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SUB BY : DENI AUROR@
https://aurorarental.blogspot.com/
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Two black holes circle each other
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in a dance of death.
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They spiral inwards,
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their immense gravities pulling them ever closer.
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When they finally collide,
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it's one of the most powerful events
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since the big bang.
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This explosive mystery
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sends ripples across the world of science.
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But can it also answer
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one of the most pressing questions in cosmology?
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How do supermassive black holes grow so large?
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Captions paid for by discovery communications
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in the known universe,
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there are roughly 2,000 billion galaxies.
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Each one has a different shape and size.
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But they may all have one feature in common ...
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a supermassive black hole buried at their center.
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As its name says, it is supermassive.
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And here, we're talking about objects
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that are millions or billions of times
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the mass of the sun.
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Supermassive black holes
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are so big that we need a special scale
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for measuring them.
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A solar mass is the mass of the sun.
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So when we study the universe,
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we have to use the tools that we have in hand.
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And what's the most massive thing that we have around us?
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It's the sun. And so we refer to things
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in multiples of the mass of the sun
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because it just makes it easier to wrap our heads around.
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However, if you have something that's 17 billion times
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the mass of the sun, that's pretty difficult
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to wrap your head around anyway.
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But we know that those kinds of black holes
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live in the centers of galaxies.
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The supermassive black hole at the center of our galaxy,
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the milky way, is called sagittarius "a"-star.
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It weighs in at 4 million solar masses.
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But compared to the other supermassive black holes
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out there, it's puny.
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This is probably one of the only contexts
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where you would think that our supermassive black hole
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isn't very supermassive.
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The supermassive black hole
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in our neighboring galaxy, Andromeda,
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is 25 times larger than sagittarius "a"-star,
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coming in at 100 million solar masses.
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But compared to the largest monsters
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out in the universe, it's a runt.
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O.j. 287's primary supermassive black hole
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weighs in at 18 billion solar masses.
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And the black hole in the core of galaxy ngc 4889
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in the coma cluster weighs 21 billion solar stars.
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That's over 5,000 times larger
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than sagittarius "a"-star.
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These are incredible things
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that are more massive than some galaxies.
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Now astronomers may have made a remarkable discovery ...
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a giant, new supermassive black hole
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that's a mind-blowing 30 billion times
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the mass of the sun.
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It's a huge puzzle.
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And we have simply no idea how it got so big.
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It's a huge mystery how black holes have become so enormous.
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We started finding black holes with millions
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and billions of times the sun's mass.
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No one expected that.
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And we have no idea how they got to be so big.
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It's not entirely clear at this point
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how supermassive black holes can get to be the masses
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that they are today.
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Regular-sized black holes form
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when large stars over 20 times the mass of our sun
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crash and burn.
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When a large star runs out of fuel,
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the core stops generating enough outward force
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to counteract the power of gravity crushing inwards.
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As the star collapses,
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the outer part explodes in a supernova.
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The inner core shrinks
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from a sphere millions of miles wide
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to one just 10 miles across.
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It's like shrinking the earth down
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to the size of a golf ball.
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This rapid collapse creates a black hole.
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So we now have seen black holes
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that are solar-mass black holes
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and black holes that are million
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or billion-solar-mass black holes.
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And the question is, how do you get from one to the other?
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Do the giants somehow grow
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from a solar-mass black hole?
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Bullock: One of the big puzzles today is,
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how do you make one of these supermassive black holes?
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One idea is, you get there by starting
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with a solar-mass black hole,
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having it grow through a stage
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of being an intermediate-mass black hole
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and then eventually getting to be
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a supermassive black hole.
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Theoretically, intermediate-mass black holes
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should be between 100 and 100,000 solar masses.
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But we've never seen one.
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Part of the mystery of supermassive black holes
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is that black holes seem to occur in two flavors.
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You have ones that are only a couple times
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the mass of the sun.
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And you have ones that are millions
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or billions of times the mass of the sun.
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So we have small and extra large.
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If we think of the stellar-mass black hole
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as sort of the baby black holes,
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and the supermassive black holes as the grown-up black holes,
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we're missing the teenage black holes.
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Where are these black holes that have masses
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that are between stellar mass and supermassive?
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Bullock: They're sort of like a holy grail
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for black hole hunters.
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Where are these things? Where can we find them?
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And how do you make them?
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Then astronomers caught a break.
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They picked up a burst of energy
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coming from the ngc 1399 galaxy.
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It was the death throes
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of a star being eaten by a black hole.
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When they measured its size, they discovered it was
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an elusive intermediate-mass black hole.
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The missing link had been found.
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But when scientists did the math
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to see if such an intermediate-mass black hole
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could grow into a supermassive black hole,
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they hit a snag.
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There hasn't been enough time
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since the birth of the universe
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for an intermediate-mass black hole
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to eat enough stars
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to grow into a supermassive black hole.
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Bullock: It doesn't seem like there's enough time
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for black holes to get as big as we see them.
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But supermassives are everywhere we look.
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How did they get there?
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And how did they grow so huge?
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In our universe, we've detected small black holes.
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And we've seen monsters,
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supermassive black holes
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billions of times the mass of our sun.
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But we'd found almost none in between.
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So how do you get from a small black hole to a giant one?
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One of the most important outstanding questions
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in cosmology is,
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how did supermassive black holes
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get as big as they are?
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And when did that happen?
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Black holes are normally surrounded by gas and stars,
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an all-you-can-eat buffet.
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One of the best ideas for how black holes grow
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is that black holes do
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what we expect black holes to do,
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and that is eat stuff.
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For a black hole,
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it's almost as if the universe is its restaurant.
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And on its menu, you'll find stars, planets,
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and clouds of gas and dust.
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So is binge-eating the answer
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to growing a supermassive black hole?
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Theoretically, black holes should keep on growing forever
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as they consume more and more food.
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But recent discoveries suggest
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that the universe puts them on a diet,
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controlling how much they eat.
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Black holes are hungry. They like to eat.
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But sometimes, they eat too much,
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and they burp it up.
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February 2015.
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Astronomers report something unusual
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in the galaxy ngc 2276.
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it looked like something had taken a bite
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out of one of its spiral arms.
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Sitting alone in the void
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was an intermediate-mass black hole,
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about 50,000 times the mass of the sun.
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One theory was that the black hole
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had eaten everything around it,
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creating the dead zone.
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But the detection of a burst of energy
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from the black hole suggests
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it may have tried to eat too much
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and, in the process, destroyed its food source,
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burping so hard, its food was blasted away.
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Turns out that black holes are actually very messy eaters.
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A lot of matter gets thrown off as it tries to absorb it.
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So things move in, gets hot.
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But then a lot of it gets thrown all the way back out.
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Isler: Black holes are not vacuums in space.
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They do not just eat everything around them.
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And so they are messy. Some things get in.
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And they take that on. And it grows their mass.
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And some things are just flung out as they're eating.
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The enormous gravity of black holes sucks gas, dust,
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and even stars towards them.
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Everybody's been to an all-you-can-eat buffet.
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But let's be honest. There really is a limit
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to how much you can eat.
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Black holes are gluttons. They're greedy.
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They don't really know when they've eaten too much.
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They just keep on cramming in more and more food.
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It doesn't just fall in.
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It has to go down the drain, more or less.
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And so it forms this disk around the hole.
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And as it does that, there's a lot of turbulence
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and magnetic fields
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and a witch's brew of forces going on there
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that get it really hot.
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As the gas and dust swirls around,
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it heats up,
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pushing temperatures to millions of degrees fahrenheit.
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This swirl, called the accretion disk,
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also generates powerful magnetic fields.
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These fields are dragged by the spin of the black hole
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and become focused above the poles.
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As energy builds up,
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the magnetic fields become so compressed
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they blast out super-energized particles.
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These beams can actually be incredibly violent.
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Matter is flung out
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at a large fraction of the speed of light.
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It's a tremendous wind
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that blows very hard away from the black hole.
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The jet hits the gas clouds
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surrounding the black hole,
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blowing the buffet away.
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If they eat too much,
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they can basically blow everything
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that's in their vicinity away.
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They lose their food supply. And then they're gonna starve.
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They can kind of shoot themselves in the foot.
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With no food available,
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the black hole stops growing.
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Astronomers think that's what happened
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to the intermediate-mass black hole
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they discovered in the dead zone.
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These burps may regulate star formation
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and stop the black hole from getting obese.
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But over time,
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the black hole will start eating again
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as gas falls back towards it.
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But can an intermediate-mass black hole eat enough
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to become a supermassive black hole
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weighing billions of solar masses?
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Could that black hole become so obese by eating?
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That's a really interesting question.
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You'd have to eat a heck of a lot
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to get that fat.
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When you think about it, if you imagine an average galaxy
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has 100 billion stars,
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the black hole would have to eat one
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in every five stars in the galaxy.
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The universe is old. But is it really old enough
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that black holes have had time to consume billions of stars?
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That seems kind of unlikely.
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Bullock: It doesn't seem to add up.
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We need some other way
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00:13:15,962 --> 00:13:17,962
to make these supermassive black holes.
266
00:13:17,964 --> 00:13:21,065
And the question is, what is that?
267
00:13:21,067 --> 00:13:23,734
Maybe we've been making this all too complicated.
268
00:13:23,736 --> 00:13:28,406
Maybe to get a big black hole is to start big in the first place.
269
00:13:28,408 --> 00:13:31,876
So how can black holes start big?
270
00:13:31,878 --> 00:13:35,280
To answer that question, scientists had to journey back
271
00:13:35,282 --> 00:13:37,849
to the very start of the universe,
272
00:13:37,851 --> 00:13:41,419
to a mysterious time called the dark ages.
273
00:14:01,006 --> 00:14:03,441
As we look out into the universe,
274
00:14:03,443 --> 00:14:08,012
we're seeing farther and farther back in time.
275
00:14:08,014 --> 00:14:09,313
We have now looked back
276
00:14:09,315 --> 00:14:12,449
over 12 billion years
277
00:14:12,451 --> 00:14:15,920
to the time when the cosmos was still an infant.
278
00:14:15,922 --> 00:14:21,225
And what we found was a huge surprise.
279
00:14:21,227 --> 00:14:22,827
We had made the assumption
280
00:14:22,829 --> 00:14:25,129
that as you look farther out into the universe,
281
00:14:25,131 --> 00:14:26,464
the black holes would be smaller.
282
00:14:26,466 --> 00:14:28,166
They haven't had much time to grow.
283
00:14:28,168 --> 00:14:30,801
But now we've found a 12-billion-solar-mass
284
00:14:30,803 --> 00:14:33,104
black hole that's actually less
285
00:14:33,106 --> 00:14:34,772
than a billion years into the universe.
286
00:14:34,774 --> 00:14:36,641
How did this thing form so early?
287
00:14:36,643 --> 00:14:38,176
How did it grow so fast?
288
00:14:38,178 --> 00:14:40,577
This is like walking into a delivery room
289
00:14:40,579 --> 00:14:42,747
and finding a 100-pound baby.
290
00:14:42,749 --> 00:14:45,449
I mean, how does that even happen?
291
00:14:45,451 --> 00:14:47,084
It doesn't make any sense.
292
00:14:47,086 --> 00:14:51,155
Physics tells us no black hole could swallow enough stuff
293
00:14:51,157 --> 00:14:54,392
to get that big that quickly.
294
00:14:54,394 --> 00:14:56,794
There really wasn't enough time between the big bang
295
00:14:56,796 --> 00:14:58,763
and when we're studying these things
296
00:14:58,765 --> 00:15:01,299
for them to grow to such large sizes
297
00:15:01,301 --> 00:15:03,902
just by eating matter around them.
298
00:15:03,904 --> 00:15:07,839
So if there's not enough time for them to grow so large,
299
00:15:07,841 --> 00:15:12,109
maybe they're born supermassive.
300
00:15:12,111 --> 00:15:17,214
To understand how, we have to travel back even farther,
301
00:15:17,216 --> 00:15:20,084
to not long after the birth of the universe.
302
00:15:22,822 --> 00:15:24,888
isler: The early universe was definitely
303
00:15:24,890 --> 00:15:27,492
a much more compact
304
00:15:27,494 --> 00:15:29,093
and richer place for material.
305
00:15:29,095 --> 00:15:31,462
It was smaller, and it was denser.
306
00:15:31,464 --> 00:15:33,464
Things were much closer. It was hotter.
307
00:15:33,466 --> 00:15:38,869
It was just a much more intense place to be.
308
00:15:38,871 --> 00:15:43,274
Clouds of hydrogen and helium gas clumped together.
309
00:15:43,276 --> 00:15:46,577
As the clouds grew, so did their gravity,
310
00:15:46,579 --> 00:15:50,114
sucking in more and more gas.
311
00:15:50,116 --> 00:15:51,783
Eventually, the ball of gas
312
00:15:51,785 --> 00:15:54,819
became so dense, it collapsed,
313
00:15:54,821 --> 00:15:58,789
triggering nuclear fusion.
314
00:15:58,791 --> 00:16:00,892
A star was born.
315
00:16:00,894 --> 00:16:03,494
These massive first stars
316
00:16:03,496 --> 00:16:07,098
are called population III stars.
317
00:16:07,100 --> 00:16:09,500
Because there was so much food around,
318
00:16:09,502 --> 00:16:12,503
these stars were huge,
319
00:16:12,505 --> 00:16:16,774
many times bigger than any stars that exist today.
320
00:16:16,776 --> 00:16:19,310
Bullock: We think a lot of these population III stars
321
00:16:19,312 --> 00:16:21,579
probably were incredibly massive,
322
00:16:21,581 --> 00:16:24,782
incredibly short-lived, and just blew up right away.
323
00:16:24,784 --> 00:16:28,219
They would've left massive black holes behind.
324
00:16:39,398 --> 00:16:41,065
With so much food available,
325
00:16:41,067 --> 00:16:45,036
these young, ravenous black holes, called quasars,
326
00:16:45,038 --> 00:16:47,505
started binge-eating
327
00:16:47,507 --> 00:16:50,408
and became incredibly bright.
328
00:16:50,410 --> 00:16:54,212
Billions of years later, we can still see their gluttony.
329
00:16:56,215 --> 00:16:59,383
The most luminous, bright objects in the universe
330
00:16:59,385 --> 00:17:00,918
are things called quasars.
331
00:17:00,920 --> 00:17:02,319
And it may seem kind of ironic.
332
00:17:02,321 --> 00:17:05,389
But what these really are are supermassive black holes.
333
00:17:05,391 --> 00:17:07,392
There's so much stuff trying to cram itself down
334
00:17:07,394 --> 00:17:10,961
the black hole that everything gets very hot, very energetic.
335
00:17:10,963 --> 00:17:13,597
And you can see them clear across the universe.
336
00:17:13,599 --> 00:17:16,567
But when we measured the size of the young quasars,
337
00:17:16,569 --> 00:17:20,705
we discovered they were already billions of solar masses.
338
00:17:20,707 --> 00:17:22,573
Isler: There's not enough time,
339
00:17:22,575 --> 00:17:25,043
a billion years after the universe was created,
340
00:17:25,045 --> 00:17:28,512
for them to get to a billion solar masses in ...
341
00:17:28,514 --> 00:17:30,714
it's just too short a time.
342
00:17:30,716 --> 00:17:33,684
Bullock: So the question becomes, how do you make black holes
343
00:17:33,686 --> 00:17:36,888
that are this big in that small amount of time?
344
00:17:36,890 --> 00:17:38,089
We need some other way
345
00:17:38,091 --> 00:17:40,624
of growing these supermassive black holes.
346
00:17:40,626 --> 00:17:42,559
There needs to be some other mechanism
347
00:17:42,561 --> 00:17:44,829
that allows them to get that massive so early.
348
00:17:44,831 --> 00:17:47,731
But what is that?
349
00:17:47,733 --> 00:17:52,803
A clue can be found in the very early universe.
350
00:17:52,805 --> 00:17:55,473
The early universe is still so much of a mystery to us.
351
00:17:55,475 --> 00:17:57,475
We know that conditions were very different.
352
00:17:57,477 --> 00:18:00,545
It was denser. There was a lot more material.
353
00:18:00,547 --> 00:18:03,815
This period is called the dark ages.
354
00:18:03,817 --> 00:18:05,616
Bullock: During the dark age, we know
355
00:18:05,618 --> 00:18:08,452
that there was basically nothing happening.
356
00:18:08,454 --> 00:18:09,720
Matter existed.
357
00:18:09,722 --> 00:18:11,856
We think that there was hydrogen and helium gas
358
00:18:11,858 --> 00:18:14,758
but really not much else.
359
00:18:14,760 --> 00:18:16,760
There were a few stars around,
360
00:18:16,762 --> 00:18:20,097
but nothing large enough to form giant black holes.
361
00:18:20,099 --> 00:18:22,967
But there were huge clouds of gas.
362
00:18:22,969 --> 00:18:26,070
And because the universe was much smaller and denser,
363
00:18:26,072 --> 00:18:29,740
the clouds were much thicker.
364
00:18:29,742 --> 00:18:33,043
The idea is that from these basic ingredients,
365
00:18:33,045 --> 00:18:34,912
gravity and gas,
366
00:18:34,914 --> 00:18:38,983
the cosmos built massive black holes.
367
00:18:38,985 --> 00:18:41,218
Somehow, the universe has created a shortcut
368
00:18:41,220 --> 00:18:42,253
to the black hole.
369
00:18:42,255 --> 00:18:44,188
We've typically thought of it as,
370
00:18:44,190 --> 00:18:46,424
cloud of gas collapses into a star,
371
00:18:46,426 --> 00:18:49,960
star evolves, star dies, leaves behind a black hole.
372
00:18:49,962 --> 00:18:51,596
Perhaps the universe has found a way
373
00:18:51,598 --> 00:18:53,697
to skip the star phase
374
00:18:53,699 --> 00:18:55,599
and go directly to the black hole.
375
00:18:58,737 --> 00:19:03,407
Clouds of gas may have built massive black holes
376
00:19:03,409 --> 00:19:06,944
in a process called direct collapse.
377
00:19:06,946 --> 00:19:09,780
As they collapsed, they never even formed a star.
378
00:19:09,782 --> 00:19:12,783
They just collapsed straight into a giant black hole.
379
00:19:12,785 --> 00:19:14,351
Through this direct collapse theory,
380
00:19:14,353 --> 00:19:16,687
you can form really big black holes.
381
00:19:16,689 --> 00:19:19,189
Imagine what it's like seeing one of these giant clouds
382
00:19:19,191 --> 00:19:21,359
of gas collapsing down into a black hole.
383
00:19:21,361 --> 00:19:23,294
You might think you start with, okay,
384
00:19:23,296 --> 00:19:25,296
cloud of gas slowly collapsing,
385
00:19:25,298 --> 00:19:27,231
and, boop, it's a black hole.
386
00:19:27,233 --> 00:19:29,466
That wouldn't be the case. It would be more like
387
00:19:29,468 --> 00:19:31,702
giant cloud of gas starts collapsing,
388
00:19:31,704 --> 00:19:34,638
then ... aah! ... Black hole.
389
00:19:34,640 --> 00:19:36,707
It's believed that direct collapse
390
00:19:36,709 --> 00:19:38,609
could have created black holes
391
00:19:38,611 --> 00:19:41,412
up to a million times the mass of the sun,
392
00:19:41,414 --> 00:19:43,214
much bigger than from the collapse
393
00:19:43,216 --> 00:19:44,882
of a single star.
394
00:19:44,884 --> 00:19:46,317
Bullock: These early black holes
395
00:19:46,319 --> 00:19:48,619
are sort of like the galaxies that never were.
396
00:19:48,621 --> 00:19:50,054
They were gonna make galaxies.
397
00:19:50,056 --> 00:19:53,457
But instead, they collapsed into very massive black holes.
398
00:19:55,460 --> 00:19:58,094
For direct collapse to form a black hole,
399
00:19:58,096 --> 00:20:01,299
the conditions need to be precise.
400
00:20:01,301 --> 00:20:04,035
The clouds must be very symmetrical,
401
00:20:04,037 --> 00:20:06,571
forming a smooth ball.
402
00:20:06,573 --> 00:20:09,406
If you have a ball of gas that isn't quite a ball,
403
00:20:09,408 --> 00:20:11,175
that's not quite homogeneous,
404
00:20:11,177 --> 00:20:13,243
as it collapses, it'll fragment.
405
00:20:13,245 --> 00:20:15,613
And it'll fragment into objects that won't form black holes.
406
00:20:15,615 --> 00:20:18,249
So you want it to be hot enough
407
00:20:18,251 --> 00:20:22,119
that it stays one big, giant thing.
408
00:20:22,121 --> 00:20:23,954
But it does need to cool a little bit, right,
409
00:20:23,956 --> 00:20:26,824
so that you get it to collapse in on itself.
410
00:20:30,295 --> 00:20:34,064
You have to get uniform collapse over time
411
00:20:34,066 --> 00:20:37,401
of a very large amount of hydrogen gas, presumably,
412
00:20:37,403 --> 00:20:40,604
which is the original matter in the universe,
413
00:20:40,606 --> 00:20:43,907
collapsing spherically symmetrically,
414
00:20:43,909 --> 00:20:45,643
without fragmenting,
415
00:20:45,645 --> 00:20:49,380
over a period of less than 500 million years.
416
00:20:55,153 --> 00:20:57,622
Direct collapse may have created black holes
417
00:20:57,624 --> 00:21:00,224
a million times the mass of the sun.
418
00:21:00,226 --> 00:21:02,126
But it can't completely explain
419
00:21:02,128 --> 00:21:06,697
the 12 billion solar-mass supermassive black holes
420
00:21:06,699 --> 00:21:09,300
we see in the early universe.
421
00:21:09,302 --> 00:21:13,703
Maybe gigantic supermassive black holes were created
422
00:21:13,705 --> 00:21:16,774
by strange, unseen forces.
423
00:21:16,776 --> 00:21:18,675
Maybe they were created
424
00:21:18,677 --> 00:21:22,079
by the mysterious dark universe.
425
00:21:35,126 --> 00:21:39,229
Astronomers looking deep into the early universe
426
00:21:39,231 --> 00:21:43,868
have discovered gigantic supermassive black holes.
427
00:21:43,870 --> 00:21:45,602
Bullock: This is a pretty deep mystery.
428
00:21:45,604 --> 00:21:47,671
There are these supermassive black holes
429
00:21:47,673 --> 00:21:49,606
that exist in the very early universe.
430
00:21:49,608 --> 00:21:52,609
And by all accounts, they should not exist.
431
00:21:52,611 --> 00:21:55,312
According to the normal laws of physics,
432
00:21:55,314 --> 00:21:56,647
it shouldn't have been possible
433
00:21:56,649 --> 00:21:59,650
for them to grow so big so quickly.
434
00:21:59,652 --> 00:22:02,653
For astrophysicists, understanding how black holes
435
00:22:02,655 --> 00:22:06,023
have grown to be so large is one of our biggest mysteries.
436
00:22:06,025 --> 00:22:07,625
Bullock: We need some other way
437
00:22:07,627 --> 00:22:09,693
of growing these supermassive black holes.
438
00:22:09,695 --> 00:22:11,495
There needs to be some other mechanism
439
00:22:11,497 --> 00:22:14,030
that allows them to get that massive so early.
440
00:22:14,032 --> 00:22:16,433
But what is that?
441
00:22:16,435 --> 00:22:18,903
Everything we can see in the night sky
442
00:22:18,905 --> 00:22:21,371
makes up just 4.8%
443
00:22:21,373 --> 00:22:24,107
of all the matter in the cosmos.
444
00:22:24,109 --> 00:22:26,410
The rest is the dark universe,
445
00:22:26,412 --> 00:22:28,746
including dark matter.
446
00:22:28,748 --> 00:22:33,083
We can't see it, feel it, or detect it directly.
447
00:22:33,085 --> 00:22:35,753
But we know dark matter is there.
448
00:22:35,755 --> 00:22:39,456
Its gravity is tugging on everything around it.
449
00:22:39,458 --> 00:22:41,058
And we're beginning to understand
450
00:22:41,060 --> 00:22:43,160
it plays a fundamental role
451
00:22:43,162 --> 00:22:45,662
in the formation of the universe.
452
00:22:45,664 --> 00:22:47,965
Most of the stuff that collects together
453
00:22:47,967 --> 00:22:49,933
gravitationally is dark matter.
454
00:22:49,935 --> 00:22:52,736
So perhaps black holes form
455
00:22:52,738 --> 00:22:55,673
somehow with the inclusion of dark matter.
456
00:22:55,675 --> 00:22:57,508
One way of looking at it is there's six times
457
00:22:57,510 --> 00:22:59,110
as much dark matter as normal matter.
458
00:22:59,112 --> 00:23:01,712
So there's six times as much food out there
459
00:23:01,714 --> 00:23:03,047
for the black holes to eat
460
00:23:03,049 --> 00:23:05,850
if they're able to tap into this dark stuff.
461
00:23:05,852 --> 00:23:08,852
Maybe these supermassive black holes are growing
462
00:23:08,854 --> 00:23:11,021
by eating dark matter.
463
00:23:11,023 --> 00:23:13,891
There are some tantalizing clues.
464
00:23:13,893 --> 00:23:16,526
The largest supermassive black holes
465
00:23:16,528 --> 00:23:19,563
don't live in the galaxies with the most regular matter.
466
00:23:19,565 --> 00:23:23,366
They live in the galaxies with the most dark matter.
467
00:23:23,368 --> 00:23:26,136
The one thing we know about dark matter right now
468
00:23:26,138 --> 00:23:28,071
is that it has gravity.
469
00:23:28,073 --> 00:23:30,074
And a black hole runs on gravity.
470
00:23:30,076 --> 00:23:31,709
It attracts anything with mass.
471
00:23:31,711 --> 00:23:33,577
So there's no reason to assume
472
00:23:33,579 --> 00:23:35,912
that black holes would only eat regular matter.
473
00:23:35,914 --> 00:23:40,251
And now we know that there's far more dark matter out there.
474
00:23:40,253 --> 00:23:45,322
Maybe dark matter helps the black holes eat.
475
00:23:45,324 --> 00:23:47,825
Maybe in some ways, dark matter is a feeder
476
00:23:47,827 --> 00:23:50,161
for these supermassive black holes.
477
00:23:50,163 --> 00:23:53,063
Perhaps what really grows a supermassive black hole
478
00:23:53,065 --> 00:23:56,133
is all of the regular matter being directed into the center
479
00:23:56,135 --> 00:23:59,103
by the dark matter around it.
480
00:23:59,105 --> 00:24:02,106
Maybe the dark matter's powerful gravity
481
00:24:02,108 --> 00:24:03,908
sucks in regular matter
482
00:24:03,910 --> 00:24:07,511
and funnels it into the black hole.
483
00:24:07,513 --> 00:24:10,548
In a sense, the dark matter is greasing the wheels.
484
00:24:10,550 --> 00:24:12,282
It's sort of tilting the table up
485
00:24:12,284 --> 00:24:14,384
so that that food can slide right in.
486
00:24:18,124 --> 00:24:21,091
But now scientists think the dark matter
487
00:24:21,093 --> 00:24:25,028
may create gigantic black holes directly
488
00:24:25,030 --> 00:24:29,333
by igniting dark stars.
489
00:24:29,335 --> 00:24:30,968
Some believe that dark matter
490
00:24:30,970 --> 00:24:33,704
sparked early universe super stars.
491
00:24:33,706 --> 00:24:39,009
When they die, they leave behind supermassive black holes.
492
00:24:39,011 --> 00:24:40,511
Dark stars sound like
493
00:24:40,513 --> 00:24:42,546
they come from the fertile imagination
494
00:24:42,548 --> 00:24:44,615
of some Sci-Fi writer.
495
00:24:44,617 --> 00:24:47,684
But Dr. Katie freese believes they may explain
496
00:24:47,686 --> 00:24:53,056
how early supermassive black holes grew so fast.
497
00:24:53,058 --> 00:24:54,491
Dark stars are amazing.
498
00:24:54,493 --> 00:24:56,893
So, when we first had this idea,
499
00:24:56,895 --> 00:24:58,195
we got excited really quickly,
500
00:24:58,197 --> 00:25:00,464
because this is a new type of star
501
00:25:00,466 --> 00:25:03,667
that has never been seen before.
502
00:25:03,669 --> 00:25:06,437
Dark stars may have been some of the first stars
503
00:25:06,439 --> 00:25:08,672
to form in the universe.
504
00:25:08,674 --> 00:25:09,873
They sparked into life
505
00:25:09,875 --> 00:25:14,078
when the universe was just 200 million years old.
506
00:25:14,080 --> 00:25:19,616
But how could dark stars form really massive black holes?
507
00:25:19,618 --> 00:25:24,488
A newborn black hole can't weigh more than its parent star.
508
00:25:24,490 --> 00:25:28,792
So in order to give birth to a really massive black hole,
509
00:25:28,794 --> 00:25:33,297
the parent star has to be supermassive, as well.
510
00:25:33,299 --> 00:25:35,833
Freese: These early objects are really strange.
511
00:25:35,835 --> 00:25:38,001
They're very cool.
512
00:25:38,003 --> 00:25:40,437
And they're really, really big.
513
00:25:40,439 --> 00:25:43,874
The size of these things is 10 times the distance
514
00:25:43,876 --> 00:25:46,476
between the sun and the earth.
515
00:25:48,679 --> 00:25:51,215
But how is that possible?
516
00:25:51,217 --> 00:25:55,619
Regular stars have an upper size limit.
517
00:25:55,621 --> 00:25:59,389
A star is a battle between gravity pushing inwards
518
00:25:59,391 --> 00:26:01,725
and nuclear fusion pushing out.
519
00:26:05,162 --> 00:26:06,730
When the star grows too big,
520
00:26:06,732 --> 00:26:11,101
its gravity becomes overwhelming.
521
00:26:11,103 --> 00:26:12,703
The delicate balance
522
00:26:12,705 --> 00:26:16,640
between gravity and fusion is broken.
523
00:26:16,642 --> 00:26:21,544
Gravity wins out, and the star collapses.
524
00:26:21,546 --> 00:26:24,414
But dark stars may have a work-around
525
00:26:24,416 --> 00:26:28,686
that lets them become supermassive.
526
00:26:28,688 --> 00:26:30,654
Freese: So, they are made of ordinary matter.
527
00:26:30,656 --> 00:26:33,256
They're made of hydrogen and helium.
528
00:26:33,258 --> 00:26:36,226
But they're powered by dark matter.
529
00:26:36,228 --> 00:26:39,196
We don't know what dark matter is made from.
530
00:26:39,198 --> 00:26:44,301
But we do have theories on how it might power a star.
531
00:26:44,303 --> 00:26:46,903
Freese: One of the best ideas we have for dark matter
532
00:26:46,905 --> 00:26:50,908
is that it's made of weakly interacting massive particles,
533
00:26:50,910 --> 00:26:52,977
or wimps for short.
534
00:26:52,979 --> 00:26:55,378
So, these wimps are their own antimatter.
535
00:26:55,380 --> 00:26:57,915
And that means, whenever they encounter each other,
536
00:26:57,917 --> 00:27:01,818
they annihilate and turn into something else.
537
00:27:01,820 --> 00:27:04,621
That means a lot of heat is released, a lot of energy.
538
00:27:04,623 --> 00:27:07,958
And it's that energy that could power stars.
539
00:27:10,895 --> 00:27:13,364
The energy from the wimps' annihilations
540
00:27:13,366 --> 00:27:18,101
keeps the star from collapsing like a normal star.
541
00:27:18,103 --> 00:27:20,404
Bullock: So it's possible that, in some stars,
542
00:27:20,406 --> 00:27:22,205
their internal reactions
543
00:27:22,207 --> 00:27:25,242
are actually being powered by dark matter.
544
00:27:25,244 --> 00:27:28,144
If that's the case, then you could imagine situations
545
00:27:28,146 --> 00:27:29,646
where, when that burns out,
546
00:27:29,648 --> 00:27:32,616
you produce very massive black holes.
547
00:27:32,618 --> 00:27:34,251
So it could be that dark matter,
548
00:27:34,253 --> 00:27:35,652
the physics of dark matter,
549
00:27:35,654 --> 00:27:38,955
plays really important roles in creating black holes
550
00:27:38,957 --> 00:27:41,491
and their prevalence in the universe.
551
00:27:49,668 --> 00:27:51,935
The energy from the dark matter
552
00:27:51,937 --> 00:27:56,907
allows the dark stars to grow huge.
553
00:27:56,909 --> 00:27:58,575
When they first form, they're small.
554
00:27:58,577 --> 00:28:01,512
They're about the mass of the sun.
555
00:28:01,514 --> 00:28:03,546
But because they're so cool,
556
00:28:03,548 --> 00:28:04,848
they keep accumulating matter
557
00:28:04,850 --> 00:28:06,416
and growing, growing, growing.
558
00:28:06,418 --> 00:28:08,852
And some of them will get to be a million times
559
00:28:08,854 --> 00:28:13,356
as massive as the sun and a billion times as bright.
560
00:28:13,358 --> 00:28:15,893
But these giants don't live for long.
561
00:28:15,895 --> 00:28:18,294
Eventually, the dark matter particles
562
00:28:18,296 --> 00:28:20,698
wipe each other out completely.
563
00:28:20,700 --> 00:28:22,198
And there is no more fuel
564
00:28:22,200 --> 00:28:24,835
to keep the massive amount of ordinary matter
565
00:28:24,837 --> 00:28:27,371
from collapsing.
566
00:28:27,373 --> 00:28:28,806
And then that's it.
567
00:28:28,808 --> 00:28:31,442
There's nothing to sustain this big, puffy object.
568
00:28:31,444 --> 00:28:36,346
If it's big enough, you collapse directly to a black hole.
569
00:28:36,348 --> 00:28:40,951
A monster supermassive black hole.
570
00:28:40,953 --> 00:28:43,287
Bullock: It's really fun to think about the possibility
571
00:28:43,289 --> 00:28:44,755
that the physics of dark matter
572
00:28:44,757 --> 00:28:47,157
is actually helping to power stars.
573
00:28:47,159 --> 00:28:48,892
If so, it would bring, you know,
574
00:28:48,894 --> 00:28:51,328
a whole new window into our understanding
575
00:28:51,330 --> 00:28:53,597
of stars and their evolution.
576
00:28:56,134 --> 00:29:00,771
At the moment, dark stars are just theoretical.
577
00:29:00,773 --> 00:29:03,607
But when the powerful James webb telescope
578
00:29:03,609 --> 00:29:05,909
comes online in 2018,
579
00:29:05,911 --> 00:29:08,011
we may get our first glimpse.
580
00:29:09,914 --> 00:29:13,616
Freese: We're gonna do an observing run and look for these things.
581
00:29:13,618 --> 00:29:14,551
And so we're very excited.
582
00:29:14,553 --> 00:29:16,686
If you would find an entirely new type of star,
583
00:29:16,688 --> 00:29:19,923
that would be huge.
584
00:29:19,925 --> 00:29:22,459
While Katie freese looks for dark stars,
585
00:29:22,461 --> 00:29:26,196
another team is investigating another radical idea
586
00:29:26,198 --> 00:29:27,997
that offers new insight
587
00:29:27,999 --> 00:29:33,370
into how supermassive black holes grow so huge.
588
00:29:33,372 --> 00:29:35,705
They detect the faint echoes
589
00:29:35,707 --> 00:29:39,809
of a violent event from across the universe,
590
00:29:39,811 --> 00:29:43,280
the remnants of an extraordinary collision,
591
00:29:43,282 --> 00:29:45,215
a supremely energetic event
592
00:29:45,217 --> 00:29:49,486
that reveals black holes are cannibals.
593
00:30:04,102 --> 00:30:06,803
Our universe is filled with enormous
594
00:30:06,805 --> 00:30:11,508
supermassive black holes that defy explanation.
595
00:30:11,510 --> 00:30:13,443
Supermassive black holes are one of the things
596
00:30:13,445 --> 00:30:15,512
in the universe that, when you run the physics,
597
00:30:15,514 --> 00:30:17,780
when you run the math of how did they evolve,
598
00:30:17,782 --> 00:30:19,849
they really shouldn't be there.
599
00:30:19,851 --> 00:30:22,853
It's still a profound mystery.
600
00:30:22,855 --> 00:30:24,855
The universe hasn't been around long enough
601
00:30:24,857 --> 00:30:26,323
for regular black holes
602
00:30:26,325 --> 00:30:29,759
to eat enough matter to get supermassive.
603
00:30:29,761 --> 00:30:31,795
So how did they get so big?
604
00:30:31,797 --> 00:30:33,197
The most logical answer
605
00:30:33,199 --> 00:30:36,333
is that large black holes are born large,
606
00:30:36,335 --> 00:30:39,202
around 1 to 2 billion solar masses.
607
00:30:39,204 --> 00:30:41,771
But that's still over 10 times smaller
608
00:30:41,773 --> 00:30:46,242
than the largest supermassive black holes out there.
609
00:30:46,244 --> 00:30:48,311
Bullock: Given the time scales, it doesn't seem to add up.
610
00:30:48,313 --> 00:30:49,980
We need some other way
611
00:30:49,982 --> 00:30:52,081
to make these supermassive black holes.
612
00:30:52,083 --> 00:30:53,950
And the question is, what is that?
613
00:30:56,254 --> 00:30:59,790
A clue came from a large, isolated galaxy
614
00:30:59,792 --> 00:31:02,092
200 million light-years away
615
00:31:02,094 --> 00:31:04,394
in a quiet part of the universe.
616
00:31:06,331 --> 00:31:10,200
nestling alone was a supermassive black hole
617
00:31:10,202 --> 00:31:15,472
with a mass of 17 billion suns.
618
00:31:15,474 --> 00:31:17,073
Normally, such monsters
619
00:31:17,075 --> 00:31:19,943
are found in dense regions of space
620
00:31:19,945 --> 00:31:24,414
with lots of galaxies and lots of stars.
621
00:31:24,416 --> 00:31:26,883
This black holes doesn't match its surroundings at all.
622
00:31:26,885 --> 00:31:29,152
It's kind of like driving to the middle of a desert
623
00:31:29,154 --> 00:31:31,120
and coming across the empire state building.
624
00:31:31,122 --> 00:31:33,857
Now, the empire state building belongs in the middle of a city.
625
00:31:33,859 --> 00:31:35,425
And a black hole this big
626
00:31:35,427 --> 00:31:38,962
belongs in a rich cluster of galaxies.
627
00:31:38,964 --> 00:31:41,698
This is the first time astronomers have found
628
00:31:41,700 --> 00:31:43,300
such a giant object
629
00:31:43,302 --> 00:31:47,571
lurking in such a relatively empty area of the universe.
630
00:31:47,573 --> 00:31:48,872
So you got to ask the question,
631
00:31:48,874 --> 00:31:52,041
if there's nothing else around, how exactly do you grow
632
00:31:52,043 --> 00:31:54,611
a 17-billion-solar-mass black hole?
633
00:31:57,815 --> 00:32:01,351
One possible answer is the stuff of nightmares.
634
00:32:01,353 --> 00:32:03,353
Maybe the story of this black hole
635
00:32:03,355 --> 00:32:05,756
is actually a little more scary than we thought.
636
00:32:05,758 --> 00:32:06,956
Maybe it's all alone
637
00:32:06,958 --> 00:32:09,259
because it ate all of its neighbors.
638
00:32:11,662 --> 00:32:14,898
Maybe it was eating more than galaxies.
639
00:32:14,900 --> 00:32:18,301
Maybe it was eating its own kind.
640
00:32:20,204 --> 00:32:22,405
The thing about black holes is they're omnivores.
641
00:32:22,407 --> 00:32:23,673
They'll eat anything.
642
00:32:23,675 --> 00:32:26,243
Anything that gets close them, they'll gobble up.
643
00:32:26,245 --> 00:32:28,244
One way black holes can grow so large
644
00:32:28,246 --> 00:32:29,880
is by eating other black holes.
645
00:32:29,882 --> 00:32:32,716
So in a sense, they may be cannibals.
646
00:32:32,718 --> 00:32:36,219
Cannibal black holes were just theoretical.
647
00:32:36,221 --> 00:32:39,156
We'd never actually seen them eat each other.
648
00:32:41,325 --> 00:32:45,128
Then scientists detected the faint echoes
649
00:32:45,130 --> 00:32:48,732
of actual ripples in space-time.
650
00:32:48,734 --> 00:32:50,267
When engineers turned on
651
00:32:50,269 --> 00:32:54,537
the laser interferometer gravitational-wave observatory,
652
00:32:54,539 --> 00:32:56,573
or ligo for short,
653
00:32:56,575 --> 00:32:58,475
they immediately picked up
654
00:32:58,477 --> 00:33:02,345
the faint signal of gravitational waves.
655
00:33:02,347 --> 00:33:04,114
Gravitational waves are created
656
00:33:04,116 --> 00:33:06,950
by huge explosions in space.
657
00:33:10,187 --> 00:33:14,924
To make them, you need an almost unimaginably energetic event,
658
00:33:14,926 --> 00:33:17,661
something really, really big...
659
00:33:19,897 --> 00:33:24,000
...something like merging black holes.
660
00:33:26,003 --> 00:33:28,305
Bullock: A black hole merger is the most violent,
661
00:33:28,307 --> 00:33:29,606
the most energetic thing
662
00:33:29,608 --> 00:33:31,875
that happens in the universe, period.
663
00:33:34,745 --> 00:33:38,715
Picture the scene, 1.3 billion years ago.
664
00:33:38,717 --> 00:33:42,819
Two black holes circle each other in a dance of death.
665
00:33:42,821 --> 00:33:46,622
The larger black hole pulls the smaller one inwards
666
00:33:46,624 --> 00:33:50,093
until they're locked together in a spiral.
667
00:33:50,095 --> 00:33:52,562
Very, very slowly, that orbit is decaying.
668
00:33:52,564 --> 00:33:54,664
They're getting closer and closer and closer.
669
00:33:54,666 --> 00:33:58,101
And then they will merge into one giant black hole,
670
00:33:58,103 --> 00:34:01,971
truly one of the most dramatic events in the universe.
671
00:34:01,973 --> 00:34:04,074
Finally, they collide
672
00:34:04,076 --> 00:34:07,844
in one of the largest bangs since the big bang.
673
00:34:11,082 --> 00:34:13,016
I would have loved to have been able
674
00:34:13,018 --> 00:34:14,818
to safely view the collision
675
00:34:14,820 --> 00:34:16,953
of these two black holes up close.
676
00:34:16,955 --> 00:34:18,255
Imagine these two black holes
677
00:34:18,257 --> 00:34:20,123
as they spiral in toward each other,
678
00:34:20,125 --> 00:34:22,358
going faster and faster and faster and faster.
679
00:34:22,360 --> 00:34:24,928
And then, suddenly, where there appears to be nothing
680
00:34:24,930 --> 00:34:27,430
or just distortions in space in front of you,
681
00:34:27,432 --> 00:34:30,700
suddenly, there is this enormous burst of energy.
682
00:34:30,702 --> 00:34:33,870
And everything just rains around you.
683
00:34:33,872 --> 00:34:37,274
By measuring the frequency of the gravitational waves,
684
00:34:37,276 --> 00:34:41,544
we can calculate the size of the objects causing them.
685
00:34:41,546 --> 00:34:43,313
When those two black holes,
686
00:34:43,315 --> 00:34:45,881
weighing 29 solar masses
687
00:34:45,883 --> 00:34:49,652
and 36 solar masses, collided,
688
00:34:49,654 --> 00:34:53,757
they created a black hole around twice the size.
689
00:34:55,793 --> 00:34:58,327
In some ways, it's very elegant and simple.
690
00:34:58,329 --> 00:35:00,596
You take two black holes. You spiral them in together.
691
00:35:00,598 --> 00:35:03,567
And you end up with one big black hole.
692
00:35:05,702 --> 00:35:09,172
The event showed that black holes can double their mass
693
00:35:09,174 --> 00:35:12,875
through cannibalism...Almost.
694
00:35:12,877 --> 00:35:17,580
The final black hole was less than the sum of its parts.
695
00:35:17,582 --> 00:35:20,883
There were 3 solar masses missing.
696
00:35:20,885 --> 00:35:23,086
That may not sound like a lot.
697
00:35:23,088 --> 00:35:25,621
So let's put it in context.
698
00:35:25,623 --> 00:35:27,890
Our sun is burning
699
00:35:27,892 --> 00:35:30,827
about 100 billion hydrogen bombs every second.
700
00:35:30,829 --> 00:35:32,829
And over its 10-billion-year lifetime,
701
00:35:32,831 --> 00:35:35,298
it will convert less than maybe 1% of the mass
702
00:35:35,300 --> 00:35:36,500
of the sun to energy.
703
00:35:36,502 --> 00:35:38,702
In 2/10 of a second,
704
00:35:38,704 --> 00:35:41,505
3 times the mass of the sun in matter
705
00:35:41,507 --> 00:35:44,173
got converted to energy in that collision.
706
00:35:46,110 --> 00:35:50,046
It was 36 septillion yottawatts.
707
00:35:50,048 --> 00:35:52,616
What does that mean? A lot of freaking energy.
708
00:35:52,618 --> 00:35:55,851
That's more energy in that 2/10 of a second
709
00:35:55,853 --> 00:35:57,987
than is emitted by all the stars
710
00:35:57,989 --> 00:36:00,122
in the visible universe in the same time.
711
00:36:02,693 --> 00:36:06,095
In its first run, ligo detected two collisions.
712
00:36:08,232 --> 00:36:10,333
This suggests that cannibal black holes
713
00:36:10,335 --> 00:36:12,035
are relatively common
714
00:36:12,037 --> 00:36:16,206
and that each feast builds a larger black hole.
715
00:36:16,208 --> 00:36:18,541
But so far, the largest black hole
716
00:36:18,543 --> 00:36:20,343
these mergers have produced
717
00:36:20,345 --> 00:36:22,812
is 62 solar masses,
718
00:36:22,814 --> 00:36:28,018
not close to the largest supermassives we've found.
719
00:36:28,020 --> 00:36:30,220
It's hard to imagine, in 13.8 billion years,
720
00:36:30,222 --> 00:36:33,122
that there'd be enough collisions of 30-solar-mass
721
00:36:33,124 --> 00:36:37,460
black holes to build up to form a billion-solar-mass black hole.
722
00:36:37,462 --> 00:36:40,430
That's 100 million collisions.
723
00:36:40,432 --> 00:36:44,067
So maybe small black holes eating each other
724
00:36:44,069 --> 00:36:45,668
isn't the solution.
725
00:36:45,670 --> 00:36:48,905
Maybe supermassive black holes
726
00:36:48,907 --> 00:36:51,841
are eating each other.
727
00:36:51,843 --> 00:36:54,677
If so, could the supermassive black hole
728
00:36:54,679 --> 00:36:58,948
at the heart of our own galaxy be on the menu?
729
00:37:13,697 --> 00:37:16,132
We've found supermassive black holes
730
00:37:16,134 --> 00:37:19,969
so large, they defy explanation.
731
00:37:19,971 --> 00:37:21,371
They're too big to have grown
732
00:37:21,373 --> 00:37:25,642
by simply eating the matter around them.
733
00:37:25,644 --> 00:37:29,178
They can't form the same way that regular black holes do.
734
00:37:29,180 --> 00:37:31,848
There must be something else that happens that lets them grow
735
00:37:31,850 --> 00:37:34,684
to such enormous mass.
736
00:37:34,686 --> 00:37:37,553
Too large to have grown from dark stars
737
00:37:37,555 --> 00:37:41,391
and too big to have grown from regular black holes
738
00:37:41,393 --> 00:37:43,727
simply eating each other.
739
00:37:43,729 --> 00:37:46,129
Merging black holes almost certainly play a role
740
00:37:46,131 --> 00:37:48,965
in our understanding of supermassive black holes.
741
00:37:48,967 --> 00:37:52,201
We think that supermassive black holes themselves also merge
742
00:37:52,203 --> 00:37:55,271
and have merged regularly over the course of the universe.
743
00:37:55,273 --> 00:37:57,240
Now, whether this merging activity itself
744
00:37:57,242 --> 00:37:59,342
is enough to make them that big,
745
00:37:59,344 --> 00:38:01,811
the jury is still out on that.
746
00:38:01,813 --> 00:38:04,948
Now a newly discovered type of galaxy
747
00:38:04,950 --> 00:38:07,317
may provide an answer.
748
00:38:07,319 --> 00:38:13,189
It's called w2246-0526.
749
00:38:13,191 --> 00:38:14,724
And we can't see it.
750
00:38:14,726 --> 00:38:18,294
But we can detect the heat it gives off.
751
00:38:18,296 --> 00:38:20,429
This galaxy is an example
752
00:38:20,431 --> 00:38:24,501
of a rare class of objects called hot dogs.
753
00:38:24,503 --> 00:38:27,237
One of the funnier terms for an exotic type of galaxy
754
00:38:27,239 --> 00:38:28,838
is a hot dog galaxy.
755
00:38:28,840 --> 00:38:31,074
And no, this is not some delicious sausage snack.
756
00:38:31,076 --> 00:38:35,412
In fact, it means "hot, dust-obscured galaxy."
757
00:38:35,414 --> 00:38:37,980
It's called obscured because it's shrouded
758
00:38:37,982 --> 00:38:42,218
in so much dust and gas, the only light that escapes
759
00:38:42,220 --> 00:38:46,822
is infrared in the form of heat.
760
00:38:46,824 --> 00:38:48,691
All this heat must be coming from somewhere.
761
00:38:48,693 --> 00:38:51,494
So in the core, there is a cauldron,
762
00:38:51,496 --> 00:38:53,430
a seething supermassive black hole,
763
00:38:53,432 --> 00:38:55,298
the likes of which we can't even imagine.
764
00:38:58,470 --> 00:39:00,670
of all the supermassive black holes we know of,
765
00:39:00,672 --> 00:39:03,106
the ones that are obscured in these hot dog galaxies
766
00:39:03,108 --> 00:39:05,207
may be the ones that are the most ravenous,
767
00:39:05,209 --> 00:39:06,810
consuming many millions of times
768
00:39:06,812 --> 00:39:09,812
the mass of the sun.
769
00:39:09,814 --> 00:39:12,214
Scientists theorize that hot dogs
770
00:39:12,216 --> 00:39:14,450
could be the offspring
771
00:39:14,452 --> 00:39:18,020
of cannibal giant black holes.
772
00:39:18,022 --> 00:39:20,122
When the monstrous black holes merge,
773
00:39:20,124 --> 00:39:23,126
they drag gas and dust with them.
774
00:39:23,128 --> 00:39:25,695
This brings more food to the table,
775
00:39:25,697 --> 00:39:29,665
allowing the new black hole to gorge itself.
776
00:39:29,667 --> 00:39:32,369
When you have these two galaxies merging,
777
00:39:32,371 --> 00:39:35,271
they have all-new food.
778
00:39:35,273 --> 00:39:36,372
It's a brand-new dinner plate,
779
00:39:36,374 --> 00:39:40,310
a brand-new buffet of food to eat.
780
00:39:40,312 --> 00:39:43,546
The combination of cannibalism and fresh food
781
00:39:43,548 --> 00:39:46,649
allows the black holes to grow super large.
782
00:39:49,186 --> 00:39:52,222
Perhaps this is how the supermassive black hole
783
00:39:52,224 --> 00:39:53,956
at the center of our galaxy
784
00:39:53,958 --> 00:39:56,626
grew when it was young.
785
00:39:56,628 --> 00:39:58,228
But what's the future
786
00:39:58,230 --> 00:40:03,032
of our supermassive sagittarius "a"-star?
787
00:40:03,034 --> 00:40:05,101
As far as supermassive black holes go,
788
00:40:05,103 --> 00:40:06,335
sagittarius "a"-star
789
00:40:06,337 --> 00:40:08,404
is actually still kind of in the minor leagues.
790
00:40:08,406 --> 00:40:10,773
It's small. But it's not done yet.
791
00:40:10,775 --> 00:40:14,777
It's still eating. It's still growing.
792
00:40:14,779 --> 00:40:17,046
And in around 4 billion years,
793
00:40:17,048 --> 00:40:21,951
it's going to become 25 times larger,
794
00:40:21,953 --> 00:40:25,888
because it's going to be eaten by its neighbor.
795
00:40:30,761 --> 00:40:34,396
The giant Andromeda galaxy is heading our way.
796
00:40:34,398 --> 00:40:37,834
And it's going to engulf our milky way.
797
00:40:37,836 --> 00:40:39,302
When galaxies merge,
798
00:40:39,304 --> 00:40:43,405
their central supermassive black holes merge.
799
00:40:43,407 --> 00:40:46,476
Andromeda's huge supermassive black hole
800
00:40:46,478 --> 00:40:50,013
will drag sagittarius "a"-star into orbit...
801
00:40:52,216 --> 00:40:56,085
...gradually drawing it closer and closer
802
00:40:56,087 --> 00:40:57,720
until it devours it.
803
00:41:00,791 --> 00:41:03,125
The new supermassive black hole will weigh
804
00:41:03,127 --> 00:41:06,729
around 100 million solar masses.
805
00:41:06,731 --> 00:41:09,198
But the disruption to the new galaxy
806
00:41:09,200 --> 00:41:12,535
will provide the new supermassive black hole
807
00:41:12,537 --> 00:41:13,836
with plenty to eat
808
00:41:13,838 --> 00:41:17,440
and the opportunity to grow a whole lot bigger.
809
00:41:20,110 --> 00:41:22,145
At present, there are many theories
810
00:41:22,147 --> 00:41:26,349
of how supermassive black holes get so big.
811
00:41:26,351 --> 00:41:30,086
Most likely, it's a combination of them all.
812
00:41:30,088 --> 00:41:34,224
But however it happens, we can be pretty sure
813
00:41:34,226 --> 00:41:38,828
it's one of the most spectacular things in the universe.
814
00:41:38,830 --> 00:41:40,930
The jury's still out on exactly
815
00:41:40,932 --> 00:41:44,033
how supermassive black holes become so massive.
816
00:41:47,372 --> 00:41:49,071
making all the black holes we see
817
00:41:49,073 --> 00:41:51,941
probably requires a pretty diverse cookbook.
818
00:41:51,943 --> 00:41:54,244
So any physicist who's looking for a really simple,
819
00:41:54,246 --> 00:41:56,479
single answer for how they get made,
820
00:41:56,481 --> 00:41:59,849
they're probably gonna be disappointed.
821
00:41:59,851 --> 00:42:02,785
It's probably a pretty complex thing that's going on.
822
00:42:06,557 --> 00:42:09,792
It could be through eating. It could be through merging.
823
00:42:09,794 --> 00:42:11,127
It could be through eating and merging.
824
00:42:11,129 --> 00:42:13,596
And usually, the answer is somewhere in the middle.
825
00:42:13,598 --> 00:42:15,932
So they will merge with other black holes.
826
00:42:15,934 --> 00:42:19,235
And they'll also have a few snacks between mergers.
64206
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