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Cosmic Queries – Black Hole Information Paradox

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Cosmic Queries – Black Hole Information Paradox

The discussion begins with an explanation of the black hole information paradox, where information seems lost when matter falls in. It is clarified that through Hawking radiation, information is preserved and emitted via particles from the black hole's gravitational field as it evaporates, resolving the paradox. Next, an asteroid's potential impact or capture by the Moon is addressed, emphasizing that while a lunar impact is possible, gravitational capture is highly improbable due to the need for a rare three-body interaction to dissipate energy. The conversation then shifts to a lighthearted segment where Neil deGrasse Tyson and Chuck Nice imagine themselves as comic book characters—Tyson as Mighty Mouse protecting nerds, and Nice as the powerful Dr. Manhattan. Finally, a question about "Back to the Future" time travel is explored, noting that the DeLorean's date setting relies on the Gregorian calendar and that traveling back in years, rather than smaller time units, ensures arrival at Earth's correct orbital location.

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Chuck, by the time we finally have a Cosmic Queries with a theme. - A proper Cosmic Queries. - Proper, like in the old days. - Yes. - This one is Black Hole Leaning. - Oh, Black Hole Leaning. - Leaning. - Oh, you can't, but you don't want to lean up again. - Oh, that's cool. - Oh, that's cool. - Bad, bad, bad analogy here. Alright, coming up. Cosmic Queries, mostly Black Hole's additional. Welcome to Star Talk. Your place in the universe where science and pop culture collide. - Star Talk. - Begin right now. This is Star Talk, Neil deGrasse Tyson, your personal astrophysicist. And we're going to do Cosmic Queries today. Cosmic Queries with Chuck Knight. Chuck your baby. - What's up? - Alright, how's your name? - Oh, feeling great. - Have you been practicing how to read people's names? - No. - Because you've got a little better. - No. - And as far as I am concerned, if I mispronounce your name, you are now officially in the Star Talk family. - Because you've mispronounced them with affection. - That's right, yes. - So I'm told this time is not entirely a grab bag. It's leans towards what subject? - Black holes. - Black holes. Everybody's favorite subject. - Everybody loves black holes. - Nobody done love a black hole. - That's right. - Okay, alright. So just go right in. - Let's rock and roll here. We're going to start off with Brian Berg and Brian says, "Hey, Dr. Tyson, Lord Knight, Chuck, you should be able to nail this one." Brian from Portugal. You know what, Brian? So then he says, "Hey, can you help explain the information paradox with black holes? My understanding is that quantum mechanics and hawking radiation are at odds about this." One says, "Information is forever." And the other says, "Information disappears when a black hole evaporates. Are we any closer to understanding how this can be?" Thanks for keeping on doing what you're doing. - Well, thank you. So I can answer this to the best of my ability. But I think that's really a janna question. - Janna, Brian. - Janna, Brian, and Brian Green. But especially Janna. - Yeah, most really janna, she's the black hole expert. - She's totally into this. - With the black hole blues. - The black hole blues. - That's her whole book. - That's her book. She's so badly wants to be able to say it that way. The black hole blues. So here is my understanding of that situation. - Okay. - All right. You have a black hole. You go in and you never come out. - Right. - So if something contains information at all, and it goes into the black hole, did that information leave your universe? That's a question. Because once you're inside the black hole, it's no longer part of your universe. You've crossed over an event horizon. So that was a question. And I think it was even a bet that involved Kip Thorn and Stephen Hawking. - Okay. - Okay. There's a history of bets with fun, sort of frontier questions on new science that's being developed and discovered. - And what do you win? - The universe. - I don't know if that was a dinner at a fancy restaurant of all wine. - Okay. - It's has something in reach of your first born or anything like where you're house, right? - Now that's a bet. - So information theory is very important. And there's sort of a ladder, emergent understanding of how we also need to think about the world. It's not just an interplay of forces and matter, emotion and energy. - Okay. - There's information contained within it. An entropy is a measure of the disorder of information. - Correct. - Okay. So we have this energy field outside of the event horizon that belongs to the black hole. - Right. - The black hole is responsible for that. - Okay. - Particle, antiparticle pairs get created. - Gotcha. - They fly in opposite directions. If the angle is right, one of them will just fall back in and the other one more. - Okay. - And the other one goes out. - Goes out. - Right, okay. If you inventory the particles that are created out of the gravitational field, it is exactly the particles that the black hole ate. - Whoa. - So somehow, knowledge of what the black hole ate that was living inside the event horizon is communicated to the gravitational field. - Right. - And it's pulling it out of what was inside the event horizon and then releasing it into the universe. - And there, there in lies the evaporation. - That is the evaporation of the black hole, but the preservation of information. - And about the preservation of information. - The preservation of the information. - It's wild. - I love it. - It's completely wild. - I love it. - Oh my gosh. - That's crazy. - Yeah. - Yeah. Now there may be nuances to that that I'm not getting or I haven't, but that's the basic thing that's going on there. - Right. - And so that resolve the information paradox. - So the information is not lost. The information is somehow known, preserved, and then demonstrated or expressed in the gravitational field. - In the gravitational field. And as the black hole gets smaller and smaller because of evaporation, it's slow. Vaporation is slow, but it's happens. There's a point where the black hole disappears altogether. And so it has returned to the universe once it came. - Wow, man. - Yeah, it is. - That's the kind of stuff that's tell you, man. That's good stuff. - All right. - All right. - What else you got? - All right, this is SP. SP says, "Greetings, my lord and my doctor, Shay from Arizona here." - All right. - I love start talking. This is my very first question. - F, excellent. - I'm welcome. - I wonder about-- - Shay, right. - Welcome. - Welcome to start talking. - To start talking. (laughing) - Very good. - So SP says, "I wonder about asteroid 2024. Why are four?" And what might happen in 2032 as it makes its approach to our planet? The odds of it impacting the Earth are almost nothing, but it has about a 4% chance of impacting our moon. My question is, what are the odds of it being captured by our moon instead? According to the paper, can moons have moons by somebody Raymond and Raymond, Colomere and Raymond? Our moon is large enough to host a moon of its own and my curiosity has peaked. Can you also talk about the effects of what we might experience if our moon has another moon? - Okay, cool. So, a couple of things. - Good question. - So, we are getting better and better. We have better and better data on asteroids that put Earth at risk. And these are called near-Earth asteroids. Any or near-Earth objects, NEOs, which would include comets, any A's would be a near-Earth asteroid, NEOs, anybody who's near-Earth object, all right? And just for context, if I had to Earth here, there's a schoolroom globe, and I asked how far away is the moon? If you're thinking about how it's drawn in textbooks, the moon is like somewhere over here, a few feet away. - Yeah, it's right there. - Right there. - Yeah, it's not. It's actually not. It's 30 feet away. - Right. - Okay. - If you were doing it. - 30 feet away. There's a lot of empty space there. - Between the moon and upright. - That's right. - That's why it takes eight minutes to get to Earth orbit. But people say, "Are you going into space?" Or if it takes eight minutes to get to Earth orbit, it takes three days to get to the moon. - Wow, that is a lot of empty space. - That's a lot of empty space. All right, so, it is of interest if an asteroid or comet comes between us and the moon. And it's what's called cis-looner space. So that's the area of the moon's orbit around the Earth. If it comes in there, that feels a little tight. But it's not as tight as you'd think. - Thanks a lot. - Because you're remembering the textbook picture of the moon sitting right off our elbow. - Right. - Oh my gosh, you're going to thread that. That's dangerous. But no, it's 30 feet away. - It's like a field-goal post that's the size of the stadium. - Oh, it's a stadium. - I don't know if I can make it. (laughing) - That's an exact analogy here. So when we think of danger and close approaches, anything closer than the moon will get reported that way in the press. - Wow. - All right. This one has a chance of hitting the moon. That'd be fun to watch. But consider the moon has been hit before. - True. - Have you looked at his face? - Yes. - All right. - So it wouldn't have a piece of face for nothing. It wouldn't be the first time the moon got slammed by an asteroid out there, just keep that in mind. Second, it is almost impossible to capture an object without consequences to another object. - Right. - The earth in the moon, if there was a third object in the system, and that other object came in from outside, moving very fast, something has to slow it down. So it's gonna need a close approach with some other object, like a third object where it exchanges gravitational energy so that the asteroid slows down while the other one speeds up. And then the other one escapes the system and then it stays with us. So it needs a third body to carry away that extra energy. - That's not gonna happen. - Right. - So the moon will not capture a moon. - Not by that mechanism, no. Now, what would it be kind of cool to see the moon at night and then a moon going around? - They would each have exactly the same phase, which is kind of cool, if you have a half moon, you have a half other thing that's up there. 'Cause they're both in the same angle between you and the sun. - The sun, right, so yeah. - So it works. So that'd be kind of fun, that's all. But yeah, don't expect it to ever get stuck. - It's not gonna fun to think about. But not gonna happen. - Capture orbit is a special case. - Okay. - Not impossible, but very special case. - Very special case. - Yeah. - Gotcha. So this is Kebo Tron. And Kebo Tron says, Hey, Dr. Tyson Lorde, nice. I'm Kevin from Charlotte, North Carolina. - Nice, I was just there in Charlotte. - Oh cool. - Just there. He says, fiction has always been my preferred type of literature throughout my life. From long novels to short comic books, I love the imagination authors put into their characters and stories to see what your imagination is like. My question for both of you is, if both were in a superhero comic book, what type of villain do you think each of you would be? - But why can't you have a kind of hero? - If you can't see yourself as a villain. (laughing) - Gosh. - So let me preface that by saying I want what I do, which is I write nonfiction. I don't want what I write to be referenced as the negative of something else. - You want every assertion to be positive. - Yes. So I invented the word. I think what I write in others who are the nonfiction world, if you write fiction, we write faction. - That's actually a better word. - A way better word. - Yes, except it also means a splintering of a group. (laughing) - But many words have more than one meaning. - So true. - So that wouldn't be the first time that happens. Okay, so Chuck, would you be a villain or a superhero? - Oh, that's a rough one, man. 'Cause the villains are often far more cool. - Really? - Oh, oh. - And the reason they do that is because if it makes the superheroes the underdog, and you always want to root for the underdog, there's some about him where you feel for them. - Yeah, like if you look at the Transformers, the Autobots are cars. Big deal. Whereas the Decepticons are, they're jet planes. Well, the Decepticons are far more cool than the Autobots. - That's okay, but the Autobots always win, you know? - But I never wanted to be Lex Luthor. - Okay. - Oh, no. - I wanted his money, but that's it. - I gotta say, I wouldn't mind being Lex Luthor. 'Cause Lex Luthor is nothing more than Batman gone wrong. - What? - Yeah, think about it. Batman is a billionaire who creates all these toys so that he can fight crime and uphold justice. Lex Luthor is a billionaire who is also a psychopath. So he creates toys to try and kill Superman. - Okay. - But if he were good, he would be an awesome, he would be an awesome like tandem hero with Superman. - Allow me to quote the Joker in Batman. - Go ahead. You complete me. - Yes. - I complete you. - Well, he says, yeah, you complete me. - Yeah, yeah, yeah. - But it's talking directly about Batman, right? - Yeah, that's it. - Without you, I'm nothing. - Right. - Yeah. - So, you know, the Yin and Yang, I like-- - Is another saying, which is said in a geopolitics, you are only as great as the greatness of your enemy. - Ooh, that's a great, that's a really profound statement. - So there was Saddam Hussein trying to hide in the desert. And he says, I got the entire US military after me. I am no longer a badass. (laughing) I went from badass to dumbass. - That's not real. - No, no, no, no. - What I'm saying is while he's alive to say that. - Right. - That's quite a boast. - Yes, it is. - Right. - Right. - But the fact is that he was the biggest baddest dude in the Middle East until Uncle Red, White, and Blue showed up. - Yeah, yeah, yeah, yeah. - So, so-- - So, who would you be? Would you be? - I know, I'd be super here. I'd be mighty mouse. (laughing) - I'll laugh. - I'm confessing my inner-- - By the way, everybody loves mighty mouse, but why mighty mouse? - 'Cause I'd like that he sings when he goes to save people. - Here I come to save the day. (laughing) - And that's how you know he's sown up on the scene. - You can hear him echoing through the corridors. - Hey, give me your money. - Oh man. - That is another key. He sings it in. - Yes. - So, somehow I was enchanted by that as a kid. - Mighty mouse. - Mighty mouse. - That's the big old chest. - Yes, he was more chest than he was anything else. - He was more chest than he was more chest. (laughing) - But my mission wouldn't to be to save the damsel, or whatever he, okay, my mission would be to save the geeks who been pummeled by the football quarterback. 'Cause in my day, that's what happened. - Any geek being bullied. - You would show up. - Exactly. - And back to my day, we hadn't figured out that you could report bullies to the principal. - Well, that's because the fundamental part of your life. - Right. And you were forced to deal with them because what happens is, you go to an adult and you say, "This guy's bullying at me." And they say, "Yeah, 'cause you're a snitch. "Look at you." (laughing) - You know what my father said? He said, "Anybody bullied you, punch him in the face." - And that's what everybody-- - Not only he said, "My grandmother told me that." - Yes. - Okay. - They will never bully you again. - And they say they'll never bully you again. I said, "Yeah, but they are gonna beat my ass right then." (laughing) You do have to take one ass whoop of it if you gonna stand up to a bully. Okay, that's the thing. They will never mess with you again. But that one time that you did that. - In my day, nerds had very low stock value in society. - Right. - Today, it's the richest people in the world. - Yes. - And I was around just before the transition with the quarterback and the athletes, they needed the nerd to help them with their computer homework. - Right. - Right. - You can't, there's a limit to it. - There's no limit to it. - You can't really put on a nerd. - On a nerd. - Also, you're probably gonna work for them one day. - Right. (laughing) - Well, that wasn't-- - That wasn't quite fully established. - No, seriously. - Okay. - And also, you might want to cheat off of them one day. - Yeah, well, that's always been the case. - That's always been the case, yeah. - So, I would be protector of the nerds. - That's cool. I'd be Dr. Manhattan. - Ooh. - Because he can go anywhere in the university once. - He can go anywhere anytime, anywhere in the college. - And also be in several places at the same time. - Yes, yeah. - So, that's kind of really cool. Plus, he knew all these secrets. - Okay, maybe feel bad if you just wanna be mighty mad. (laughing) - Well, listen, it's fun to think about. There's a cool-- - Dr. Manhattan from the-- - A watchman. - The watchman. - Yeah. - Serious. - Yeah. The movie got-- I mean, always-- - The watchman was the graphic novel. - Correct. - Then there was the movie. - Right. - Then there was the series. - Yes, and I was gonna say, I just liked him in the graphic novels, but it wasn't until the movie that I wanted to be Dr. Manhattan because he was in his lab working and in the bedroom, having a threesome with his wife with himself, which is awesome. (laughing) - Oh, man, we're still working on his science and getting in with his wife and himself. - And himself. - I'm in the threesome. - Okay, you can't beat that. - Okay, that's weird. - Here we go. - That's a little weird. - And add to this, though, to understand the severity of what I have to come save, that there'd be a little signal for me. - What would it be? - It would be digits of pi in the sky. - Oh, that is cool, though. - So the more digits, the more serious-- - The more serious the case, the more-- - The case, the case, the case. - Increase the urgency. - Wow, that's so funny. - It was just three point-- - 52 decimal places. (laughing) - That's atomic, right? - Exactly. - I have to go in and wrap there. If it's one decimal place, it's just someone trash talking you. - Right, right. - That's great. - That's what it would be. - That's funny. - Thank you for that question. - All right. (upbeat music) - I'm Joel Cherico and I support Star Talk on Patreon. This is Star Talk with Neil DeGrasse Tyson. (upbeat music) - This is William Heisenberg, the third. He says, "Gee, greetings, Dr. Tyson, Lord and I." - My name is Heisenberg. - He says, "I'm William Heisenberg." - Heisenberg, okay. - Yeah. - The third. And then he phonetically, Wilheim. - Wilhelm. - Heisenberg. - Heisenberg. - Heisenberg. - Heisenberg. - He says, "So I got it right, Wilhelm." I didn't say Wilhelm, though, okay. 'Cause I'm not that pretentious. And you're an American now, it's Bill. (laughing) Not really. - You have Bill Heisenberg. - Okay. (laughing) All right, buddy, here we go. He says, "In back to the future, you had to hit 88 miles per hour to activate time travel." I was thinking about that. First, you have to set the date to 1955. Who's to say that the actual cosmic time reference is? For all we know, time could interpret that as 1955 years from the Big Bang. Now, that would be an uncomfortable arrival. Second, they never programmed a location. So you'd probably appear in open space. And without anything to slow you down from 88 miles per hour, would you be stuck endlessly slipping through time, unable to decelerate below the activation speed? What do you think? - Whoa. - So here's what I think. - Okay. - Here's what I think. You need a second job. (laughing) - You just spent too much time thinking about this. - You didn't, you didn't. - I'm gonna say shipbuilding is what you need in a bottle, ships in a bottle. This is too much thought. I'm joking. What an interesting thing, though, it's fun. - So a couple of things. - Couple of things. - We can unpack that one bit at a time. - Okay. - The Time Machine panel. - Okay. - Which you program. - Mm-hmm. - That knows that it's 1955 on the Gregorian calendar. - Right. - You see it on the display. - It's on the display. - Right. - I don't remember it said AD, but it's completely implicit in how the whole thing was conceived. - Okay. - Okay. - All right, so that's the first point. So there's no risk of going back to 1955. A, B, B, after the big bang, right? It's not gonna get it after big bang. - Right. - All right. - Okay. - Of course, AD, the A doesn't stand for after. - What's the stand for? - It's for the year. - It stands for what? - The year in Latin. - Oh, okay. - Annel. - It's Annel Domini. - So that's the gear in time. - Because the whole panel lit up, all right. And now, significantly, he goes back a number of years, not a number of months, or a number of days. If he'd gone back 30 days, he'd land in the middle of space, because Earth is not there now. - Correct. - Okay. - All right. - Okay. - We're then. - Right. - Any actual time travel machine ideally should also be a space travel machine. - Right. - Right. - Okay. You sit in here, you say, "I want to go back to yesterday." And you walk in, you want to come out, you want to still be here. - Right. - That had to transport you in space as well. - So it's a space time machine. It's not just a time machine. - Correct. - It's got to be a space time machine. - Otherwise, you'd be dead on your first transport. - Exactly. - Because you're going to be in empty space. - Right. - All right. So, had he gone back 30 days, 30 minutes, 30 hours, 30 days, 30 months, he'd be dead. But he went back 30 years. And a year, Earth returns to its place. - Okay. - And it's orbit. - Right. - He's still on Earth in any whole number of years. - Right. - Because it's a whole year. So you're right, a year ago to, no, a year ago, this time, the Earth was here. - Correct. - Right. - Now, we're ignoring the leap days. - But also, what about the fact that in our solar system on the tip of that spiral, that thing is moving too. - Are you talking about the whole solar system moving through space? - Yeah, the whole solar system is moving too though. - So, the question is, how far do the solar system move in a day? - Right. - So, do you have to factor that in? - Okay. - You would. But, to factor in one of them, cinematically, that's good enough. - Okay. - All right. - All right, to get them all, then you just be in. - Yeah, well, you've been annoying. - Right, exactly. - It's like saying that football is not, you're not first in 10. You're first in 30 feet. Well, okay, shut up. (laughing) You're not first in 10 yards. (laughing) - Well, it would be. - No, but you don't say it that way because you're just over complicating things. - Oh, I got you. - You know what I'm saying? - You don't say, first down, 30 feet to go. No, it's first in 10. - Yeah. - You know, 'cause we know what it is. - We know. - I got you. - So, it's 30 years. So, now, apparently. - What's his name? - This is Villheim. - Villheim, Bell. (laughing) - You didn't pay close enough attention to that scene. - Really? - That mall is called Twin Pines Mall. Where do we think it got its name? Marty, exactly 30 years goes back in time and he arrives at Twin Pines Ranch. The ranch gave itself up to be a mall as is so common with the strip malls of the suburbs. - Right. - All right, and so out of an homage, you keep the name that it once was. Twin Pines Ranch. - Right. - And it says it in that scene back in 1955 when he arrives crashing down the door of the barn of Mr. Peabody's Ranch. Okay. So, we've got him going back in time, still arriving on Earth. We've got him going back in time, arriving in Twin Pines Ranch, which is the same places where the mall was that he just left. - Okay. - It's America, so what does the farmer do upon seeing a DeLorean arrive with Marty who has a hazmat outfit on because he's handling plutonium. - Right. - Okay. - What does the farmer do? - He invokes his second amendment rights. (laughing) - God damn it, get off my property right now. Tell you what. No, you don't ask them first. - No, that's right. - You should first, and then ask. - That's right, yeah. - I forgot, that's the-- - So the shotgun comes out. - The shotgun, right. - Marty is trying to escape. He's driving fast. He bowls over one of the two saplings that are the Twin Pines of his ranch. There are two five foot tall saplings with a picket fence around it. And that's the Twin Pines of the Twin Pines Ranch. Marty bowls over it, attempting to escape and not get shot. Okay? Okay. Now, hang on. Hang on. - I thought Vilheim put too much of a thought into this. Damn. - Wait a minute. - So the second shot against Marty hits Mr. Peabody's mailbox. - Okay. - And that's how you know it says Peabody on it. So let's tell you, he's Mr. Peabody. When it hits the mailbox, the mailbox explodes. It's shotgun. I didn't think anything of it. Until, I gave a talk where I described that scene in Southern Georgia and somebody in the audience looked like someone who owns a few guns. - Of course. - You know, I had like a camouflage. - A camo hat? - A camo hat, you know? - So they'd probably held a few guns. He said, "I have something to comment." I said, "Oh, did I miss something?" He says, "Yeah, that shotgun would not have blown up to the mailbox." I said, "What would it have done?" He said, "We just would have put holes in it." - Okay. - Like a shotgun pellets would do. - And where were you when you gave this talk? - Southern Georgia. - Oh, he wouldn't know. (laughs) - So, so that's when I said, that's what, that's why I discovered, he introduced himself as a nerd redneck. And that's where I discovered this beautiful kind of nerd, new kind of nerd. Welcome to the nerd club. - The nerd neck. - The nerd neck. And we agreed he could be a nerd neck. And that's where we had, for our patronon, we had private Q and A with patronon. And one of them is also a self-proclaimed nerd neck. - Oh cool. - And he'd let us say, "Sign your nerd neck." So anyhow, so, Marty leaves, okay. Then he goes into town and he has to figure out how to get back and all of this. Then he goes back to the future and we rejoin him at the mall. - Right, 'cause that's where he left. - That's where he left. - Right. - It's no longer called Twin Pines Mall. - Are you for real? - It's called Lone Pine Mall. Oh snap. (laughing) Oh snap. And the camera doesn't zoom in on it. It's just there. It's just there. - Oh man. - Okay. - Okay. - So my boy, he's gotta go back and watch. - Well, Villeheim, there you have it, my friend. - No, no, he just got out geeks. - You did. I thought you had a lot of attention to the detail here, but apparently, you may have wake up early in the morning. You can't out back to the future Neil on this one. Wow, that was something else, man. - All right. - That was something else. All right, let's go to Colin Montout. Yeah, Montout, who says, "Hello, this is Colin from the Berkshires of Massachusetts." He says, "I'm asking this question for my wife, Billy. "I would like you to explain what information means "when it's used by you astrophysicists, "like the question of whether black holes "destroy the information and all that, "hocking radiation." What is the information? - I need help on that. Okay, because for me, as I came to understand it, the information, it was good enough to simply have the inventory of particles that went in and came out, all right? But we know that if a molecule goes in, the molecule has more information there. - Absolutely. - There's order 'cause it's a construction. - It's a construction of these particles, right. - And when the Hocking radiation re-emerges, it doesn't give us whole molecules. - Right. - So I cannot answer that. I have to check with my black hole people. - Okay. - Okay. - So because to me, a molecule will have more information than a particle. - Right. - What? - Absolutely. Well, look at that. What a great question, Colin. - And what? - What? - We're going to dig into a black hole. - Mm-hmm. - And get back to you. - Unless? - Unless. - The act of making the molecule reduce the information somewhere else. - Ooh. Okay. We're going to reduce the, so you have less entropy here, more entropy over there. So instead of thinking about it as how much information is in the molecule, look at the entropy budget. - Right. - Why are we complex? Where did that come from? - Mm-hmm. - In a closed system, that can't happen. - Right. - Thermodynamics. - Right. Go ahead. - We're not a closed system. - No. There's introduction of energy into the system. - From where? - Um, our great Lord Ra. - Ha! - The sun. - Yes. - Okay. - So we're getting energy from the sun. - Right. - Using information here, building complexity, reducing entropy here. - Right. - However, the sun's entropy increased. - Right. - The sun is going to burn one day. - Burn one day. - That's right. - So I'm thinking that's how that is reckoned. - That makes a lot of sense though. - Yeah. - That does. - Pretty sure that's how that will go. - Okay, cool. - All right. - I love that answer. - But I'm going to double check with Janet. - We still got to get to where to talk with Janet. - Yeah. - It's a great answer though. I hadn't thought of it that way. - Subscribe her. She's a friend of start talks. She's a professor of physics at Barnard College in Columbia University. And she's written a couple of books on black holes. - Black holes. - Yeah. - She's a theorist. - A theoretical physicist. - Physicist, yes. - He's our resident black hole expert. - Yes. - So. (upbeat music) - All right. This is Jo Kiyareli. Jo Kiyareli, who says this. Hey, Dr. Tyson, Lord nice. Jo Kiyareli, here from Connecticut as a new patron member. - Nice. - A new Patreon member. He says, "I had the pleasure of meeting you and Gary at Chuck Special in New York City." - Oh my god. - Oh my god. Look at that. - Look at that. - Thank you for coming to that. We were all there in good numbers. - Yes, it was. Chuck gave a stand-up, a science-informed stand-up routine. - Stand-up routine. - Yeah. Do you have a title for it? Let's go. - It's called Chuck Nice. Just smart enough. - Oh, okay. - That's the name of the special. - All right. - Because everybody I'm with is always smarter than me. That's one of the things that happens when you work here. Well, you do what I do for the, I'm surrounded by him and all his buddies and they're all freaking super geniuses and I'm a dumbass sitting here, but I'm dumb enough to know how dumb I am. - That makes you smart. - So that's what I do. I just sit and listen and learn. - So my motto is from Michael Dell. - Okay. - Okay. - Okay. - My sister used to work for Dell computer in Austin, Texas, and she would tell me stories. So Michael Dell said, "The day you wake up and find yourself as the smartest person in the room. Change rooms." - Well, you need to get up and leave. (laughing) - Because it's just us here in his office, you need to go right now. (laughing) - All right. Let's see what Joseph says. He says, "And by the way, Joe, thanks for all the nice words." He says, "Neal, when we think about things getting hot, we think of them expanding. So why do clothes shrink in the dryer?" (laughing) - Thanks for the love, thanks for the show, I love it for the mysteries of the universe. - That's so funny. - Wow. - That's funny. Why do clothes shrink in the dryer? - Wow. - When things normally expand when you hit them. I mean, that's kind of a. - You know, 'cause you know, it shrinks the most as wall. - Right. - But what I never understood is, like, because you have to wash wool very special, you know, a special way. - Like, if it's sun-water and wool-eye. - If it's summertime, and you hose down sheep, and then the sun comes out and it heats it. - Yeah, they don't become tiny or sheep. - They don't become tiny. - So, what's up with that? (laughing) - Stop leaving us out in the sun. - Yes. - That's so funny. - So, not all material behaves in the same way by the same thermodynamic forcing. - Right. - So. - Okay. - Here's one that we just accept, the ice floats. - Right. - Well, ice is water that is colder than the water it's floating in. - Right. - Things that get cold normally shrink and shrink. - They'll shrink, right? - They'll get denser and denser and shrink. - They'll shrink. - Cold things shrink. - Right. - Ice at three degrees Celsius expands. - It expands. - Yeah. - I'm sorry. - Water at three degrees Celsius. - They become nice. - It's not ice yet. - Right. - At three degrees, it expands. - Okay. - And that floats to the top of the lake where it freezes and it stays at that larger state. - Right. - Floating actually insulating the water below. - Right. - Allowing fishes to survive the winter. - Right. - Because once you put a layer, an ice layer on top, the bottom of the lake no longer is climatically connected to the water connected to much above. - That ice actually becomes insulation. - Insolaceous. - Insolaceous. - Insolaceous. - Exactly. So, ice does the opposite of that and there's a few other materials that will do this and the chemists know about them. So for example, if you want something that does not expand or contract at all, you combine two materials that have opposite properties. - That's cool. - So, work opposite each other. - Right. - In this way. - Nice. - The thermal couplers are these metals that bend when they're heated. - Mm-hmm. - Okay. So typically these would be valves to a gas, gas valves. - Mm-hmm. - All right. So, you heat it, it stays open when you turn it off and it cools down and closes back naturally, just because of its own response to temperature. So, with regard to clothes in the dryer, it can help you, what can you do? I gave you the rest of the physics of what's going on. - Right. - What's going on, but yeah, that will remain a mystery along with what happened to my other sock. - And along with, does the refrigerator like turn off when you turn the refrigerator? - Right. Yeah. - Even if people say, of course it does, because you just press the button on the side and you see the light goes down and I'm like, yeah, but that's because the door is open. - So, I was tweeted this, I said, one of the mysteries of the universe does the refrigerator, so someone put their cell phone in their refrigerator. - Oh, hilarious. - Okay. And it started filming and then they closed the door and then they got dark. - You got dark. - You got to love people. - All right. Chuck, we only got five minutes. How many do we do? We got like a boat load of questions there. - Oh, who cares? - Let me go. - Let's go. Let's see how I can answer them fast. - All right. This is Tom Lindellius who says, greetings from Upsala. - Upsala. - Upsala. - Upsala. Speed them. - Speed them. - Yes. - He says, there's an important observatory there. - Oh. - From the early, early 20th century. - Did you know that? - Probably goes earlier, but the data that I've seen from them is quite relevant and significant at the moment. - No, I didn't. - When they were a player in that space. - Very cool. - He says, if our universe actually existed inside a black hole, wouldn't everything seem to be converging into a single point, the singularity, rather than expanding also, wouldn't we be able to spot any evidence of spaghettification, like large galaxies or gas clouds appearing stretched, thanks to the band? - The spaghettification happens when you get very close to the singularity. - Right. - The bigger the black hole, the less the spaghettification is at the outer edge. - At the outer edge. - At the beginning. You're just falling. - You're just falling through. - Right. - If we are in a black hole, and our black hole is the size of our universe, then the spaghettification is not a thing, which is occupying the volume inside the black hole. - Inside the black hole. - And we're not the collapsed system when a star collapses to make the black hole in the first place. - Right. - Yeah, to spaghettification is not an inevitable fact of falling into a black hole. - Okay. - All right. - Very cool. - That's all. I mean, all right. This is RID, R-Y-D. Hey, Dr. Tyson, Lorde Nice, Remy from Nante France. Love this show. If black holes are actually newborn universes with different physics, can a wormhole cross them or get us out of our own universe or are space times separated, and we're just stuck. - Yeah, I do not know for sure, but everything I know about wormholes tells me they can get you anywhere. - Anywhere. - And if there's a multiverse, and there's another universe over here, in principle, you should be able to-- - Pop up that wormhole. - The tunnel. To that multiverse. - To that multiverse. - However, in a multiverse, every universe has slightly different laws of physics. - Oh, that's not good. - So you open them, open the portal, and then like flip a coin through there, and then they grab it. If they explode or disintegrate, the coin melts, and then just stay, you can grab it here. - Exactly. - So that's another universe, in the same way, the forward-facing universe in a black hole would be another universe. I don't see any reason why a black hole couldn't connect any two of those. And that's exactly what Rick has is-- - The portal gun. - The portal gun. - Right. - In Rick and Morty. - There you go. All right. This is Kristoff Day, a machineeer who says, hello, Dr. Tyson. - What, a senior? - No. M-A-E-S-E-N-E-R, machineeer who says, hello, Dr. Tyson Lorde, nice, Kristoff, calling from Belgium. - Love it. - I know that the answer today would be, we'll get spaghettified, but let's suppose our current limits in technology are an issue. What would it take to fend off a black hole coming towards our solar system? A mission like dark would be out of the question because it would get equally spaghettified. Curse to hear you're encounter your counter apocalypse ideas. - So a black hole is coming at us. - Yeah, in my day, what you would say is kiss your ass goodbye. - All right. But more seriously, what we would have to do is get all the rockets we have, attach it to the side of the earth and get us to allow the solar system before the black hole gets close enough. - A literally space of earth is the answer because you're not, you can't touch the black hole, you can't could nudge it out of the way. - Right. You can do to the black hole. - To the black hole. - And if you are on the course to fall into it, once you get to that event horizon, it's over. - So you want to move earth to another place, ideally to another star system because we value you. - Yeah, because we need sunlight. - I need sunlight. - Right. - Exactly. - Very cool. One more. Here we go. This is Jeff. He says hello. Dr. Tyson. Lorde. Nice. I'm Gweem. Hewitt from Birmingham. UK. - Birmingham. - Yeah. Oh. I was Gary was here. The other day, I was reading the elegant universe, that's Brian Green. - Brian Green. - Yeah. He said, and it was explaining black hole entropy and mentioned that after every interaction, for example, an asteroid falling into the black hole, it's a creation disk expands. I find myself wondering why this happens, why the accretion disk expands after these interactions, by the way, love the show. - Excellent. That's really cool. The disk is the holding pattern for the material that ultimately will fall in. - That's the bright hot thing that you see going around the black hole. The bright hot thing. - The reason why it exists at all is because rarely is anything moving through space and had it exactly toward the black hole. - Okay. - Even if the black hole influences its path, it'll curve it around, but it's never had it straight in. That's a very rare trajectory to head straight in. - Okay. - All right. So, the material gathers and all right, it wants to fall in. Now, if you jump off a roof, why does hitting the ground kill you? - Well, you know, because the ground is not going anywhere. - When you jump off, you're speeding. - You're speeding up. - Yeah. - You just fall and fall and fall. And you're not going to die because you weren't falling long enough to have high speed. - Gotcha. - It's a simple point. - It's a real simple point. - Okay. So, where did you get the energy that was ultimately manifest as high speed at the bottom? The elevator gave you that energy. - Right. - Go gravitational potential energy. - Gotcha. - So, you at the top, you fall at the bottom, you die. - Gotcha. - Here is material falling into the black hole. - It's energy go, because it's speeding up, but then you get stuck in the. - Ah, that's so cool. - You get stuck in the. - No, that's the ground for the black hole. - Yes, yes. - That is awesome. - Yes. - Yes. - That's why it's all hot and hot. - That's right, hot. - Because normally, when you hit the ground, it breaks all your bones. - Yes. - But if you're gas cloud, that becomes heat. - Dude, that's amazing. - It heats up. And it heats up to such high temperatures, it begins to radiate ultraviolet X-rays. And so, X-ray telescopes would discover black holes. So, if the asteroid simply fell straight into the black hole, nothing would happen to the equation disk. - Right. - Nothing. - Because it would just speed up and get lost on the other side. - Right. - But if you hit the equation disk, all that extra speed has to go somewhere. - And it's. - And it's. - It's distributed throughout the. - Throughout energy is. - And now energy is going to be. - It's in the equation disk. - And that's why. - And it heats up and then it expands. - So, when you see light from a black hole, you're not seeing any light from inside, it says light can't escape a black hole. - No! - That's what you're seeing. - You're seeing the equation disk. - That's. - Or. - The material is trying to get in so fast that the heat is so immense, that the equation disk is preventing the heat from escaping, what's the only way that the heat can escape? If it can't get out through the disk, how's it going to get out? - It can't. It has to join. - No. - There's other ways you can get out. - What the heat from the disk? - Yeah. - It's so ferocious. It is trying to get out of the disk, but it can't, okay? - Right. - This. - Two ways it can get out. Up and down. - Okay. - These are the jets that we see coming out of black hole jets. - Oh, the black hole jets. - Very cool. - Black hole jets. - Nice. - You get the equation disk, black hole jets. - And the black hole jets. - There you go. - That's what we're seeing. - Yeah. - That's. - Black holes are cool. - Dude, what a great question. - Yeah. - That was cool. - Yeah, very good. - No, but the equation disk ate it and it gets hot and expands. You guys, that's what we'll get time for. - That was great. - A black hole leaning cosmic queries. - Right. - Love that. So Chuck, we gotta call it quits there. - Oh, it's the same. - But we'll be back. - Yeah. Oh, I'm gonna shamelessly plug my next book. - Oh, cool. - Because it's a question and answer book. - I love it. - It's called just visiting this planet. - Just visiting. - It's Merlin returning. Because Merlin was a column that I wrote in a magazine for, like, 15 years. - Right. - I wrote it in with questions. That's why I'm very comfortable in that space. Because I cut my teeth as a scientist and as an educator responding to people's questions. However crazy they were. - Wow. - And so it's just coming out like-- - This is another extension of that. - Yeah, and it's illustrated by my brother who's an artist. He went to high school at Music and Art in New York City. - Very cool. - And I went to the Bronx High School of Science. - And now you guys are working together. - Yeah, we're working out. I'm loving it. - This is true steam in a family coming together. Family steam. - Hmm. Nice. - So, yeah. So people who love queries about the universe, it's questions answered with this character called Merlin. And I think it's more fun. You could type it into chat GPT, but you know and I know there's no soul behind those words. - Exactly. - There's no entity, there's no personality. - Yeah. - Just the dead eyes of AI. - All right. This has been Star Talk, Cosmic Queries. Until next time, I bid you to keep looking up.

Podcast Summary

Key Points:

  1. The information paradox of black holes is resolved by Hawking radiation, which preserves information from inside the event horizon by encoding it in particles emitted from the gravitational field as the black hole evaporates.
  2. An asteroid's chance of being captured by the Moon is extremely low, as capture requires a complex three-body gravitational interaction to slow the asteroid, making it a very special and unlikely case.
  3. In a superhero context, Neil deGrasse Tyson humorously identifies as Mighty Mouse, a protector of nerds, while Chuck Nice prefers the omnipotent Dr. Manhattan for his ability to be in multiple places at once.
  4. Time travel mechanics in "Back to the Future" are analyzed, noting that the DeLorean's date setting implicitly uses the Gregorian calendar, and traveling back in years (not days) accounts for Earth's orbital position to avoid appearing in space.

Summary:

The discussion begins with an explanation of the black hole information paradox, where information seems lost when matter falls in. It is clarified that through Hawking radiation, information is preserved and emitted via particles from the black hole's gravitational field as it evaporates, resolving the paradox. Next, an asteroid's potential impact or capture by the Moon is addressed, emphasizing that while a lunar impact is possible, gravitational capture is highly improbable due to the need for a rare three-body interaction to dissipate energy.

The conversation then shifts to a lighthearted segment where Neil deGrasse Tyson and Chuck Nice imagine themselves as comic book characters—Tyson as Mighty Mouse protecting nerds, and Nice as the powerful Dr. Manhattan. Finally, a question about "Back to the Future" time travel is explored, noting that the DeLorean's date setting relies on the Gregorian calendar and that traveling back in years, rather than smaller time units, ensures arrival at Earth's correct orbital location.

FAQs

The paradox questions whether information is lost when objects fall into a black hole. It is resolved by Hawking radiation, which preserves information by encoding it in particles emitted from the black hole's gravitational field as it evaporates.

It is highly unlikely because capturing an object requires a third body to carry away excess energy, which is a very special and rare case. The Moon's gravitational influence alone is insufficient for such a capture.

Near-Earth objects are asteroids or comets that come close to Earth's orbit. They are monitored to assess potential impact risks and improve planetary defense strategies.

Neil deGrasse Tyson would protect nerds from bullies, inspired by Mighty Mouse, while Chuck Nice humorously considered being Dr. Manhattan for his omnipresence and knowledge.

The Moon is about 30 Earth diameters away, much farther than often depicted. This vast distance explains why space missions take days to reach it, not minutes.

While some asteroids have a small chance of hitting the Moon, such impacts are rare. The Moon's surface shows evidence of past collisions, but new impacts are infrequent.

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