
main asteroid belt made its way into the inner solar system until it became a near-earth asteroid
accessible for our spacecraft to go and visit. OSIRIS trained its camera on Bennu.
One of the biggest surprises on arrival at Bennu was the large number of large boulders on its
surface. Bennu is really littered with huge boulders and littered with medium-sized boulders
and littered with small boulders. Bennu is not a solid lump of rock. It's made up of thousands of
bits of rock forming what we call a rubble pile. These asteroids aren't big singular spherical
balls of rock but rather they're literally piles of rubble. They're all sorts of pieces and
fragments from another asteroid that had previously been disrupted that have all come back together
and formed literally a pile of rocks held together by their own gravity. We think rubble piles formed
from collisions inside the asteroid belt. Each impact blasted bits off. Then over time they came
back together to form a loose pile of rocks. Imagine taking a big cosmic dump truck full of
gravel and rubble and dumping it out there into space and letting gravity weakly hold it together.
When scientists probed deeper into Bennu they found another surprise. It's full of holes like
Swiss cheese. If you could slice open one of these asteroids you'd see there are a lot of voids. In
fact 60% of what we're looking at is a void space. So they're actually really fluffy. So even though
they're made of rocks they're sort of the lint of rocks. Bennu helps us understand Apophis.
Radar data shows that Apophis is also a rubble pile. If you look at Apophis we really want to
know how its orbit will evolve in the future. What we learn at Bennu about similar size rubble pile
asteroids might help us understand the future of an asteroid like Apophis. So what would happen
if the rubble pile called Apophis hits earth? You probably don't want that to hit you still but it
definitely makes it a lot weaker than something like a solid rock or even more a chunk of nickel
iron metal. Does its composition make it any less of a threat? A rubble pile like Apophis is especially
unnerving because we don't know when it interacts with the atmosphere if it's going to stay as one
solid piece. Will it break up? When these rubble piles start interacting with planets if they fly
near a planet they can get pulled apart into all of their little pieces. Or if they enter the
atmosphere of a planet to impact the surface they might slowly get pulled apart as they enter the
atmosphere and end up being an array of little impacts instead of one big single impact.
But what would happen if these impacts occur at sea? Will our oceans save us or will a giant tsunami
wipe us out? Our hunt for the Milky Way's next supernova has identified some potential suspects.
Very massive lonely stars and stars with smaller sidekicks. In 2018 astronomers found a system
called APEP 8,000 light years away with two very massive stars. Each one about as massive as
Betelgeuse. These are giant stars nearing the end of their lives with massive outer layers of gas
that continually contract and heat up again and again. They become really huge and bloated and
swollen and they're prone to huge outbursts. These unstable stars are called Wolf-Rayet stars.
They're very rare and so hot and bright they emit more radiation than a million sun-like stars.
This intense energy is blasting their outer layers off into space. Mass loss has been occurring
from the star so much so that you've actually lost all the hydrogen that was wasn't burned
into helium. So now you have a star that's made entirely of helium and heavier elements.
With no hydrogen left these massive stars are running low on usable fuel.
They're like ticking time bombs made even more dangerous because they're spinning so fast.
It's spinning so quickly it's on the verge of ripping itself apart. And this means that when
this thing blows it's gonna blow hard. When a star goes supernova its core collapses.
The smaller it gets the faster it spins. Some cores collapse into fast spinning neutron stars.
Heavier ones like APEP collapse into even denser and more mysterious objects. Black holes.
The immense gravity within APEP's collapsing core will drag back some of the gas and dust
into a spinning disk. As the material falls onto the core it compresses and it speeds up.
The dying star spins faster and faster as it collapses. And this incredible rotation
drives the creation of massive magnetic fields that are capable of funneling material around
and up and out in the form of huge beams of radiation.
So the energy from the supernova collapse instead of being emitted spherically in every direction
comes at us in a tightly focused beam. Like a laser from the death star it is pointed in one
direction. This is a gamma ray burst. It is the single scariest thing the universe has to offer.
This is an explosion so powerful that in a few seconds or minutes it can release as much energy
as the sun will over its entire lifetime. You do not want to get caught in a gamma ray burst.
Let's just put it that way. The impact of a nearby gamma ray burst on our home planet
is almost too terrible to think about. It would be a very bad day for Earth. Earth's atmosphere
could be partly blown away and there could be chemical reactions in the atmosphere that would
form all kinds of noxious products. A gamma ray burst from APET might last only 10 seconds
but its impact would last for decades. The generation of nitrogen oxide from a gamma
ray burst would be disastrous. In the upper atmosphere it would eat away at our ozone layer.
In the lower atmosphere it would come out as acid rain. And the acid rain would destroy our crops.
Nitrogen dioxide also filters out sunlight
turning the skies dark and cooling the earth enough to trigger a new ice age. Any life on the
land in the shallow parts of the sea or that live near the sea surface would be done. In fact it
would ultimately result in extinction. Blasted by ultraviolet radiation from our sun, freezing cold
and hungry, humanity's future would be bleak. So we really need to know. When APEP goes supernova
and produces its deadly beam of gamma rays, are we in its line of fire? The good news is that we are
probably not right in the direct firing line of APEP. The axis of rotation of the APEP system
is pointed 30 degrees away from us. So if it does blow it's likely that the jets are going to miss
us. Makes me feel better that this gamma ray burst isn't pointing at us. But of course there are many
other cosmic catastrophes potentially waiting to get us. APEP is on the edge of an enormous
explosion. Its huge gravity and incredible spin should produce a spectacular supernova.
But what if some stars are too big to blow?
