StarTalk Radio - Tour of the Solar System

Episode Date: March 28, 2013

Take a tour of the solar system with Mars Exploration Rover scientist Steve Squyres and planetary scientist Heidi Hammel. Subscribe to SiriusXM Podcasts+ on Apple Podcasts to listen to new episodes ad...-free and a whole week early.

Transcript
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Starting point is 00:00:00 Welcome to StarTalk, your place in the universe where science and pop culture collide. StarTalk begins right now. Welcome back to StarTalk Radio. I'm Neil deGrasse Tyson. I'm an astrophysicist and director of New York City's Hayden Planetarium. And joining me this week as my guest co-host, Chuck Nice. Chuck. Thanks for having me back, Neil. I will not soon forget the Super Bowl show, the football show.
Starting point is 00:00:34 You were on fire. Dude, that was great fun. You were out of control. That was great fun, man. Ready to get back into it today and get high on science. We're going to get really high on science. Today's show is a tour of the solar system. Sweet.
Starting point is 00:00:50 A tour of the solar system. I think every now and then you've got to take a tour of your backyard. Fantastic. That's what you've got to do. Will you be our tour guide? I will be your tour guide, but I have some help from two very competent colleagues of mine. One of them is Steve Squires. He's the scientist behind the Mars rovers.
Starting point is 00:01:05 Wow. You know, we all read about the rovers, and you saw pictures of the terrain. He's in charge. And these are his babies. Did they blame him when they broke down? No, they blame him when they save, you know, these things should have broken down long ago. Oh, really? Way long ago.
Starting point is 00:01:21 Oh, cool. So he's been saving them. He's their savior, as it were. We're also, we'll be hearing from Heidi Hamels. She's a senior research scientist at the Space Sciences Institute in Boulder, Colorado. Colorado, yeah. So that should be fun. But you know who's a friend of StarTalk Radio?
Starting point is 00:01:37 I do know. Bill Nye. Bill Nye, the science guy. So were you influenced by him when you were a kid? Absolutely. Absolutely. And by kid, you were a kid? Absolutely. Absolutely. And by kid, if you mean 20, yes. So I got a hold of Bill Knight.
Starting point is 00:01:52 By the way, lately he's the executive director of the Planetary Society. He finally has like a real job, you know? Oh, really? He gets a paycheck and everything. Honestly, I always wonder, what else does he do? What does he do? Except show up on TV and talk to kids. Exactly.
Starting point is 00:02:06 No, no. He's actually talking to grown-ups now, including Congress. Okay. So he's going to start us off and put us in a good way, getting us to think about where we are in the solar system and where we might one day go. The most recognizable image to anyone on Earth is the Earth, as seen from space. When you look above you at night these days, I hope you notice occasional very bright objects among the stars, other planets. Humans have spent centuries trying to know all about them. By exploring the solar system, first with our eyes, then telescopes, and these days with extraordinary spacecraft,
Starting point is 00:02:43 we have come to know that Mars is cold, Venus is hellishly hot, Saturn would float if it could, and our Earth is but one world among thousands of objects whirling about a common star. Between and beyond the planets are all manner of objects, comets, moons, asteroids, distant icy plutoids, and dust. Often as a young scientist, I'd be given a textbook with a place to write my name inside the cover. Below that, my street, my city and state. But I'd go on. United States, North American continent, Earth and sun. Because we've explored our solar system, I could have added the third rocky ball from the medium-sized star. Have a look around. Your life is changed every day by explorers who've pondered our place in space. For StarTalk Radio, I'm Bill Nye the Science Guy.
Starting point is 00:03:31 That's my boy, Bill Nye. Nice. Okay, I just got to ask you, man. What's that? Plutoids? Plutoids, yeah. Is that like a cosmic mint? Plutoids. A Plutoid?
Starting point is 00:03:42 That's a great product name there. That would be. We should start that out. But what would your breath smell like? That's a great product name there. That would be. We should start that out. But what would your breath smell like? That's the question. Hopefully not cosmic dust. Yeah, you've got to watch out what stuff smells like out there. Plutoids.
Starting point is 00:03:54 So the solar system, its formation was four and a half billion years ago from a huge giant gas cloud. And right in the middle of that gas cloud, where it's densest and hottest, that's where you get the sun. And that's what forms first. And then you get planets and other stuff forming around it there was a day when if you learned about the solar system right it would be like an enumeration of the planets one after another and but excuse me that the solar system is so much more than that from the moons around planets to to the dust and the plane of the solar system, to asteroids, some of which hit the Earth, comets. It's a very rich, dynamic place.
Starting point is 00:04:29 And in case you really want to geek out on the sun, the sun has an actual official classification code. Okay. It's a G, capital letter G, Arabic numeral 2, Roman numeral 5. Arabic numeral two. Okay. Roman numeral five. So G25.
Starting point is 00:04:46 Yes. In three different languages and letters and alphabets and number systems. Each one means something different. Each one means something different. Yes. If you want to geek out on the sun, that's what it is. Now, why G25? Because that really, I don't get it. Okay.
Starting point is 00:04:58 G25. G tells you what the temperature is, okay? Which is a gazillion degrees. That's what G stands for. Really? No. For a moment, I almost felt smart. you what the temperature is, okay? Which is a gazillion degrees. That's what G stands for. Really, does it? No. For a moment, I almost felt smart. I was like, I got it right.
Starting point is 00:05:11 So a star is in order of decreasing temperatures, O-B-A-F-G-K-M. So the sun is one of the cooler of the stars. Oh, yeah. You know it is, baby, because it's here in our solar system. It's cool, but it's actually white hot. And the sun is often portrayed as yellow, but it's actually white. Just go outside and look. It's white.
Starting point is 00:05:29 In broad daylight, it's white. Right. What happens when it gets low on the horizon, then you can look at it without burning out your eyes. Hey, look, the sun is yellow-orange because the atmosphere just changed its color. So those are particles in our atmosphere that actually change the color. Actually, what the particles do is scatter the blue light out of the rainbow, leaving behind the red and the orange. So basically, if you were in space, you would look at the sun. It'd be white no matter what.
Starting point is 00:05:51 It'd be white no matter what. No matter how you put your head. Burn your eyes out, and that'd be the end of it. That'd be the end. The last experiment you did. So what I've got is, let's go to my colleagues. They visited me in New York in my office. Steve Squires, principal investigator of the Mars rovers, professor of astronomy at Cornell University, and Heidi Hamel, who is
Starting point is 00:06:11 total planet babe. She's all about planets. Sweet. And so let's find out what we all have to talk about. So Steve, I keep thinking of you as like Mr. Mars. Anytime I look up in the sky and Mars is there, I'm thinking of your two rovers there. When you look up at Mars in the night sky, do you think that too? Would you just wish you were there? Mars looks different to me than it used to. It used to be, I can remember before we launched them,
Starting point is 00:06:36 looking at Mars in the night sky and it just looked impossibly far away. So now it's your backyard. I look at it now and I think I know this place. You're a kid playing in your backyard. It's a sandbox. It feels totally different to look at Mars now than it did a long
Starting point is 00:06:52 time ago. Do you see it though when you see it in the sky, do the pictures from the rovers, is that what you see? Kind of, except I don't think in terms of pictures. I sort of feel like I know what it would be like to be there. Not just the pictures of the surface, but I don't think in terms of pictures. I sort of feel like I know what it would be like to be there. You know, not just the pictures of the surface, but I know what the clouds in the sky look like.
Starting point is 00:07:09 I know the seasons. The rovers are his avatar. It kind of feels like that. Yeah, it does. And we've experienced Mars through those rovers for so long. I kind of feel like I know what the place is like now. Yeah, but are you now sort of, do you have Mars on the brain so that it's hard to think about the rest of the solar system? No. Heidi,
Starting point is 00:07:27 you get around the solar system, right? I sure do. Yeah, I look at a lot of other planets besides just Mars. We don't have that. We don't have those images. We don't have those rovers on the surface. So I still think a lot in pictures. Plus half your planets don't have surfaces. Well, that's true, yeah. I have to ask, what's your favorite?
Starting point is 00:07:43 You know, it changes with time. It's just like picking your children, right? true, yeah. Right. But they've got... I have to ask, what's your favorite? You know, it changes with time. It's just like picking your children, right? Yeah, exactly. I don't play favorites. You know, at different times, different planets do different things. And so if you were looking at, you know, Uranus at Equinox, and it's busted out with clouds... And that's the official, it's not Uranus, right?
Starting point is 00:08:01 It's Uranus? Yeah, you know, I kind of gave up on that whole thing. I gave up on that. For a while, I was on a mission to educate people about Uranus. And then my own hometown paper wrote a story about those yellow lights, you know, that they were trying for cost efficiency. And the headline in my book. Oh, for the nighttime. Yeah, yeah, yeah.
Starting point is 00:08:20 For street lights. Right, street lights at night so that it would be darker, less light pollution. And some people didn't like it, and they ran a headline about the Uranus-colored lights. And that's when I gave up. I would call it Uranus. That's more traditional. But, you know, when Voyager flew by Uranus in 1986, it was dead. There was like maybe 10 clouds.
Starting point is 00:08:43 It really stretched the contrast. So Uranus was a big ball of gas with no surface features. Basically, yeah. I was like maybe ten clouds. It really stretched the contrast. So you're just a big ball of gas with no surface features. Basically, yeah. I mean, that's right. If you and I were on a spaceship outside it, when Voyager flew by, when Voyager flew by, it didn't see anything. And so everyone thought it's dull and boring. Well, that's not what it's like right now.
Starting point is 00:09:00 It's in a completely different season. And the atmosphere is turning on, and there's bright clouds, and there's dark spots, and there's all kinds of activity on this planet. And it's my favorite right now, because flies in the face of what we were taught in school about Uranus, you know, we were taught that I remember the books.
Starting point is 00:09:16 Uranus was an example of a boring It's the boring one, yeah. That's right, which is just absolutely not true right now. And the books are starting to finally catch up with reality. Now, Mars, of course, is a dynamic place. Yeah, it's changing all the time. I mean, it's got seasons very much like the Earth does. Very different at different times of year.
Starting point is 00:09:32 It's not only very much like, it's like almost exactly like the Earth does, right? I mean, it's tipped how many? 25 degrees. And we're 23 and a half. So it's almost the same. The year is longer, of course. Rotates once in how many? 24 hours and 39 minutes. And let me tell you, if you're operating rovers on Mars, that just plays havoc with your life.
Starting point is 00:09:50 Okay, next time that happens to me, I'll keep that in mind. Listeners, when you're operating rovers, just get ready for this. You would think it would be nice to be able to sleep in an extra 39 minutes each day, but it kind of adds up in weird ways. It gets out of sync, doesn't it? It gets out of sync. Well, you think it's like a slow jet lag that eats away at you. We lived on Mars time for months. We had Mars alarm clocks, Mars stopwatches.
Starting point is 00:10:14 We had food service on Mars time, maid service in an apartment on Mars time. We had blackout curtains on the windows, so you couldn't tell if it was daytime or nighttime. It was like being in a casino. Did you adjust to it, or did you really feel human and terrestrial because your bodies couldn't tell if it was daytime or nighttime. It was like being in a casino. Did you adjust to it or did you really feel human and terrestrial because your bodies couldn't adjust to it? Our bodies could adjust to it just fine as long as Earth did not interfere in our lives. In other words, the blinds on the windows were absolutely good. That was fine.
Starting point is 00:10:38 If you have to live a day that's 24-39, it's perfectly easy to lead unless you have to interact with real human beings in the real world on Earth. Like a spouse or you walk your dog or something. That sort of thing. So what you're saying is you were basically in a Mars habitat. Yeah, we kind of were, but then there would be events
Starting point is 00:10:58 you know, somebody would decide there had to be a meeting at 8 o'clock in the morning Pacific time. And if it's in the middle of my night, I was still expected to show up. And that was when it got difficult. Wait, I thought you were in charge. Not when it came to interacting with the press. When we had press conferences, they were
Starting point is 00:11:13 at 8 a.m. Pacific, and that was it. And yeah, telling CNN that we want to have our press conference at 3 a.m. just didn't work real well. So the press likes your rovers? I think they do. Wow. Geeking out on the planets right there.
Starting point is 00:11:27 Dude, that was like geek-a-palooza. Geek-a-palooza. Isn't it great? Everybody has a favorite planet. Yeah. How many people in the street, you know, just, well, that's my favorite planet for these 11 reasons. Yeah.
Starting point is 00:11:36 Well, most people you ask, what's your favorite planet? They're going to be like, the one I'm standing on. Not the one. Well, this one used to have no surface features and then cloud layer. There's a whole analysis of what they follow and why. Right. And it keeps them pumped every single day. Yeah.
Starting point is 00:11:50 I'm just glad to know that Mars has seasons. Yes. Yes. And polar ice caps. Yeah. This accounts for its allure in the history of science fiction writing. Yeah. Why people have chosen Mars as a target for life more so than other planets.
Starting point is 00:12:04 Oh, darling, I can't wait until we take spring in Mars. Not only that, what we have on Mars is not only the rovers, they're orbiters as well, so that we can know where we might send the rovers next. Otherwise, you're kind of driving blind. And what's good about rovers is it's a mobile geologist, and you don't have to go there. Plus, the rover doesn't have to come back. So if you send a human being, they usually want to come back. Normally.
Starting point is 00:12:27 You got to feed them, you know. You got to send a misanthrope. I hate you guys. Yeah, yeah. Get out of here and go to Mars. So one of the things we found recently in Mars is methane emanating from the sides of ravines in Mars. Really? Yeah, and methane is the kind of gas that is produced in the anaerobic digestion of food. Okay. So, actually, Mars is a big, giant fart, is what you're saying.
Starting point is 00:12:52 Well, no, did I say, did I? I did. Okay. Chuck, that's why we have you on the show. That actually sounds more like Uranus. Or should I say Uranus? No, Uranus. Uranus.
Starting point is 00:13:03 We just got schooled on that one. Uranus, that's what it is say Uranus? No, Uranus. We just got schooled on that one. Uranus. That's what it is. Uranus. So after the break, we'll talk about the search for life and how the search for water is driving the search for life. Because everywhere on Earth where you find liquid water, you find life. Every place, including places like the Dead Sea. The reason why they call it the Dead Sea, they didn't have a microscope to tell them what would do the backstroke. But there are things alive in the Dead Sea. The reason why they call it the Dead Sea? They didn't have a microscope to tell what would do the backstroke. But there
Starting point is 00:13:25 are things alive in the Dead Sea. Not fishes, but there's other stuff that's alive for sure. Right. We've got to take a quick break, but more StarTalk when we return. Welcome back to StarTalk Radio. I'm Neil deGrasse Tyson with Chuck Nice, comedian and TV host and all-around good, funny guy. And I got him here just to chew the fat. And I appreciate it.
Starting point is 00:14:12 Well, it is a pleasure and an honor to have you on board. Thank you, sir. And we're talking about the solar system today, a tour of the solar system, basically. We have two of the world's experts to serve that up. One is Steve Squires, who runs the Mars Rovers, which we've all heard about. Everyone's heard about the Rovers, even if you didn't know he was the man in charge. There's a whole team, of course, but he's the main. He's the top banana.
Starting point is 00:14:33 The top banana. There you go. And Heidi Hamill, who's an all-around planet geek-tress. I mean, is that the word? Geek-tress. You just made it up. I like it. We make it right on the spot.
Starting point is 00:14:43 It's how we roll. And so the solar system is full of a lot of sort of alien worlds. There are moons and planets and comets and asteroids. And one planet is different from the next one. Moon is different from the next one. These are exotic places. Yes. Is there any place, one of these you might want to visit one day?
Starting point is 00:15:01 Pandora. I just love those blue people. They're so adorable with their little tails. I love them. And they're so nimble on tree limbs. Exactly. You worry about me sometimes. You know, because there's so much going
Starting point is 00:15:17 on in the solar system, not everything has a perfectly circular orbit around the sun. A circular orbit is the only orbit you can have and not hit something else. If you do not have a circular orbit, there's a chance you're going to hit something. Something's going to hit you. Now, from what I understand, aren't there planets
Starting point is 00:15:34 here in our solar system that have an elliptical orbit? Yes. No, not anymore. Pluto. Don't get me started on Pluto. Take it outside. Let's go back to Steve Squires and Heidi Hamel. They're going to tell us what kind of a shooting gallery the solar system actually is. Now, Heidi, you go way back with the press.
Starting point is 00:15:56 My first encounters with you, as I think with many, were with the comet impact on Jupiter. You were like the face of the comet. The first impact on Jupiter. There's more than one? We just had another one in July. Oh, I know about that. I forgot all about that. I've been the face of the comet. The first impact on Jupiter. There's more than one? We just had another one in July. Oh, I know about that. I forgot all about that.
Starting point is 00:16:07 Where have you been, man? I've been busy. I'm sorry. I'm sorry. It's an impact. It's the size of the Earth kind of thing. Big explosion.
Starting point is 00:16:14 So Jupiter's kind of asking for it, right? Yeah, well, yeah. Well, it's a big target. Well, it's there to take one on the chin for us. It's a big target. That's really true.
Starting point is 00:16:22 Really true. It's protecting us. It's protecting us. It's a big brother protecting us. But yeah, my first. That's really true. It's protecting us. It's a big brother protecting us. But yeah, my first interactions with the press on any large scale were back in 94 when we were doing weather
Starting point is 00:16:31 broadcasting from Jupiter. What was going on every day on Jupiter? Absolutely. It was pretty exciting stuff. Yeah. So if that happens just in the last couple of decades, this must be going on all the time. We're not living in some special time when Jupiter's getting hit. We thought we might have been
Starting point is 00:16:48 lucky the first time, and when it happened just exactly 15 years later, we realized, hmm, maybe we aren't so lucky. Here's a question. Now that you know what to look for, now that you know what an impact on Jupiter looks like, is there data mining you can do? Can you go back to old pictures? Data mining. So it's like looking back and...
Starting point is 00:17:03 Even after the 94 impact, some folks went and did do that. They went back and looked. We had the Planetary Patrol telescopes. I don't know if you're aware of that. Network of 24-inch telescopes that were just studying Jupiter. Creating an archive of data. Exactly. There's nothing like Shoemaker-Levy 9.
Starting point is 00:17:19 The big one, the 94. So you would have seen it. The pictures are good enough that you'd know. Absolutely. That's right. And people do talk about the historical record. There's reports of Cassini himself, not Cassini the spacecraft, but Mr. Cassini. Cassini the guy. Cassini the guy who did these drawings. It's weird to think there are people with names after spacecraft.
Starting point is 00:17:37 What a coincidence. When you say Galileo, we're talking about Galileo the guy or Galileo the spacecraft. Cassini drew pictures. Or the European navigation system, Galileo. That's right. Their counterpart to our GPS. You've got to get some more astronomers' names in play. He's up, you know, Neil deGrasse Tyson.
Starting point is 00:17:54 He had a mission named after you. You have to die. That's right. These are named after dead people. But people did go back and look. And they haven't seen conclusive evidence in the past of any big events like this. But I'll tell you, nowadays, these amateurs
Starting point is 00:18:09 have terrific telescopes. They have amazing CCD systems. Allow me to clarify. In most professions, if you accuse them of being an amateur, it would be an insult. Whereas in astronomy, amateurs are a badge of pride and courage. And also, they do terrific science now. There's a synergy between
Starting point is 00:18:26 the professional astronomy community that basically has the really huge telescopes, and the amateurs who have smaller telescopes, but they're terrific. And they have tons of time because the amateur just goes out at night and spends all night looking, whereas... And they're in every time zone. Every time zone, all around
Starting point is 00:18:42 the world. With these big telescopes like Hubble or the Keck 10 meter, you might get half an hour a year. And that's all the time you have to look at your objects. So we rely on the amateur community to feed us information about things like impacts on Jupiter. It was an amateur who spotted that and alerted the professional community. This later, the second impact. The second one, that's right. So I'm sitting between two very different kinds of scientists now.
Starting point is 00:19:08 One who you, Heidi, who are still using telescopes. She's kind of behind the time. No, I'm looking at things that are far away. You're still looking at telescopes. And Steve, you're just there, you know? You don't worry about the optics. You don't worry about bad weather. Oh, we worry about both of those, my friend.
Starting point is 00:19:26 First of all, we've got optics all over these rovers. Second, we are very, very sensitive to the weather on Mars. Okay. But it is true that he can send spacecraft to his object and get them there within, you know, a reasonable funding cycle. Before he dies. Before he dies. Yeah. If we want to start talking about planets around other
Starting point is 00:19:45 stars, we aren't going to be sending spacecraft. Or even some of the planets in the outer solar system. If you're talking about a Neptune a mission to Neptune, the time scales for pulling that off are very long. So that's why the Pluto mission, the New Horizons, that was like a light payload
Starting point is 00:20:02 with some really huge engines to get it there. That's right, yeah. Yeah, that one was booking. And it's still on its way, and we've got years to go. Yeah, another five years. So it's humans attack the solar system. That's what this is about, Jack.
Starting point is 00:20:15 I've learned some things, man. Well, this is what we're, this is at the point of the show. The thing I learned that most stuck out was that in astronomy, size matters. Yes, it does. Everybody has telescope envy. Yeah, so whatever size is your – in fact, you go to astronomy conventions, how big is yours? Right.
Starting point is 00:20:34 It's true. But here's the problem. At some point, you got to carry the thing to the observing site. And above a certain size, you just can't carry it. You can't do it. Yeah, you can't even do it. Yeah, I know what you mean. It's not – Chuck, Chuck out of control. Okay, let me shut up. So what we have going on in the solar
Starting point is 00:20:52 system is that planets are no longer just dots of light with pretty atmospheric conditions that photograph through a telescope. We can actually go there and look at surface features. And so there's a whole frontier of planetary science called comparative planetology. And if there's a mountain on one planet, look for a mountain on the other. There's craters, valleys, riverbeds. You compare one object to another. And especially for the terrestrial planets, Mercury, Venus, Earth, and Mars. They're small.
Starting point is 00:21:19 They're rocky. And so we can learn about one by studying another. For example, so we can ask, well, while we've been going to Mars for the past 30 years, guess where the Soviet Union back in the old days, guess where they went the most? Venus. Really? Yes. And they had a whole series of Venera spacecraft.
Starting point is 00:21:37 Venera spacecraft. Yes, that's what they're called. That's right, Venera. So that's the genitive. Kind of sounds like a medical condition. That's all I'm saying. I'm just saying. Well, it's funny that you should ask. Man, I got a bad case of Venera. So that's the genitive. Kind of sounds like a medical condition. That's all I'm saying. I'm just saying. Well, it's funny that you should ask.
Starting point is 00:21:47 Man, I got a bad case of Venera, man. Let me tell you. Go ahead. So what happened was astronomers, when we figured you try to come up with words for names for where you come from. If you're from Earth, Earthling. Okay. If you're from Jupiter, you're Jovian. I did not know that.
Starting point is 00:22:02 You didn't know that? You didn't. By Jove. By Jove comes from? Jupiter, of course. Jupiter, of're Jovian. I did not know that. You didn't know that? You didn't, by Jove. By Jove comes from? Jupiter, of course. Jupiter. Of course, yes. Okay.
Starting point is 00:22:08 And Venus would be Venusian. Venusian. If you come from Venus, you're Venusian. Okay. And so the reason why we came up with Venusian is because the proper genitive form of Venus is venereal. And the medical doctors got to that word before we did. I am so pissed off.
Starting point is 00:22:29 That is so cool. I am so angry about that. And now they took the word right out from underneath. Right out from under you guys. And why name it after Venus? Because it's the diseases common to love and beauty and all that go with it. That makes sense. And that's Venus, the goddess of love and beauty.
Starting point is 00:22:44 Oh, my God. I'm just happy to know that this little condition I have that it needs antibiotics is so romantic. TMI right there. TMI. Oh, it'll clear up. Don't worry. Now, here's the problem on Venus. Yeah, if we sent you to Venus, it would all be cleared up because it's 900 degrees Fahrenheit there.
Starting point is 00:23:03 Oh, sweet. There's a runaway greenhouse effect going on there. And that makes it very hard to investigate because your metals melt. It'll melt lead, for example. You can't have lead solder or anything. Only Superman could do that. So that's hot. Is that right?
Starting point is 00:23:16 Yeah, his laser vision. Okay. Yeah, we should do it. What's funny, he couldn't see through lead, but yet he could melt it with his heat vision. Interesting. How crazy is that? That's crazy. You know, we're going to do a special show on the physics of it with his heat vision. Interesting. How crazy is that? That's crazy. You know, we're going to do a special show on the physics of superheroes.
Starting point is 00:23:27 Get out. Should I get you back for that? Oh, man, if you don't, I will never speak to you again. All right. That's not – we'll work that one out. And so of these destinations, Pluto is on our targets, the ex-planet Pluto. It's got what's called the New Horizons mission. It's booking.
Starting point is 00:23:44 It's the fastest hunk of hardware we have ever sent anywhere. Wow. It's on its way to Pluto right now. It'll get there in 2015. And we're headed there. That's one hell of a road trip, man. It's one hell of a road trip. And it's on hugely powerful rockets because the principal investigator of that mission
Starting point is 00:24:02 wants to make sure you get to Pluto before he dies. See, that's how that works. This is the number one rule of scientific investigation. And so we have spacecraft going to comets, to asteroids. And so we're all over the solar system now. It's a fun time to be alive because the solar system is no longer this distant place. And when we come back after the break, as I promised before, we're going to talk about life, the search for life in the universe. What are the conditions that a planet or an object have to have in order for there to have life as we know it?
Starting point is 00:24:36 Right. Because maybe this could be some stuff that life is you don't know. StarTalk Radio, we're back. You know, over the break, Chuck Nice and I were talking about this mission to Pluto, and he was bugging out the whole time. Yeah, well, first of all, you told me that this thing starts in 2006. Yeah, it was launched in 2006. And then you said, when we were talking on the air, 2015. Yeah, it's a 10-year mission, yeah.
Starting point is 00:25:25 So what do you do in the 10 years? Oh, so the PI is... I mean, you shoot the thing up there, and now you got 10 years. You go to the Bahamas for 10 years. No, I think that I'm told that they're working hard trying to make sure. No, you actually can take images. You test the equipment along the way. Okay.
Starting point is 00:25:43 You get data. It passes other planets. It needs a gravity assist. Okay, gotcha. You know, it's doing things. It's not just... But see, the thing is, Pluto is moving. Yes, it is.
Starting point is 00:25:54 Not very fast, but it is moving. Yeah, so now you're shooting a rocket at a moving target. Yeah, you're not shooting where it is. You're shooting where it will be when you get there. Or at least you hope. Well, that's when... Laws of physics, you don't have to hope. Oh, you're not shooting where it is. You're shooting where it will be when you get there. Or at least you hope. Well, that's when laws of physics, you don't have to hope. Oh, really? Okay, good. So it's not like, you know,
Starting point is 00:26:11 hey man, we got here. Pluto's not home. Yeah, that would be bad. It's like, yeah, it was here three days ago. Okay, so cool. Newton's laws of physics allow you to hit it where it will be, when it will be there. Hence the gravitational adjustments. Is that what you're saying?
Starting point is 00:26:27 No, we know the gravity fully and advance the whole route. Oh, man. We have the capacity to make tiny mid-course adjustments if there's something we hadn't figured. Right. But lately, these things have been going without hardly any use of fuel. Sweet. Oh, yeah. Yeah.
Starting point is 00:26:39 It's a lob shot, basically. So now we're not going to Pluto to look for life. It's too cold. It's too far. It's a lob shot, basically. So now we're not going to Pluto to look for life. It's too cold. It's too far. It's too dark. It's too everything that we can imagine that could serve life. But there are other places in the solar system that could serve this need. And we talked to two of my favorite colleagues, Steve Squires and Heidi Hamill.
Starting point is 00:27:00 We had a geek fest in my office. Geeking out. We were geeking out on the solar system. Just giddy. I can hear you giggling now. We were giddy. Let's find out what they say about our search for life in the solar system. We love the planets, but the real goal is
Starting point is 00:27:15 we want to find life. Mars has been a seductive prospect for life since Lowell. Percival Lowell thought he saw Mars. A little misled, but he had the right idea. His heart was in the right place. He's the beginning, since Lowell. Yep. Okay, Percival Lowell thought he saw Martian. A little misled, but he had the right idea. His heart was in the right place. Yeah, his heart was in the right place. You know, he's the one who invented the canal story.
Starting point is 00:27:31 Do you want to quickly tell us that, the canal story? Well, basically what happened was that people looked through a telescope. A hundred years ago. Yeah, a hundred years ago, in moments of brief atmospheric clarity, they could see what looked like a fine network of straight lines on the planet's surface. And they were so straight and so regular that the people looking at these concluded that not only were they evidence of life, they were evidence of intelligence life. Now, they were correct, but the life was at the wrong end of the telescope. What they were seeing was an optical illusion.
Starting point is 00:28:05 And didn't know enough about illusions to... Yeah, and in fact there's nothing of the sort on the surface of Mars, but as we've learned in recent decades, Mars is very interesting in other ways. Nonetheless. Yes. Nonetheless, with possible evidence of running water. So the two water places that I know of is Europa, one of Jupiter's moons, one of my favorite places just to think about, to dream about, because I want to go
Starting point is 00:28:25 ice fishing on Europa one day. And of course Mars, possibly under surface aquifers. And Heidi, how is Europa kept warm? It's not the sun. No, it's really kind of a gravitational tidal pumping with the other moons around Jupiter that kind of bend it. You know, the
Starting point is 00:28:41 analogy I use is if you take a credit card and you bend it back and forth, a lot of it gets warm. I try not to do that. With old credit cards. Piece of bend it. You know, the analogy I use is if you take a credit card and you bend it back and forth, a lot of it gets warm. I try not to do that. With old credit cards. A piece of coat hanger. A coat hanger. A paper clip. How's that?
Starting point is 00:28:51 You bend a paper clip back and forth a whole bunch, and you touch it, and you feel it gets warm. The same thing is happening with this moon. You know, Europa and Io, they're kind of getting flexed and bent, flexed and bent, and it heats them up. And you know what? Don't forget about Enceladus when you're talking about water worlds.
Starting point is 00:29:08 Enceladus, we now know, is just moon of Saturn. A little tiny one, too. It's also tidally heated. Tidally heated, the same flexing to heat it up. But it's just blasting water out of its southern pole. Geysers, basically. Are these not ice volcanoes? It's liquid water coming out?
Starting point is 00:29:27 It's water. Yeah, you can think of it as volcanoes. It's just that the magma is water instead of being molten rock. It's pressure that builds up and it spews water. It's water. I mean, if you flew a spacecraft through it and collected it and you were able at room temperature, you could drink it. And, of course, every place on Earth we have liquid water, we have life. So therein is the temptation.
Starting point is 00:29:46 That's where the temptation is. What would you bet on, Mars or Europa, as the place, if there's life other than Earth in the solar system, that we would find it? Today. Today. Yeah, see, that's the question. You're talking about life today or life ever existed, because it's a different question. Today. I would say Europa.
Starting point is 00:30:03 Europa, not Mars. If I knew how to do submarines on Europa, I wouldn't be screwing around with rovers on Mars. Yes, sir. What if you dug down into Mars? Doesn't it get warmer? Yeah, it does. And you've got water as you get further.
Starting point is 00:30:16 I don't know how to drill down hundreds of meters on Mars. You don't know how to drill on Europa. Yeah, I mean, they're both huge technological challenges. But if there truly is... Wait, wait, just how thick is to drill on Europa, you don't know how to drill on Europa. They're both huge technological challenges, but if there truly is... How thick is the ice on Europa, approximately? We don't even know for sure that there's an ocean there. I saw the picture. 10 kilometers, 100 kilometers.
Starting point is 00:30:36 It's unproven. It's likely. I saw the ice. It looks like... I can make a picture for you, Neil. It looks like, but you're going to spend tens of billions of dollars doing a submarine mission to an ocean that you don't know for sure exists. Okay. All right. We got work to do there. We got to learn a lot about the environment. I want this to happen in my lifetime. You got two key people here. Eat healthy, get lots of exercise. Okay. Go on that low calorie diet.
Starting point is 00:31:04 1700 calories a day. Get you an extra year per year wear my seat belt yeah yeah but you know what um what might happen in your lifetime is we may find earth-like planets around other stars in a distance from that star where water could be liquid yep i'll tell you another one that could happen in your lifetime, and that is bringing rock samples back from Mars that contain definitive evidence one way or the other on whether or not there was life at the location
Starting point is 00:31:34 from which the rocks came. And ideally, you get to choose your own rocks. Yeah, see, I mean, we have rocks from in fact, I'm sure you've got them in your museum here. We've got rocks from Mars here on Earth in the form of meteorites, but these are rocks that literally fell from the sky. We don't know where on Mars they came from.
Starting point is 00:31:50 We didn't pick them. They just came here. They don't have the pedigree that you need to order them. Mars is a very, very complex place geologically, and to be perfectly honest, most of Mars is pretty boring. Most of Mars is just covered with lava, very dry, very desolate. Solid lava. No evidence that water was there.
Starting point is 00:32:05 Solid lava. Yeah. Yeah, solid lava. And very ancient volcanic rocks and evidence for life you're not going to find in a place like that. To find it, you've got to go to the special places where you have the right minerals, the right sediments, the kind of stuff that can preserve evidence of ancient habitable watery conditions. And those are few and far between. Okay, so we have Mars as a good example of where to look for evidence of ancient habitable watery conditions. And those are few and far between. Okay, so we have Mars as a
Starting point is 00:32:26 good example of where to look for evidence of past life. Europa as a place to look for possible evidence of current life. You could look for evidence of current life on Mars as well, but you probably have to drill deep, and that's hard. GeekFest continues. Man, that
Starting point is 00:32:42 was serious. Now Chuck, do you realize that interview in my office took place a few weeks before the announcement that we found Goldilocks planets orbiting distant stars? Yeah, where they're close enough or far enough from the sun where they can have water. At the right distance, not too close. At the right distance, not too close, not too far. You evaporate too far. Hence the Goldilocks, right? The Goldilocks, exactly.
Starting point is 00:33:02 And so for them to say, this will happen in your lifetime, then happen three weeks later, you know. You ask, you receive. Yeah, like they've worked it up. We have a tweet that someone asked from a tweet. This is Trudvertite. That's the Twitter handle. Is the thought of exploring and terraforming Mars even relevant if we can't even take care of our own planet? Yes, it is.
Starting point is 00:33:26 Let me just field this one. Okay, this one goes to Chuck, apparently. We're going to need a place to go. After we mess up the Earth. Because we're screwing this one up royally, buddy. So we need a place to go. Okay, so you have the opposite sense of this question. This question is, we don't deserve another planet if we can't take care of our own.
Starting point is 00:33:43 You're saying it's because we can't take care of our own that we gotta have the planet. My reply is, if you have the power to terraform another planet, you have the power to fix your own planet. Wow. Just think about that. If you have that much control over geoengineering, what's
Starting point is 00:34:00 a few degrees warming? Just crank the knob that lowers the temperature back again. Exactly, because you'll know what to do. You'll know exactly what to do. Basically, you'll be able to create a geothermal thermostat. A thermostat. Exactly. Awesome phrase.
Starting point is 00:34:13 Shock. Yeah. I don't even know where that came from. A geothermal thermostat. Dude, hanging out with you is rubbing off on me. This is great. That just felt good. I felt smart for a second.
Starting point is 00:34:25 Still don't know what I said. And so we got these. Chuck. And so you got these places. You know, Heidi raised an interesting point. And that if you're looking around for other solar systems, star systems, we don't know yet how common our star system is. We've got these eight planets. Get over it.
Starting point is 00:34:50 We've got eight. We've got sort of Earth and Mars sort of in the Goldilocks zone, but we have these places outside of the Goldilocks zone kept warm. In the case of Jupiter, it's Jupiter's gravity stressing the moons. By the way, in the old days, people said, let's find a planet with life. But you can have a moon. If the moon is big enough, why not have life on a moon? Right.
Starting point is 00:35:10 And if the host planet keeps the moon warm, you don't even have to be in the Goldilocks zone of the host star. So now when you guys were talking about this, wait a minute, tidal heat. Oh, tidal heat, yes. Is that when the gravity moves the planet back and forth or stretches it? It stretches. And that creates the heat. It's a stretching kind of gravity. And it does that to the oceans of the Earth that stretches them.
Starting point is 00:35:33 And Earth turns inside and out of the stretched ocean on the Earth. Wow. Yeah. Oh, yeah. More about tidal heating when we get back on StarTalk Radio. Welcome back to the show. You know, there's a mission up there right now getting data like gangbusters called Kepler. Kepler. Kepler.
Starting point is 00:36:13 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:14 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:15 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:15 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:16 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:17 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:17 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:18 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:18 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Kepler.
Starting point is 00:36:22 Kepler. Kepler. Kepler. Kepler. Kepler. Kepler. Keplers. Keplers. Ke down an equation that told you how planets orbit the sun they call kepler's three laws of motion wow it was awesome first the first law of science in the universe was kepler's three kepler's three laws of motion so basically predictive physical science has only really been around for 400 years
Starting point is 00:36:35 since he wrote down those equations yeah we're pretty new at this we're kind of new yeah compared to other stuff that humans have been doing right So Kepler is specially designed to find Earth-sized planets orbiting sun-like stars. And there's a recent data that was released that had a set of 1,000 stars, 1,000 planets orbiting other stars. And so it tripled the number of total. So we went from 500 to now 1,500 stars, 1,500 planets. 1,500 planets. 1,500 planets. In orbit around stars that are not the sun. Okay.
Starting point is 00:37:08 And out of those, there's about 40 or 50 Goldilocks planets that were found. So there's about 40 or 50 other Earths floating around out there. That could sustain liquid water. That could sustain our life. Or Jupiter-sized planets with moons that are outside the Goldilocks zone. So we're casting a pretty wide net in the search for this. Do you realize this whole field, the search for life in the universe, it's called astrobiology? That's a term, if you went 20 years ago, the term never, no one knew how to use it.
Starting point is 00:37:33 Nobody even knew. It was not really part of the parlance of scientific discourse. And it's a field essentially invented by NASA. Right. So 15 years ago, that would have been just called BS. Well, you need data. Data converts BS to real, to real discourse. Carl Sagan was, of course, a very early proponent of the search for life in the universe.
Starting point is 00:37:55 And we can call him the father of astrobiology in that sense, although there are other people who had done sort of Earth-based bioexperiments that preceded that. But do you want to stay current on the frontier of astrobiology? Right. There's an online NASA magazine called AstroBio. AstroBio. .net. .net.
Starting point is 00:38:10 AstroBio.net. For all of your astrobiology needs, it's AstroBio.net. So now one of the great frontiers here is where you have to ask, how are you going to explore the nearby planets or the distant ones? Do you send a robot? Do you send a human? Do you send a human? Do you send a robot to do what a human can do? This is the major issue, a major question,
Starting point is 00:38:31 and I brought that up with Steve Squires and Heidi Hamel. And let's see what their take is on it. One of them is a geologist and one of them is a telescope astronomer. Let's see where they take us on this issue. Given the choice, because it costs more to send people than to send robots if you had the choice of sending 30 robots to 30 different locations on mars or you going yourself as a scientist not as adventure explorer indiana jones hat wearing expedition head i'm talking about how about we talk about sending you instead yeah wouldn't you be able to come back
Starting point is 00:39:01 i forgot about whether we should bring him back. No, look, I see where you're going with this. Where's the tradeoff? The answer, my personal answer, is that I would send a human. Okay? And I'll give you two reasons for that. One reason is that what humans can do is so much greater than what robots are capable of now or for the foreseeable future. Wait a minute.
Starting point is 00:39:23 Every time we send a human, they bring out a black box that makes the measurement. Well, why not make the robot pull out the black box? No, no, no. There's much more to it than that. Okay, Neil, I have spent the last 20 years of my life trying to design and operate robots that can replicate what a human might be able to do on the Martian surface. What our rovers do in a day, you and I could do in about 30 seconds. That's one thing.
Starting point is 00:39:45 The other thing is that humans have a capability to synthesize information, to digest it, to figure out the next thing to do, and to improvise. Robots can't improvise the way humans can. But it's not just that we're not there yet. I mean, Moore's Law gave us this ever-increasing rate of... I think you've got a couple of million years of evolution to go to that point. We're very, very far away from that. The other reason that I would send humans...
Starting point is 00:40:10 So the brain is still a pretty good device. It's a terrific processor. The other reason I would send humans is that humans have a capability to inspire that robots simply lack. Someone once famously said, nobody's ever going to give a robot a tech-or-tech parade. And there is something to that. It's a little squishy. It's a little intangible.
Starting point is 00:40:26 But I will tell you that our rovers were built by people like me who grew up in the 60s and 70s watching Mercury and Gemini and Apollo on TV and dreaming of sending spaceships to Mars someday. And now we do that. Okay? We were inspired by what we saw as kids. And I think sending humans does that in a way that robots never will. So I think there's a real value to it. Where do you want to go? We could send you somewhere.
Starting point is 00:40:48 And bring you back. You know, there's a lot of great stuff in the solar system to see. And just picking off the low-hanging fruit, you know, I'd love to... Where would you go? I didn't really know. The next place that I would go... The fruit wouldn't have to be low-hanging. Reach for it.
Starting point is 00:41:02 Where would you go? I'm so intrigued by the outer solar system because we know so little about it. There's good scientific juices flowing here. Yeah, we just know absolutely nothing about it. You're drawn to where you are most ignorant. Yeah, because that's where you learn the most. Most people are only comfortable where they know the most. Oh, no.
Starting point is 00:41:21 I want to uncover some of these things that we just don't know. So give me a place. I would like to go to Neptune. Neptune? Yeah. Neptune's a beautiful place. Or Neptune. Yeah. Because that planet system, not just the planet itself, but it's got an incredible ring system that's chunky and it's not smooth
Starting point is 00:41:39 and beautiful like Saturn's. It's clumpy. It's very dynamic. It's changing with time. It's got a terrific moon called Triton, which was captured. It wasn't born with Neptune. It was some object that just got, oops, too close, and Neptune stole it. Stole it. Grabbed from
Starting point is 00:41:55 interplanetary space. This thing is like a twin to Pluto. And we know that it has... Triton is a twin. Triton is a twin to Pluto. We know it has ice volcanoes. It's got geysers. We've seen them. And so this moon is dynamic and changed. So the whole planetary system has something for everyone.
Starting point is 00:42:12 I mean, we'll just learn so much. So you're attracted by the abject ignorance of what we know of the system. That's what attracts you. Plus it's just really alien. It's a really alien place. It's very different. I mean, these ice giants are just so different from Earth. I mean, they don't have surfaces.
Starting point is 00:42:27 You couldn't land on it. But you could land on one of its moons, and that would be great. See, since I'm fundamentally like a galactic person, not a planet person, my destination within the solar system has nothing to do with how much we know. It's just what looks the coolest. So where would you go? Where would you go? I would so go to Titan and just watch Titan.
Starting point is 00:42:45 That's the one with the rivers of methane. It's got lakes and the poles. Lakes of liquid methane. And meanwhile, you're orbiting Saturn. Well, I'll tell you, if you want to go there, you really better eat healthy and get plenty of exercise. It's going to take a while. All right. Thanks, guys, for being on Star Talk.
Starting point is 00:43:03 Chuck, you know, if we find life on Europa, you know what we should call it? What? The Europeans. So, Chuck, take us out of here. What do you? You know, I was listening to that, and I could just think, you know, if the advantage of sending a robot is, you know, they're never going to ask, are we there yet?
Starting point is 00:43:19 You've been listening to StarTalk with Neil deGrasse Tyson. And as always, I bid you to keep looking up.

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