StarTalk Radio - Cosmic Queries – Cosmic Conundrums

Episode Date: May 4, 2020

Neil deGrasse Tyson and comic co-host Chuck Nice answer fan-submitted Cosmic Queries on black holes, dark matter, the Higgs boson, extraterrestrial life in our solar system, higher dimensions, and muc...h more! 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-cosmic-conundrums/ Thanks to our Patrons Darrell R. Scott, Sand McDowall, Simon Kent, Daniel Chellew, Nathaniel Armstrong, Patrick OBrien, Evan Kelly, and Francois Fraser for supporting us this week. Image Credit: ESA and the PACS, SPIRE & HSC consortia, F. Motte (AIM Saclay,CEA/IRFU - CNRS/INSU - U.ParisDidedrot) for the HOBYS key programme. 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. StarTalk. Neil deGrasse Tyson here, your personal astrophysicist. This is Cosmic Queries Edition. Ah. Cosmic Conundrums. Ooh. Which sound like we couldn't fit them together
Starting point is 00:00:27 into one category. Right. Just put them all together. Better known as Hodgepodge. Hodgepodge. Chuck Nice in the house. We are in the Coroniverse. Yes, we are. Alright. Well, of course, we always have our different
Starting point is 00:00:43 inquiries gleaned from all over the internet. And as usual, we start with… Wait, wait. We're not bringing in another expert. So this means I have to know all the answers. Yes, you do. Okay, fine. Like you don't anyway.
Starting point is 00:00:54 But yeah, we always start with a Patreon patron because you guys give us money. Thank you. Thank you, by the way. Thank you for your money. Isn't there a nicer way to say that? No, I just like being direct like that. Okay, fine. Because it sounds cool, you know?
Starting point is 00:01:09 Thank you for your money, which is what I just want to say on every birthday. And allow me to say that we're using the money to invent other incarnations of what it is we do. Absolutely. Which are all in themselves experiments that we test. You know, we battle test them, see if they work, refine them. And that takes money that we're not otherwise getting from sponsors.
Starting point is 00:01:34 No, exactly. I mean, it keeps us vibrant. It does. The Patreon people don't even know. There's stuff that we've done because of you. Yeah, yeah. You know, which is cool. All right, let's go to Stacey Brown, who's our first Patreon patron.
Starting point is 00:01:45 And she says, Dr. Tyson, if you were captain of the Starship Enterprise, where would you go first and why? And of course, we have to suspend disbelief and say that warp is real. So traveling beyond the speed of light is now a capability.
Starting point is 00:02:06 So now that gives you the option to leave this galaxy, go anywhere you want in the observable universe. I would stick in my own galaxy. Oh. Because there's not enough we know about it. So let me just know my backyard first. All righty. All right. So I would take a tour around the galaxy. Okay. Around the hood. Right. All right. Once then I, so I would take a tour around a galaxy.
Starting point is 00:02:25 Okay. Around a hood. Around a, right. All right. Once around the block, James. Once around the block. If left to the solar system's own motion, that takes about 200 million years for one trip. Cool.
Starting point is 00:02:38 And so, you know, that's still fast given the scale of all of this. But the sun and all the planets and all the comets and all the asteroids and everybody is all moving around the galaxy together. Nice. Okay? Now, there's something that happened on the internet recently. Of course, if we are going around the sun. Correct.
Starting point is 00:02:58 And the entire system is orbiting the galaxy. Right. It means we don't complete a closed orbit around the sun all orbits are corkscrews right because the galaxy is also moving well the solar system is moving it's moving right so if you followed the path so there was this all this attention given to someone showing the video of this and saying oh this is a new theory of the solar system. Oh my gosh, did the experts know this? It's like, people, this is just two motions simultaneously.
Starting point is 00:03:32 Right. Okay, if you do this, you go your orbit. If you go that way, it's a straight line. If you do this and that, you get a helix. Yeah, a corkscrew, right? It's like when you drop a ball on a plane. Oh, yeah. It goes straight down to you. It goes straight down to you.
Starting point is 00:03:46 It goes straight down to you. But if I'm watching you, the ball actually went forward at 500 miles an hour. Exactly. Yeah. Yeah. It's cool. But so did you. Right.
Starting point is 00:03:54 So it just went straight down to you. Exactly. Right, right, right. So that's cool. Yeah, wait, wait. So I would do that. That's just to, but then I'd go straight to the center and observe the supermassive black hole dining upon stars that have come too close.
Starting point is 00:04:10 Nice. That's what I would do. All right. Going to watch the galaxy have a snack. Okay. There you go, Stacy. All right. Let's go to another Patreon.
Starting point is 00:04:20 Tony Mirabella wants to know this. That is a cool name. Tony Mirabella. He does sound That is a cool name. Tony Mirabella. He does sound like a Vegas act, right? That's kind of cool. Tonight only. That's right. Tony Mirabella.
Starting point is 00:04:33 Welcome to the beautiful downtown Stardust Lounge here in Vegas. Ladies and gentlemen, it is my pleasure to bring to you the one, the only, Tony Mirabella. And he's singing before he comes out. Well, that talk's hot. Yeah And he's singing before he comes out. Well, that talk's half. Yeah, you get it. He's singing offstage first, and he comes on. Exactly.
Starting point is 00:04:52 All right. That was so stupid. Okay. He says, What do you think unlocking the secrets of dark matter could do for us scientifically? Would it lead us to being able to harness it wow those are two really big questions how old is he is he some kid in a basement trying to he's trying to figure something out future superhero nemesis in the making he's
Starting point is 00:05:20 making his own little universe or something can we we harness this? We have no idea what dark matter is. The best, I have my own preferences, but my preferences don't matter. What matters is what experiments are active and in progress. And right now, the going thinking is that it is a category of particle that simply doesn't interact with us electromagnetically. So electromagnetism is like light and magnetism and all the things that make atoms stick together as molecules. So you are held together by electromagnetic forces. All right. That's why.
Starting point is 00:06:00 And therapy twice a week. No, I don't have that holding you together. But physically. Emotionally is another thing. Oh, okay. Okay. I don't know what's holding you again emotionally. Right. Physically, you're held together by electromagnetic forces.
Starting point is 00:06:12 This would be a category of particles that does not interact with our electromagnetic forces, which means they just pass right on through like you're not even there. Right. So how do you observe something like that? Gravitationally. Okay. on through like you're not even there right but so how do you observe something like that gravitationally okay so we have a dark we only know the only reason why we know there's dark matter here is because well we have some galaxies but add up all the matter in those galaxies it doesn't account for what's going on in this part of the neighborhood because you see galaxies from behind whose light gets lensed according to Einstein's general relativity.
Starting point is 00:06:46 And you can ask how much mass does it take, how much gravity does it take to lens by that amount? And you come up with a number way bigger than simply counting the galaxies that are there. Something else is happening. So we call it dark matter because we don't know what else to call it. Like I said, I've said many times, it's really dark gravity.
Starting point is 00:07:08 Right. It's literally dark gravity. Right. We don't know if it's matter. The folks betting on it think it is matter, and there's a new kind of particle that we have yet to isolate. That's all. That is cool.
Starting point is 00:07:18 That's what that is. So if we do isolate it, what would you do with it? You put it in your hand. No, it'll pass right through your hand because it doesn't interact with your hand. All right? So I don't know how you would contain it. How do you contain it? You would need a dark matter box.
Starting point is 00:07:31 Right. But who's going to make the dark matter box? I mean, it's a philosophical problem. It really is. If there's a thing that passes right through you, how do you contain it? How do you contain the thing that passes through everything? Everything.
Starting point is 00:07:47 So everything it passes through, you need to find something that can hold it. Thing to hold the thing in. Right. Correct. There you go. You need something that interacts
Starting point is 00:07:55 not only with our forces, but also with its forces. Exactly. That could be yet another frontier of discovery in the universe. What is that intermediary thing? If you were that civilization, Right. you'd be badass. my gosh you control not only all the universe that we know about right but the rest of the universe that's influenced by dark matter you'd be able to grab
Starting point is 00:08:15 it make dark matter planets out of it if you can make it stick to itself so yeah that would be a a powerful posture to purvey. All right. So now, take that and dark energy. Is that also in the question? Oh, no, that was... No, it's not in the question. I answered
Starting point is 00:08:33 Vegas Act. Okay, you answered Tony Mirabella's question. I'll move on. All right. Maybe it'll come up in a different question. You're like,
Starting point is 00:08:40 don't push it, bro. All right, here we go. Eduardo Munoz from Facebook says, Eduardo. He's selling. Hello, my name is Eduardo. Perhaps you know my good friend, Kitty Softbuzz. Who was that in Shrek?
Starting point is 00:09:02 That's, what's his name? Antonio Banderas. Antonio Banderas. That's Puss in Boots. Puss in Boots in Shrek. That was, what's his name? Antonio Banderas. Antonio Banderas. That's Puss in Boots. Puss in Boots in Shrek. That was really good. Yeah, I love it. Okay, so Eduardo says,
Starting point is 00:09:12 can you explain to us immortal language? By the way, he's from Brooklyn. He's named Eddie. Yeah, that'd be funny. You are fantasizing about Shrek 4 or whatever. And he's sitting in Brooklyn. He's in Park Slope going, somebody going, yo, Eddie. All right.
Starting point is 00:09:31 Can you explain to us in mortal language how the boson gives mass to matter? So how does Higgs work, the Higgs boson? How does it give mass? Yeah, yeah. So let me attempt this, okay? That's a lot. So you need to think of mass not as mass in the traditional sense and not in this explanation. Think of it as inertia, okay? So inertia in common parlance is the tendency of something to want to stay in motion. But it's also the opposite of that, or the inverse of that.
Starting point is 00:10:10 It's the tendency of something to not want to move. To stay at rest. Okay. Right. Okay. So inertia is whatever the thing's doing, that's what it wants to keep doing. That's it. All right, that's it.
Starting point is 00:10:17 Okay. Inertia. Okay. Lazy. So you can measure the mass of something by finding a way to measure the inertia that it wields. Gotcha. Okay, so now watch. Let's go to Hollywood. All right.
Starting point is 00:10:32 And we're going to a Hollywood party. Okay. I'm already uncomfortable. And... I used to have a drug problem. No, go ahead. Pick an actor who no one has heard of, that you know of. Chuck Nice of Chuck Nice
Starting point is 00:10:45 Chuck Nice okay you acted a couple of things what have you been in oh please let's not embarrass me no no tell me one
Starting point is 00:10:54 tell me one I just did Kevin Can Wait oh Kevin Can Wait the TV series and it got cancelled okay I did an episode
Starting point is 00:11:02 and they were like well this is over this will never work this is over. This will never work. This is over. He broke it. There we go. But anyway, go ahead. Okay.
Starting point is 00:11:10 So Chuck Nice walks into a party. Right. In Hollywood. And? And the bar is on the opposite side of the floor. Okay. Okay? It's a crowded party.
Starting point is 00:11:22 All right. You want a drink. Okay. You walk straight to the bar. Absolutely. You'll get there in 10 seconds. Of course I will. Okay. Okay? It's a crowded party. All right. You want a drink. Okay. You walk straight to the bar. Absolutely. You'll get there in 10 seconds. Of course I will. Okay.
Starting point is 00:11:30 Beyonce walks in. Okay. She wants to go to the bar. Thank God, because I'm already there. That's what I'm saying. She wants to go to the bar. Right. But what happens?
Starting point is 00:11:42 She begins to accrete people. Beyonce! Oh, my God, Beyonce! That's correct so she can't get to the bar in 10 seconds no way she has a very high uh a famous person mass because everyone wants to be around her and so her her posse moves slowly through the room. Gotcha. And if you move fast, you have low party inertia. She moves slow. She has high party inertia, a resistance to going fast.
Starting point is 00:12:16 Okay? So you have low resistance to going fast. You just walk right across the thing. Right. Or no resistance. Or no resistance. Exactly. Yeah, that would be me.
Starting point is 00:12:24 Yeah, people, in fact, if you're funky smelling, they're parked away. I was going to say. You get there faster. If it's me, I go straight past the bar, out the back door.
Starting point is 00:12:32 Out the back door. Because that's how much they actually want me at the party. Okay, but go ahead. All right. So this is making sense so far. So, so there's, think of it as the party field.
Starting point is 00:12:42 Okay? Okay. The party field is giving mass to the particles moving through it. Gotcha. Okay? That party field is like a Higgs field. Right, because those are the party goers.
Starting point is 00:12:55 The Higgs field is like they're like the party goers in Los Angeles. In Los Angeles. Okay? Right. So you got that? So the more famous you are, the slower you can move through a crowd because everybody wants a piece of you. Right. All right.
Starting point is 00:13:10 So in that way, Beyonce has a very high party mass. You have a very low party mass. Correct. And you get everybody else in between. Gotcha. So that's kind of what the Higgs field is doing. It is the resistance to movement of the particles that pass through it god first of all it's a just a great picture you know because we can all imagine that right that's a great
Starting point is 00:13:34 depiction yeah and that is fascinating like who who thought of that i don't know i might have heard it somewhere i don't remember that's awesome. I mean, that's probably the best way you're ever going to understand. I think so. I think so, yeah. That's great. That is really, really good. Oh, and one other little thing that we learned from Jaina, okay, friend of StarTalk. Jan 11.
Starting point is 00:13:57 Jan 11. That grants particles its mass, but it's not most of the mass of the universe. Most of the mass in atoms comes from the force fields inside the atom, not from the particles themselves. Wow. Binding energy of the atoms. So, yes, it gives mass to quarks and electrons and this sort of thing. Yes. But the total mass of everything in the universe
Starting point is 00:14:27 is not represented by the Higgs field. It's just the particles within that are out there. Okay, so just a little detail. And I got straightened out on that by Jaina. That's cool, man. Well, that's all really good stuff. Man, Eduardo, I hope that cleared some things up. It cleared.
Starting point is 00:14:46 We're going to take a quick break. When we come back, more... You got to take us out in that voice. Go, go. Stay tuned. More StarTalk Cosmic Conundrums when we return. We're back. Start talk. Sorry, did I do it too?
Starting point is 00:15:26 Sorry, I don't have it. I don't have the, what should we call that? That is an accent. I guess so. I don't have the accent. All right. Keep going. Cosmic conundrums.
Starting point is 00:15:38 Here we are. All right, here we go. Woo, here we go. Jenny Totten wants to know this. She's coming to us from Facebook. Hey, Neil, does time move faster at the expanding edge of the universe and slower at the center? Now, in there, there are some assumptions that I don't know. I don't know.
Starting point is 00:16:04 I might have to talk to, first of all, the center part, and I don't know. However, I love the question in terms of the expanding edge. Okay, here's something interesting. It might not be what you were thinking. All right. If you're moving away from me in an expanding universe, and you have a clock that's ticking seconds, if I watch that clock,
Starting point is 00:16:33 consecutive seconds that I observe will come to me more and more delayed. Right. Okay? So when I observe you, it will look like you have slowed down. Right. But as far as you're concerned, you're just running a stopwatch. I'm just running a stopwatch. That's right. That. Okay. So when I observe you, it will look like you have slowed down. Right. But as far as you're concerned, you're just running a stopwatch. I'm just running a stopwatch. That's right. That's right. So when she talked about the expanding edge, if you're going to
Starting point is 00:16:54 watch that edge, you will see things slow down in that place. Right. Okay? But it's not an actual edge. Right. It's not a physical edge. It's just a horizon where you, that's all that is. If you go to that edge, now you're in the middle of a new horizon that is itself whatever distance away it would need to be if you did the math on that.
Starting point is 00:17:20 Right. So the way to answer that is if you want to make any of that true, it's the opposite of what she said. You'd be observing objects evolve more slowly on the edge, the expanding edge, relative to you. Right. Gotcha. Okay.
Starting point is 00:17:36 That's pretty cool, actually. That's pretty dope, I got to say. I like that. All right. Let's go to Virgil Hayward. And Virgil says, it's pretty cool, man. I got to tell you, these people, they're into this stuff. We got good people.
Starting point is 00:17:54 We do. We got good people. Damn. He says, is there any theoretical way to destroy a black hole? Oh, yeah. Yeah? Yeah, yeah. Cool. You just wait around until it evaporates? Oh, yeah. Yeah? Yeah, yeah. You just wait around
Starting point is 00:18:07 until it evaporates. Oh, man. Gave me the oaky joke. That's the oaky joke. I'm sorry. It's an answer. It's the answer. You just wait around.
Starting point is 00:18:16 Small ones evaporate faster. Right. Big ones, like the ones in the centers of galaxies, they might take, I don't know, a trillion years. Oh, much longer than that what oh yeah yeah yeah a google year google years i'll give it a google but the google
Starting point is 00:18:32 people is an actual number yeah and it was a number before it was the name of a corporation okay yeah and it's spelled differently g-o-o-g-o-l google well they actually misspelled it yeah they misspelled it for the company. So Google years is a one followed by 100 zeros. Then you can evaporate the seriously large, massive black holes in the centers of galaxies.
Starting point is 00:18:53 And yeah, then in that future, it'll be a universe with nothing because all the stars would have died. The proton would have decayed. So the very foundations of matter
Starting point is 00:19:04 would have broken up into fundamental particles. Really all you have is particles. Particles would have decayed. Right. So the very foundations of matter would have broken up into fundamental particles. And really all you have is particles. Particles. That's all you have. That's all you have. Right.
Starting point is 00:19:10 The fundamental particles of the cosmos. So the universe will end not with a bang, but with a whimper. Cool. And not in fire, but in ice.
Starting point is 00:19:22 Cool. Literally. Cosmic conundrum. Cool. Cool. Yeah. Cosmic conundrum. Cool. Cool. It reminds me, there's a line in Back to the Future,
Starting point is 00:19:30 the second one, where, I think it's the second, no, the first, whichever one it is, Marty keeps saying, oh, that's heavy. Oh, that's heavy.
Starting point is 00:19:40 And Doc says, why do you keep saying, because it's 1955, right? Why do you keep saying it's heavy?'s 1955, right? Why do you keep saying it's heavy? Is something wrong with Earth gravity in the future? That's exactly what I would have asked if I were Doc. I like that. Yeah.
Starting point is 00:19:51 All right. That's Back to the Future 1. So, yeah, there you have it, Virgil. It's weight is your answer. We'll just wait around. You got to wait, bro. Yeah, that's why we don't know any way to undo the black hole. Right.
Starting point is 00:20:02 The theoretical way to destroy it is time. There you go. All right, here we go. Lee C. Schneider from Facebook says, Which is more likely, extraterrestrial contact celestially or interdimensionally? Oh, definitely physically. Dimensions, we don't. Wait, no, no.
Starting point is 00:20:22 No. No, no, I want it to be true. You do. Oh, yes. Access to higher dimensions? Come on now. Right. I think we even't, no, no. No. No, no, I want it to be true. You do. Oh, yes. Access to higher dimensions? Come on now. Right. I think we even did a thing on going to the fourth dimension
Starting point is 00:20:31 from the three dimensions, two dimensions. With the sphere that drops through a piece of paper. Exactly. Which is just a painterly, beautiful. You love that analogy. I do because it makes things so easy. Well, let me describe it for people. So if you have an intersection of dimensions,
Starting point is 00:20:48 the consequences can be extraordinary. Yes. So if we live inside a sheet of paper and a three-dimensional being says, I've got this sphere, and they don't even know what a sphere is. All they have are circles. Ha, ha, ha, right?
Starting point is 00:21:01 So a circle is a sphere in two dimensions. Or a sphere is a circle in three dimensions. You can say it either way. So if I'm a mighty three-dimensional creature and I take a sphere, a hollow sphere, and I pass it through your universe. Right, my paper universe. How would you describe this? You say, oh, there's a dot.
Starting point is 00:21:20 Where did that dot come from? Right. It's mysterious. Right. Then the dot becomes a circle. Right. Now, you only know it's hollow in the inside because I have to open up a portal so you can look in.
Starting point is 00:21:31 Otherwise, it's just a, you wouldn't know it's hollow. Right. But anyhow, so it's a circle. And what happens to the circle? It grows. Until what size? Until it's the diameter of the sphere. Until the full diameter of the sphere.
Starting point is 00:21:42 Right. And then what happens? And then it would shrink. Shrink down and then becomes a point and then disappears completely. And you have to explain that to your friends. Right. That is so cool. So imagine a four-dimensional thing passing through our universe.
Starting point is 00:21:54 Right. That would be, how would you even describe? You'd see a cube show up in the middle of nowhere and then disappear. Right. Right? That would be the three-dimensional slice of the four-dimensional hypercube passing through
Starting point is 00:22:08 our three-dimensional world. Wow. So in other words, the two-dimensional slice of the sphere is a circle passing through your paper world.
Starting point is 00:22:17 Right. The three-dimensional slice through a four-dimensional hypercube is just a cube. Right. So the cube will start small, get bigger, and then shrink down again, disappear. Damn.
Starting point is 00:22:29 Wow. I know. Dimensions are cool. I don't know how to access another dimension. I wouldn't even know where to begin. So I will bet that we will contact extraterrestrials before we know how to go in and out of higher dimensions. Right. But the idea would be that... So here's what I want to tack on to this, though.
Starting point is 00:22:48 How would, they would know how to observe us, but how would we ever be able to observe them, though? If they're a higher dimensions, they could observe us and we would not even know they were there. Never even know they were there. Correct. So then, you know, oh, okay. And so then what we would only be able to observe is what they are able
Starting point is 00:23:07 to put into our... No, not to put into it, but to pass through it. Pass through. Not put in, but pass through our reality. Yes.
Starting point is 00:23:15 I guess they could put it in our reality, but it would be so... Their reality is so much richer. It'd be... They'd want to just pass it through. Right.
Starting point is 00:23:23 It's like, so let me give the paper people something to play with and just pass it through. It's like, so let me give the paper people something to play with and just draw a circle. You know. Right, exactly. That's not going to do much.
Starting point is 00:23:31 Yeah, right. So we would observe that we would never be able to observe their universe. Unless we had access out of our dimensions to their dimension.
Starting point is 00:23:38 That's correct. Wow. Now, here's something interesting, ready? Go ahead. If you're a two-dimensional being and you have skin, so you draw the skin, we have an inside. Here's something interesting. Go ahead. If you're a two-dimensional being, and you have skin,
Starting point is 00:23:48 so you draw the skin, we have an insides. Okay. We three-dimensional beings would be able to see inside their bodies. The heart, the lungs, the mouth, the eyes, everything. Right. But they would not be able to because they can only see in the paper,
Starting point is 00:24:02 and they would just see the outer skin, which is just a line. Right. What that means is a four-dimensional person can see every one of our organs at all times. I feel so naked. I feel bi. They can see inside your organs.
Starting point is 00:24:17 That's cool. So surgery, the future of surgery could be four-dimensional surgery, where they come at you from a fourth dimension and never have to cut you open. Think about that. I like it. That's a sci-fi story right there.
Starting point is 00:24:31 Got to tell you, never going to happen in America. Not with this healthcare. That's all I can say. Yo, that is so cool. Well, hey, Lee, thanks so much for that question, man. That's very, very cool. Let's go with- Time for a couple more questions.
Starting point is 00:24:48 Okay. Mario Fierera says, Do you think it's possible we'll find complex organisms like fish in the liquid water masses in the planets and moons of, he says, our solar system? Yeah. Okay, so first, a fish is a way complex organism, right? Generally, when biologists speak of complex organisms, they're not talking about fish. Right. They're talking about multicellular creatures that might have some appendages.
Starting point is 00:25:24 They might have, like at the Cambrian explosion of life, when was that, 450, 500 million years ago? Right. We went from single-celled creatures rapidly, when the conditions changed on Earth, to multicellular life. And that multicellular life had like limbs and eyes and antennae. It had features that you could talk about and point to. Generally, we call that complex life.
Starting point is 00:25:50 Complex life. Okay, and then you want to- So how about it's a single-cell organism, but it has propulsion, like celia or- Oh, you mean a way to move around? A way to move around. No, no, that'd still be simple. If it's single-cell, that's simple. Single-cell is still simple.
Starting point is 00:26:03 Correct, correct. Even if it's moving or not. Even if it can do all that. But we're talking about I got legs and I got eyeballs and I got a nose and ears, that sort of thing. That's complex. Features, as you said. So the question was, will we find something? Okay.
Starting point is 00:26:17 I want to find life in the oceans beneath the frozen surfaces of the moons of Jupiter and Saturn. And I want there to be life there. But if there isn't, you know, okay, I'll deal. I'll recover. But if there is life, it'll be something that swims. It'll be something that, and think of all the things in the ocean that swim that are not fish. That's so true. Well, swims are that is alive, like coral.
Starting point is 00:26:46 Right. You have shellfish. Right. I mean, you know, swimmy fish, right? Yeah, exactly. So, who else do we have? We have Ariel, isn't there? Sebastian.
Starting point is 00:26:58 Yeah, Sebastian. I can't forget Sebastian. Yeah, the hermit crab. Right. No, no, the hermit crab. He's got a Jamaican accent. Why you do this to your father? Ariel. Your father,. The hermit crab. He's got a Jamaican accent. Why you do this to your father? That'll be your one.
Starting point is 00:27:07 Your father, he love you so bad. Anyway. So, you got Ariel Sebastian. You got, you've got, what else? You've got Sponges. Sponges. Yeah, I mean, just. Crams and oysters.
Starting point is 00:27:21 You got Spongebob is down there. Yes, Spongebob. Spongebob. So, so, oh, who's the starfish got spongebob is down there yes spongebob spongebob so so oh uh who's the starfish in spongebob uh patrick patrick of course correct i was confused with mr widward squidward squidward squidward i just realized i know too much about spongebob that was too easy for me that was you didn't even i didn't even bat an eye yet you. That was way too easy for me, man. That should not have happened. That should not have happened.
Starting point is 00:27:49 We doing a show about astrophysics. And who's SpongeBob? Just laying out the SpongeBob character. Patrick and the nurse, Mr. Crab. And of course, there's Squidward. Oh, God. And who's the squirrel? Sandy.
Starting point is 00:28:03 Sandy, that's right. Thank you. Yeah. So anyhow, where was I? Where the hell was I? So, you're saying if the life is going to be there, it's going to have features and, you know, you want that. It could be. I mean, think about it.
Starting point is 00:28:14 It'll be at least as exotic as the range of creatures that are exotic in our own ocean. Exactly. And the funny thing is the deeper you go in our ocean, the more exotic the life becomes. Well, unless you've seen it before. Unless they've seen you. You look exotic to them too. We got to take a break.
Starting point is 00:28:33 Thank you. When we come back. That was not a compliment, Chuck. Cosmic queries, cosmic conundrums when we come back. Hey, we'd like to give a Patreon shout out to the following Patreon patrons. Daniel R. Scott
Starting point is 00:28:56 and Sand McDowell. Thank you so much, guys, for your help. Without you, we couldn't make this show. And for those of you who are listening who would like your very own patreon shout out go to patreon.com star talk radio and support us we'll love you for it we're back cosmic queries cosmic conundrums. Very nice. Chuck.
Starting point is 00:29:26 Yes, sir. Bring them on. All right, let's just jump right back into this. This is Ross. We have a good question so far. These are very good questions so far. Ross Nippold says, do you... Oh, just one thing about the previous segment's question. Yeah.
Starting point is 00:29:41 Asking about what kind of life we might find, if we find life in the oceans and things. Just there's, it's not only if there's water there. Right. Okay. I just want to get thermodynamic on you. Okay. Okay.
Starting point is 00:29:52 Go for it. All right. As far as we know, whatever life is, it will require metabolism. Okay. Right. It'll have to process energy in some way.
Starting point is 00:30:04 Okay. For it to process energy in some way okay for it to process energy in its environment there has to be a place that has more energy than in another place so that there is energy flow okay exactly like our sun if the entire entire ocean were exactly the same temperature and there were no water currents and there was no source of energy, we don't know how life could come to be or exist or even thrive. So life does not happen without a transference of energy. Correct. And technically you'd call that an energy gradient. Okay. Okay. Gotcha. So that's what you need. All right.
Starting point is 00:30:47 And so under there, there's sources of energy from like the gravitational stress from Jupiter and from Saturn and other moons on those moons. And that pumps energy like deep in the center. And so… So what… If it's hotter in the center than in the edge, then we're good. So you mean the gravitational forces of the planet that this moon is orbiting. Yes. The tidal forces.
Starting point is 00:31:14 The tidal forces causes an undulation that creates energy heat like when you bend a paper clip back and forth, back and forth. A better example would be when they say, if you're going to play racquetball, let's warm up the ball. And what are you doing? You hit the ball. You squeeze in and it pops back up. It's a deformation and a restoration. And every time you do that,
Starting point is 00:31:37 you're pumping energy into the ball from your racquet. That's what's going on to those moons right now. All right, that's dope. That's really dope. That's dope. That's really dope. That's dope. And the hottest moon in the solar system is called Io, and it's closest moon to Jupiter, and it's feeling this ferociously,
Starting point is 00:31:53 and it's got the most ferocious volcanoes that ever were. Because it's hot in the middle, the stuff has got to get out, and it's hurling every day. And that is basically from gravity. Gravity stress. Gravity stress. Stress of gravity.
Starting point is 00:32:09 Pumping it. And by the way, it's outside of the Goldilocks zone. Right. So we used to think, oh, you need the sun and it's got to be just right. No, you just need energy. Right. All right. There you go.
Starting point is 00:32:20 Okay. Damn. God, I just love science. It's so good. That is so. All right, keep going. God, I just love science. It's so good. That is so. All right. All right, Roy Luckett from Facebook says this. Roy what?
Starting point is 00:32:34 Luckett. Luckett? Luckett. That's a word? That's a name? That's a name, man. All right, Roy. Roy says, hey, Neil.
Starting point is 00:32:39 Roy Luckett, that's a cowboy name. Hey, I'm Roy Luckett. How y'all doing? I'm Roy Luckett. Welcome to Grand Ole Opry. I'm Roy Luckett. How y'all doing? I'm Roy Luckett. Welcome to Grand Ole Opry. I'm Roy Luckett. Come on by for the rodeo. Roy Luckett says this.
Starting point is 00:32:53 Hey, Neil, let's talk about low orbit. Nice. And that's all he says. Okay. Okay. Is that all? That's it. Oh.
Starting point is 00:33:01 That's why I wanted to read it because who writes that question? That's cool. Roy Luckett said that. Roy Luckett. And you know what that does to him? He's kicking back with a beer, and he wants it. Talk to me. Bring it on.
Starting point is 00:33:11 That's right. All right. So, ooh, how deep into this rabbit hole do you want to go? I don't know, man. All right. You ready? Low orbit. You ready?
Starting point is 00:33:24 Go. I don't think you're ready you ready low orbit low you ready go i don't think you're ready all right are you ready i'm about as ready as i'm ever gonna be as ready as you think you can be for what i'm about to tell you that's right all right so does it make sense to you that people this is like inside baseball here okay just be ready for this okay does it make sense to you that on earth's equator people weigh a little less than people anywhere else on Earth because of the centrifugal force of Earth's rotation? Okay. Okay, the equator is moving the fastest.
Starting point is 00:33:56 Right. Basically, 1,000 miles an hour. Okay. Because we have 25,000 miles in the circumference. And how long does it take Earth to rotate once? 24 hours. About 24 hours. So you divide those. It's about 1,000 miles in an hourference. And how long does it take Earth to rotate once? 24 hours. About 24 hours. So you divide those.
Starting point is 00:34:06 It's about 1,000 miles in an hour. About. Okay? All right. If you had a different latitude, the circle you take in 24 hours is smaller. Right on down to the pole, where Santa's got no circle at all.
Starting point is 00:34:19 He's just pirouetting. Okay? Very nice. All right. So, yes, we're rotating as a solid object, but the folks moving the fastest are right on the equator. And I forgot, I did the calculation once, they weigh about
Starting point is 00:34:31 you know, four ounces, about a quarter of a pound less. That's a lot. Yeah, no, it's a lot. No, it's very, it's measurable with a household scale. Yeah, I was going to say, I thought you were going to come up with some like No, no, micro something. No, no, no. It's real. It's real. Okay. No, it's real. It's real. Whoa.
Starting point is 00:34:45 Okay. Okay, that's cool. That's cool so far, so good. So let's spin Earth faster. All right. They'll weigh even less. Okay. Poor Santa, his weight doesn't change at all.
Starting point is 00:34:55 Right. Well, because first of all, he's fat. No, stop. Let's be honest. No, he's just pirouetting. Of course. So there's no centrifugal force on the pole. Right.
Starting point is 00:35:05 All right. So, now you weigh a pound less. Mm-hmm. Or kilogram less, whatever is your favorite unit. We just keep doing this. And you can ask yourself, at what speed must I rotate Earth so that you don't weigh anything?
Starting point is 00:35:27 You'll just float there on the equator. That's an askable question, isn't it? It is. If I'm spinning you up and you're weighing less and less and less. Right. You know what speed that is? What? You rotate the Earth once every 90 minutes.
Starting point is 00:35:41 Every, instead of 24 hours. Yes. It's an hour and a half. An hour and a half. And everything on Earth would just fly out into space. Everything on the equator. Everything on the equator, because that's right.
Starting point is 00:35:49 Everything on the equator. Because the other stuff doesn't weigh as much. Okay. Right. All right. The other stuff doesn't have as much centrifugal force.
Starting point is 00:35:55 Right. All right. So. Go ahead. Keep going. Okay, so wait a minute. Keep going. So if I'm on the equator now,
Starting point is 00:36:03 and my feet aren't even touching the ground. I'm just floating if I'm on the equator now, and my feet aren't even touching the ground. I'm just floating. I'm just floating. Right. Yet somehow I'm staying with Earth, as you had always been, even up to that moment.
Starting point is 00:36:13 Correct. Up to that moment. You're there now. You just weighed one pound. You can jump high, but you're still rotating with Earth. You rotate Earth a little extra. Now you're just floating.
Starting point is 00:36:25 I just described for you orbit. Low Earth orbit. You know, I forgot that that's where we're going. That's where we're going. Do you know how long it takes the space station to orbit the Earth? 90 minutes. 90 minutes. So that, oh, wow, that is cool, man. I dig it. Is that good? That's it.
Starting point is 00:36:49 Is that good? That makes sense. Is that good? That's good. That's an orbit. I love it. Okay. So low earth orbit is now, now of course, low earth orbit in practice, you want to be in above, above enough of the atmosphere. So you're not so you're not burning up through the atmosphere. Of course. You want to be high enough. So you go up 100 kilometers, about 60 miles. You're high enough above most of the atmosphere so that you can now orbit the Earth
Starting point is 00:37:14 faster than the Earth would take you, and you complete one orbit in 90 minutes. If you're right exactly above Earth's surface, it's actually 88 minutes. Okay. If you do the math, it's 88 minutes. You go up to where the space station is about 90 minutes. Got you.
Starting point is 00:37:29 Okay? All of that's low Earth orbit. LEO, we call it. LEO. Affectionately. Low Earth orbit. Yeah. You go a little higher up.
Starting point is 00:37:36 Right. 500 miles up, that kind of thing. Mm-hmm. You get to MEO. Mm-hmm. Medium Earth, middle Earth orbit. Okay. Not middle Earth. Right. But middle earth orbit okay not middle earth right but middle earth orbit middle okay right and there you'll find the gps satellites okay all right so they'll do an orbit it'll take longer than an hour and a half but slower than 24 hours okay okay then you
Starting point is 00:37:58 go a little higher you get geo geosynchronous orbits. So these are orbits where, you can do the opposite and say, if I go farther away, I can stay in orbit with a lower and lower speed. Okay? Here's Earth turning beneath my feet. Is there a distance where I can orbit exactly with the rotation of the Earth
Starting point is 00:38:21 so that I take one orbit in 24 hours? Yes, there is. It's 23,000 miles up, and it's called geosynchronous orbit. the rotation of the Earth so that I take one orbit in 24 hours. Yes, there is. It's 23,000 miles up, and it's called geosynchronous orbit. And there's the synchronicity. There's the synchronicity. Wow. So you launch that satellite, it just hovers overhead.
Starting point is 00:38:34 That's very cool. And if you park one park between Europe and the United States, you can beam signals up to it, and you can talk to beyond the curvature of the Earth. That's it. is up to it and you can talk to beyond the curvature of the earth. That's it. Elon Musk wants to launch
Starting point is 00:38:46 constellations of satellites so that you don't have to beam out to 23,000 miles. You know why? Because if you beam a light signal 23,000 miles, that's far enough away that the round trip,
Starting point is 00:38:58 you notice that in telecommunications. It's a lag. There's a lag. It's a lag. You'll notice it. And sometimes you'll see it in a broadcast or even sometimes you've been on a phone and there was a lag. There's a lag. It's a lag. You'll notice it. And sometimes you'll see it in a broadcast
Starting point is 00:39:05 or even sometimes you've been on a phone and there was a lag. That's probably hitting a geosynchronous site. So communication, you want the satellites to be lower. Right. But if it's lower, you're not always in view of it. Right. Because its orbit's out of your zone.
Starting point is 00:39:19 It doesn't stay with you. So now, once this goes out of the thing, you want another one coming in right behind it. Right. That's why Elon is launching hundreds of satellites so that everyone has fast internet and with with no lag cool yeah well thank you elon and and and thank you uh roy roy luckett roy luckett oh damn boy i didn't know that was such a good question leo right there that was uh chuck we got time for one more question.
Starting point is 00:39:45 Make it a good one. All right. Or make it a bad one. We'll turn it into a good one. Okay. Sean Farouk says this. If a faraway planet emits a light of low frequency and light of high frequency, which one of them will win the race and reach us first oh the speed of
Starting point is 00:40:09 light in a vacuum does not discriminate by frequency boom there you go however if it goes through a medium mm-hmm it. Gotcha. And it is because different frequencies move through media at different speeds that the colors manifest after it comes through. Okay. So if you put light through a prism, and you put it at the right angle, at the correct angle, the white light comes in and the prism says,
Starting point is 00:40:47 blue, you're coming out first. Red, you're coming out last. I'm spreading. And since it's spread, since they go through at different speeds, all the colors reveal themselves as they come out of the prism. There you go.
Starting point is 00:40:59 Separating in the process. So the prism is glass. Air will separate the colors. Diamond does it the best. It's the most transparent. It's the densest transparent thing we know. Okay. So that'll do it the most.
Starting point is 00:41:15 Slows down the light better than anything. And it slows down light to 40% of its vacuum speed. Of course that makes sense, which is when you look at a diamond and it refracts all the light and you see all the pretty colors. All the pretty colors. Right. That's what's going on.
Starting point is 00:41:29 And it does that better than glass does. Right. That's why diamonds are diamonds and glass are glass. Right. Don't tell my wife that. Cubic zirconium gets you halfway there. I don't know.
Starting point is 00:41:45 So different frequencies of light do travel at different speeds through a medium. And just to make that clear. And so now there is medium in space like gas clouds. When light comes through there, you get this effect.
Starting point is 00:42:01 Right. You get this effect. And you can get a time lag in an explosion if the explosion happens in multiple frequencies. You'll see it happen in one frequency before it does in another. And we have coordinated our telescopes to check for this.
Starting point is 00:42:13 Nice. You have a radio telescope, a visible light telescope, an infrared telescope, and you can see phenomenon if it's coming through a medium that will differentially slow down the frequencies of light.
Starting point is 00:42:25 It's very cool. That is excellent. But in a vacuum? That's it. It's a tie. The speed of light is the speed of light. That's very cool. Okay. Neil deGrasse Tyson and Chuck Nice, signing off from the Coronaverse, StarTalk
Starting point is 00:42:41 Cosmic Queries. Keep looking up.

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