StarTalk Radio - Cosmic Queries – Cosmological Curiosities

Episode Date: August 15, 2023

What is nothing? Does nothing exist? Neil deGrasse Tyson and comedian Chuck Nice explore cosmological curiosities about the end of the universe, dark matter, and more!NOTE: StarTalk+ Patrons can liste...n to this entire episode commercial-free.Thanks to our Patrons Matej Dvonč, Robert Weaver, David Lindberg, Denis, Jesus Hernandez, and Jack Reeves for supporting us this week.Photo Credit:  NASA / JPL-Caltech / L. Jenkins (GSFC), 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
Discussion (0)
Starting point is 00:00:00 So there are galaxies that are like 65 million light years away from Earth, okay? From our galaxy. So right now, if they had a super-duper telescope and they looked towards Earth 65 million years ago, what are they witnessing? Dinosaurs, right? Oh, and they're getting killed! Yeah! It just dawned on me what that time frame was. I'm like, oh, snap.
Starting point is 00:00:27 I know. The Earth is putting on a show for them. Welcome to StarTalk. Your place in the universe where science and pop culture collide. StarTalk begins right now. This is StarTalk. Neil de. This is StarTalk. Neil deGrasse Tyson here, your personal astrophysicist. Today we're doing the ever-popular Cosmic Queries edition.
Starting point is 00:00:55 Chuck, good to have you, man. Yeah, always a pleasure to be here. You're preloaded with Cosmic Queries from our Patreon members. So what's the topic today? We have cosmological curiosities. Which, you know, that covers enough of it. I got you. I got you.
Starting point is 00:01:10 And if something I don't know, I have to call my people. I got cosmology friends. So what do you have? All right, let's jump into it with Danny K. Danny K says, he's no. Okay. Danny K from the ether. He's just Danny K from the ether.
Starting point is 00:01:24 He goes, good morning, gentlemen of the court of knowledge and his majesty, Neil deGrasse Tyson. Dude, we're going to answer your question anyway. You didn't have to. Yes. Even though you are asking that question first. I don't know. And actually, he does put in here. He goes, I am hailing from the netherlands rotterdam come to thee and these humble inquiries of knowledge
Starting point is 00:01:50 niederland okay so what does he have there he goes he goes in a previous episode there was a mention of an expanding of our universe and that there could be a point in the distant future where we would be stretched to a point where our neighboring galaxies would be too far to reach? Would this expansion also affect our solar system as well? Does it mean that our blue ball would slowly drift away from our star? And would our star dim before that time comes? And if so, would you suggest how we might be able to survive something like this? We're all going to die. Very simple.
Starting point is 00:02:28 Yeah, so in the vacuum of space there's this mysterious pressure forcing an acceleration of the expanding universe. We have a word for it, but we don't know what it is. We had no business naming it, really. And it's called dark energy.
Starting point is 00:02:46 And I joke that we should just, you know, know dark matter we don't know what that is either we should just call it fred and wilma you know just two words that don't hint at anything physical right because we don't really know what's causing it but we can measure it and so this expansion of the universe that's accelerating, that will continue to grow. And the bigger the universe is, the more vacuum there is. And this pressure is a property of the vacuum. So as the universe expands, the gravity gets thinner. What we call the gravity density gets thinner, but the dark energy continues to grow relative to the gravity. So initially, all the galaxies will expand beyond our horizon.
Starting point is 00:03:37 And then after that, it will start ripping apart the galaxies themselves, because that's a stronger gravitational force holding them together. Start ripping that apart. And so the solar systems will be flung hither and yon. Then it'll start ripping the planets out of their solar systems. Then it'll start ripping moons from their host planets. Then it'll start ripping planets apart structurally. Then it'll start ripping apart the molecules.
Starting point is 00:04:11 Then it'll start ripping apart the atoms in the molecules. Then it'll rip apart the nuclei of the atoms. Then it'll reach the point where the very pixels that comprise the fabric of the universe will succumb to this ripping force and it's called the big rip because we do not know what will happen after that moment at At that moment, the universe will tear because it will no longer be able to stretch in response to that force. We call it the Big Rip,
Starting point is 00:04:53 and it will happen if nothing else is in the way. It's going to happen in 22 billion years. Well, there you go, Timmy. Good night, and you sleep well. Have a nice day. Have a nice day, Timmy. So,. And you sleep well. Have a nice day. Have a nice day, Timmy. So, yeah, the sun will be long dead by then. Sun will give up the ghost in about five billion years.
Starting point is 00:05:14 We're about halfway through the life expectancy of the sun. So the sun will be dead long before that happens. And so I wouldn't worry about it. Yeah, there you go. So that's the real answer. That happens. And so I wouldn't worry about it. Yeah. There you go. So that's the real answer. The real answer is, Danny, you shouldn't care. Exactly.
Starting point is 00:05:35 But I want to be around to watch that rip. That would be, yes. Except I would be in the universe that was ripping. And so I would be ripping apart as well. I live every day in a universe that's ripping. Because, you know, think about it. When you zoom in on a photo, that only works until you start seeing the pixels that comprise the photo.
Starting point is 00:05:58 If you keep zooming in, there's no more information there. But what happens if you keep zooming in and you want to break apart the pixels themselves? What's between them? Who knows? In between the pixels of the photo that you're zooming in on. And so this is the mystery and the uncertainty we have in 22 billion years. I have it on my calendar, by the way. As they say, October 12th, 22 billion years from now. 22 billion years from now. There you go.
Starting point is 00:06:29 That's very cool. I believe that's a Wednesday. Thank you. Thank you. Chuck the savant. Yes. You pick any date 22 billion years from now, I'll tell you what day it's on. All right.
Starting point is 00:06:43 This is James Booth, and he says, my question is about dark gravity. Okay. I understand. Which is what most people would call dark matter, but he knows I'm calling it dark gravity because that's literally what it is. It is gravity, and we have no idea what's causing it. It's not even black holes, by the way, or unilluminated matter. We have good reason to know that that's the case.
Starting point is 00:07:05 But go on. He says most of the matter we experience that makes up the stars of the galaxy only makes up about 5% of the content of the universe. Okay. If that's the case, which you just said it is, is it possible that given we interact with such a small percentage of the universe, we are indeed the anomaly? This really makes me feel weird. Yes, yes. So, it's imagine you're at night, and there's an ocean in front of you,
Starting point is 00:07:34 but you don't really know it. And you turn on your light, and you see these white caps, okay, which show up nicely under moonlight. And we are the white caps of an ocean that surrounds us so correct we we are if if if there were beings made of dark matter dark energy they would see us as a contaminant in their universe that's right right. Oh, look at that. Yeah, I know. I know. It's sad. Well, yeah, it is.
Starting point is 00:08:09 We are not representative of the most common stuff in the universe, which, by the way, is a violation of the Copernican principle. Copernican principle says that we are not special in time or in place or in location. We're orbiting an average star in an average galaxy.
Starting point is 00:08:27 Statistically, it says that we're average. But if we are contained within that 5% of all the laws of physics, chemistry, biology, and all the ingredients that make up matter as we know it, then we are something unusual in the universe. But could we be the average inside of the unusual? Yes, we are. So I was going to complete the thought and say, given that we are unusual, we are average. There you go.
Starting point is 00:08:59 Okay, there you go. Very nice, very nice. You know, another example of that is, you know how the school system try to corral all the smart people together, right? Well, they used to do this. They put the smart people in their own class. No, they do it still.
Starting point is 00:09:12 Okay. They have all the AP kids. Exactly, exactly. So in the general population, you're unusual because you're like smarter than everybody else. Then they put you in the AP class and now you are... And you're just average. You're then they put you in the ap class and now
Starting point is 00:09:25 you are and you're just average you see that's not everybody's smart that's right that's it that is very cool what else you got a problem i did not have therefore that little bit of math was something you didn't have to think about is that what you did not have to worry about i remember okay so i was not in the smart class in elementary school but i was in the next class because they they they totally ranked these classes and i and i remembered the kids in the smart class they got to take french i'm talking about sixth grade my elementary school before there was middle schools that would absorb a sixth grade class they took french and a french person and i said they're learning a foreign language and learning how to smoke
Starting point is 00:10:06 with the hand and a bunch of fourth graders sitting around you speak my language and it sounds like how you say a dog pissing in my ear i don't know why but you bore me a dog pissing in my ear. I don't know why, but you bore me. Why does every French person you imitate smoke a cigarette? Why?
Starting point is 00:10:35 Yeah, so I always wanted that and that was, you know, I was... Yeah. What they... They were deciding what you would be... What you would learn. Without me saying, I want to learn it and would not measure my ambitions for what I could be in life.
Starting point is 00:10:52 And this is, for me, that's a travesty. Who have we lost in the educational system for want of an educational program to identify where the ambitious kids actually are versus those who score high on a test. And more importantly, not just the ambitious kids, but what are identifying their ambitions. Exactly. Because if you identify an ambition,
Starting point is 00:11:17 you automatically excite the person to learn because they're pursuing what they already lack. Yes. Dr. lack. Yes. Doctor President. Okay. All right, next one. All right, here we go.
Starting point is 00:11:30 This is, let's go to, hey guys, this is Rotten Josh here from Somerville, Florida. My question, instead of the Big Bang, could the universe have formed from a big implosion instead of an outwards explosion? When I think of the Big Bang, I imagine exploding outwards. So I was thinking maybe it exploded inwards. And thank you for your time. I'm going to let you. Yeah, yeah.
Starting point is 00:11:58 So before we had good data on the very distant future history of the universe, there was our equations that are traceable to Einstein and others, including, what's that dude's name? He was a Belgian priest, actually, who contributed mightily to our understanding of the Big Bang. bang. And he, so, so, so it, under the Einstein's equations,
Starting point is 00:12:28 it can sustain a collapsing universe as well as an expanding universe. So people naturally said, if we measure an expanding universe, maybe it'll one day recollapse and then start all over again. Start all over. And that's where you get this sort of, um, these,
Starting point is 00:12:44 these, these rhythms. By the way, the name of that Belgian priest is Georges Le Matre. Georges Le Matre. Georges Le Matre. Le Matre, yeah, yeah. And so he took Einstein's equations and said, wait a minute, this can give us an expanding universe. And if we're expanding, that means it had a beginning.
Starting point is 00:13:02 If it had a beginning, that's interesting. And then a lot of religious people said, oh, a Catholic priest says that, in fact, there was a beginning because before then, no one knew how to think of a beginning of the universe. It was not a thought. It's not that they thought about it and said there wasn't. It's like, of course, the universe was always here. How could everything that there is have a beginning?
Starting point is 00:13:24 So we have Einstein's equations. George Lamontre says there's a beginning. And then everyone is jumping on that saying, see, Genesis is true. God's made the beginning. And so he said, no, this ain't got nothing to do with Genesis. Okay? So it was a little spat between the religious folks who are who were reaching for this scientific result and the catholic priest who came up with the result
Starting point is 00:13:51 who was in denial of it confirming biblical genesis that's all oh wow look at and and he was catholic that's not that's kind of rough when your own people are just like you know nah that's it's kind of like you appoint like you appoint a special counsel and he goes, yeah, there was no fraud in this election. And you go, yeah, you're fired. So anyhow, so in that scenario, until you have data to show which version of these, what variant on this equation is operating, you could have a cycling universe. And this is how old I am. When I was in graduate school,
Starting point is 00:14:30 we explored all of these solutions to the equation. But we know now from data that we're on a one-way trip. The universe will never re-collapse. So, no, we're not going to have a collapsing universe. And the birth of the universe, could it have been a universe before that that collapsed and then birthed us again? We don't know. Okay. It would be hard to have a collapsing system expand and then never re-collapse.
Starting point is 00:14:58 You see what I'm saying? So, because whatever made it collapse should make it collapse again. And there's nothing out there that's going to make that happen. So. Interesting. There you go. There you go. All right.
Starting point is 00:15:10 Hey, nice question, man. Way to go. Hi, I'm Chris Cohen from Hallward, New Jersey, and I support StarTalk on Patreon. Please enjoy this episode of StarTalk Radio with your and my favorite personal astrophysicist, Neil deGrasse Tyson. So this is Gaud Paraginidoni. I'm from San Jose, California. My question regarding shyness of dark matter when interacting with other matter. If we think dark matter as a giant spider web that holds the Earth and the Sun and the gravity,
Starting point is 00:15:54 why does it interact with dark matter that holds the Earth and the Moon together? Or the dark matter that holds our solar system and the Milky Way and the galaxy? With normal matter, these three spider webs would scrape and break each other. Dark matter is pretty outgoing all over the place, holding galaxies together and whatnot. But when it comes to interacting with other dark matter, why is it so bashful? Is it because it's afraid of rejection? Or maybe it's just not interested in a three-way or whatever reason? I'm just curious.
Starting point is 00:16:24 Please let me know. You know, I think he was trying to do a bit at the end there. Maybe it's just not interested in a three-way or whatever reason. I'm just curious. Please let me know. You know, I think he was trying to do a bit at the end there. I'm pretty sure he was trying to get a little bit at the end, you know. But I read it anyway just to satisfy you. You got your little comedy bit in there, gal. But, yeah. Is there different dark matter that's doing different things? Yeah, so dark matter
Starting point is 00:16:45 is not holding Earth together. The molecular forces are, the electromagnetic attraction forces are. Dark matter is not holding the solar system together. All the objects there is sufficient gravity to make that happen.
Starting point is 00:16:58 But dark matter is holding together the galaxy. And it's holding together galaxy clusters. So it turns out, other than through gravity we don't interact with dark matter so you could just walk through dark matter you wouldn't know it and it wouldn't know it more more more accurately said you wouldn't know it and it wouldn't care okay so now not only do you not interact with dark matter, dark matter does not interact with itself.
Starting point is 00:17:29 Because if it did, you would have concentrations of dark matter. Just think about it. If you have two hot marshmallows and they meet at night, okay, over the fire, what will they do? Well, they'll get it on because they're both hot. So, I mean, that sounds like a recipe for marshmallow love if I ever heard it. Two hot marshmallows
Starting point is 00:17:52 coming together? That was not my intent for you to take it down that path. Two hot marshmallows, they'll stick. They'll stick to each other. So there are forces within the marshmallow, material forces, that when it sees other marshmallows, that they'll stick. Okay?
Starting point is 00:18:07 Right. So we, our matter knows how to do this. All right? That's how you get planets. That's how you get stars. Right. Dark matter does not stick to us. So it's not with the marshmallow or with the planet or with the star.
Starting point is 00:18:23 And it doesn't stick to itself. So dark matter does not make concentrations. So as far as we know and understand the behavior of dark matter, you don't expect to see dark matter planets or dark matter galaxies. Dark matter is the Unabomber. It's just lone. It's a lone wolf. It's lone.
Starting point is 00:18:43 It's out there by itself. By itself. And it does not care. Okay. There it is. Unabomber, that's a lone wolf. It's lone. It's out there by itself. By itself. And it does not care. Okay. There it is. Unabomber, that's a stretch, I think. But okay. Yeah, you know, it was kind of a hermit, right?
Starting point is 00:18:52 He didn't care about anybody. I mean, listen. There's a morbid stretch, I might add. It was a morbid stretch. But anyhow, so yeah. It's just the fun, the interesting part is that it doesn't even interact with itself physically, only through the force of gravity. Nice. So watch.
Starting point is 00:19:10 All right. So watch. You have a forming solar system, and two bits of matter know this, and they fall towards each other and stick. All right? Right. Now watch. Right. You have bits of dark matter, all right, and they fall towards each other, and they pass through each other.
Starting point is 00:19:27 Pass through each other. And they'll just rock. There it is. Very rude. Right. Very rude. Very. There you have it.
Starting point is 00:19:35 Yeah. Oh, very cool. That's a great question, man. We're getting through these, Chuck. We're getting through them. People have made note that sometimes we take and luxuriate in our question answers. No, we're making progress here.
Starting point is 00:19:52 Yep. So this is Bob Dan. And Bob Dan says this. Hi, this is Bob. It's from the US of A. If space in the universe is expanding, then why aren't we being stretched thin and ripped apart atom by atom? And what am I missing here?
Starting point is 00:20:06 I mean, wouldn't the expansion apply at every level right down to the subatomic? And how is this current expansion different from the so-called big rip you talk about? And here's what I want to know, Bob Dan. Why do you have such a damn attitude? You gave me attitude. I'm just reading the way it's ready no you you are imbuing this boy's question with attitude okay i mean it's just i don't know the way it sounds i could have read it maybe please
Starting point is 00:20:40 peacefully and calmly i'm sure okay okay yeah. So, the expansion of the universe, depending on the rate and where it's happening, it will not overcome the gravitational forces and the electromagnetic forces that are otherwise binding solar systems and objects together. The expansion of the universe has to be way stronger before that happens. So in other words, yes, you're stretching space, but I'm holding on to myself within the stretching space until the force of the expressing space exceeds that of my gravity
Starting point is 00:21:18 or exceeds that of the electromagnetic force. Then it'll pull you apart. So the fundamental forces of the universe right now are greater than the ripping forces that are upon it. Correct. So you got it. So the gravity, if you got a tight gravity system, you're not pulling that apart with your expanding universe yet.
Starting point is 00:21:37 Cool. Very cool. Well, I'm sorry for giving you so much attitude. I read the question. It's a good question, man. What sentence had the most attitude there? Read it to me. Okay, okay.
Starting point is 00:21:49 And how is this current expansion different from the so-called big rip? Okay, so I would read that. Oh, and how is this current expansion different from the so-called big rip? See? See, that's why you're an astrophysicist and I have problems with my phone carrier. All right, next question. What do you have? I'm just saying,
Starting point is 00:22:17 I get on the phone with them and they're just like, sir, you cannot talk to me that way and I will not have you talk to me. Click, right. They can hang up on your ass. They can hang up on you now. If you use profanity, they'll just hang up. They can hang up on your ass. They can hang up on you now. If you use profanity,
Starting point is 00:22:25 they'll just hang up. They can hang up on you now and it's totally fine. I don't have to use profanity. The only question is if it's AI and you have the cover, will the AI hang up on you? Or will it crush you back?
Starting point is 00:22:36 And that's what I'll say from now on. I was just trying to figure out if you were AI. Don't hang up. Don't hang up. Just wanted to make sure you weren't AI.
Starting point is 00:22:49 Anyway, this is Michael Rivera. Michael Rivera says, hello, Dr. Tyson and Lord Nice. Michael here from Las Vegas. My question is, would it be possible for humans to artificially create a black hole with significant mass in order to further study the mysteries of how black holes work and what they do? If so, how dangerous would this be, this artificial black hole made here on Earth at a sustainable size? And would there be any way of containing it? This guy, Michael, I have a feeling is trying to make a black hole in his basement or something. These basement people, I worry about them. See, I grew up in an apartment. We don't have any basement projects.
Starting point is 00:23:26 You know? It's hidden from the parents. That's funny. Neil, don't make me come in here. I feel like I hear a black hole being built. What's going on? What would that sound like?
Starting point is 00:23:40 So, yeah, you wouldn't know how to contain a black hole. It's like, Chuck, pass me that black hole. Chuck, where'd you go? That's funny. Chuck?
Starting point is 00:23:52 No. Oh, that's funny. So, yeah, we don't know how to manipulate a black hole. And so maybe someday we could like bunch up space time and make a little container out of, I don't know. I don't know. So yeah, this would be a really bad idea because a black hole is a voracious eater. So let's say you had a black hole on your desk and it fell to the floor, it would start eating Earth. And it would just fall through Earth, eating anything that,
Starting point is 00:24:30 any part of Earth that was near it. And it would continue to do this until the entire Earth was inside the black hole. You know how big an Earth-mass black hole is? No. About the size of a plum. Oh, wow. That's crazy. Yeah, that's a sad day for Earth. That's a sad day.
Starting point is 00:24:46 So, yeah, so your black hole eating Earth would become the size of a plum. Wow. That's the entire Earth fitting inside the black hole. That's the entire Earth inside the black hole, right? Yeah. Look at that. Oh, man, that's so cool. Yeah, it's scary, too.
Starting point is 00:25:01 All of Earth crunched down into something smaller than the size of my fist. Yeah. It's very difficult to really conceive when you think about it. Yeah, because you're limited to your five biological senses. And the universe is, repeat with me, under no obligation to make sense to you.
Starting point is 00:25:20 There you go. And guess what? It does a very good job of that. Okay. There you go. And guess what? It does a very good job of that. It's winning that battle as far as I'm concerned. All right, this is Captain James Riley. We got a lot of his questions. Captain Riley. Captain Riley.
Starting point is 00:25:40 Yeah. He says, why do galaxies form a web or a sponge-shaped structure? It seems that on small scales, gravity forms spheres and disks. So I'm a little confused. Oh, good question. Right. The large-scale structure of the universe is not with galaxies equally spread. It's not with galaxies all in tidy spheres, although some galaxy clusters are. For example, the Coma Cluster of galaxies. This is a cluster of galaxies that lines up with the stars in the constellation called Coma, okay?
Starting point is 00:26:17 A Coma Bernice, so it's the hair of Bernice, okay? So if you look at constellation maps from like centuries ago when they used to draw this stuff, it's just somebody's hair. Okay. So if you look at on constellation maps from like centuries ago, when they used to draw this stuff, it's just somebody's hair. Right. Not to be confused with the comb over galaxy. Commonly, commonly seen in boardrooms around America.
Starting point is 00:26:38 Comb over. Comb over galaxy. Okay. So the coma cluster, that's a nicely spherical cluster of galaxies. And in fact, that's the first galaxy cluster where dark matter was discovered. Because you looked at all the speeds of the...
Starting point is 00:26:55 And there's a certain amount of mass, gravity required to keep all of them in this ball. Whole galaxies now. Thousands of galaxies. I think like maybe 800. I forgot the exact number, but it's around a thousand galaxies and many, many hundreds. And so you calculate that up and you find out that it needs like 10 times that much mass
Starting point is 00:27:18 to keep the galaxies contained. If you add up the mass of every galaxy, it doesn't add up to the gravity needed to contain them. So that was a guy named Fritz Zwicky in the 1930s, 1936, I think it was, where he's a Caltech, Swiss-born Caltech astrophysicist
Starting point is 00:27:36 who discovered this. And it's the longest unsolved problem in modern astrophysics, the dark matter problem, birthed with his observations. Anyhow, there are some galaxy clusters that are nice, spherically shaped. Others, you see
Starting point is 00:27:52 these filaments. It's as though you had a sponge and you cut it, and you looked at the cross-section where there's some concentrations of sponge, but mostly there are these sort of bridges between concentrations. That's what the universe looks like.
Starting point is 00:28:08 The inside cross-section of a sponge. Here's the problem. If you look at how fast the galaxy is moving along one filament, and look at the size of the filament, the universe is not old enough for the galaxy to have crossed that filament. Ooh. So you don't have structures that represent what the galaxies really want to do if they had enough time. Right. So that's what's going on here.
Starting point is 00:28:39 Interesting. Right? So you have systems that are not gravitationally settled in what they should look. The coma cluster is, and it's a term we use for this. I forgot it. What is it? It's a relaxed cluster. It's one where, okay, we got this.
Starting point is 00:28:58 Everybody's orbiting just the way they should. Take a chill, baby. It's chill. Exactly. And they could cross the size of the cluster in the time the universe has been around so that how you know everybody's everybody's settled into their routines any structure is bigger than that they've not had time to settle and so and they may never settle given how long it takes and given how fast the galaxies are moving through space. So, yeah.
Starting point is 00:29:26 That's how and why we get that. Wow. Very cool. Yeah. This is Lou Perrault. Lou Perrault says this. Perrault, is that a final T or are you... A-U-L-T.
Starting point is 00:29:51 Oh, Perrault. Okay. Perrault. Okay, Lou Perrault. He says, hi, Neil Hatchuk. My name is Lou and I'm writing from the Seven Islands. Septiles. He says...
Starting point is 00:30:03 Where are those islands? In Quebec. Quebec. Quebec has islands? Thatiles. He says... Where are those islands? In Quebec. Quebec has islands? That's what I'm... Hey, listen. Isn't Quebec inland? I thought it was. You know?
Starting point is 00:30:12 Okay. But we're Americans, so we don't know. Yeah, what do we know about the French-speaking province of Canada? We're not... We're bad. We're the worst in the world in geography. With geography, that's for sure. We don't know our own damn states. Well, geography, that's for sure. We don't own damn states.
Starting point is 00:30:26 Well, some of them we don't want to know. Let's be honest. Let's, come on. I know we're 50 states, but we kind of should be about 40. Okay, let's come on. Seriously?
Starting point is 00:30:42 All right. He says... Come on, seriously? All right. He says... All right. He says... That's cool, Chuck. That's cool.
Starting point is 00:30:51 I know. I know. He goes, my question is, is it possible to see past by looking in the... See the past by looking into deep space? And if so,
Starting point is 00:31:04 which direction do we have to look? And also, is it possible to see the Earth by sending a telescope multiple light years away? Yeah, so only if you can travel faster than light can you see your own past. So you can't do that. But so I know what he's saying, but I wanted to lead up to that.
Starting point is 00:31:24 So clearly he knows that the farther out you look the farther back in time you see okay right so there are galaxies that are like 65 million light years away from earth okay from our galaxy so right now if they had a super duper telescope and they look towards Earth, what do they see? If they're seeing us however many light years ago. 65 million years ago. What are they witnessing? Dinosaurs, right?
Starting point is 00:31:57 Oh, and they're getting killed. Yeah. It just dawned on me what that time frame was. I'm like, oh, snap. I know. The Earth is putting on a show for them. Yeah, so the galaxy that's 65 million light years away is witnessing the extinction of the dinosaurs
Starting point is 00:32:15 because that light is only now just reaching them. Okay? Right. But we can't see our own past. That doesn't work. So, yeah. But if you send a telescope out there, you know, let's say a thousand light years away, and then come back, it will be seeing whatever happened here a thousand years ago.
Starting point is 00:32:40 Right. Right. So it's that simple. So, yeah, that's it. And then what you'd have to be, like you say, is faster than the speed of light so that you could go place it and come back and have it and be like, yo, what's up?
Starting point is 00:32:53 Yo, what's up? It's me. Yeah. But once you go faster than the speed of light, then all bets are off. And then you can do all kinds of paradox-y things. Paradoxical things. Yeah, cool. Alright, this is Connor
Starting point is 00:33:09 Holm. He says, Hi, if the big rip does occur. A lot of big rip questions today. People got it on their mind, man. Because no one wants to be torn asunder by the universe itself. No one wants to get
Starting point is 00:33:25 No one wants a new one torn into them. Okay. Yes. I'm the universe, boy. I will tear you a new one. That's what I will do. You keep on. You say another word. Say another word. I'll tear you. That's what I
Starting point is 00:33:44 I'm the universe. You know who you're talking to? I will tear you in half. Okay. What is he asking? Connor says, if the big rip does occur, what would be the immediate results of tearing of the fabric of space-time? fabric of space-time? Would these tears, tears be black holes or would they simply just be voids of nothingness? What is nothing? How could nothing come out of something? What would these voids be? Wow. That's freaking crazy. I love this, Connor. Okay. So my simple answer is we have no idea.
Starting point is 00:34:31 Okay. The state of the universe post Big Rip is a complete mystery. And what we don't know is there's some law of physics that will manifest at that time. Think about that. You know, when do we discover new laws of physics? When we step where we had never previously stepped. When we look where we never previously looked. When we bring a new kind of apparatus, a new kind of detector that we never had before. Then we see the universe behaving in ways we've never seen before. Then we see the universe behaving in ways we've never seen before. Sends us back to the drawing board to say, is this understandable with previously known physics?
Starting point is 00:35:12 Or do we have to invent new physics? So Einstein said to himself, I don't think we'll ever have a black hole, even though his own damn equations predicted it. Because a black hole in his equations have infinite density occupying zero volume in the center of the black hole. And he said, surely there's some new law of physics that's going to show up and save us from ourselves, save us from this mathematical craziness where God divides by zero, right? So what happens in the big rip? What would it look like? We do not know. And I'd like to know before that day happens so that we can protect ourselves, if that's possible at all. We don't know. And he's wondering if it rips, does nothing show up?
Starting point is 00:35:59 Okay? Something we call nothing. Something we call nothing. Okay, but then what is nothing? What is? Okay. I think we have a whole explainer on nothing. Something we call nothing. Okay, but then what is nothing? What is? Okay, I think we have a whole explainer on nothing. We did do an explainer on that. Okay, let me tap some of that.
Starting point is 00:36:11 And what we got out of that was there is no nothing. Because, you know, is air nothing? Well, you can see through it, but we know there's air there, right? So clearly it's not nothing. So now take away the air. So what's left? Is that nothing? Well, it's still space.
Starting point is 00:36:33 Well, it's empty space, nothing. And we know from quantum physics that empty space is a seething soup of what we call virtual particles popping in and out of existence. And so, and this is what we call the vacuum energy. Just Google that, vacuum energy. There's an energy in the vacuum of space that quantum physics puts there. And we thought, hey, that could be the dark energy in the vacuum of space. So you do the calculation, how much dark energy we measure, then you do the calculation for how much pressure is coming in from these virtual particles popping
Starting point is 00:37:16 in and out of existence, and we are off by 100 orders of magnitude. It is the biggest mismatch between an observation and a theory that has ever occurred. This is further evidence that we have no clue what dark energy is. Okay. Wow. So, there it is. Now, could we imagine a place where there's not even these virtual particles? Okay, but then you can't have quantum physics. So, all right.
Starting point is 00:37:51 So, now we have a place where there's not only not nothing, there's not even the laws of physics. Right. Whoa. So could you exist in that nothing? Because you only exist because they're like molecules hold you together and, you know, and light and energy and electro. You only exist because the laws of physics allow you to.
Starting point is 00:38:26 Right. So the best nothing, if the rip gets you there, if you step through that rip, maybe that nothing does not even contain the fabric of empty space. Look at that. Because the laws of physics tell us what the fabric of empty space does. So if you take away not only the empty space, but the laws of physics that would describe it,
Starting point is 00:38:53 then that's as good a nothing as I can imagine. Right. And that nothing exists inside of a bomb. I've been there. I've been there. I've been there. I've been there. Tell you. The bong nothing.
Starting point is 00:39:14 Okay. It's the bong nothing. It's a nothing bong. Okay. So, Chuck, we have a couple minutes left. I think I'm going to allow you to give me one question even though you you you're you're a cheap ass comedian not paying your patreon dues all right okay all
Starting point is 00:39:34 right well you know uh i'm gonna i'm gonna make it uh okay so uh i was watching this thing on listening to NPR and they were doing this thing about energy and all the different forms of energy. And then they, for some reason, played a clip from what I know is one of your and my favorite movies, The Matrix. And they played the clip about how the AI basically, after a singularity, saw us as a form of energy to be used as little batteries. So my question to you is, do we put out enough energy that if something were an AI would say, you know what?
Starting point is 00:40:27 I need to put them to work. And line us up head to toe. That's right. So that we would become little batteries as opposed to just taking us and literally putting us to work by subjugating us all and making us do their will. Right, right, right, right, right. Yeah, I'm just trying to think, if they put you and me in a battery socket, I say, no, Chuck, we got to be head to toe, right? Exactly.
Starting point is 00:40:56 You see the AI keep coming around and flipping us over. Put it in the wrong way. Now, doesn't this go on the spring side? The feet go on the spring side, right? That's what the wrong way. Now, doesn't this go on the spring side? Does the feet go on the spring side? That's what AI sounds like. That's an exasperated AI. Exactly. That's my AI that sounds like Chris Tucker.
Starting point is 00:41:17 Say, man, does the feet go on the spring side? Okay, anyway. All right, so this energy described in the matrix is drawn from the human body. So, you can look at our metabolism, all right? If you're a calorie counter, you'll know that there's something called your basal metabolism. So, this is the energy you burn, pay or play, okay? Just for existing. Just for existing.
Starting point is 00:41:44 Right. And for some people, it's maybe 1,500 calories a day. For me, it's more like I'm bigger. So for average, I'm a little bigger than average. So like 2,000 calories a day is my basal average. Okay. So now, do you realize that the food calorie is written with a capital C? You may not have noticed that.
Starting point is 00:42:09 There's a reason for that. Because a physics calorie is written with a lowercase c. Because a food calorie, one food calorie, equals a thousand physics calories. So when I say I burn 2,000 calories a day, it's 2,000 physics calories. Ah, okay. So when I say I burn 2,000 calories a day, it's 2,000 food calories. It's 2 million physics calories. And what is a physics calorie? It's the amount of energy required
Starting point is 00:42:35 to raise the temperature of one cubic centimeter of water one degree Celsius. Interesting. That is one calorie. That's one calorie. Okay? All right. So, once you have all these calories, it's a rate at which you're burning energy.
Starting point is 00:42:55 We have a unit of measure for that. It's called watts. Okay? Watts. Mm-hmm. watts. And so, when you do the math on this, the average person is operating anywhere between 50 and 100 watts.
Starting point is 00:43:15 Okay? So, it's like a light bulb, you know, like an 80-watt light bulb, okay? The 80-watt light bulb consumes energy at a rate, so do we we we radiate that okay well we consume that much energy our circulation and everything else so what the what the what the machines did the computers did in the matrix is line us all up and draw the 80 watts of power
Starting point is 00:43:42 from every person at all times. Okay. That's very inefficient. So the answer is yes, that's how they did the movie. However, it's extremely inefficient. Yeah. You know why? Because I don't want to power a city off a light bulb. No, no.
Starting point is 00:44:01 No, if you get enough of us. I use a light bulb as an example of something that uses that much. I know, I know. Here's why it's inefficient. Okay? You're burning 2,000 calories a day as long as what is
Starting point is 00:44:17 happening? As long as I'm living and breathing. No. Well, yes, but more fundamental than that, well, equally as fundamental as that, how long can you keep burning 2,000 calories a day? I thought you said that was my base. Yes, that's your base.
Starting point is 00:44:38 I got to be eating something to... Thank you. Yeah. Thank you. Where do you think that... I got to eat something to burn. Where do you think those calories came from? From the food you? Yeah. Thank you? Right. Where do you think that? I got to eat something to burn. Where do you think those calories came from? From the food you're eating.
Starting point is 00:44:47 So in order for all of the matrix people, the people in the pods, to be feeding 80 watts of power to the matrix, the matrix has to feed them. That's a lot of, that's 8 billion mouths. Okay, so what I'm saying is, if the Matrix is feeding you 2,000 calories a day, so that it can then pull your 80 watts off of you, why use the middleman? Right. Just burn the food calories that you're feeding the people. In fact, every time energy changes from one form to another,
Starting point is 00:45:26 it's not 100% efficient. You lose some energy to heat all the time. So you look at the energy in a gallon of gasoline, okay? And that gets burned to drive the car. I forgot the number, 80% of that energy goes into heat. It does not go into moving your car forward. That's funny. Okay? So this is a fundamental feature of thermodynamics in the universe. So they were being inefficient.
Starting point is 00:45:57 So this is their weak point in their storytelling. And I will give them a hall pass because they did everything else so brilliantly. But that one was just plain stupid because the machines, the computers, just would have used the food that they're feeding them and get their energy off of that
Starting point is 00:46:16 and leave the people out of it. Look at that. But then they wouldn't have had a movie. Well, you know, that's a problem. Yeah, that makes things difficult yeah yeah all right yeah cool all right that that's all the time we have chuck okay all right so this was cosmic cosmological curiosity cosmic queries cosmological curiosities i got it i got the tongue twister.
Starting point is 00:46:46 All right, Chuck, always good to have you here. Always a pleasure. All right, this has been StarTalk Cosmic Queries, Cosmology Edition. Neil deGrasse Tyson here. As always, keep looking up.

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