1 00:00:01,400 --> 00:00:05,000 Speaker 1: Hey, Welcome to Science Stuff, a production of iHeartRadio. Hoor 2 00:00:05,040 --> 00:00:09,639 Speaker 1: Hey cham and today we're talking about asteroids. What exactly 3 00:00:09,680 --> 00:00:12,200 Speaker 1: are they? Should we go out there and mind them 4 00:00:12,440 --> 00:00:14,880 Speaker 1: or is one of them going to crash into Earth 5 00:00:15,080 --> 00:00:17,880 Speaker 1: and wipe us out. We're going to be talking to 6 00:00:17,880 --> 00:00:20,800 Speaker 1: one of the most famous astronomers on the planet about this, 7 00:00:21,079 --> 00:00:23,799 Speaker 1: Who's going to step us through the nuances of how 8 00:00:24,000 --> 00:00:27,120 Speaker 1: asteroids form, what it would be like to step on one, 9 00:00:27,520 --> 00:00:31,600 Speaker 1: and what the most valuable resource in them actually is. 10 00:00:32,159 --> 00:00:35,839 Speaker 1: So get your asteroids and gear as we tackle the 11 00:00:36,040 --> 00:00:45,960 Speaker 1: meaty or topic of space rocks enjoying. Hey everyone. I 12 00:00:45,960 --> 00:00:49,040 Speaker 1: don't know about you, but I like planet Earth and 13 00:00:49,440 --> 00:00:51,839 Speaker 1: I'm not in a big hurry to leave it. But 14 00:00:51,880 --> 00:00:54,400 Speaker 1: it does seem that at the rate we're going, we 15 00:00:54,640 --> 00:00:57,480 Speaker 1: might run out of things here, which is why billionaires 16 00:00:57,520 --> 00:01:01,400 Speaker 1: and space enthusiasts have proposed maybe goin shopping out there 17 00:01:01,600 --> 00:01:05,240 Speaker 1: in the asteroid belt. I also like our planet enough 18 00:01:05,280 --> 00:01:07,440 Speaker 1: that I don't want to see anything happen to it, 19 00:01:07,880 --> 00:01:12,080 Speaker 1: like getting hit by an asteroid. So basically I had 20 00:01:12,120 --> 00:01:15,520 Speaker 1: a lot of asteroid questions to answer them, I thought 21 00:01:15,520 --> 00:01:17,280 Speaker 1: I'd reach out to one of the most well known 22 00:01:17,280 --> 00:01:21,760 Speaker 1: astronomers on the planet. Doctor Phil Plait Doctor Plate, is 23 00:01:21,760 --> 00:01:24,800 Speaker 1: the creator of the website Bad Astronomy, as well as 24 00:01:24,840 --> 00:01:29,120 Speaker 1: the author of several books, including Death from Disguise, a 25 00:01:29,200 --> 00:01:31,880 Speaker 1: fun survey of all the ways things from space can 26 00:01:32,360 --> 00:01:34,959 Speaker 1: kill us, including asteroids. 27 00:01:37,640 --> 00:01:39,000 Speaker 2: He also wrote Under. 28 00:01:38,800 --> 00:01:41,720 Speaker 1: Alien Skies about what it would be like to visit 29 00:01:41,800 --> 00:01:45,440 Speaker 1: other parts of the universe, like an asteroid. So I 30 00:01:45,520 --> 00:01:49,520 Speaker 1: had three questions for doctor Plate. Number one, what exactly 31 00:01:49,840 --> 00:01:52,640 Speaker 1: is an asteroid? It turns out there's a lot of 32 00:01:52,680 --> 00:01:56,400 Speaker 1: people get wrong about that. Number two, is an asteroid 33 00:01:56,480 --> 00:01:58,680 Speaker 1: going to hit the Earth and why it was out? 34 00:01:59,160 --> 00:02:03,480 Speaker 1: And three should we mine the asteroid belt? It turns 35 00:02:03,520 --> 00:02:06,480 Speaker 1: out there's more than just rocks and metals out there. 36 00:02:07,040 --> 00:02:11,360 Speaker 1: We'll start with the first question, what exactly is an asteroid? 37 00:02:11,760 --> 00:02:17,200 Speaker 1: Here's my conversation with doctor Phil Plate. Well, thank you 38 00:02:17,240 --> 00:02:18,400 Speaker 1: doctor Plate for joining us. 39 00:02:18,800 --> 00:02:21,080 Speaker 3: Oh my pleasure. It's nice to see you and hear you. 40 00:02:21,280 --> 00:02:23,120 Speaker 3: I suppose hear you. Well. 41 00:02:23,160 --> 00:02:25,120 Speaker 1: I think we're both not enough that everyone knows what 42 00:02:25,160 --> 00:02:27,120 Speaker 1: we look like, or can know what we look like 43 00:02:27,240 --> 00:02:28,080 Speaker 1: with a simple search. 44 00:02:28,280 --> 00:02:30,959 Speaker 3: I'm not too hard to picture, you know, little aged, balding, 45 00:02:30,960 --> 00:02:31,720 Speaker 3: bearded white guy. 46 00:02:31,800 --> 00:02:32,640 Speaker 2: Yeah, you've seen me. 47 00:02:33,760 --> 00:02:35,919 Speaker 1: Well, you famously read a book called Death from the 48 00:02:35,960 --> 00:02:39,160 Speaker 1: Skies in which you talk about, among other things, the 49 00:02:39,200 --> 00:02:41,799 Speaker 1: possibility of an asteroid hitting the Earth. 50 00:02:41,880 --> 00:02:43,120 Speaker 2: We'll get into that, but. 51 00:02:43,120 --> 00:02:46,160 Speaker 1: I guess maybe for people who are not familiar, what 52 00:02:46,240 --> 00:02:48,079 Speaker 1: is technically an asteroid? 53 00:02:48,320 --> 00:02:50,400 Speaker 3: Yeah, you know, this is one of those questions where 54 00:02:50,400 --> 00:02:53,240 Speaker 3: it's like this is really easy to ask and super 55 00:02:53,280 --> 00:02:55,880 Speaker 3: hard to answer. When you think of an asteroid, you 56 00:02:55,919 --> 00:02:58,960 Speaker 3: probably think of a you know, big rock in space 57 00:02:59,040 --> 00:03:02,560 Speaker 3: that's floating around orbiting the Sun. But it gets complicated. 58 00:03:02,880 --> 00:03:04,079 Speaker 2: That's not the definition of it. 59 00:03:04,480 --> 00:03:08,200 Speaker 3: Well, there's no real definition. There's not really a size 60 00:03:08,320 --> 00:03:11,120 Speaker 3: on these things. The biggest ones are a few hundred 61 00:03:11,200 --> 00:03:14,239 Speaker 3: kilometers across or miles if you're an American, but there's 62 00:03:14,280 --> 00:03:17,720 Speaker 3: no sort of lower size limit to them. You could 63 00:03:17,760 --> 00:03:20,520 Speaker 3: think of something a meter across, the size of a 64 00:03:20,600 --> 00:03:24,640 Speaker 3: chair as an asteroid, and that's not wrong. But if 65 00:03:24,639 --> 00:03:27,120 Speaker 3: it's the size of a grain of sand, I don't 66 00:03:27,160 --> 00:03:30,000 Speaker 3: know what you would call that necessarily a meteoroid, but 67 00:03:30,040 --> 00:03:31,919 Speaker 3: it's still kind of an asteroid. So that's what these 68 00:03:31,960 --> 00:03:34,720 Speaker 3: things are. You know. I wouldn't call something the size 69 00:03:34,720 --> 00:03:37,080 Speaker 3: of a grape an asteroid, but. 70 00:03:37,120 --> 00:03:39,240 Speaker 2: It kind of is kind of that's what happens. 71 00:03:39,280 --> 00:03:40,240 Speaker 3: You don't have a definition. 72 00:03:40,600 --> 00:03:42,960 Speaker 2: It's a like a vibe. You go in by vibes. 73 00:03:43,840 --> 00:03:48,000 Speaker 1: For the definition of asteroids, Yeah, yes, there is no 74 00:03:48,240 --> 00:03:52,080 Speaker 1: clear definition of what an asteroid is. I mean, it 75 00:03:52,160 --> 00:03:56,480 Speaker 1: basically means space rock, but not always. If the rock 76 00:03:56,560 --> 00:03:59,680 Speaker 1: is mostly made of ice, then astronomers call it a 77 00:04:00,680 --> 00:04:02,960 Speaker 1: or If the rocks are small enough, they call it 78 00:04:03,200 --> 00:04:05,480 Speaker 1: space dust. And if the rock is on t way 79 00:04:05,520 --> 00:04:09,000 Speaker 1: to Earth, they might call it a meteority. Now, the 80 00:04:09,040 --> 00:04:12,600 Speaker 1: size of asteroids vary according to what scientists call an 81 00:04:12,720 --> 00:04:16,640 Speaker 1: inverse law, meaning the bigger an asteroid is. 82 00:04:16,720 --> 00:04:18,040 Speaker 2: The rarer it is. 83 00:04:18,440 --> 00:04:23,400 Speaker 1: For example, really really big asteroids about one thousand kilometers wide. 84 00:04:23,600 --> 00:04:28,720 Speaker 1: There's one it's called series asteroids about one hundred or 85 00:04:28,760 --> 00:04:32,080 Speaker 1: more kilometers wide. There are about two hundred of them. 86 00:04:32,480 --> 00:04:35,719 Speaker 1: But smaller asteroids there are a lot. 87 00:04:37,320 --> 00:04:38,960 Speaker 3: As they get bigger, there are a fewer of them, 88 00:04:38,960 --> 00:04:41,080 Speaker 3: which is just kind of how nature operates. And it 89 00:04:41,080 --> 00:04:43,880 Speaker 3: turns out bigger than about one hundred meters you know, 90 00:04:44,080 --> 00:04:47,960 Speaker 3: football field sized. There are probably a billion of them 91 00:04:48,120 --> 00:04:51,640 Speaker 3: orbiting between Mars and Jupiter, which is a lot. But 92 00:04:52,200 --> 00:04:54,160 Speaker 3: if you say how many are bigger than a meter across. 93 00:04:54,320 --> 00:04:56,240 Speaker 3: I heave't no, it's hundreds of billions, trillions. I don't 94 00:04:56,240 --> 00:04:56,600 Speaker 3: even know. 95 00:04:58,080 --> 00:05:01,200 Speaker 1: There are a lot of asteroids out there. But before 96 00:05:01,200 --> 00:05:03,480 Speaker 1: you get the idea that space is full of rocks 97 00:05:03,520 --> 00:05:06,279 Speaker 1: flying all over the place, kind of like that asteroid 98 00:05:06,360 --> 00:05:09,760 Speaker 1: field and solo flu, the Millennium falcon through and the 99 00:05:09,760 --> 00:05:14,719 Speaker 1: Empire strikes back, you should know two things. First, space 100 00:05:15,160 --> 00:05:16,560 Speaker 1: is big. 101 00:05:17,960 --> 00:05:19,160 Speaker 3: And the thing is there are so many of them, 102 00:05:19,160 --> 00:05:21,680 Speaker 3: and you think, my heavens Empire strikes back. You know, 103 00:05:21,680 --> 00:05:23,599 Speaker 3: if I can quote what is now an. 104 00:05:23,440 --> 00:05:26,520 Speaker 2: Ancient movie, let's not get into how the artful. 105 00:05:27,000 --> 00:05:29,520 Speaker 3: Yeah, you have a space ship and it's going through 106 00:05:29,520 --> 00:05:31,599 Speaker 3: an asteroid belt and they're asteroids everywhere, and it's like, no, 107 00:05:31,640 --> 00:05:34,240 Speaker 3: it's not like that. In fact, when you look at 108 00:05:34,320 --> 00:05:37,000 Speaker 3: how much space is between Mars and Jupiter, and it's 109 00:05:37,160 --> 00:05:40,600 Speaker 3: you know, it's a several hundred million kilometers between them. 110 00:05:41,040 --> 00:05:43,520 Speaker 3: And a friend of mine who studies asteroids actually told 111 00:05:43,520 --> 00:05:45,400 Speaker 3: me this that if you take all of the one 112 00:05:45,480 --> 00:05:49,279 Speaker 3: hundred meter sized asteroids a hundred meters, you know, that's decent, 113 00:05:49,800 --> 00:05:52,320 Speaker 3: and you stand on one in the asteroid belt. If 114 00:05:52,320 --> 00:05:54,440 Speaker 3: you were to spread them out evenly, you would not 115 00:05:54,520 --> 00:05:58,200 Speaker 3: be able to see another asteroid with your naked eye. Whoa, 116 00:05:59,279 --> 00:06:01,400 Speaker 3: they would all be so far away they'd be too 117 00:06:01,400 --> 00:06:03,599 Speaker 3: faint to see. They're actually really far apart. 118 00:06:04,320 --> 00:06:07,240 Speaker 1: Wow, it's pretty rare in the Solar System. It seems 119 00:06:07,360 --> 00:06:08,719 Speaker 1: to run into one an asteroid. 120 00:06:08,880 --> 00:06:11,599 Speaker 3: Yeah, and it just depends on what you mean, right, Yeah, 121 00:06:11,640 --> 00:06:14,960 Speaker 3: there's zillions of them, so they're not rare, but they're 122 00:06:15,000 --> 00:06:17,559 Speaker 3: so few and far between because of the just vast 123 00:06:17,600 --> 00:06:21,280 Speaker 3: amount of space out there that you could go and 124 00:06:21,400 --> 00:06:24,200 Speaker 3: travel to Jupiter and back thousands of times and never 125 00:06:24,240 --> 00:06:25,640 Speaker 3: get even close enough to one to see. 126 00:06:26,720 --> 00:06:29,840 Speaker 1: So there are hundreds of millions of asteroids out there, 127 00:06:30,080 --> 00:06:33,559 Speaker 1: but space is so big you would rarely run into one, 128 00:06:33,880 --> 00:06:36,600 Speaker 1: even in the area of the Solar System called the 129 00:06:36,640 --> 00:06:39,880 Speaker 1: asteroid Belt. And the other thing is that even though 130 00:06:39,920 --> 00:06:43,400 Speaker 1: there are huge asteroids out there and hundreds of millions 131 00:06:43,480 --> 00:06:47,559 Speaker 1: of little asteroids, they actually don't add up too very much. 132 00:06:49,080 --> 00:06:51,480 Speaker 1: Do you have a sense of how much asteroid mass 133 00:06:51,600 --> 00:06:52,159 Speaker 1: is out there? 134 00:06:52,440 --> 00:06:55,600 Speaker 3: The weird thing is if you add them all up together, 135 00:06:56,000 --> 00:06:58,120 Speaker 3: you don't get a very big object. Even though there 136 00:06:58,120 --> 00:07:01,240 Speaker 3: could be a trillion little ones. The biggest ones really 137 00:07:01,480 --> 00:07:04,000 Speaker 3: eat up most of the space, and so you wind 138 00:07:04,120 --> 00:07:06,440 Speaker 3: up getting something that's actually quite small. It's just a 139 00:07:06,480 --> 00:07:10,440 Speaker 3: couple of thousand kilometers across what's smaller maybe than Earth's moon, 140 00:07:10,560 --> 00:07:13,000 Speaker 3: or maybe the size of Earth's moon, something like that. 141 00:07:13,200 --> 00:07:15,000 Speaker 3: Although there are lots of them, they don't add up 142 00:07:15,000 --> 00:07:15,560 Speaker 3: too much. 143 00:07:15,880 --> 00:07:18,400 Speaker 1: Interesting, and you're talking about all the asteroids in the 144 00:07:18,480 --> 00:07:19,800 Speaker 1: asteroid belt. 145 00:07:19,920 --> 00:07:23,080 Speaker 3: Yeah, and I could include the entire Solar System, although 146 00:07:23,320 --> 00:07:25,560 Speaker 3: it gets more complicated if you go out past Neptune. 147 00:07:25,560 --> 00:07:27,760 Speaker 3: There are these bodies out there that we call the 148 00:07:27,800 --> 00:07:31,320 Speaker 3: Kuiper Belt and the ort Cloud, which is comets. There 149 00:07:31,320 --> 00:07:34,520 Speaker 3: are objects that orbit the Sun beyond Neptune, and those 150 00:07:34,520 --> 00:07:36,880 Speaker 3: get pretty big. I mean, you're talking about Pluto. There 151 00:07:36,880 --> 00:07:39,960 Speaker 3: are probably a handful of objects roughly the size of Pluto, 152 00:07:40,320 --> 00:07:43,360 Speaker 3: and so these are actually decent size. Those would add up, oh, 153 00:07:43,400 --> 00:07:45,640 Speaker 3: I don't know, twice the volume, ten times the volume 154 00:07:45,640 --> 00:07:48,320 Speaker 3: of the Moon. So you're still not talking about a planet. 155 00:07:48,360 --> 00:07:52,520 Speaker 3: I don't think. You know, it's certainly not Jupiter or 156 00:07:52,560 --> 00:07:54,160 Speaker 3: that sort of thing. You've got a lot of these things, 157 00:07:54,200 --> 00:07:55,119 Speaker 3: but they're small. 158 00:07:55,360 --> 00:07:57,840 Speaker 1: Oh, that's fascinating. It doesn't seem like a lot. Yeah, 159 00:07:57,880 --> 00:08:02,679 Speaker 1: it's amazing, Okay, The last cool thing about asteroids before 160 00:08:02,680 --> 00:08:04,680 Speaker 1: we get to the questions of whether we should mind 161 00:08:04,720 --> 00:08:06,320 Speaker 1: them or whether one of them is going to hit 162 00:08:06,360 --> 00:08:09,360 Speaker 1: the Earth and kill us all, is that asteroids are 163 00:08:09,400 --> 00:08:12,520 Speaker 1: not as solid as some people would think. According to 164 00:08:12,600 --> 00:08:15,120 Speaker 1: doctor Plate, they can be kind of crumply. 165 00:08:16,640 --> 00:08:19,440 Speaker 3: Some of them are. And this gets weird. Oh, this 166 00:08:19,480 --> 00:08:22,240 Speaker 3: gets so weird. This is a relatively new concept. Are 167 00:08:22,280 --> 00:08:26,160 Speaker 3: there rubbel piles? So instead of being a solid object 168 00:08:26,200 --> 00:08:28,720 Speaker 3: like a rock in your backyard, a chunk of rock, 169 00:08:29,640 --> 00:08:34,079 Speaker 3: there are actually thousands or millions or billions of smaller rocks, 170 00:08:34,640 --> 00:08:37,080 Speaker 3: tiny ones up to maybe the size of boulders, that 171 00:08:37,160 --> 00:08:39,760 Speaker 3: are all held together by their very weak gravity. What 172 00:08:40,360 --> 00:08:42,680 Speaker 3: and so it's like having a bag of rocks, but 173 00:08:42,760 --> 00:08:45,520 Speaker 3: you remove the bag and what you're lift with is 174 00:08:45,559 --> 00:08:47,920 Speaker 3: just the gravity holding them together. And a lot of 175 00:08:47,960 --> 00:08:51,400 Speaker 3: the smaller ones, and we think the majority of smaller 176 00:08:51,480 --> 00:08:53,920 Speaker 3: asteroids are these rubble piles. So that's what they look like. 177 00:08:53,960 --> 00:08:56,160 Speaker 3: When you see pictures of them, you're like, yeah, that's 178 00:08:56,240 --> 00:08:58,880 Speaker 3: actually not a solid surface, that is just a bunch 179 00:08:58,960 --> 00:08:59,400 Speaker 3: of rocks. 180 00:09:00,760 --> 00:09:02,360 Speaker 2: Well, what was happened? If you went there and he 181 00:09:02,440 --> 00:09:04,599 Speaker 2: stood on this, would you think. 182 00:09:04,480 --> 00:09:07,559 Speaker 3: Well, that's a good question. The thing is, these rocks, 183 00:09:07,640 --> 00:09:11,160 Speaker 3: as we found, are very friable, which means they are 184 00:09:11,240 --> 00:09:13,800 Speaker 3: incredibly fragile, and if you were to hold one in 185 00:09:13,840 --> 00:09:17,040 Speaker 3: your hand, you could just crush it. There's very little 186 00:09:17,080 --> 00:09:20,240 Speaker 3: structural strength to these things, and we found that out 187 00:09:20,320 --> 00:09:22,840 Speaker 3: when a spacecraft, and I want to say it was 188 00:09:22,920 --> 00:09:25,760 Speaker 3: Osiris Rex, went up to the asteroid and hit it 189 00:09:25,800 --> 00:09:28,880 Speaker 3: at a very slow speed to collect material. It had 190 00:09:29,400 --> 00:09:32,080 Speaker 3: a sample collector, and the idea was that it would 191 00:09:32,080 --> 00:09:34,480 Speaker 3: go up to the asteroid and it would blow rocks 192 00:09:34,480 --> 00:09:37,440 Speaker 3: off and stuff and collect them into this collector. It 193 00:09:37,559 --> 00:09:42,160 Speaker 3: hit the asteroid and actually kept going. It penetrated down 194 00:09:42,640 --> 00:09:45,800 Speaker 3: about a half a meter into the asteroid itself, which 195 00:09:46,120 --> 00:09:48,800 Speaker 3: was a surprise, and they had to like break and 196 00:09:48,920 --> 00:09:50,880 Speaker 3: reverse thrust and get it back out of there. They 197 00:09:50,880 --> 00:09:52,640 Speaker 3: thought it might penetrate a little bit, but I think 198 00:09:52,640 --> 00:09:54,880 Speaker 3: they were surprised by how much. So, Yeah, if you 199 00:09:54,960 --> 00:09:57,000 Speaker 3: were to visit one of these things in a spaceship 200 00:09:57,480 --> 00:09:59,760 Speaker 3: and say I'm going to jump from my ship and 201 00:10:00,120 --> 00:10:03,040 Speaker 3: land on this asteroid feet first, you might just sink 202 00:10:03,440 --> 00:10:08,280 Speaker 3: right into it, which would be embarrassing and potentially life threatening, 203 00:10:09,480 --> 00:10:11,199 Speaker 3: So don't do it. 204 00:10:11,280 --> 00:10:13,280 Speaker 1: So what you say, at least a lot of the 205 00:10:13,480 --> 00:10:16,400 Speaker 1: what we think of as large ash asteroids out there 206 00:10:16,440 --> 00:10:18,679 Speaker 1: are actually just kind of like crumbly cookies. 207 00:10:19,200 --> 00:10:23,360 Speaker 3: Crumbly cookies, that's pretty good. It is true that a 208 00:10:23,360 --> 00:10:24,920 Speaker 3: lot of the ones that get in near Earth that 209 00:10:24,960 --> 00:10:28,600 Speaker 3: we have visited are like this. Some comets are like this. 210 00:10:29,000 --> 00:10:32,040 Speaker 3: I think this is not at all how I was 211 00:10:32,120 --> 00:10:33,640 Speaker 3: raised learning about asteroids. 212 00:10:33,720 --> 00:10:34,000 Speaker 2: Yeah. 213 00:10:34,160 --> 00:10:37,440 Speaker 1: Yeah, I feel like we've concluded that Star Wars has 214 00:10:37,760 --> 00:10:44,280 Speaker 1: misled us for years unbelievably. Yes, so it's hard to 215 00:10:44,360 --> 00:10:47,800 Speaker 1: run into an asteroid a large asteroid, and a lot 216 00:10:47,840 --> 00:10:50,280 Speaker 1: of them are not sort of big solid rocks, the 217 00:10:50,480 --> 00:10:52,000 Speaker 1: sort of crumbly cookies. 218 00:10:52,040 --> 00:10:54,800 Speaker 3: Basically, the force is not worth it. 219 00:10:56,480 --> 00:10:59,679 Speaker 1: Okay, so those are the basics of asteroids. Now I'll 220 00:10:59,679 --> 00:11:04,040 Speaker 1: get to the big questions. Should we mind the asteroid belt? 221 00:11:04,720 --> 00:11:08,480 Speaker 1: And is an asteroid gonna hit the Earth? It turns 222 00:11:08,480 --> 00:11:11,320 Speaker 1: out that the answer to both of these questions, according 223 00:11:11,360 --> 00:11:17,080 Speaker 1: to doctor Plate, is yes. When we come back, we're 224 00:11:17,080 --> 00:11:21,040 Speaker 1: gonna venture out even further to examine how asteroids can 225 00:11:21,120 --> 00:11:24,040 Speaker 1: kill us and how they can also save us. 226 00:11:24,559 --> 00:11:26,200 Speaker 2: To stay with us, we'll. 227 00:11:25,960 --> 00:11:46,240 Speaker 1: Be right back. Hey, we'll come back. We're talking about asteroids. 228 00:11:46,520 --> 00:11:49,040 Speaker 1: Whether we should mind them and if one of them 229 00:11:49,120 --> 00:11:51,120 Speaker 1: is going to hit the Earth and wipe us out. 230 00:11:52,600 --> 00:11:55,560 Speaker 1: So far, we've talked about what an asteroid actually is 231 00:11:56,080 --> 00:11:58,960 Speaker 1: and how many are out there now. Most of what 232 00:11:59,000 --> 00:12:02,480 Speaker 1: we call asteroids, meaning rocks floating in space, come from 233 00:12:02,520 --> 00:12:05,720 Speaker 1: the asteroid belt, which is the big ring between the 234 00:12:05,840 --> 00:12:08,880 Speaker 1: orbits of Mars and Jupiter. So if you were to 235 00:12:08,920 --> 00:12:11,840 Speaker 1: fly from Earth towards the edge of the Solar System, 236 00:12:12,000 --> 00:12:15,040 Speaker 1: you'd hit the orbit of Mars, then the asteroid belt, 237 00:12:15,320 --> 00:12:19,640 Speaker 1: then the orbit of Jupiter, Saturn, Urinus, and Neptune. And 238 00:12:19,800 --> 00:12:23,920 Speaker 1: the reason the asteroid belt is there is pretty cool. Basically, 239 00:12:24,120 --> 00:12:25,920 Speaker 1: you can blame Jupiter. 240 00:12:27,920 --> 00:12:31,880 Speaker 3: So the early Solar System was the Sun, the young Sun, 241 00:12:31,960 --> 00:12:35,120 Speaker 3: surrounded by this disk of material that's gas and dust 242 00:12:35,200 --> 00:12:38,440 Speaker 3: and rock and stuff like that. These things started to accumulate. 243 00:12:38,679 --> 00:12:40,880 Speaker 3: Grains would bump into each other and turn into pebbles. 244 00:12:40,880 --> 00:12:43,800 Speaker 3: Pebbles bump into each other, turn into boulders, and eventually 245 00:12:43,840 --> 00:12:46,040 Speaker 3: you would grow to get something like a planet. That's 246 00:12:46,040 --> 00:12:50,040 Speaker 3: how our planets formed. But between Mars and Jupiter, Jupiter's 247 00:12:50,080 --> 00:12:52,679 Speaker 3: gravity is very strong, and so any sort of object 248 00:12:52,720 --> 00:12:54,880 Speaker 3: that would try to get big enough to form a planet. 249 00:12:55,240 --> 00:12:57,760 Speaker 3: Jupiter's gravity would kind of swing it around, make it 250 00:12:57,800 --> 00:13:00,960 Speaker 3: move faster, slam into other stuff in the asteroid belt, 251 00:13:01,000 --> 00:13:01,559 Speaker 3: shatter it. 252 00:13:02,400 --> 00:13:06,080 Speaker 1: So basically, the asteroid belt is the graveyard of the 253 00:13:06,160 --> 00:13:10,680 Speaker 1: chaos caused by the huge gravity of Jupiter. Any planets 254 00:13:10,679 --> 00:13:13,199 Speaker 1: that try to form there would get dragged by Jupiter 255 00:13:13,400 --> 00:13:15,679 Speaker 1: and slammed into other rocks. 256 00:13:16,000 --> 00:13:18,400 Speaker 2: And as we mentioned before, there are a lot. 257 00:13:18,240 --> 00:13:21,920 Speaker 1: Of rocks in the asteroid belt, and sometimes those rocks 258 00:13:21,920 --> 00:13:24,880 Speaker 1: can bump into each other and get nudge to fall 259 00:13:25,040 --> 00:13:28,600 Speaker 1: in our direction, which raises the possibility that one of 260 00:13:28,640 --> 00:13:32,120 Speaker 1: them could hit us. It wouldn't be the first time. 261 00:13:32,679 --> 00:13:37,040 Speaker 1: Sixty five million years ago, an asteroid called the Chicchulub impactor, 262 00:13:37,280 --> 00:13:40,520 Speaker 1: which was about fourteen kilometers wide, hit the Earth and 263 00:13:40,640 --> 00:13:43,840 Speaker 1: caused so much mayhem that it killed fifty percent of 264 00:13:43,880 --> 00:13:47,120 Speaker 1: all species on Earth, including the dinosaurs. 265 00:13:48,440 --> 00:13:49,400 Speaker 2: Could it happen again? 266 00:13:50,080 --> 00:13:54,720 Speaker 1: That was the next question I asked, Doctor Blade, Doctor Plade, 267 00:13:54,760 --> 00:13:56,600 Speaker 1: is an asteroid going to hit the Earth? What's the 268 00:13:56,720 --> 00:13:59,319 Speaker 1: likelihood of that happening? One hundred percent? 269 00:14:00,000 --> 00:14:02,640 Speaker 3: One hitting us right now as we're talking? What there 270 00:14:02,640 --> 00:14:05,040 Speaker 3: are thousands of hitting us right now? Well, I said, 271 00:14:05,040 --> 00:14:07,240 Speaker 3: there's no lower limit to the size of an asteroid. Right, 272 00:14:07,280 --> 00:14:09,800 Speaker 3: So if you consider something like a grain of sand 273 00:14:10,000 --> 00:14:13,720 Speaker 3: an asteroid, there are fifty to one hundred tons of 274 00:14:13,800 --> 00:14:17,520 Speaker 3: material that hits Earth every day. What so, zillions of 275 00:14:17,520 --> 00:14:19,240 Speaker 3: these things are hitting Earth all the time, and you 276 00:14:19,240 --> 00:14:22,200 Speaker 3: see them burning up as meteors shooting stars. If you 277 00:14:22,240 --> 00:14:24,840 Speaker 3: call those asteroids, then we're getting hit all the time. 278 00:14:25,040 --> 00:14:30,040 Speaker 3: If you say, oh, let's say something that's a meter across, 279 00:14:30,120 --> 00:14:32,320 Speaker 3: then we get hit by something that size once a month, 280 00:14:32,680 --> 00:14:36,600 Speaker 3: as we're speaking. One fell over Europe a few days ago, 281 00:14:36,760 --> 00:14:39,320 Speaker 3: and a couple of nights ago, one came over Ohio 282 00:14:39,360 --> 00:14:41,680 Speaker 3: and Pennsylvania was seen by thousands of people. 283 00:14:41,760 --> 00:14:43,880 Speaker 2: You heard about that, Yeah, I saw the needs. 284 00:14:44,000 --> 00:14:46,240 Speaker 3: Yeah, it was really bright. Yeah, I've seen the videos. 285 00:14:46,280 --> 00:14:49,480 Speaker 3: It's pretty cool. We get hit by those on timescales 286 00:14:49,480 --> 00:14:51,680 Speaker 3: of a month or so, and the bigger they are, 287 00:14:51,720 --> 00:14:52,680 Speaker 3: the more rare they are. 288 00:14:53,560 --> 00:14:55,680 Speaker 1: What picker Plate is saying is that just like the 289 00:14:55,720 --> 00:14:59,080 Speaker 1: sizes of asteroids out in space, follow an inverse law, 290 00:14:59,480 --> 00:15:02,040 Speaker 1: so that the asteroids that happened to hit the Earth, 291 00:15:02,680 --> 00:15:05,520 Speaker 1: small asteroids hit Earth all the time, but as they 292 00:15:05,520 --> 00:15:09,520 Speaker 1: get bigger, they get rarer and rarer. One of the 293 00:15:09,560 --> 00:15:12,000 Speaker 1: biggest ones to hit US in recent years with the 294 00:15:12,160 --> 00:15:16,080 Speaker 1: Cheliabinsk meteor event, which you can find video of if 295 00:15:16,120 --> 00:15:17,600 Speaker 1: you search for it online. 296 00:15:18,120 --> 00:15:31,920 Speaker 3: Actually, so when you talk about something like the chel 297 00:15:31,960 --> 00:15:36,360 Speaker 3: Yabinsk impact, which was in Russia in twenty thirteen, that 298 00:15:36,560 --> 00:15:38,800 Speaker 3: was nineteen meters across, so you're talking to something the 299 00:15:38,880 --> 00:15:41,400 Speaker 3: size of a house, big house. Those are much more rare. 300 00:15:41,440 --> 00:15:45,160 Speaker 3: Those you're talking about every few decades or century. If 301 00:15:45,160 --> 00:15:47,880 Speaker 3: one is fifty meters across and gets closer than that, 302 00:15:48,120 --> 00:15:50,760 Speaker 3: it's not great. You don't want that, but it's not 303 00:15:50,920 --> 00:15:54,480 Speaker 3: classified as potentially hazardous. It's still if it hits Earth, 304 00:15:54,520 --> 00:15:56,360 Speaker 3: it'll blow up like a nuclear weapon. I mean, you're 305 00:15:56,360 --> 00:15:59,960 Speaker 3: still talking about a megaton or more explosion. That's bad, 306 00:16:00,680 --> 00:16:02,440 Speaker 3: but it's not a global catastrophe. 307 00:16:02,680 --> 00:16:05,600 Speaker 1: Okay, but at around one hundred and footy meters that 308 00:16:05,640 --> 00:16:07,880 Speaker 1: could be a global catastrophe, Yeah. 309 00:16:07,840 --> 00:16:09,880 Speaker 3: I think regional. So you're talking about if one hit 310 00:16:09,920 --> 00:16:12,120 Speaker 3: in the middle of the US, it would be catastrophic 311 00:16:12,160 --> 00:16:15,280 Speaker 3: for US, but not necessarily for you know, India or 312 00:16:15,280 --> 00:16:18,840 Speaker 3: something like that, although it's not great and certainly economically 313 00:16:18,920 --> 00:16:21,479 Speaker 3: you know, if you hit a country that is economically 314 00:16:21,520 --> 00:16:22,880 Speaker 3: critical to the rest of the world. 315 00:16:23,200 --> 00:16:23,840 Speaker 2: That's bad. 316 00:16:23,920 --> 00:16:26,320 Speaker 3: I mean, we saw what happened when like a terrorist 317 00:16:26,360 --> 00:16:28,720 Speaker 3: attack can cripple the economy of a country and bring 318 00:16:28,720 --> 00:16:31,280 Speaker 3: about a global recession. So you don't want these things 319 00:16:31,360 --> 00:16:35,480 Speaker 3: hitting over New York City, Moscow, you know, anything like that. 320 00:16:35,480 --> 00:16:36,720 Speaker 3: That would be very, very bad. 321 00:16:37,440 --> 00:16:39,640 Speaker 1: So's if a one hundred footy meter asteroids hit is 322 00:16:39,880 --> 00:16:41,920 Speaker 1: it would be about how many nuclear weapons? 323 00:16:42,080 --> 00:16:47,800 Speaker 3: Oh golly, so something like two hundred megatons, so multiple 324 00:16:47,880 --> 00:16:52,560 Speaker 3: times the largest nuclear weapon ever dropped. But it's not radioactive, 325 00:16:52,600 --> 00:16:56,680 Speaker 3: so at least you know, yay, no fallout. Hooray. 326 00:16:57,000 --> 00:17:00,800 Speaker 2: It's still bad, Okay, quick recap here. 327 00:17:00,960 --> 00:17:04,480 Speaker 1: Earth is hit by asteroids all the time, but most 328 00:17:04,480 --> 00:17:07,280 Speaker 1: of the time they're small and they end up burning 329 00:17:07,359 --> 00:17:09,920 Speaker 1: up when they hit all that air in the atmosphere. 330 00:17:10,240 --> 00:17:13,440 Speaker 1: That's what a shooting star is. When the asteroids start 331 00:17:13,480 --> 00:17:16,400 Speaker 1: getting about fifty to one hundred and forty meters wide, 332 00:17:16,640 --> 00:17:19,440 Speaker 1: that's when they can do a lot of damage. 333 00:17:19,560 --> 00:17:20,520 Speaker 2: They could wipe by. 334 00:17:20,400 --> 00:17:23,520 Speaker 1: The city and maybe cause a global crisis, but it 335 00:17:23,560 --> 00:17:27,520 Speaker 1: wouldn't end the human race. And luckily that size of 336 00:17:27,560 --> 00:17:32,200 Speaker 1: asteroid only hits Earth statistically every one hundred years or so. 337 00:17:32,280 --> 00:17:34,800 Speaker 1: Now you might be wondering, what about the big ones, 338 00:17:35,040 --> 00:17:37,280 Speaker 1: you know, like the one that took out the dinosaurs, 339 00:17:37,280 --> 00:17:39,640 Speaker 1: that are like several kilometers wide. 340 00:17:40,000 --> 00:17:41,960 Speaker 2: Those would be really bad. 341 00:17:42,520 --> 00:17:46,240 Speaker 1: But actually scientists are not too worried about those because 342 00:17:46,400 --> 00:17:49,960 Speaker 1: remember the inverse law of asteroids says, there aren't that 343 00:17:50,040 --> 00:17:51,359 Speaker 1: many of them out there. 344 00:17:53,760 --> 00:17:56,320 Speaker 3: We know there are no large asteroids big enough to 345 00:17:56,359 --> 00:18:00,600 Speaker 3: be catastrophic globally, like an extinction level event. There's none 346 00:18:01,040 --> 00:18:03,400 Speaker 3: that can get near us for at least the next century. 347 00:18:03,480 --> 00:18:05,240 Speaker 3: It just gets hard to predict farther in the future 348 00:18:05,240 --> 00:18:07,880 Speaker 3: because we don't know their orbits perfectly. But you know, 349 00:18:08,160 --> 00:18:10,680 Speaker 3: something that's a global like like out of a movie 350 00:18:10,800 --> 00:18:12,960 Speaker 3: armagedd and deep impact, something like that. If you remember 351 00:18:12,960 --> 00:18:17,040 Speaker 3: those movies from thirty years ago, Now those are extraordinarily rare. 352 00:18:17,080 --> 00:18:20,280 Speaker 3: Those are like every you know, tens of millions of years, 353 00:18:20,320 --> 00:18:22,640 Speaker 3: like dinosaur killer impacts. Those are extremely rare. 354 00:18:23,840 --> 00:18:26,960 Speaker 1: And in fact, there is an office at NASA called 355 00:18:27,119 --> 00:18:30,760 Speaker 1: the Center for Near Earth Object Studies where the main 356 00:18:30,840 --> 00:18:33,480 Speaker 1: job of the scientists there is to keep track of 357 00:18:33,480 --> 00:18:36,080 Speaker 1: all the big asteroids in the Solar System and make 358 00:18:36,119 --> 00:18:38,960 Speaker 1: sure we're not in a collision course with them. And 359 00:18:39,000 --> 00:18:40,600 Speaker 1: according to their calculations. 360 00:18:40,760 --> 00:18:43,200 Speaker 2: We're good for now. 361 00:18:43,720 --> 00:18:48,280 Speaker 1: Now, does that mean we're totally safe? Not quite. Remember, 362 00:18:48,600 --> 00:18:51,440 Speaker 1: those smaller asteroids in the fifty to a few hundred 363 00:18:51,520 --> 00:18:54,600 Speaker 1: meters wide range can still come out of nowhere and 364 00:18:54,640 --> 00:18:57,320 Speaker 1: do a lot of damage. But there is good news. 365 00:18:57,440 --> 00:19:01,720 Speaker 1: According to doctor Plate, the good. 366 00:19:01,560 --> 00:19:03,440 Speaker 3: News is we can do something about them. The first 367 00:19:03,440 --> 00:19:04,800 Speaker 3: thing we have to do is find them, and we 368 00:19:04,880 --> 00:19:08,880 Speaker 3: are building observatories now. The Vera Ruben Observatory takes huge 369 00:19:08,920 --> 00:19:11,280 Speaker 3: images of the sky and looks for things that change 370 00:19:11,320 --> 00:19:13,280 Speaker 3: from night to night. So an asteroid is, you know, 371 00:19:13,400 --> 00:19:14,840 Speaker 3: in one spot, and the next night it's in the 372 00:19:14,880 --> 00:19:17,400 Speaker 3: next spot. Reuben will see it. And in its first 373 00:19:17,520 --> 00:19:20,800 Speaker 3: night it observed two thousand asteroids and so it's going 374 00:19:20,840 --> 00:19:22,480 Speaker 3: to do this every night. So it's going to map 375 00:19:22,520 --> 00:19:25,439 Speaker 3: out zillions of these things, and that's good because you 376 00:19:25,440 --> 00:19:27,439 Speaker 3: want to know if one's coming toward us, or if 377 00:19:27,480 --> 00:19:29,360 Speaker 3: it's orbit it's going to intersect ours in twenty years 378 00:19:29,440 --> 00:19:31,440 Speaker 3: or something like that. Next thing you have to do 379 00:19:31,720 --> 00:19:33,560 Speaker 3: is push it out of the way. You know, you 380 00:19:33,600 --> 00:19:37,280 Speaker 3: don't necessarily want a nuke it because that's illegal and 381 00:19:37,359 --> 00:19:40,920 Speaker 3: that may not do the trick. Well, is it illegal, Yeah, 382 00:19:40,960 --> 00:19:43,679 Speaker 3: it's actually, the Outer Space Treaty, which was signed by 383 00:19:43,680 --> 00:19:46,480 Speaker 3: a lot of nations in the sixties, makes it illegal 384 00:19:46,520 --> 00:19:50,159 Speaker 3: to test nuclear weapons or detonate them in space, but 385 00:19:50,440 --> 00:19:52,359 Speaker 3: in general, like blowing up a nuke and space is 386 00:19:52,359 --> 00:19:54,920 Speaker 3: illegal and it's a bad idea. But on the other hand, 387 00:19:55,040 --> 00:19:58,520 Speaker 3: NASA has just tested a few years ago in twenty two, 388 00:19:58,640 --> 00:20:03,040 Speaker 3: twenty twenty two, to spacecraft into an asteroid. Ditamos was 389 00:20:03,080 --> 00:20:05,439 Speaker 3: the name of the asteroid, a few hundred meters across. 390 00:20:05,440 --> 00:20:08,480 Speaker 3: It has a moon called Dimorphos, which is one hundred 391 00:20:08,520 --> 00:20:12,639 Speaker 3: and seventy meters across, and they slammed this dishwasher size 392 00:20:12,680 --> 00:20:16,040 Speaker 3: spacecraft into it called DART, which was the Double Asteroid 393 00:20:16,119 --> 00:20:19,920 Speaker 3: Redirection Test DART. DART. It hit the Moon at high 394 00:20:19,960 --> 00:20:23,720 Speaker 3: speed and the idea was the impact would change the 395 00:20:23,880 --> 00:20:26,040 Speaker 3: orbit of the Moon. And then this thing hit it 396 00:20:26,200 --> 00:20:28,800 Speaker 3: and the period of that object changed by half an hour, 397 00:20:29,280 --> 00:20:32,760 Speaker 3: which means we significantly changed the orbit of that asteroid. 398 00:20:32,800 --> 00:20:35,560 Speaker 3: And that's good because that means that if you have 399 00:20:35,720 --> 00:20:38,920 Speaker 3: enough time, like ten years lead time, you can build 400 00:20:38,960 --> 00:20:41,639 Speaker 3: a rocket, send a probe to it, slam it, and 401 00:20:41,680 --> 00:20:43,760 Speaker 3: then hopefully move it enough that over the next few 402 00:20:43,840 --> 00:20:46,600 Speaker 3: years you've pushed its orbit enough that it misses the 403 00:20:46,640 --> 00:20:51,199 Speaker 3: Earth with a dishwasher something like that. So really the 404 00:20:51,320 --> 00:20:54,560 Speaker 3: key here, the absolute key here, is finding them early. 405 00:20:55,000 --> 00:20:57,800 Speaker 3: And if you have twenty years before you think this 406 00:20:57,800 --> 00:21:00,280 Speaker 3: thing's going to hit us, that is plenty of time 407 00:21:00,320 --> 00:21:02,040 Speaker 3: to get to work and try to do something about 408 00:21:02,040 --> 00:21:03,320 Speaker 3: getting it to move out of the way. 409 00:21:03,640 --> 00:21:06,640 Speaker 2: So we do have a system in case that happens. 410 00:21:06,760 --> 00:21:09,160 Speaker 3: Oh, I don't know if I'd glorify it by calling 411 00:21:09,200 --> 00:21:13,120 Speaker 3: it a system. We have rockets and we've done this. 412 00:21:13,280 --> 00:21:15,919 Speaker 3: We hit an asteroid in two thousand and five. There 413 00:21:15,960 --> 00:21:18,280 Speaker 3: was a mission called Deep Impact and that hit an 414 00:21:18,320 --> 00:21:20,960 Speaker 3: asteroid to see what would happen. And then we hit 415 00:21:21,240 --> 00:21:24,639 Speaker 3: dimorphos a few years ago, and that's really it. But 416 00:21:24,680 --> 00:21:27,439 Speaker 3: we're getting better at this all the time. In thirty years, 417 00:21:27,480 --> 00:21:29,919 Speaker 3: hopefully we'll have learned enough about how to do this 418 00:21:30,280 --> 00:21:32,439 Speaker 3: that if anything's coming our way, we'll be able to 419 00:21:32,680 --> 00:21:35,159 Speaker 3: whack it and stop it. You're not trying to shatter 420 00:21:35,160 --> 00:21:38,200 Speaker 3: it necessarily, you're just trying to change its trajectory. 421 00:21:38,440 --> 00:21:39,120 Speaker 2: I see, I see. 422 00:21:39,119 --> 00:21:41,080 Speaker 1: You don't want to stop the asteroid. You just wind 423 00:21:41,160 --> 00:21:42,520 Speaker 1: to nudget out of the way. 424 00:21:42,720 --> 00:21:45,320 Speaker 3: Yeah, gently persuade it maybe you should go. 425 00:21:45,359 --> 00:21:48,840 Speaker 1: Over there hit Mars part is looking pretty good. Yeah, 426 00:21:48,880 --> 00:21:50,800 Speaker 1: but I guess the take home message is that we 427 00:21:50,920 --> 00:21:54,560 Speaker 1: have the ability and we have actually hit an asteroid 428 00:21:54,640 --> 00:21:57,320 Speaker 1: that was out there flying and been able to just 429 00:21:57,440 --> 00:21:58,399 Speaker 1: its trajectory. 430 00:21:58,640 --> 00:21:58,960 Speaker 2: Yeah. 431 00:21:59,119 --> 00:22:02,120 Speaker 3: I mean, that's great, fantastic news. I was really excited 432 00:22:02,119 --> 00:22:05,280 Speaker 3: and I'll tell you relieved in that mission work when 433 00:22:05,320 --> 00:22:06,920 Speaker 3: dart work, because it shows we can do it. 434 00:22:07,160 --> 00:22:08,480 Speaker 2: Oh, fascinating. 435 00:22:08,760 --> 00:22:11,000 Speaker 3: Yeah, it's just all relatively new knowledge. It's pretty cool. 436 00:22:12,920 --> 00:22:13,240 Speaker 2: Okay. 437 00:22:13,560 --> 00:22:15,760 Speaker 1: Few for those of you worried we were going to 438 00:22:15,840 --> 00:22:18,639 Speaker 1: go extinct because of an asteroid hitting us, you can 439 00:22:18,720 --> 00:22:22,000 Speaker 1: rest a little easier knowing that NASA has our backs 440 00:22:22,440 --> 00:22:27,200 Speaker 1: at least against asteroids now, assuming something else doesn't do us, 441 00:22:27,240 --> 00:22:30,160 Speaker 1: and then the big question becomes, how do we survive 442 00:22:30,600 --> 00:22:33,640 Speaker 1: in the long term. It's possible that in the future 443 00:22:33,840 --> 00:22:36,000 Speaker 1: we might run out of resource this year on Earth, 444 00:22:36,440 --> 00:22:40,320 Speaker 1: and in that case, maybe asteroids can save us. There 445 00:22:40,359 --> 00:22:43,159 Speaker 1: are a ton of asteroids out there, but things that 446 00:22:43,200 --> 00:22:46,119 Speaker 1: we could potentially mine to bring back to Earth. 447 00:22:46,560 --> 00:22:47,720 Speaker 2: But is that really feasible? 448 00:22:48,080 --> 00:22:51,960 Speaker 1: Can we or should we mine the asteroid belt while 449 00:22:52,000 --> 00:22:54,680 Speaker 1: we come back. I'll ask doctor Plate this question, and 450 00:22:54,920 --> 00:22:57,600 Speaker 1: I think you might be surprised by the answer, so 451 00:22:57,760 --> 00:23:19,560 Speaker 1: stay with us. We'll be right back. Hey, welcome back. 452 00:23:20,280 --> 00:23:23,920 Speaker 1: We're talking about asteroids and pew. So far, we've learned 453 00:23:23,920 --> 00:23:26,919 Speaker 1: that while the Earth is getting hit by small asteroids 454 00:23:26,920 --> 00:23:30,159 Speaker 1: all the time, the likelihood of a big one coming 455 00:23:30,240 --> 00:23:34,080 Speaker 1: and ending the human race anytime soon is fairly small. 456 00:23:34,680 --> 00:23:37,639 Speaker 1: NASA and other space agencies around the world are keeping 457 00:23:37,680 --> 00:23:40,359 Speaker 1: track of all the big asteroids in our Solar system, 458 00:23:40,640 --> 00:23:43,240 Speaker 1: and even if a medium size one comes our way, 459 00:23:43,560 --> 00:23:48,560 Speaker 1: we are getting better at reaching them and deflecting them. Now, 460 00:23:48,600 --> 00:23:52,199 Speaker 1: the question is good asteroids actually be good for us? 461 00:23:52,560 --> 00:23:54,959 Speaker 1: A lot of people have noticed that asteroids in the 462 00:23:55,000 --> 00:23:58,280 Speaker 1: asteroid belt are full of materials that we meet here 463 00:23:58,320 --> 00:24:01,040 Speaker 1: on Earth, and so a possible is for us to 464 00:24:01,119 --> 00:24:05,359 Speaker 1: go out there and mine them. But is that a 465 00:24:05,400 --> 00:24:08,520 Speaker 1: good idea? Should we send a spacecraft out there to 466 00:24:08,640 --> 00:24:11,679 Speaker 1: check out the metals and minerals and those floating space rocks. 467 00:24:12,400 --> 00:24:15,199 Speaker 1: Actually it furs out we already have. 468 00:24:17,840 --> 00:24:21,119 Speaker 3: There's a current mission NASA launched called Psyche, which is 469 00:24:21,119 --> 00:24:24,080 Speaker 3: on its way. The asteroid's name is Psyche. It's this 470 00:24:24,200 --> 00:24:26,520 Speaker 3: big asteroid. It's one of the biggest ones, and we 471 00:24:26,560 --> 00:24:29,119 Speaker 3: think it's mostly metal. And when we say metal, we 472 00:24:29,200 --> 00:24:33,520 Speaker 3: mean iron, nickel, and mostly silicon, and then a lot 473 00:24:33,520 --> 00:24:38,240 Speaker 3: of lesser ones titanium, tungsten, aluminum, Platinum, for example, is 474 00:24:38,359 --> 00:24:40,560 Speaker 3: very valuable on Earth and it's used in electronics. It's 475 00:24:40,680 --> 00:24:43,000 Speaker 3: very important metal for a lot of reasons. Palladium is 476 00:24:43,000 --> 00:24:46,680 Speaker 3: another one. And it's not like these are abundant in asteroids, 477 00:24:46,680 --> 00:24:48,320 Speaker 3: but they are out there. And so if you could 478 00:24:48,320 --> 00:24:51,840 Speaker 3: take an asteroid and grind it up and extract these metals, 479 00:24:52,359 --> 00:24:53,840 Speaker 3: you could then sell them on Earth and make a 480 00:24:53,840 --> 00:24:54,919 Speaker 3: lot of money. 481 00:24:56,240 --> 00:24:59,960 Speaker 1: Yes, you could technically mine asteroids and bring back their 482 00:25:00,160 --> 00:25:02,720 Speaker 1: precious metals and sell them for a lot of money. 483 00:25:03,240 --> 00:25:04,840 Speaker 2: So why don't we do it? 484 00:25:05,359 --> 00:25:08,399 Speaker 1: I mean, sending a spacecraft to an asteroid is hard, 485 00:25:08,600 --> 00:25:11,800 Speaker 1: but we've done it before. In fact, we've managed to 486 00:25:11,800 --> 00:25:15,399 Speaker 1: get to flying asteroids several times. In the nineteen eighties, 487 00:25:15,560 --> 00:25:19,199 Speaker 1: we sent fly spacecraft from three space agencies around the 488 00:25:19,200 --> 00:25:22,359 Speaker 1: world to get a close look at hay Least comment. 489 00:25:23,080 --> 00:25:25,840 Speaker 1: Since then, there have been about a dozen more missions 490 00:25:25,880 --> 00:25:29,080 Speaker 1: that were sent to either fly by or actually land 491 00:25:29,240 --> 00:25:30,960 Speaker 1: on comets or asteroids. 492 00:25:31,400 --> 00:25:32,120 Speaker 2: But here's the thing. 493 00:25:32,520 --> 00:25:35,240 Speaker 1: Getting to an asteroid to mine it is not the 494 00:25:35,280 --> 00:25:41,160 Speaker 1: main problem. The real problem is bringing back what you mind. 495 00:25:42,480 --> 00:25:44,719 Speaker 3: The big step is you then bring these things back 496 00:25:44,720 --> 00:25:47,520 Speaker 3: to Earth. But bring it back to Earth it's not straightforward. 497 00:25:47,720 --> 00:25:50,199 Speaker 3: You have something that's moving eight kilometers a second. If 498 00:25:50,240 --> 00:25:52,080 Speaker 3: it's coming from deep space, it could be doing twice 499 00:25:52,119 --> 00:25:54,760 Speaker 3: that fast. You have to slow this thing down and 500 00:25:54,800 --> 00:25:57,040 Speaker 3: then somehow get it to the surface of the Earth 501 00:25:57,480 --> 00:26:00,399 Speaker 3: in quantities that are usable. Right, if I'd drop a 502 00:26:00,440 --> 00:26:02,600 Speaker 3: pound of platinum on the Earth, that's not really going 503 00:26:02,680 --> 00:26:04,480 Speaker 3: to help. And you can just drop that from orbit, 504 00:26:04,560 --> 00:26:06,399 Speaker 3: let it hit. It'll actually lose a lot of it. 505 00:26:06,440 --> 00:26:09,440 Speaker 3: You could encase it in concrete or something whatever, let 506 00:26:09,440 --> 00:26:12,040 Speaker 3: that burn off as it goes through the atmosphere. But now, 507 00:26:12,080 --> 00:26:14,480 Speaker 3: if you're talking about one hundred tons of something, how 508 00:26:14,480 --> 00:26:15,640 Speaker 3: do you get that to the surface. 509 00:26:16,080 --> 00:26:20,240 Speaker 1: That's hard without basically creating a giant asteroid that will 510 00:26:20,320 --> 00:26:21,280 Speaker 1: kill people on Earth. 511 00:26:21,400 --> 00:26:26,520 Speaker 3: Yeah, you could build some sort of machinery that would 512 00:26:26,560 --> 00:26:28,320 Speaker 3: slow these things down and drop them for more of it, 513 00:26:28,400 --> 00:26:30,920 Speaker 3: but that's also very expensive, and to do this at 514 00:26:30,960 --> 00:26:34,320 Speaker 3: scale where you're talking about you know, a building weighs 515 00:26:34,680 --> 00:26:37,440 Speaker 3: tens of thousands of tons, so you need a lot 516 00:26:37,480 --> 00:26:40,480 Speaker 3: of this material to build a rocket or to provide 517 00:26:40,520 --> 00:26:43,760 Speaker 3: for the electronics industry or whatever. And right now it's 518 00:26:43,800 --> 00:26:47,159 Speaker 3: just cheaper to keep doing this on Earth. Some day 519 00:26:47,200 --> 00:26:48,720 Speaker 3: it might be easier to do this. We're just not 520 00:26:48,800 --> 00:26:50,159 Speaker 3: there yet. 521 00:26:51,280 --> 00:26:51,800 Speaker 2: That's right. 522 00:26:51,960 --> 00:26:56,159 Speaker 1: Getting things from space to Earth is hard, or at 523 00:26:56,240 --> 00:26:58,800 Speaker 1: least it's easy. But the hard part is having what 524 00:26:58,920 --> 00:27:02,480 Speaker 1: did drop from faith Land in one piece. And even 525 00:27:02,520 --> 00:27:04,800 Speaker 1: if you do manage to figure out how to, say, 526 00:27:04,920 --> 00:27:07,879 Speaker 1: bring all those precious metals from asteroids to Earth, there 527 00:27:07,960 --> 00:27:11,280 Speaker 1: could be other things that can happen that you didn't expect. 528 00:27:12,320 --> 00:27:14,200 Speaker 3: There are other problems like crashing the market if you 529 00:27:14,240 --> 00:27:17,399 Speaker 3: suddenly introduce a vast amount of material into the market. 530 00:27:17,440 --> 00:27:19,520 Speaker 3: You know, the reason these things are expensive is because 531 00:27:19,560 --> 00:27:21,880 Speaker 3: they are rare, and if you bring in a lot, 532 00:27:22,119 --> 00:27:23,679 Speaker 3: there's more than one hundred tons of gold out there, 533 00:27:23,680 --> 00:27:25,080 Speaker 3: but if you bring in a lot, it could actually 534 00:27:25,160 --> 00:27:28,359 Speaker 3: damage the market. This, I can't stress this enough, is 535 00:27:28,760 --> 00:27:32,280 Speaker 3: super super hard to do. We do not have the 536 00:27:32,320 --> 00:27:35,719 Speaker 3: technology in place to do this. We have the technology 537 00:27:35,880 --> 00:27:38,400 Speaker 3: where we can start looking at it and investigating it 538 00:27:38,720 --> 00:27:41,280 Speaker 3: and doing this step by step. But right now, if 539 00:27:41,320 --> 00:27:44,920 Speaker 3: you wanted to mine an asteroid, I think you're looking decades. 540 00:27:45,080 --> 00:27:47,720 Speaker 3: I don't know how many to at least, but it's 541 00:27:47,760 --> 00:27:49,280 Speaker 3: going to be a while. I may be wrong. 542 00:27:50,200 --> 00:27:53,600 Speaker 1: So mining the asteroid belt for materials to bring back 543 00:27:53,640 --> 00:27:57,480 Speaker 1: to birth is a bit of a hard sell. Or 544 00:27:57,600 --> 00:28:01,240 Speaker 1: at least, you'd have to be really, really really desperate 545 00:28:01,520 --> 00:28:04,080 Speaker 1: to make it worth all that money and development and 546 00:28:04,160 --> 00:28:07,480 Speaker 1: risk to do it. But according to doctor Playd, there 547 00:28:07,560 --> 00:28:10,359 Speaker 1: is one other reason we might want to mine the 548 00:28:10,480 --> 00:28:14,040 Speaker 1: asteroid belt that is not about bringing stuff back to Earth, 549 00:28:14,640 --> 00:28:17,600 Speaker 1: and that is for space exploration. 550 00:28:20,080 --> 00:28:21,800 Speaker 3: If we want to build a space station on Earth, 551 00:28:21,880 --> 00:28:23,800 Speaker 3: we have to build it down here, all the pieces, 552 00:28:23,960 --> 00:28:26,840 Speaker 3: and then launch each piece into space and put it together. 553 00:28:27,240 --> 00:28:28,920 Speaker 3: And that takes a long time. It costs a lot 554 00:28:28,920 --> 00:28:31,240 Speaker 3: of money. The space station International Space Station was one 555 00:28:31,280 --> 00:28:34,680 Speaker 3: hundred billion dollars and took ten years to complete. Something 556 00:28:34,720 --> 00:28:37,880 Speaker 3: like that. The rocket launches are expensive. Takes a lot 557 00:28:37,880 --> 00:28:40,240 Speaker 3: of energy to move those things out of Earth's gravity 558 00:28:40,280 --> 00:28:44,120 Speaker 3: into orbit or off the surface. If you mind an asteroid, 559 00:28:44,640 --> 00:28:47,800 Speaker 3: it's out there in space already. Oh and if you 560 00:28:47,880 --> 00:28:50,640 Speaker 3: can figure out a way of processing it, smelting it 561 00:28:50,880 --> 00:28:52,320 Speaker 3: and processing it in a way that you can use 562 00:28:52,360 --> 00:28:55,840 Speaker 3: it to build structures, that is a lot, lot, lot 563 00:28:55,920 --> 00:28:58,760 Speaker 3: easier than trying to lift everything off of Earth. And 564 00:28:58,840 --> 00:29:00,840 Speaker 3: so this is something that people looked into them. 565 00:29:00,920 --> 00:29:02,840 Speaker 2: I see, it's like it's possible. 566 00:29:03,520 --> 00:29:06,560 Speaker 3: Yeah. I don't think there's anything physically or in an 567 00:29:06,600 --> 00:29:10,240 Speaker 3: engineering sense impossible about any of this. You can imagine 568 00:29:10,400 --> 00:29:13,320 Speaker 3: building a factory around an asteroid, using it, having it 569 00:29:13,440 --> 00:29:16,840 Speaker 3: spin for centrifugal force, which is like gravity, and that 570 00:29:16,920 --> 00:29:18,480 Speaker 3: you can use to separate out metals. 571 00:29:18,840 --> 00:29:19,280 Speaker 2: I see. 572 00:29:19,400 --> 00:29:21,480 Speaker 1: Okay, so let me see if I can recap so 573 00:29:21,680 --> 00:29:24,360 Speaker 1: the idea of going to an asteroid mining it to 574 00:29:24,400 --> 00:29:28,800 Speaker 1: bring back material like rare earth metals technically possible, but 575 00:29:29,280 --> 00:29:30,239 Speaker 1: maybe not worth it. 576 00:29:30,680 --> 00:29:32,640 Speaker 3: Questionably profitable, Yeah. 577 00:29:32,800 --> 00:29:37,560 Speaker 2: Questionably profitable, I mean maybe just not right now. I see. 578 00:29:37,600 --> 00:29:39,280 Speaker 1: But then there's sort of the other reason why we 579 00:29:39,360 --> 00:29:43,520 Speaker 1: might mind the asteroid belt, which is for space exploration, 580 00:29:43,680 --> 00:29:46,360 Speaker 1: Like if we wanted to, we could use it as 581 00:29:46,360 --> 00:29:49,840 Speaker 1: a source of metals to build spacecraft and space stations 582 00:29:49,960 --> 00:29:52,800 Speaker 1: and there. It's not so much a business consideration, it's 583 00:29:52,840 --> 00:29:54,280 Speaker 1: just like if we want to do it or not. 584 00:29:54,600 --> 00:29:57,400 Speaker 3: Yeah, I mean it's a sort of government level idea. Yeah, 585 00:29:57,440 --> 00:30:00,640 Speaker 3: if you wanted to explore the outer planets, if you 586 00:30:00,720 --> 00:30:04,600 Speaker 3: want to put humans out in space on Mars, for example, 587 00:30:04,680 --> 00:30:08,000 Speaker 3: where some of these materials are scarce. Then yeah, going 588 00:30:08,040 --> 00:30:10,080 Speaker 3: to the asteroid belt and figuring out how to do 589 00:30:10,080 --> 00:30:12,560 Speaker 3: all this is not the worst idea. 590 00:30:12,480 --> 00:30:14,920 Speaker 2: In that case. Maybe it's the cheaper option. 591 00:30:14,960 --> 00:30:17,200 Speaker 3: Rather than lifting it from Earth. Yeah, because right now 592 00:30:17,240 --> 00:30:19,960 Speaker 3: it still costs a lot of money per kilogram to 593 00:30:20,160 --> 00:30:24,360 Speaker 3: just send air, water, food to people living on the 594 00:30:24,400 --> 00:30:28,120 Speaker 3: Moon or Mars. If you could start in space already, 595 00:30:29,160 --> 00:30:33,360 Speaker 3: it's vastly easier. You're getting rid of some majority of 596 00:30:33,400 --> 00:30:36,120 Speaker 3: the cost of just launching something off Earth is so 597 00:30:36,160 --> 00:30:39,160 Speaker 3: expensive and hard. If you're starting in space, it's way easier, 598 00:30:39,200 --> 00:30:42,040 Speaker 3: and so it's a lot simpler technologically, and it's a 599 00:30:42,080 --> 00:30:43,640 Speaker 3: lot cheaper, a lot less expensive. 600 00:30:44,640 --> 00:30:48,360 Speaker 1: So the asteroid belt could become like the wild West 601 00:30:48,560 --> 00:30:52,280 Speaker 1: of the space frontier. And here's the interesting thing. Most 602 00:30:52,320 --> 00:30:56,040 Speaker 1: people assume, like I did, that the most valuable materials 603 00:30:56,080 --> 00:30:58,360 Speaker 1: in the asteroid belt that we would want to mine 604 00:30:58,600 --> 00:31:03,000 Speaker 1: are the metals and the like iron or copper. But 605 00:31:03,040 --> 00:31:07,840 Speaker 1: actually the most important raw element in them is wetter. 606 00:31:09,160 --> 00:31:12,880 Speaker 3: This wasn't known until relatively recently, a few decades ago, 607 00:31:12,880 --> 00:31:15,840 Speaker 3: that asteroids can have a lot of water in them. Oh, 608 00:31:16,000 --> 00:31:20,120 Speaker 3: what series for example, has a mountain on it that 609 00:31:20,240 --> 00:31:23,840 Speaker 3: seems to be salty water from the interior that oozed 610 00:31:23,880 --> 00:31:27,280 Speaker 3: out and froze in place, and it's a mesa. It's 611 00:31:27,320 --> 00:31:30,280 Speaker 3: like this big flat topped mountain. It's huge, and it's 612 00:31:30,280 --> 00:31:33,440 Speaker 3: made of dirty ice, basically dirty salt water ice. Whoa. 613 00:31:33,880 --> 00:31:36,160 Speaker 3: So these things do have water, and you need water. 614 00:31:36,480 --> 00:31:38,960 Speaker 3: Water is the most useful thing you can have in space. 615 00:31:39,040 --> 00:31:41,160 Speaker 3: You drink it. We need that to live. You can 616 00:31:41,200 --> 00:31:43,800 Speaker 3: break it down and make oxygen to breathe. Water is 617 00:31:43,960 --> 00:31:46,720 Speaker 3: h two Oh, it's hydrogen and oxygen together. You can 618 00:31:46,800 --> 00:31:51,000 Speaker 3: recombine these to make hydrogen peroxide, which in its pure form, 619 00:31:51,040 --> 00:31:52,800 Speaker 3: not like the stuff you buy at the drug store, 620 00:31:52,960 --> 00:31:54,280 Speaker 3: which is like three percent. 621 00:31:54,880 --> 00:31:56,160 Speaker 2: You can diyur hairt space. 622 00:31:56,440 --> 00:31:59,040 Speaker 3: Yeah. Yeah, it's like you know, it's three percent hydrogen 623 00:31:59,080 --> 00:32:01,000 Speaker 3: peroxide and the rest of its water, and it's more 624 00:32:01,040 --> 00:32:04,120 Speaker 3: pure form. It's like ninety percent hydrogen peroxide. It burns 625 00:32:04,400 --> 00:32:06,640 Speaker 3: and it becomes a really good fuel. So you can 626 00:32:06,720 --> 00:32:08,120 Speaker 3: drink it, you can breathe it, and you can move 627 00:32:08,160 --> 00:32:10,360 Speaker 3: around with it. So water is it, that's what you want. 628 00:32:10,800 --> 00:32:13,560 Speaker 3: It's actually the single most important thing if you want 629 00:32:13,560 --> 00:32:17,480 Speaker 3: to have a permanent presence in space. Water is the 630 00:32:17,480 --> 00:32:21,600 Speaker 3: most important thing besides you know, food, but even more 631 00:32:21,600 --> 00:32:24,360 Speaker 3: than food, because again with water you can make air and. 632 00:32:24,240 --> 00:32:27,280 Speaker 2: Fuel right right, the grow food, you need water as well. 633 00:32:27,440 --> 00:32:29,520 Speaker 3: Yeah, humans need a lot of water just to survive 634 00:32:29,560 --> 00:32:32,080 Speaker 3: because of not just our direct needs but also our 635 00:32:32,400 --> 00:32:35,960 Speaker 3: needs like growing plants and protection from radiation. Water is 636 00:32:36,000 --> 00:32:39,640 Speaker 3: great at absorbing radiation, so you can encase your ship 637 00:32:39,680 --> 00:32:42,120 Speaker 3: in a tank of water and protect it from solar 638 00:32:42,120 --> 00:32:45,160 Speaker 3: flares and such. So it's all around. It's just like 639 00:32:45,280 --> 00:32:46,720 Speaker 3: the most useful thing ever in. 640 00:32:46,680 --> 00:32:49,360 Speaker 1: Space, right, and you need it to shower if you 641 00:32:49,520 --> 00:32:51,880 Speaker 1: were so inclined to shower in space, Yeah, that would 642 00:32:51,880 --> 00:32:52,320 Speaker 1: be a good. 643 00:32:52,160 --> 00:32:54,160 Speaker 3: Idea too, although who knows, you know, by then we'll 644 00:32:54,200 --> 00:32:58,440 Speaker 3: have sonic showers like in Star Trek. Who knows it's 645 00:32:58,480 --> 00:33:01,680 Speaker 3: out there. There's lots of their comments that are mostly 646 00:33:01,720 --> 00:33:05,000 Speaker 3: water asteroids. There are moons of Jupiter and Saturn that 647 00:33:05,080 --> 00:33:08,000 Speaker 3: are mostly water. Those are harder to get through than asteroids. 648 00:33:08,000 --> 00:33:11,080 Speaker 3: But still there's a lot out there plenty for everybody. 649 00:33:11,760 --> 00:33:13,960 Speaker 1: Yes, it turns out the real question we should be 650 00:33:14,040 --> 00:33:17,600 Speaker 1: asking it's not whether we should mine the asteroid belt, 651 00:33:17,760 --> 00:33:21,080 Speaker 1: but whether we should drink it. Hey, this puts a 652 00:33:21,080 --> 00:33:25,040 Speaker 1: whole new spin on the phrase meteor shower. All right, 653 00:33:25,400 --> 00:33:28,160 Speaker 1: Hopefully this all gives you a good sense of what's 654 00:33:28,160 --> 00:33:31,320 Speaker 1: out there sprinkled in our solar system that could hit 655 00:33:31,400 --> 00:33:35,080 Speaker 1: us or potentially save us as we keep traveling through 656 00:33:35,520 --> 00:33:39,640 Speaker 1: the vastness of space. Thanks for joining us. See you 657 00:33:39,640 --> 00:33:40,360 Speaker 1: next time. 658 00:33:44,040 --> 00:33:45,720 Speaker 2: You've been listening to Science Stuff. 659 00:33:45,960 --> 00:33:49,880 Speaker 1: Production of iHeartRadio written and produced by me or Hey 660 00:33:49,960 --> 00:33:54,320 Speaker 1: Cham edited by Rose Seguda, Executive producer Jerry Rowland, an 661 00:33:54,360 --> 00:33:57,720 Speaker 1: audio engineer and mixer Casey Peckron, and you can follow 662 00:33:57,720 --> 00:34:00,800 Speaker 1: me on social media to search for PhD comics and 663 00:34:00,840 --> 00:34:03,520 Speaker 1: the name of your favorite platform. Be sure to subscribe 664 00:34:03,560 --> 00:34:06,480 Speaker 1: to Sign Stuff on the iHeartRadio app, Apple Podcasts, or 665 00:34:06,520 --> 00:34:09,720 Speaker 1: wherever you get your podcasts, and please tell your friends 666 00:34:10,080 --> 00:34:23,439 Speaker 1: we'll be back next Wednesday with another episode. Hey, please 667 00:34:23,480 --> 00:34:26,840 Speaker 1: take a second and leave us a review on Apple Podcasts, Spotify, 668 00:34:27,120 --> 00:34:28,960 Speaker 1: or wherever you listen to the podcast. 669 00:34:29,480 --> 00:34:30,040 Speaker 2: Thanks a lot,