StarTalk Radio - Cosmic Queries – Science to Know

Episode Date: June 8, 2020

Neil deGrasse Tyson and comic co-host Chuck Nice answer fan-submitted Cosmic Queries on a variety of topics including life on Mars, the expansion of the universe, building wormholes, and more to mark ...hitting one million subscribers on YouTube. NOTE: StarTalk+ Patrons and All-Access subscribers can watch or listen to this entire episode commercial-free here: https://www.startalkradio.net/show/cosmic-queries-science-to-know/ Thanks to our Patrons Chris Goshorn, Russell Konicki, Pat Simmons, Trinity Goodwill, Chris Davis, Mike Jordan, Michelle Danic, and Sylvia Mangold for supporting us this week. Image Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), A. Nota (ESA/STScI) and the Westerlund 2 Science Team. 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 Welcome to StarTalk, your place in the universe where science and pop culture collide. StarTalk begins right now. This is StarTalk. I'm your host, Neil deGrasse Tyson, your personal astrophysicist. And I got with me, as always, Chuck. Nice, Chuck. Hey, Neil. So we are live.
Starting point is 00:00:29 Live. Oh, my God. What does that mean? It means I get to hold up a newspaper and it will have today's date on it. You still read newspapers? What is that? Your news comes to you in paper? Wait a minute.
Starting point is 00:00:42 It means I get to hold up my tablet. So anyway, why are we doing this? YouTube Live. First, I just want to say thank you to our Patreon members. These are people who basically actively subscribe to us by giving us money each month. This is a higher level of participation. And we do things for them, exclusive things for them.
Starting point is 00:01:09 Like they get their own cosmic queries, for example. And there are other things. There's like a scale, depending on how much you put in, and becomes a fundamental buoyant force in what we do to bring this show to you. And also, I think some people don't know that we have this sort of topical spinoff of StarTalk called StarTalk Sports Edition. That's right.
Starting point is 00:01:32 And you're my co-host with Gary O'Reilly. That's right. Who's a former footballer. Footballer. Translate that, Chuck. That's a professional soccer player across the Great Pond. He played for Crystal Palace and Tottenham Hotspur. Okay, very good.
Starting point is 00:01:51 And so we realized that there's a lot of science in sports and a lot of actual athletes and coaches and trainers and all of what goes on in sports is such a big part of modern life, social life, really, that we felt it deserved its own sort of path within the StarTalk universe. So StarTalk Sports Edition is there. So you can check that out. But anyway, I want to open this. Can I open this now?
Starting point is 00:02:18 Please. Let us see. Here we go. Oh, so here's what happens. So if you have a YouTube channel, as we do, StarTalk channel, when you hit these milestones, these are milestones in base 10, okay? Okay. So 10 to a power of some number.
Starting point is 00:02:38 So if you hit 10,000, 100,000, and we recently hit a million. Looks heavy. Ooh. Oh, that's really pretty. Yeah. So I'll read it to you. It says, presented to StarTalk
Starting point is 00:02:56 for passing one million subscribers. Oh, that's very cool, though. Yeah, so we'll find a place to hang this. And so next target, I guess, would be 10 million. 10 million, there you go. Maybe. The power of the 10.
Starting point is 00:03:09 So anyhow, we're going to do what we do best and take some questions from the audience. Some have already rolled in, and then we can take some live, since this is live. I might as well. And you've got it all. I haven't seen any of them, Chuck. Yeah, yeah.
Starting point is 00:03:22 And it's funny. I love it because I lifted them right off of the YouTube site, as you can see. And they say like 18 hours ago, 12 hours ago. It's kind of cool. Yeah, yeah, yeah. When they arrived, yes. Yeah, right from when they arrived. So this is SnackDealer1.
Starting point is 00:03:41 He says, if a separate human colony was well-established on Mars, what would likely be the most valuable resource Mars could trade with Earth? Ooh, so kind of reminiscent of a television series called The Expanse, except it's not Mars. The humans that move to Mars become far more advanced because they're all like real science-y minded. And then the ones left on Earth are just like, you know, Trump supporters.
Starting point is 00:04:13 No, I'm joking. I'm joking. That was a joke. The ones left on Earth, you know, they continued on in the path that we Earthlings could have, the trajectory that we're on uh but then there's a separate group of earthlings that go out to the kuiper belt and they're miners and so they're they're actually bringing all the good stuff out of these mining these asteroids and it's funny because the the three of them together have like commerce and so when
Starting point is 00:04:47 he says this i immediately thought of that if we were if there was a mars earth 2 how interesting would it be would mars have something to give to us okay so first of all the capra belt has mostly icy objects icy bodies and which is much less used to us than heavy metals. And the Asteroid Belt is way closer than the Kuiper Belt. Oh, I'm sorry. It is the Asteroid Belt. I'm sorry. I said Kuiper Belt.
Starting point is 00:05:16 I meant to say Asteroid Belt. Fine. Don't get me started. That's my fault. More often in your situation. Don't blame the writers of The Expanse on that. Okay. That was me.
Starting point is 00:05:26 That was my slip up in words. They're not in the Kuiper Belt. They're in the asteroid belt, hence the mining operations because they're grabbing these large, craggy, floating boulders and drilling down into them and pulling out all kinds of good stuff. Okay. So here's the thing. We don't yet know the full depth profile of Mars and what it contains and what's there. There's probably not oil deposits, I'm guessing. Oil on Earth comes
Starting point is 00:05:52 from dead vegetation from millions of years ago. So, no. But that's what discovery is all about, right? But who knew that Earth had oil that you could pull out of the ground and build civilization on it and then have to get rid of it later, right? You just don't know. You just don't. That's a whole point of exploration. So Mars, it would be interesting. What I can imagine is you can have inventive people there that use the natural resources that are common on the surface of Mars and do something inventive with that and then trade that.
Starting point is 00:06:30 And that way, so it wouldn't have to be only something that Mars has. It could be that Mars has the intellectual capital, that is the people who went to Mars, are of a particular variety of people who have certain inventive ways that then create a resource that other people want. Look at Switzerland, okay? Switzerland's in the mountains, all right? It's like, what do they have? So they took their natural resource and made stuff.
Starting point is 00:06:58 They pioneered chocolate and clocks and the Swiss Army knife. The top three. No, just they made precision timekeeping an art. And so the Swiss watch wasn't just a sales tag. It was a real thing. And you don't mine watches out of the mountains. This is an expertise that your culture brings that you then put into commerce.
Starting point is 00:07:28 So I can imagine if we are a multi-planet species, that not everybody's going to be building the same stuff. And so whether or not there's a natural resource that you would trade as natural ore, which surely would still happen, it could be that you got people who like making one thing versus another and you need it on another planet. So then you'd have this interplanetary commerce, which would be great. I look forward to that.
Starting point is 00:07:52 Very cool. And by the way, asteroids, like you incorrectly had remembered, asteroids from the asteroid belt, if you get a metallic asteroid, that is a concentration of all the heavy elements that we've cared about in our civilization. Cadmium, platinum, gold, what else?
Starting point is 00:08:08 Just name all the rare earth elements. Yttrium. All of these are in high supply in these asteroids. gets to lasso the asteroids best, then their commerce is not only what they do on their planet, but their ability to exploit the resources of wandering objects within space itself. So, yeah,
Starting point is 00:08:35 that's the future of, what did they call it before they invented capitalism? A mercantilism. Interplanetary mercantilism. That's what that is. Very nice. Oh, yeah. Very nice. I love that word. mercantilism. Interplanetary mercantilism. That's what that is. Very nice. Oh, yeah. Very nice. I love that word, mercantilism. Mm-hmm.
Starting point is 00:08:47 Mm-hmm. All right. That's what made Venice and Amsterdam and all. The mercantiles. In the day, the mercantiles. Yeah. Merchant of Venice. Merchant of Venice. They didn't say capitalist of Venice.
Starting point is 00:08:58 They said merchant of Venice. Right. That's right. Cool. Shakespeare's play, of course. All right. All right. What else you got?
Starting point is 00:09:04 Okay. This is Kevin. By the way, of course. All right. All right. What else you got? Okay. This is Kevin. By the way, wait. Were these focused into any theme or is it just any question about anything? Well, I don't see a theme. Okay. Okay. All right.
Starting point is 00:09:16 Okay. So here's what I'll do. And we discussed this on another episode where it's not that I know the answer to everything, but I know some things about a lot of things. So if you ask me a question I can't answer, I might give you something to know about that that might still not answer your question, but gives you still something to walk away with. All right. So we'll call this one Cosmic Queries, something to know.
Starting point is 00:09:38 Okay. Let's do it. There you go. Kevin Vivale says this. Is it Devayi? Is it two L's and an E? No, no. It's not a Yardro type deal.
Starting point is 00:09:50 All right. Those for whom this is their first Cosmic Queries, Chuck don't know how to pronounce anybody's name. No, I do not. I do not know how to pronounce anyone's name. And by the way, when I mispronounce your name, the great thing is you now have a new name. You can hide from the government. Chuck will baptize you with a new name. That's right. I'm giving you a new name. This is the beauty of being on StarTalk. All right. So Kevin wants to know this. Why is our galaxy in the shape of a spiral?
Starting point is 00:10:28 And why do other galaxies have other shapes? What determines the shape of a galaxy? Most galaxies in the universe are spiral galaxies. So we're in the club, okay? We are not rare in this, first of all. Second, so the two main things, that's a great question, by the way, an observant question, all right, because some galaxies are kind of elliptically shaped and others are sort of spiral, flat spirals. So we call the elliptically shaped galaxies elliptical galaxies.
Starting point is 00:10:55 And we call the spiral shaped galaxies spiral galaxies, all right, because that's how we roll as astrophysicists. Astrophysicists are too busy doing math to come up with inventive names for stuff. We just call it. They just call it what it is. Oh, look at that. It's the Sagara galaxy. That's what it is.
Starting point is 00:11:16 Oh, my goodness. Region of space, you fall in, you don't come out. Black hole, okay? Light doesn't come. Black origin of space time big bang right we are we we fully embrace one syllable communication with each other okay it's about a economy of words jupiter has a a big red spot on its surface right you know we call it? What? Jupiter's red spot. There you go.
Starting point is 00:11:46 Wait, wait, wait. That's not the only spot, right? The sun has spots. And we call them? Sun spots. Sun spots. Okay? There you go.
Starting point is 00:11:55 Yeah. Okay. Look at that. And now back to this equation. What should we call this? Neil, what should we call this? It's spots on the sun. Call it sun spots, man. Back to this? It's spots on the sun. Call it sunspots, man.
Starting point is 00:12:05 Back to this equation. Back to this equation. So what determines the shape of a galaxy? Okay, so watch. So you have this huge gas cloud, and it begins to collapse. All right? And because gravity, that's the natural thing gravity wants to do. I'm talking about a gas cloud larger than a galaxy that will become a galaxy.
Starting point is 00:12:29 All right? If the galaxy has any kind of extra spin to it, as it collapses, it spins faster. Okay? You've seen this on ice. We're ice skaters. Right? If they're spinning at all, if they bring in their hands, they end up spinning faster. Right.
Starting point is 00:12:46 There's a basic feature of physics. It's called the conservation of angular momentum. But that's what happens. If you shrink down, you spin faster. If I weren't in a chair, I would do it physically. The next time we'd have StarTalk Live, I'll do it StarTalk Live. In fact, we did it in one of the StarTalk Live. We had an ice skater on one of our guests.
Starting point is 00:13:07 Sasha Cohen. That's Sasha Cohen, yes. Exactly. Thanks for remembering that. Yeah. But anyhow. Go ahead. So if you're one of these higher spinning, faster spinning, as it begins to shrink, it spins faster and faster.
Starting point is 00:13:21 And as it spins faster, that part of the galaxy has a harder time making it into the middle whereas the top and bottom just falls in so you get a nice big bulge in the middle but the rest flattens to make this disc okay it's what happens when you spin pizza dough it flattens okay and so if if you took Pillsbury Doughboy and started spinning him, he'd flatten, okay? Wow. This is hazardous activity for...
Starting point is 00:13:53 Exactly. If you are not a solid shape. And if you throw some chocolate chips on him and put them in the oven... That's worse. So these galaxies have a lot of gas in them, and it's gas out of which you make stars okay stars are gas and so you have all this gas and here's what happens we think that there is a shock wave within the rotating system that compresses the gas.
Starting point is 00:14:25 And where that gas compresses, you make extra stars. So the spiral structure of a galaxy is where extra new stars are being made. And so it's the stellar nurseries that trace the spiral pattern. There's still stars everywhere else. All right, if you look carefully at spiral galaxies, there's stars everywhere. But along these spiral edges, that's where you get very high mass,
Starting point is 00:14:51 high star formation activity. And galaxies that don't rotate much at all, they don't flatten out. And they forever stay as these spherical elliptical shapes. And they're not making many stars today. these spherical elliptical shapes. And they're not making many stars today. You're not going to find exploding stars there, which is the sign of newly formed stars that have high mass that become supernova and black holes and all the cool stuff. So we live in a really cool galaxy because we have a lot of stuff going on. Nice.
Starting point is 00:15:19 So were you first asking Patreon questions? No, I was not. Okay. So in a normal Cosmic Queries, the first section is occupied by Patreon questions. Plus, like I said, they get their own exclusive poster. That's right. Yeah. Their own Cosmic Queries, a command performance where you get to ask whatever you want to Neil.
Starting point is 00:15:46 And that happens once a month if you are a Patreon patron. So go to patreon.com slash startalkradio and support us right now. And then if you're $10 and above, then, you know, we can do this privately for you. Just for you. Yeah. Yeah. Yeah. Welcome back to StarTalk. We're in the middle of a live Cosmic Queries.
Starting point is 00:16:28 Let's jump right back in. All right, here we go. This is, why don't we take a live question, all right? Wait, and just to be clear, you're watching, people are watching this on YouTube, right? Yes, they are. So I just want to remind people, this million plaque, million. So thank you all for having done that. And if you haven't done it yet, what's stopping you?
Starting point is 00:16:52 I'm just asking. Right. If you haven't subscribed yet, right. Right. Now's the time. Now's the time. Now's the time. If not now, when?
Starting point is 00:17:00 Right? And if not who, you. There you go. If not now, when? And if not who, you. There you go. If not now, when? If not who, you. Right. There you go. All right. Let's go to live from our YouTube chat room.
Starting point is 00:17:13 And this is Isra Gashi. Sorry, Isra, if that's not right. It is right, according to Chuck. There you go. In the Chuckiverse, it's correct. There you go. I like that. Israel says this.
Starting point is 00:17:28 If light has no mass, why is it affected by gravity? That's a brilliant question. Because, you know, gravity attracts mass, right? And so if you've got no mass, why should you care? Right. Okay. And so if you've got no mass, why should you care? Okay.
Starting point is 00:17:51 Because according to, well, so there are a couple of ways out of that one, but let me give you the cleanest. The cleanest explanation is gravity is not a force on a mass. Gravity is the distortion in the fabric of space and time caused by any concentration of mass and energy. Uh-huh. And so if you are moving through space, you are moving on a path that your speed plus the curvature of space requires of you. And so if you're a matter moving substantially less than the speed of light, you will curve in towards the object.
Starting point is 00:18:28 If you're moving the speed of light, you will follow the pure curvature of space-time itself. Wow. As distorted by the effects of any kind of concentration of mass. So we say the light bends, but if you are the light, you think you're going in a straight line. Oh, wow. So if you look along this direction, even if it curves down like that,
Starting point is 00:18:57 it'll appear to you as that thing down here is right in front of you because you are traveling the shortest distance between those two points, and it's a straight line to you. Step back, and you see the curvature in the fabric of space. So there you have it. Another way to think about it is E equals mc squared, energy and mass, and c squared is the speed of light. So energy and mass are equivalent. If you drive an electric car, let's say a Tesla, and then you fill it up, fill it up by charging the batteries, your car weighs slightly more for having charged batteries given the energy that you put into the car than it did before you put in the energy.
Starting point is 00:19:36 Okay? So that's the equals MC squared equation. So you can convert the energy of the photon into a mass and then treat it as though it had that mass and then follow the equations thenceforth. So there you have it. That's why. That's pretty wild.
Starting point is 00:19:58 Yeah. That's so cool. So that's why when you look at a black hole, you see the light around the black hole, but you're not really, that's not light from the black hole. It's light that was behind it that got curved. That got curved around. So if my head is the black hole, and the light here came up and around, and then it came out the other side, and you're over here watching it, and you saw something on the other side of the black hole, and that works in all directions around the black hole so in that famous photo of the black hole that made headlines yeah several months back what you saw is light surrounding the black hole having come around it so you see the shadow of the black hole
Starting point is 00:20:35 in a sense yeah very very cool okay that's light so that's light being affected by the the force of gravity nice oh. Oh, yeah. All right. Lucid Potato. Okay. Okay, Lucid Potato wants to know, what are your thoughts on NASA's recent remarks on the possibility of parallel universes? I'd ask a lot of questions if I could,
Starting point is 00:21:01 but this has been bugging me since i don't trust news articles oh okay so there was a an experiment conducted where they're looking for particles from space these are called cosmic rays they're called rays but they're actually high energy particles and they collide with the atmosphere and they make a stream of other particles and you can measure them and we've been doing this for like since back in the since the early 19th century. So these particles are coming through. Well, okay.
Starting point is 00:21:32 This apparatus that's measuring these particles found a particle come from the opposite direction. Okay? They didn't expect that. One interpretation is that this particle is, in fact, from another universe where time moves backwards, and you're watching this particle travel backwards through time.
Starting point is 00:22:00 Okay. So it had already passed you, but you're seeing it move backwards through the other direction. Okay? Or there was a glitch in their apparatus. I mean... There you go. There's 99 explanations you can put into this before you're compelled to have to say,
Starting point is 00:22:23 this is a parallel universe where time moves backwards and that particle happens to be detected. That's all I'm saying. So what makes headlines is the one that gets the click, that's the click bait. Okay? If it's probably something wrong with the apparatus or they made a mistake or whatever,
Starting point is 00:22:40 that doesn't get the clicks. So I think on that level, what's the person's name? What's his name? Lucid Potato. On that level, Mr. Potato, you should be skeptical of the magnitude of news headlines when they are reporting a scientific result. In almost every case, if you read the original scientific paper and look at how they couched the explanations, it will have nowhere near the hyperbole
Starting point is 00:23:12 of how the newspaper article was written. Because scientists are trained to be conservative in our estimates. Yeah, but like you said, that is not a very good news story you know uh could be a parallel universe probably a malfunctioning piece of equipment i mean i'm just there's a ranking of things you know if if you can have an extraordinary explanation for something you better have extraordinary confidence that the whole uh chain of your experiment was working.
Starting point is 00:23:49 That's all. All right, cool. I see here in the chat that... You got another one? Rishabh says this. It's a really cool question. How is the universe 92 billion light years across when the Big Bang happened only 14 billion years ago? Wow. So. Oh. Okay, so let me put some context in that 92 billion light years across. Okay? billion light years across, okay? So you cannot see 45 billion light years in one direction or the other, right? That'd be 45 billion that way, 45 billion that way. This plus this equals to get
Starting point is 00:24:36 you to 90 or 46, right? So no, you can't see that because their light has not reached you yet, see that because their light has not reached you yet. Okay? We calculate that as the current size of the universe based on the rate of expansion from the Big Bang. Okay? So what's the farthest you can see? The farthest you can see is 14 billion light years away. Okay?
Starting point is 00:25:03 That galaxy that's giving you light, well, 13, the universe is 14 billion light years away. Okay? That galaxy that's giving you light, well, 13, the universe is 14 billion years old. The first galaxy light is like a 12 billion. But for the answer to this question, that distinction doesn't matter. Put a galaxy at 12, 13 billion light years away, we are seeing that galaxy being born. Its light is now just reaching us.
Starting point is 00:25:24 Okay? All right. All right. Right now, in this instant, that galaxy is 45 billion light years away. In this instant. If you could see everything all at once, that's where that galaxy is. That's why you would say the diameter of the universe
Starting point is 00:25:40 is 92 billion light years across. So, the horizon is smaller than that. That's how you get those two numbers. Okay, all right. And, okay, that makes sense. But I think what he's also saying is if light is time, like the passage of time in order for a light year, you're talking about time as well, then how did you get so many more light years in the totality even though you're only seeing the horizon?
Starting point is 00:26:24 So what you see is not all that's out there. That's my only point. There you go. So what would be a good example of that? Let's say a turtle had a message on its back. Okay. It said, the universe just began, okay? And you put it in St. Louis and have it walk towards New York, okay?
Starting point is 00:26:49 Okay. It'll be a long while before that happens. About 45 billion years. No, no. No, no. It'll take the turtle 13 billion years to get to you. Right. Okay?
Starting point is 00:27:01 But what has happened to St. Louis that it's expanding beyond that horizon. It is something, it is, and you put in the model, the model, the expansion of the universe. Right. Puts that far beyond. And that's really where that's really what he... By the way, the model
Starting point is 00:27:20 could have been different. Right. And it could have been even farther than that. Exactly. But we have modeled the expansion of the universe, and that's where you have it. So it's not about the 14.8 billion light years. It's about the expansion of the universe. That's really
Starting point is 00:27:35 what it's about. Cool. You got it. And is that model also... Well, it's modeled just by the rate of the expansion of the universe. You see how fast it was expanding early on, and then a little later, and a little later. So you look at that expansion rate between then and now. Gotcha. Light is still doing its own thing, but what is the galaxy?
Starting point is 00:27:53 So in other words, the moment that galaxy emitted the light from 13 billion years ago, the light is en route. Right. Okay? And it is decoupled from what the rest of the universe is doing. It's a mobile post office they put the letter the letter the letter is on the way but the post office is still headed off yeah that's kind of cool exactly that's it all right there you go all right let's go to um let's go into like soundbite mode samir and r we running out we running out of time already? No, but I just want to
Starting point is 00:28:25 get back into that rhythm. All right, let's get back into rhythm. Samir says this. Congratulations. Coming to us from YouTube. Congratulations, Dr. Tyson on one million subscribers.
Starting point is 00:28:34 Hey, Chuck. When the James Webb telescope is finally in orbit and operational, what kind of discoveries will it expect to make and which discovery are you most excited for okay excellent
Starting point is 00:28:47 so a false assumption was made that it would just be in orbit like the hubble telescope this is going to be a million miles on the other side of the moon wow now it will be orbiting the earth but in a way that is out at that distance okay so it's it's not like astronauts. If something goes wrong with that telescope, ain't nobody going to fix it. Wow. Okay, it's not going to be serviced. It's not going to have hero astronauts replacing the lenses or the detectors
Starting point is 00:29:13 or the computer chips. No Bruce Willis. No. Saving us from an asteroid, I presume, is your reference there. So that telescope, here you go. You ready? Newly born galaxies, 13 billion years ago, okay, had emitted a lot of, most of the energy was high energy light emitted by these galaxies.
Starting point is 00:29:43 Mostly from the birth of brand-new high-mass stars. A lot of blue light is coming from them. However, that light has been moving through an expanding universe, and that light has redshifted. It has become lower-energy light. So it shifted from blue to go backwards through it. So it's, what is it, green and then orange and yellow, green, and then red. And then infrared.
Starting point is 00:30:16 You go through the whole spectrum. It has shifted so much that the principal light from those galaxies is now in the infrared part of the spectrum. This telescope was conceived and designed to observe red-shifted light from galaxies born at the beginning of the universe. Ooh. It is brilliant. Brilliant.
Starting point is 00:30:42 Wow, that is really brilliant. So it's almost like a little visual time machine to go back and look at the near beginnings. Because we know, you see, originally we were just discovering stuff with our normal optical telescopes. And it's like, okay, is it there or is it not? I don't know. What am I looking at? Let me decode it. Now we know what that light would look like, even though we have no data.
Starting point is 00:31:11 If there are galaxies being born, this telescope will see them in the infrared because we know what galaxies would look like being born. being born. So it is the invocation of very deep understanding of the history of the universe and the formation of stars and the formation of galaxies to have the audacity to build a telescope just to sneak in and observe that in the way no other telescope has done before. Wow. Now, because it's sensitive to infrared, it can also look deep into gas clouds that are nearby because infrared penetrates gas clouds in the way visible light does not. And so you can look and see stellar nurseries, stars being born, planets taking shape in the disks around the stars being formed. So it'll be hugely useful for nearby gas clouds
Starting point is 00:32:00 as well as the origin of the universe itself. James Webb Space Telescope. Can't wait. Yeah, that's pretty exciting. And it will also be able to see Predator. So. What? Nothing. Oh, because Predator sees it.
Starting point is 00:32:14 It's an infrared. See? See what I did there? Okay. Yeah, I had to like, okay. Yeah, it was a walk. Predator the movie. It was a walk around the block, man.
Starting point is 00:32:24 That was a total walk around three blocks. That was a walk around the block. walk. Predator the movie. It was a walk around the block, man. That was a total walk around three blocks. That was a walk around the block. Okay. Predator the movie. Right. Was an alien who happens to be about the same size as humans and walks on two legs, has two arms and a head and eyes, nose and mouth. But he's from outer space.
Starting point is 00:32:50 Look at me starting and arnold arnold and others you know you make fun of arnold you make fun of arnold schwarzenegger okay english is not his first language if if he speaks however however much you make fun of him, he speaks English better than you have ever spoken German. Well, this is true. Okay. And I'm sure he could pronounce these names. Jack, I can pronounce the names better than you.
Starting point is 00:33:18 Okay? Listen to me, Jack. You screw up the names all the time. I pronounce it better than you. Okay. So, I'm sure. Anyway, up the names all the time. I pronounce it better than you. Okay. So I'm sure. Anyway, so he starred in the movie. We had some other sort of muscled soldier types with very powerful guns.
Starting point is 00:33:35 And it's they against Predator. And Predator, you got to see what Predator saw. And Predator saw in very low res infrared images. and Predator saw in very low-res infrared images. We have detectors that have way better resolution than Predator saw when you saw just this sort of glowing heat source moving in front of them. There you go. All right. It's time to give a Patreon shout-out to the following Patreon patrons.
Starting point is 00:34:08 Chris Gashorn and Russell Kanicki. Guys, thank you so much for your assistance as we make our way across the cosmos. We could not do this show without you. And for those of you listening who would like your very own Patreon shout-out, go to patreon.com slash star talk radio and support us welcome back to star talk we are in the middle of a live cosmic queries so let's jump right back in okay here we go uh i love this question from Extra Crispy Colonel. He says this, how plausible do you think the idea that it is possible for light to reach around the universe and reach us again? For example, I've heard on the show from people like Jan 11 that it is possible
Starting point is 00:34:58 that some distant galaxies might be our galaxies billions of years ago. The light is just reaching us again. Yeah. So you need a different kind of geometry of the universe. What's his person? Mr. Crispy what? Extra Crispy Colonel. Colonel.
Starting point is 00:35:18 Okay, Mr. Colonel. Mr. Colonel. Okay. No, so it needs a different kind of geometry. And, but so the point is there exists a geometry where the light will go out from our universe, curve in the curved fabric of the entire universe, come back and then you can see that light from this direction
Starting point is 00:35:44 and it would be our own galaxy but the the shape of our universe is not one that allows that but people have posed that question and attempted to answer that by looking at the birthday photo of the universe this is the famous cosmic microwave background the cmb CMB. It is a background of microwave light. So here's another redshift thing. That light started out as visible light, like the surface of the sun. It's very rich in visible light. And over the expansion of the universe, it has redshifted way through,
Starting point is 00:36:19 came out the other side, went down through the infrared, and it landed in microwaves. That's how redshifted it got. And so that is a record of the structure of the universe when that light was released. That's when the universe was about 380,000 years old. That's a baby picture right there, relative to the 14 billion year age of the universe that we have today. So there exists shapes of the universe where that could happen, but we're not in one of them. But that would be a fun, interesting universe.
Starting point is 00:36:56 Yeah, that's very cool. You know, Chuck, was it one of our other cosmic queries? It might have been a Patreon cosmic query where someone suggested, can we set up a sequence of mirrors in space? And so you can see our past. And there's nothing preventing that. So if there was a perfect mirror 33 million light years away, okay? Okay. And we took out our telescopes and looked at that mirror we would see earth from
Starting point is 00:37:28 how long ago 33 million years no wait 33 million light years away yes sure wait what am i missing sir don't make me go in there and slap you okay so there's a mirror 33 million light years away. Okay? Oh, 66. Thank you. Yeah, I'm sorry. Thank you. I forgot about the mirror.
Starting point is 00:37:52 It's a mirror. I forgot the mirror. We're looking in the mirror. I missed that part. I missed the mirror. So it goes out there and it comes back. So the light that we see now is like the left earth 66 million years ago okay and that's just on the cusp of when the dinosaurs were taken out by an asteroid and possibly other natural forces on earth like super volcanoes so so if you had a series of mirrors you
Starting point is 00:38:20 could in principle see the history of the earth you You could see your own past. Yeah. You'd have to pre-set those up and then get back here. That's part of the problem. Well, yeah. We'll work that part out, you know. Right, right. So, no, no, think about it. If you put a mirror 33 million light years away, you have to travel there. At the speed of light, we wait for you.
Starting point is 00:38:41 You come back 66 million years later. We wait for you. You come back 66 million years later. Now you'll only see what Earth looked like when you left, not in our past, because you can't see into the past of when you first put up the mirror. And this is why— Unless you can travel faster than light. Right. And wormhole will allow that, by the way. I can't wait till we have wormholes.
Starting point is 00:39:06 Really. Right, yeah. Well, this is why we have to shore up Social Security. What does that have to do? So when you get back, it'll still be here for you. All right. Okay, okay. Here we go.
Starting point is 00:39:22 How about this one? I said I'd give soundbite answers, and I haven't been. I don't care. They're good answers. Okay. I don't like your soundbite answers. I'm going to be honest. I mean, they're all-
Starting point is 00:39:30 Let's try one. Try one. Let's try one. All right. Here we go for a soundbite. This is Cesar Ruiz, who wants to know this. If the universe is expanding and galaxies are moving away from each other, how come the Milky Way will collide with Andromeda?
Starting point is 00:39:43 Shouldn't they be moving farther away from one another? Galaxies that are near each other have speeds that are greater than the expansion speed of the universe at those close distances. So their orbital speeds override the expansion of the universe, and that's true for our solar system. It's true for galaxies that are nearby each other. That's why we have galaxies colliding all across the universe. These are galaxies that already started nearby each other.
Starting point is 00:40:16 Now, I got to break soundbite mode and give you something that will prevent you from having restful sleep this evening. Uh-oh. Here we go. Okay. You've heard of dark energy. Yes. So dark energy is a pressure in the vacuum of space causing an acceleration of the expansion. Right. That acceleration is, if it is caused by a pressure in the vacuum, then the more vacuum you have, that is the more the universe expands, then the more of this dark energy you have relative to gravity. Because gravity is thinning, okay? As things get farther out, gravity gets thinner and thinner. And if you live in the vacuum of space as dark energy, you win.
Starting point is 00:41:03 And you not only beat gravity, your rate of expansion becomes exponential. Oh. A word we've heard a lot about in the coronavirus. Okay. So calculations show that in 10 to the 22 years from now, okay? The expansion, the accelerated expansion will be so severe that we'll have what's called the big rip. Oh, yeah. That happened to me once on stage. It was terrible. Oh, my God.
Starting point is 00:41:37 It was so embarrassing. And, you know, you got to go on with the show, man. You can't just say, I'm sorry, guys. I got to. Give me five minutes. So it reaches a point where even the gravitational attraction of the planets and their moons and the planets and the host star and in a galaxy and nearby galaxies, even those will not be able to stay together. And galaxies that would have collided would get ripped apart. not be able to stay together.
Starting point is 00:42:04 And galaxies that would have collided would get ripped apart. Then it starts stripping planets from their host solar systems, their star systems. Then it begins ripping matter apart. Okay? This is the big rip. And this accelerates. Okay? So the scenario I'm describing happens fast after you've waited that much time. The scenario I'm describing happens fast after you've waited that much time because the power of this rip, okay, manifests on large scales first.
Starting point is 00:42:37 And then it's happening so much that the very fabric of space itself feels it even on the small scales. And so it starts ripping apart solar systems, ripping apart matter. Then it rips apart atoms. Then. Game over, dude. Game over. Then it might even rip apart the particles themselves. Oh, that's just terrible.
Starting point is 00:42:53 The big rip. So this person wants two galaxies to spread apart. Be careful what you wish for. Wow, Cesar. There you go, buddy. You opened a whole can of galaxies, didn't you? Holy moly. By the way, that's a really depressing thought.
Starting point is 00:43:11 Yeah, just think about it. Just imagine that beginning to happen around you. Oh, my gosh. Dude, that's the Thanos snap. It's like everything just, ugh. That's just terrible. That's terrible. Yeah. Dude, that's the Thanos snap. It's like everything just, ugh. That's just terrible. That's terrible. Yeah.
Starting point is 00:43:28 Okay, here we go. But Thanos saved some people. He didn't do that to everybody. That's true. Yeah. But see, the universe doesn't even have as much compassion as Thanos. Thanos. Damn, universe.
Starting point is 00:43:40 Damn, universe. You cold. Universe. Absolute zero cold. Damn. Okay, here we go. Wait, wait. That was beautifully geeky.
Starting point is 00:43:51 What? I just want you to say. Because in the hood you say, you know, that's cold. That's cold. It insults you. Then you say, yeah, that's so cold. That's absolute zero cold. Yeah.
Starting point is 00:43:59 That's. Oh, my God. Okay. Oh, my God. Okay. You can write a whole play on, like, really geeky street hoods. Yeah. That's so cool.
Starting point is 00:44:14 Call it Blurreds. Blurreds. Yeah, Black Nerds. Black Nerds. There you go. That's so cool. In fact, I think Saturday Night Live had a skit about that. About Black Nerds? Yeah.
Starting point is 00:44:22 Yeah, in the street. They're hanging out on the street. I did not know that. I might have to look that up. Yeah, check that out. And you know what's funny? The one time in life when I'm home to watch Saturday Night Live, because I'm not allowed to go out, because I'm never home on Saturday
Starting point is 00:44:36 nights. I'm always working. And there's no Saturday Night Live. All right. They had a few in the coronavirus episodes. Okay. All right. Hunter Coleman wants to know this. Could the fourth dimension be holding together the fabric of space,
Starting point is 00:44:50 the one that we just talked about ripping all apart? For instance, in our 2D dimension being stuck on a flat surface that our 3D world makes up and holds together, is space the flat surface for us? Yeah, it could be, but I don't think it requires higher dimensions to contain us. It could just be that our life in three spatial dimensions, one time dimension, is the flat surface for the five, six, seven dimensional beings. But it doesn't necessitate that that is the-
Starting point is 00:45:22 That that contains us. That's holding us, right. Right, right. And I would say they would pity us for living in a mere four dimensions. Wow. As we would pity anyone that exists only drawn in a sheet of paper in 2D. That's so true. All right, keep going.
Starting point is 00:45:37 Lightning round. Five minutes. Go. Here we go. NebulaMan6007 says, Would it be possible to make your own man-made wormhole? Is it ever possible? Yeah, so we know how to make a wormhole?
Starting point is 00:45:52 Ooh. No, no, sorry. We know the mathematics of it. Oh, okay. You got me really excited. I was like, what? No, no, it's like, oops, did I just? No. You gave up the tapes and it was too late.
Starting point is 00:46:05 It's too late. No, we don't know how to make a manhole. No, I mean a wormhole. I promise we don't know how. But on paper, we can describe it. But it turns out to configure matter and energy to open the hole, it makes a very unstable conduit. And so we don't know how to keep it propped open
Starting point is 00:46:24 so that if you step in it, then it would collapse around you and no telling what that looks like if it collapses around you. Ah. So. There you go.
Starting point is 00:46:33 And I have to tell this, this is probably the fifth time I've said it on StarTalk. I was in Charlotte Airport and going from a big plane to a little plane. I swear it's three miles to walk that distance.
Starting point is 00:46:43 And it was early in the days of Twitter and I thought I was cute. I tweeted about's three miles to walk that distance. And it was early in the days of Twitter and I thought I was cute. I tweeted about that and I said, you know, I can't wait for when we have wormholes
Starting point is 00:46:51 that when all gates are adjacent to one another. That'd be an awesome airport, right? You just sort of step and then you're there. And then someone replied, Dr. Tyson, if we have wormholes,
Starting point is 00:47:04 you don't need airports. Oh! But the wormhole is the airport. See? Yeah, that's what I'm saying. All right. All right, here we go. Keep going.
Starting point is 00:47:12 A couple more. Here we go. Here we go. This is Raman Sage who wants to know this. How recent is the information our telescope is giving us about anything up there? Since the light is a lot in the past, how are x-ray and other telescopes or even radio signals doing in this context of bringing us information yeah so we speak of things in the present just because it's easier in the same way you speak of the sun rising even though earth is rotating such
Starting point is 00:47:40 that the sun comes in view above your local horizon, it's easier to say the sun rose, okay? In astrophysics, it's easier to say, oh, we observed the star blow up yesterday, or this thing happened two days ago. Well, it happened way longer ago than that, and the light is just reaching us. It just becomes very clumsy to say that. We have no way of knowing anything in the present moment because it takes light time to reach us. You can't even know what the sun is doing right now. If Thanos came in and removed the sun, we would still be in orbit around the sun. You'd still feel the sun's rays. Everything would be the same for eight minutes and 20 seconds. You would have no idea there was no sun there so we
Starting point is 00:48:26 see things not as they are but as they once were and the farther away it is the more ago it once was wow and we're just stuck with that so in a way everything we see in the universe is kind of like a ghost it's all yesterday's news and in in fact, there's an Italian movie called La Correspondenza. La Correspondenza? Correspondence. Jeremy Irons starred in it as an astrophysicist. And he had a terminal illness
Starting point is 00:48:57 and he had a love interest and he would send her letters, okay? But she didn't know he was dying. And I think it was overseas or whatever. But he would send her letters, okay? But she didn't know he was dying. And I think it was overseas or whatever. But he would send her letters so that after he died, she would still get letters. Ah. Like stars that might have died long ago but still send you their love. It's kind of cruel, man.
Starting point is 00:49:22 No, it was an astrophysics love story. Yeah, like I said, it's kind of cruel. All right. All right, one more. How about this one? One more, okay. Archer 12, 123,000 says this. Do you believe in life on other planets?
Starting point is 00:49:40 Yeah, it's not about belief. Is there evidence? There's no evidence yet. What are we made of? Life on Earth? The most common ingredients in the universe is what life is made of. And I've said before, if we were made of like some isotope of bismuth, you would have good arguments to say, hey, life is special. Well, life is rare.
Starting point is 00:50:02 Life is, we're made of hydrogen, oxygen, carbon, nitrogen. This stuff is the top four ingredients in the entire universe. So, as we look for life, just because we haven't found it yet, absence of evidence is not evidence of absence. Okay? So, and by the way, how much of the universe have we looked? I quote Jill Tarter from the SETI Institute. Jill Tarter says, based on how much we've looked in the universe for life so far,
Starting point is 00:50:33 to declare that there is no life would be like going to the ocean with a cup of water, with an empty glass, and you scoop up some water and look at it and say, oh, there's no whales in the ocean. Or no fish at all, right? No fish at all. That's how much of the ocean you've looked at by scooping up a glass. That's how much of what we call parameter space of life in our galaxy that we have studied, that we have observed.
Starting point is 00:51:01 So restricted by time, restricted by frequency, all these factors combined is like dipping a cup in the ocean. So just because we haven't found it doesn't mean every one of my people, astrophysicists have very high confidence to look for it on the expectation that one day we will find it.
Starting point is 00:51:21 The real test is, and the scary and tantalizing part is, could there be intelligent life out there? And if there is, is it more intelligent than we are? Would we even know it if we found it? Because as we've said, one thing is for sure, there is no sign of intelligent life on Earth. Nah. Chuck, I think we've got to stop it there.
Starting point is 00:51:46 Yeah, damn. That's a shame. This was fun. Yeah, yeah. All right, and again, we welcome any and all Patreon members. You're part of our lifeblood. So, Chuck, always good to have you. Always a pleasure, Neil.
Starting point is 00:51:58 And, yeah. And I know we couldn't get to all of the thousand questions, of course, but, you know, that's how this goes. Well, that means we have to do it again. All right. There you go. All right, Chuck. I'm Neil deGrasse Tyson, your personal astrophysicist.
Starting point is 00:52:12 As always, bidding you, especially in the Coronaverse, to keep looking up. Signing off.

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