WEBVTT - Flares from Infinity: Sagittarius A* Part 2

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<v Speaker 1>Welcome Stuff to Blow Your Mind, a production of I

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<v Speaker 1>Heart Radios How Stuff Works. Hey, you welcome to Stuff

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<v Speaker 1>to Blow your Mind. My name is Robert Lamb and

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<v Speaker 1>I'm Joe McCormick, and we're back with part two of

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<v Speaker 1>our exploration of Sagittarius, a star, the compact radio source,

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<v Speaker 1>the supermassive black hole we think at the center of

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<v Speaker 1>the Milky Way galaxy. Yeah, this is uh so, so,

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<v Speaker 1>as we mentioned in the last episode, we had what

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<v Speaker 1>three episodes we've done previously just on black holes in general,

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<v Speaker 1>and in these two episodes deal with supermassive black holes

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<v Speaker 1>more specifically. Uh and uh yeah, So if you're listening

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<v Speaker 1>to this episode, you do need to have at least

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<v Speaker 1>listened to the previous supermassive black hole episode. But I

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<v Speaker 1>think the supermassive black hole episodes are are are tailored

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<v Speaker 1>to stand on their own without necessarily having listened to

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<v Speaker 1>the previous black hole episodes. In either case, it is

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<v Speaker 1>recommended that you have seen either Walt Disney's The black

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<v Speaker 1>Hole or Event Horizon, so they have a proper basis

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<v Speaker 1>for all of our terrible jokes. Which one of those

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<v Speaker 1>two is more kid friendly? You think, Oh, blow. I

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<v Speaker 1>think it's the Disney movie, but the Disney movie is

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<v Speaker 1>also surprisingly dark. Like, uh, Anthony Perkins is eviscerated by

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<v Speaker 1>a killer robot um Like this is awful scene where

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<v Speaker 1>Maximilian the robots coming at him with the spinning blade

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<v Speaker 1>arm and he holds up like a giant dictionary to

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<v Speaker 1>block it, and he like cuts right through the dictionary

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<v Speaker 1>and uh and you know, apparently like just disembowels Anthony Perkins.

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<v Speaker 1>It cuts out the definition of in trails. Well you

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<v Speaker 1>don't see any in trails, but it's still pretty horrific.

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<v Speaker 1>There's some scary moments in it. But I loved it

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<v Speaker 1>as a kid. I really need to sit down and

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<v Speaker 1>watch it again. Now, speaking of a visceration, we're gonna

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<v Speaker 1>be talking about some somewhat violent events going on around

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<v Speaker 1>a black hole, or at least they presumed black hole today.

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<v Speaker 1>And one thing we promised you last time is that

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<v Speaker 1>we would answer a few questions every You've always wanted

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<v Speaker 1>to know about the supermassive black hole at the center

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<v Speaker 1>of the galaxy, but we're afraid to ask. And one

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<v Speaker 1>of the questions people most often ask about black holes.

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<v Speaker 1>If you're ready to jump right in robert Is. With

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<v Speaker 1>this big supermassive black hole at the center of the

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<v Speaker 1>Milky Way, will the rest of the Milky Way, including Earth,

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<v Speaker 1>one day gets sucked into this black hole? And I

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<v Speaker 1>was trying to find a good answer for this. I

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<v Speaker 1>think the short answer is no, or at least that's

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<v Speaker 1>not a given. All evidence indicates that, of course, the

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<v Speaker 1>Milky Way does have this supermassive black hole at its center.

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<v Speaker 1>The galaxy is sort of orbiting around it, or at

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<v Speaker 1>least roughly orbiting around it, But our Solar system is

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<v Speaker 1>in a stable orbit that is pretty far out. It's

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<v Speaker 1>something like light years away from the galactic center. And

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<v Speaker 1>black holes, even unbelievably giant black holes, still basically behave

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<v Speaker 1>like stars until you get really close to them. They're

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<v Speaker 1>not vacuum cleaners just sucking down the entire universe. You know.

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<v Speaker 1>They're objects traveling through space with a gravitational attraction that

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<v Speaker 1>is a product of their mass and your distance from them,

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<v Speaker 1>and like other objects, if you're far enough away, they're

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<v Speaker 1>gravitational attraction is negligible. So we've got no indication that

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<v Speaker 1>there is a risk of a black hole swallowing our

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<v Speaker 1>Solar system or the Earth or the rest of the

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<v Speaker 1>Milky Way. But of course, if anything as massive as

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<v Speaker 1>a black hole pass near our Solar system, I think,

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<v Speaker 1>I mean that that would be a problem. It might

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<v Speaker 1>not swallow our Solar System, but it's gravitational influence could

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<v Speaker 1>alter the orbits of the planets, which would be not good. Obviously,

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<v Speaker 1>life on Earth depends very heavily on us being where

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<v Speaker 1>we are relative to the Sun and other objects in

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<v Speaker 1>the Solar System staying where they are. You don't want

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<v Speaker 1>to say the orbits of comets and other objects like

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<v Speaker 1>that thrown out of whack, because then that can lead

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<v Speaker 1>to interplanetary bombardment. Yeah. I think the fact that a

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<v Speaker 1>black hole is an object is something that we do

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<v Speaker 1>have to come back to again and again because especially

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<v Speaker 1>with science fiction treatments, especially those especially the Disney black Hole.

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<v Speaker 1>So you know, there's this idea of like thinking of

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<v Speaker 1>it as a whirlpool it's a hungry, hungry hippo, yeah,

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<v Speaker 1>or thinking of it as a tunnel or just an

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<v Speaker 1>open like some of these you know, these analogies. They

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<v Speaker 1>they may be useful to a certain extent. It gives

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<v Speaker 1>us something to picture in our mind, but it kind

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<v Speaker 1>of drifts away from the idea that this is an object.

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<v Speaker 1>This is a highly dense thing, and now, of course

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<v Speaker 1>in the region really close to it, it doesn't behave

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<v Speaker 1>like most other objects too. But once once you get

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<v Speaker 1>farther away, I would say that the ways in which

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<v Speaker 1>it is unique become less relevant to you. Does that

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<v Speaker 1>make sense? Yes? Now, Um, you touched on some of this,

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<v Speaker 1>but but I was looking around like, Okay, what is

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<v Speaker 1>the scenario in which the supermassive black hole at the

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<v Speaker 1>center of our galaxy uh could conceivably destroy us? And

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<v Speaker 1>that there is one very strong possibility. So and we've

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<v Speaker 1>mentioned that our system is again in a stable orbit

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<v Speaker 1>around the galactic center. Um, we're not being pooled pulled

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<v Speaker 1>into Sagittarius M A star. But in four point five

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<v Speaker 1>billion years, the Milky Way galaxy will likely merge with

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<v Speaker 1>the Andromeda galaxy. And when this happens, all bets are off.

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<v Speaker 1>It's possible that everything gets pushed around, gets shuffled around,

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<v Speaker 1>and our solar system then could be gulped up or

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<v Speaker 1>just hideously disrupted by Sagittarius A star in the process. This,

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<v Speaker 1>according to Fabio Pacucci, b Hi Fellow at Harvard University

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<v Speaker 1>and Clay Fellow at the Smithsonian Astrophysical Observatory. He has

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<v Speaker 1>a wonderful ted Ed video about this. So if you

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<v Speaker 1>just go to if you go to YouTube and you

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<v Speaker 1>look up, just look up ted Ed in general, because

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<v Speaker 1>they're great educational short form videos to watch with the

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<v Speaker 1>entire family. We watch them all the time in my household.

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<v Speaker 1>But they have an extra excellent one about black holes

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<v Speaker 1>that Fabio is the contributor for. Yeah, now, when we

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<v Speaker 1>talk about the collision of galaxies, maybe someday we could

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<v Speaker 1>do a whole episode just on the upcoming collision between

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<v Speaker 1>the Milky Way and the Andromeda galaxy because yeah, so

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<v Speaker 1>they're on a collision course. Uh. On one hand, that

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<v Speaker 1>sounds like, okay, so that's just the end of everything, right, Actually,

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<v Speaker 1>I think not necessarily, because you have to remember, well,

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<v Speaker 1>you know there is a lot of space in between stars, right,

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<v Speaker 1>you know, there's there's a lot of space for things

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<v Speaker 1>to go by. But one of the big fears I

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<v Speaker 1>think is not necessarily that like Earth will smash directly

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<v Speaker 1>into a star from Andromeda or something. That the fear

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<v Speaker 1>is about gravitational disruption. Right, things moving past each other

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<v Speaker 1>in space can still have a perturbation effects on on stars,

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<v Speaker 1>on the planet's orbiting stars, on the objects and junk

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<v Speaker 1>in space all around stars. Well, none of that's good. Yeah,

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<v Speaker 1>I mean it's kind of like, and this is a

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<v Speaker 1>terrible analogy, I'm sure, but it's like, if two companies merge,

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<v Speaker 1>your your concern is not that, you know, if you're

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<v Speaker 1>an editor at one company and you emerge with another company,

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<v Speaker 1>you're not concerned that there's another editor over there that

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<v Speaker 1>you're just going to smack into so hard that you

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<v Speaker 1>both explode. No, you're worried about redundancies. You're worried about

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<v Speaker 1>reshuffling of titles and priorities, etcetera. Which you know, all

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<v Speaker 1>of that can be can can certainly be catastrophically disruptive

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<v Speaker 1>to your life. Um, but you're not worried about, you know,

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<v Speaker 1>like physically, you know, exploding or you know, melting into

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<v Speaker 1>them like Ron Silver and time coop. So I guess

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<v Speaker 1>that is possible. I mean, whenever things drift past each

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<v Speaker 1>other in space, there's always a potential for a collision.

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<v Speaker 1>It's just you know that that's not necessarily the thing

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<v Speaker 1>you should be worried about. I think the bigger thing

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<v Speaker 1>would be, Yeah, do you get thrown out of place?

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<v Speaker 1>You get thrown in? You getting thrown into the near

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<v Speaker 1>orbit or towards the black hole would obviously be bad

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<v Speaker 1>and and catastrophic in its own right for sure. Alright,

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<v Speaker 1>So the next big question that that you might be

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<v Speaker 1>wondering about. Could intelligent life forms live of and or

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<v Speaker 1>operate in orbit around a supermassive black hole, specifically our

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<v Speaker 1>supermassive black hole? Uh? You know, how would this factor

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<v Speaker 1>into a like a galactic civilization? Yeah? Or in the

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<v Speaker 1>in the galaxy center more generally, right, can you get

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<v Speaker 1>close to the galaxy center and have life there? This

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<v Speaker 1>seems debatable, right, Like, So there are some scientists who

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<v Speaker 1>think that just the way solar systems have a habitable

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<v Speaker 1>zone for planetary orbits, the galaxy as a whole has

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<v Speaker 1>some kind of habitable zone for star systems. Now in

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<v Speaker 1>star systems, of course, this habitable zone has temperature as

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<v Speaker 1>a primary variable, right, And this depends on the radiation

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<v Speaker 1>coming off of the parent star and how far away

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<v Speaker 1>that planet is from the star. So if your planet

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<v Speaker 1>is too close it's too hot to have liquid water,

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<v Speaker 1>you'd be something like mercury, or could be a hot

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<v Speaker 1>gas planet too far away, it's too cold to have

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<v Speaker 1>liquid water. You might be like Jupiter or Saturn, And

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<v Speaker 1>it's generally believed that liquid water is sort of a

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<v Speaker 1>prerequisite for life, or at least the kind of life

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<v Speaker 1>that we understand. Could it be the galaxies as a

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<v Speaker 1>whole have zones kind of like this where life is

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<v Speaker 1>statistically more likely to emerge, thrive, and survive than in

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<v Speaker 1>other zones of the galaxy. Some scientists have proposed this.

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<v Speaker 1>And if that is the case, what characterizes this zone? Uh?

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<v Speaker 1>First of all, if the proponents of the idea of

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<v Speaker 1>a galactic hapitable zone are correct, the zone of the

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<v Speaker 1>galaxy most suitable for life would tend to be a

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<v Speaker 1>sort of wide ring around the center of the galaxy,

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<v Speaker 1>so not farther out in the galactic halo, not not

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<v Speaker 1>way out there, but also not deep in the middle

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<v Speaker 1>near the galactic center. Now, why would this region be

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<v Speaker 1>potentially better to live in than say, the galactic center. Uh?

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<v Speaker 1>Just the short and basic version of your main consideration

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<v Speaker 1>here would be first of all, conditions that give rise

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<v Speaker 1>to life, and then the conditions that can sustain life.

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<v Speaker 1>So to give rise to life, we assume you need

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<v Speaker 1>first of all, terrestrial planets with stable orbits, right, and

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<v Speaker 1>and this means solar systems with a moderate amount of

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<v Speaker 1>metal in them. If you've got a solar system that's

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<v Speaker 1>like mostly hydrogen and doesn't have much that looks like

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<v Speaker 1>it could turn into rocky terrain, that probably means you're

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<v Speaker 1>not going to have life forms at least as we

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<v Speaker 1>understand them. But this isn't the primary concern for our question. Uh.

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<v Speaker 1>A big one for our question would be conditions that

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<v Speaker 1>can sustain life, Like how often or how intensely would

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<v Speaker 1>a planet in a given region be subjected to outside

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<v Speaker 1>damaging influences. Examples of this could be radiation from violent

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<v Speaker 1>nearby phenomena their stars. Uh, you know, violent things going

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<v Speaker 1>on Obviously nearby supernova would be a huge problem. If

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<v Speaker 1>a star anywhere near I you goes supernova, it will

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<v Speaker 1>blast your planet and could potentially sterilize it. Uh. The

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<v Speaker 1>near passage of of other massive objects like stars or

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<v Speaker 1>black holes is a huge issue that could potentially disturb

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<v Speaker 1>planetary orbits or bring about a bombardment of terrestrial planets

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<v Speaker 1>by comets and other junk from space. So like, if

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<v Speaker 1>something passes through your Solar System, and it's really heavy.

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<v Speaker 1>It will disturb these commetary orbits and then suddenly, you know,

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<v Speaker 1>things that haven't been hitting your planet for a long

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<v Speaker 1>time suddenly are This even makes me think about the

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<v Speaker 1>Lisa Randall dark matter and the dinosaurs hypothesis. I can't

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<v Speaker 1>remember if we ever talked about that on the show,

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<v Speaker 1>but basically her idea was that, you know, it's possible that, uh,

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<v Speaker 1>some extinction events in Earth's history are correlated to Earth's

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<v Speaker 1>passage through a region of the galactic plane where dark

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<v Speaker 1>matter is concentrated, and the extra gravitational influence of that

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<v Speaker 1>dark matter along that plane, uh disturbs the orbits of

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<v Speaker 1>some objects in the Solar System and makes you know,

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<v Speaker 1>the Earth get bombarded by stuff or maybe influences. I

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<v Speaker 1>can't remember. I think it was mainly comments she was

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<v Speaker 1>talking about, but maybe it was also vulcanism. I didn't

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<v Speaker 1>actually read the book, but I remember reading articles about

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<v Speaker 1>it when it came out. It seemed interesting. Maybe we'll

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<v Speaker 1>have to come back and take a look at that someday. Yeah,

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<v Speaker 1>that sounds frightening. I don't know whether that theory is

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<v Speaker 1>widely believed to to you know, have credence or not.

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<v Speaker 1>But but generally, if something disturbs the gravitational field of

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<v Speaker 1>your of your star system, that can be really bad

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<v Speaker 1>for anything living there. Yes, and so there are a

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<v Speaker 1>lot of variables at play, but generally these kinds of

0:12:35.840 --> 0:12:39.480
<v Speaker 1>dangerous conditions, like being subjected to more intense or more

0:12:39.520 --> 0:12:45.719
<v Speaker 1>frequent radiation or radiation events, and more more frequent disturbances

0:12:45.800 --> 0:12:49.080
<v Speaker 1>of gravity by large objects, that's going to be more

0:12:49.200 --> 0:12:53.520
<v Speaker 1>likely in densely packed regions of a galaxy, like closer

0:12:53.559 --> 0:12:56.560
<v Speaker 1>to the galactic center. The higher the density of nearby

0:12:56.679 --> 0:13:00.120
<v Speaker 1>stars and other stuff, the more dangerous there are. And

0:13:00.120 --> 0:13:02.880
<v Speaker 1>a very crude analogy is you're more likely to have

0:13:02.960 --> 0:13:05.520
<v Speaker 1>some kind of auto accident or mishap on a busy

0:13:05.600 --> 0:13:08.679
<v Speaker 1>city street than on some empty country road. Right, Yeah,

0:13:08.720 --> 0:13:10.600
<v Speaker 1>they're just well there's you know, there's just more going

0:13:10.640 --> 0:13:13.360
<v Speaker 1>on there. But then again, I do want to say

0:13:13.480 --> 0:13:15.640
<v Speaker 1>it seems like a lot of the writing about galactic

0:13:15.679 --> 0:13:19.680
<v Speaker 1>habitable zones is subject to ongoing criticism and dispute. Uh,

0:13:19.920 --> 0:13:22.400
<v Speaker 1>it does seem clear that there are at least some

0:13:22.600 --> 0:13:26.400
<v Speaker 1>risks to life associated with moving closer to the galactic center.

0:13:26.880 --> 0:13:29.719
<v Speaker 1>But you know where exactly this habitable zone of a

0:13:29.760 --> 0:13:32.920
<v Speaker 1>galaxy would be if it in fact is true that

0:13:33.040 --> 0:13:36.280
<v Speaker 1>some regions of the galaxy or on average more habitable

0:13:36.280 --> 0:13:38.880
<v Speaker 1>than others. I think that's highly disputed. So this is

0:13:38.920 --> 0:13:41.280
<v Speaker 1>not settled science. Alright, We're gonna take a quick break.

0:13:41.280 --> 0:13:43.480
<v Speaker 1>When we come back, we have a little more information

0:13:43.520 --> 0:13:48.240
<v Speaker 1>about just how chaotic and destructive uh, the inner reaches

0:13:48.280 --> 0:13:50.880
<v Speaker 1>of the galaxy seem to be, and then we'll move

0:13:50.880 --> 0:13:55.880
<v Speaker 1>on to some other possibilities for uh, extraterrestrial activity in

0:13:55.880 --> 0:13:59.800
<v Speaker 1>the inner galaxy. All right, we're back, all right, So

0:13:59.840 --> 0:14:03.400
<v Speaker 1>we were just talking about this question of like, could you,

0:14:03.400 --> 0:14:06.160
<v Speaker 1>you know, could you tend to find life for intelligent

0:14:06.240 --> 0:14:09.480
<v Speaker 1>life forms in orbit around a central supermassive black hole

0:14:09.520 --> 0:14:12.360
<v Speaker 1>in our galaxy or in the galactic center more generally,

0:14:12.600 --> 0:14:15.160
<v Speaker 1>would you expect to see something like that? Would it

0:14:15.200 --> 0:14:18.480
<v Speaker 1>be a survivable region? And and it uh, it seems

0:14:18.520 --> 0:14:20.560
<v Speaker 1>like this is not fully settled, but we were discussing

0:14:20.600 --> 0:14:25.240
<v Speaker 1>some potential risks of living in the galactic center. Yes,

0:14:25.480 --> 0:14:27.440
<v Speaker 1>I was looking around for some more details on this,

0:14:27.520 --> 0:14:29.560
<v Speaker 1>and this brought me as questions like this often due

0:14:29.600 --> 0:14:33.720
<v Speaker 1>to Centauri Dreams, which is a wonderful space website and

0:14:33.760 --> 0:14:36.560
<v Speaker 1>I was reading a blog post by the writer Paul

0:14:36.640 --> 0:14:40.840
<v Speaker 1>Gilster of The Planetary Society, in which he looks to

0:14:40.880 --> 0:14:44.720
<v Speaker 1>the work of Sergey n Action at Leicester on the

0:14:44.760 --> 0:14:48.600
<v Speaker 1>idea that the doughnut shaped dust clouds obscuring half of

0:14:48.920 --> 0:14:52.200
<v Speaker 1>supermassive black holes might be the you know, the result

0:14:52.280 --> 0:14:56.120
<v Speaker 1>of crashes between planets and asteroids occurring at a thousand

0:14:56.160 --> 0:15:00.760
<v Speaker 1>kilometers per second speeds, pounding everything into micros copic dust.

0:15:01.120 --> 0:15:03.520
<v Speaker 1>So it's a realm of you know, of a violent

0:15:03.640 --> 0:15:07.560
<v Speaker 1>collision high radiation. But he points out that while those

0:15:07.560 --> 0:15:09.840
<v Speaker 1>planets are doomed, you know anything, actually any of the

0:15:09.840 --> 0:15:13.160
<v Speaker 1>planets actually in that region or potentially doomed, the resulting

0:15:13.320 --> 0:15:17.480
<v Speaker 1>dust blocks harmful radiation from all of this chaos from

0:15:17.480 --> 0:15:21.600
<v Speaker 1>reaching the rest of the galaxy, the host galaxy. That's interesting.

0:15:21.600 --> 0:15:23.520
<v Speaker 1>I mean, yeah, we were talking in the last episode

0:15:23.520 --> 0:15:26.960
<v Speaker 1>about how dust clouds obscure the galactic center from our

0:15:27.000 --> 0:15:29.440
<v Speaker 1>point of view, like it's harder to do astronomy looking

0:15:29.440 --> 0:15:32.320
<v Speaker 1>towards the galactic center. I mean, I would imagine that

0:15:32.400 --> 0:15:34.560
<v Speaker 1>brightness has something to do with it. But also, yeah,

0:15:34.600 --> 0:15:38.240
<v Speaker 1>the dust blocks our view and does significant dimming. It

0:15:38.320 --> 0:15:41.400
<v Speaker 1>causes many magnitudes of extinction to the sources coming from

0:15:41.400 --> 0:15:43.680
<v Speaker 1>that direction. But we do have methods of looking that

0:15:43.720 --> 0:15:46.560
<v Speaker 1>way now, and we can do astronomy focused on the

0:15:46.560 --> 0:15:48.440
<v Speaker 1>center of the galaxy, I think, you know, due to

0:15:48.480 --> 0:15:52.000
<v Speaker 1>stuff like looking at infrared and X rays. I was

0:15:52.040 --> 0:15:54.440
<v Speaker 1>also looking around, uh and found some writings on this

0:15:54.520 --> 0:15:57.600
<v Speaker 1>from Phil Plate of Bad Astronomy, always a great read

0:15:57.680 --> 0:16:00.560
<v Speaker 1>on space related topics, and he points out in some

0:16:00.640 --> 0:16:05.520
<v Speaker 1>galaxies called active galaxies, gas and dust fall into the

0:16:05.560 --> 0:16:07.800
<v Speaker 1>yawning black hole at the center of the galaxy, forming

0:16:07.800 --> 0:16:12.040
<v Speaker 1>a disc of material sometimes hundreds of light years across. Again,

0:16:12.120 --> 0:16:14.120
<v Speaker 1>this here is going to be a realm of high temperatures,

0:16:14.200 --> 0:16:17.800
<v Speaker 1>high radiation, and intense light that outshines the rest of

0:16:17.800 --> 0:16:20.480
<v Speaker 1>the galaxy, and that would mirror some of the phenomenon

0:16:20.480 --> 0:16:22.560
<v Speaker 1>we were talking about in the last episode, where yeah,

0:16:22.600 --> 0:16:25.920
<v Speaker 1>like you've got like this quasar or something super powerful

0:16:25.960 --> 0:16:28.400
<v Speaker 1>in the middle of the galaxy that just sort of

0:16:28.440 --> 0:16:31.480
<v Speaker 1>like you know, it sort of is the galaxy, right,

0:16:31.680 --> 0:16:35.200
<v Speaker 1>But fortunately, the Milky Way galaxy is not an active galaxy.

0:16:35.400 --> 0:16:38.760
<v Speaker 1>It's a quiescent galaxy, so it's not quite the cosmic

0:16:38.840 --> 0:16:41.880
<v Speaker 1>forge we find in other galaxies where you know, it's

0:16:41.920 --> 0:16:46.040
<v Speaker 1>just super intense. It is to a certain extent slumbering,

0:16:46.480 --> 0:16:48.680
<v Speaker 1>and we're able. I mean, I keep coming back to

0:16:48.720 --> 0:16:51.720
<v Speaker 1>the idea of their just being like an awful, all

0:16:51.800 --> 0:16:55.960
<v Speaker 1>powerful eldric deity the center of the cosmos, and we're

0:16:56.000 --> 0:16:58.840
<v Speaker 1>just lucky that it's that we're in a cosmos. It's

0:16:58.880 --> 0:17:01.360
<v Speaker 1>a little worn out and take in a lengthy slumber.

0:17:01.400 --> 0:17:03.640
<v Speaker 1>I think at the end of the last episode you Were,

0:17:03.680 --> 0:17:06.359
<v Speaker 1>You Were, you sort of fought against the idea of

0:17:06.359 --> 0:17:09.000
<v Speaker 1>thinking of black I know, I don't want to think

0:17:09.040 --> 0:17:10.840
<v Speaker 1>of a black hole as being you know, and this

0:17:11.040 --> 0:17:14.160
<v Speaker 1>has his off figure, but it's hard and it's hard

0:17:14.200 --> 0:17:17.439
<v Speaker 1>not to when we used to read things like this.

0:17:17.600 --> 0:17:20.120
<v Speaker 1>So I guess we've been looking at answers for mostly

0:17:20.200 --> 0:17:22.160
<v Speaker 1>like no, we're looking at the idea of the inner

0:17:22.200 --> 0:17:26.320
<v Speaker 1>galaxy is a place where you're probably not encountering um,

0:17:26.359 --> 0:17:30.280
<v Speaker 1>you know, planets where life is evolved. There. There are

0:17:30.280 --> 0:17:33.199
<v Speaker 1>a lot of risks in the galactic center because you know,

0:17:33.320 --> 0:17:36.120
<v Speaker 1>the things are more densely packed. There's probably more radiation risk,

0:17:36.200 --> 0:17:39.080
<v Speaker 1>probably more gravity disturbance risk. But at the same time

0:17:39.119 --> 0:17:42.040
<v Speaker 1>there are more stars. You might just get more chances

0:17:42.119 --> 0:17:45.040
<v Speaker 1>for things to evolve there. So it's it's like I

0:17:45.080 --> 0:17:47.600
<v Speaker 1>was saying, it's not settled science, but you can point

0:17:47.640 --> 0:17:49.520
<v Speaker 1>to some things going on there and say it looks

0:17:49.560 --> 0:17:53.240
<v Speaker 1>like there are are risky phenomena near the galactic center. Now, indeed,

0:17:53.240 --> 0:17:56.639
<v Speaker 1>if we are dealing with habitable zones and uh, you know,

0:17:57.000 --> 0:18:00.280
<v Speaker 1>uninhabitable zones of the galaxy, one thing to keep in

0:18:00.359 --> 0:18:04.479
<v Speaker 1>mind is that technology can potentially change things. Like just

0:18:04.520 --> 0:18:07.840
<v Speaker 1>look to our solar system. Yes, Earth is the like

0:18:07.960 --> 0:18:11.520
<v Speaker 1>it's it's the bowl of porridge. That's just right. But

0:18:11.840 --> 0:18:13.919
<v Speaker 1>we've discussed on the show plenty of times that you know,

0:18:13.960 --> 0:18:17.359
<v Speaker 1>there are plans, there are ideas and concepts where with

0:18:17.400 --> 0:18:22.600
<v Speaker 1>sufficient technology, humans could live on Mars, they could live

0:18:22.680 --> 0:18:25.399
<v Speaker 1>in the clouds of Venus. Even here on Earth we

0:18:25.440 --> 0:18:28.720
<v Speaker 1>have a neutrino observatory at the South Pole. You know,

0:18:28.800 --> 0:18:32.760
<v Speaker 1>we've got or at least yeah, deepen Antarctica. That's not

0:18:32.920 --> 0:18:36.520
<v Speaker 1>a place that's inhabitable by mammals. So you know, so

0:18:36.680 --> 0:18:41.280
<v Speaker 1>like we we have found technological ways of overcoming the

0:18:41.400 --> 0:18:44.920
<v Speaker 1>environmental limitations imposed by the universe. And you can see

0:18:44.920 --> 0:18:48.119
<v Speaker 1>that even without us leaving our host planet. So you know,

0:18:48.160 --> 0:18:50.600
<v Speaker 1>if you can build a research station on the South Pole,

0:18:50.640 --> 0:18:52.960
<v Speaker 1>where no mammal like us should be able to survive

0:18:53.320 --> 0:18:55.520
<v Speaker 1>if you can potentially build it. Oh, if you can

0:18:55.520 --> 0:18:57.720
<v Speaker 1>build an I. S. S. Yeah, and live out in space.

0:18:58.080 --> 0:19:01.919
<v Speaker 1>Yeah you can imagine. Okay, just extra appellate that up. However,

0:19:01.920 --> 0:19:04.800
<v Speaker 1>many orders of magnitude of whatever scale you're talking about

0:19:05.400 --> 0:19:09.600
<v Speaker 1>to our power to live beyond our original organic means. Yea.

0:19:09.640 --> 0:19:11.680
<v Speaker 1>So we have to come back to something we've discussed

0:19:11.680 --> 0:19:15.040
<v Speaker 1>in the show before, sort of a propose technological ladder

0:19:15.119 --> 0:19:18.600
<v Speaker 1>to um to godhood if you will. The Cardassie of

0:19:18.720 --> 0:19:22.200
<v Speaker 1>scale an old favorite. Yes, so you got you got.

0:19:22.320 --> 0:19:25.359
<v Speaker 1>Basically you've got type one, Type two, and type three,

0:19:25.600 --> 0:19:28.240
<v Speaker 1>and you know, I've also seen people discuss the possibility

0:19:28.240 --> 0:19:30.120
<v Speaker 1>of the type four. But a Type four is so

0:19:30.160 --> 0:19:32.200
<v Speaker 1>far beyond where we are now it's almost not even

0:19:32.240 --> 0:19:34.520
<v Speaker 1>worth thinking about. Well, I'd say even like type three

0:19:34.680 --> 0:19:37.880
<v Speaker 1>is hard to imagine what that would look like. Uh,

0:19:37.920 --> 0:19:40.280
<v Speaker 1>you know, we've got more like science fiction that kind

0:19:40.280 --> 0:19:42.760
<v Speaker 1>of deals on the realm of one and two. Yeah,

0:19:43.119 --> 0:19:46.840
<v Speaker 1>so we're not even type ones yet. Time close. Yeah,

0:19:46.840 --> 0:19:50.520
<v Speaker 1>Type A Type one civilization, the cardassi of scale should

0:19:50.560 --> 0:19:53.879
<v Speaker 1>be capable of harnessing all the energy of their planet,

0:19:53.920 --> 0:19:55.960
<v Speaker 1>because basically that's what the scale is about. It's about,

0:19:56.240 --> 0:20:00.639
<v Speaker 1>you know, civilization's ability to to harness in yeah, to

0:20:00.720 --> 0:20:03.040
<v Speaker 1>take what's there in the universe and turn that into

0:20:03.119 --> 0:20:06.080
<v Speaker 1>the ability to do work. Now, of course that doesn't

0:20:06.080 --> 0:20:08.400
<v Speaker 1>necessarily mean work, like it's hard to do. That could

0:20:08.400 --> 0:20:10.720
<v Speaker 1>be you know, operating the video game systems of the

0:20:10.760 --> 0:20:14.720
<v Speaker 1>future or whatever to turn it into usable energy. Right. Yeah.

0:20:14.840 --> 0:20:17.320
<v Speaker 1>So so again we're not type one yet. If we

0:20:17.359 --> 0:20:20.760
<v Speaker 1>could harness all the power, all the energy of our planet,

0:20:20.880 --> 0:20:23.679
<v Speaker 1>we would be type one. The next step is is

0:20:23.720 --> 0:20:25.919
<v Speaker 1>a is a type two in which a civilization has

0:20:25.960 --> 0:20:30.960
<v Speaker 1>become masters of their own star, essentially solar solar system

0:20:31.119 --> 0:20:35.479
<v Speaker 1>level power. And then that type three, which is an

0:20:35.680 --> 0:20:39.199
<v Speaker 1>an enormous step. Then from from from step to tow

0:20:40.119 --> 0:20:43.240
<v Speaker 1>a step three civilization has the power of an entire

0:20:43.359 --> 0:20:46.600
<v Speaker 1>galaxy at its disposal. That's hard to imagine, it is,

0:20:46.640 --> 0:20:48.639
<v Speaker 1>It is very difficult to imagine it. It It gets so

0:20:48.680 --> 0:20:52.520
<v Speaker 1>difficult to imagine it's almost ridiculous to try and think

0:20:52.520 --> 0:20:55.840
<v Speaker 1>of what is beyond that, you know, uh, and and

0:20:55.880 --> 0:20:58.160
<v Speaker 1>so most of our contemplations deal with one, two and three.

0:20:58.440 --> 0:21:01.200
<v Speaker 1>Most deal with one and two. So level one and

0:21:01.280 --> 0:21:04.320
<v Speaker 1>two on the Kardaship scale would theoretically have access to

0:21:04.359 --> 0:21:08.480
<v Speaker 1>technology we refer to as a Dyson sphere, named for

0:21:08.640 --> 0:21:13.639
<v Speaker 1>theoretical physicist Freeman Dyson, and these are essentially means of

0:21:13.880 --> 0:21:17.040
<v Speaker 1>surrounding a power source and harvesting all of its energy.

0:21:17.520 --> 0:21:19.560
<v Speaker 1>There are different varieties of this. You don't need to

0:21:19.600 --> 0:21:22.960
<v Speaker 1>necessarily think of a hard sphere, um though I love

0:21:23.000 --> 0:21:24.800
<v Speaker 1>too because it should pops up in that episode of

0:21:24.800 --> 0:21:27.080
<v Speaker 1>Star Trek. But it could also be you know, more

0:21:27.160 --> 0:21:29.000
<v Speaker 1>like a dice in cloud. It could be you know,

0:21:29.119 --> 0:21:33.840
<v Speaker 1>satellites surrounding something and absorbing its energy. Um. So it's

0:21:33.880 --> 0:21:38.520
<v Speaker 1>maybe oversimplified, but the classic example would be just surrounding

0:21:38.560 --> 0:21:41.560
<v Speaker 1>the Sun with something like solar panels, so you get

0:21:41.600 --> 0:21:43.359
<v Speaker 1>all of the energy out of it. You can just

0:21:43.400 --> 0:21:46.560
<v Speaker 1>sort of like release the waste exhaust outside and and

0:21:46.680 --> 0:21:49.760
<v Speaker 1>use everything the sun can give you. Yeah, the still

0:21:49.800 --> 0:21:52.399
<v Speaker 1>suits of Dune are sort of like Dyson spheres for

0:21:52.520 --> 0:21:56.800
<v Speaker 1>human sweat, you know, for human moisture. Don't waste to drop.

0:21:57.680 --> 0:22:00.760
<v Speaker 1>So how does this tie into supermassive black hole old holes?

0:22:00.760 --> 0:22:04.160
<v Speaker 1>You might wonder, Well, I was reading a very interesting paper. Uh,

0:22:04.160 --> 0:22:06.919
<v Speaker 1>this is from a two thousand and eleven edition of

0:22:06.960 --> 0:22:10.560
<v Speaker 1>the Journal of the British Interplanetary Society. And this is

0:22:10.560 --> 0:22:14.000
<v Speaker 1>by an o U and you Ku titled Type three

0:22:14.080 --> 0:22:18.040
<v Speaker 1>Dicen sphere of highly advanced civilizations around a supermassive black hole.

0:22:19.320 --> 0:22:23.560
<v Speaker 1>Uh So, I'm gonna read a quick quote from this quote.

0:22:24.720 --> 0:22:27.919
<v Speaker 1>A society of a highly advanced civilization is supposed to

0:22:27.960 --> 0:22:32.359
<v Speaker 1>require a huge amount of energy to operate the social system.

0:22:32.400 --> 0:22:35.720
<v Speaker 1>As the gravitational energy released by the accretion of matter

0:22:35.840 --> 0:22:39.400
<v Speaker 1>into a supermassive black hole is huge, a system must

0:22:39.440 --> 0:22:42.679
<v Speaker 1>be developed to use this energy. In such a society,

0:22:42.960 --> 0:22:45.399
<v Speaker 1>the condition around a supermassive black hole at the center

0:22:45.480 --> 0:22:48.840
<v Speaker 1>of a of a galaxy would be more efficient both

0:22:48.880 --> 0:22:52.320
<v Speaker 1>in extracting energy and exhausting the waste energy for advanced

0:22:52.320 --> 0:22:57.800
<v Speaker 1>civilizations than those of a Dicen sphere. So basically they're arguing, like, hey,

0:22:57.920 --> 0:22:59.919
<v Speaker 1>like we've touched on before, there's a lot going on

0:23:00.000 --> 0:23:01.800
<v Speaker 1>on at the center of the galaxy. There's a lot

0:23:01.840 --> 0:23:05.320
<v Speaker 1>of energy at the center of the galaxy. Any sufficiently

0:23:05.359 --> 0:23:09.840
<v Speaker 1>advanced civilization would go where the energy is and presumably

0:23:09.840 --> 0:23:13.200
<v Speaker 1>have the technology to harness it right, extract that energy

0:23:13.200 --> 0:23:15.280
<v Speaker 1>and do something with it rather than letting it just

0:23:15.359 --> 0:23:18.359
<v Speaker 1>turn into radiation and in space. Yeah. So yeah. They

0:23:18.359 --> 0:23:21.760
<v Speaker 1>point out that a huge amount of radiation energy generates

0:23:21.760 --> 0:23:24.200
<v Speaker 1>in close vicinity to a supermassive black hole, and here,

0:23:24.280 --> 0:23:27.880
<v Speaker 1>you know, this accretion disc rotates around it, so the

0:23:27.920 --> 0:23:31.720
<v Speaker 1>potential energy of the accreting matter releases to form a

0:23:31.760 --> 0:23:35.040
<v Speaker 1>hot and dense disk. Sorry, I was just for a

0:23:35.080 --> 0:23:37.840
<v Speaker 1>moment trying to imagine what we would do with it,

0:23:37.920 --> 0:23:40.479
<v Speaker 1>and it would be like, I, let's load up, you know,

0:23:40.600 --> 0:23:44.040
<v Speaker 1>ten billion spaceships full of coal and take them to

0:23:44.200 --> 0:23:47.320
<v Speaker 1>the center of the galaxy and let the supermassive black

0:23:47.320 --> 0:23:51.199
<v Speaker 1>hole burn the coal and then we can use the

0:23:51.200 --> 0:23:54.400
<v Speaker 1>heat from the cold power. So yeah, that's our solution.

0:23:55.480 --> 0:23:58.320
<v Speaker 1>Uh yeah, that's not quite the system that that that

0:23:58.400 --> 0:24:01.600
<v Speaker 1>they're proposing. Here, this is what they add quote, radiation

0:24:01.720 --> 0:24:04.480
<v Speaker 1>from the accretion disk will be collected by a mirror

0:24:04.520 --> 0:24:09.040
<v Speaker 1>system as a type three dycen sphere. Waste material and

0:24:09.200 --> 0:24:12.400
<v Speaker 1>energy could be thrown off towards the central supermassive black hole,

0:24:12.640 --> 0:24:15.320
<v Speaker 1>and the supermassive black hole would be the final reservoir

0:24:15.440 --> 0:24:19.359
<v Speaker 1>for all the waste materials for any civilizations. Thus, the

0:24:19.400 --> 0:24:23.160
<v Speaker 1>most advanced civilizations would develop their activities using a supermassive

0:24:23.359 --> 0:24:27.439
<v Speaker 1>black hole efficiency, putting the power plants around the supermassive

0:24:27.480 --> 0:24:31.000
<v Speaker 1>black hole at the center of their home galaxy. Wow, well,

0:24:31.040 --> 0:24:34.840
<v Speaker 1>I mean that's pretty out there. Yeah, that that's interesting. Yeah.

0:24:34.840 --> 0:24:37.639
<v Speaker 1>So from here they lay out a power plant system

0:24:37.680 --> 0:24:41.040
<v Speaker 1>that amounts to a sort of Dyson's sphere or shell.

0:24:41.480 --> 0:24:44.639
<v Speaker 1>The energy from the power plants is then transferred by

0:24:44.680 --> 0:24:49.600
<v Speaker 1>electromagnetic waves the habitats of advanced civilizations, which would be

0:24:49.640 --> 0:24:56.320
<v Speaker 1>as imagining more sustainable, stable regions. And then these transmissions

0:24:56.320 --> 0:24:58.720
<v Speaker 1>would also serve would serve as a power grid, but

0:24:58.800 --> 0:25:02.680
<v Speaker 1>also as highways, four vessels, uh, you know, more or

0:25:02.760 --> 0:25:05.320
<v Speaker 1>less sailing them as if they were sailing, you know,

0:25:05.400 --> 0:25:09.960
<v Speaker 1>the solar wind. So putting power plants on a supermassive

0:25:10.000 --> 0:25:13.520
<v Speaker 1>black hole, well, well, not quite on, but close to.

0:25:13.680 --> 0:25:15.719
<v Speaker 1>And then they touched on that to uh you know,

0:25:15.960 --> 0:25:18.560
<v Speaker 1>basically asking asking answering the question how close would these

0:25:18.560 --> 0:25:22.840
<v Speaker 1>power plants be. Yeah, they say that considering Sagittarius a star,

0:25:23.000 --> 0:25:27.520
<v Speaker 1>that the closest you would be dealing with the closest distance,

0:25:27.680 --> 0:25:32.160
<v Speaker 1>the closest orbit would be six hundred r s. That's

0:25:32.200 --> 0:25:35.679
<v Speaker 1>a swords child radius, and uh, they say that the

0:25:35.760 --> 0:25:38.240
<v Speaker 1>proper area for the power plants and their model would

0:25:38.280 --> 0:25:41.359
<v Speaker 1>be around one hundred three to one hundred four r

0:25:41.600 --> 0:25:46.400
<v Speaker 1>s is um. Also basically just like a hundred of

0:25:46.560 --> 0:25:50.480
<v Speaker 1>the radius of the black hole region itself out And

0:25:50.560 --> 0:25:55.160
<v Speaker 1>that sounds frighteningly close. But then again, conceivably this would

0:25:55.160 --> 0:25:59.280
<v Speaker 1>be a civilization that assuming they're not entirely technological by

0:25:59.320 --> 0:26:01.359
<v Speaker 1>this point, you know, and they even have any kind

0:26:01.400 --> 0:26:05.880
<v Speaker 1>of like you know, a physical remainder in their their

0:26:05.960 --> 0:26:09.400
<v Speaker 1>their being and their culture. Again, it's difficult to imagine

0:26:09.440 --> 0:26:11.800
<v Speaker 1>some of these civilizations with him they could consist of.

0:26:12.320 --> 0:26:16.840
<v Speaker 1>But even if they were in some way organic, still like,

0:26:17.040 --> 0:26:19.800
<v Speaker 1>surely this would be the domain of robots that they

0:26:19.840 --> 0:26:22.640
<v Speaker 1>send out, sending the robots in to do the hard

0:26:22.640 --> 0:26:25.399
<v Speaker 1>work at the center and then being that energy back

0:26:26.040 --> 0:26:29.600
<v Speaker 1>to the centers of civilization. I feel so two ways

0:26:29.640 --> 0:26:32.960
<v Speaker 1>about this, because on one hand, it's like, I love

0:26:33.040 --> 0:26:35.800
<v Speaker 1>the idea of people trying to work out how CARDASHEV

0:26:35.920 --> 0:26:40.040
<v Speaker 1>level three power plants would work out would function. But

0:26:40.080 --> 0:26:42.320
<v Speaker 1>on the other hand, it's just like, we don't even

0:26:42.440 --> 0:26:45.640
<v Speaker 1>we're not even you know, level one yet, So you

0:26:45.640 --> 0:26:48.840
<v Speaker 1>you have to imagine that even if these authors are

0:26:48.840 --> 0:26:51.159
<v Speaker 1>totally on the right track, there's probably a lot of

0:26:51.200 --> 0:26:54.119
<v Speaker 1>details we haven't we haven't really faced yet and and

0:26:54.160 --> 0:26:56.680
<v Speaker 1>don't really know how to incorporate. But at the same time,

0:26:56.800 --> 0:27:00.280
<v Speaker 1>this is this is such a blessed project, trying to eagine.

0:27:00.320 --> 0:27:03.280
<v Speaker 1>All right, maybe like a billion years in the future,

0:27:03.480 --> 0:27:06.840
<v Speaker 1>what does what does the civilization do to get their power? Yeah?

0:27:06.840 --> 0:27:08.919
<v Speaker 1>I love I love papers like this. Now, now to

0:27:08.920 --> 0:27:11.880
<v Speaker 1>be clear again, this is all theoretical and it's something

0:27:11.960 --> 0:27:15.320
<v Speaker 1>the authors say we might look for, but there's no

0:27:15.400 --> 0:27:18.920
<v Speaker 1>evidence that something like this is actually going on anywhere

0:27:18.920 --> 0:27:21.920
<v Speaker 1>in the universe. Okay, So this is another example, as

0:27:21.960 --> 0:27:26.280
<v Speaker 1>has often been done before, where working out the details

0:27:26.320 --> 0:27:31.400
<v Speaker 1>of a potential uh Dyson sphere type project would be

0:27:31.560 --> 0:27:34.919
<v Speaker 1>mostly useful in the search for extraterrestrial life. Right, right,

0:27:35.080 --> 0:27:37.600
<v Speaker 1>What would be the signatures of this type of technology?

0:27:37.840 --> 0:27:40.160
<v Speaker 1>Do we look out into the universe and see anything

0:27:40.240 --> 0:27:43.520
<v Speaker 1>like that? Right? And and and Astronomers have observed objects

0:27:43.560 --> 0:27:47.960
<v Speaker 1>that could potentially be explained by dimming due to a

0:27:48.080 --> 0:27:51.800
<v Speaker 1>Dyson sphere. For instance, in two thousand and sixteen, scientists

0:27:51.840 --> 0:27:56.000
<v Speaker 1>observed a dimming of the star Epic to zero four

0:27:56.080 --> 0:27:59.240
<v Speaker 1>to seven eight, nine one six that was out of

0:27:59.320 --> 0:28:02.439
<v Speaker 1>keeping with a large planet, you know, passing between us.

0:28:02.520 --> 0:28:06.920
<v Speaker 1>And they presented a few possible explanations, but the last

0:28:07.119 --> 0:28:10.440
<v Speaker 1>of them was a dicense fhere, because there's always aliens,

0:28:11.040 --> 0:28:13.879
<v Speaker 1>should always be the last explanation we turned to, no

0:28:13.920 --> 0:28:17.199
<v Speaker 1>matter how exciting that explanation might be. But which of

0:28:17.200 --> 0:28:20.720
<v Speaker 1>their potential explanations made the headlines? Well, of course it's

0:28:20.720 --> 0:28:22.760
<v Speaker 1>the dicense fhere right. In fact, I think one of

0:28:22.760 --> 0:28:25.120
<v Speaker 1>the headlines I was looking at was researchers just found

0:28:25.119 --> 0:28:30.760
<v Speaker 1>a second dicense fhere star, What what happened to the

0:28:30.800 --> 0:28:33.480
<v Speaker 1>first one? That's brilliant? Well, I mean, like, like I said,

0:28:33.480 --> 0:28:35.920
<v Speaker 1>there have been at least a couple of cases where

0:28:36.000 --> 0:28:38.120
<v Speaker 1>people have seen something and they're like, we don't really

0:28:38.160 --> 0:28:40.720
<v Speaker 1>fully understand what it is, but here a list of

0:28:40.720 --> 0:28:43.360
<v Speaker 1>things it could be. And yeah, number three or four

0:28:43.440 --> 0:28:47.000
<v Speaker 1>or five is sometimes a dicense here. Yeah. Um, I

0:28:47.120 --> 0:28:49.200
<v Speaker 1>just like that. It sounds like it was assumed that

0:28:49.320 --> 0:28:51.960
<v Speaker 1>the first one they found actually is a license fhere,

0:28:52.000 --> 0:28:54.240
<v Speaker 1>and not just like there's an off chance that it

0:28:54.280 --> 0:28:56.560
<v Speaker 1>could be and that would be consistent with what we saw.

0:28:56.960 --> 0:28:58.960
<v Speaker 1>All right. On that note, We're gonna take one more break,

0:28:59.000 --> 0:29:01.280
<v Speaker 1>but when we come back, we have some more mysteries

0:29:01.280 --> 0:29:05.040
<v Speaker 1>to consider, not about uh, you know, hypothetical you know,

0:29:05.840 --> 0:29:11.680
<v Speaker 1>super advanced technological societies, but rather mysteries concerning the supermassive

0:29:11.720 --> 0:29:16.320
<v Speaker 1>black hole at the center of our galaxy. Thank all right,

0:29:16.360 --> 0:29:18.560
<v Speaker 1>we're back. Now it's time to talk about how our

0:29:18.600 --> 0:29:22.920
<v Speaker 1>own galaxy supermassive black hole, Sagittarius A star has been

0:29:22.920 --> 0:29:27.040
<v Speaker 1>showing some weird and mysterious behavior lately, just just in

0:29:27.080 --> 0:29:29.400
<v Speaker 1>the past few years or this year. Yeah, that's right.

0:29:29.720 --> 0:29:32.960
<v Speaker 1>NASA Schandra X ray Observatory has observed a mysterious daily

0:29:33.000 --> 0:29:36.320
<v Speaker 1>flares from Sagittarius A Star, and it leads us to,

0:29:36.440 --> 0:29:39.240
<v Speaker 1>you know, wonder what's going on? Um so. One theory

0:29:39.360 --> 0:29:42.480
<v Speaker 1>is that the dust cloud around it contains comments and

0:29:42.520 --> 0:29:46.400
<v Speaker 1>asteroids stripped away from other stars, and then when collisions occur,

0:29:46.520 --> 0:29:51.840
<v Speaker 1>it's sometimes sends one off into Sagittarius A Star. And

0:29:51.920 --> 0:29:54.720
<v Speaker 1>according to a NASA report from two thousand twelve, quote,

0:29:54.960 --> 0:29:57.760
<v Speaker 1>if the asteroid passes within about one million miles of

0:29:58.000 --> 0:30:00.440
<v Speaker 1>the black hole, roughly the distance between the Earth the Sun,

0:30:00.760 --> 0:30:03.120
<v Speaker 1>it would be torn to pieces by the tidal forces

0:30:03.160 --> 0:30:05.440
<v Speaker 1>from the black hole. So basically, you know, you're just

0:30:05.680 --> 0:30:08.719
<v Speaker 1>ripping apart a huge chunk of metal or rock in space, right,

0:30:08.720 --> 0:30:11.000
<v Speaker 1>and this produces a flare as the asteroid than as

0:30:11.080 --> 0:30:14.560
<v Speaker 1>the pieces of it consumed by the black hole. Comets

0:30:14.560 --> 0:30:18.160
<v Speaker 1>have been observed to impact our Sun with almost identical

0:30:18.200 --> 0:30:21.920
<v Speaker 1>frequency uh and with a resulting flare. You can even

0:30:21.960 --> 0:30:24.600
<v Speaker 1>get a really cool flare in astronomy just looking at

0:30:24.640 --> 0:30:26.600
<v Speaker 1>like Jupiter. Have you seen some of these when like

0:30:26.640 --> 0:30:30.920
<v Speaker 1>a comet goes into Jupiter. Yeah, amazing. Now there have

0:30:31.040 --> 0:30:36.080
<v Speaker 1>been other recent observations of of big flare ups right. Yeah.

0:30:36.160 --> 0:30:39.640
<v Speaker 1>In May nineteen, a sizeable flare was was observed by

0:30:39.680 --> 0:30:43.040
<v Speaker 1>a team using the CAT ten meter telescope, and this

0:30:43.120 --> 0:30:46.160
<v Speaker 1>was in the near infrared range. There they're also variable

0:30:46.160 --> 0:30:49.480
<v Speaker 1>blasts from Sagittarius a star, and other frequencies like the

0:30:49.600 --> 0:30:52.760
<v Speaker 1>X ray range. This was the brightest flare we've ever

0:30:52.840 --> 0:30:56.440
<v Speaker 1>observed in the infrared or near infrared. In fact, according

0:30:56.480 --> 0:30:59.320
<v Speaker 1>to the u c l A astronomer Twine Doe, who

0:30:59.400 --> 0:31:02.560
<v Speaker 1>was the lead researcher on these uh, these latest latest

0:31:02.680 --> 0:31:06.480
<v Speaker 1>radiation bursts are our telescopes only caught the tail end

0:31:06.520 --> 0:31:09.520
<v Speaker 1>of the flare. It was probably much brighter right before

0:31:09.560 --> 0:31:12.680
<v Speaker 1>we started looking at it. Yeah, as Phil Play reported

0:31:12.680 --> 0:31:15.920
<v Speaker 1>in Bad Astronomy, the flare was well over two thousand

0:31:16.040 --> 0:31:18.959
<v Speaker 1>times more luminous than the Sun in the infrared. Right.

0:31:19.200 --> 0:31:22.760
<v Speaker 1>But yeah, and and furthermore, the scientists judged it to

0:31:22.760 --> 0:31:26.040
<v Speaker 1>be basically a one and two thousand occurrence compared to

0:31:26.360 --> 0:31:29.360
<v Speaker 1>two past observed fluctuations. Right, so it's probably not just

0:31:29.440 --> 0:31:32.600
<v Speaker 1>a random fluctuation in the brightness of the radio source

0:31:32.680 --> 0:31:36.520
<v Speaker 1>there it is. It is a an event, right. So

0:31:36.960 --> 0:31:38.880
<v Speaker 1>this led researchers who think it might be tied to

0:31:38.880 --> 0:31:42.440
<v Speaker 1>a star known as S two, which regularly makes a

0:31:42.560 --> 0:31:46.640
<v Speaker 1>super close pass by the supermassive black hole. Uh, super close,

0:31:46.840 --> 0:31:50.160
<v Speaker 1>you know, in astronomical terms. But in doing so, it

0:31:50.240 --> 0:31:53.400
<v Speaker 1>drags a kind of wind of particles with it. Well,

0:31:53.560 --> 0:31:56.280
<v Speaker 1>I think the star puts out a stellar wind, just

0:31:56.320 --> 0:31:58.280
<v Speaker 1>like our sun does. Yeah, and and but then there

0:31:58.280 --> 0:32:01.400
<v Speaker 1>in their particles within that wind, And so it could

0:32:01.480 --> 0:32:04.040
<v Speaker 1>be that that wind of particles is crashing into the

0:32:04.040 --> 0:32:07.800
<v Speaker 1>black hole. Uh. They considered this, but they decided, well,

0:32:08.120 --> 0:32:10.320
<v Speaker 1>I don't I don't think this would be strong enough

0:32:11.200 --> 0:32:14.760
<v Speaker 1>thing to actually make that flare. So another possibility, though,

0:32:14.840 --> 0:32:18.080
<v Speaker 1>is that S two's pass disturbed clouds of gas and

0:32:18.240 --> 0:32:21.400
<v Speaker 1>caused them to fall into the black hole. It's also

0:32:21.440 --> 0:32:24.960
<v Speaker 1>possible that an unknown object known as G two on

0:32:25.080 --> 0:32:28.320
<v Speaker 1>a two hundred and sixty year orbit around the black

0:32:28.320 --> 0:32:31.440
<v Speaker 1>hole might have caused such a you know, in an

0:32:31.440 --> 0:32:33.960
<v Speaker 1>area of gas to fall into it. You know, it

0:32:34.080 --> 0:32:37.080
<v Speaker 1>moved close enough. In fact, it moved close enough that

0:32:37.240 --> 0:32:40.760
<v Speaker 1>you have G two itself were a dust cloud, as

0:32:40.760 --> 0:32:43.200
<v Speaker 1>some have thought it might be, it would have just

0:32:43.280 --> 0:32:45.440
<v Speaker 1>fallen in. But we don't know for sure exactly what

0:32:45.480 --> 0:32:47.320
<v Speaker 1>G two is, right, right, I thought it was maybe

0:32:47.320 --> 0:32:49.680
<v Speaker 1>gas or dust, but it didn't behave like that when

0:32:49.680 --> 0:32:52.040
<v Speaker 1>it went by the supermassive black holes. Right, there's at

0:32:52.120 --> 0:32:54.840
<v Speaker 1>least one idea that it could be a star. There

0:32:54.840 --> 0:32:56.800
<v Speaker 1>could be a star in the middle of a of

0:32:56.800 --> 0:33:00.600
<v Speaker 1>a cloud of of of of gas and or a particle, etcetera.

0:33:00.800 --> 0:33:02.960
<v Speaker 1>And the or it could be two stars that have

0:33:03.120 --> 0:33:06.040
<v Speaker 1>merged due to their you know, proximity to the black

0:33:06.080 --> 0:33:08.880
<v Speaker 1>hole and then blow they end up blowing off dust

0:33:08.880 --> 0:33:11.800
<v Speaker 1>in the process. Okay, So if there's a star within it,

0:33:11.880 --> 0:33:15.240
<v Speaker 1>that would explain like gravity holding it sort of together

0:33:15.360 --> 0:33:18.040
<v Speaker 1>when goes by the black hole. Yeah, there's something strong

0:33:18.120 --> 0:33:20.720
<v Speaker 1>inside it, or the flare could just be due to

0:33:20.760 --> 0:33:22.760
<v Speaker 1>an asteroid or come it stripped away from a star

0:33:22.840 --> 0:33:25.480
<v Speaker 1>system falling into the black hole. That's that's always a

0:33:25.520 --> 0:33:27.600
<v Speaker 1>possibility that's discussed as well. You know. One of the

0:33:27.680 --> 0:33:29.480
<v Speaker 1>sad things about trying to look at the center of

0:33:29.520 --> 0:33:32.480
<v Speaker 1>the galaxy is that sometimes the Sun gets in the way.

0:33:32.680 --> 0:33:35.320
<v Speaker 1>Like our our viewing window is limited because the Sun

0:33:35.440 --> 0:33:38.320
<v Speaker 1>passes between the Earth and Sagittarius at a you know,

0:33:38.320 --> 0:33:41.440
<v Speaker 1>a certain time each year. Also along the same lines

0:33:41.480 --> 0:33:45.040
<v Speaker 1>of mysteries dealing with Sagittarius a star, I was reading

0:33:45.040 --> 0:33:47.120
<v Speaker 1>an article from just a couple of days ago about

0:33:47.160 --> 0:33:51.959
<v Speaker 1>weird observations regarding what are called Fermi bubbles and Sagittarius

0:33:51.960 --> 0:33:54.400
<v Speaker 1>a star. This was on space dot com, authored by

0:33:54.480 --> 0:33:59.080
<v Speaker 1>the Ohio State astrophysicist Paul im Sutter. Uh So, Okay,

0:33:59.120 --> 0:34:02.720
<v Speaker 1>what you've got here are two giant bubbles of stuff

0:34:02.800 --> 0:34:07.080
<v Speaker 1>including hot gas and cosmic rays, and they're globbing onto

0:34:07.120 --> 0:34:10.200
<v Speaker 1>the middle of the galaxy, of the Milky Way galaxy.

0:34:10.239 --> 0:34:13.480
<v Speaker 1>And we can see these bubbles are emitting high frequency

0:34:13.600 --> 0:34:17.080
<v Speaker 1>radiation like gamma rays and X rays. They were discovered

0:34:17.120 --> 0:34:20.200
<v Speaker 1>in two thousand ten by researchers working with the Fermi

0:34:20.280 --> 0:34:25.160
<v Speaker 1>gamma ray space telescope, and they extend out vertically from

0:34:25.200 --> 0:34:28.880
<v Speaker 1>the flat axis of the galaxy to a distance of

0:34:28.960 --> 0:34:31.759
<v Speaker 1>roughly twenty five tho light years in each direction. So

0:34:31.800 --> 0:34:34.000
<v Speaker 1>if you're trying to picture this and you're picturing the

0:34:34.040 --> 0:34:37.239
<v Speaker 1>disc of the galaxy as a vinyl record, imagine a

0:34:37.360 --> 0:34:40.279
<v Speaker 1>balloon tied to the middle of the record, like the

0:34:40.320 --> 0:34:42.440
<v Speaker 1>hole in the middle of the record on each side,

0:34:42.560 --> 0:34:45.440
<v Speaker 1>and this will give you an idea. So, these huge

0:34:45.520 --> 0:34:48.400
<v Speaker 1>blobs of stuff are referred to as Fermi bubbles, But

0:34:48.520 --> 0:34:50.799
<v Speaker 1>what are they and how do they get there? Well?

0:34:50.840 --> 0:34:54.480
<v Speaker 1>An interesting development is that more recently, the Ice Cube

0:34:54.520 --> 0:34:59.879
<v Speaker 1>Neutrino Observatory and in Antarctica has observed high energy neutrinos

0:35:00.520 --> 0:35:04.640
<v Speaker 1>blasting directly from these bubbles, indicating that perhaps, in in

0:35:04.680 --> 0:35:08.960
<v Speaker 1>Sutter's words quote, some crazy sub atomic interactions are afoot.

0:35:09.560 --> 0:35:12.960
<v Speaker 1>He writes that the position of these bubbles right above

0:35:13.000 --> 0:35:15.400
<v Speaker 1>and below the center of the galaxy could point to

0:35:15.440 --> 0:35:18.399
<v Speaker 1>their origin, and that would be the supermassive black hole.

0:35:18.480 --> 0:35:21.960
<v Speaker 1>Of course, Sagittary essay star Now, like what could have happened,

0:35:22.160 --> 0:35:25.759
<v Speaker 1>that's not really known. He supposes maybe millions of years ago,

0:35:26.400 --> 0:35:30.080
<v Speaker 1>something significant fell into the black hole quote with the

0:35:30.120 --> 0:35:34.360
<v Speaker 1>infalling material heating up, twisting around in a complicated dance

0:35:34.360 --> 0:35:37.719
<v Speaker 1>of electric and magnetic forces, and managing to escape the

0:35:37.719 --> 0:35:41.799
<v Speaker 1>clutches of the event horizon before falling in. That material

0:35:41.880 --> 0:35:45.239
<v Speaker 1>energized beyond belief, raced away from the center of the galaxy,

0:35:45.719 --> 0:35:49.000
<v Speaker 1>riding on jets of particles accelerated to nearly a speed

0:35:49.040 --> 0:35:52.560
<v Speaker 1>of light as they fled to safety. These particles spread

0:35:52.600 --> 0:35:56.520
<v Speaker 1>and thinned out, but maintained their energetic state to the

0:35:56.560 --> 0:36:00.560
<v Speaker 1>present day. So maybe we've got these gigantic, almost galaxy

0:36:00.640 --> 0:36:03.200
<v Speaker 1>sized bubbles reaching out of the top and bottom in

0:36:03.239 --> 0:36:06.720
<v Speaker 1>the milky way that it looks very possibly like something

0:36:07.080 --> 0:36:10.480
<v Speaker 1>fell or almost fell into the black hole and created these.

0:36:11.000 --> 0:36:14.120
<v Speaker 1>So possibly a star got too close, was torn apart

0:36:14.200 --> 0:36:18.680
<v Speaker 1>and ejected by the gravitational forces, or maybe many of

0:36:18.680 --> 0:36:20.839
<v Speaker 1>the stars in the dense core of the galaxy all

0:36:20.880 --> 0:36:24.120
<v Speaker 1>went supernova around the same time. This created this highly

0:36:24.239 --> 0:36:27.720
<v Speaker 1>energetic stuff to get ejected out in these these polar

0:36:27.840 --> 0:36:30.839
<v Speaker 1>jets from the black hole. But anyway, it created these

0:36:30.840 --> 0:36:33.800
<v Speaker 1>bubbles that are full of all this high energy stuff

0:36:33.800 --> 0:36:37.200
<v Speaker 1>that's still ejecting neutrinos today, and you know, that's exactly

0:36:37.239 --> 0:36:40.600
<v Speaker 1>the kind of thing that would interest be very interesting

0:36:40.680 --> 0:36:45.400
<v Speaker 1>to uh type two civilization or a type three. Uh. Yeah, well,

0:36:45.400 --> 0:36:47.440
<v Speaker 1>I guess at this point we've we've come to the

0:36:47.520 --> 0:36:50.520
<v Speaker 1>end of the episode, uh, and come to the end

0:36:50.560 --> 0:36:55.360
<v Speaker 1>of this uh this two episode exploration of Sagittarius a

0:36:55.480 --> 0:36:59.560
<v Speaker 1>star and supermassive black holes in general. But obviously we'd

0:36:59.560 --> 0:37:02.880
<v Speaker 1>love to hear from everybody out there. Um. You know,

0:37:02.880 --> 0:37:06.200
<v Speaker 1>obviously nobody has personal experience with a supermassive black hole,

0:37:06.360 --> 0:37:10.000
<v Speaker 1>but we would love I'm always happy to hear from uh.

0:37:10.280 --> 0:37:12.520
<v Speaker 1>You know, some of our listeners are have read a

0:37:12.960 --> 0:37:15.719
<v Speaker 1>quite a lot of science fiction, and even they've read

0:37:15.719 --> 0:37:18.000
<v Speaker 1>science fiction that I have not read and you haven't read.

0:37:18.200 --> 0:37:20.759
<v Speaker 1>So I love to hear anytime, you know, someone's like, hey,

0:37:20.760 --> 0:37:23.719
<v Speaker 1>I actually I know a science fiction novel that or

0:37:23.719 --> 0:37:26.080
<v Speaker 1>a short story that deals with exactly that concept, and

0:37:26.120 --> 0:37:28.560
<v Speaker 1>here's their solution to it. Oh. But we also know

0:37:28.680 --> 0:37:32.240
<v Speaker 1>from past listener mail that we have listeners in astrobiology,

0:37:32.320 --> 0:37:35.120
<v Speaker 1>astronomy and astrophysics. If you've got something to add to

0:37:35.160 --> 0:37:38.760
<v Speaker 1>this topic, please get in touch absolutely uh. In the meantime,

0:37:38.760 --> 0:37:40.239
<v Speaker 1>you can find all the episodes of Stuff to Blow

0:37:40.239 --> 0:37:41.719
<v Speaker 1>Your Mind at stuff to Blow your Mind dot com.

0:37:41.800 --> 0:37:44.600
<v Speaker 1>You can find our other show, Invention and Invention Pod

0:37:44.680 --> 0:37:48.200
<v Speaker 1>dot com. Uh yeah. If you're looking for another episode

0:37:48.320 --> 0:37:52.400
<v Speaker 1>of per week from from the two of us, consider Invention.

0:37:52.520 --> 0:37:55.719
<v Speaker 1>Each each episode is a different invention and it you

0:37:55.760 --> 0:37:59.279
<v Speaker 1>know it is essentially an invention by invention exploration of

0:37:59.320 --> 0:38:02.600
<v Speaker 1>human techno history. Uh And if you want to support

0:38:02.680 --> 0:38:04.279
<v Speaker 1>either show, really the best thing you can do is

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<v Speaker 1>make sure you've subscribed, and wherever you get get our shows,

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<v Speaker 1>just make sure you leave a nice rating and a

0:38:10.320 --> 0:38:13.160
<v Speaker 1>review that really helps us out huge. Thanks as always

0:38:13.160 --> 0:38:17.160
<v Speaker 1>to our excellent audio producers, Maya Cole and Seth Nicholas Johnson.

0:38:17.480 --> 0:38:18.960
<v Speaker 1>If you would like to get in touch with us

0:38:18.960 --> 0:38:21.360
<v Speaker 1>with feedback on this episode or any other, to suggest

0:38:21.480 --> 0:38:23.920
<v Speaker 1>topic for the future, or just to say hello, you

0:38:23.960 --> 0:38:27.000
<v Speaker 1>can email us at contact. That's Stuff to Blow your

0:38:27.040 --> 0:38:38.239
<v Speaker 1>Mind dot com. Stuff to Blow Your Mind is a

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<v Speaker 1>production of iHeart Radio's How Stuff Works. For more podcasts

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<v Speaker 1>from my heart Radio, visit the iHeart Radio app, Apple Podcasts,

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<v Speaker 1>or wherever you listen to your favorite shows. The First

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<v Speaker 1>Times has Baby Attic