StarTalk Radio - Cosmic Queries – The Atlas of Peculiar Galaxies with Charles Liu

Episode Date: May 12, 2023

How can we use AI to explore the universe? Neil deGrasse Tyson and co-hosts Chuck Nice and Gary O’Reilly answer grab-bag questions about simulations, black holes, warp drive and more with astrophysi...cist and “Geek-in Chief '' Charles Liu. NOTE: StarTalk+ Patrons can listen to this entire episode commercial-free here: https://startalkmedia.com/show/cosmic-queries-the-atlas-of-peculiar-galaxies-with-charles-liu/Thanks to our Patrons Heike Stoll, Mugglewatcher, Chip Gallo, Alexander Rauschenbach, Samuel Joseph, and Capt. James Riley for supporting us this week.Photo Credit: NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), Public domain, via Wikimedia Commons Subscribe to SiriusXM Podcasts+ on Apple Podcasts to listen to new episodes ad-free and a whole week early.

Transcript
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Starting point is 00:00:00 Welcome to StarTalk, your place in the universe where science and pop culture collide. StarTalk begins right now. This is StarTalk Sports Edition, and this time we're doing a Cosmic Queries grab bag. Got with me Chuck O'Reilly. Wow, you just married us. January's Grab Bag. Got with me, Chuck O'Reilly. Wow, you just married us. You married us, and somehow I had to take Gary's name. What does that say?
Starting point is 00:00:36 What is going on here? Gary O'Reilly. I think of you as my one common conjoined co-host. I'm sorry. So, Chuck Nice. Yes, Dr. Franken nice. Good to have you there, ma'am. Good to be here. All right. Gary O'Reilly, former footballer from the UK and broadcaster.
Starting point is 00:00:55 Yes. And we've got a little piece of him for us. Very good to have you. This is a grab bag. And anytime we have a grab bag, this is like the bat signal going up into the clouds. We've got to reach for our geek in chief. The one, the only. Hold your applause till the end. Charles Liu!
Starting point is 00:01:12 Charles! Hey! Okay. Hey, Neil. Hey, Chuck. Hey, Gary. So good to see you guys. A friend and colleague, astrophysicist Charles Liu, who's a professor of astronomy and physics at the City University of New York in Staten Island. And always good to have you here.
Starting point is 00:01:31 You're a fan favorite. And so you're going to help us in this grab bag. I mean, I might be able to do some, but when it comes to really geeky answers to cool questions, I am unworthy. geeky answers to cool questions, I am unworthy and I will just sit back while you take the But I'm happy to be here. It's always fun.
Starting point is 00:01:52 And the questions are always the best. They're always cool. So, Gary, Chuck, you got questions lined up? Yes. Right, let's start with one of our very favorites and I can't do the voice anywhere near the ability that Chuck has, but it's Alejandro Reynoso.
Starting point is 00:02:10 No, no, no. Give it to Chuck. Why are you reading that? Chuck? I didn't know we were starting here, so. I got to pull up. I got to pull up Alejandro. Pull up the message.
Starting point is 00:02:21 So, again, all of our Cosmic Queries today are exclusively asked by Patreon members with our new entry-level category of $5 a month. So you can't argue with that. All right, here we go. Let's start it off with our friend Alejandro Reynoso, who comes to us from Monterey, Mexico. And he says, Mexico.
Starting point is 00:02:47 And he says, hello. Or should I say, hola. My question is, how do you think we can use artificial intelligence in exploring the universe? So there it is. So Charles Liu, what do you have to say about AI and our field? Alejandro, let me tell you,
Starting point is 00:03:09 you are right on the mark. And in fact, we are already trying to do precisely this. As many of you know, I am part of the Cosmos collaboration working with the
Starting point is 00:03:21 James Webb Space Telescope. Neil, you're familiar with that. Yeah, back when we were working on it with just the Hubble Space Telescope data, right? But now we have a James Webb Space Telescope. Just to be clear, the Cosmos Collaboration is a consortium of people and institutions that have targeted sections of the sky and others just to hammer it with as many kinds of telescopic observations and detectors as possible
Starting point is 00:03:45 to learn basically everything knowable about sections of the sky that we target. So continue. So now we've applied this to the James Webb. So what do you have going? Well, the James Webb Space Telescope's first season's most significant observing project is to use the James Webb to aim at the cosmos field, which you described so aptly just a few seconds ago. And so we are spending 270 hours of James Webb time in just a small patch of sky about the size of your pinky fingernail.
Starting point is 00:04:19 At arm's length. Yeah. At arm's length. That's right. When you're looking up at the sky. Yes, yeah. Pinky at arm's length. Nut finger in your eyeball. Right. I'll do that.
Starting point is 00:04:32 All right, good. Yeah, that would be difficult. So there's literally terabytes and terabytes worth of data coming from all the different observatories around the world. And James Webb is just layering on that next layer of information about this patch of sky. And no human being can individually process all of that information in any meaningful way. So what we need instead is the opportunity to use machines, machine learning, deep learning, artificial intelligence, to help us make sense of all of this incredible amount of information.
Starting point is 00:05:09 So, for example, we have information about possibly 2 million or so galaxies within this cosmos field, ranging all the way out to 13.5 billion light years away. Just to be clear, this fingernail at arm's length blots out two million galaxies on the sky to the edge of the universe. Each of these two million galaxies has thousands of pieces of information about it that have been gathered by all these telescopes that have been trained on it for the past 20 years off and on. And now we've added James Webb on top.
Starting point is 00:05:44 Can we make a pattern? Can we understand what actually matters? Can we ask ourselves, can we look at all two million of these galaxies and find something new? Actually, probably not. But using artificial intelligence, we can do that. We can say, here are the parameters
Starting point is 00:06:01 of what we think are normal. Can you please find for us all the normal things and then all the abnormal things? And then tell us what is normal and what is abnormal? Or what should we be looking at that allows us to sort of understand the change of the galaxies in the universe from 13 billion years ago to the present day? I mean, that's a heady question, which any individual human can sort of grab the most creative and interesting ways. But processing all of that information, AI is the answer. We're not there yet. So Charles, why isn't this just more powerful computing rather than what people generally today think of as AI. Because we've always needed computers
Starting point is 00:06:49 ever since computers have been brought to our field. We've needed it to reduce and analyze massive amounts of data, even when massive amounts of data in the day was only a kilobyte or a megabyte. And so now we're up to terabytes. So isn't it just more powerful computing? Number crunching as opposed to thinking.
Starting point is 00:07:11 Right, yeah, is it really thinking? Number crunching has been going up. It actually is extremely important. And you're right. That's most of what computers are doing for us in astronomy today. But it's that next step. I think it started maybe three or four years ago
Starting point is 00:07:27 that we really started shifting over toward machine learning and artificial intelligence. So both are still working hand in hand together. And in the current circumstance, the AI part is still in its infancy. A lot of times when people publish scientific results that they found using AI or machine learning, they're probably not right. But we publish them anyway because we say, hey, it might be right. Please, let us let the rest of us colleagues go back and check to see if what this machine found is actually something in reality.
Starting point is 00:08:03 The all-important verification step. That's right. You've got to have that. Compare all of that to neural nets. Mm-hmm. Well, neural net is just another way that we can abstractly map the idea of intelligence and
Starting point is 00:08:19 pattern recognition. Because we think that's how our brain works. That's why we say neural, right? That's right. It's just the connectivity to find patterns and whatever it is that might manifest. That's right. The neural net itself is a pretty complicated thing, but we can strip it down to very basic components
Starting point is 00:08:40 and say, can you do a one-dimensional or two-dimensional or three-dimensional discussion about all this information? Try to make connections that we otherwise wouldn't be able to see if we were just trying to use one CPU by itself, you know, one brain or one process. The neural nets in our brains are not just three-dimensional. They're four, five, six, ten. You know, each neuron attaches in many unusual ways to many others. So there's a sort of an emergence of awareness that comes about from these networks of that kind of complexity.
Starting point is 00:09:14 So these are the things, I think you did a Cosmos episode on this, right, Neil, once? Yeah, we did. About how intelligence and the concept of a very complicated neural net, like a human brain, can actually be more complicated than even an entire galaxy worth of stars and their interactions and so forth. It's very, very powerful, but poorly understood. All right. Are we looking for the right things?
Starting point is 00:09:40 I mean, using AI obviously should be an advantage, but are we looking for the right, because there must be things out there we don't know exist, but we should be looking for, but we don't know to look for them. Is AI going to be able to assist in us in that kind of capture of data? In other words, can it discover what it's not looking for? Right. Thank you. It can discover what it's not looking for.
Starting point is 00:10:01 That's a great question. It can discover what it's not looking for if we tell it to look for things that it's not looking for. That's a great question. It can discover what it's not looking for if we tell it to look for things that it's not looking for. Right. So in a sense, your number crunching, right? Data reduction or, say, computational work. That will give you the answers to things that you are looking for. Now you tell a machine and say,
Starting point is 00:10:19 these are what we are looking for. Can you tell us any exceptions to what we found? So anything, it would have to be something anomalous, but wouldn't you have to program the parameters of what an anomaly is in order for- No, no. You only have to know what we're familiar with and anything-
Starting point is 00:10:34 Well, anything else would be an anomaly. That box would be an anomaly. That is an anomaly. So, okay. So that means, well, that is kind of like- That's the easiest part of the job. If it doesn't fit, stick it in a box. He goes, oh, that's odd.
Starting point is 00:10:47 Okay, now let's look at that. Okay. In fact, 60 years ago, one of our colleagues did that. He looked at all these beautiful galaxies in the night sky. It was a beautiful spiral and a beautiful elliptical-shaped galaxy. Who ordered this one, which was tangled and mangled? And he made a catalog of just the tangled, mangled-looking galaxies. And it was called the Atlas of Peculiar Galaxies.
Starting point is 00:11:11 And it was just, it was the catch basin of nothing that fit anything else. And Charles, you remember, it became one of the most studied catalogs in the canon of cosmology. Alton C. Arp. Chip Arp's Atlas of Peculiar Galaxies, published in 1966. Yes, tremendously interesting. And what it was, was it turned out that Chip Arp's ideas of why they looked peculiar
Starting point is 00:11:34 were incorrect. But by putting them together into a catalog, people could look at them and start wondering and thinking about what actually was going on. And it helped us understand that galaxies collide, that they crash into each other, and they create amazing structures, which we could not have imagined had they not collided. And that led to the entire field of computational astrophysics as applied to galaxies. And by the way, we needed the computers to make that happen.
Starting point is 00:12:03 So that was in the 1970s, computing power rose to then say, well, I wonder what a galaxy would look like if it collided with another galaxy. Hey, that matches ARP's catalog number 32.3. And then you look at it at a different angle. That's a different object in the catalog. And so all of a sudden, we don't explain all the galaxies just as witnesses to train wrecks. You guys keep saying collide. When you say galaxies collide,
Starting point is 00:12:30 is it that the galaxy's gravity affects another galaxy's gravity? Or are you looking at actual objects hitting one another? Because aren't galaxies so spread out? What is it? What's an actual collision? Chuck on the case. Beautiful,
Starting point is 00:12:48 beautiful question. When galaxies collide. When galaxies collide. That's a movie title right there. We need that one. They do. The stars are so far apart that they almost never hit each other directly. So it's like swarms of bees
Starting point is 00:13:04 or hornets, you know, nests, wings, rats through one another and affecting one another from a distance. Okay. But a collision doesn't have to happen only when a physical object hits another physical object.
Starting point is 00:13:18 Okay. What you said, the gravitational effects of one object affecting the other is indeed as much of a collision as we might think of, say, two vehicles hitting one another or something. And so instead, you get these twists and turns.
Starting point is 00:13:33 You get bends. You get loops and whirls. And it is all gravitational. Yes, indeed. So we count a gravitational encounter as a collision because they affect each other. But I've quantified this bee analogy. So if there were four bumblebees
Starting point is 00:13:47 flying randomly across the continental United States, the chances of them accidentally bumping into one another is the same as two stars colliding in two galaxies. So yeah, basically two stars are not going to physically collide, but they'll all feel each other's gravity, and that's enough to make a train wreck. And a beautiful train wreck they can be.
Starting point is 00:14:12 These kinds of train wrecks cause the formation of new stars, new planets, sometimes in the billions at a time. They feed supermassive black holes. They create quasars and active nuclei. They're one of the most important engines of the evolution of the universe itself. Wow.
Starting point is 00:14:30 The engine of the evolution. We've got to take a quick break. When we come back, more cosmic queries. Grab back. We'll be right back. StarTalk Sports Edition. Cosmic Queries. Grab Bag.
Starting point is 00:14:58 With our geek in chief, Charles Liu. All right. And, of course, Chuck and Gary. Give me some more questions. We're on a roll here. Okay. This one I think is pretty topical. So this is from Samuel Fairchild.
Starting point is 00:15:10 Greetings from San Antonio, Texas. What can we learn from the runaway supermassive black hole that was spotted by the Hubble telescope trailing a 200,000 light-year-long tail of new star formations? Answers, please. It is most likely a classic example of what happens when galaxies collide. When galaxies collide. Lots of things can happen.
Starting point is 00:15:39 In a galaxy far, far away? Yes. They could be far away. We hope they're far away, but they could be close by. Remember, in a few billion years, the Andromeda galaxy will collide with the Milky Way. Then we'll have a close-up view of what happens when galaxies collide. So the story is this, right? You have a galaxy, and it's about 100,000 light years across.
Starting point is 00:15:59 Here comes another galaxy that's also 100,000 light years across. They hit each other at just the right angle, and you can pull a trail of gas outward a couple hundred thousand light years long. Wow. When that happens, you're basically creating a stream of new stars forming all along this trail. And so there's your 200,000 light years long trail of new stars forming. Meanwhile, part of that collision could have hit. And there are many different ways galaxies can collide, but perhaps at just the right angle and at just the right speed, the supermassive black hole in one of those galaxies got stripped out of the body of the galaxies that are colliding. So whereas the rest of the galaxy's material is sort of coalescing into a single blob, that supermassive black hole
Starting point is 00:16:53 is out on a trajectory that looks like it's following that gas going outward. There's a lot of possibilities, and we've only just begun to figure out what's going on. And by the way, the gas, unlike the stars, the gas doesn't really pass through itself. When the gas collides, it's like two hot marshmallows sticking. So a lot of interesting things can happen in the gas part of the colliding galaxies, separate from the stars. Right. You can often think of the gas in a galaxy like the water in a swimming pool or something. They have a dissipative force. They are viscous. Even though they're very sparse by Earth standards, they wind up out in space sort of along the millions of years type time scales and the millions of light years type size scales acting very similarly to what you might expect. So, Charles, I did an
Starting point is 00:17:44 episode of Nova Science Now once where it was exactly that reference. I was at a swimming pool and I had a bucket, if I remember this correctly, I think I had a bucket of ping pong balls and so did someone else. And we tossed them towards each other and only a few of the ping pong balls hit,
Starting point is 00:18:00 would hit each other. But then we had buckets of water and we threw the buckets of water at each other and the water just, it was there, as you said, it's dissipative. And we did it in slow-mo and you can see it. It was pretty cool. All right, keep going.
Starting point is 00:18:13 What else you got? All right, next question up is from Moe. M-O-E. Aloha, Neil and Chuck. What evidence can you provide to show that we aren't in a simulation? Aren't? Are not.
Starting point is 00:18:29 Oh, interesting. Proving the negative. Can you prove the negative? Oh, okay. I have an attempt at it, but go on. I want to hear what my geek in chief has to say. Rene Descartes. Hundreds of years ago, right?
Starting point is 00:18:45 The guy who, you know, after whom we've named the Cartesian coordinate plane, but also a great philosopher, a rationalist of his time. Right. I think, therefore, I am. I am. Yes, yes, that's right. And he basically set out the idea that if there were a simulation that was good enough, we would not be able to tell.
Starting point is 00:19:05 There's just no philosophical way to tell as long as the simulation is good enough. So the only evidence that we can give that we are in a simulation is if somehow we see a glitch. You may remember the movie Inception. When the people in the dreams were trying to figure out whether or not they were in a reality or not in a reality. And one particular person figured out that he was in a dream because the texture of the carpet was different from what he remembered in reality. Right. So every single piece of evidence out in the universe
Starting point is 00:19:43 has to be consistent with what we think is real, right? And if not, if there's a glitch, then we're in a simulation. We can also go to the Matrix and talk about that. And how the reason they were able to know they were in a simulation was because something just didn't happen correctly. able to know they were in a simulation was because something just didn't happen correctly that's the only way according to descartes that we can prove that we are in a simulation but how can we prove we're not in one you just have to keep looking for the glitches oh wow look at that well wait so if if we don't find any glitches we're either not in a simulation or it's a perfect simulation and therefore what's the point of even distinguishing the two?
Starting point is 00:20:25 Well, then, okay. So with that, with that lineup with paranormal activities counting as a glitch. So paranormal activities are not, you know, following the laws of nature or physics or what have you. Would that count as a glitch? Listen to Chuck. That would say that we are in… So what are we calling a glitch? Or…
Starting point is 00:20:53 What's the definition? Or a miracle. A miracle or something that happens outside of the laws of physics. that happens outside of the laws of physics. Miracles and paranormal activity at this point in our understanding of the universe are only things that we don't understand yet. There's nothing that's been shown to be conclusively a violation of the laws of physics.
Starting point is 00:21:19 Just something that we haven't explained the rest of physics yet. Wait, wait, wait. Jesus walking on water violates a ton of laws of physics right there. If that actually happened. Well, now, in all defense, he has some really good sandals. Okay. Yeah, Jesus sandals.
Starting point is 00:21:43 He had Jesus sandals now. Jesus sandals. He had Jesus sandals now. Jesus sandals. So we all have to think about these questions as skeptically and as optimistically as we can at the same time. Okay, I got to add another pop culture reference. My single favorite episode of the two and a half seasons
Starting point is 00:22:03 or whatever it was of Black Mirror was the episode titled Hang the DJ, which has nothing to do with the entire story. It's the name of the song that you hear at the end. In that, it's a dating community. You date multiple people to see who one you like, and then at the end, you get married to them. And we learn. Should I give it away? I have to give it away. Otherwise, I can't talk about it. We learned that all the people in this story are being simulated.
Starting point is 00:22:34 But you don't know this because you're with them and they're testing their dating. And oh, that didn't work out. Let's date another. I got to stay three months with this person. It's all prescribed and let's all do it. And they hate each other or they love each other whatever and one of the people one of the women who likes skipping rocks skipped rocks and said you know every time i
Starting point is 00:22:54 skip rock it only skips three times and she said oh so she figured out the glitch some should skip one and some should skip four she just She just tossed it up and you don't even know to pay attention to that when that's happening. These are characters that have their own sense of free will and one of them noticed that every time she skipped rock, it was exactly
Starting point is 00:23:18 and identically three times. And we later learned that all of these people are a simulation so that when at the end you emerge and the two people, they escape the simulator, they escape this place. And as they escape, you see the digitization of things happening. And the next scene are two people meeting up in a bar who were matched by that simulation. It was like, holy shit. It's the ultimate swipe left
Starting point is 00:23:46 or swipe right. Oh my gosh. So the simulation tested everybody's compatibilities. And it was like, oh my. But in it was that one observation. So ever since then, and a little bit before then,
Starting point is 00:24:00 I've been checking for things that maybe should have different kind of variation than what should. That's interesting about the carpet, though, Charles. But do we then project our desire to find a glitch into our thinking and observations? Without question, Gary. That's a great point.
Starting point is 00:24:17 So it creates a bias. We humans are biased in one direction or another in general, right? Yeah. And just like it's very hard for all of us to be rational all the time, and maybe we shouldn't be, the circumstance is of our detecting whether we're in a simulation or not are almost secondary in importance to whether or not we are in whatever environment we are,
Starting point is 00:24:42 real or simulated, and live the way we want to live and do the things we want to do. So in my recent book, Story Messenger, I reflect on what a simulated world would be, and I use that as evidence that we're not in a simulated world. You know what it is? A simulated world is created by computers, and computers are absolutely logical.
Starting point is 00:25:02 And computers are absolutely logical. And so no set of computers would ever create the world we live in. So it's the inanity defense. It's like Earth is inane in every way. Computers have higher integrity than that, even in a simulation. That's my evidence. That's great evidence, except that you may be putting too much stock in our inanity.
Starting point is 00:25:30 It may well be that inanity is an inherent part of logical systems. No, I'm not going... Okay, Neil, would a computer be able to generate or recreate love? Oh, yeah. I don't see why not. You sure?
Starting point is 00:25:48 Yeah, I don't see why not. Depends on what you think love is. Well, no, I got this. I got that. I'm past that. Okay? So watch. So watch.
Starting point is 00:25:56 You get everybody who's in love with something or some other person, right? And then you do a brain scan. And I'm making this up, but it's plausible. You do a brain scan, and everyone has the same part of their brain lit up while they have these feelings of love. Right. Then you take someone who doesn't have those areas of the brain lit up and show them
Starting point is 00:26:13 something that's completely neutral, right? Like a book, just a book cover or something. Then you light up that part of their brain and see if they fall in love with the book. And if they do, we know exactly what love is. It's the neurosynaptic of this section of the brain. There it is. And we can create it for you
Starting point is 00:26:29 if you want it. If two people are in long marriage and they're falling out of love, go back and re-stimulate them. Go back in love if they're newlyweds. I mean, clearly love is a neurochemical synaptic function of the brain. It just has to be on a biological level.
Starting point is 00:26:47 Otherwise, you know, I mean, you can attach ethereal qualities to it, yes. But, I mean, people who, if you don't have, if you are brain dead, you can't be in love, period. Right. In fact, you don't have to be fully brain dead. You can be partly brain dead in the section that would matter in that category right but sometimes it makes no sense no no way as a matter of fact we have people who are incapable of love okay we call them sociopaths yes they're incapable of of empathy and capable of, but you have to have empathy to have love. Imagine a person who does not, imagine a person that is somehow perhaps what we might call defective and unable to experience empathy or love.
Starting point is 00:27:37 This person carefully studies thousands of people who are happily in love, figures out all the behaviors that are observable from an outside person of how to be a person who expresses and shows love, and then just mimics all those behaviors beautifully. Running into a person or choosing a person to treat that person that way, to work with that person that way, to do the things with that person that all those other people in love are behaving. Is that person exhibiting love to another person? No. You can't tell.
Starting point is 00:28:17 That's why we go inside your brain with the brain scan. That's what a brain scan is for. That's the whole point of the brain scan. If you don't have that part of the brain lit up, but you behave as if that part of the brain with the brain scan. That's what a brain scan is for. That's the whole point of the brain scan. If you don't have that part of the brain lit up, but you behave as if that part of the brain were lit up, are you still behaving with love? So I'm going to say from a utilitarian standpoint, no, you are not.
Starting point is 00:28:35 Because the only reason you would do that is because somehow you are being served. Otherwise, you would not be a sociopath. You would actually be exhibiting love itself. Perhaps your definition of behaving in a way that's self-serving is to behave in a way that everybody else in the world looks to you as if you are in love. But then are you? You may not be from your brain's point of view.
Starting point is 00:28:59 Carl, that's why I introduced you to science here, where you go inside the brain. That's the whole point of that. I'm asking you a different kind of science. From the observable perspective, assuming no hidden variables, assuming that the interior of the brain is unknowable. I'm not going to have to assume something that's not true. But quantum mechanics, for example,
Starting point is 00:29:22 suggests that indeed there are things about particles at certain levels which are not observable. I agree, but we're talking about your brain and not a particle. Can your brain behave in that way if the brain were considered not something that you can poke and prod? What if love, in fact, does not light up the same part of your brain? All right. When we come back, more StarTalk Sports Edition Cosmic Queries with our geek and chief, Charles Liu. We'll be right back.
Starting point is 00:30:02 We're back. StarTalk Sports Edition. Cosmic Queries Grab Bag with our geek and chief, Charles Liu. Charles, how do we find you on the internet? Oh, well, at Chuck Liu, C-H-U-C-K-L-I-U, on Twitter, and at TheLuniverse,
Starting point is 00:30:20 T-H-E-L-I-U-N-I-V-E-R-S-E, on a wide variety of platforms. The Loonaverse. Yeah. Podcast is going wherever you get your podcasts. We have lots of conversation and fun with that.
Starting point is 00:30:34 Yeah. All right. Cool. Cool. And Chuck Nice, you're still Chuck Nice comic? Everywhere, sir. Thank you.
Starting point is 00:30:39 Everywhere. Cool. Cool. Gary, are you still three left feet? Yes, I am. On Twitter. On Twitter. All right. My three left feet. All words. My three left feet? Yes, I am. On Twitter. On Twitter.
Starting point is 00:30:45 All right. My three left feet. All words. My three left feet. You got it. All words. Sorry. So, we got more questions here. Bring it on.
Starting point is 00:30:52 We have. Right. Matt Berg says, Hello from Sheboygan Falls. I believe that's Wisconsin. Sheboygan. You're welcome. I have used many of your discussions in my classroom
Starting point is 00:31:03 to have my middle school students think a bit deeper about things. Teacher in the house. All right. Is there a simple… So, here we go. Pay attention. Is there… Sit up straight.
Starting point is 00:31:14 Is there a simple way to… I'd start now. Is there a simple way to explain to students what our universe is expanding into? In other words, if the Big Bang Theory to students what our universe is expanding into. In other words, if the Big Bang Theory created everything in our universe, does that mean that there has to be something outside of our universe, or how can there be
Starting point is 00:31:33 a nothing that is being expanded into? At this moment, this gentleman, Matt Berge, his mind starts to hurt. Ooh. That's not so bad. There's nothing wrong with a head hurt. Yeah. Have you know that a friend of mine who is a doctor, graduated from Ivy League school
Starting point is 00:31:52 and Stanford and stuff, asked me that very same question not that long ago. So you are in good company, Mr. Berg. Here's my way of explaining it. You are at the center of the universe right now. When we make measurements and try to figure out where the center of the universe was that it was expanding out of, it always goes to you. Whoever is observing observes that they are the center of the universe. So in other words, we are part of the Big Bang.
Starting point is 00:32:27 When the universe was microscopically tiny, that is what has become us today. There's no central point because we are at the center. The center just happens to have gotten really, really big. That's one way of thinking about where the center of the universe is. You are the center of the universe. I'm sure your mom told you that at one time or another,
Starting point is 00:32:46 or you thought that you were that at one time or another. I loved when she told you that. That's right. In fact, physically. So what are we expanding into? Because that's where it started. The expansion into, you can think of as a different dimension. You can think of it as, say, space being three-dimensional, length, width, and height, expanding intotime where the expansion direction is in time, Neil.
Starting point is 00:33:27 Where t equals zero, at time zero was the Big Bang, the universe was very small. And now time has gone on, t is about 13.8 billion years, and now the universe has expanded in that fourth dimension of time. You can find lots of different ways of thinking about it that are mathematically equivalent. So maybe if you're not exactly getting the way that I'm describing it, maybe the way that you foresee it or think about it or envision it
Starting point is 00:33:53 is just as mathematically valid as the way that I'm talking about it right now. Wow. That was elegant, Charles. I got to give it to you. That was... I can't take credit for that. That was really cool, man. Well, thank you, Chuck. But, you know, remember, I didn't come up with this, right?
Starting point is 00:34:10 Our scientific forebears, you know, have been working on this for a long time. And when they first came up with these ideas, they were hard-pressed to explain them and understand them because they're so different from what we thought about when we were in those times. I'd like to add to it that you can have a multiverse where everybody's expanding, but if you're embedded in a higher dimension, then you will not necessarily collide,
Starting point is 00:34:35 even if you can go to infinity. So if you take a sheet of paper and send it to infinity in every direction, so it's an infinitely large sheet of paper, now I can take another sheet of paper, lift it off of that into a higher dimension, a third dimension. Right.
Starting point is 00:34:51 All right? And now it's just, quote, parallel to the other one. That can go to infinity and never intersect the other sheet. And I could do that into infinity. To infinity. And beyond. And beyond, yeah. Wow. So if you embed our three dimensions into a higher dimension,
Starting point is 00:35:10 you can expand higher dimensions, and then they'll never collide if they're all in a dimension yet higher than themselves. Interesting. So there you have it. That's amazing. That's amazing. All right, another question. Let's keep them rolling.
Starting point is 00:35:19 We're on a roll. So what else do we got? Is it Gary or Chuck? Who's got the next question? Go ahead, Gary. Okay, you want another one? Just like the other one. Bring it on. Alright, Kartik.
Starting point is 00:35:30 Kartik is from Germany. If the Earth's magnetic field is caused by the iron in our core rotating within the magma outer core, how does gas giant planets like Jupiter also have a magnetic field? Do we know anything about the composition of the
Starting point is 00:35:46 interior of the gas giants? We do. And the answer we think at this moment is that far enough down in a gas giant like Jupiter, the hydrogen, which we think of as a gas, turns into a metal. It becomes what we call metallic hydrogen. And so you have a core of metal of conducting stuff that can swirl, just like the core of metal in the earth. And that's how you can get a magnetic field. Just to be clear, we didn't pull this out of our ass. If you remember your periodic table of elements,
Starting point is 00:36:29 if you remember your periodic table of elements, hydrogen is, if it's a full fleshed out table, hydrogen appears twice, once in the upper left and once in the upper right. Once in the upper left is hanging out with the metals, and in the upper right is hanging out with the gases. And if I'm remembering that correctly, Charles, is that right? It can be written that way, yes. Written that way.
Starting point is 00:36:51 And I said, well, why is it twice? And somebody said, well, sometimes it's metallic. I said, it's a freaking gas. What the hell are you talking about? Later I would learn under pressure behaves just like a metal does, just like iron. And so, yeah, so it doesn't have an iron core, but it's got a metallic hydrogen core under all that pressure, for sure.
Starting point is 00:37:07 And there it is, running the dynamo on Jupiter. A rather ferocious one at that. Sweet. Oh, yeah. Look at that. That was good. We got one more in there. Quick one.
Starting point is 00:37:19 Let's get a quick one. A quick one. Okie dokie. Let's see. Pim Bilek. I was wondering what you think is the biggest obstacle for developing working warp drive and would you see this becoming a reality?
Starting point is 00:37:34 And if yes, when? Curious about Charles' theoretical view on this. Impatient Patreon member. So, Pim, here's the answer. Charles has already built a warp engine in his basement. That's it. And he can't tell you when it's going to be released because, you know, that's classified information. The 1.3 gigawatts are the same.
Starting point is 00:38:01 Well, let me think. Let me see. Okay. The thing that is most blocking our ability to create a warp drive quickly is physics. The actual ability to travel faster than light at this point through the universe that we have right now, we don't have it. We don't have that ability. that we have right now, we don't have it.
Starting point is 00:38:23 We don't have that ability. So you have to find a way to travel through space, but not in the way that everything else travels through space. So can we actually do what the Star Trek folks are thinking or Miguel and Cubierre said,
Starting point is 00:38:37 where you create a subspace field and you put yourself inside a warp bubble, which can travel through space faster than time because the warp bubble can which can travel through space faster than time because the warp bubble can, but you can't, right? Or is it some other way where you actually have to exit our three dimensions
Starting point is 00:38:54 and go into a fourth spatial dimension and then come back in? These are the questions. The basic fundamental physics are still beyond us. We can imagine. We can have fun with it on television. Give me a date when we're going to have it. Next Wednesday.
Starting point is 00:39:11 At 3 p.m. According to reliable sources, the date is April 5th, 2063. That is according to Star Trek First Contact, the movie where Picard travels through time and goes to the board. He goes back.
Starting point is 00:39:27 He goes and sees Zephyr Cochran in Montana. The one who invented the drive. That's right. And the Vulcans came. And the Vulcans just happened to notice it. And they picked up his warp signature. And that changes all of human history. Right.
Starting point is 00:39:40 That event happened on April 5th, 2063. Okay, well, there it is then. Wow. That's the day April 5th, 2063. Okay. Well, there it is then. Wow. That's the day. I got to tell you, that was amazing. Let's get reality imitating art. Yeah. And make that happen. All right. I'm going to put that in my calendar right now.
Starting point is 00:39:59 Right when we're done here. All right. Charles, always good to have you, man. Thanks so much. All right. All right. Charles, always good to have you, man. Thanks so much. All right. Love to the family. And Chuck, nice. Always good to have you there.
Starting point is 00:40:11 Gary, we're all in here. Thank you. All right. Pleasure. Star Talk Sports Edition. Cosmic Queries Grab Bag. That's like the randomest fun anyone can ever have. Yeah.
Starting point is 00:40:20 I think. Just did. Yeah. All right. Neil deGrasse Tyson here. Thanks for listening. And as always, keep looking up.

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