1 00:00:08,560 --> 00:00:11,760 Speaker 1: What if we've been looking for life in all the 2 00:00:11,800 --> 00:00:16,200 Speaker 1: wrong places. Sure, we're searching for signs of life on Mars, 3 00:00:16,280 --> 00:00:20,160 Speaker 1: and we're hunting down planets around other stars and far 4 00:00:20,200 --> 00:00:23,400 Speaker 1: away solar systems, hoping to find one with an atmosphere 5 00:00:23,680 --> 00:00:27,280 Speaker 1: and maybe even signs of life. But what if life 6 00:00:27,320 --> 00:00:30,360 Speaker 1: could be out there, but not on a planet, not 7 00:00:30,480 --> 00:00:33,280 Speaker 1: even on a moon. What if life could be out 8 00:00:33,280 --> 00:00:53,600 Speaker 1: there but hiding in something much smaller. Hi, I'm Daniel. 9 00:00:53,640 --> 00:00:58,280 Speaker 1: I'm a particle physicist, a sometimes author, and a twice 10 00:00:58,320 --> 00:01:01,640 Speaker 1: a week podcast host. You are listening to the podcast 11 00:01:01,960 --> 00:01:05,720 Speaker 1: Daniel and Jorge Explain the Universe, brought to you by 12 00:01:05,760 --> 00:01:09,479 Speaker 1: I Heart Radio. My usual co host, Jorge isn't here 13 00:01:09,520 --> 00:01:11,720 Speaker 1: still this week. He'll be away for a little while, 14 00:01:11,720 --> 00:01:15,080 Speaker 1: but don't worry, folks, he'll be coming back soon. Our 15 00:01:15,160 --> 00:01:19,000 Speaker 1: podcast is dedicated to zooming around the universe, exploring everything 16 00:01:19,040 --> 00:01:22,760 Speaker 1: that's weird, that's amazing, that's crazy, that blows your mind, 17 00:01:22,840 --> 00:01:26,160 Speaker 1: that maybe you hear scientists talking about but never really 18 00:01:26,240 --> 00:01:30,080 Speaker 1: understood until today until we break it down for you. 19 00:01:30,319 --> 00:01:32,600 Speaker 1: So the goal of our podcast is to share with 20 00:01:32,640 --> 00:01:36,280 Speaker 1: you the amazing, crazy bunkers universe that we live in. 21 00:01:36,560 --> 00:01:39,960 Speaker 1: Without blowing your mind too much. We want to download 22 00:01:40,000 --> 00:01:42,600 Speaker 1: that information into your brain so that you really get it, 23 00:01:42,600 --> 00:01:45,400 Speaker 1: so you can appreciate, just like scientists on the cutting 24 00:01:45,440 --> 00:01:49,040 Speaker 1: edge of knowledge, how amazing and crazy this universe is. 25 00:01:49,760 --> 00:01:51,600 Speaker 1: And a lot of times on this podcast we go 26 00:01:51,760 --> 00:01:53,920 Speaker 1: far away and talk about the center of the galaxy 27 00:01:54,040 --> 00:01:57,000 Speaker 1: or other galaxies, or the structure of the whole universe, 28 00:01:57,320 --> 00:01:59,560 Speaker 1: or we zoom down a tiny little particles and talk 29 00:01:59,600 --> 00:02:02,720 Speaker 1: about how amazing and weird they are and the strange 30 00:02:02,840 --> 00:02:05,440 Speaker 1: rules that governed life of the quantum realm. But there 31 00:02:05,440 --> 00:02:08,600 Speaker 1: are mysteries close to home, and we have talked, for example, 32 00:02:08,600 --> 00:02:11,600 Speaker 1: about the mysteries of lightning and house skip stones, and 33 00:02:11,680 --> 00:02:14,400 Speaker 1: also about weird things going on in our solar system, 34 00:02:14,440 --> 00:02:17,320 Speaker 1: and that is the focus of today's episode. We want 35 00:02:17,320 --> 00:02:20,480 Speaker 1: to understand the weird stuff that's in our neighborhood. We 36 00:02:20,520 --> 00:02:23,000 Speaker 1: want to make sure, then we look over our shoulder, 37 00:02:23,240 --> 00:02:26,320 Speaker 1: we understand what's going on, because people think, oh, our 38 00:02:26,360 --> 00:02:28,760 Speaker 1: solar system, we've been exploring it for hundreds of not 39 00:02:28,880 --> 00:02:31,960 Speaker 1: thousands of years. Surely we understand what there is to 40 00:02:32,040 --> 00:02:34,600 Speaker 1: know there. Surely we have a grasp on everything that's 41 00:02:34,639 --> 00:02:38,000 Speaker 1: going on in the Solar System. Well, not true, and 42 00:02:38,080 --> 00:02:40,640 Speaker 1: some of those amazing mysteries are hiding in a place 43 00:02:40,720 --> 00:02:43,080 Speaker 1: you probably don't even think about. If I tell you 44 00:02:43,120 --> 00:02:46,519 Speaker 1: to imagine the Solar System, you probably think of the Sun. 45 00:02:46,639 --> 00:02:49,920 Speaker 1: First off, it's the biggest, baddest object in the Solar System, 46 00:02:50,240 --> 00:02:52,519 Speaker 1: and then of course the planets zooming around it, with 47 00:02:52,600 --> 00:02:55,280 Speaker 1: the star being our blue globe that we call home. 48 00:02:55,880 --> 00:02:59,520 Speaker 1: But there's something else there. There's another big piece of 49 00:02:59,560 --> 00:03:01,920 Speaker 1: the Solar System that takes up a huge chunk. It's 50 00:03:01,960 --> 00:03:05,400 Speaker 1: an important element, but it's not a dense object like 51 00:03:05,480 --> 00:03:09,239 Speaker 1: planets in the Sun. It's the asteroid belt. The asteroid 52 00:03:09,240 --> 00:03:12,840 Speaker 1: belt is this weird collection of rocks between Mars and Jupiter, 53 00:03:13,240 --> 00:03:15,239 Speaker 1: and it turns out there's a lot of things we 54 00:03:15,280 --> 00:03:18,119 Speaker 1: don't understand about. It's starting off with why is there 55 00:03:18,120 --> 00:03:21,639 Speaker 1: an asteroid belt. It goes planet planet, planet, planet, planet, 56 00:03:21,760 --> 00:03:26,440 Speaker 1: asteroid belt, planet, planet, planet, planet, anything that's weird in science, 57 00:03:26,440 --> 00:03:29,120 Speaker 1: anything that sticks out, that's a clue that's going to 58 00:03:29,240 --> 00:03:32,120 Speaker 1: show you the path to an answer. It's gonna reveal 59 00:03:32,280 --> 00:03:35,040 Speaker 1: something about why it looks that way and not some 60 00:03:35,280 --> 00:03:38,480 Speaker 1: other way. So every time we find a pattern that 61 00:03:38,600 --> 00:03:42,120 Speaker 1: doesn't quite fit, we ask why, and hopefully those answers 62 00:03:42,200 --> 00:03:46,080 Speaker 1: lead to mind blowing discoveries and probably more questions. But 63 00:03:46,160 --> 00:03:48,560 Speaker 1: it's not just the fact of the asteroid belt that's weird, 64 00:03:48,680 --> 00:03:52,280 Speaker 1: it's what's inside it. So the question will be answering 65 00:03:52,320 --> 00:04:01,640 Speaker 1: today is what's going on with the asteroid belt? And 66 00:04:01,680 --> 00:04:03,800 Speaker 1: I have to share with you that learning about the 67 00:04:03,840 --> 00:04:07,360 Speaker 1: asteroid belt, I had a personal oh my god, is 68 00:04:07,400 --> 00:04:11,360 Speaker 1: it aliens moment when one of these strange, bizarre, crazy 69 00:04:11,440 --> 00:04:14,640 Speaker 1: features of the asteroid belt was first discovered. We'll talk 70 00:04:14,680 --> 00:04:18,040 Speaker 1: about that soon, but first I was wondering, what do 71 00:04:18,080 --> 00:04:20,440 Speaker 1: people know about the asteroid belt? Do people out there 72 00:04:20,480 --> 00:04:23,120 Speaker 1: even know what's in the asteroid belt? And why it's interesting? 73 00:04:23,320 --> 00:04:26,240 Speaker 1: Does everybody know that there is an asteroid belt? So, 74 00:04:26,320 --> 00:04:28,800 Speaker 1: as usual to sort of get a sense for how 75 00:04:28,880 --> 00:04:31,640 Speaker 1: much people know and what their questions are, I walked 76 00:04:31,680 --> 00:04:34,880 Speaker 1: around campus at you see irvine and I asked people, Hey, 77 00:04:35,000 --> 00:04:38,159 Speaker 1: what do you think is in the asteroid belt? People 78 00:04:38,160 --> 00:04:40,760 Speaker 1: thought that was a weird question, but as usual, they 79 00:04:40,760 --> 00:04:42,760 Speaker 1: were games. So thank you again to the students that 80 00:04:42,880 --> 00:04:47,400 Speaker 1: use the irvine for answering a weirdos weird questions. Here's 81 00:04:47,400 --> 00:04:49,640 Speaker 1: what they had to say. But before you answer, think 82 00:04:49,680 --> 00:04:52,119 Speaker 1: to yourself, do you know what's in the asteroid belt? 83 00:04:52,279 --> 00:04:55,080 Speaker 1: How accurately could you describe it? Here the answers from 84 00:04:55,120 --> 00:04:58,440 Speaker 1: students at you see irvine for the most precious rocks, 85 00:04:58,480 --> 00:05:01,719 Speaker 1: and then now it's a debris because space jump in 86 00:05:01,760 --> 00:05:05,120 Speaker 1: all that, and then it's accumulating, So it can be 87 00:05:05,320 --> 00:05:08,159 Speaker 1: I believe, a combination of things of sizes at least 88 00:05:08,279 --> 00:05:14,360 Speaker 1: from larger to smaller, tiny rocks next to moon, maybe 89 00:05:14,400 --> 00:05:17,719 Speaker 1: the size of the moon, bigger, I don't know, combination 90 00:05:17,760 --> 00:05:21,880 Speaker 1: of sand and some other chemicals. I would say they're 91 00:05:21,920 --> 00:05:24,560 Speaker 1: pretty big rocks, but there's a lot of diversity there. 92 00:05:24,800 --> 00:05:26,919 Speaker 1: I'm under the impression that it's a lot of rocks 93 00:05:26,960 --> 00:05:31,320 Speaker 1: and maybe a couple of like icy stuff in there too. 94 00:05:31,640 --> 00:05:33,800 Speaker 1: They could be as big asn't want to as big 95 00:05:33,839 --> 00:05:36,520 Speaker 1: as Earth. It just depends, like where you are. I 96 00:05:36,520 --> 00:05:39,800 Speaker 1: would say it varies a lot, like maybe somewhere from 97 00:05:39,839 --> 00:05:43,400 Speaker 1: like the car through maybe like a small moon or something. 98 00:05:43,600 --> 00:05:46,880 Speaker 1: So of course the most popular answer is asteroids. That 99 00:05:46,920 --> 00:05:49,520 Speaker 1: makes sense. You wouldn't call it the asteroid belt if 100 00:05:49,520 --> 00:05:52,840 Speaker 1: you didn't have asteroids in it. But what are asteroids? 101 00:05:52,839 --> 00:05:54,920 Speaker 1: And of course you heard a lot of people say, rocks, 102 00:05:55,120 --> 00:05:58,599 Speaker 1: big rocks, small rocks, read the little rocks. Some people 103 00:05:58,640 --> 00:06:00,839 Speaker 1: even thought that there were rocks in there the size 104 00:06:00,880 --> 00:06:04,200 Speaker 1: of the moon. So there's a big variety of reactions 105 00:06:04,200 --> 00:06:06,880 Speaker 1: out there to what's in the asteroid belt. So that 106 00:06:06,920 --> 00:06:09,240 Speaker 1: makes me feel like, yeah, let's dig into it. Let's 107 00:06:09,279 --> 00:06:12,400 Speaker 1: make sure everybody out there knows what the asteroid belt is, 108 00:06:12,720 --> 00:06:15,160 Speaker 1: what we know about it, what we don't know about it, 109 00:06:15,200 --> 00:06:19,480 Speaker 1: and what amazing potential alien discoveries it might be hiding. 110 00:06:20,160 --> 00:06:23,719 Speaker 1: All right, So first of all, where is the asteroid belt. 111 00:06:23,880 --> 00:06:27,400 Speaker 1: The asteroid belt is between Mars and Jupiter, right, so 112 00:06:27,440 --> 00:06:30,120 Speaker 1: we got four inner planets and then we got this 113 00:06:30,560 --> 00:06:33,920 Speaker 1: big swath or rocks or asteroids, and then we got 114 00:06:33,960 --> 00:06:37,640 Speaker 1: the outer planets Jupiter, Saturn, and the Neptune Uranus. Of course, 115 00:06:38,040 --> 00:06:40,359 Speaker 1: so we sort of divides the Solar system. Right, you 116 00:06:40,400 --> 00:06:43,839 Speaker 1: have these inner rocky planets and then the asteroid belt, 117 00:06:43,839 --> 00:06:46,440 Speaker 1: and then you've got the big gas planets on the outside. 118 00:06:46,800 --> 00:06:49,880 Speaker 1: And that seems like a clue, right, So let's dig 119 00:06:49,920 --> 00:06:53,039 Speaker 1: in a little bit. What is in the asteroid belt. Well, 120 00:06:53,080 --> 00:06:57,120 Speaker 1: it's not just asteroids, right, Asteroids means a lot of things, 121 00:06:57,160 --> 00:07:00,640 Speaker 1: and the asteroid belt was discovered actually in the eight hundreds, 122 00:07:00,640 --> 00:07:03,920 Speaker 1: because some of these asteroids in the belt are big, like, 123 00:07:04,000 --> 00:07:07,799 Speaker 1: they are really big. In fact, the asteroid belt doesn't 124 00:07:07,880 --> 00:07:11,360 Speaker 1: just have asteroids in it, it also has dwarf planets, 125 00:07:11,760 --> 00:07:15,000 Speaker 1: planets that are as big as Pluto, not quite the 126 00:07:15,040 --> 00:07:18,240 Speaker 1: size of our moon, right, but these are big rocks. 127 00:07:18,400 --> 00:07:20,480 Speaker 1: And remember, the way we see these things in the 128 00:07:20,480 --> 00:07:23,480 Speaker 1: sky is we can't see them glow directly. They don't 129 00:07:23,560 --> 00:07:26,040 Speaker 1: give off light the way the sun does. We can 130 00:07:26,120 --> 00:07:28,640 Speaker 1: only see them when the Sun's light shines on them 131 00:07:28,760 --> 00:07:31,480 Speaker 1: and then bounces back to Earth, the same way we 132 00:07:31,560 --> 00:07:34,760 Speaker 1: see our own moon, which also doesn't actually glow in 133 00:07:34,800 --> 00:07:36,920 Speaker 1: the sky. It's just a reflection of the light from 134 00:07:36,920 --> 00:07:39,880 Speaker 1: the Sun. So any of these objects for us to 135 00:07:39,960 --> 00:07:42,360 Speaker 1: see them, they have to be shiny, and they have 136 00:07:42,480 --> 00:07:44,560 Speaker 1: to be big, because that's the only way we can 137 00:07:44,560 --> 00:07:47,080 Speaker 1: see this stuff. So of course, in the eighteen hundreds, 138 00:07:47,120 --> 00:07:49,640 Speaker 1: the first thing we found were the biggest ones. That's 139 00:07:49,680 --> 00:07:52,880 Speaker 1: back before we had amazing space telescopes to track all 140 00:07:52,920 --> 00:07:55,960 Speaker 1: these things down. And there are four objects in the 141 00:07:56,000 --> 00:07:59,720 Speaker 1: asteroid belt that take up a whopping half of the mass. 142 00:08:00,120 --> 00:08:02,120 Speaker 1: That's right. You add up all the rocks and set 143 00:08:02,240 --> 00:08:04,400 Speaker 1: and sand and dust and ice and all that stuff 144 00:08:04,400 --> 00:08:07,840 Speaker 1: in the asteroid belt, and why it Half of it 145 00:08:07,880 --> 00:08:10,320 Speaker 1: is in just four objects, and these were the first 146 00:08:10,360 --> 00:08:13,800 Speaker 1: four scene. Those are Series, which is a little dwarf planet, 147 00:08:14,280 --> 00:08:18,240 Speaker 1: Vesta Palace, and Hygia. Again, I don't know who's in 148 00:08:18,320 --> 00:08:20,760 Speaker 1: charge of naming these objects. I'm not even sure how 149 00:08:20,760 --> 00:08:23,120 Speaker 1: to officially do pronounce them, but I think it's sort 150 00:08:23,160 --> 00:08:25,640 Speaker 1: of awesome that they're out there, that's sort of dominating 151 00:08:25,680 --> 00:08:30,120 Speaker 1: the asteroid belt. So it's mostly these big four asteroids. 152 00:08:30,200 --> 00:08:32,880 Speaker 1: And then in the late eighteen hundreds people were looking 153 00:08:32,960 --> 00:08:34,959 Speaker 1: more and more and they saw smaller rocks. But it 154 00:08:35,040 --> 00:08:38,480 Speaker 1: drops off pretty fast, and so it took until about 155 00:08:38,559 --> 00:08:41,280 Speaker 1: eighteen sixty eight before people had seen a hundred of 156 00:08:41,320 --> 00:08:44,719 Speaker 1: these things, and then in the early nineteen hundreds they 157 00:08:44,720 --> 00:08:48,280 Speaker 1: had seen a thousand, and then by one we had 158 00:08:48,280 --> 00:08:52,720 Speaker 1: found ten thousand individual objects in the asteroid belt. And 159 00:08:52,760 --> 00:08:56,679 Speaker 1: now we have more than a hundred thousand individual objects characterized. 160 00:08:56,960 --> 00:08:59,480 Speaker 1: We know where they're going, we know half fast they're spinning, 161 00:08:59,840 --> 00:09:02,800 Speaker 1: we know their orbit. They each probably have names, though 162 00:09:02,800 --> 00:09:05,200 Speaker 1: those names, of course are probably not very creative. If 163 00:09:05,240 --> 00:09:07,800 Speaker 1: you have to name a hundred thousand objects in the 164 00:09:07,800 --> 00:09:10,120 Speaker 1: Solar System. You probably come up with a scheme, and 165 00:09:10,160 --> 00:09:13,640 Speaker 1: they probably have really boring names like letters and numbers. 166 00:09:13,679 --> 00:09:17,120 Speaker 1: So most of the mass is in just four these objects, right, 167 00:09:17,120 --> 00:09:19,920 Speaker 1: and those are really sort of like many planets. They 168 00:09:19,960 --> 00:09:22,800 Speaker 1: can't really even call those asteroids. But you know, a 169 00:09:22,800 --> 00:09:25,280 Speaker 1: lot of this is just terminology. What do you call 170 00:09:25,320 --> 00:09:27,280 Speaker 1: a planet? What do you call it dwarf planet? What 171 00:09:27,320 --> 00:09:29,440 Speaker 1: do you call an asteroid? This is just sort of 172 00:09:29,520 --> 00:09:32,439 Speaker 1: arbitrary stuff that we made up. Like a whole controversy 173 00:09:32,520 --> 00:09:35,520 Speaker 1: about whether Pluto is a planet or a dwarf planet 174 00:09:35,679 --> 00:09:38,560 Speaker 1: comes down to semantics. It's not like there's a clear 175 00:09:38,640 --> 00:09:41,240 Speaker 1: difference between one object and the other. People just have 176 00:09:41,320 --> 00:09:43,120 Speaker 1: to draw a line somewhere and then you say, well, 177 00:09:43,160 --> 00:09:45,000 Speaker 1: on this side of the line your planet over here, 178 00:09:45,040 --> 00:09:49,200 Speaker 1: your dwarf planet. Doesn't really necessarily mean anything. So sometimes 179 00:09:49,200 --> 00:09:52,000 Speaker 1: I feel like the whole controversy about whether Pluto is 180 00:09:52,040 --> 00:09:54,920 Speaker 1: a planet or not is a bit overblown. It's there, 181 00:09:55,360 --> 00:09:57,800 Speaker 1: we know what it is. It's a thing, you know, 182 00:09:57,880 --> 00:09:59,520 Speaker 1: it's part of our family. Do we have to be 183 00:09:59,520 --> 00:10:03,439 Speaker 1: so we're about labels anyway? Even if you add up 184 00:10:03,520 --> 00:10:06,240 Speaker 1: all the stuff in the asteroid belt, all the rocks 185 00:10:06,280 --> 00:10:08,680 Speaker 1: and dust and ice and all of that stuff that's there. 186 00:10:09,200 --> 00:10:11,880 Speaker 1: It's only four percent of the mass of the Moon. 187 00:10:12,360 --> 00:10:16,079 Speaker 1: That's right. The Moon is more than twenty five times 188 00:10:16,080 --> 00:10:18,760 Speaker 1: more massive than all the stuff in the asteroid belt 189 00:10:18,800 --> 00:10:22,680 Speaker 1: put together. And that tells you two things. One, we've 190 00:10:22,679 --> 00:10:24,720 Speaker 1: got a big moon, like it's the truth, like, of 191 00:10:24,760 --> 00:10:27,080 Speaker 1: all the moons in the Solar System, Earth is odd 192 00:10:27,360 --> 00:10:31,440 Speaker 1: for having such a big moon. Also, it tells you 193 00:10:31,480 --> 00:10:34,240 Speaker 1: that the asteroid belt is not that big, right, There's 194 00:10:34,280 --> 00:10:37,120 Speaker 1: not that much stuff in it. You probably imagine the 195 00:10:37,120 --> 00:10:40,640 Speaker 1: asteroid belt is like space totally dotted with rocks, and 196 00:10:41,000 --> 00:10:43,680 Speaker 1: like that scene in Star Wars where the Millennium Falcon 197 00:10:43,760 --> 00:10:46,320 Speaker 1: is trying to navigate its way at high speed through 198 00:10:46,320 --> 00:10:49,400 Speaker 1: those rocks and just barely whizzing by and almost crashing. 199 00:10:49,800 --> 00:10:53,080 Speaker 1: That's not the experience we have when we send probes 200 00:10:53,480 --> 00:10:56,040 Speaker 1: through the asteroid belt, because the asteroid belt is not 201 00:10:56,160 --> 00:11:00,920 Speaker 1: that dense. Remember, space is big, like really really big. 202 00:11:01,280 --> 00:11:03,559 Speaker 1: If you're gonna fly out into the Solar System, you're 203 00:11:03,679 --> 00:11:06,280 Speaker 1: very unlikely to hit a planet, right, because even though 204 00:11:06,320 --> 00:11:10,240 Speaker 1: planets are big, they're not big compared to the Solar System. 205 00:11:10,280 --> 00:11:13,280 Speaker 1: In the same way, the asteroid belt. Even though it's 206 00:11:13,280 --> 00:11:17,080 Speaker 1: distributed across lots of little rocks, it still doesn't fill 207 00:11:17,160 --> 00:11:19,880 Speaker 1: up space. It doesn't even come close to filling up space. 208 00:11:20,080 --> 00:11:22,199 Speaker 1: We have sent lots of probes to the outer part 209 00:11:22,240 --> 00:11:25,280 Speaker 1: of the Solar System and never even worried about having 210 00:11:25,320 --> 00:11:28,280 Speaker 1: them hit an asteroid. It's difficult, in fact, to hit 211 00:11:28,320 --> 00:11:32,120 Speaker 1: an asteroid. The Japanese recently sent up an awesome probe 212 00:11:32,160 --> 00:11:34,920 Speaker 1: to land on an asteroid and punch it to see 213 00:11:34,920 --> 00:11:37,000 Speaker 1: what it's made out of and understand, you know, is 214 00:11:37,000 --> 00:11:39,319 Speaker 1: it made out of carbon or silicon or ice or whatever. 215 00:11:39,679 --> 00:11:42,680 Speaker 1: And that was hard, right, So it's not easy to 216 00:11:42,760 --> 00:11:44,960 Speaker 1: run into an asteroid. If you want to fly your 217 00:11:44,960 --> 00:11:47,680 Speaker 1: spaceship through the asteroid belt, most likely you'll never even 218 00:11:47,760 --> 00:11:50,240 Speaker 1: see one. And if you just watch these things, they 219 00:11:50,280 --> 00:11:53,080 Speaker 1: don't even bounce into each other. Very often. Asteroids of 220 00:11:53,080 --> 00:11:56,240 Speaker 1: any size hit each other around every ten million years. 221 00:11:56,600 --> 00:11:59,559 Speaker 1: And that's because number one, there aren't very many in 222 00:11:59,600 --> 00:12:02,480 Speaker 1: space big, but also number two, because it's been around 223 00:12:02,520 --> 00:12:05,319 Speaker 1: for billions of years, and so by now a lot 224 00:12:05,400 --> 00:12:08,000 Speaker 1: of those collisions that were if they were going to happen, 225 00:12:08,160 --> 00:12:10,760 Speaker 1: they sort of already happened. And what you have left 226 00:12:10,800 --> 00:12:13,680 Speaker 1: is a bunch of asteroids in their own lane. It's 227 00:12:13,720 --> 00:12:16,560 Speaker 1: like a huge traffic jam, but all the collisions have 228 00:12:16,600 --> 00:12:19,079 Speaker 1: happened already, and all those wrecks have been towed off 229 00:12:19,120 --> 00:12:21,080 Speaker 1: the road, and now you just have a bunch of 230 00:12:21,080 --> 00:12:24,000 Speaker 1: clean lanes and safe drivers and everybody's sort of go 231 00:12:24,080 --> 00:12:27,600 Speaker 1: in their own way, so you can very safely navigate 232 00:12:27,720 --> 00:12:30,760 Speaker 1: through the asteroid belt, though you'll see some weird stuff, 233 00:12:30,800 --> 00:12:32,319 Speaker 1: like some of these rocks that we see in the 234 00:12:32,320 --> 00:12:35,040 Speaker 1: asteroid belt are kind of hard to understand. Some of 235 00:12:35,040 --> 00:12:38,040 Speaker 1: them are spinning super fast, Like it takes the Earth 236 00:12:38,200 --> 00:12:41,680 Speaker 1: twenty four hours to rotate one time, but it takes 237 00:12:41,679 --> 00:12:44,480 Speaker 1: these rocks less than thirty seconds some of them to 238 00:12:44,679 --> 00:12:47,640 Speaker 1: rotate to do a full rotation, and one of them, 239 00:12:47,679 --> 00:12:51,240 Speaker 1: the speed champion the asteroid belt, doesn't complete turn in 240 00:12:51,400 --> 00:12:54,960 Speaker 1: ten seconds, so it's spinning like crazy. And while most 241 00:12:55,000 --> 00:12:56,920 Speaker 1: of the things in the Solar System go in the 242 00:12:56,960 --> 00:13:00,800 Speaker 1: same direction, and that comes from the initial angular momentum 243 00:13:00,800 --> 00:13:03,440 Speaker 1: in the Solar system that's rotating blob of gas and 244 00:13:03,559 --> 00:13:06,160 Speaker 1: dust that formed the star and the planets and all 245 00:13:06,240 --> 00:13:09,160 Speaker 1: that stuff, some of them are going the opposite direction 246 00:13:09,200 --> 00:13:13,040 Speaker 1: their retrograde. They're like spinning the wrong way. So there's 247 00:13:13,080 --> 00:13:14,559 Speaker 1: a lot of clues there, and there's a lot of 248 00:13:14,559 --> 00:13:17,160 Speaker 1: clues about how the Solar System was formed. Why is 249 00:13:17,200 --> 00:13:19,480 Speaker 1: the asteroid belt there? Why is it there and looked 250 00:13:19,520 --> 00:13:21,560 Speaker 1: like this, Why does it have these weird elements in 251 00:13:21,600 --> 00:13:25,040 Speaker 1: it doing this strange stuff? A lot of fascinating questions 252 00:13:25,080 --> 00:13:27,600 Speaker 1: to dig into, and we'll dig into them, but first 253 00:13:27,720 --> 00:13:42,760 Speaker 1: we'll take a quick break. All right, So we're talking 254 00:13:42,800 --> 00:13:45,800 Speaker 1: about the asteroid belt. What mysteries does it contain? What 255 00:13:46,000 --> 00:13:49,200 Speaker 1: secrets of the origin of the Solar System are hidden 256 00:13:49,240 --> 00:13:52,000 Speaker 1: there in the asteroid belt? Well, it turns out a lot. 257 00:13:52,440 --> 00:13:54,600 Speaker 1: And the first question you might ask, if you're a 258 00:13:54,600 --> 00:13:58,320 Speaker 1: scientist is why isn't there a planet there? Like why 259 00:13:58,440 --> 00:14:00,880 Speaker 1: is there an asteroid belt and not just a planet? 260 00:14:01,280 --> 00:14:03,520 Speaker 1: If you make a plot of the distance from the 261 00:14:03,600 --> 00:14:06,800 Speaker 1: Sun of the various planets and you start with the ones, 262 00:14:06,880 --> 00:14:09,200 Speaker 1: you know, then there's sort of a gap there. You 263 00:14:09,520 --> 00:14:13,240 Speaker 1: expect there to be a planet there between Mars and Jupiter. 264 00:14:13,520 --> 00:14:16,080 Speaker 1: And very early astronomers, they were big into these kind 265 00:14:16,120 --> 00:14:19,400 Speaker 1: of patterns. We didn't have a detailed mathematical understanding of 266 00:14:19,400 --> 00:14:23,280 Speaker 1: how things worked, even before gravity and understanding orbits and stuff. 267 00:14:23,440 --> 00:14:26,400 Speaker 1: People were just looking at patterns like the distances from 268 00:14:26,480 --> 00:14:30,040 Speaker 1: these planets to the Sun, and it just didn't look right. 269 00:14:30,040 --> 00:14:32,080 Speaker 1: There was this weird gap there and made people think 270 00:14:32,360 --> 00:14:35,640 Speaker 1: could there be another planet there hiding. Then of course 271 00:14:35,640 --> 00:14:38,400 Speaker 1: we saw the little rocks there, and people understood, oh, 272 00:14:38,400 --> 00:14:41,000 Speaker 1: there's no planet there. There's just sort of a big 273 00:14:41,080 --> 00:14:44,560 Speaker 1: slew of rocks. But it makes you wonder why. And 274 00:14:44,680 --> 00:14:47,400 Speaker 1: one of the most natural stories to imagine is maybe 275 00:14:47,400 --> 00:14:50,360 Speaker 1: there used to be a planet there. Maybe there was 276 00:14:50,360 --> 00:14:53,560 Speaker 1: an ancient planet and got ripped apart by some disaster, 277 00:14:53,960 --> 00:14:56,520 Speaker 1: and what we're looking at now is basically the shrapnel 278 00:14:56,600 --> 00:14:59,640 Speaker 1: from some ancient murder mystery. They even named it. It's 279 00:14:59,680 --> 00:15:03,880 Speaker 1: called Phaeton, which is a really cool name for a planet. Unfortunately, 280 00:15:03,920 --> 00:15:06,320 Speaker 1: that's a cool story, but it's unlikely to be the 281 00:15:06,360 --> 00:15:09,720 Speaker 1: accurate scientific description of what happened there. But it just 282 00:15:09,760 --> 00:15:11,680 Speaker 1: shows you that people have been thinking about this for 283 00:15:11,720 --> 00:15:14,360 Speaker 1: a long time. People have been wondering why is an 284 00:15:14,360 --> 00:15:17,640 Speaker 1: asteroid belt there, Why isn't there a planet. And to 285 00:15:17,720 --> 00:15:19,920 Speaker 1: understand why there isn't the planet there, why we have 286 00:15:19,960 --> 00:15:22,840 Speaker 1: an asteroid belt, we have to understand two things. First 287 00:15:23,200 --> 00:15:25,720 Speaker 1: is how the Solar System was formed, Like, where did 288 00:15:25,760 --> 00:15:27,960 Speaker 1: this all come from? Anyway? How are any of the 289 00:15:28,000 --> 00:15:31,320 Speaker 1: planets made? And why wasn't there one made there? Well, 290 00:15:31,360 --> 00:15:34,720 Speaker 1: we think that the Solar System, it's ancient progenitor, is 291 00:15:34,760 --> 00:15:37,800 Speaker 1: just a big cloud of gas and dust and stuff. 292 00:15:38,280 --> 00:15:41,120 Speaker 1: Some of that gas is hydrogen, which probably comes from 293 00:15:41,160 --> 00:15:44,080 Speaker 1: the Big Bang. It's left over from billions of years ago. 294 00:15:44,720 --> 00:15:46,880 Speaker 1: Some of it is helium, also maybe from the Big 295 00:15:46,920 --> 00:15:50,760 Speaker 1: Bang or fused together hydrogen in the COREUS stars. And 296 00:15:50,760 --> 00:15:53,240 Speaker 1: then the rest of it, the heavier elements, either made 297 00:15:53,400 --> 00:15:56,360 Speaker 1: in old stars which then blew up and spewed their 298 00:15:56,400 --> 00:15:59,920 Speaker 1: remains all over the university, gathered back together by gravity, 299 00:16:00,520 --> 00:16:03,840 Speaker 1: or even the remnants of neutron star collisions. Remember, all 300 00:16:03,840 --> 00:16:06,720 Speaker 1: the gold and the heavy elements on Earth were made 301 00:16:06,800 --> 00:16:10,200 Speaker 1: not in stars, not in supernovas, but instead they were 302 00:16:10,240 --> 00:16:15,080 Speaker 1: made when neutron stars collided. Because that's the crazy situation. 303 00:16:15,120 --> 00:16:17,520 Speaker 1: You need to fuse those heavy metals. And we have 304 00:16:17,520 --> 00:16:20,320 Speaker 1: a whole podcast episode about that, which I suggest people 305 00:16:20,640 --> 00:16:23,000 Speaker 1: dig into if they like these questions. So we have 306 00:16:23,040 --> 00:16:25,880 Speaker 1: the raw materials, we've got the hydrogen, we've got the helium, 307 00:16:25,920 --> 00:16:28,040 Speaker 1: we got the heavy stuff. All this is left over 308 00:16:28,120 --> 00:16:32,640 Speaker 1: from previous activity in the universe and then what happens. Well, gravity, 309 00:16:32,960 --> 00:16:36,400 Speaker 1: Gravity is the dominant force that controls the structure of 310 00:16:36,440 --> 00:16:39,600 Speaker 1: the universe. It's the weakest force. It's totally weird. We 311 00:16:39,640 --> 00:16:42,040 Speaker 1: don't understand is it a force, is it just a 312 00:16:42,080 --> 00:16:44,720 Speaker 1: bending of space? Is it something else? Can it be 313 00:16:44,800 --> 00:16:48,160 Speaker 1: described by quantum mechanics. We have so many questions about gravity, 314 00:16:48,520 --> 00:16:50,480 Speaker 1: But one thing we do know about it is that 315 00:16:50,520 --> 00:16:53,440 Speaker 1: it almost always wins in the end because it's patient. 316 00:16:54,000 --> 00:16:57,480 Speaker 1: And remember that gravity has this other feature that, unlike 317 00:16:57,520 --> 00:17:01,800 Speaker 1: the other forces, it can't be opposed, like electromagnetism can 318 00:17:01,800 --> 00:17:04,080 Speaker 1: be balanced. You can have things that are neutral, but 319 00:17:04,160 --> 00:17:07,600 Speaker 1: gravity operates on everything with mass, and because we've never 320 00:17:07,640 --> 00:17:11,720 Speaker 1: seen anything with negative mass, gravity is only attractive. And 321 00:17:11,760 --> 00:17:15,240 Speaker 1: so it just keeps pulling and pulling and pulling. It's patient, 322 00:17:15,760 --> 00:17:19,200 Speaker 1: it's slow, but eventually it does what it needs to do. 323 00:17:19,560 --> 00:17:22,280 Speaker 1: And so you take this huge cloud of gas and 324 00:17:22,359 --> 00:17:26,080 Speaker 1: dust spread out across an enormous area, and slowly the 325 00:17:26,119 --> 00:17:30,720 Speaker 1: gravitational forces between these particles, tiny little objects. It tugs 326 00:17:30,720 --> 00:17:33,679 Speaker 1: them closer and closer, and it gathers them together and 327 00:17:33,720 --> 00:17:36,880 Speaker 1: eventually gathers it together. So densely that you get things 328 00:17:36,920 --> 00:17:41,639 Speaker 1: like stars and planets and other stuff. And you might think, first, well, 329 00:17:42,000 --> 00:17:46,120 Speaker 1: why doesn't it just gather everything together into one big blob, right, 330 00:17:46,119 --> 00:17:48,320 Speaker 1: Why doesn't it just make a big star? Why do 331 00:17:48,359 --> 00:17:51,679 Speaker 1: you get anything but the star? Then initial cloud of 332 00:17:51,720 --> 00:17:54,840 Speaker 1: gas and dust and particles. It's spinning, of course, because 333 00:17:54,840 --> 00:17:58,000 Speaker 1: everything in the universe is spinning from some previous interaction 334 00:17:58,080 --> 00:18:00,600 Speaker 1: that happened, maybe from the initial looks illusion of the 335 00:18:00,640 --> 00:18:04,120 Speaker 1: supernova or whatever that generated that stuff. And that spinning 336 00:18:04,160 --> 00:18:07,600 Speaker 1: can't just go away. Remember, in our universe we have momentum, 337 00:18:07,760 --> 00:18:10,600 Speaker 1: so if you push something in space, it will go forever. 338 00:18:10,840 --> 00:18:14,119 Speaker 1: If you start something spinning, it'll spin forever until something 339 00:18:14,119 --> 00:18:16,960 Speaker 1: stops it. And so this cloud of gas and dust 340 00:18:17,000 --> 00:18:19,520 Speaker 1: that created our solar system was spinning, and it is 341 00:18:19,560 --> 00:18:23,240 Speaker 1: still spinning, and that spinning keeps it from collapsing, but 342 00:18:23,400 --> 00:18:27,320 Speaker 1: only in the direction that it's spinning. It's spinning around 343 00:18:27,359 --> 00:18:29,760 Speaker 1: a plane. That plane is now the plane of our 344 00:18:29,800 --> 00:18:32,720 Speaker 1: solar system, and that's why everything in our solar system 345 00:18:32,760 --> 00:18:35,160 Speaker 1: is sort of flat, is spinning around the same axis 346 00:18:35,400 --> 00:18:39,120 Speaker 1: because that's the original access of spin. And in that direction, 347 00:18:39,160 --> 00:18:43,119 Speaker 1: gravity can't do everything. It's opposed by this rotation. The 348 00:18:43,240 --> 00:18:46,280 Speaker 1: rotation keeps it from falling into the very center. That's 349 00:18:46,320 --> 00:18:48,760 Speaker 1: why the Earth is in orbit around the Sun rather 350 00:18:48,760 --> 00:18:51,040 Speaker 1: than just falling in. That's why the Moon is in 351 00:18:51,240 --> 00:18:54,560 Speaker 1: orbit around the Earth rather than just falling in. But 352 00:18:54,640 --> 00:18:57,439 Speaker 1: in the other direction, perpendicular to the plane of the 353 00:18:57,440 --> 00:19:01,040 Speaker 1: Solar System, there's no rotation, and so gravity can do 354 00:19:01,119 --> 00:19:03,560 Speaker 1: its job and it flattens things as much as it can. 355 00:19:04,320 --> 00:19:07,280 Speaker 1: So gravity does all this work, and some of the 356 00:19:07,320 --> 00:19:09,240 Speaker 1: stuff is spread out, some of the gas and the 357 00:19:09,320 --> 00:19:12,040 Speaker 1: dust doesn't fall all the way into the center because 358 00:19:12,080 --> 00:19:14,960 Speaker 1: of this rotation. So the stuff in the center condenses 359 00:19:15,000 --> 00:19:17,440 Speaker 1: into a star, and the rest of the stuff grabs 360 00:19:17,480 --> 00:19:20,560 Speaker 1: itself together. It forms into these distributed objects, and that's 361 00:19:20,560 --> 00:19:23,160 Speaker 1: how you get the planets. The planets are only there 362 00:19:23,400 --> 00:19:26,480 Speaker 1: because the original blob was rotating. If it wasn't rotating, 363 00:19:26,640 --> 00:19:28,840 Speaker 1: we would just have one star. But now you have 364 00:19:28,920 --> 00:19:32,119 Speaker 1: these large gravitational objects, these planets, and they start to 365 00:19:32,119 --> 00:19:35,159 Speaker 1: affect the stuff around them. And Jupiter, of course, is 366 00:19:35,240 --> 00:19:38,480 Speaker 1: the monster planet. It has most of the mass of 367 00:19:38,520 --> 00:19:41,639 Speaker 1: all the planets. It's tiny compared to the Sun, but 368 00:19:41,680 --> 00:19:44,119 Speaker 1: of course it's huge compared to the Earth. And it 369 00:19:44,200 --> 00:19:47,760 Speaker 1: has its own gravity, and that gravity is very powerful, 370 00:19:47,960 --> 00:19:50,120 Speaker 1: and it yanks and it pulls on things. We've talked 371 00:19:50,119 --> 00:19:53,040 Speaker 1: to in this podcast about how Jupiter massages its own 372 00:19:53,119 --> 00:19:56,440 Speaker 1: moons because of the tidal forces, and this is exactly 373 00:19:56,440 --> 00:19:59,560 Speaker 1: the issue. We think that the gravity from Jupiter is 374 00:19:59,640 --> 00:20:02,760 Speaker 1: too strong to let the stuff in the asteroid belt 375 00:20:03,000 --> 00:20:06,400 Speaker 1: ever pull together to form a planet. So the asteroid 376 00:20:06,400 --> 00:20:09,480 Speaker 1: belt is sort of like leftovers from the original formation 377 00:20:09,520 --> 00:20:12,240 Speaker 1: of the Solar System. We think that a long time ago, 378 00:20:12,680 --> 00:20:15,280 Speaker 1: maybe in the first ten million years of the Solar System, 379 00:20:15,560 --> 00:20:17,800 Speaker 1: most of the Solar System looked a lot like the 380 00:20:17,840 --> 00:20:20,200 Speaker 1: asteroid belt ahead rocks and chunks of stuff that were 381 00:20:20,240 --> 00:20:23,919 Speaker 1: slowly gathering together. But Jupiter prevents those rocks in the 382 00:20:23,920 --> 00:20:26,879 Speaker 1: asteroid belt from getting any further. It keeps them down 383 00:20:27,160 --> 00:20:29,720 Speaker 1: from creating their own planet. It's like Jupiter is like 384 00:20:29,760 --> 00:20:32,719 Speaker 1: a union buster, right. It says, nobody get together. I'm 385 00:20:32,720 --> 00:20:36,120 Speaker 1: gonna treat you all individually. And so the tidal forces 386 00:20:36,119 --> 00:20:39,520 Speaker 1: from Jupiter prevent this from happening. Every time Jupiter sweeps around, 387 00:20:39,560 --> 00:20:41,960 Speaker 1: it tugs on all these objects and prevents them from 388 00:20:42,000 --> 00:20:46,040 Speaker 1: gathering together. Remember, gravity is slow, and gravity is gentle 389 00:20:46,280 --> 00:20:49,040 Speaker 1: and it doesn't take that much perturbation to prevent it 390 00:20:49,320 --> 00:20:51,639 Speaker 1: from pulling all of this stuff together. And Jupiter is 391 00:20:51,680 --> 00:20:54,680 Speaker 1: a big, popa planet, and when it sweeps around it 392 00:20:54,720 --> 00:20:56,959 Speaker 1: messes it all up. And you might think, well, if 393 00:20:57,040 --> 00:20:59,199 Speaker 1: Jupiter can do that on the inside, wasn't to do 394 00:20:59,240 --> 00:21:01,399 Speaker 1: that on the out side. Well, the reason is that 395 00:21:01,400 --> 00:21:03,640 Speaker 1: Saturn is further away from Jupiter. There's a bit more 396 00:21:03,680 --> 00:21:06,760 Speaker 1: space there, and literally there's more space there, not just 397 00:21:06,800 --> 00:21:10,040 Speaker 1: in the gap between the objects, but because Saturn is 398 00:21:10,080 --> 00:21:13,119 Speaker 1: further out, it has much more space to move, and 399 00:21:13,200 --> 00:21:16,159 Speaker 1: Jupiter's gravity drops from much more rapidly as you got 400 00:21:16,240 --> 00:21:19,000 Speaker 1: on the outside compared to being on the inside. While 401 00:21:19,040 --> 00:21:21,440 Speaker 1: it seems more dramatic to have had a planet there 402 00:21:21,440 --> 00:21:23,520 Speaker 1: which then got torn up in some sort of ancient 403 00:21:23,560 --> 00:21:26,880 Speaker 1: battle or collision between objects, that's not the case. In fact, 404 00:21:27,119 --> 00:21:29,880 Speaker 1: nothing really even got started there. They think there used 405 00:21:29,920 --> 00:21:32,160 Speaker 1: to be a lot more asteroids than the asteroid belt 406 00:21:32,440 --> 00:21:34,720 Speaker 1: when the Solar System was young, but then those got 407 00:21:34,720 --> 00:21:37,560 Speaker 1: tugged out of orbit and collided and probably a lot 408 00:21:37,560 --> 00:21:39,520 Speaker 1: of those hit the Earth. There's this period in the 409 00:21:39,560 --> 00:21:42,600 Speaker 1: early Solar System called the late heavy bombardment when a 410 00:21:42,680 --> 00:21:45,199 Speaker 1: lot of objects came raining in and landing on the 411 00:21:45,240 --> 00:21:47,760 Speaker 1: Earth and the other inner planets. So most of the 412 00:21:47,800 --> 00:21:50,439 Speaker 1: asteroid belt from the very early days has been lost, 413 00:21:50,720 --> 00:21:53,440 Speaker 1: either due to collisions like we talked about earlier, hitting 414 00:21:53,440 --> 00:21:56,280 Speaker 1: other planets, or just getting tugged out of their orbit 415 00:21:56,480 --> 00:21:59,560 Speaker 1: by Jupiter. So what we have is a small remnant 416 00:21:59,800 --> 00:22:02,520 Speaker 1: of our original asteroid belt. We're lucky, frankly, they even 417 00:22:02,560 --> 00:22:05,160 Speaker 1: have it at all. But there are some really fascinating 418 00:22:05,160 --> 00:22:08,040 Speaker 1: objects in the asteroid belt, and one in particular, that 419 00:22:08,119 --> 00:22:11,760 Speaker 1: dwarf planet Series that holds a special mystery, one that's 420 00:22:11,800 --> 00:22:14,199 Speaker 1: been in my mind for years, and we'll talk all 421 00:22:14,240 --> 00:22:29,480 Speaker 1: about it, but first let's take another break, al right. 422 00:22:29,560 --> 00:22:31,760 Speaker 1: So we're talking about the mysteries of the asteroid belt, 423 00:22:32,040 --> 00:22:34,520 Speaker 1: why we have it where it is, what's in the 424 00:22:34,560 --> 00:22:37,880 Speaker 1: asteroid belt, And the big Papa asteroid in the asteroid 425 00:22:37,880 --> 00:22:40,720 Speaker 1: belt is actually a planet, and it's called Series C 426 00:22:40,920 --> 00:22:44,000 Speaker 1: E R E S. And it's pretty big. It's almost 427 00:22:44,040 --> 00:22:47,360 Speaker 1: a thousand kilometers in diameter. This is no small rock. 428 00:22:47,440 --> 00:22:50,159 Speaker 1: This is something to be taken seriously. And Series is 429 00:22:50,200 --> 00:22:53,199 Speaker 1: a fascinating object for many reasons. But the thing that 430 00:22:53,320 --> 00:22:56,560 Speaker 1: really sticks out of me is something which literally sticks out. 431 00:22:57,119 --> 00:22:59,080 Speaker 1: They sent a probe past and it took a picture 432 00:22:59,080 --> 00:23:02,680 Speaker 1: of Series, and he saw something really weird on the surface. 433 00:23:02,840 --> 00:23:04,880 Speaker 1: All right, if you haven't heard of this before, it's 434 00:23:04,920 --> 00:23:06,960 Speaker 1: gonna blow your mind. It blew my mind when I 435 00:23:07,000 --> 00:23:09,920 Speaker 1: heard it. Series has something on it which looks like 436 00:23:10,240 --> 00:23:14,200 Speaker 1: a pyramid. Now, I know, pyramids are a favorite element 437 00:23:14,320 --> 00:23:17,320 Speaker 1: of stories of the occult, and people think maybe aliens 438 00:23:17,359 --> 00:23:19,879 Speaker 1: came to Earth and built pyramids and all sorts of stuff, 439 00:23:20,040 --> 00:23:22,359 Speaker 1: and a lot of that, of course, is nonsense. But 440 00:23:22,520 --> 00:23:25,879 Speaker 1: there is a weird pyramid on Series. And when I 441 00:23:25,920 --> 00:23:30,200 Speaker 1: first saw these pictures, I gasped. I thought, oh my gosh, 442 00:23:30,480 --> 00:23:33,920 Speaker 1: maybe this is the moment we find an alien artifact. 443 00:23:34,200 --> 00:23:36,280 Speaker 1: And I read a lot of science fiction and I'm 444 00:23:36,359 --> 00:23:39,359 Speaker 1: desperate defined aliens, and in a lot of those science 445 00:23:39,400 --> 00:23:43,080 Speaker 1: fiction stories where humanity comes across aliens, this is how 446 00:23:43,119 --> 00:23:46,480 Speaker 1: it starts. We find some weird feature on somewhere in 447 00:23:46,480 --> 00:23:48,919 Speaker 1: the Solar System and can't be explained. I mean, think 448 00:23:48,960 --> 00:23:51,520 Speaker 1: about two thousand and one, right, the monolith it was 449 00:23:51,560 --> 00:23:55,359 Speaker 1: there orbiting Jupiter. What we're looking for is something unnatural, 450 00:23:55,440 --> 00:24:00,000 Speaker 1: something strange, something which we cannot explain without invoking intelligent life. 451 00:24:00,440 --> 00:24:04,439 Speaker 1: And something like a pyramid. Wow, that's amazing. Now, this 452 00:24:04,520 --> 00:24:07,960 Speaker 1: pyramid on Series is pretty weird. First of all, it 453 00:24:08,200 --> 00:24:13,440 Speaker 1: rises five thousand meters above the surface. That's not tiny. 454 00:24:13,480 --> 00:24:18,080 Speaker 1: That's enormous, especially compared to the size of Series. It's 455 00:24:18,119 --> 00:24:22,359 Speaker 1: fully one percent of the height of Series itself. If 456 00:24:22,400 --> 00:24:24,240 Speaker 1: you had an object, if you had a feature that 457 00:24:24,400 --> 00:24:27,520 Speaker 1: big on Earth, it would be eight times higher than 458 00:24:27,560 --> 00:24:31,199 Speaker 1: Mount Everest right in relative size to the Earth. So 459 00:24:31,280 --> 00:24:33,480 Speaker 1: this is not a tiny mountain. If you are on Series, 460 00:24:33,760 --> 00:24:36,120 Speaker 1: you would definitely know about it. It seems like it's 461 00:24:36,119 --> 00:24:39,240 Speaker 1: about two hundred million years old. And they can date 462 00:24:39,280 --> 00:24:42,720 Speaker 1: these things by seeing how many collisions there are nearby stuff. 463 00:24:43,000 --> 00:24:45,359 Speaker 1: You can tell how old something is on in the 464 00:24:45,400 --> 00:24:48,040 Speaker 1: Solar System just by counting the sort of collision to 465 00:24:48,080 --> 00:24:50,960 Speaker 1: impact craters, because everything in the Solar System eventually is 466 00:24:51,040 --> 00:24:53,600 Speaker 1: hit with little rocks. Now, NASA, when they first saw it, 467 00:24:53,840 --> 00:24:55,840 Speaker 1: they announced this and they describe this, and I'm gonna 468 00:24:55,920 --> 00:24:59,680 Speaker 1: quote here they say, it's quote like nothing humanity has 469 00:24:59,760 --> 00:25:02,920 Speaker 1: ever scene. And not only is it something we've never 470 00:25:02,960 --> 00:25:06,200 Speaker 1: seen before, there's not even any other one on Series. 471 00:25:06,680 --> 00:25:09,320 Speaker 1: It's not like we saw this planet and we're like, oh, look, 472 00:25:09,359 --> 00:25:12,160 Speaker 1: it has all these weird bumps on it. How could 473 00:25:12,160 --> 00:25:15,159 Speaker 1: that be? What makes those It's maybe evidence of some 474 00:25:15,240 --> 00:25:18,840 Speaker 1: new geological feature. There's only one. So we have this 475 00:25:19,040 --> 00:25:22,640 Speaker 1: weird planet in the asteroid belt with this strange pyramid 476 00:25:22,680 --> 00:25:25,720 Speaker 1: on it. And this is not just a mountain which 477 00:25:25,760 --> 00:25:28,280 Speaker 1: looks a little bit like a pyramid. The first pictures 478 00:25:28,480 --> 00:25:30,720 Speaker 1: it looked a lot like a pyramid. It looked like 479 00:25:30,760 --> 00:25:33,159 Speaker 1: an artificial structure. This is the kind of thing that 480 00:25:33,200 --> 00:25:36,159 Speaker 1: makes people go, wow, we better get another picture of 481 00:25:36,200 --> 00:25:38,280 Speaker 1: this thing. And so of course they did. They sent 482 00:25:38,359 --> 00:25:40,679 Speaker 1: out more probes and they focus telescopes on it, and 483 00:25:40,760 --> 00:25:44,160 Speaker 1: everybody wanted to know what is this weird thing on Series? 484 00:25:44,400 --> 00:25:47,240 Speaker 1: And the short answer is we still don't really know. 485 00:25:47,720 --> 00:25:51,920 Speaker 1: There are some nice ideas. People think that Series underneath 486 00:25:52,160 --> 00:25:55,000 Speaker 1: has a molten core, but it's not molten rock. The 487 00:25:55,080 --> 00:25:57,639 Speaker 1: inside of the earth. When you dig down into the earth, 488 00:25:57,920 --> 00:26:01,360 Speaker 1: this molten rock. Because of all the pressure, Series has 489 00:26:01,560 --> 00:26:04,919 Speaker 1: molten mud. Right. Do you think that there's water on Series? 490 00:26:05,000 --> 00:26:07,600 Speaker 1: Maybe liquid water and it combines with a service to 491 00:26:07,600 --> 00:26:11,239 Speaker 1: make this sort of molten mud, and that sometimes this 492 00:26:11,359 --> 00:26:14,359 Speaker 1: mud might push up or spew up based on something 493 00:26:14,400 --> 00:26:18,000 Speaker 1: happening on the inside of series, and this mud is 494 00:26:18,040 --> 00:26:20,280 Speaker 1: actually not that hot, and so they call this sort 495 00:26:20,280 --> 00:26:24,800 Speaker 1: of like a cryo volcano, like a cold volcano. So 496 00:26:24,840 --> 00:26:28,639 Speaker 1: they think it's like some salty, rocky, frozen mud that 497 00:26:28,760 --> 00:26:30,840 Speaker 1: came out from the interior and pushed up like a 498 00:26:30,880 --> 00:26:34,480 Speaker 1: big ZiT. And that's possible, and they have some simulations 499 00:26:34,480 --> 00:26:37,120 Speaker 1: that suggests this kind of thing could happen. But then 500 00:26:37,440 --> 00:26:40,159 Speaker 1: why is there only one? Why is there just this 501 00:26:40,440 --> 00:26:42,719 Speaker 1: one feature? If this is the kind of thing that 502 00:26:42,800 --> 00:26:45,920 Speaker 1: happens inside series, you would expect to see more than one, 503 00:26:46,280 --> 00:26:48,880 Speaker 1: and you'd expect to see big ones and then lots 504 00:26:48,960 --> 00:26:52,720 Speaker 1: of little ones. But you know, sometimes weird things happen. 505 00:26:52,800 --> 00:26:55,560 Speaker 1: Sometimes in the solar system, there's a one off event, 506 00:26:56,040 --> 00:26:58,840 Speaker 1: and that could explain it. It could just be a strange, 507 00:26:59,080 --> 00:27:02,119 Speaker 1: one off event in the solar system that nobody understands. 508 00:27:02,880 --> 00:27:06,960 Speaker 1: Or hey, it could be aliens. We're still not are now. 509 00:27:07,240 --> 00:27:09,480 Speaker 1: Don't go running off and tell people that Daniel said 510 00:27:09,480 --> 00:27:12,959 Speaker 1: they're aliens in the Solar system. There probably aren't. That 511 00:27:13,040 --> 00:27:17,080 Speaker 1: kind of explanation requires extraordinary evidence. But I really enjoy 512 00:27:17,160 --> 00:27:19,919 Speaker 1: thinking about it. I really enjoy holding out hope that 513 00:27:20,040 --> 00:27:22,119 Speaker 1: maybe one of these things we're seeing in the Solar 514 00:27:22,160 --> 00:27:24,479 Speaker 1: system is not just going to tell us about the 515 00:27:24,480 --> 00:27:26,879 Speaker 1: origins of our solar system and how it was formed 516 00:27:26,920 --> 00:27:29,960 Speaker 1: and how planets are formed, and how solar systems everywhere 517 00:27:30,000 --> 00:27:32,520 Speaker 1: put together, and those are all fascinating questions I want 518 00:27:32,600 --> 00:27:35,160 Speaker 1: the answer to. But I'm holding out hope that maybe 519 00:27:35,200 --> 00:27:37,520 Speaker 1: there's a clue in our Solar system of something weirder, 520 00:27:37,840 --> 00:27:41,720 Speaker 1: something grander, something which reveals the secret about the universe 521 00:27:41,760 --> 00:27:44,159 Speaker 1: we have been dying to know the answer to, namely, 522 00:27:44,520 --> 00:27:47,240 Speaker 1: are we alone? And so it turns out that the 523 00:27:47,240 --> 00:27:49,920 Speaker 1: asteroid belt not only does it have lots of these 524 00:27:49,960 --> 00:27:52,800 Speaker 1: fun mysteries in it, but there's lots of places to hide. 525 00:27:52,840 --> 00:27:55,880 Speaker 1: There's lots of these asteroids we haven't examined, and there's 526 00:27:55,880 --> 00:27:58,439 Speaker 1: still the possibility that we could land on one of 527 00:27:58,440 --> 00:28:00,879 Speaker 1: these and explore it and find some thing weird, something 528 00:28:01,080 --> 00:28:04,320 Speaker 1: weirder even than a pyramid. We could find alien technology, 529 00:28:04,400 --> 00:28:06,800 Speaker 1: We could find all sorts of crazy stuff. The point 530 00:28:06,880 --> 00:28:09,040 Speaker 1: is that there's a huge amount of area in our 531 00:28:09,080 --> 00:28:13,720 Speaker 1: Solar system that remains unexplored, lots of opportunities to find life, 532 00:28:13,880 --> 00:28:17,000 Speaker 1: to find alien civilization, to find all sorts of crazy 533 00:28:17,040 --> 00:28:20,000 Speaker 1: stuff that would literally blow our minds. And so while 534 00:28:20,040 --> 00:28:22,479 Speaker 1: we should zoom our minds around the universe and think 535 00:28:22,520 --> 00:28:25,040 Speaker 1: about all the crazy stuff happening far away and also 536 00:28:25,359 --> 00:28:28,800 Speaker 1: under our feet, remember that right here in our neighborhood 537 00:28:28,920 --> 00:28:32,920 Speaker 1: there are plenty of opportunities to make mind blowing, earth shattering, 538 00:28:33,320 --> 00:28:37,640 Speaker 1: paradigm shifting discoveries. All right, this has been an episode 539 00:28:37,640 --> 00:28:40,320 Speaker 1: of Daniel and Jorge Explain the Universe, all about the 540 00:28:40,400 --> 00:28:43,240 Speaker 1: mysteries of the Asteroid Belt. Thanks for tuning in, and 541 00:28:43,320 --> 00:28:45,640 Speaker 1: if you have questions about something you'd like to hear 542 00:28:45,720 --> 00:28:48,560 Speaker 1: us talk about, please send them to us at Questions 543 00:28:48,600 --> 00:28:51,800 Speaker 1: at Daniel and Jorge dot com. Thanks for tuning in. 544 00:28:59,640 --> 00:29:02,000 Speaker 1: If you still have a question after listening to all 545 00:29:02,040 --> 00:29:05,280 Speaker 1: these explanations, please drop us a line. We'd love to 546 00:29:05,320 --> 00:29:07,720 Speaker 1: hear from you. You can find us at Facebook, Twitter, 547 00:29:07,800 --> 00:29:11,480 Speaker 1: and Instagram at Daniel and Jorge That's one word, or 548 00:29:11,600 --> 00:29:15,520 Speaker 1: email us at Feedback at Daniel and Jorge dot com. 549 00:29:15,520 --> 00:29:18,360 Speaker 1: Thanks for listening, and remember that Daniel and Jorge Explain 550 00:29:18,400 --> 00:29:21,280 Speaker 1: the Universe is a production of I Heart Radio. For 551 00:29:21,440 --> 00:29:24,360 Speaker 1: more podcast from my heart Radio, visit the i heart 552 00:29:24,440 --> 00:29:28,040 Speaker 1: Radio app, Apple Podcasts, or wherever you listen to your 553 00:29:28,080 --> 00:29:34,200 Speaker 1: favorite shows yea