StarTalk Radio - Cosmic Queries – Cosmic Collisions

Episode Date: May 31, 2022

What happens when two galaxies collide? On this episode, Neil deGrasse Tyson and comic cohost Chuck Nice answer questions about explosions, asteroids, quarks, and all things that go BOOM. Was our Big ...Bang someone elses Big Rip?NOTE: StarTalk+ Patrons can watch or listen to this entire episode commercial-free here: https://startalkmedia.com/show/cosmic-queries-cosmic-collisions/Thanks to our Patrons badutjelek2000, Dominik Appl, Justin Quinones, Sandra Makela, REGAN MCGEE, Dana S., Howard Clemetson, George Sharabidze, GR 只, and RK Threethreethree for supporting us this week.Photo Credit: NASA 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, Cosmic Queries Edition. Neil deGrasse Tyson, your personal astrophysicist, with Chuck Nice, Chuckie Baby, my co-host. Hey, Neil, What's happening? Yeah, yeah. And on your resume now, it starts saying Chuck Nice actor. Yes.
Starting point is 00:00:31 In addition to comedian. What's up with that? Well, I just figured, what the hell? Put it on my resume. Did you say you were acting like a comedian? Right. Yeah. That's what I'm on as well.
Starting point is 00:00:42 I'm acting like a comedian. So let me just put that on the resume. Put that in there? Why not? Right. Exactly. You's what I'm, I'm mine as well. I'm acting like a comedian. So let me just put that on the resume. Put that in there, why not? Right, exactly. You know what I mean? So today's topic is a fascinating one, and it's so ubiquitous. It is so ubiquitous that, in fact, in the repertoire of public talks I give, one of them is entirely on this subject.
Starting point is 00:01:03 Okay. And so I will visit a town, go to a theater, and 3,000 people will come and listen to me talk for two hours on this subject. And it's called Cosmic Collisions. Oh. Oh. Have you been injured in an accident? Minus the attorneys.
Starting point is 00:01:24 Yeah, most Cosmic Coll collisions, you're not injured. You are vaporized or you die in some way. Wow. So it's just things that go bump in the night and in the day. So much that drives this universe is the result of things slamming into other things. It's just astonishing. Ways you might not have even thought about it. I'll give you a simple one.
Starting point is 00:01:49 For example, you've heard of aurora, like aurora borealis. I've heard of northern lights. You know what the southern lights are called? No. Aurora australis. Oh, okay. Didn't know that.
Starting point is 00:02:01 There you go. Crikey. Yeah, it's your northern hemisphere bias for you to only think of northern lights and not think of southern lights, right? So these are collisions between charged particles from the sun, what we call the solar wind, and our atmosphere, our upper atmosphere.
Starting point is 00:02:24 These particles slam into atmospheric molecules, and it kicks them up to higher energy levels. And generally, atoms and molecules don't like staying at higher energy levels. They can't help it. And so then they de-excite. And to de-excite, in many cases… They get married. In the cases...
Starting point is 00:02:47 My life is way too exciting. I need to calm this down. God, stop. So they'll de-excite. And in many of the cases, the de-excitation gives off visible light. And the visible light is oxygen, it's nitrogen, sometimes it's sodium, other sort of chemical elements in our atmosphere.
Starting point is 00:03:14 That's what gives you the different colors. Like fireworks. And because the solar wind comes in sort of waves, if I call it that. It blows in. From across the solar system. So the aurora can change shape, like, instantly, right? It's an active, dynamic phenomenon. And so that's just one example of cosmic collisions.
Starting point is 00:03:40 And so I'm leading off with that. I don't know if anyone's going to ask that. But apparently you got, like, a whole boatload of questions on this very subject. So let's see what you got. You're absolutely right. It is a boatload. Look at this. Every time I do this and I still have like…
Starting point is 00:03:55 You're scrolling the screen? I'm scrolling. Like, yeah, look at that. Look at that. Look at that. It's unbelievable. All right. The number of questions we have.
Starting point is 00:04:04 And because I gave an entire talk on this, I am the local expertise on the topic. So normally if it's a new topic, we bring in somebody to help us out on the Cosmic Queries. No need for this. No, I'm good for this, yeah. Oh, cool. And if I don't know, I'll say I don't know.
Starting point is 00:04:20 All right. But you never believe me. I was going to say, okay. I mean, that's just not going to happen. All right. Actually, never believed me. I was going to say, okay. I mean, that's just not going to happen. All right. Actually, that's not true. There are times when you're like, okay, well, we don't know. But that's not going to stop you from talking to the subject in some way.
Starting point is 00:04:37 That's true because we might know something. Plus, there are two kinds of I don't knows. There is I, Neil deGrasse Tyson, don't know because I haven't learned it. And we don't know as it is unknown to all humans on earth. And part of what it is when you get your PhD in a subject is you learn thoroughly what we know and what we don't know so that you know where the frontier is so you can go there and advance human understanding of the universe or whatever is the subject of your expertise. Irrespective of the question, the answer will never be from either you nor any of your colleagues who hold that PhD. The answer will never be.
Starting point is 00:05:19 Oh, as an educator, I want you to leave still having learned something. Right. But all right, look, we can test it. I was like, oh. Oh. Oh. Yeah, I'm more literate than that. By the way, how cool would that be?
Starting point is 00:05:40 Oh. Or you know what else would be cool? What? When you give an answer and at the end of it you go, doy. No. I know. All right, give it to me. All right, here we go.
Starting point is 00:05:58 Here we go. This is Dade Bloomfield. From? Do we know where they're from? I like when they tell us where they're from, no? Dade does not. Okay, we got to solic Do we know where they're from? I like when they tell us where they're from, no? Dade does not. Okay, we got to solicit that next time. Okay, so go on.
Starting point is 00:06:09 So Dade says, hey, Dr. Tyson, Lord Nice. I'm Dade from Milwaukee. Sorry, there it is, Neil. You got it. Milwaukee in the house. Inside the body of the question. How likely is it? That just means you didn't read the questions in advance.
Starting point is 00:06:27 I think I got time to read these questions. You know how long some of these questions are? Okay. Dave, who secretly two sentences later is from Milwaukee. There you go. Dade, as in Dade County. Okay. That's so funny because I'm so busted.
Starting point is 00:06:47 He says, how likely is it that if an asteroid were to hit the Earth, that we would actually notice it in time enough to react? If we noticed it today, how long do you think it would take us to come up with an executable plan? Yeah, so I assume he means that if we know that tomorrow an asteroid is going to hit, what can we do in the next 24 hours? Right. Okay.
Starting point is 00:07:08 So, of course, it depends on the size of the asteroid, right? So, 65 million years ago, when an asteroid the size of Mount Everest struck the Yucatan Peninsula, what is today the Yucatan Peninsula, left a, you know, 100-mile diameter crater, on that order of size. It doesn't, you just kiss your ass goodbye. You know, 70% of the world's species went extinct, okay, including all the big-toothed dinosaurs.
Starting point is 00:07:38 So there's certain size asteroids where you just sit on the beach and just watch it happen because there's really nothing we know how to do about it. All right. So that's just that. So it's not that in principle, nothing can be done. Right now, we have people fighting over whether Earth is flat or whether they should take a vaccine. And you think we're going to coordinate in order to deflect an asteroid? I don't have that much confidence in civilization, sadly.
Starting point is 00:08:05 So, but if it's smaller, let's say something that might take out a city, right? Oh, okay, that's, yeah, so manageable. Death matter, totally manageable. Yeah. Yeah, so what you do is you find out where it's going to hit. Usually there's uncertainty in the calculations of where it's going to hit.
Starting point is 00:08:20 So we have what's called an error circle. But if it's something coming in at an angle, it becomes an error ellipse, an uncertainty ellipse. So usually, in other words, you know better where it's going to land left to right than you will front to back because it's headed in that direction, right? So the error ellipse is this elongated circle
Starting point is 00:08:43 in the direction of the path of the asteroid itself. So you find out what that is and then evacuate it. Okay, that's not all that hard. I mean, think about what happens. I live in Manhattan. And think about it. Every 24-hour period, millions of people enter and exit that island. Very poorly.
Starting point is 00:09:06 In their workday, okay? Through a system of bridges and tunnels and boats even. So that's New York. Millions move, okay? So it seems to me if we have some idea of the region where we'll hit, we could notify local authorities and they can clear out that zone, allowing the thing to fall so no one will actually get hit. Now, if you happen to be nearby,
Starting point is 00:09:31 it's going to explode on impact, make a crater, but that explosion will scatter debris into the area and it'll rain down asteroid particles and Earth particles that have been kicked up. But that's less deadly than being where it actually hits and explodes. And by the way, it will explode. And you say, well, how is it going to explode if it doesn't have any bombs? So here's how that works.
Starting point is 00:09:57 Okay. This is a very subtle point. It's a high-speed impact, which has a very specific meaning. It's not just that it's going fast, okay? All right. So here's an object moving through space. And you ask, well, how fast is it going? How fast is it going?
Starting point is 00:10:13 At its speed, it'll hit us at a minimum of 25,000 miles an hour. Okay? That's about seven miles per second as a minimum. All right? But that's if it just sort of fell to Earth. If it has motion of its own combined with motion from Earth, then what you really care about is the closing speed. And then that could be upwards of 40,000 miles an hour, okay?
Starting point is 00:10:38 Nearly double that, okay? So you have to just sort of watch for those numbers. So here we go. So here's it coming in at very high speeds. Now, you can calculate what we call the kinetic energy. You probably heard the term. It's a very specific measurement you make. You ask how much mass is there and how fast is it going.
Starting point is 00:10:57 Okay, that's all the only two things you need. That's all you need. That's all you need. And so kinetic energy is… Two ingredient cakes. It's one half times the mass of the object times its velocity squared. Okay? Okay.
Starting point is 00:11:09 But the mass times the velocity squared. Oh, by the way, it's not an accident that the famous, what's Einstein's most famous equation? E equals mc squared. Notice there's a mass and c is the speed of light squared. But notice it's a mass and a velocity squared. It's an energy. So mass and a velocity squared are energy no matter how you slice them. Okay?
Starting point is 00:11:32 So one way to write down a value of energy is the mass times the velocity of that object squared. That's all. That's all I'm talking about. It's not an accident. Okay. That equals MC squared has that same structure to it. So kinetic energy is one half MV squared. All right.
Starting point is 00:11:47 Write down that number. Okay. Write it down. Now ask yourself, what's holding the thing together? All right. Right. So go down to the molecules. And they're molecules connected to each other inside this solid object.
Starting point is 00:12:04 Molecules connected to each other inside this solid object. And you can ask, with what energy are these molecules hanging on to each other? Okay? So imagine you and I are standing next to each other. We just lock elbows. Okay? So we're all just molecules locking elbows. What will it take for two people to pull us apart?
Starting point is 00:12:21 That's a certain energy. Right. That will either release your grip. Or rip your arm off. Or rip your arm energy. Right. That'll either release your grip. Or rip your arm off. Or rip your arm off. Right. Both of them. You can calculate what those energies are.
Starting point is 00:12:33 You can either release the molecule or bust the molecule open. All right. Right. Do that for all molecules in the object. That's a total energy. It's called a binding energy of the object. Okay. Okay. So now I have a kinetic energy of its motion and a binding energy of the object. Okay. So now I have a kinetic energy of its motion
Starting point is 00:12:46 and a binding energy of the physical object. And you ask yourself, which of these is larger? If the kinetic energy is larger than the binding energy, we'll call it a high-speed collision. And here's what happens. This object is coming in. It slams into Earth with very high kinetic energy. Well, velocity is one of the terms in the kinetic energy equation.
Starting point is 00:13:14 After it hits Earth, how fast is it moving? Oh, minus whatever. How fast? Oh, as it hits Earth, it's moving at the velocity. Oh, it already hit Earth. It hit Earth. How fast is it moving? It's just stopped.
Starting point is 00:13:27 Give me a velocity. Right. Oh, minus the... No, no, didn't minus... I'm asking a simple question. Oh, how fast is it moving? The velocity. What is the velocity after it has hit the Earth?
Starting point is 00:13:38 Oh, I don't know. Yes, you do. It hit Earth. Oh, zero. Thank you. Zero. It's zero okay so then i asked you where did all the kinetic energy go no such thing as a free lunch in this universe so all that kinetic energy on impact with the earth it did several things things. One, it makes a crater. It flies things up into space.
Starting point is 00:14:08 But it also goes back into the object itself, completely destabilizing everything that's binding it together. Because it's more energy that's holding it together. And so the instant that happens, the thing can't stay together, and so it explodes. Period. That's how you get the explosion. That's why you get the explosion.
Starting point is 00:14:33 In fact, that's why every crater you have ever seen on the moon is a good example. But look, anywhere in the solar system is a perfect circle. Right. Even if these suckers come in at an angle, you'd think, oh, it'll make an oval crater. Yes, the uncertainty ellipse
Starting point is 00:14:49 is an ellipse, but once it hits, it explodes. And the explosion is what we say is isotropic. The force is the same in every direction. It makes a perfectly circular crater, and usually the object can't be found it'll vaporize 90 something
Starting point is 00:15:08 percent of the object if you're going to look for a big rock that's there you're not going to find it wow in fact they did you know that big arizona is known for its holes in the ground okay yeah so one of them is a meteor crater we call it, you mean actual celestial-caused holes in there. I thought you meant dive bars. I was going to say, yeah, you're absolutely right. All those are holes in the wall, not holes in the ground. Oh, that's right. They are holes.
Starting point is 00:15:34 Yeah, yeah, that's right. So with that, when people said, you know, if this is left by a meteor, there ought to be a big meteor down in the middle. So they started excavating. They could find anything. It's before we understood this whole concept of a high-speed impact, a high-velocity impact, where you basically vaporize the object in an explosion.
Starting point is 00:15:58 It's a cosmic pillow fight where the pillow explodes and there's all the feathers. And we're still frolicking. Well, that's an important analogy because a high-speed collision has not as much to do with the speed as it does what is the thing made of, right? So what's holding your pillow together is some stitching around the edge. Exactly. If I slam it hard with more energy than that stitching, and it hits you upside the head, the stitching will break and the pillow will break open
Starting point is 00:16:29 because in that moment, the pillow engaged in a high-speed collision. Yeah. Same thing happens with a sock full of oranges. Don't ask me how I know. Yeah, I'm not coming over for your next sleepover. What the hell are you doing? All right.
Starting point is 00:16:49 So, yeah, that's a long answer to that very good question. Nah, that was cool, man. You can just evacuate. You can evacuate in 24 hours. That's why we have roads, right? And why everybody has cars. So, plus you can evacuate in every direction, okay? In most places.
Starting point is 00:17:04 Unless you're like in the Florida Keys or something now you gotta go just that one direction by the way if it falls in the ocean then you gotta watch out
Starting point is 00:17:11 for the tsunami okay yeah just something to keep in mind but most of the earth is ocean right
Starting point is 00:17:18 yes and so you just leave away from the coastline and most of that which is land is not inhabited so chances are it's not gonna hit a city even if it had the power leave away from the coastline, and most of that, which is land, is not inhabited. So chances
Starting point is 00:17:26 are it's not going to hit a city, even if it had the power to destroy one. Now I can sleep. Okay. That's not bad at all. All right. Give me another one. Okay, this is Teresa Anosky. She says, how can there be a collision, cosmic or otherwise, without a lawyer being
Starting point is 00:17:42 involved? Oh, so this is a new dimension for lawyer ads, right? Exactly. Was your house destroyed by a meter? Yeah, who are you going to sue on that one? Yeah, yeah, yeah. So just an interesting point there. One of the brightest, most devastating recent,
Starting point is 00:18:04 now nine years ago, was in Chelyabinsk, Russia. There was an air blast of an asteroid 17 meters across. Some of the best footage we have of that coming in are from forward-facing dash cam footage of cars. And so here's an interesting point. And that's, you know, Europe and parts of Asia have these to obtain video of a collision that you might be in, which reduces the need for lawyers. Okay. Often a lawyer is arguing whether something did or didn't happen or who was at fault or who was more at fault than they're claiming. And all of this, if you have video, that just cuts through so much of what might otherwise happen in a courtroom.
Starting point is 00:18:55 So you can imagine a day where everything, I mean, I wouldn't want this because it's an invasion of privacy, but if everything, we had a video of everything. Well, okay, that didn't make a difference with uh in los angeles in 1991 not i was about to say sorry you have all the video you want what's that boy's name i forgot uh that was rodney king King. Okay, so I take it back. Apparently, video doesn't matter in some cases. Okay? If you're getting your ass whooped by the cops, apparently, it doesn't matter. But for everything else, it might matter.
Starting point is 00:19:33 Exactly. So, yeah, it's a testament to the fact that human sensory systems are rife with error. Not only seeing what isn't there, thinking you're not seeing something that is, hearing something that's not, perceiving. So it's such rife with error that science really didn't take off until we were able to replace our senses with machines that would have a reliability that we could only dream of having with our own eyes, ears, nose, mouth, and touch. Chuck, we got to take a quick break, but when we come back,
Starting point is 00:20:09 more Cosmic Queries on Cosmic Collisions on StarTalk. I'm Joel Cherico, and I make pottery. You can see my pottery on my website, CosmicMugs.com. Cosmic Mugs, art that lets you taste the universe every day. And I support StarTalk on Patreon. This is StarTalk with Neil deGrasse Tyson. We're back. StarTalk Cosmic Queries. Cosmic collisions is the subject.
Starting point is 00:20:48 One of my favorite subjects. In fact, I give a series of public talks around the country at a theater near you. And I give the host a choice of what topics they might want to hear from me. Because I have nothing really to sell you other than the universe itself. And the ticket. And so they see the, I don't have a product to sell you other than, like I said, the universe.
Starting point is 00:21:14 I was joking. I know what you meant. And so it's, one of the subjects is cosmic collisions. And every now and then they pick that. And they're usually in for a treat because it's just a fun topic. And so many things shape the universe by slamming into other things, giving us what we think of as something that's beautiful or spectacular. They're really just something coming upside the head of something else.
Starting point is 00:21:37 And I think we also have an odd fascination with the macabre. Yes, we do. We do. People just want to know, like, how are we going to die? How's it all end? It's like the same thing you watch NASCAR for. For the crash. Oh, yeah.
Starting point is 00:21:52 Not one crash. This was the worst race ever. No, stop. All right. Here we go. This is Deb Beach. Deb says, hey, Dr. Tyson, a recent article from the New York Times about research in 2003 astrophysics working with astrophysicists working with NASA's orbiting Chandra X-ray Observatory.
Starting point is 00:22:13 The article notes that the sound waves were coming from a giant cluster of galaxies in the constellation Perseus caused by explosions from a huge black hole 250 million light years away. They provided a sound clip that was modified so that we could hear the quote-unquote music of the black hole. My question is, how musical noisy is our galaxy? And what other phenomena creates sounds in space? So, here's the thing. Here's the thing. I'm not a fan of turning astrophysical data into sound.
Starting point is 00:22:56 I get it, and it has some value. I'm just not a fan because of all of the off-ramps that that gives a person into thinking the wrong thing about the universe. Okay? Okay. So let me just start it out by saying anything, any energy that creates a change of pressure through a medium is creating sound. That's how your eardrum works. That's how your eardrum works.
Starting point is 00:23:23 Okay? It's creating sound. That's how your eardrum works. That's how your eardrum works, okay? There's air, there's pressure in the air, puts pressure on the eardrum, it gets converted to electrical, chemical signals that your brain then interprets as sound. Okay. Anything. So most things actually make sounds, okay? If you could hold a microphone up to the sun,
Starting point is 00:23:43 it is gurgling and they're like pressure waves inside the sun oh my gosh i'm gurgling the sun is actually boiling all right it's a very hot it's hot in the middle less hot at the surface and anytime you have a heat gradient if that gradient is strong enough it will gradient is a fast change in what it is, then you'll have boiling, such as what would happen on your stove. So, point is, what they did was, they found places in the universe where the medium,
Starting point is 00:24:15 the interstellar, intergalactic medium, depending on which research results they're looking at, that there are these pressure waves through it. Now, but they're very low frequency. Very low. Like Vaso Profundo low? Like Vaso Profundo. You all never heard Vaso Profundo.
Starting point is 00:24:41 Just Google some YouTube videos of it. It is a hoot it's nutty man it's nutty they go the voice is so low you can almost look at their their their vocal cords vibrate you know yeah anyhow so it is such low frequency that in order to hear it they had to artificially boost the frequency by 47, 48 octaves. Well, that's nothing. Octaves. Like what you heard then. Right.
Starting point is 00:25:12 So if you were there, you just wouldn't hear it. The sound would sort of wash over you. You wouldn't even know it was sound. Right. So you boost the frequency. Now you can hear it in this narrow range. Well, we have several orders of magnitude, 20 hertz to 20,000 hertz, if I remember correctly.
Starting point is 00:25:27 And that's a nice range, but it's small compared to the total possible ranges that are out there. Go ask your dog, okay? Yeah. Okay? All right. So, you know, it's funny, Chuck,
Starting point is 00:25:42 you and I grew up at a time when, in our biology books, the human body was praised as some kind of pinnacle of evolution. Yet we still use our dog to sniff out drugs because we can't, right? Dogs can hear frequencies. We can't. People say if a tree fell in a forest and no one was there to hear it, did it make sound? Yeah, because the dogs heard it.
Starting point is 00:26:02 Right. That's what your dog is hearing every time you see him just look up like, what? And there's nothing going on. Just nothing. They heard the tree fall. I like that. Yeah, he was like, another tree? Chuck, I'm going to tweet that. Right. He was like, wait, somebody just destroyed my bathroom.
Starting point is 00:26:19 Another meat on that tree yesterday. Another perfectly good bathroom just destroyed. So, so, anyhow, the point is that if you do that and then say these are the sounds of the universe, it's a little misleading because it's not what you would hear. Plus, most of the rest of space is empty and sound needs a medium through which to transmit. And so not only wouldn't you hear it when it was there, it wouldn't travel to you anyway.
Starting point is 00:26:51 So that's why I'm always a little uncomfortable talking about and thinking about sounds in space. Got you. And by the way, there's a medical condition called synesthesia. I find a fascinating condition where your sensory wiring is crossed. So I think I get it right. There's some people who hear colors, who see sounds. Okay. Yeah, so it's fascinating sort of cross-wiring of your senses.
Starting point is 00:27:32 So what we've also done is we've taken frequencies of light in images because the different frequencies, there's red, orange, yellow, green, blue, violet. Those are different frequencies of light. But we see way more than that with our modern equipment. We see ultraviolet, infrared, X-rays, gamma rays. So I've seen some people take those frequencies and attach a sound to them. And then they have that sound emanating from an image and the combination of sounds
Starting point is 00:27:54 from all the data that's in the picture. So when I first heard that, I said, no, that's wrong. You can't do that. But then I realized I was speaking with Richard Dawkins, who strongly suspects that because bats are mammals, and they have basically the same brains we do, a lot of the same processing power,
Starting point is 00:28:15 he thinks that bats hear in color. Because what else would they be doing with the part of their brain that sees color why not hand it the audio signals that they're getting from their echolocation so if a bat can hear color then i thought to myself why should i have a problem with us seeing sounds. Right. See? So in that regard, maybe we're at the beginning of a whole new way to bring data to people. Because if you're sight impaired, for example, you'd want to hear what the picture looks
Starting point is 00:28:58 like. I mean, why not? That's kind of cool. Yeah, it'd be kind of cool. There's surely a whole future in that. If you're hearing impaired or vision impaired, you bring the data into another sense, but you want to do it sort of authentically, right?
Starting point is 00:29:11 If there's a separation of frequencies, you map them into a new set of frequencies that are still separated in that new regime. So anyhow, so yeah, so that's how you get sounds in the universe. Nice. And by the way, collisions and things, they all make sounds if you're right where they are. But you wouldn't hear them if you're out in space.
Starting point is 00:29:30 That's the only difference. So in that regard, Star Wars would be silent loopy. Right. Just so you know. And there goes the box office. Okay. All right. God, it was so great.
Starting point is 00:29:46 If only they had some kind of sound effects with it, it would have been even so much better. Yeah, we don't like watching silent explosions. I think that's what that comes down to. That is murica, baby. Murica. Murica. We're really good at blowing stuff up,
Starting point is 00:30:04 and we're less good at knowing where the pieces go at the end, by the way. That's a whole other conversation. Chuck, we've got to take a quick break. When we come back, part three of our three-segment Cosmic Queries about cosmic collisions. Chuck, we're back. You know, I've been giving sort of luxurious answers to those several questions we've had so far.
Starting point is 00:30:29 That's fine. No, let's do a little bit of lightning round. I want to show people I'm capable of that. Yeah, I'd just say we do another show, a second show. If you didn't get your question asked, then come back. We'll do it again. We'll do it again. You'll get your question.
Starting point is 00:30:44 I'm still going to try. Okay, go. We'll try. Here we go. Here we go. Zachary Clire? Clire. Clire. Okay. Zachary says, Greetings, Dr. Tyson, Lord Nice. I recently read that upon a recent published work in which researchers
Starting point is 00:30:59 suggest that when two progenitor galaxies collided head-on, their dark matter and stars would have sailed past each other. The dark matter would not have interacted with the stars, which would not have been able to, too far apart, to collide. But as the dark matter and the stars sped up, the gas in the space between the two galaxies and stars would have crashed together, compacted, and slowed down,
Starting point is 00:31:26 leaving a trail of matter that formed, dun-dun-dun, a new galaxy. You just described galaxy sex, bro. Wait, did his question have the sound effects in there, too? Or did you add those? No, I… Did he go, da-da-da? No.
Starting point is 00:31:49 Everything spoken there is accurate. So here's what happens. The galaxy collision is one of the most beautiful, balletic things you've ever seen. Okay. So first of all, galaxies are mostly empty of stars. Right. All right? seen. So first of all, galaxies are mostly empty of stars. So if there were just a few bumblebees flying randomly in the continental United States, there's a greater chance that two of them would accidentally bump into each other than for two stars to collide when two
Starting point is 00:32:20 galaxies come together in space. That's how empty, empty space is. Wow. So when the two galaxies come, they will basically pass through each other and come out the other side, okay? The dark matter, whatever that is, we don't know what it is. The dark matter will do the same. Why?
Starting point is 00:32:38 Because dark matter not only doesn't interact physically with our matter, it doesn't interact chemically, it doesn't interact with itself our matter, it doesn't interact chemically, it doesn't interact with itself. So it would have to interact in order to make a dark matter planet, for example, or a dark matter star. Something has to work such that it can become compactified.
Starting point is 00:32:57 Why are you a solid object, Chuck? Because your molecules are sticking to each other in some way that turn you into Chuck. Dark matter, as far as we know, has no ability to stick to us or to stick to itself. So the dark matter passes. But the gas clouds, oh, they are not going to, you can't pass gas through gas. Yeah. All right.
Starting point is 00:33:19 I'm sorry. Before I trigger a cascade of flatulence jokes. Not that we can't pass gas. Gas clouds cannot move through other gas clouds without consequence. And it's like two hot marshmallows touching each other. They stick. Right. You ever done that? Two hot marshmallows? Absolutely other, they stick. Right. You ever done that, two hot marshmallows?
Starting point is 00:33:45 Absolutely. It's like contact cement. So everything else passes through each other, the gas sticks together, and that energy feeds the formation of new stars. And so these filaments of gas that are left over from these collisions, you can basically form an entire family of dwarf galaxies by doing this.
Starting point is 00:34:10 That is pretty damn amazing. So yeah, so these are collisions. And the problem is it takes about a quarter billion years to fully go through this collision. So we know they happen primarily only because we simulate them on the computers. And just so you, I want you to appreciate my people, okay? If you're going to collide two galaxies,
Starting point is 00:34:33 every inch the galaxy moves closer to itself, the sum of all the gravity vectors operating on every point in space changes. Right. So if you're a star, you take three steps to the left. Everybody else took three steps to whatever they're going. And now the total gravity field is different. So you have to recalculate what's tugging on you and in what direction.
Starting point is 00:35:01 And once you go through this exercise, that's when you find this extraordinarily balletic collision. It's like a train wreck, right? The structure, the beautiful structures of the galaxies get completely destroyed and distorted. And it's just beautiful. So if I wanted to see a phenomenon in the universe, I would want front row seats for a quarter billion years on the collision of galaxies. Very cool. Oh, I left something out. So these gas clouds will make their own shards of galaxies.
Starting point is 00:35:32 But the system of stars, they will pass through each other, come out the other side, but they still see one another. And then they'll slow down, stop, and then collide again. they'll slow down, stop, and then collide again. And this will continue until it settles into a new galaxy, into a new galaxy that is completely
Starting point is 00:35:52 that has lost all of its if there were spiral galaxies, completely lost all of its beautiful spiral structure. And it'll become one big giant blob of stars. And if they each had black holes, the black holes will find each other and merge in the middle. Okay. Yeah.
Starting point is 00:36:07 Alright. To back up when that's happening. Yeah, man. Alright, that was not a soundbite answer, so keep going. That was fascinating. All good. Fascinating. Here we go. Hello, Dr. Tyson. Lord, nice. This has been plaguing me for a couple of years now. Who is this?
Starting point is 00:36:23 Who is this? Oh, I'm sorry. Yeah, James Weldon. Sorry, James. Thank you. Yeah. This has been plaguing me for a couple of years now. Who is this? Who is this? Oh, I'm sorry. Yeah, James Weldon. Sorry, James. Thank you. Yeah. This has been plaguing me for a couple of years now. Is it possible the Big Bang and the Big Rip are causally connected? I heard from a science YouTuber once that the amount of energy needed to split elementary particles such as quarks is so infinitely great that
Starting point is 00:36:47 the very act would mathematically create new elementary particles rather than actually splitting them. Well, I'd like that. By the way, the namesake of this format, Cosmic Queries, became a book published by National Geographic a couple of years ago, and there's an entire section on how the universe will land. All right. And all of the hypotheses are there, including the Big Rip, which would happen in 22 billion years if, in fact, the acceleration of the universe continues. So here's what's interesting about the universe.
Starting point is 00:37:21 Wherever you have a lot of energy, stuff happens. Okay. Stuff happens. Okay. Stuff happens. I'll give you an example, okay? Do you know what protons and neutrons are made out of? Sugar and spice and everything nice. Yes, precisely that, Jackson. Made out of quarks, okay?
Starting point is 00:37:39 Now, we've never found an isolated quark. They're always in pairs. Okay. Always. Okay? All right, so now, well, why not? Now, we've never found an isolated quark. They're always in pairs. Okay. Always. Okay. All right. So now, well, why not? Why don't we just get in there and rip them apart?
Starting point is 00:37:50 Right. Okay. Well, here's what happens. As you pull them apart, they pull on each other more strongly. Oh. As the distance increases. It's like a finger puzzle. Okay.
Starting point is 00:38:02 Or something even, do people have finger puzzles anymore? No. Okay, they don't really have, but, well, just a rubber band does that. Right, that's true, yeah. Right? As you pull on it, it's pulling on you more strongly. So this is a force that operates the way a rubber band does, but watch what happens. If you pull on a cork
Starting point is 00:38:20 with enough strength, I finally got it, check, check, I got it, I got it, and then it snaps into two. The energy you put in was exactly enough for the snapping rubber band to create another quark. And now you have two pairs of quarks
Starting point is 00:38:38 instead of one. Nice. Yes, yes. It is like, don't F with me. Okay? You see I'm happy here as a pair of quarks. Don't.
Starting point is 00:38:48 Yeah. That's some loan shark stuff right there. That's right. So I'd like the idea that the energy required to rip the universe, the very fabric in the universe, is sufficiently high that it could create multiple big banks. I haven't researched that enough to know if there's something that would prevent it. But I'm telling you that energy is opportunistic.
Starting point is 00:39:10 Right. And so I like that possibility. Yeah, this is kind of cool. It could be that our Big Bang was somebody else's Big Rip. Somebody's Big Rip. Yeah, yeah, there you go. Oh, man. I don't want everything to come from anything termed the Big Rip.
Starting point is 00:39:25 So I don't want that to be. I don't want everything to come from any term anything termed the big rip so I don't want that to be I don't I don't know what else to call it it is the universe is ripping I don't know what else I'm going to do you know yeah but if you go
Starting point is 00:39:35 if you check out the book there's a whole section if you want to know all the ways the world would end alright Chuck do we spend so much time Chuck
Starting point is 00:39:42 we don't have time no alright one more quick quick quick. All right, here we go. Dr. Tyson, Lord and I, when we detect a gravitational... Who is this? Wait, wait, who is it?
Starting point is 00:39:50 Who is it? Jason Whiter. Okay. Jason Whiter. Okay. Dr. Tyson, Lord and I, when we detect gravitational waves from the collision of two black holes, what happened to their event horizon? Oh, very cool. Whoa, that's a great event horizon? Oh, very cool.
Starting point is 00:40:07 Whoa, that's a great question. It is, it is. And in fact, don't we have an explainer on this with our Black Hole in residence, Black Hole expert in residence? Jan 11. Jan 11. Yes, we do.
Starting point is 00:40:17 I think we do talk about this. Yes, we do. I think it was in an explainer, but I'll just tell you right now, and then we got to call it a quits. Okay. So what happens is the two event horizons merge to become one larger event horizon
Starting point is 00:40:32 surrounding the total mass of the two objects together. That's what happens. Okay. They enter each other's event horizon when this happens. And Jana gives a brilliant explanation for how that happens and why it happens. And so I recommend you do a fast search on that and you'll get there. All right, Chuck, we're going to call
Starting point is 00:40:52 it quits there. That was great, man. And guess what? We still have like 60 questions left. Okay. Which is awesome. All right, we'll do this again. We totally will do this again. Cosmic Queries, second edition, the sequel. We'll just number them up because there's no end of this.
Starting point is 00:41:10 And like I said, it's one of my favorite subjects. So Chuck, tweeting at Chuck Nice Comic. Thank you, sir. Yes. I never give my social media handles on this, but maybe I'll. Because you don't need to. Stop. If I had 14 million people following me on anything,
Starting point is 00:41:27 by the way, I would stop giving it. Like, hey, guys, stop. Take it easy. Chill out, okay? I need a second. Can I get a second? You know. All right, I'll do this one time, okay?
Starting point is 00:41:39 On Twitter, it's Neil Tyson. And on everything else, it's Neil deGrasse Tyson. On Facebook, TikTok even. And the TikTok is an official TikTok of StarTalk, by the way. Nice. We have a bunch of us making sure that works out.
Starting point is 00:41:53 And I'm in all the content, but we have people, experts, TikTok, you know, people one-third my age. That's a definite TikTok expert. It's cool, man. Oh, that's so funny. Yeah. You got a toddler just like. It's cool, man. Oh, that's so funny. Yeah. You got a toddler just like,
Starting point is 00:42:07 here's your problem. You're not going to be able to get engagement if you keep doing this. Exactly. By the way, do you know when they're going to stop this shortage of baby formula? All right.
Starting point is 00:42:29 This has been Cosmic Queries, Cosmic Collisions Edition, the first of what will surely be many. Neil deGrasse Tyson here. Keep looking up.

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