WEBVTT - Black Holes, Part 2: Detection

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<v Speaker 1>My welcome to Stuff to Blow Your Mind from how

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<v Speaker 1>Stuff Works dot com. Hey you welcome to Stuff to

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<v Speaker 1>Blow your Mind. My name is Robert Lamb and I'm

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<v Speaker 1>Joe McCormick, and we're back. It's part two of our

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<v Speaker 1>multi part exploration of black holes. Because you know what,

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<v Speaker 1>this year Robert went to the World Science Festival in

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<v Speaker 1>New York and came back with black Hole Fever. Yeah.

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<v Speaker 1>It was a great It was a great talk that

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<v Speaker 1>really opened my eyes a little more to some of

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<v Speaker 1>the finer details of of black holes. And you mean

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<v Speaker 1>that Brian Green talk with the guests. Yeah, Darkness made visible,

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<v Speaker 1>wonderful talk. It's available online. Will include a link to

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<v Speaker 1>that in the landing page for this episode. Certainly inspired

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<v Speaker 1>us to to really give black holes a proper shake

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<v Speaker 1>on Stuff to Blow your Mind. Yeah, I mean, there's

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<v Speaker 1>so much interesting stuff to talk about, and the fact

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<v Speaker 1>that they're just one of the most interesting objects in

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<v Speaker 1>the entire universe. It's not that they're probably I would say,

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<v Speaker 1>maybe the most interesting non living thing in the universe.

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<v Speaker 1>What do you think about that? Yeah, yeah, I would

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<v Speaker 1>say that because we're pretty interesting ultimately humans are. Um.

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<v Speaker 1>I do want to remind everyone. If you did not

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<v Speaker 1>listen to the previous episode on black holes, you do

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<v Speaker 1>want to go back and listen to it, because this

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<v Speaker 1>is this is not one of those where you can

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<v Speaker 1>kind of take part one and part two in any order.

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<v Speaker 1>You really need to hit the first episode. I mean,

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<v Speaker 1>you could if you really wanted, But we're going to

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<v Speaker 1>be referring back to the groundwork we laid in the

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<v Speaker 1>previous episode. And the previous episode we talked a lot

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<v Speaker 1>about the development of black holes. Uh, sort of as

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<v Speaker 1>the history of an idea, something that was unlike the

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<v Speaker 1>stars in the sky. You know, the stars in the sky,

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<v Speaker 1>we first observed and we could see them, and then

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<v Speaker 1>by making observations about them, we were able to come

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<v Speaker 1>up with theories to explain them. Black holes weren't like that.

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<v Speaker 1>It went the other way around. Black Holes existed in

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<v Speaker 1>theory long before anybody accepted that they existed in reality,

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<v Speaker 1>and long after they existed in theory, many scientists ardently

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<v Speaker 1>opposed the idea that black holes could exist in nature. Yeah,

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<v Speaker 1>it's the idea that that these various individuals said, well, X, Y,

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<v Speaker 1>and Z are true, then this thing might exist and uh,

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<v Speaker 1>and and that thing is the black hole. But of course,

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<v Speaker 1>you know, lots of people when a thing sounds outlandish,

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<v Speaker 1>even if your best theories tell you it might be possible,

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<v Speaker 1>people want to find a way to say, no, that

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<v Speaker 1>just sounds unintuitive. It couldn't be real. It doesn't fit

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<v Speaker 1>my picture of how the universe works. It doesn't feel right. Yeah,

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<v Speaker 1>maybe that's a thought experiment, but I doubt will actually

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<v Speaker 1>find something like this when we start looking out into

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<v Speaker 1>the cosmos with better observational technology. You know, it's often

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<v Speaker 1>said that Albert Einstein did some of his worst work ever,

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<v Speaker 1>Like the worst science of his entire career was him

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<v Speaker 1>trying to write papers to prove that black holes didn't

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<v Speaker 1>exist in reality. It just didn't seem right to him,

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<v Speaker 1>even though his general relativity became the basis of our

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<v Speaker 1>modern theory of black holes. But so anyway, yeah, so

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<v Speaker 1>how did today? We want to explore making the darkness flesh,

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<v Speaker 1>making the black hole into a thing that is real

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<v Speaker 1>in existence in the universe and we can detect it.

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<v Speaker 1>So I think first we want to tell the story

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<v Speaker 1>of sort of like a bridging the gap between the

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<v Speaker 1>black holes of general relativity theory and the actual observations

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<v Speaker 1>of them and then talk a little bit about what's

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<v Speaker 1>it like to detect black holes and how we might

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<v Speaker 1>do it. And we do have to distress that in

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<v Speaker 1>today's world, black holes are pretty much an established reality.

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<v Speaker 1>You talk to experts and they say yes, without a

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<v Speaker 1>shadow of a doubt. Yeah. I don't know if it's

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<v Speaker 1>the case that every single expert would say without a

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<v Speaker 1>shadow of a doubt, but yeah, they're They're generally accepted

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<v Speaker 1>as a fact of reality. You know, we've reached the

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<v Speaker 1>point where black holes exist and they're completely non politicized.

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<v Speaker 1>That's the other great Yeah, oh man, I love a

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<v Speaker 1>scientific controversy that doesn't never have a political angle. Yeah,

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<v Speaker 1>it's the black holes are are. Thus far, they've remained

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<v Speaker 1>pretty safe. Well, maybe we can muck it up today.

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<v Speaker 1>Let's let's get people taking tribal sides on it. Okay,

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<v Speaker 1>So the story of how black holes went from this

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<v Speaker 1>theoretical anomaly to a thing known to exist in the world,

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<v Speaker 1>it's a long, complicated story, so we definitely can't explore

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<v Speaker 1>all of it, but I just want to mention a

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<v Speaker 1>few highlights, and one of the first ones is serious

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<v Speaker 1>b Now, Serious is the brightest star in the night.

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<v Speaker 1>Sky from Earth, often known as the Dog Star because

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<v Speaker 1>it's part of the Cannus Major constellation, the Great Dog constellation.

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<v Speaker 1>Side note, I didn't know this until I was reading

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<v Speaker 1>this the other day. Do you know the origin of

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<v Speaker 1>the term dog days of summer doesn't actually have anything

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<v Speaker 1>to do with the behavior of dogs. Really. I always

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<v Speaker 1>thought it came from a Don Henley song. Wait, one

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<v Speaker 1>of the Boys of Summer. Sorry, after the dog Days

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<v Speaker 1>of Summer have gone. Yeah, man, I grew so hard

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<v Speaker 1>whenever that song comes on the radios. It's a great

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<v Speaker 1>it's a great track. I love it. It's yacht rock

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<v Speaker 1>that touches my heart. Yeah. So the term dog days

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<v Speaker 1>of Summer actually refers to the period of Serious, the

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<v Speaker 1>star in the Cannus Major constellation, rising roughly in conjunction

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<v Speaker 1>with the Sun, which happens in July through August in

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<v Speaker 1>the Northern Hemisphere, and so this is also the hottest

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<v Speaker 1>time of the summer, and so it came to be

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<v Speaker 1>associated with Okay, so Serious is coming up with the

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<v Speaker 1>sun in the morning, and that means it's going to

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<v Speaker 1>be real hot out. But back in the eighteen hundreds,

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<v Speaker 1>it had been observed that the extremely bright star we

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<v Speaker 1>now call Serious A behaved oddly. Its motion was not

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<v Speaker 1>it was it was not smooth. It was kind of wobbly,

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<v Speaker 1>as if it were being destabilized and tugged on by

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<v Speaker 1>an invisible hand. And it turned out that Serious A

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<v Speaker 1>actually had a very dim companion star. It was a

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<v Speaker 1>binary star system, and the companion was what we now

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<v Speaker 1>call Serious B. But it was a very strange type

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<v Speaker 1>of companion because based on the motion of the two

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<v Speaker 1>bodies and the light they produced, astrophysicists could calculate that

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<v Speaker 1>the companion of Sirius at the same time was somewhere

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<v Speaker 1>around the mass of our Sun, and yet was barely

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<v Speaker 1>larger than the size of planet Earth and burning extremely hot,

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<v Speaker 1>much hotter than the Sun. So Serious Be turned out

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<v Speaker 1>to be an early example of what would later be

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<v Speaker 1>called a white dwarf, a tiny, hot, massive star that

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<v Speaker 1>proved matter could be compressed to pressures previously thought absolutely impossible.

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<v Speaker 1>In the words of Arthur Eddington, quote a ton, and

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<v Speaker 1>he's talking about the the material making up the star.

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<v Speaker 1>A ton of this material would be a little nugget

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<v Speaker 1>that you could put in a matchbox. So imagine something

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<v Speaker 1>matchbox size. But that weighs a ton, and so for many,

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<v Speaker 1>including Eddington, the very concept of this density was so

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<v Speaker 1>absurd that it should just basically cause us to dismiss

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<v Speaker 1>the observations out of hand, dismiss the idea of a

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<v Speaker 1>white dwarf. It's absurd, but reality is stranger than our imagination.

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<v Speaker 1>White dwarves came to be accepted as a feature of

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<v Speaker 1>the universe and a part of ller revolution, especially after

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<v Speaker 1>quantum mechanics eventually came along. To explain how matter could

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<v Speaker 1>be compressed to such an unbelievable density. Basically has to

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<v Speaker 1>do with packing atomic nuclei tighter and tighter, and you

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<v Speaker 1>can actually do this to some extent because most of

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<v Speaker 1>an adam is empty space. There's a good explanation of

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<v Speaker 1>this actually in a book that's one of our sources

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<v Speaker 1>on this episode, Black Hole, by Marcia Bartousciak, which I

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<v Speaker 1>thought I should mention again, which is a good good

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<v Speaker 1>book if you want to go in more depth than

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<v Speaker 1>we're going into here. But so with serious b you've

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<v Speaker 1>got these white dwarves, You've got these objects that are

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<v Speaker 1>observed to be tiny and very hot and very bright

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<v Speaker 1>and very massive, and so what would be the limits

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<v Speaker 1>on what a star like that could be like uh

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<v Speaker 1>In nineteen thirty, the young Indian astrophysicist Supermania and Chandra

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<v Speaker 1>Sheker calculated that there was an upper limit to the

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<v Speaker 1>mass of a white dwarf. White dwarves could vary in size,

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<v Speaker 1>but somewhere around one point four solar masses. If a

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<v Speaker 1>white dwarf is about one point four times the mass

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<v Speaker 1>of our Sun, something happens. This is now known as

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<v Speaker 1>the chander Shaker limit, and it around this mass, the

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<v Speaker 1>force of gravity chander Shaker calculated appears to become more

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<v Speaker 1>powerful than the force that's known as the electron degeneracy pressure.

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<v Speaker 1>And what that is is it just causes atoms to

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<v Speaker 1>push against one another and resist compression. So why can't

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<v Speaker 1>you keep compressing it down more and more? There's this

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<v Speaker 1>electron degeneracy pressure pushing back, but at a certain point, gravity,

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<v Speaker 1>at least on paper, appears to completely overwhelm this degeneracy

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<v Speaker 1>pressure and just crush everything down. So any clump of

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<v Speaker 1>white dwarf stellar matter more massive than this could not

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<v Speaker 1>maintain the white dwarf density at a stable pressure given

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<v Speaker 1>the laws of general relativity. Past this point of star's

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<v Speaker 1>density would just not scale up regularly, but would collapse,

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<v Speaker 1>and it would collapse toward infinity. But when you think

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<v Speaker 1>about that, like try to imagine your in Chonder Shaker's

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<v Speaker 1>position infinite density, what does it mean to collapse to

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<v Speaker 1>infinite density? You'd almost be tempted to think, Okay, well

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<v Speaker 1>I made a mistake. Yeah. It's like it's like suddenly

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<v Speaker 1>everything is reduced to zero and you know that the

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<v Speaker 1>equation must be flowed. Yeah, it's like you've you've hit

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<v Speaker 1>a divide by zero area or something. You you know

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<v Speaker 1>that you must have done something wrong. It was difficult

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<v Speaker 1>to believe that something like this could be possible in reality.

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<v Speaker 1>How could a real physical object collapse toward a point

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<v Speaker 1>of infinite density? Though this is what the math appeared

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<v Speaker 1>to show. But Chonder Shaker did not actually argue about

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<v Speaker 1>what physically happened to the white dwarf past the limit

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<v Speaker 1>that he had established, only that the limit of stability

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<v Speaker 1>at about one point four solar masses existed, and Chandra

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<v Speaker 1>Shaker spent years arguing against the grain of scholarship on

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<v Speaker 1>this point. There's a famous story about how when he

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<v Speaker 1>presented his findings at a meeting of the Royal last

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<v Speaker 1>Atronomical Society of London and nineteen thirty five our old

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<v Speaker 1>friend Arthur Eddington's uh. He supposedly exclaimed there should be

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<v Speaker 1>a law of nature to prevent a star from behaving

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<v Speaker 1>in this absurd way. That's some wicked cantankerousness, just like

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<v Speaker 1>yelling at the laws of physics. But but no, I

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<v Speaker 1>mean so, that kind of attitude from Eddington actually kept

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<v Speaker 1>this idea down for a long time, even though we

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<v Speaker 1>would eventually find out that chander Shaker was on the

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<v Speaker 1>right side of this argument, and the prolific Soviet physicist

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<v Speaker 1>live Landau also made a similar calculation around this point,

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<v Speaker 1>and he also arrived at the conclusion that a heavy

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<v Speaker 1>enough star could collapse to what appears to be a point.

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<v Speaker 1>But he said, that can't be quite right, so he

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<v Speaker 1>ignored this result and instead concluded that the core of

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<v Speaker 1>a star like this that at the core of a

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<v Speaker 1>star like this, matter sort of begins to ignore the

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<v Speaker 1>laws of physics and becomes quote, one gigantic nucleus. Now,

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<v Speaker 1>chander Shaker was eventually recognized for being in the right

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<v Speaker 1>on this question. He see the Nobel Prize in Physics

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<v Speaker 1>for his work on stellar evolution, and he got that

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<v Speaker 1>in nineteen eighty three. Now, also in the nineteen thirties,

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<v Speaker 1>a parallel idea to the idea of the black hole emerges,

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<v Speaker 1>and that is the idea of a neutron star. Now,

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<v Speaker 1>a neutron star is another form that stellar collapse can take,

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<v Speaker 1>in which you've got protons and electrons that form the

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<v Speaker 1>core of a star and they compressed together with such

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<v Speaker 1>force that they combine and form neutrons, which have mass

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<v Speaker 1>but no electric charge. And a neutron star is not

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<v Speaker 1>as a reality warping as a black hole, but it

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<v Speaker 1>is an unbelievably exotic type of object composed matter so

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<v Speaker 1>dense that it's been compared to an atomic nucleus the

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<v Speaker 1>size of a city. If you can picture that, Uh,

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<v Speaker 1>can you picture that? Of course you can't, nobody can,

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<v Speaker 1>but just just try. I can picture an illustration that

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<v Speaker 1>was presented of this. That's that's the best I can do. Well.

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<v Speaker 1>I mean, part of the problem is that matter already

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<v Speaker 1>looks solid enough to us, right, I mean, you take

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<v Speaker 1>a rock or something like that, You're like, this looks

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<v Speaker 1>really really solid, but most of it is empty space.

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<v Speaker 1>Most of it is just the space between the atomic

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<v Speaker 1>nuclei and the electrons orbiting them, and the other atomic

0:12:14.320 --> 0:12:18.160
<v Speaker 1>nuclei that they're bonded with. Um. I mean, the molecules

0:12:18.320 --> 0:12:22.120
<v Speaker 1>that make that very solid seeming object are mostly empty space,

0:12:22.400 --> 0:12:24.920
<v Speaker 1>and there's a lot of space you can press things

0:12:25.040 --> 0:12:28.719
<v Speaker 1>further and further into if you really must. You may

0:12:28.720 --> 0:12:30.360
<v Speaker 1>not be able to get blood from a stone, but

0:12:30.440 --> 0:12:32.920
<v Speaker 1>there's a lot of empty space there. If empty space

0:12:32.960 --> 0:12:34.920
<v Speaker 1>is when you're after, it's there, you can get space

0:12:34.960 --> 0:12:38.120
<v Speaker 1>from a stone. So, just to show how much things

0:12:38.160 --> 0:12:40.480
<v Speaker 1>can be compressed, it's often said that, like a square

0:12:40.600 --> 0:12:44.120
<v Speaker 1>centimeter of a neutron star, material might weigh more than

0:12:44.160 --> 0:12:48.680
<v Speaker 1>a billion tons. Uh So. In the late nineteen thirties, J.

0:12:48.840 --> 0:12:52.959
<v Speaker 1>Robert Oppenheimer, who's famous for working on the Manhattan Project,

0:12:53.000 --> 0:12:56.760
<v Speaker 1>among many things. Oppenheimer and some students of his published

0:12:56.800 --> 0:13:00.160
<v Speaker 1>work tending in the same direction as Chandra shako Are.

0:13:00.160 --> 0:13:03.520
<v Speaker 1>Oppenheimer and George Volkoff did work on the emerging idea

0:13:03.520 --> 0:13:05.960
<v Speaker 1>of neutron stars, which we were just talking about, and

0:13:05.960 --> 0:13:09.319
<v Speaker 1>found that neutron stars, like white dwarves, had an upper

0:13:09.440 --> 0:13:13.040
<v Speaker 1>limit of mass, after which something very strange seems to

0:13:13.120 --> 0:13:15.679
<v Speaker 1>happen to them. You've got this upper limit, and if

0:13:15.720 --> 0:13:18.920
<v Speaker 1>they have more mass than this limit, there's some kind

0:13:18.920 --> 0:13:23.599
<v Speaker 1>of collapse, something, something goes wrong with the physics. Oppenheimer

0:13:23.640 --> 0:13:26.960
<v Speaker 1>also published a paper on stellar evolution with Heartland Snyder

0:13:27.320 --> 0:13:30.640
<v Speaker 1>in which they determined that late stage stellar remnants of

0:13:30.679 --> 0:13:33.920
<v Speaker 1>stars passed a certain mass would seem to enter this

0:13:34.000 --> 0:13:37.960
<v Speaker 1>state of permanent infinite collapse. The matter within them would

0:13:37.960 --> 0:13:40.880
<v Speaker 1>exist in this perpetual free fall towards a point of

0:13:40.960 --> 0:13:44.520
<v Speaker 1>infinite density, the singularity. And that is a that is

0:13:44.559 --> 0:13:48.840
<v Speaker 1>a mind boggling concept to toy around with, falling forever.

0:13:49.880 --> 0:13:53.240
<v Speaker 1>The never ending pit essentially, which was it was something

0:13:53.240 --> 0:13:54.960
<v Speaker 1>like as a kid, you, or at least when I

0:13:55.000 --> 0:13:56.800
<v Speaker 1>was a kid, that's what we played instead of the

0:13:56.800 --> 0:13:58.520
<v Speaker 1>floor is lava. Always said the floor is an never

0:13:58.640 --> 0:14:01.439
<v Speaker 1>ending pit. That's more than lava. Yeah. I think it's

0:14:01.440 --> 0:14:04.400
<v Speaker 1>because we saw it on like key Man cartoons or something.

0:14:04.440 --> 0:14:07.319
<v Speaker 1>I feel like it isn't that what's underneath Castle Gray

0:14:07.320 --> 0:14:09.839
<v Speaker 1>Skull and never ending pit? I don't remember it is

0:14:09.880 --> 0:14:12.440
<v Speaker 1>in my mind. Well, then what's Castle gray Skull built on.

0:14:13.280 --> 0:14:15.360
<v Speaker 1>It's built over and never ending. I see it's called

0:14:15.360 --> 0:14:17.360
<v Speaker 1>a strut since yeah, yeah, I guess they had to

0:14:17.400 --> 0:14:20.120
<v Speaker 1>cap that thing, you know up, They're like, don't people

0:14:20.160 --> 0:14:21.920
<v Speaker 1>gonna fall into that, Let's put a castle on top

0:14:21.960 --> 0:14:25.000
<v Speaker 1>of it. So it's playing fast and loose with masters

0:14:25.000 --> 0:14:27.720
<v Speaker 1>of the universe. Um myth those here. By the way,

0:14:27.760 --> 0:14:29.960
<v Speaker 1>I apologize for just trying to move us along. I

0:14:29.960 --> 0:14:34.479
<v Speaker 1>think we should dwell. No, no, I'm good, I'm good. Okay,

0:14:34.720 --> 0:14:38.480
<v Speaker 1>don't ever let me be too square. Okay. Uh So,

0:14:38.680 --> 0:14:42.240
<v Speaker 1>starting in the nineteen fifties and sixties, both experimental and

0:14:42.320 --> 0:14:45.400
<v Speaker 1>theoretical work really seems to accelerate in the direction of

0:14:45.440 --> 0:14:48.920
<v Speaker 1>indicating the reality of neutron stars and black holes. These

0:14:49.040 --> 0:14:54.480
<v Speaker 1>these really exotic collapsed star remnant objects and theoretical models

0:14:55.040 --> 0:14:58.720
<v Speaker 1>are affirmed over and over and they appear increasingly sound.

0:14:58.800 --> 0:15:04.480
<v Speaker 1>While new astro comical observations really seem to make us think, wow, yeah,

0:15:04.480 --> 0:15:06.760
<v Speaker 1>there could be black holes out there. I think some

0:15:06.840 --> 0:15:09.920
<v Speaker 1>of the skepticism could be unfounded. Like in the nineteen

0:15:10.000 --> 0:15:14.360
<v Speaker 1>sixties you had scientists identifying quasars, which are these distant

0:15:14.400 --> 0:15:17.960
<v Speaker 1>high energy objects, possibly young galaxies, with black holes at

0:15:17.960 --> 0:15:21.120
<v Speaker 1>the center of them, emitting trillions of times the energy

0:15:21.120 --> 0:15:24.080
<v Speaker 1>of a sun. And you had pulsars, which are spinning

0:15:24.120 --> 0:15:27.640
<v Speaker 1>objects emitting a repeating pattern of radio bursts. And around

0:15:27.640 --> 0:15:31.120
<v Speaker 1>the same time, astronomers identified sources of X rays and

0:15:31.160 --> 0:15:34.360
<v Speaker 1>gamma rays from all over the celestial map. And these

0:15:34.400 --> 0:15:38.160
<v Speaker 1>signals really strongly pointed to the physical reality of collapse

0:15:38.200 --> 0:15:41.920
<v Speaker 1>stars like neutron stars and black holes. And now we

0:15:42.000 --> 0:15:45.280
<v Speaker 1>know that actually pretty much every mature galaxy in the

0:15:45.360 --> 0:15:48.640
<v Speaker 1>universe that we know of seems to have a supermassive

0:15:48.680 --> 0:15:51.200
<v Speaker 1>black hole at its center. It may be the black

0:15:51.200 --> 0:15:55.000
<v Speaker 1>holes are necessary for the formation of galaxies, and galaxies

0:15:55.080 --> 0:15:57.440
<v Speaker 1>are where things like us live. The black hole the

0:15:57.520 --> 0:16:03.080
<v Speaker 1>life giver. Yeah, we were rebrand rebranding the black hole today. So,

0:16:03.120 --> 0:16:06.240
<v Speaker 1>speaking of supermassive black holes, I I do want to

0:16:06.280 --> 0:16:09.920
<v Speaker 1>just touch in once more on the three forms of

0:16:09.960 --> 0:16:12.720
<v Speaker 1>black holes that we tend to discuss. Okay, so we've

0:16:12.760 --> 0:16:16.000
<v Speaker 1>mainly been talking about stellar black holes, right right. The

0:16:16.000 --> 0:16:17.960
<v Speaker 1>idea of a collapse star. Yeah, these would be as

0:16:18.040 --> 0:16:21.760
<v Speaker 1>massive as as twenty of our sons uh fit inside

0:16:21.760 --> 0:16:24.680
<v Speaker 1>a one mile radius sphere. Uh. These are the would

0:16:24.680 --> 0:16:27.080
<v Speaker 1>be the remnants of very massive stars that have run

0:16:27.120 --> 0:16:29.760
<v Speaker 1>through their innergy energy reserves. They go supernova and then

0:16:29.760 --> 0:16:32.360
<v Speaker 1>they collapse upon themselves and they're thought to be the

0:16:32.360 --> 0:16:35.920
<v Speaker 1>most common type of black holes, and there are likely

0:16:36.080 --> 0:16:39.320
<v Speaker 1>dozens within our own Milky Way galaxy. And then they're

0:16:39.320 --> 0:16:42.000
<v Speaker 1>the primordial black holes. These tho I touched on the

0:16:42.040 --> 0:16:44.560
<v Speaker 1>first episode that the size of an atom. They have

0:16:44.560 --> 0:16:47.080
<v Speaker 1>the massive a mountain, So these are hypothetical, and they

0:16:47.080 --> 0:16:50.520
<v Speaker 1>probably formed soon after the Big Bang. And then of

0:16:50.560 --> 0:16:54.600
<v Speaker 1>course they're the big ones, the supermassive black holes. They

0:16:54.640 --> 0:16:57.160
<v Speaker 1>likely exist at the center of most galaxies. Our own

0:16:57.400 --> 0:17:01.240
<v Speaker 1>galaxy boast Sagittarius A, and it has a mass equal

0:17:01.280 --> 0:17:05.639
<v Speaker 1>to about four million sons. And uh, these black holes

0:17:05.680 --> 0:17:09.760
<v Speaker 1>formed with their respective galaxies and are proportional in size.

0:17:10.119 --> 0:17:13.679
<v Speaker 1>And again these these are these are a part of

0:17:13.720 --> 0:17:16.560
<v Speaker 1>our universe. You know, as much as we we tend

0:17:16.560 --> 0:17:17.960
<v Speaker 1>to sort of fall into the trap of thinking of

0:17:18.000 --> 0:17:22.720
<v Speaker 1>black holes as you know, cosmic love crafty and evil consumers,

0:17:23.200 --> 0:17:26.520
<v Speaker 1>they're they're just a part of the life cycle of stars.

0:17:26.560 --> 0:17:30.280
<v Speaker 1>They are part of the general physical reality of the universe. Yeah,

0:17:30.320 --> 0:17:34.520
<v Speaker 1>they're not reapers from another dimension. They're the life givers.

0:17:36.520 --> 0:17:40.040
<v Speaker 1>Let's not go too far alright. Well, on that note,

0:17:40.480 --> 0:17:42.480
<v Speaker 1>we're gonna take a quick break and when we come back,

0:17:42.600 --> 0:17:47.399
<v Speaker 1>we will get into the science detecting black holes. Thank you,

0:17:47.600 --> 0:17:50.760
<v Speaker 1>thank you. All Right, we're back. So I want to

0:17:50.760 --> 0:17:54.840
<v Speaker 1>tell you a story about signas X one. Okay, let's

0:17:54.840 --> 0:17:56.840
<v Speaker 1>have it. So. Way back in the nineteen sixties and

0:17:56.880 --> 0:18:00.920
<v Speaker 1>the Swinging sixties, the astronomers out there, we're making use

0:18:00.960 --> 0:18:04.120
<v Speaker 1>of a new class of tools to study distant regions

0:18:04.119 --> 0:18:08.040
<v Speaker 1>of the sky, and these were space based X ray detectors.

0:18:08.480 --> 0:18:12.720
<v Speaker 1>They were attached to orbital rockets and artificial satellites, and

0:18:12.840 --> 0:18:16.159
<v Speaker 1>these instruments looked for X ray signals the astronomers and

0:18:16.200 --> 0:18:20.840
<v Speaker 1>astrophysicists thought they might find emanating from all kinds of

0:18:20.840 --> 0:18:24.000
<v Speaker 1>celestial sources, from say, the surface of the Moon. You know,

0:18:24.040 --> 0:18:27.560
<v Speaker 1>it's the moon shooting X rays. Two distant star systems

0:18:27.560 --> 0:18:31.960
<v Speaker 1>and nebulae, and one strong source of X ray radiation

0:18:32.040 --> 0:18:35.480
<v Speaker 1>detected by rockets in the nineteen sixties was a point

0:18:35.520 --> 0:18:39.040
<v Speaker 1>in the constellation Scorpius, and the source of the radiation

0:18:39.119 --> 0:18:41.560
<v Speaker 1>came to be known as s c O X one

0:18:41.680 --> 0:18:43.400
<v Speaker 1>or SCO X one. I don't know if you say

0:18:43.440 --> 0:18:45.720
<v Speaker 1>it like SCO that makes it sound kind of scummy,

0:18:46.640 --> 0:18:50.120
<v Speaker 1>but it was a truly remarkable fine because this radiation

0:18:50.200 --> 0:18:53.560
<v Speaker 1>source was about nine thousand light years from our solar system,

0:18:53.640 --> 0:18:57.280
<v Speaker 1>and it's X ray output was millions of times stronger

0:18:57.320 --> 0:19:01.000
<v Speaker 1>than that of normal sun like stars. And this massive

0:19:01.080 --> 0:19:04.960
<v Speaker 1>energy output came we discovered from a neutron star in

0:19:05.000 --> 0:19:08.919
<v Speaker 1>a binary system, and since then other similar sources have

0:19:09.040 --> 0:19:12.760
<v Speaker 1>been discovered. These X rays are generated when matter from

0:19:12.960 --> 0:19:14.600
<v Speaker 1>so you've got a binary system, you've got like a

0:19:14.640 --> 0:19:17.200
<v Speaker 1>neutron star or a black hole, and then some other

0:19:17.280 --> 0:19:21.160
<v Speaker 1>kind of object like a star. They're dancing, Yeah, they're

0:19:21.200 --> 0:19:24.720
<v Speaker 1>they're they're doing the polka out there in space. And

0:19:25.119 --> 0:19:28.280
<v Speaker 1>the X rays are generated when matter from the surface

0:19:28.320 --> 0:19:32.159
<v Speaker 1>of the more normal star gets sucked violently into the

0:19:32.200 --> 0:19:35.800
<v Speaker 1>gravitational field and onto the surface of the neutron star.

0:19:35.960 --> 0:19:38.159
<v Speaker 1>That's what's going on in the case of s c

0:19:38.320 --> 0:19:42.200
<v Speaker 1>O X one. And during so so this this gets

0:19:42.240 --> 0:19:44.560
<v Speaker 1>sucked in, the matter gets heated up a lot, and

0:19:44.840 --> 0:19:47.840
<v Speaker 1>X rays get blasted out into space. But during these

0:19:47.840 --> 0:19:50.439
<v Speaker 1>surveys of the nineteen sixties, one X ray source in

0:19:50.440 --> 0:19:53.840
<v Speaker 1>the sky was not like the others. In nineteen sixty

0:19:53.920 --> 0:19:55.840
<v Speaker 1>four we started to get a clear picture of the

0:19:55.960 --> 0:20:00.119
<v Speaker 1>radiation output of one source in the Sickness constellation, and

0:20:00.160 --> 0:20:02.919
<v Speaker 1>this source came to be known as signus X one,

0:20:03.200 --> 0:20:06.720
<v Speaker 1>and unlike the X ray sources that emitted like regular

0:20:06.840 --> 0:20:10.440
<v Speaker 1>pulses you know sometimes that would happen be be beep,

0:20:10.760 --> 0:20:15.159
<v Speaker 1>Signus X one seemed to be releasing unbelievably powerful, irregular

0:20:15.240 --> 0:20:19.640
<v Speaker 1>bursts of this deadly high frequency radiation, and sometimes these

0:20:19.680 --> 0:20:22.560
<v Speaker 1>irregular bursts were incredibly short, like on the scale of

0:20:22.680 --> 0:20:26.040
<v Speaker 1>millionths of a second, and so at a meeting in

0:20:26.200 --> 0:20:31.919
<v Speaker 1>March ninety one, the Italian astrophysicist Ricardi Giaconi speculated that

0:20:31.960 --> 0:20:34.840
<v Speaker 1>the source of the X one signal might be a

0:20:34.960 --> 0:20:39.720
<v Speaker 1>real black hole, the first black hole apparently observed in space,

0:20:40.200 --> 0:20:43.720
<v Speaker 1>and later analysis did seem to bear out this hypothesis.

0:20:43.760 --> 0:20:46.919
<v Speaker 1>The signus X one system seems to consist of a

0:20:47.000 --> 0:20:51.000
<v Speaker 1>blue giant star orbiting with a much smaller object that

0:20:51.119 --> 0:20:54.040
<v Speaker 1>we can't see. And by observing the size of the

0:20:54.040 --> 0:20:56.840
<v Speaker 1>companion star, the blue giant known as h d E

0:20:56.920 --> 0:20:59.960
<v Speaker 1>two to six six eight, and the rate of its

0:21:00.200 --> 0:21:03.040
<v Speaker 1>orbit it completes an orbit in less than six earth

0:21:03.160 --> 0:21:06.919
<v Speaker 1>days and the size of that orbit, astronomers began to

0:21:06.960 --> 0:21:11.080
<v Speaker 1>get a picture of this unseen orbital center. It appears

0:21:11.080 --> 0:21:14.800
<v Speaker 1>to be invisible, tiny and heavy. Current estimates of its

0:21:14.840 --> 0:21:18.520
<v Speaker 1>mass are at about fourteen point eight of our sons,

0:21:18.560 --> 0:21:21.600
<v Speaker 1>and the radiation coming from this source is emitted as

0:21:21.640 --> 0:21:25.639
<v Speaker 1>this apparent black hole sucks matter off of the orbiting

0:21:25.680 --> 0:21:27.720
<v Speaker 1>star like we were just talking about with the neutron star.

0:21:27.760 --> 0:21:30.760
<v Speaker 1>It sucks gas or matter off of that star, and

0:21:30.800 --> 0:21:34.560
<v Speaker 1>the matter swirls down into the gravity pit of this object,

0:21:34.920 --> 0:21:37.359
<v Speaker 1>heating up as it does, and eventually it heats to

0:21:37.400 --> 0:21:40.080
<v Speaker 1>the point that it gives off X rays, and of course,

0:21:40.160 --> 0:21:43.679
<v Speaker 1>once that gas falls past the event horizon, presumably nothing

0:21:43.720 --> 0:21:46.919
<v Speaker 1>more is emitted. It's stuck inside. But you've got so

0:21:46.960 --> 0:21:51.360
<v Speaker 1>you've got these observations. It's massive, it's tiny, it's invisible,

0:21:51.640 --> 0:21:54.560
<v Speaker 1>and it shoots radiation out into space as it appears

0:21:54.600 --> 0:21:58.320
<v Speaker 1>to suck matter from neighboring bodies. Really really seems like

0:21:58.320 --> 0:22:02.000
<v Speaker 1>a black hole. But was it proof? This was actually

0:22:02.160 --> 0:22:05.600
<v Speaker 1>famously the subject of a bet between physicist Stephen Hawking,

0:22:06.280 --> 0:22:08.600
<v Speaker 1>who did plenty of his own important work on black

0:22:08.640 --> 0:22:11.480
<v Speaker 1>holes in Kip Thorn in nineteen seventy four. Real quick

0:22:11.600 --> 0:22:15.680
<v Speaker 1>Kip Thorne, by the way, not only physicists, but executive

0:22:15.720 --> 0:22:19.160
<v Speaker 1>producer of the two thousand fourteen film Interstellar. Oh yeah,

0:22:19.240 --> 0:22:22.600
<v Speaker 1>that that was probably the best black hole movie I've seen. Yeah,

0:22:22.680 --> 0:22:26.120
<v Speaker 1>and that's why. Right, So he tried to get them

0:22:26.160 --> 0:22:29.080
<v Speaker 1>to like get the science right, Yeah, to say, be accurate,

0:22:29.200 --> 0:22:31.240
<v Speaker 1>make it look like a black hole would really look

0:22:31.320 --> 0:22:33.720
<v Speaker 1>Let's do some math. Yeah, and they did the math,

0:22:33.800 --> 0:22:36.520
<v Speaker 1>and that's a that's that's that's something that most people

0:22:36.520 --> 0:22:39.800
<v Speaker 1>tend to to praise Interstellar for as being the best

0:22:40.080 --> 0:22:44.199
<v Speaker 1>depiction of a black hole in at least cinematic science fiction. Well,

0:22:44.320 --> 0:22:46.159
<v Speaker 1>as I've said on the show before, my favorite thing

0:22:46.160 --> 0:22:48.160
<v Speaker 1>about it is how it actually deals with the time

0:22:48.200 --> 0:22:52.159
<v Speaker 1>dilation effects of relativity. Uh. Yeah, there's a lot to

0:22:52.240 --> 0:22:54.800
<v Speaker 1>like about Interstellar. But coming back to that bet. I'm

0:22:54.800 --> 0:22:56.480
<v Speaker 1>sure you've heard about this bet before. This is a

0:22:56.520 --> 0:23:00.600
<v Speaker 1>famous bet in the history of physics astrophysics. So Thorn

0:23:00.640 --> 0:23:04.040
<v Speaker 1>and Hawking had this bet. Hawking was the pessimist, Thorn

0:23:04.200 --> 0:23:06.719
<v Speaker 1>was the optimist. Well, I guess depending on what you

0:23:06.720 --> 0:23:09.800
<v Speaker 1>think you know regarding the nature of black holes, right,

0:23:10.119 --> 0:23:12.760
<v Speaker 1>Thorn bet that Signals X one would turn out to

0:23:12.760 --> 0:23:15.080
<v Speaker 1>be a black hole. Hawking bet that it would not

0:23:15.200 --> 0:23:17.760
<v Speaker 1>turn out to be a black hole, and Hawking was wrong.

0:23:18.160 --> 0:23:21.840
<v Speaker 1>By Hawking admitted that the evidence for X one's black

0:23:21.880 --> 0:23:24.800
<v Speaker 1>hole status was so strong that he had to concede

0:23:24.800 --> 0:23:26.880
<v Speaker 1>the bet. So we live in a world now where

0:23:26.880 --> 0:23:31.200
<v Speaker 1>astronomers and astrophysicists are almost totally convinced that black holes exist.

0:23:31.680 --> 0:23:34.320
<v Speaker 1>You can fly out into space in theory, and you

0:23:34.359 --> 0:23:38.359
<v Speaker 1>could fly right into them, but they nevertheless remain tricky

0:23:38.440 --> 0:23:41.800
<v Speaker 1>from an observational standpoint. So I think now for the

0:23:41.800 --> 0:23:44.040
<v Speaker 1>rest of the episode, we should try to explain some

0:23:44.160 --> 0:23:46.720
<v Speaker 1>of the ways that we can use to try to

0:23:46.760 --> 0:23:50.400
<v Speaker 1>detect black holes in space. Yeah, a thing that by

0:23:50.400 --> 0:23:55.080
<v Speaker 1>its very definition cannot be seen, cannot be seen directly,

0:23:55.480 --> 0:23:57.440
<v Speaker 1>of what are the ways in which we can observe

0:23:57.480 --> 0:24:00.080
<v Speaker 1>their presence? Right? Because one of the very things that

0:24:00.160 --> 0:24:02.680
<v Speaker 1>makes a black hole unique is that it neither emits

0:24:02.760 --> 0:24:05.680
<v Speaker 1>nor reflects detectable light of its own. So how would

0:24:05.680 --> 0:24:08.160
<v Speaker 1>we ever know if it one exists? Well, there are

0:24:08.160 --> 0:24:11.000
<v Speaker 1>lots of indirect ways of detecting them. And of course,

0:24:11.080 --> 0:24:13.359
<v Speaker 1>even though it doesn't emit light of its own, that

0:24:13.400 --> 0:24:16.240
<v Speaker 1>doesn't mean it's necessarily dark, because, as we explained in

0:24:16.280 --> 0:24:19.199
<v Speaker 1>the last episode, there's stuff going on around it. And

0:24:19.240 --> 0:24:21.520
<v Speaker 1>in fact, we just touched on one example of this.

0:24:21.920 --> 0:24:25.360
<v Speaker 1>Uh of the idea of stuff falling into the black hole,

0:24:25.400 --> 0:24:28.680
<v Speaker 1>stuff being material being sucked into it. Yeah, so black

0:24:28.720 --> 0:24:32.439
<v Speaker 1>holes themselves are dark, but from our perspective, the region

0:24:32.520 --> 0:24:35.320
<v Speaker 1>around the black hole can be anything. But So imagine

0:24:35.920 --> 0:24:38.920
<v Speaker 1>there's this region of space where we observe extremely hot,

0:24:39.000 --> 0:24:42.120
<v Speaker 1>high energy radiation. You've got X rays spewing out all

0:24:42.119 --> 0:24:44.760
<v Speaker 1>over the place. What's going on there? Well, a good

0:24:44.840 --> 0:24:48.040
<v Speaker 1>chances you've got a black hole with matter falling into it.

0:24:48.359 --> 0:24:50.679
<v Speaker 1>The matter gets heated up to hundreds of millions of

0:24:50.720 --> 0:24:53.960
<v Speaker 1>degrees and produces all these kinds of powerful radiation that

0:24:54.040 --> 0:24:58.120
<v Speaker 1>are visible from Earth until it passes that threshold, however,

0:24:58.200 --> 0:25:00.760
<v Speaker 1>and falls into the black hole, after which admits nothing.

0:25:01.240 --> 0:25:04.359
<v Speaker 1>To revisit what we uh the example I brought up

0:25:04.359 --> 0:25:05.919
<v Speaker 1>in the last episode, I think it's kind of like

0:25:05.920 --> 0:25:08.119
<v Speaker 1>you've got a haunted house and you've got like a

0:25:08.119 --> 0:25:11.159
<v Speaker 1>car that takes people around the haunted house. And the

0:25:11.200 --> 0:25:13.919
<v Speaker 1>car is soundproof, so you can't hear people screams from

0:25:14.000 --> 0:25:17.000
<v Speaker 1>inside the car, but as the tourists line up to

0:25:17.119 --> 0:25:19.600
<v Speaker 1>get into the car, you will probably hear them doing

0:25:19.600 --> 0:25:22.440
<v Speaker 1>all kinds of things as they're like sort of loading in.

0:25:22.960 --> 0:25:25.399
<v Speaker 1>And the fact that you can observe. Often all of

0:25:25.440 --> 0:25:28.439
<v Speaker 1>this violence and radiation around a black hole came up

0:25:28.440 --> 0:25:31.760
<v Speaker 1>in that darkness visible presentation. Right. Yeah, it was pointed

0:25:31.800 --> 0:25:34.720
<v Speaker 1>out that the despite they're inherent darkness, black holes are

0:25:34.720 --> 0:25:38.800
<v Speaker 1>among the brightest objects and the cosmos often, uh pinpointed

0:25:38.880 --> 0:25:42.240
<v Speaker 1>is points of extreme brightness in a relatively compact region

0:25:42.280 --> 0:25:44.399
<v Speaker 1>of space. And this is due to all of the

0:25:45.160 --> 0:25:48.840
<v Speaker 1>material and light surging in and orbiting around the objects

0:25:48.840 --> 0:25:51.840
<v Speaker 1>of the horizon, the point again at which even light

0:25:51.880 --> 0:25:56.200
<v Speaker 1>cannot escape. Right, this is probably a terrible, a terrible comparison.

0:25:56.240 --> 0:25:58.240
<v Speaker 1>But to come back to the Texas chainsaw mask your house,

0:25:58.280 --> 0:26:01.160
<v Speaker 1>it's like, oh again, yeah, they're all the is, all

0:26:01.200 --> 0:26:04.439
<v Speaker 1>these missing teenagers and all of these looted graveyards. Uh.

0:26:04.520 --> 0:26:07.560
<v Speaker 1>And then we have this one area here, uh clear,

0:26:07.600 --> 0:26:09.800
<v Speaker 1>look at all this activity around the house. That's how

0:26:09.840 --> 0:26:12.320
<v Speaker 1>we have some idea about what's going on inside it. Right,

0:26:12.400 --> 0:26:14.760
<v Speaker 1>Maybe you can't get a warrant to go inside the house,

0:26:14.840 --> 0:26:17.040
<v Speaker 1>but you can see there's a ruckus going on or

0:26:17.119 --> 0:26:19.440
<v Speaker 1>in the general vicinity, right, And that's what we're looking

0:26:19.440 --> 0:26:21.560
<v Speaker 1>at here, the black hole ruckus. But that's not the

0:26:21.600 --> 0:26:24.800
<v Speaker 1>only way that we can we can detect the presence

0:26:24.800 --> 0:26:26.760
<v Speaker 1>of a black hole. No, there are lots of other

0:26:26.840 --> 0:26:30.520
<v Speaker 1>really interesting ways. So here's another one. Imagine you are

0:26:30.560 --> 0:26:33.560
<v Speaker 1>to look at a place in the galaxy where visible

0:26:33.640 --> 0:26:38.280
<v Speaker 1>objects are acting weird. Planets are stars travel in these

0:26:38.320 --> 0:26:42.040
<v Speaker 1>repeating loops as if in orbit around something, but we

0:26:42.200 --> 0:26:44.600
<v Speaker 1>can't see what that thing is for them to be

0:26:44.640 --> 0:26:47.080
<v Speaker 1>an orbit around, or if we can see it, maybe

0:26:47.080 --> 0:26:49.840
<v Speaker 1>it's like they're orbiting an invisible star, or we can

0:26:49.920 --> 0:26:53.320
<v Speaker 1>see something very bright that they're orbiting, and the way

0:26:53.359 --> 0:26:56.760
<v Speaker 1>that they're orbiting it indicates that this thing they're orbiting

0:26:56.880 --> 0:27:00.880
<v Speaker 1>might be both very very small and very very massive.

0:27:01.320 --> 0:27:04.119
<v Speaker 1>It's essentially the invisible man scenario, you know, like you

0:27:04.160 --> 0:27:06.960
<v Speaker 1>can see the hat, but there's no person there. Well,

0:27:07.000 --> 0:27:09.080
<v Speaker 1>something must be holding up the hat. Yeah, something's hold

0:27:09.119 --> 0:27:11.840
<v Speaker 1>up the hat and the umbrella. So, uh, for example,

0:27:12.280 --> 0:27:14.240
<v Speaker 1>what do we see when we look closely at the

0:27:14.280 --> 0:27:17.320
<v Speaker 1>center of our own Milky Way galaxy? We mentioned this

0:27:17.400 --> 0:27:20.240
<v Speaker 1>darkness visible presentation at the World Science Festival this year.

0:27:20.840 --> 0:27:24.679
<v Speaker 1>Uh So that presentation featured, among others, the u c

0:27:24.840 --> 0:27:28.359
<v Speaker 1>l A astronomer Andrea Gays, who has spent her career

0:27:28.480 --> 0:27:31.919
<v Speaker 1>examining exactly this question. What's going on at the center

0:27:31.960 --> 0:27:34.560
<v Speaker 1>of the galaxy. Now, of course, we mentioned in the

0:27:34.600 --> 0:27:37.840
<v Speaker 1>previous episode and earlier today that researchers have come to

0:27:37.880 --> 0:27:41.080
<v Speaker 1>believe that there is a supermassive black hole at the

0:27:41.119 --> 0:27:44.240
<v Speaker 1>center of most are all mature galaxies, and our galaxy

0:27:44.280 --> 0:27:46.680
<v Speaker 1>is no different. At the center of our galaxy, there's

0:27:46.720 --> 0:27:50.320
<v Speaker 1>an object called Sagittary Essay, which is believed to be

0:27:50.560 --> 0:27:53.840
<v Speaker 1>a black hole about four point three million times the

0:27:53.880 --> 0:27:56.720
<v Speaker 1>mass of our Sun, though Gays actually says that this

0:27:56.800 --> 0:27:59.680
<v Speaker 1>is on the low end of supermassive black holes, which

0:27:59.720 --> 0:28:02.239
<v Speaker 1>can be up to a billion times the mass of

0:28:02.240 --> 0:28:05.200
<v Speaker 1>our son. Though I want, I want to be impressed

0:28:05.240 --> 0:28:07.920
<v Speaker 1>by that, but I'm running into like the scale problem

0:28:08.040 --> 0:28:11.720
<v Speaker 1>right where somebody says like, hey, Robert, I want to

0:28:11.760 --> 0:28:16.000
<v Speaker 1>give you a hundred billion dollars or I want to

0:28:16.040 --> 0:28:19.960
<v Speaker 1>give you five hundred billion dollars. Yeah, up saying with

0:28:20.040 --> 0:28:22.080
<v Speaker 1>the scales that they might as well be the same

0:28:22.160 --> 0:28:25.679
<v Speaker 1>number because they're just so beyond my ability to, you know,

0:28:25.720 --> 0:28:27.920
<v Speaker 1>to fit them within the confines of my own life. Yeah,

0:28:27.960 --> 0:28:29.840
<v Speaker 1>what does that mean? What does that difference even matter?

0:28:30.160 --> 0:28:32.680
<v Speaker 1>What am I supposed to do with that information? Yeah?

0:28:32.720 --> 0:28:35.560
<v Speaker 1>So even though I recognize that that is a big difference,

0:28:35.600 --> 0:28:38.760
<v Speaker 1>and that that's it should be really impressive. I can't

0:28:38.760 --> 0:28:41.640
<v Speaker 1>actually picture it, so I'm I'm kind of stuck there.

0:28:41.960 --> 0:28:43.760
<v Speaker 1>You often run into this with some of the most

0:28:43.800 --> 0:28:46.960
<v Speaker 1>impressive stuff, and in astronomy it's like you want to

0:28:47.000 --> 0:28:51.920
<v Speaker 1>be accurately appreciative, but you can't visualize the scale. Yeah,

0:28:51.920 --> 0:28:55.080
<v Speaker 1>because then the numbers just become meaningless to most minds

0:28:55.120 --> 0:28:57.600
<v Speaker 1>after a point. But anyway, back to so Sagittary is,

0:28:57.600 --> 0:29:00.000
<v Speaker 1>say this thing that we believe to be a super

0:29:00.040 --> 0:29:03.120
<v Speaker 1>supermassive black hole. How how would you detect if it

0:29:03.160 --> 0:29:05.960
<v Speaker 1>really were a supermassive black hole? And just to note,

0:29:06.200 --> 0:29:09.120
<v Speaker 1>we keep calling it Sagittarius A, but technically the object

0:29:09.120 --> 0:29:12.280
<v Speaker 1>believed to be the black hole is Sagittarius A with

0:29:12.360 --> 0:29:16.640
<v Speaker 1>little asterisks. They call that Sagittarius A star. While Sagittarius

0:29:16.680 --> 0:29:19.160
<v Speaker 1>A as a whole is this more complex source of

0:29:19.280 --> 0:29:22.800
<v Speaker 1>radio signals, including the object we're talking about. So technically

0:29:22.800 --> 0:29:25.600
<v Speaker 1>it's Sagittarius A star, but I think we will keep

0:29:25.600 --> 0:29:29.360
<v Speaker 1>calling it Sagittarius A because when you're also talking about stars,

0:29:29.520 --> 0:29:32.680
<v Speaker 1>saying a star over and over can be confusing. So

0:29:32.840 --> 0:29:36.280
<v Speaker 1>the main method that Gaye talks about is to demonstrate

0:29:36.320 --> 0:29:39.560
<v Speaker 1>that a mass is within its short shield radius. We

0:29:39.600 --> 0:29:42.160
<v Speaker 1>talked about the short shield sphere in the last episode,

0:29:42.560 --> 0:29:45.800
<v Speaker 1>and in simple terms, what you're looking for is big mass,

0:29:45.960 --> 0:29:49.720
<v Speaker 1>small volume. We know that any mass contained within the

0:29:49.840 --> 0:29:53.800
<v Speaker 1>volume of its short shield radius will inevitably collapse into

0:29:53.840 --> 0:29:57.000
<v Speaker 1>a black hole. Nothing can stop it. At this scale,

0:29:57.240 --> 0:30:00.840
<v Speaker 1>gravity always wins, and a if you can show this,

0:30:00.960 --> 0:30:03.160
<v Speaker 1>if you can show that an object is of a

0:30:03.200 --> 0:30:06.760
<v Speaker 1>mass that's within the volume of its short shield radius,

0:30:07.000 --> 0:30:10.240
<v Speaker 1>you've effectively demonstrated that it must be a black hole.

0:30:10.720 --> 0:30:12.880
<v Speaker 1>So to see what's happening at the center of our galaxy,

0:30:12.920 --> 0:30:16.320
<v Speaker 1>we can look toward the constellation Sagittarius, and if you

0:30:16.320 --> 0:30:18.440
<v Speaker 1>have the right kind of telescope, you can peer straight

0:30:18.440 --> 0:30:21.000
<v Speaker 1>through to the group of stars at the core of

0:30:21.040 --> 0:30:24.520
<v Speaker 1>the Milky Way, the galactic center. And these stars really

0:30:24.560 --> 0:30:27.800
<v Speaker 1>do behave in an odd way, especially like a central

0:30:27.840 --> 0:30:32.120
<v Speaker 1>star called s O two, which orbits the object Sagittarius

0:30:32.160 --> 0:30:35.120
<v Speaker 1>A in a pattern of one orbit every sixteen years.

0:30:35.480 --> 0:30:37.719
<v Speaker 1>There are animations of this that are worth looking up.

0:30:37.760 --> 0:30:40.240
<v Speaker 1>In fact, there's even direct imaging. I don't know, but

0:30:40.320 --> 0:30:42.520
<v Speaker 1>it might be infrared imaging. But they're there. You can

0:30:42.560 --> 0:30:45.560
<v Speaker 1>like see the stars actually moving over a long time

0:30:45.640 --> 0:30:48.320
<v Speaker 1>lapse video, and the path of s O two looks

0:30:48.320 --> 0:30:51.280
<v Speaker 1>almost like a I'm trying to find the right point

0:30:51.280 --> 0:30:53.880
<v Speaker 1>of comparison. It's sort of like a pendulum or something,

0:30:53.960 --> 0:30:56.840
<v Speaker 1>you know, where you see something kind of slowly go

0:30:57.120 --> 0:30:59.760
<v Speaker 1>up to one side and then zoom down along the

0:30:59.800 --> 0:31:03.200
<v Speaker 1>other side. Um. And so that's what happens with the

0:31:03.280 --> 0:31:06.720
<v Speaker 1>start cruises slowly through a lot of its elliptical path

0:31:07.080 --> 0:31:09.960
<v Speaker 1>and then whips lightning fast through one end of the

0:31:10.000 --> 0:31:12.880
<v Speaker 1>ellipse of its orbit. And what's going on there is

0:31:12.920 --> 0:31:16.240
<v Speaker 1>apparently when s O two travels through the closest part

0:31:16.240 --> 0:31:20.480
<v Speaker 1>of its orbit with Sagittarius AY about seventeen light hours away,

0:31:20.680 --> 0:31:23.280
<v Speaker 1>it's moving at about three percent of the speed of light,

0:31:23.520 --> 0:31:28.040
<v Speaker 1>or roughly thirty million kilometers per hour, and that even

0:31:28.080 --> 0:31:30.240
<v Speaker 1>if you just look at the animations, you can tell

0:31:30.280 --> 0:31:33.959
<v Speaker 1>it's super fast. So because we can image the region

0:31:33.960 --> 0:31:37.920
<v Speaker 1>of Sagittarius AY and the objects traveling around Sagittarius A,

0:31:38.280 --> 0:31:41.400
<v Speaker 1>we can do physics calculations to determine the size and

0:31:41.440 --> 0:31:43.920
<v Speaker 1>the mass of what this object is, and it turns

0:31:43.920 --> 0:31:46.640
<v Speaker 1>out that it's more than four million times the mass

0:31:46.640 --> 0:31:49.280
<v Speaker 1>of our sun and appears to be crammed into this

0:31:49.480 --> 0:31:52.080
<v Speaker 1>very very tiny region at the center of the galaxy.

0:31:52.160 --> 0:31:55.400
<v Speaker 1>So it looks very much like a supermassive black hole.

0:31:55.720 --> 0:31:57.520
<v Speaker 1>All Right, we're gonna take one more break and we

0:31:57.600 --> 0:32:00.280
<v Speaker 1>come back. We will jump into more ways that we

0:32:00.360 --> 0:32:07.480
<v Speaker 1>detect black holes, including gravitational lensing. Thank thank Alright, we're back, Hey, Robert,

0:32:07.960 --> 0:32:10.320
<v Speaker 1>So what would happen do you think if you were

0:32:10.440 --> 0:32:14.920
<v Speaker 1>looking at something and a black hole passed between you

0:32:15.040 --> 0:32:18.000
<v Speaker 1>and the thing you were looking at. Ah? Well, I

0:32:18.040 --> 0:32:21.160
<v Speaker 1>think on one hand, a lot of people are attempted

0:32:21.200 --> 0:32:23.200
<v Speaker 1>to say, oh, you wouldn't be able to see it,

0:32:23.240 --> 0:32:25.000
<v Speaker 1>because the black hole would be in the way. It'd

0:32:25.000 --> 0:32:27.200
<v Speaker 1>be opaque. It would be like taking a black piece

0:32:27.240 --> 0:32:31.080
<v Speaker 1>of paper across your field division just blotted out. But

0:32:31.680 --> 0:32:35.120
<v Speaker 1>that doesn't quite seem to be the case. Definitely, not necessarily.

0:32:35.680 --> 0:32:39.200
<v Speaker 1>What occurs is something called gravitational lensing, and this occurs

0:32:39.240 --> 0:32:43.600
<v Speaker 1>when a strong gravitational field bends light around it, creating

0:32:43.600 --> 0:32:47.440
<v Speaker 1>a lens like effect, warping and magnifying light coming from

0:32:47.480 --> 0:32:50.760
<v Speaker 1>the opposite direction of the view. Yeah. So the simplified

0:32:50.880 --> 0:32:53.080
<v Speaker 1>version of this, I suspect it wouldn't actually work for

0:32:53.120 --> 0:32:56.720
<v Speaker 1>objects this small. But it's that if you, you know, Robert,

0:32:56.720 --> 0:32:58.640
<v Speaker 1>you and I stand on opposite ends of the room

0:32:59.080 --> 0:33:01.760
<v Speaker 1>and you put a black hole directly between us, instead

0:33:01.800 --> 0:33:05.280
<v Speaker 1>of just being completely blotted out, we'll sort of see weird,

0:33:05.640 --> 0:33:10.200
<v Speaker 1>warped fun house mirror versions of each other wrapped around

0:33:10.280 --> 0:33:13.440
<v Speaker 1>this dark spot. In our field of view. We will

0:33:13.480 --> 0:33:18.400
<v Speaker 1>be essentially distorted through the lens created by the gravity

0:33:18.440 --> 0:33:21.480
<v Speaker 1>distortion of the black hole. Yeah. One example of this

0:33:21.560 --> 0:33:25.600
<v Speaker 1>is frequently um used is what's known as Einstein's cross

0:33:26.160 --> 0:33:29.760
<v Speaker 1>These are four images of the same distant quasar that

0:33:29.840 --> 0:33:33.440
<v Speaker 1>appear around a four ground galaxy due to strong grave

0:33:33.720 --> 0:33:37.840
<v Speaker 1>gravitational lensing. So there's kind of this blur in the center,

0:33:38.280 --> 0:33:42.080
<v Speaker 1>and then the same star is pictured four different places

0:33:42.120 --> 0:33:44.920
<v Speaker 1>around it. That's interesting, So you might think of it

0:33:44.960 --> 0:33:47.600
<v Speaker 1>that way. In our our our rough example, here, I'm

0:33:47.600 --> 0:33:50.360
<v Speaker 1>looking across the room. I see a basic like blur

0:33:50.520 --> 0:33:52.560
<v Speaker 1>where you should be, where the black hole is is

0:33:52.600 --> 0:33:55.320
<v Speaker 1>blocking my view. And then perhaps to either side of you,

0:33:55.520 --> 0:33:59.000
<v Speaker 1>I see distorted versions of Joe, a beautiful image. Yeah,

0:33:59.000 --> 0:34:01.080
<v Speaker 1>maybe one floating a of you as well, kind of

0:34:01.080 --> 0:34:05.000
<v Speaker 1>like an angelic visitor with like kind of crazy warped

0:34:05.120 --> 0:34:07.680
<v Speaker 1>arms flapping around on both sides, like one of those

0:34:07.680 --> 0:34:11.239
<v Speaker 1>inflatable dude dads you see it to use car dealership.

0:34:12.320 --> 0:34:15.520
<v Speaker 1>Another example that I came across was that in two

0:34:15.520 --> 0:34:18.719
<v Speaker 1>thousand and ten, the Keck two telescope in Hawaii and

0:34:18.760 --> 0:34:22.919
<v Speaker 1>it's in I r C two instruments observed a four

0:34:23.040 --> 0:34:27.520
<v Speaker 1>ground quasar causing gravitational lensing of a galaxy in the

0:34:27.520 --> 0:34:29.920
<v Speaker 1>background behind it. So I think it's actually the reverse

0:34:30.040 --> 0:34:33.920
<v Speaker 1>of the example you just gave. So the quaysar is

0:34:34.000 --> 0:34:36.960
<v Speaker 1>likely to be a giant black hole that's spewing huge

0:34:36.960 --> 0:34:39.680
<v Speaker 1>amounts of radiation into the universe around it, making it

0:34:39.760 --> 0:34:44.399
<v Speaker 1>extremely bright. And this foreground quasar is known as sd

0:34:44.760 --> 0:34:48.560
<v Speaker 1>s J zero zero thirteen plus one to three. I

0:34:48.560 --> 0:34:50.840
<v Speaker 1>almost stopped reading there, but you know, you got to

0:34:50.840 --> 0:34:53.640
<v Speaker 1>say all the numbers, uh. And it's about one point

0:34:53.640 --> 0:34:56.200
<v Speaker 1>six billion light years from Earth, so this is very,

0:34:56.320 --> 0:34:58.719
<v Speaker 1>very far away. I included a picture here for us

0:34:58.760 --> 0:35:01.600
<v Speaker 1>to look at, but you can see how the quays

0:35:01.640 --> 0:35:05.799
<v Speaker 1>are in the foreground because of its great gravitational distortion effects,

0:35:05.960 --> 0:35:10.239
<v Speaker 1>seems to create a lensed image. These distorted side effects

0:35:10.280 --> 0:35:13.640
<v Speaker 1>of a galaxy that's in the background right behind it.

0:35:14.600 --> 0:35:16.680
<v Speaker 1>But we should get to the next method because actually,

0:35:16.760 --> 0:35:19.080
<v Speaker 1>I think this is maybe the most interesting and one

0:35:19.120 --> 0:35:22.080
<v Speaker 1>of the most conclusive methods that we have come up

0:35:22.080 --> 0:35:25.600
<v Speaker 1>with so far to demonstrate not only the existence of

0:35:25.640 --> 0:35:27.879
<v Speaker 1>black holes in the universe, but some of the most

0:35:28.040 --> 0:35:31.839
<v Speaker 1>violent black hole behaviors in the known universe. And that

0:35:31.960 --> 0:35:34.200
<v Speaker 1>is finally getting to a world where we can observe

0:35:34.200 --> 0:35:38.080
<v Speaker 1>gravitational waves. That's right, So we already discussed the general

0:35:38.160 --> 0:35:42.680
<v Speaker 1>relativity concept that mass distorts space time. As part of this,

0:35:42.719 --> 0:35:46.800
<v Speaker 1>Einstein also predicted that we'd observed ripples in spacetime gravitational

0:35:46.920 --> 0:35:50.600
<v Speaker 1>waves caused by some of the more extreme occurrences linked

0:35:50.640 --> 0:35:55.000
<v Speaker 1>to massive accelerating objects, like like a massive star being

0:35:55.120 --> 0:35:59.680
<v Speaker 1>hit with God's pool cue what ripping up the fabric

0:36:00.600 --> 0:36:03.040
<v Speaker 1>or just just the shock wave, the sound, you know,

0:36:03.080 --> 0:36:04.879
<v Speaker 1>however you want to, you know, interpret it just the

0:36:05.000 --> 0:36:07.360
<v Speaker 1>violence of the act. Well, you know, one of the

0:36:07.360 --> 0:36:11.200
<v Speaker 1>funny things in the last episode we mentioned the English

0:36:11.640 --> 0:36:14.200
<v Speaker 1>you guess you might call him a poly mauth, John Michelle,

0:36:14.200 --> 0:36:16.440
<v Speaker 1>who was one of the early people to write about

0:36:16.440 --> 0:36:18.680
<v Speaker 1>the idea of something like a black hole and a

0:36:18.800 --> 0:36:21.640
<v Speaker 1>thing that he posited that many people might not have

0:36:22.360 --> 0:36:24.400
<v Speaker 1>been able to imagine at the time, was the idea

0:36:24.440 --> 0:36:28.120
<v Speaker 1>of ripples going through the earth. The earth the like

0:36:28.200 --> 0:36:31.400
<v Speaker 1>earthquakes could be caused by shock waves and the earth

0:36:31.480 --> 0:36:35.680
<v Speaker 1>flexing up and down due to friction events. And so

0:36:35.880 --> 0:36:37.799
<v Speaker 1>you know, it's hard for somebody to imagine, how could

0:36:37.800 --> 0:36:40.480
<v Speaker 1>there be ripples in the ground. The ground is just solid.

0:36:40.600 --> 0:36:42.880
<v Speaker 1>You know, I see waves in water, but surely not

0:36:42.960 --> 0:36:46.200
<v Speaker 1>in the ground. Take this the next step. Take this

0:36:46.280 --> 0:36:50.480
<v Speaker 1>to ripples and waves emanating through the geometry of spacetime itself.

0:36:50.880 --> 0:36:53.600
<v Speaker 1>So what kind of violence would we be talking about here?

0:36:53.719 --> 0:36:55.880
<v Speaker 1>So obviously God doesn't play pool, so we can't go

0:36:55.920 --> 0:36:57.800
<v Speaker 1>with the pool que example as far as you know

0:36:58.000 --> 0:37:00.279
<v Speaker 1>as well. Yes, so he doesn't play it in this

0:37:00.440 --> 0:37:02.600
<v Speaker 1>universe in a way that we can observe it, But

0:37:02.800 --> 0:37:07.319
<v Speaker 1>we can look to other cataclysmic events like supernova and

0:37:07.480 --> 0:37:12.440
<v Speaker 1>colliding black holes. Now, we were not able to observe

0:37:12.480 --> 0:37:15.200
<v Speaker 1>any proof of this until nineteen four and that's when

0:37:15.480 --> 0:37:20.040
<v Speaker 1>astronomers at Aricibo Radio Observatory in Puerto Rico discovered a

0:37:20.080 --> 0:37:25.200
<v Speaker 1>binary pulsar. And then it wasn't until astronomers using the

0:37:25.280 --> 0:37:32.600
<v Speaker 1>Ligo that's a laser interferometer gravitational wave observatory actually physically,

0:37:32.640 --> 0:37:37.840
<v Speaker 1>since gravitational waves emitted by two colliding black holes nearly

0:37:38.239 --> 0:37:42.480
<v Speaker 1>one point three billion light years away billion light years,

0:37:42.640 --> 0:37:46.680
<v Speaker 1>So how could we detect something that far away? Well,

0:37:47.120 --> 0:37:49.960
<v Speaker 1>the whole set up here is really fascinating because when

0:37:49.960 --> 0:37:52.480
<v Speaker 1>you when you look at pictures of it, it does

0:37:52.520 --> 0:37:57.240
<v Speaker 1>not look like a telescope. Uh. They use special detectors

0:37:57.280 --> 0:38:02.480
<v Speaker 1>in at the time to locations Washington State and Louisiana, uh,

0:38:02.680 --> 0:38:07.520
<v Speaker 1>separated Uh, this way across you know, of what, three

0:38:07.560 --> 0:38:11.560
<v Speaker 1>thousand kilometers in order to rule out localized distortions, right,

0:38:11.640 --> 0:38:13.880
<v Speaker 1>So you wouldn't want to rumble in one place to

0:38:13.920 --> 0:38:17.440
<v Speaker 1>give you a false positive on gravitational waves. So what

0:38:17.520 --> 0:38:21.879
<v Speaker 1>these things looked like are two blind l shaped detectors

0:38:22.280 --> 0:38:26.880
<v Speaker 1>with with the four kilometer long vacuum chambers essentially long

0:38:26.960 --> 0:38:32.040
<v Speaker 1>tubes with lasers shining through them, uh, calibrated to detect

0:38:32.120 --> 0:38:37.560
<v Speaker 1>like just just minute motions to measure emotion ten thousand

0:38:37.640 --> 0:38:41.919
<v Speaker 1>times smaller than an atomic nucleus, the smallest measurement ever

0:38:41.960 --> 0:38:45.960
<v Speaker 1>attempted by science. And again this is calibrated to to

0:38:46.080 --> 0:38:50.279
<v Speaker 1>observe these oscillations caused by the most violent and cataclysmic

0:38:50.320 --> 0:38:52.600
<v Speaker 1>events in the universe that are occurring millions or billions

0:38:52.600 --> 0:38:57.080
<v Speaker 1>of light years away. So both detectors picked up on

0:38:57.120 --> 0:39:01.200
<v Speaker 1>the black hole emitted gravitational waves at the expected intervals

0:39:01.640 --> 0:39:04.960
<v Speaker 1>dancing black holes in another galaxy, and then the waves

0:39:04.960 --> 0:39:07.880
<v Speaker 1>stop as the merger becomes absolute. Is the two black

0:39:07.880 --> 0:39:10.680
<v Speaker 1>holes stop dancing and become one. Okay, So you've got

0:39:10.680 --> 0:39:14.880
<v Speaker 1>this picture created by these two different laser observatories at

0:39:14.920 --> 0:39:18.279
<v Speaker 1>different parts of the country that something happened very very

0:39:18.320 --> 0:39:21.560
<v Speaker 1>far away where suddenly there was this escalating ripple as

0:39:21.600 --> 0:39:24.400
<v Speaker 1>these black holes kind of swirled into each other and

0:39:24.400 --> 0:39:28.239
<v Speaker 1>then merged and then boom nothing right, And that's exactly

0:39:28.280 --> 0:39:31.720
<v Speaker 1>what they expected to find. That the results match simulations

0:39:32.000 --> 0:39:35.680
<v Speaker 1>and therefore expectations the basic template for black hole merger.

0:39:35.880 --> 0:39:38.439
<v Speaker 1>And because they've got these two different stations, they could

0:39:38.480 --> 0:39:41.919
<v Speaker 1>say with really good confidence that they know this really

0:39:41.960 --> 0:39:44.120
<v Speaker 1>came from space and what it really is. It wasn't

0:39:44.160 --> 0:39:46.360
<v Speaker 1>just some kind of local fluke. Yeah, or you know,

0:39:46.400 --> 0:39:48.680
<v Speaker 1>like a car driving by with its stereo turned up right.

0:39:49.080 --> 0:39:52.319
<v Speaker 1>Uh No, Jack Burton and his rig uh. And And

0:39:52.360 --> 0:39:54.640
<v Speaker 1>since that time we've added there's they've added a less

0:39:54.640 --> 0:39:57.960
<v Speaker 1>sensitive Italian telescope into the mix and have observed waves

0:39:57.960 --> 0:40:01.879
<v Speaker 1>generated by a pair of neutron stars as well. Now,

0:40:01.920 --> 0:40:04.799
<v Speaker 1>when you were talking to Brian Green, the physicist at

0:40:04.840 --> 0:40:07.239
<v Speaker 1>the World Science Festival, and you asked him what the

0:40:07.280 --> 0:40:10.640
<v Speaker 1>most interesting research frontier and experimental physics was today, he

0:40:10.719 --> 0:40:14.880
<v Speaker 1>named gravitational waves because he basically said that this opens

0:40:14.960 --> 0:40:18.240
<v Speaker 1>up a whole new way of looking at the universe

0:40:18.280 --> 0:40:20.560
<v Speaker 1>that we did not have before, and so there are

0:40:20.560 --> 0:40:23.640
<v Speaker 1>all kinds of surprises we could discover through it. Yeah,

0:40:23.680 --> 0:40:25.479
<v Speaker 1>I mean in a in a in a weird way.

0:40:25.560 --> 0:40:29.280
<v Speaker 1>And it's almost like we're suddenly able to to listen

0:40:29.280 --> 0:40:32.320
<v Speaker 1>to the pulse of of of things in the universe

0:40:32.360 --> 0:40:36.080
<v Speaker 1>that were previously silent to us but that we suspected

0:40:36.200 --> 0:40:38.560
<v Speaker 1>would be present. I like that, And so that brings

0:40:38.640 --> 0:40:41.640
<v Speaker 1>us back, That brings us up to that that basically

0:40:41.640 --> 0:40:44.520
<v Speaker 1>brings us up to the present. Now, that's definitely not everything.

0:40:44.520 --> 0:40:46.640
<v Speaker 1>I mean, there's all kinds of interesting work that's been

0:40:46.680 --> 0:40:48.719
<v Speaker 1>done in the years in between on black holes, like

0:40:48.719 --> 0:40:51.360
<v Speaker 1>all the work of Stephen Hawking and everything, but um

0:40:51.480 --> 0:40:56.240
<v Speaker 1>Hawking radiation and entropy and information loss and uh and stuff.

0:40:56.239 --> 0:40:59.320
<v Speaker 1>And so I think we in the next episode should

0:40:59.440 --> 0:41:03.600
<v Speaker 1>explore a little bit of the weirder side and outstanding

0:41:03.680 --> 0:41:07.440
<v Speaker 1>mysteries about black holes, questions that are as yet unsolved,

0:41:07.880 --> 0:41:11.319
<v Speaker 1>or the weirdest thought experiments about black holes. Oh yes,

0:41:11.320 --> 0:41:13.879
<v Speaker 1>because that's the that's the wonderful part, right. Black holes

0:41:13.880 --> 0:41:18.880
<v Speaker 1>began as thought experiments, and thought experiments concerning black holes continue.

0:41:19.200 --> 0:41:21.759
<v Speaker 1>So black holes already maybe the weirdest thing in the

0:41:21.880 --> 0:41:24.759
<v Speaker 1>universe that's not alive. And in the next episode we're

0:41:24.760 --> 0:41:26.880
<v Speaker 1>going to find out what are the weirdest things about

0:41:26.920 --> 0:41:29.520
<v Speaker 1>them and the biggest mysteries yet unsolved. That's right. And

0:41:29.560 --> 0:41:32.160
<v Speaker 1>I'm also going to try and rewatch Event Horizon before

0:41:32.200 --> 0:41:36.200
<v Speaker 1>that episode as well. Prepare for leather punk Spaceship. Yeah,

0:41:36.520 --> 0:41:39.680
<v Speaker 1>and and I can truly, I can truly say where

0:41:39.680 --> 0:41:42.040
<v Speaker 1>we're going. You won't need eyes to see because it's

0:41:42.040 --> 0:41:44.560
<v Speaker 1>a podcast, you really don't have to to see anything.

0:41:44.680 --> 0:41:47.200
<v Speaker 1>And because it's a black hole and no light escapes exactly,

0:41:47.560 --> 0:41:50.200
<v Speaker 1>it all fits together. It's a great script that Event

0:41:50.239 --> 0:41:54.399
<v Speaker 1>Horizon alright. In the meantime, head on over to Stuff

0:41:54.440 --> 0:41:56.680
<v Speaker 1>to Blow your Mind dot com. That is the mothership.

0:41:56.719 --> 0:41:58.719
<v Speaker 1>That's where we'll find all the episodes of the podcast,

0:41:58.800 --> 0:42:01.440
<v Speaker 1>as well as links out to our us social media accounts.

0:42:01.719 --> 0:42:03.760
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0:42:03.800 --> 0:42:05.840
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0:42:06.080 --> 0:42:09.319
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0:42:09.360 --> 0:42:13.760
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0:42:13.800 --> 0:42:17.480
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0:42:17.520 --> 0:42:19.080
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0:42:19.080 --> 0:42:22.120
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0:42:22.200 --> 0:42:24.120
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0:42:24.120 --> 0:42:26.120
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0:42:26.239 --> 0:42:28.440
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0:42:28.440 --> 0:42:31.120
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0:42:31.200 --> 0:42:42.840
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0:42:43.080 --> 0:43:04.600
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