1 00:00:08,039 --> 00:00:09,639 Speaker 1: You know, I look up at the sky at night, 2 00:00:09,840 --> 00:00:11,959 Speaker 1: and one of the most amazing things to stare at 3 00:00:11,960 --> 00:00:15,240 Speaker 1: as the moon, because it just seems so calm and peaceful, 4 00:00:15,320 --> 00:00:18,040 Speaker 1: hanging up there in the sky and looking down at us. Yeah, 5 00:00:18,160 --> 00:00:22,560 Speaker 1: moonlight is so calming, right and reassuring. Yes, especially if 6 00:00:22,600 --> 00:00:27,360 Speaker 1: you're a vampire or a werewolf. I heard that the 7 00:00:27,440 --> 00:00:33,040 Speaker 1: moon actually has this crazy, violent, cataclysmic past. Yeah, that's right, 8 00:00:33,080 --> 00:00:35,720 Speaker 1: hanging up there in the sky acting all common nights. 9 00:00:35,720 --> 00:00:37,760 Speaker 1: It turns out it may have been party to one 10 00:00:37,760 --> 00:00:40,080 Speaker 1: of the greatest murder mysteries in the history of the 11 00:00:40,120 --> 00:00:45,599 Speaker 1: Solar system, a very impactful event, that's right. And I 12 00:00:45,680 --> 00:00:48,559 Speaker 1: love when there are things hanging out right there on 13 00:00:48,600 --> 00:00:52,080 Speaker 1: our faces that give us clues as to great drama 14 00:00:52,280 --> 00:01:12,800 Speaker 1: that took place in deep dark history. Hi. I'm Jorge. 15 00:01:12,840 --> 00:01:16,000 Speaker 1: I'm a cartoonist, and I'm Daniel. I'm a particle physicist, 16 00:01:16,200 --> 00:01:18,920 Speaker 1: And welcome to our podcast. Daniel and Jorge explained the 17 00:01:19,000 --> 00:01:21,400 Speaker 1: universe in which we look around at anything in the 18 00:01:21,480 --> 00:01:25,200 Speaker 1: universe and try to explain it to you. On today's program, 19 00:01:25,319 --> 00:01:31,080 Speaker 1: that big white, shiny thing in the night sky, the 20 00:01:31,160 --> 00:01:34,319 Speaker 1: thing you referred to as the moon, not any moon, 21 00:01:34,880 --> 00:01:39,080 Speaker 1: Not a moon, The moon, the moon earth little sidekick. 22 00:01:39,720 --> 00:01:42,679 Speaker 1: That's right. And if you're a person who wonders and 23 00:01:42,720 --> 00:01:45,440 Speaker 1: thinks about the history of things, you like all of 24 00:01:45,520 --> 00:01:47,720 Speaker 1: humanity must have looked up in the night sky wondered 25 00:01:47,760 --> 00:01:49,800 Speaker 1: what are the stars? Where do they come from? But 26 00:01:49,880 --> 00:01:52,120 Speaker 1: the biggest thing, the fattest thing out there in the 27 00:01:52,240 --> 00:01:54,760 Speaker 1: night sky is the moon. And what a mystery that 28 00:01:54,840 --> 00:01:57,640 Speaker 1: must have presented to ancient man and woman. Right, what 29 00:01:57,760 --> 00:02:01,280 Speaker 1: is that giant disk and where did it come from? 30 00:02:01,360 --> 00:02:04,240 Speaker 1: That's right, And that's a question that science is still 31 00:02:04,280 --> 00:02:07,040 Speaker 1: trying to answer. We've gone to the moon, We've looked 32 00:02:07,040 --> 00:02:10,000 Speaker 1: at the moon with crazy telescopes, people have walked across 33 00:02:10,000 --> 00:02:12,320 Speaker 1: it and brought samples back. But we still don't know 34 00:02:12,360 --> 00:02:15,440 Speaker 1: the answer to the question how did the Earth get 35 00:02:15,520 --> 00:02:18,200 Speaker 1: its moon. That's a crazy idea to me that we 36 00:02:18,240 --> 00:02:20,800 Speaker 1: don't know where the moon came from, you know, like 37 00:02:20,919 --> 00:02:23,600 Speaker 1: we it could have just appeared out of door one day, 38 00:02:24,240 --> 00:02:26,920 Speaker 1: or aliens could have dropped it off. Oh that's an 39 00:02:26,960 --> 00:02:29,000 Speaker 1: option I haven't heard yet that like somebody opened a 40 00:02:29,040 --> 00:02:32,000 Speaker 1: wormhole in the moon just look popped, there's a moon 41 00:02:32,160 --> 00:02:35,320 Speaker 1: all of a sudden. That's an awesome idea. Yeah, how 42 00:02:35,320 --> 00:02:38,359 Speaker 1: does something that big just come about right, so perfectly 43 00:02:38,480 --> 00:02:42,960 Speaker 1: round and pretty smooth and bright. Yeah, but it turns 44 00:02:42,960 --> 00:02:45,240 Speaker 1: out the Earth's moon is not like the other moon's. 45 00:02:45,280 --> 00:02:47,200 Speaker 1: You know, one of these things is not like the 46 00:02:47,240 --> 00:02:49,920 Speaker 1: other things, and the moon is kind of weird, which 47 00:02:49,919 --> 00:02:52,720 Speaker 1: makes it hard to explain. Yeah, it's a weird moon. 48 00:02:53,960 --> 00:02:55,280 Speaker 1: It's the only one we have, and so for a 49 00:02:55,280 --> 00:02:58,440 Speaker 1: long time it's sort of defined the whole concept of moon. Right, 50 00:02:58,840 --> 00:03:00,839 Speaker 1: But now that we've seen other planet and we've seen 51 00:03:00,840 --> 00:03:03,320 Speaker 1: how many little moons they have, were like, jeez, our 52 00:03:03,360 --> 00:03:05,080 Speaker 1: moon is kind of weird. Does my moon make me 53 00:03:05,120 --> 00:03:08,320 Speaker 1: look fat? You know, because we've got a big, fat moon. Yeah. 54 00:03:08,440 --> 00:03:11,040 Speaker 1: So this is an interesting question, and we wondered how 55 00:03:11,080 --> 00:03:13,520 Speaker 1: many of you out there no or think they know 56 00:03:13,600 --> 00:03:16,480 Speaker 1: the answer to the question where did the moon come from? 57 00:03:16,760 --> 00:03:19,440 Speaker 1: So I walked around the campus of UC Irvine and 58 00:03:19,480 --> 00:03:22,240 Speaker 1: accosted random strangers who are willing to talk to me 59 00:03:22,280 --> 00:03:24,760 Speaker 1: and asked them this question, where do you think the 60 00:03:24,840 --> 00:03:27,440 Speaker 1: moon came from? Yeah, so before you listen to these answers, 61 00:03:27,520 --> 00:03:31,000 Speaker 1: think for yourself what would be your best guess. Here's 62 00:03:31,040 --> 00:03:33,760 Speaker 1: what people have to say. I'm not entirely certain. I 63 00:03:33,800 --> 00:03:36,920 Speaker 1: just know gravity plays a part in it. There was 64 00:03:36,960 --> 00:03:38,840 Speaker 1: like a meteorite that hit the Earth which broke off 65 00:03:38,880 --> 00:03:41,000 Speaker 1: some rocks or something like that. From what I remember, 66 00:03:41,200 --> 00:03:43,640 Speaker 1: it might be that, well this is like the big Thing, 67 00:03:43,800 --> 00:03:49,200 Speaker 1: but I don't really know, no, No, My best guess 68 00:03:49,360 --> 00:03:53,080 Speaker 1: is that it either came from some sort of material 69 00:03:53,200 --> 00:03:59,640 Speaker 1: that was already in the atmosphere and by some sort 70 00:03:59,680 --> 00:04:03,320 Speaker 1: of a potational pull was brought in. Alright, So not 71 00:04:03,440 --> 00:04:06,840 Speaker 1: a lot of strong ideas here. I think it's a 72 00:04:06,920 --> 00:04:09,760 Speaker 1: pretty there's a good breath of ideas. Yeah. I like 73 00:04:09,800 --> 00:04:11,560 Speaker 1: the people who answer where did the moon come from? 74 00:04:11,800 --> 00:04:16,560 Speaker 1: And they would just say gravity, Like that's the answer too, 75 00:04:16,600 --> 00:04:20,320 Speaker 1: pretty much everything there, or the or someone said the 76 00:04:20,400 --> 00:04:23,400 Speaker 1: Big Bang. I'm like, yeah, of course everything came from 77 00:04:23,440 --> 00:04:26,360 Speaker 1: the Big Bang. That is that is a good default 78 00:04:26,360 --> 00:04:28,320 Speaker 1: physics answer that somebody asked you a physics question. The 79 00:04:28,320 --> 00:04:31,000 Speaker 1: answer is always the Big Bang. How does the hig 80 00:04:31,040 --> 00:04:35,000 Speaker 1: boson give mass to other particles? It's the Big Bang? Really, 81 00:04:35,120 --> 00:04:37,760 Speaker 1: you can't go wrong. So could have see that person 82 00:04:37,839 --> 00:04:44,280 Speaker 1: on the street figured out how to always be right? Well, 83 00:04:44,360 --> 00:04:46,919 Speaker 1: let's talk about the moon. How big is the moon? Daniel? 84 00:04:47,200 --> 00:04:50,159 Speaker 1: Or let's maybe take a step back. What is the moon? Right, 85 00:04:50,200 --> 00:04:52,800 Speaker 1: So it's just a definitional thing, right. You have solar 86 00:04:52,839 --> 00:04:55,440 Speaker 1: systems that have these hierarchies. You almost always have the 87 00:04:55,480 --> 00:04:58,520 Speaker 1: main masses in the center. You have star where most 88 00:04:58,520 --> 00:05:01,080 Speaker 1: of this has gathered, and then you have the planets 89 00:05:01,360 --> 00:05:03,080 Speaker 1: orbiting around it. And then you know, you have need 90 00:05:03,080 --> 00:05:05,520 Speaker 1: a name for the stuff orbiting around the planets. The 91 00:05:05,640 --> 00:05:07,440 Speaker 1: theory this could go on forever. Right, you have the 92 00:05:07,440 --> 00:05:10,719 Speaker 1: star with planets around it, and then moons around the planets, 93 00:05:10,800 --> 00:05:12,640 Speaker 1: and then you can have things orbiting around the moon, 94 00:05:13,120 --> 00:05:16,120 Speaker 1: and then things orbiting around those things, like moons can 95 00:05:16,200 --> 00:05:18,960 Speaker 1: have moonies. Yeah, I think they're called moonlits moon or 96 00:05:19,040 --> 00:05:23,960 Speaker 1: moon ETOs or something. Yeah. So so it's just it's 97 00:05:24,040 --> 00:05:29,039 Speaker 1: just the name given to something floating around a planet. Yeah, exactly. 98 00:05:29,080 --> 00:05:30,960 Speaker 1: If you're a blob of stuff floating around the planet, 99 00:05:31,000 --> 00:05:33,000 Speaker 1: then we call you a moon. But it's interesting because 100 00:05:33,000 --> 00:05:34,880 Speaker 1: you've got to be big enough, right, Like, if you're 101 00:05:34,920 --> 00:05:37,480 Speaker 1: just specks of stuff, then we call you a ring. Right, 102 00:05:37,480 --> 00:05:39,560 Speaker 1: if you're like distributed all the way around the planet, 103 00:05:39,680 --> 00:05:42,240 Speaker 1: then we got then you've got rings, Like Saturn has rings. 104 00:05:42,400 --> 00:05:46,160 Speaker 1: Saturn's got rings Jupiter's got rings, you know. Um, and 105 00:05:46,480 --> 00:05:48,760 Speaker 1: it's in some ways a question of definition, Like there 106 00:05:48,839 --> 00:05:51,240 Speaker 1: is stuff floating around the Earth into sort of a vague, 107 00:05:51,360 --> 00:05:53,560 Speaker 1: hazy rings. So could you say the Earth has rings? 108 00:05:53,680 --> 00:05:55,640 Speaker 1: You know, people argue about that kind of stuff, but 109 00:05:55,640 --> 00:05:57,800 Speaker 1: that's just like that's arguing about the definition. It's not 110 00:05:57,839 --> 00:06:00,080 Speaker 1: really arguing about the science generally. But it has it 111 00:06:00,120 --> 00:06:03,000 Speaker 1: has to have a certain size to be called a moon, 112 00:06:03,360 --> 00:06:07,920 Speaker 1: I think, so, yeah, otherwise it's just a rock rock 113 00:06:08,360 --> 00:06:12,360 Speaker 1: rock or rock let or rocky rocky dough. Yeah, there 114 00:06:12,440 --> 00:06:15,560 Speaker 1: must be some organization out there that's tasked with classifying 115 00:06:15,600 --> 00:06:17,560 Speaker 1: what the moon and what's the moonlit, and what's just 116 00:06:17,600 --> 00:06:20,480 Speaker 1: a piece of ring and with just random garbage in space. 117 00:06:20,600 --> 00:06:23,680 Speaker 1: You know. Um, that doesn't sound a very glamorous job. 118 00:06:24,080 --> 00:06:26,520 Speaker 1: So how big is our moon? Our Our moon is 119 00:06:26,600 --> 00:06:30,680 Speaker 1: really big. Our moon is two thousand miles across, which 120 00:06:30,720 --> 00:06:32,400 Speaker 1: is pretty big compared to the Earth, which you know, 121 00:06:32,520 --> 00:06:35,280 Speaker 1: is only eight thousand miles across, and most of the 122 00:06:35,320 --> 00:06:38,039 Speaker 1: other planets their moons are tiny in comparison to the 123 00:06:38,080 --> 00:06:40,000 Speaker 1: size of the planet. So it's pretty big. So it's 124 00:06:40,040 --> 00:06:44,440 Speaker 1: like from California to about like Arkansas or something, you're 125 00:06:44,480 --> 00:06:46,200 Speaker 1: giving me the worries here, Like if you took the 126 00:06:46,240 --> 00:06:48,600 Speaker 1: Moon and sort of gently put it down, how far 127 00:06:48,680 --> 00:06:51,960 Speaker 1: would it would it look? Like? Why do you even 128 00:06:52,000 --> 00:06:54,720 Speaker 1: imagine that? Like placing the Moon on the Earth just 129 00:06:54,760 --> 00:06:57,000 Speaker 1: for scale, you know, like you were to walk across 130 00:06:57,000 --> 00:07:00,280 Speaker 1: the Moon, how long would it take you? You know? Right? Yeah, um, 131 00:07:00,279 --> 00:07:01,920 Speaker 1: well not that long because you could bounce because of 132 00:07:01,920 --> 00:07:04,360 Speaker 1: the gravity is pretty low. But yeah, it's like two 133 00:07:04,440 --> 00:07:06,480 Speaker 1: thousand miles, so it's not as far as l A 134 00:07:06,560 --> 00:07:08,680 Speaker 1: to New York, for example. But it's pretty big, right, 135 00:07:08,680 --> 00:07:10,760 Speaker 1: It's pretty big. And the interesting thing is that it's 136 00:07:10,800 --> 00:07:15,119 Speaker 1: at the same scale as other planets in the Solar System. Okay, 137 00:07:15,120 --> 00:07:17,160 Speaker 1: so I looked it up, uh, and I did some 138 00:07:17,240 --> 00:07:20,000 Speaker 1: quick calculations because I'm a train engineer and I can 139 00:07:20,280 --> 00:07:24,000 Speaker 1: do some math here, and so like if the Earth 140 00:07:24,080 --> 00:07:26,520 Speaker 1: was the size of a basketball, the Moon would be 141 00:07:26,800 --> 00:07:29,160 Speaker 1: a little bit under the size of a tennis ball. 142 00:07:29,280 --> 00:07:32,160 Speaker 1: I prefer I preferred fruit based analogy. So I'm gonna 143 00:07:32,160 --> 00:07:35,320 Speaker 1: go with a watermelon and an apple. Watermelon, and then 144 00:07:35,360 --> 00:07:37,560 Speaker 1: are you hungry, Daniel? Do we need to take a 145 00:07:37,640 --> 00:07:40,560 Speaker 1: break here and break for a while? A right, as 146 00:07:40,600 --> 00:07:43,800 Speaker 1: a watermelon and an apple. Except what this interesting? The 147 00:07:43,840 --> 00:07:47,480 Speaker 1: distance is maybe a lot larger than most people think. So, 148 00:07:47,520 --> 00:07:51,120 Speaker 1: like you would have to put a watermelon down and 149 00:07:51,120 --> 00:07:54,240 Speaker 1: then walked about twenty five ft and then set down 150 00:07:54,320 --> 00:07:57,320 Speaker 1: that apple. And that's about the distance between the Earth 151 00:07:57,640 --> 00:08:01,720 Speaker 1: and the Moon. Yeah, it's crazy. These things seem big, 152 00:08:01,720 --> 00:08:04,280 Speaker 1: but they're tiny compared to the distances between them, right, 153 00:08:04,320 --> 00:08:07,480 Speaker 1: which is sort of a larger lesson for everything in space, right, 154 00:08:07,480 --> 00:08:09,840 Speaker 1: Like the Sun and the Earth seem huge, but they're 155 00:08:09,920 --> 00:08:13,040 Speaker 1: really far apart compared to their diameters. And our solar 156 00:08:13,080 --> 00:08:15,720 Speaker 1: system is far from the next star and and it's 157 00:08:15,760 --> 00:08:19,040 Speaker 1: incredible the distances between stuff and space. Yeah, okay, so 158 00:08:19,080 --> 00:08:22,360 Speaker 1: that's the moon. Um. The crazy thing is that we 159 00:08:22,360 --> 00:08:24,679 Speaker 1: don't know where the moon came from. That's right. People 160 00:08:24,680 --> 00:08:27,000 Speaker 1: have been trying to figure out how do you get 161 00:08:27,000 --> 00:08:30,400 Speaker 1: the Moon this big and this weird around the planet 162 00:08:30,520 --> 00:08:33,200 Speaker 1: this close to the Sun, and they can't figure it out. 163 00:08:33,280 --> 00:08:35,120 Speaker 1: You know, they have simulations and theories, and you know, 164 00:08:35,160 --> 00:08:37,600 Speaker 1: this is what scientists do. They say, can we explain 165 00:08:37,640 --> 00:08:39,720 Speaker 1: what we see? And they start with an idea and 166 00:08:39,760 --> 00:08:42,200 Speaker 1: they see does that work? Right? Can I take that 167 00:08:42,280 --> 00:08:44,520 Speaker 1: idea and end up with the situation I see in 168 00:08:44,559 --> 00:08:47,160 Speaker 1: front of me, and they have some ideas, and we'll 169 00:08:47,160 --> 00:08:49,439 Speaker 1: talk about them, we'll dig into them. But the bottom 170 00:08:49,440 --> 00:08:51,480 Speaker 1: line is that none of the ideas we currently have 171 00:08:51,720 --> 00:08:55,160 Speaker 1: completely work. They all have problems, which suggests that the 172 00:08:55,200 --> 00:08:57,280 Speaker 1: answer is something we haven't yet thought of, or some 173 00:08:57,360 --> 00:09:01,000 Speaker 1: weird twist on one of the current ideas. All right, 174 00:09:01,080 --> 00:09:03,360 Speaker 1: bring it down for us. How what are the different 175 00:09:03,360 --> 00:09:06,120 Speaker 1: ways that a planet can get a moon? Like? If 176 00:09:06,120 --> 00:09:08,320 Speaker 1: I wanted a moon, what would I need to do? 177 00:09:08,360 --> 00:09:10,600 Speaker 1: You just go on Amazon, man, you can order anything. Well, 178 00:09:10,720 --> 00:09:13,040 Speaker 1: you can probably get a moon. Tomort. You want a moon, 179 00:09:13,160 --> 00:09:15,040 Speaker 1: I get you a moon by tomorrow afternoon. That's what 180 00:09:15,080 --> 00:09:16,920 Speaker 1: Walter from the Big Labowski would saying. Can I just 181 00:09:16,960 --> 00:09:19,320 Speaker 1: get a slightly a shorter person to just follow me 182 00:09:19,360 --> 00:09:23,880 Speaker 1: around and turn around me? That's not a moon, that 183 00:09:23,880 --> 00:09:27,200 Speaker 1: that's an assistant. You want somebody in your orbit, right 184 00:09:27,400 --> 00:09:30,079 Speaker 1: who protects you from stuff? Right, cleans out all the 185 00:09:30,120 --> 00:09:32,440 Speaker 1: space junk that's coming at you. Um. Yeah, So how 186 00:09:32,440 --> 00:09:35,040 Speaker 1: does the planet get a moon? Well? One option is 187 00:09:35,080 --> 00:09:37,360 Speaker 1: that it's formed when the planet is formed. Right, Let's 188 00:09:37,360 --> 00:09:40,199 Speaker 1: remember how our planets formed, and it's um not from 189 00:09:40,200 --> 00:09:43,720 Speaker 1: the Big Bang, right, Like our professional physicist from earlier. Directly, 190 00:09:43,760 --> 00:09:46,760 Speaker 1: it is from gravity though, So you're saying that the 191 00:09:47,120 --> 00:09:49,560 Speaker 1: planet can get a moon at the same time that 192 00:09:49,640 --> 00:09:52,760 Speaker 1: it's forming, kind of like a little twin brother. Yeah, exactly. 193 00:09:52,760 --> 00:09:54,840 Speaker 1: So imagine how is the planet formed. Well, it starts 194 00:09:54,840 --> 00:09:57,200 Speaker 1: from a big poof of gas and dust and rocks, right, 195 00:09:57,200 --> 00:10:00,800 Speaker 1: and then gravity coalesces it together gradually, slowly, slowly into 196 00:10:00,800 --> 00:10:03,000 Speaker 1: a big clump. And you might wonder, why doesn't it 197 00:10:03,040 --> 00:10:05,280 Speaker 1: all form into one big clump, right? Why do you 198 00:10:05,280 --> 00:10:09,040 Speaker 1: get little bits left over as moons or other stuff? Um? 199 00:10:09,080 --> 00:10:10,960 Speaker 1: And this sort of two answers to that, like most 200 00:10:10,960 --> 00:10:13,199 Speaker 1: of it goes into the big clump. Right. First of all, 201 00:10:13,360 --> 00:10:15,800 Speaker 1: like most of the stuff goes into the planet. Um. 202 00:10:15,960 --> 00:10:17,600 Speaker 1: The reason it doesn't all is that some of it's 203 00:10:17,640 --> 00:10:21,040 Speaker 1: traveling really fast, and so rather than getting pulled down 204 00:10:21,120 --> 00:10:23,679 Speaker 1: into the central clump, essentially ends up in orbit. Right. 205 00:10:24,040 --> 00:10:26,320 Speaker 1: So what we call in physics, we call it angular momentum. 206 00:10:26,360 --> 00:10:28,760 Speaker 1: Supported you know, it's the reason that the Earth doesn't 207 00:10:28,800 --> 00:10:32,080 Speaker 1: just fall into the Sun. Right, It's because it's moving fast. Oh. 208 00:10:32,280 --> 00:10:34,320 Speaker 1: I see, So there's a bunch of stuff that came together, 209 00:10:34,520 --> 00:10:37,040 Speaker 1: But some of that stuff was a little bit out 210 00:10:37,040 --> 00:10:40,240 Speaker 1: on the periphery and didn't quite make it into the 211 00:10:40,280 --> 00:10:43,520 Speaker 1: main planet clump exactly. And it's all spinning, right, the 212 00:10:43,520 --> 00:10:46,120 Speaker 1: whole thing is spinning and it's going and so it 213 00:10:46,200 --> 00:10:48,960 Speaker 1: starts out spinning around and it's moving too fast to 214 00:10:48,960 --> 00:10:51,520 Speaker 1: get sucked in. Um. And the other part of the 215 00:10:51,559 --> 00:10:53,880 Speaker 1: story is that none of this happens in isolation, right. 216 00:10:53,920 --> 00:10:56,040 Speaker 1: The Earth is not in the middle of totally empty 217 00:10:56,080 --> 00:10:59,079 Speaker 1: space forming quietly. This stuff going on all the time, 218 00:10:59,120 --> 00:11:01,240 Speaker 1: And in the early soul or system, we think things 219 00:11:01,240 --> 00:11:04,200 Speaker 1: were pretty crazy and so um. It might have been 220 00:11:04,240 --> 00:11:06,000 Speaker 1: that the early blob that formed the Earth could have 221 00:11:06,080 --> 00:11:07,959 Speaker 1: formed a single planet with no moon and no other 222 00:11:08,000 --> 00:11:10,520 Speaker 1: objects or whatever. But it probably got perturbed a lot, 223 00:11:10,559 --> 00:11:13,000 Speaker 1: you know, things crash into it, things bump into it. 224 00:11:13,080 --> 00:11:15,280 Speaker 1: Even just the tugging of the Sun and other planets 225 00:11:15,280 --> 00:11:18,040 Speaker 1: coming nearby keep that stuff from really settling, and so 226 00:11:18,080 --> 00:11:20,800 Speaker 1: some of it ends up still out in space opening 227 00:11:20,840 --> 00:11:23,760 Speaker 1: around the planet. Okay, it formed at the same time 228 00:11:23,800 --> 00:11:26,959 Speaker 1: as the planet. Yeah, that happens in some cases, we think, um, 229 00:11:26,960 --> 00:11:28,800 Speaker 1: so sorry it's too late for you there. Or if 230 00:11:28,800 --> 00:11:31,160 Speaker 1: you wanted a moon from the from zero, you've missed 231 00:11:31,160 --> 00:11:34,240 Speaker 1: your window. I need to go back to the to 232 00:11:34,320 --> 00:11:39,680 Speaker 1: the womb. That's right, the womb moon the moon. That's 233 00:11:39,720 --> 00:11:43,000 Speaker 1: a that's a tongue twist right there. Um yeah. But 234 00:11:43,040 --> 00:11:45,240 Speaker 1: the better way, I think, the more popular way the 235 00:11:45,280 --> 00:11:48,120 Speaker 1: planets gives moves. All the cool planet at least get 236 00:11:48,200 --> 00:11:52,360 Speaker 1: moons by basically interacting with other objects. You know, like, um, 237 00:11:52,480 --> 00:11:55,360 Speaker 1: something smashes into them, or something flies by and they 238 00:11:55,440 --> 00:11:58,560 Speaker 1: capture it. Um, that kind of stuff. Wait wait wait wait, um, 239 00:11:58,600 --> 00:12:01,560 Speaker 1: so those are two other things. You can either capture 240 00:12:01,720 --> 00:12:04,560 Speaker 1: a moon, Like if the Earth was flying around and 241 00:12:04,600 --> 00:12:06,600 Speaker 1: suddenly there was a little bit of rock out there, 242 00:12:06,640 --> 00:12:09,160 Speaker 1: it would it could like bring it into its orbit. 243 00:12:09,480 --> 00:12:11,760 Speaker 1: It could bring it into its orbit. That's not very 244 00:12:11,800 --> 00:12:15,280 Speaker 1: easy to do because much more likely is that something 245 00:12:15,320 --> 00:12:18,440 Speaker 1: comes and smashes into the Earth and then the resulting 246 00:12:18,480 --> 00:12:23,199 Speaker 1: debris floats up into space and then turns into a 247 00:12:23,240 --> 00:12:26,439 Speaker 1: system of rings and then coalesces into a moon. That's 248 00:12:26,520 --> 00:12:29,959 Speaker 1: much more likely. It's because it's hard to capture something entirely. 249 00:12:30,280 --> 00:12:33,520 Speaker 1: Either it deflects right, it bounces off into space, or 250 00:12:33,520 --> 00:12:36,080 Speaker 1: it hits the Earth getting captured. It means you have 251 00:12:36,120 --> 00:12:38,440 Speaker 1: to be exactly the right speed at exactly the right 252 00:12:38,480 --> 00:12:41,199 Speaker 1: angle at exactly the right orbit. It's a difficult thing 253 00:12:41,200 --> 00:12:43,600 Speaker 1: to do. It's like getting a perfect pool shot, you know, 254 00:12:44,080 --> 00:12:46,559 Speaker 1: jumping the eight ball or something. You're saying, that's harder 255 00:12:46,600 --> 00:12:49,720 Speaker 1: than getting hit by something out in space. Yeah, because 256 00:12:49,720 --> 00:12:51,800 Speaker 1: the Earth has gravity, right, So if something comes close by, 257 00:12:51,840 --> 00:12:53,800 Speaker 1: it's most likely just going to spiral in and smash 258 00:12:53,880 --> 00:12:56,760 Speaker 1: into the Earth, or it's going to bounce off into flect. 259 00:12:56,840 --> 00:12:58,920 Speaker 1: So coming in from somewhere else and then ending up 260 00:12:58,920 --> 00:13:01,160 Speaker 1: in orbit is pretty trick. Okay, So I think the 261 00:13:01,200 --> 00:13:04,040 Speaker 1: most likely way to get a moon is for something 262 00:13:04,040 --> 00:13:06,680 Speaker 1: to smash into the planet and the debris to float 263 00:13:06,760 --> 00:13:10,480 Speaker 1: up and then coalesce into a moon. Alright, let's get 264 00:13:10,559 --> 00:13:14,120 Speaker 1: into this smashing idea, but first let's take a quick break. 265 00:13:27,080 --> 00:13:28,800 Speaker 1: All right. So you're saying that one way to get 266 00:13:28,800 --> 00:13:31,160 Speaker 1: a moon, and maybe our moon came this way, is 267 00:13:31,160 --> 00:13:34,920 Speaker 1: that something smashed into the Earth and kind of like 268 00:13:35,200 --> 00:13:38,600 Speaker 1: broke off a piece that then became the moon. That's right, Yeah, 269 00:13:38,679 --> 00:13:40,240 Speaker 1: And that's a that's the way we think some of 270 00:13:40,280 --> 00:13:43,600 Speaker 1: the moon's have occurred in the Solar System. But it's 271 00:13:43,960 --> 00:13:48,920 Speaker 1: tricky to explain our moon, right, Um, and because our 272 00:13:48,960 --> 00:13:52,360 Speaker 1: moon is so big, right, Our moon is huge compared 273 00:13:52,400 --> 00:13:54,960 Speaker 1: to the planet, and so in order to make that 274 00:13:55,160 --> 00:13:58,320 Speaker 1: size the Moon work, you need a huge impact, right, 275 00:13:58,320 --> 00:14:00,480 Speaker 1: You need a ridiculously big effact. You can't just be 276 00:14:00,559 --> 00:14:03,000 Speaker 1: hit by laroc that knocks off a bunch of stuff. 277 00:14:03,160 --> 00:14:07,640 Speaker 1: You need a giant impact, like a planet killing impact. Yeah. 278 00:14:07,679 --> 00:14:10,679 Speaker 1: And the current models say that the kind of thing 279 00:14:10,720 --> 00:14:12,680 Speaker 1: that hit the Earth a long long time ago to 280 00:14:12,720 --> 00:14:15,000 Speaker 1: make the Moon might have been something the size of 281 00:14:15,000 --> 00:14:16,800 Speaker 1: a planet. It might have been a proto planet, might 282 00:14:16,840 --> 00:14:19,240 Speaker 1: have been something the size of Mars. Right, So we're 283 00:14:19,280 --> 00:14:22,880 Speaker 1: talking about like two planets colliding, right, This must have 284 00:14:22,920 --> 00:14:26,240 Speaker 1: been amazing to watch, right, right or not if you're 285 00:14:26,280 --> 00:14:29,960 Speaker 1: living in these planets, that's right. Well, we don't think 286 00:14:30,000 --> 00:14:31,760 Speaker 1: there was anything alive on Earth when it happened. The 287 00:14:31,760 --> 00:14:35,320 Speaker 1: best estimates say that this happened about um zero point 288 00:14:35,400 --> 00:14:38,280 Speaker 1: one billion years or a hundred million years after the 289 00:14:38,280 --> 00:14:41,120 Speaker 1: Earth was formed, So the Earth was still pretty hot 290 00:14:41,560 --> 00:14:44,240 Speaker 1: and a nasty when this kind of stuff happened. We 291 00:14:44,280 --> 00:14:47,400 Speaker 1: don't think there was any atmosphere of life yet collided 292 00:14:47,640 --> 00:14:51,960 Speaker 1: with another planet about its size. That's incredible, right, two 293 00:14:52,040 --> 00:14:57,320 Speaker 1: giant balls of rock just yeah, exactly, and um and 294 00:14:57,400 --> 00:14:59,960 Speaker 1: that must have been pretty kindaclasmic, right, A lot of 295 00:15:00,000 --> 00:15:03,120 Speaker 1: stuff must have gotten thrown off into space, and some 296 00:15:03,200 --> 00:15:06,320 Speaker 1: of that stuff coalesced into rings. So the Earth probably 297 00:15:06,360 --> 00:15:09,400 Speaker 1: had rings for a while, no way like Saturn. Yeah, 298 00:15:09,480 --> 00:15:11,320 Speaker 1: I know that has been pretty awesome, right, I kind 299 00:15:11,320 --> 00:15:12,880 Speaker 1: of wish the Earth had rings, Like what would that 300 00:15:12,880 --> 00:15:15,000 Speaker 1: look like at night or during the day, you know, 301 00:15:15,120 --> 00:15:17,080 Speaker 1: to see rings up in the sky. That would be 302 00:15:17,080 --> 00:15:20,480 Speaker 1: pretty incredible. So then the two planets collected is the 303 00:15:20,520 --> 00:15:23,600 Speaker 1: idea to planets collided, they form a new Earth with 304 00:15:23,760 --> 00:15:27,680 Speaker 1: some stuff out there in rings that eventually became the Moon. 305 00:15:28,000 --> 00:15:30,080 Speaker 1: That's right. And this collision was huge, right, It was 306 00:15:30,160 --> 00:15:33,760 Speaker 1: like a hundred million times the energy of the asteroid 307 00:15:33,760 --> 00:15:36,240 Speaker 1: that hit the Earth and probably killed the dinosaurs. So 308 00:15:36,320 --> 00:15:40,800 Speaker 1: it's a ginormous explosion. It's nothing that anybody could ever survive. Yeah, 309 00:15:40,840 --> 00:15:43,000 Speaker 1: I've seen I've seen the videos of the stimulations. Like 310 00:15:43,040 --> 00:15:46,600 Speaker 1: it's basically the Earth just gets pulverized and then just 311 00:15:46,720 --> 00:15:49,680 Speaker 1: kind of coagulates into this new thing. But it's like 312 00:15:49,720 --> 00:15:52,640 Speaker 1: it's basically obliterated. Yeah, and here you'll see the strength 313 00:15:52,680 --> 00:15:55,560 Speaker 1: of my fruit based analogy, which is imagined you take 314 00:15:55,560 --> 00:15:58,040 Speaker 1: two watermelons and you throw them together. What happens, right, 315 00:15:58,120 --> 00:16:01,560 Speaker 1: that's pretty much what's happened. You know, it's complete destruction. 316 00:16:01,720 --> 00:16:08,280 Speaker 1: The watermelons do not survive that kind of impact. So 317 00:16:08,320 --> 00:16:11,960 Speaker 1: then how do rings become moons? And why? Like, why 318 00:16:12,000 --> 00:16:14,600 Speaker 1: does Saturn still have rings and nut moons? Yeah, that's 319 00:16:14,600 --> 00:16:17,360 Speaker 1: a really awesome question because gravity, right, you would think 320 00:16:17,440 --> 00:16:20,240 Speaker 1: if stuff is floating out there in space, then eventually 321 00:16:20,320 --> 00:16:22,880 Speaker 1: gravity would coalesce, it would pull it all together into 322 00:16:22,880 --> 00:16:25,800 Speaker 1: a moon. And that does happen if you're far enough 323 00:16:25,840 --> 00:16:29,000 Speaker 1: away from the planet. If you're too close to the planet, 324 00:16:29,360 --> 00:16:31,600 Speaker 1: then the strength of gravity tugging on you from one 325 00:16:31,640 --> 00:16:33,640 Speaker 1: side and the strength of gravity tugging you from the 326 00:16:33,640 --> 00:16:36,600 Speaker 1: other side are too different. Because remember the force of 327 00:16:36,600 --> 00:16:39,440 Speaker 1: gravity depends on your distance from an object, and so 328 00:16:39,480 --> 00:16:41,640 Speaker 1: one side of the Moon is closer to the Earth 329 00:16:41,680 --> 00:16:44,280 Speaker 1: than the other side of the Moon, So the Earth 330 00:16:44,400 --> 00:16:46,720 Speaker 1: pulls on one side of the Moon more than the 331 00:16:46,720 --> 00:16:49,560 Speaker 1: other side, So it's literally pulling the Moon apart. But 332 00:16:49,600 --> 00:16:51,680 Speaker 1: the Moon is far enough away from the Earth that 333 00:16:51,760 --> 00:16:54,320 Speaker 1: the Earth is not strong enough to shred the Moon. 334 00:16:54,960 --> 00:16:58,160 Speaker 1: But if the Moon was a lot closer right then 335 00:16:58,160 --> 00:17:00,960 Speaker 1: it then it would be pulled apart. By these gravitational 336 00:17:01,000 --> 00:17:04,600 Speaker 1: they're called tidal forces. By the tidal forces, so there's 337 00:17:04,600 --> 00:17:06,840 Speaker 1: a region around every planet where you just cannot be 338 00:17:06,920 --> 00:17:09,879 Speaker 1: a moon because if you are, you're gonna get shredded, right, 339 00:17:10,400 --> 00:17:12,560 Speaker 1: So you just kind of get ripped apart. Yeah, it's 340 00:17:12,600 --> 00:17:16,320 Speaker 1: like a blender. There is like a blender. Yeah, and 341 00:17:16,359 --> 00:17:19,040 Speaker 1: we've seen this happen if you remember the comment that 342 00:17:19,119 --> 00:17:22,480 Speaker 1: hit Jupiter um in the nineties. It passed really close 343 00:17:22,480 --> 00:17:24,879 Speaker 1: by Jupiter before it hit and Jupiter pulled it apart 344 00:17:24,920 --> 00:17:28,119 Speaker 1: into twenty six pieces because of his tidal forces. And 345 00:17:28,119 --> 00:17:30,480 Speaker 1: so the larger the planet, the stronger the force of gravity, 346 00:17:30,760 --> 00:17:33,160 Speaker 1: and the more likely this is to happen. Oh I see. 347 00:17:33,760 --> 00:17:36,440 Speaker 1: So if Saturn had bigger rings or rings that were 348 00:17:36,480 --> 00:17:40,199 Speaker 1: further apart, then the tidal forces would be less and 349 00:17:40,200 --> 00:17:42,919 Speaker 1: then the little bits of it would have time when 350 00:17:43,400 --> 00:17:47,800 Speaker 1: and kind of space to clump together. Yeah, but that's 351 00:17:47,800 --> 00:17:50,760 Speaker 1: a whole other fascinating mystery, like how long has Saturn 352 00:17:50,800 --> 00:17:53,360 Speaker 1: hand rings? How long will it continue to have rings? Right? 353 00:17:53,600 --> 00:17:56,560 Speaker 1: We think that those rings are pretty stable because they 354 00:17:56,560 --> 00:18:00,000 Speaker 1: have been there for like a hundred million years and um, 355 00:18:00,000 --> 00:18:02,639 Speaker 1: and because Saturn has really strong title forces. So anything 356 00:18:02,680 --> 00:18:05,160 Speaker 1: that coalesces, Saturn will tear up again, but we don't 357 00:18:05,160 --> 00:18:07,720 Speaker 1: really know for sure. And Saturn does have some moons, 358 00:18:07,720 --> 00:18:09,159 Speaker 1: and we don't know like are those moons in the 359 00:18:09,160 --> 00:18:11,680 Speaker 1: process of being trashed, Like if you fast forwarded a 360 00:18:11,760 --> 00:18:13,840 Speaker 1: billion years with Saturn look totally different or is it 361 00:18:13,880 --> 00:18:16,320 Speaker 1: looked this way for a long time. It's amazing to 362 00:18:16,400 --> 00:18:18,760 Speaker 1: me how dynamic the Solar system is. You know, like 363 00:18:18,880 --> 00:18:20,439 Speaker 1: if you look at a picture of the Solar System 364 00:18:20,480 --> 00:18:23,439 Speaker 1: from two billion years ago, you might not recognize it. 365 00:18:23,440 --> 00:18:25,439 Speaker 1: You could have a different number of planets, and all 366 00:18:25,480 --> 00:18:27,040 Speaker 1: the planets could have different number of moons, or the 367 00:18:27,040 --> 00:18:29,719 Speaker 1: planets could even be in a different order. It's crazy 368 00:18:29,760 --> 00:18:32,040 Speaker 1: stuff that's happened in our Solar system. Or even two 369 00:18:32,040 --> 00:18:34,919 Speaker 1: billion years from now, it might look totally different. Yeah, well, 370 00:18:34,920 --> 00:18:36,600 Speaker 1: in two billion years from now, I hope we've built 371 00:18:36,880 --> 00:18:40,879 Speaker 1: massive interstellar structures so we're recognizable from space. Um. But 372 00:18:41,040 --> 00:18:44,480 Speaker 1: even without that, Yeah, the planets could reorganize or realign, 373 00:18:44,640 --> 00:18:46,200 Speaker 1: or things could drift this way or the other way, 374 00:18:46,280 --> 00:18:48,520 Speaker 1: or something could come from another Solar system and knock 375 00:18:48,760 --> 00:18:51,760 Speaker 1: knock into something and change everything. Yeah, you know, people 376 00:18:51,840 --> 00:18:54,480 Speaker 1: might imagine the Solar system is really static because it's old, 377 00:18:55,040 --> 00:18:57,159 Speaker 1: but we've only seen the recent history of it. And 378 00:18:57,400 --> 00:18:59,280 Speaker 1: one of the best ways to figure out what is 379 00:18:59,320 --> 00:19:01,240 Speaker 1: the history, what is the whole story here, what is 380 00:19:01,280 --> 00:19:04,240 Speaker 1: the drama that's taking place out there in space, is 381 00:19:04,280 --> 00:19:06,399 Speaker 1: to ask these questions, you know, like how did the 382 00:19:06,400 --> 00:19:10,000 Speaker 1: moon form? Yeah, so that's one possibility, is that something 383 00:19:10,040 --> 00:19:12,680 Speaker 1: smashed into the Earth through all this stuff out there 384 00:19:12,840 --> 00:19:15,600 Speaker 1: that became a moon because it was far enough away 385 00:19:15,600 --> 00:19:19,440 Speaker 1: from the Earth. But there's some that's not quite right, right, 386 00:19:19,680 --> 00:19:22,280 Speaker 1: Like that doesn't quite fit what we see or know 387 00:19:22,400 --> 00:19:25,760 Speaker 1: about the moon. Yeah, it's interesting because we can't quite 388 00:19:25,920 --> 00:19:29,480 Speaker 1: make that story explain everything we see. And so one 389 00:19:29,520 --> 00:19:31,160 Speaker 1: of the things we see, for example, is that we've 390 00:19:31,200 --> 00:19:33,520 Speaker 1: been to the moon and we've looked at rocks from 391 00:19:33,520 --> 00:19:36,760 Speaker 1: the moon. You've been to the moon. I mean we 392 00:19:36,960 --> 00:19:40,840 Speaker 1: collectively as humanity. I like to take credit for humanities 393 00:19:41,640 --> 00:19:46,000 Speaker 1: of humanities collective. The Royal week there. Okay, we have 394 00:19:46,119 --> 00:19:48,640 Speaker 1: won a bunch of NBA championships, by which I mean 395 00:19:48,800 --> 00:19:53,720 Speaker 1: me and Lebron James. Yeah, we are an acclaimed internet cartoonist. 396 00:19:53,960 --> 00:19:57,280 Speaker 1: But which I mean me and you. We are Tom Cruise. 397 00:19:57,960 --> 00:20:02,399 Speaker 1: You know, we are sexy in our fifties exactly. Humanity, 398 00:20:02,520 --> 00:20:04,520 Speaker 1: not me personally, has been to the Moon and brought 399 00:20:04,520 --> 00:20:06,760 Speaker 1: back rocks, and we've looked at those rocks, and those 400 00:20:06,840 --> 00:20:09,639 Speaker 1: rocks look really similar to rocks on Earth. And you 401 00:20:09,640 --> 00:20:12,000 Speaker 1: should know that rocks on every planet look different because 402 00:20:12,000 --> 00:20:14,879 Speaker 1: they're formed under different circumstances from different bits and different 403 00:20:14,880 --> 00:20:17,960 Speaker 1: temperatures and different ages. So you can sort of tell 404 00:20:18,359 --> 00:20:21,040 Speaker 1: where a rock came from, Like really that different because 405 00:20:21,040 --> 00:20:23,920 Speaker 1: they it all came from the debris of this Solar system, right, 406 00:20:24,080 --> 00:20:26,000 Speaker 1: wouldn't it all be sort of the same. But like 407 00:20:26,160 --> 00:20:28,560 Speaker 1: Mars is different from Earth, and we can we we 408 00:20:28,680 --> 00:20:31,640 Speaker 1: found rocks on Earth that we can tell came from 409 00:20:31,640 --> 00:20:34,520 Speaker 1: Mars because we know they're different. They have different structures, 410 00:20:34,560 --> 00:20:37,199 Speaker 1: formed in different temperatures at different times and this you know, 411 00:20:37,240 --> 00:20:40,919 Speaker 1: different totally different kind of tectonic activity on different planets, 412 00:20:40,960 --> 00:20:43,280 Speaker 1: like Mars doesn't have any at all, you know, and 413 00:20:44,119 --> 00:20:50,320 Speaker 1: letters of the bottoms that made in Mars Mars first, Yeah, exactly, 414 00:20:50,760 --> 00:20:54,159 Speaker 1: make Mars great again. They don't like, they don't want 415 00:20:54,160 --> 00:20:56,880 Speaker 1: to import our rocks anymore. The high tariffs on Earth 416 00:20:57,000 --> 00:20:59,640 Speaker 1: rocks anyway, So they can look at these rocks from 417 00:20:59,640 --> 00:21:01,720 Speaker 1: the Moon and they say, they looked just like rocks 418 00:21:01,720 --> 00:21:05,359 Speaker 1: from Earth. Right. So that's really interesting because suggests that 419 00:21:05,400 --> 00:21:07,399 Speaker 1: the stuff that the Moon is made out of is 420 00:21:07,440 --> 00:21:09,280 Speaker 1: really similar to the stuff that the Earth is made 421 00:21:09,280 --> 00:21:12,040 Speaker 1: out of. But if a really really big planet came 422 00:21:12,080 --> 00:21:13,920 Speaker 1: and smashed into the Earth, that's not what you would 423 00:21:13,960 --> 00:21:17,040 Speaker 1: really expect. You would expect that planet to have mostly 424 00:21:17,040 --> 00:21:20,000 Speaker 1: survived or that or to bounce off, or for this 425 00:21:20,119 --> 00:21:22,280 Speaker 1: stuff in the Moon to be made from that planet 426 00:21:22,280 --> 00:21:24,600 Speaker 1: that came. Right, You started out with two objects, you 427 00:21:24,640 --> 00:21:27,320 Speaker 1: have a collision, you end up with two objects. You 428 00:21:27,320 --> 00:21:29,720 Speaker 1: expect sort of a you know, a connection between the 429 00:21:29,760 --> 00:21:32,600 Speaker 1: incoming and the outgoing too, but instead both objects that 430 00:21:32,640 --> 00:21:35,639 Speaker 1: survives seem to be like the Earth stuff, which is 431 00:21:35,680 --> 00:21:39,360 Speaker 1: a bit weird. But we couldn't, um, couldn't this new 432 00:21:39,400 --> 00:21:42,320 Speaker 1: planet have also mixed in with our old Earth. And 433 00:21:42,359 --> 00:21:44,160 Speaker 1: so that's why it's the same, you know what I mean? 434 00:21:44,200 --> 00:21:46,199 Speaker 1: Like maybe the Moon and Earth is a mix of 435 00:21:46,240 --> 00:21:49,800 Speaker 1: these two pre crash planets. They have these simulations that 436 00:21:49,840 --> 00:21:53,399 Speaker 1: are totally crazy where essentially the other planet gets like 437 00:21:53,600 --> 00:21:57,880 Speaker 1: subsumed into the Earth like including it's it's like core, right, 438 00:21:57,880 --> 00:22:02,399 Speaker 1: So there's some other planets internal bits, right, the iron 439 00:22:02,440 --> 00:22:03,960 Speaker 1: and the nickel that makes up the inside of a 440 00:22:04,000 --> 00:22:06,840 Speaker 1: planet is inside the Earth. Now, like if you cut 441 00:22:06,880 --> 00:22:09,560 Speaker 1: the Earth open, you would find evidence for like, you know, 442 00:22:09,800 --> 00:22:12,840 Speaker 1: a second planet in there. And then what made the 443 00:22:12,880 --> 00:22:15,760 Speaker 1: Moon was like the Earth's crust just got ejected. It's 444 00:22:15,760 --> 00:22:18,720 Speaker 1: like ice cream, like a swirly ice cream doesn't completely 445 00:22:18,840 --> 00:22:22,920 Speaker 1: just mixed together, and that you would expect chunks. Yeah, 446 00:22:23,000 --> 00:22:24,919 Speaker 1: I'm glad you're with me on the food out analogies. Now, 447 00:22:25,080 --> 00:22:27,719 Speaker 1: trying to move us here towards dessert. We had our 448 00:22:27,800 --> 00:22:32,399 Speaker 1: fruit as the meal is wrapping up. In some places 449 00:22:32,400 --> 00:22:34,080 Speaker 1: fruit is considered dessert. I think we should do something 450 00:22:34,080 --> 00:22:36,760 Speaker 1: a little bit more meaty. Um. Yeah. So that's one 451 00:22:36,840 --> 00:22:38,840 Speaker 1: mystery is like why does the stuff on the Moon 452 00:22:38,880 --> 00:22:40,640 Speaker 1: look just like the stuff in the Earth. And they 453 00:22:40,640 --> 00:22:43,160 Speaker 1: can kind of make it work, right, Like they can 454 00:22:43,200 --> 00:22:45,040 Speaker 1: make it work that most of the stuff from the 455 00:22:45,040 --> 00:22:47,840 Speaker 1: Earth's crust turned into the Moon and the other planet 456 00:22:47,880 --> 00:22:51,159 Speaker 1: just sort of got swallowed by the Earth. But it's tricky. 457 00:22:51,359 --> 00:22:54,360 Speaker 1: It's not an easy thing to make work. And if 458 00:22:54,400 --> 00:22:57,000 Speaker 1: that happened, then you'd expect crazy stuff to have happened 459 00:22:57,000 --> 00:23:00,200 Speaker 1: on Earth, like you know, huge oceans of molten talk 460 00:23:00,200 --> 00:23:03,200 Speaker 1: of magma like magma oceans which is just a phrase 461 00:23:03,280 --> 00:23:06,919 Speaker 1: I love saying and hearing, magma oceans um. But we 462 00:23:06,960 --> 00:23:08,680 Speaker 1: don't see any evidence of that on Earth. Like people 463 00:23:08,680 --> 00:23:10,560 Speaker 1: who look at the history of rocks on Earth don't 464 00:23:10,600 --> 00:23:13,480 Speaker 1: see evidence of these of these magma ocetions that you 465 00:23:13,520 --> 00:23:15,879 Speaker 1: would expected from a huge such a huge collision. It 466 00:23:15,920 --> 00:23:18,280 Speaker 1: doesn't look like we were hit by a big rock. Yeah, 467 00:23:18,400 --> 00:23:20,159 Speaker 1: we don't see evidence for that on Earth. And you know, 468 00:23:20,200 --> 00:23:22,000 Speaker 1: when you put together this kind of story, you want 469 00:23:22,000 --> 00:23:24,119 Speaker 1: to check it multiple ways and does this make sense? 470 00:23:24,119 --> 00:23:26,679 Speaker 1: And let's see it in this other way? And we 471 00:23:26,720 --> 00:23:29,240 Speaker 1: can't find any confirmation for that currently, and the simulations 472 00:23:29,240 --> 00:23:32,360 Speaker 1: are are pretty hard to get right. Before we keep going, 473 00:23:32,480 --> 00:23:47,720 Speaker 1: let's take a short break. Man, that's wild. So we 474 00:23:47,800 --> 00:23:50,840 Speaker 1: really don't know where the moon came from. Kind of Yeah. 475 00:23:50,960 --> 00:23:53,320 Speaker 1: There are some other ideas, you know, crazy ideas about 476 00:23:53,320 --> 00:23:56,800 Speaker 1: how two other planets may have collided and basically totally 477 00:23:56,840 --> 00:24:00,800 Speaker 1: annihilated each other into some other sort of cosmic doughnut, 478 00:24:00,880 --> 00:24:03,200 Speaker 1: which then spun around and formed the Earth in the moon. 479 00:24:04,720 --> 00:24:08,280 Speaker 1: I said, that's right, we're doing double dessert here. One 480 00:24:08,320 --> 00:24:11,280 Speaker 1: of the crazy ideas is that the Earth essentially was 481 00:24:11,320 --> 00:24:15,120 Speaker 1: obliterated in this collision, and everything just became a big cloud, 482 00:24:15,560 --> 00:24:18,600 Speaker 1: really fast spinning cloud, which ended up shaping shaped into 483 00:24:18,600 --> 00:24:21,280 Speaker 1: this crazy donut shape. It's spun out a blob which 484 00:24:21,320 --> 00:24:24,160 Speaker 1: became the Moon. Um. That theory has some trouble because 485 00:24:24,200 --> 00:24:27,040 Speaker 1: it turns out the Moon doesn't really have like a 486 00:24:27,080 --> 00:24:30,080 Speaker 1: solid iron core like you would expect, like, you know, 487 00:24:30,119 --> 00:24:33,480 Speaker 1: the Earth has a as a release heavy metallic core 488 00:24:33,560 --> 00:24:36,040 Speaker 1: like most rocky planets, but the Moon is pretty light. 489 00:24:36,200 --> 00:24:38,879 Speaker 1: It's mostly fluffy, right. It has a little bit of 490 00:24:38,880 --> 00:24:42,240 Speaker 1: a core, but not very much. And so that's better 491 00:24:42,280 --> 00:24:44,520 Speaker 1: explained by saying that the Moon mostly came from Earth 492 00:24:44,600 --> 00:24:48,560 Speaker 1: crust stuff rather than from like an entire blob of 493 00:24:48,880 --> 00:24:51,120 Speaker 1: planetary stuff, where you would get like the same same 494 00:24:51,160 --> 00:24:53,439 Speaker 1: amount of serving of the core as you would have 495 00:24:53,440 --> 00:24:57,159 Speaker 1: the crust. Um. So all these theories have some problems. Well, 496 00:24:57,200 --> 00:25:00,560 Speaker 1: what are some other crazy ideas? Yeah, Well, a theory 497 00:25:00,560 --> 00:25:02,040 Speaker 1: that exists for a long time was just that the 498 00:25:02,040 --> 00:25:04,000 Speaker 1: Moon was captured, you know, like maybe the Moon came 499 00:25:04,040 --> 00:25:06,240 Speaker 1: from somewhere else or used to be its own planet, 500 00:25:06,600 --> 00:25:09,359 Speaker 1: or was wandering around just sort of got sucked into 501 00:25:09,440 --> 00:25:12,680 Speaker 1: the Earth's orbit. And this theory has a couple of problems. 502 00:25:13,080 --> 00:25:15,240 Speaker 1: One is that that's really hard to do. Like you 503 00:25:15,280 --> 00:25:18,200 Speaker 1: do simulations and you have another planet approach Earth, as 504 00:25:18,200 --> 00:25:20,920 Speaker 1: we were saying before, usually they you know, spin off 505 00:25:20,960 --> 00:25:23,000 Speaker 1: each other and then one gets flung out into space 506 00:25:23,520 --> 00:25:26,119 Speaker 1: or they end up colliding right to get it to 507 00:25:26,200 --> 00:25:28,919 Speaker 1: come into stable or with that last for billions of years. 508 00:25:29,280 --> 00:25:31,600 Speaker 1: That's really really hard to do. That's a one in 509 00:25:31,680 --> 00:25:34,280 Speaker 1: a billion chance. So that might be possible, but it's 510 00:25:34,320 --> 00:25:36,920 Speaker 1: hard to do. And the other problem is it doesn't 511 00:25:36,920 --> 00:25:39,679 Speaker 1: explain why the Earth and the Moon looks so similar, right, 512 00:25:39,760 --> 00:25:41,919 Speaker 1: they have like these really similar rocks on them. The 513 00:25:41,960 --> 00:25:44,360 Speaker 1: Moon came from somewhere else. I was captured. It shouldn't 514 00:25:44,400 --> 00:25:48,000 Speaker 1: have the same basically rock d n a that we have. Okay, 515 00:25:48,040 --> 00:25:50,359 Speaker 1: but I heard another idea is that maybe the Moon 516 00:25:51,040 --> 00:25:53,159 Speaker 1: fell off to Earth like it was part of us, 517 00:25:53,200 --> 00:25:56,880 Speaker 1: but then it was like I'll see you later. Yeah. 518 00:25:56,960 --> 00:25:59,280 Speaker 1: I think this is a really popular, super ancient idea, 519 00:25:59,359 --> 00:26:01,920 Speaker 1: Like if you look in the historical documents, people speculate 520 00:26:01,960 --> 00:26:04,000 Speaker 1: about this, you know, a thousand years ago before really 521 00:26:04,040 --> 00:26:07,520 Speaker 1: anybody knew physics, and somebody even wrote that the Pacific 522 00:26:07,560 --> 00:26:10,160 Speaker 1: Ocean was like the scar of the moon leaving the Earth. 523 00:26:10,640 --> 00:26:12,679 Speaker 1: You know that a huge chunk of land to just 524 00:26:12,720 --> 00:26:16,800 Speaker 1: like floated off into into space because the Earth of spinning, um, 525 00:26:16,840 --> 00:26:20,000 Speaker 1: and it got turned into the moon. The moon is Atlantis? 526 00:26:21,119 --> 00:26:23,520 Speaker 1: Is Atlantis? Oh my gosh. I love when you can 527 00:26:23,640 --> 00:26:26,880 Speaker 1: connect to mysteries at once. Um. But there's basically no 528 00:26:27,160 --> 00:26:29,159 Speaker 1: data to support that at all. I mean, it's just 529 00:26:29,720 --> 00:26:31,720 Speaker 1: I mean, we know the Pacific Ocean is not formed 530 00:26:31,720 --> 00:26:34,879 Speaker 1: by somebody taking a scoop out of the Earth, um. 531 00:26:35,000 --> 00:26:37,600 Speaker 1: And so it was just like random speculation. But it 532 00:26:37,640 --> 00:26:39,639 Speaker 1: was a popular idea for you know, a long time 533 00:26:40,000 --> 00:26:47,280 Speaker 1: among the medieval and ancient folks. So what's kind of 534 00:26:47,280 --> 00:26:49,920 Speaker 1: the best current thinking about where the moon came from? 535 00:26:49,960 --> 00:26:52,159 Speaker 1: I think, um, if you ask most scientists, and I 536 00:26:52,200 --> 00:26:54,800 Speaker 1: haven't asked most scientists, but I've asked a few. He 537 00:26:54,920 --> 00:27:00,399 Speaker 1: was asked science scientists. I've asked a scientist who's an 538 00:27:00,440 --> 00:27:04,600 Speaker 1: expert in planetary science, and I've asked myself. I'm a scientist. Um, 539 00:27:04,640 --> 00:27:10,600 Speaker 1: So yes, I've asked scientists about this. That's the deep 540 00:27:10,640 --> 00:27:13,359 Speaker 1: research we do for this show, folks. UM. And the 541 00:27:13,760 --> 00:27:16,960 Speaker 1: prevailing theory is the giant impact, right, it has some problems. 542 00:27:16,960 --> 00:27:18,680 Speaker 1: There are things we don't understand about it. But that's 543 00:27:18,680 --> 00:27:21,480 Speaker 1: sort of the progress of science. Right, we say, here's 544 00:27:21,480 --> 00:27:23,760 Speaker 1: a bunch of ideas. This one doesn't quite work, but 545 00:27:23,840 --> 00:27:26,560 Speaker 1: it mostly works. The elements of it that explain things 546 00:27:26,640 --> 00:27:29,439 Speaker 1: we see. There's just stuff to figure out. And so 547 00:27:29,560 --> 00:27:32,159 Speaker 1: that's that's the prevailing ideas, the giant impact. It's the 548 00:27:32,200 --> 00:27:34,680 Speaker 1: best idea we have. That's right, that it's that or 549 00:27:34,720 --> 00:27:40,200 Speaker 1: the Big bang? Man. Yeah, and I like this process 550 00:27:40,200 --> 00:27:42,560 Speaker 1: of science. You know, we have one idea, we refine it, 551 00:27:42,600 --> 00:27:44,440 Speaker 1: We refined it, and then we see doesn't fit the 552 00:27:44,520 --> 00:27:46,560 Speaker 1: data better than it used to. Is it sort of 553 00:27:46,560 --> 00:27:49,280 Speaker 1: coming together? It's like solving a murder mystery, right, You 554 00:27:49,359 --> 00:27:51,440 Speaker 1: look for clues, you come up with the theory. Something 555 00:27:51,480 --> 00:27:54,919 Speaker 1: doesn't quite work, makes you change your theory. Eventually you 556 00:27:54,960 --> 00:27:57,679 Speaker 1: have a story that explains everything you see and that 557 00:27:57,760 --> 00:27:59,760 Speaker 1: fits in with what other people say and that makes sense. 558 00:28:00,080 --> 00:28:02,159 Speaker 1: You get more data, and that's what we're looking for, 559 00:28:02,240 --> 00:28:04,840 Speaker 1: and we have a story. They definitely wasn't murder. A 560 00:28:04,920 --> 00:28:07,960 Speaker 1: huge planet died um in the making of our moon, 561 00:28:08,040 --> 00:28:10,679 Speaker 1: but we don't quite know how it happened. And it 562 00:28:10,800 --> 00:28:12,600 Speaker 1: might be that, you know, it's just sort of weird, 563 00:28:12,640 --> 00:28:15,680 Speaker 1: and it's it seems unlikely that this sort of configuration 564 00:28:15,720 --> 00:28:18,360 Speaker 1: would happen, and maybe it was unlikely, or maybe there's 565 00:28:18,400 --> 00:28:20,679 Speaker 1: some part of the story we haven't understood, like there 566 00:28:20,760 --> 00:28:23,080 Speaker 1: was two cataclysms, or you know, two planets hit the 567 00:28:23,080 --> 00:28:25,880 Speaker 1: Earth or something like that makes you wonder, what if 568 00:28:25,960 --> 00:28:28,639 Speaker 1: that other planet or asteroid hadn't hit us, you know, 569 00:28:28,680 --> 00:28:32,320 Speaker 1: if it just missed by a few degrees, we wouldn't 570 00:28:32,320 --> 00:28:34,720 Speaker 1: have a moon and we would have a super different 571 00:28:34,840 --> 00:28:37,840 Speaker 1: planet Earth, right, Yeah, and things could be very different. 572 00:28:37,880 --> 00:28:39,520 Speaker 1: You know. The reason we have tides is because we 573 00:28:39,560 --> 00:28:42,720 Speaker 1: have the Moon, and the moon stabilizes the Earth's orbit, 574 00:28:43,080 --> 00:28:45,800 Speaker 1: and we think that the collision that caused the moon 575 00:28:45,880 --> 00:28:48,160 Speaker 1: might have also caused the tilt of the Earth, which 576 00:28:48,160 --> 00:28:50,320 Speaker 1: means if we didn't have a moon, we might not 577 00:28:50,400 --> 00:28:53,120 Speaker 1: have tides, we might not have seasons, and that's a 578 00:28:53,120 --> 00:28:55,360 Speaker 1: pretty big change in what life on Earth is like, right, 579 00:28:55,560 --> 00:28:57,480 Speaker 1: And a lot of people think the tides were critical 580 00:28:57,520 --> 00:29:00,520 Speaker 1: to life because as the sea comes in and out, 581 00:29:00,560 --> 00:29:02,600 Speaker 1: it's sort of like a lot of slashing around, which 582 00:29:02,640 --> 00:29:04,960 Speaker 1: is what you need to mix up those basic organic 583 00:29:05,000 --> 00:29:08,120 Speaker 1: chemicals into something that might turn into life and so yeah, 584 00:29:08,160 --> 00:29:09,880 Speaker 1: we might have the Moon to thank for the fact 585 00:29:09,920 --> 00:29:12,000 Speaker 1: that we're even here to ask about it. It just 586 00:29:12,080 --> 00:29:15,080 Speaker 1: that a planet had to die. That's right to get 587 00:29:15,120 --> 00:29:17,560 Speaker 1: to But in the interest of all things good, so 588 00:29:17,600 --> 00:29:20,400 Speaker 1: that we could be here eating watermelons, somebody had to 589 00:29:20,440 --> 00:29:25,280 Speaker 1: sacrifice a big planet. So yeah, that's another one of 590 00:29:25,280 --> 00:29:28,000 Speaker 1: these crazy mysteries that are just staring at us in 591 00:29:28,040 --> 00:29:30,720 Speaker 1: the face every single night. And when you think about 592 00:29:30,720 --> 00:29:33,960 Speaker 1: the Solar System next time, remember it's not static, it's dynamic. 593 00:29:33,960 --> 00:29:35,920 Speaker 1: There is stuff happening, and there is a story. It's 594 00:29:35,960 --> 00:29:40,480 Speaker 1: playing out really slowly right geological cosmic time scales. But 595 00:29:40,520 --> 00:29:42,680 Speaker 1: if you took a time lapse video of the Solar system, 596 00:29:42,800 --> 00:29:45,960 Speaker 1: it would seem like a crazy dance party. Yeah, so 597 00:29:46,080 --> 00:29:48,200 Speaker 1: next time you are mooning the moon, pull up your 598 00:29:48,200 --> 00:29:50,400 Speaker 1: pants and show some respect, because that we owe the 599 00:29:50,440 --> 00:29:52,800 Speaker 1: Moon a big thank you. All right, thanks for listening 600 00:29:52,800 --> 00:30:02,880 Speaker 1: to everyone, See you next time. If you still have 601 00:30:02,920 --> 00:30:06,320 Speaker 1: a question after listening to all these explanations, please drop 602 00:30:06,360 --> 00:30:08,440 Speaker 1: us a line. We'd love to hear from you. You 603 00:30:08,440 --> 00:30:11,880 Speaker 1: can find us at Facebook, Twitter, and Instagram at Daniel 604 00:30:11,920 --> 00:30:15,440 Speaker 1: and Jorge that's one word, or email us at Feedback 605 00:30:15,520 --> 00:30:26,360 Speaker 1: at Daniel and Jorge dot com