1 00:00:04,280 --> 00:00:06,200 Speaker 1: Hey, and welcome to the short Stuff. I'm Josh, and 2 00:00:06,240 --> 00:00:09,120 Speaker 1: there's Chuck and Jerry's here too. We're just zooming through 3 00:00:09,160 --> 00:00:14,960 Speaker 1: the universe trio of cool cats who apparently can survive 4 00:00:15,040 --> 00:00:16,200 Speaker 1: in the vacuum of space. 5 00:00:16,880 --> 00:00:21,520 Speaker 2: That's right, we're talking about Saturn's rings and big thanks 6 00:00:21,560 --> 00:00:25,480 Speaker 2: to doctor Ian O'Neil, who wrote this for houstuffworks dot com. 7 00:00:26,160 --> 00:00:30,840 Speaker 2: And we're talking about Saturn's rings because semi recently, in 8 00:00:30,880 --> 00:00:33,000 Speaker 2: the grand scheme of things, what like six years ago 9 00:00:33,120 --> 00:00:35,720 Speaker 2: or so, and in the time since, we have learned 10 00:00:35,760 --> 00:00:39,560 Speaker 2: a couple of kind of cool things about Saturn. One 11 00:00:40,680 --> 00:00:42,960 Speaker 2: not cool as in like, hey, it's good that this 12 00:00:43,000 --> 00:00:46,040 Speaker 2: is happening, but cool as in we never knew this stuff. Yeah. One, 13 00:00:46,120 --> 00:00:48,680 Speaker 2: in the next one hundred million years, Saturn's rings will 14 00:00:48,680 --> 00:00:51,760 Speaker 2: no longer be around. They're going to disappear, completely denuded. 15 00:00:52,680 --> 00:00:56,160 Speaker 2: And Two, because of what we're going to tell you 16 00:00:56,200 --> 00:00:59,200 Speaker 2: about in a second, we learned a lot more about 17 00:00:59,240 --> 00:01:01,480 Speaker 2: those rings and the fact that they are a lot 18 00:01:01,520 --> 00:01:02,400 Speaker 2: younger than we thought. 19 00:01:03,000 --> 00:01:05,920 Speaker 1: Chuck, that was such an amazing intro. I'm that was 20 00:01:06,000 --> 00:01:07,000 Speaker 1: great stuff. Man. 21 00:01:07,720 --> 00:01:10,479 Speaker 2: Hey, Jerry just said we were on fire before we recorded. 22 00:01:10,360 --> 00:01:13,080 Speaker 1: So we can thank our friends at NASA for launching 23 00:01:13,120 --> 00:01:15,640 Speaker 1: the Cassini mission and more robe. 24 00:01:15,880 --> 00:01:18,840 Speaker 2: Yeah, NASA in the it was a three three uh 25 00:01:20,200 --> 00:01:23,319 Speaker 2: what do you call it? A monagatwa Sure, NASA and 26 00:01:23,360 --> 00:01:26,440 Speaker 2: the we got to shout out the euro Space Agency ESA, 27 00:01:26,600 --> 00:01:30,000 Speaker 2: sure and the utality in a space agency which is 28 00:01:30,120 --> 00:01:32,800 Speaker 2: not of the ISA. But it's the aside, don't. 29 00:01:32,760 --> 00:01:38,039 Speaker 1: Ask very nice. So this this Cassini mission, great stuff, Chuck, chuck. 30 00:01:39,080 --> 00:01:42,160 Speaker 1: It was flying around Saturn for I saw thirteen years. 31 00:01:42,160 --> 00:01:45,120 Speaker 1: I think doctor o'neilsa's thirteen years. I saw up to twenty. 32 00:01:45,600 --> 00:01:48,280 Speaker 2: Yeah, they launched in ninety seven, but it entered the 33 00:01:48,560 --> 00:01:50,120 Speaker 2: orbit of Saturn in two thousand and four. 34 00:01:50,280 --> 00:01:53,480 Speaker 1: Ah, there's the discrepancy. Yeah, but we learned a lot 35 00:01:53,560 --> 00:01:55,520 Speaker 1: about Saturn, which is, by the way, one of the 36 00:01:55,560 --> 00:01:59,200 Speaker 1: gas giants of our of our Solar system. 37 00:01:59,320 --> 00:02:01,600 Speaker 2: Any who else is Jerry. 38 00:02:03,040 --> 00:02:04,640 Speaker 1: She is kind of gassy, isn't she. 39 00:02:04,880 --> 00:02:05,960 Speaker 2: He's a gas giant. 40 00:02:06,280 --> 00:02:09,800 Speaker 1: So we learned a lot about Saturn. And one of 41 00:02:09,800 --> 00:02:12,680 Speaker 1: the things we learned, number one, that there's tons of 42 00:02:12,720 --> 00:02:15,560 Speaker 1: moons around Saturn. Number two that there's some of these 43 00:02:15,880 --> 00:02:19,280 Speaker 1: moons might be habitable. And so as a result, when 44 00:02:19,320 --> 00:02:22,280 Speaker 1: they launched the Cassini mission. They were like, okay, we've 45 00:02:22,360 --> 00:02:24,360 Speaker 1: we've got to figure out a way to dispose of 46 00:02:24,400 --> 00:02:28,120 Speaker 1: the Cassini probe without just crash landing it, because you 47 00:02:28,160 --> 00:02:30,960 Speaker 1: know it could be lousy with earth germs on it. Still, 48 00:02:31,440 --> 00:02:34,760 Speaker 1: I don't want to infect one of these moons. So 49 00:02:34,800 --> 00:02:37,280 Speaker 1: they burned it up in the atmosphere instead. And I 50 00:02:37,320 --> 00:02:39,640 Speaker 1: realized that this is like the NASA equivalent of wearing 51 00:02:39,720 --> 00:02:46,880 Speaker 1: a mask. Explain, well, they didn't want to contaminate the moon, 52 00:02:47,040 --> 00:02:49,920 Speaker 1: so they burned the thing up in the atmosphere. 53 00:02:50,080 --> 00:02:50,519 Speaker 2: I got you. 54 00:02:51,400 --> 00:02:53,000 Speaker 1: It was way better on paper. 55 00:02:53,160 --> 00:02:55,919 Speaker 2: Yeah, but you actually wrote that out. 56 00:02:56,440 --> 00:03:00,560 Speaker 1: Yeah. Actually, some of them are so good I don't 57 00:03:00,560 --> 00:03:01,320 Speaker 1: want to forget them. 58 00:03:02,360 --> 00:03:02,960 Speaker 2: Yeah, I gotcha. 59 00:03:03,040 --> 00:03:04,280 Speaker 1: And that's a good example of it. 60 00:03:04,360 --> 00:03:07,400 Speaker 2: Uh huh. So that's what happened, right, This thing was 61 00:03:07,400 --> 00:03:11,520 Speaker 2: low on fuel and so they did that. They burned 62 00:03:11,520 --> 00:03:12,799 Speaker 2: it up in that upper atmosphere. 63 00:03:12,840 --> 00:03:15,360 Speaker 1: They did, but they said, you know what we're going 64 00:03:15,440 --> 00:03:18,200 Speaker 1: to do, We're going to do something crazy. Cassini's at 65 00:03:18,200 --> 00:03:20,920 Speaker 1: the end of its mission. I'm gonna say her. Cassini's 66 00:03:20,919 --> 00:03:24,320 Speaker 1: at the end of her mission. She's been a stout 67 00:03:24,360 --> 00:03:27,480 Speaker 1: and true pioneer for US teaching us all sorts of 68 00:03:27,480 --> 00:03:29,800 Speaker 1: great stuff about Saturn. But one thing we don't know 69 00:03:29,880 --> 00:03:35,320 Speaker 1: about is what is between Saturn's rings and the planet itself. 70 00:03:35,560 --> 00:03:39,040 Speaker 1: That's great gap between the planet and its innermost ring. 71 00:03:39,640 --> 00:03:40,840 Speaker 1: What's going on there? 72 00:03:41,080 --> 00:03:43,080 Speaker 2: Yeah, and like, not only what's going on there, but 73 00:03:43,160 --> 00:03:46,000 Speaker 2: what can we learn a about the rings and about 74 00:03:46,040 --> 00:03:48,680 Speaker 2: Saturn as a whole if we learn about what's going 75 00:03:48,720 --> 00:03:52,440 Speaker 2: on in between those rings. They thought, well, you know, 76 00:03:52,640 --> 00:03:55,800 Speaker 2: I'm sure we're going to find some gases. But they 77 00:03:55,800 --> 00:03:58,920 Speaker 2: basically thought, like, you know, it's empty in between there, 78 00:03:58,920 --> 00:04:03,200 Speaker 2: as Dave Matthews would, there's space between, and that's what 79 00:04:03,240 --> 00:04:06,119 Speaker 2: they thought. But what they found was not that at all. 80 00:04:06,560 --> 00:04:13,280 Speaker 2: What they found was a virtual rainstorm of particles and 81 00:04:13,480 --> 00:04:17,960 Speaker 2: elements and molecules raining down between the gaps. And what 82 00:04:18,000 --> 00:04:21,159 Speaker 2: they found out was hold on a second, these That is, 83 00:04:21,200 --> 00:04:24,520 Speaker 2: the rings sort of falling apart, right. 84 00:04:24,600 --> 00:04:28,480 Speaker 1: Yeah, they're dissolving onto it's just falling into the atmosphere 85 00:04:28,800 --> 00:04:32,159 Speaker 1: of Saturn, which is pretty cool. But what that implies 86 00:04:32,279 --> 00:04:35,200 Speaker 1: is that since there's a finite amount of these rings, 87 00:04:35,800 --> 00:04:39,159 Speaker 1: eventually they're going to dissolve. There won't be any rings 88 00:04:39,200 --> 00:04:41,480 Speaker 1: any longer. And that was a big thing that they 89 00:04:42,040 --> 00:04:44,480 Speaker 1: did not know before. They didn't know the age of 90 00:04:44,520 --> 00:04:47,400 Speaker 1: the rings. They didn't know that the rings were slowly dissolving. 91 00:04:47,760 --> 00:04:51,520 Speaker 1: And they learned it by sending Cassini on a crazy 92 00:04:52,320 --> 00:04:58,720 Speaker 1: screw e mission flying orbits inside the gap between the 93 00:04:58,760 --> 00:05:02,000 Speaker 1: planet and its inner string, which is really really cool. 94 00:05:02,200 --> 00:05:03,680 Speaker 1: And I say, we take a break, we'll come back 95 00:05:03,720 --> 00:05:05,760 Speaker 1: and talk about what Cassini taught us. 96 00:05:06,480 --> 00:05:38,440 Speaker 2: Let's do it. So first off, we've been saying just Cassini, 97 00:05:38,480 --> 00:05:40,240 Speaker 2: it was technically the Cassini Huygens. 98 00:05:40,960 --> 00:05:42,760 Speaker 1: Oh yeah, I didn't see that anyway. 99 00:05:42,480 --> 00:05:45,960 Speaker 2: But Huygens is kind of clunky, so everyone in Cassini 100 00:05:46,040 --> 00:05:49,880 Speaker 2: just I guess that was the Italian input. Sure, so 101 00:05:50,080 --> 00:05:52,600 Speaker 2: Cassini sounds better. But one of the things they learned, 102 00:05:52,600 --> 00:05:54,960 Speaker 2: like we said, is that these rings have about one 103 00:05:55,000 --> 00:05:57,280 Speaker 2: hundred million years to live, which sounds like a long 104 00:05:57,320 --> 00:06:00,320 Speaker 2: time and it is, but considering Saturn is a about 105 00:06:00,320 --> 00:06:03,520 Speaker 2: four billion years old, it's much shorter than they thought. 106 00:06:04,040 --> 00:06:06,760 Speaker 1: Did you say that it's raining ten tons of material 107 00:06:06,880 --> 00:06:07,560 Speaker 1: per second? 108 00:06:08,000 --> 00:06:10,080 Speaker 2: No? No, no, I didn't. That's a great stat. 109 00:06:10,000 --> 00:06:12,240 Speaker 1: It is, and it's hilarious that they went with ten 110 00:06:12,279 --> 00:06:15,520 Speaker 1: tons because it's nine thousand and seventy two kilograms. But 111 00:06:15,640 --> 00:06:18,000 Speaker 1: ten metric tons is ten thousand. 112 00:06:17,680 --> 00:06:20,400 Speaker 2: Kilograms, okay if you say so. 113 00:06:20,960 --> 00:06:24,520 Speaker 1: Regardless, that's how much is raining down in particulate form. 114 00:06:24,600 --> 00:06:27,160 Speaker 1: So that's a lot of particles that it's using every second. 115 00:06:27,320 --> 00:06:29,120 Speaker 1: But there's still so much of it that's going to 116 00:06:29,200 --> 00:06:31,320 Speaker 1: take one hundred million years to dissolve. 117 00:06:32,040 --> 00:06:36,360 Speaker 2: Yeah, totally. And here's I mean, this is this kind 118 00:06:36,360 --> 00:06:39,240 Speaker 2: of tough stuff. But here's how I understand it and 119 00:06:39,279 --> 00:06:42,280 Speaker 2: how they figured some of this stuff out was while 120 00:06:42,400 --> 00:06:47,200 Speaker 2: Cassini Huygens was going through that that ring plane, they said, 121 00:06:47,200 --> 00:06:50,200 Speaker 2: the people running the mission that that three pronged Manasata 122 00:06:50,320 --> 00:06:54,080 Speaker 2: as you said, said, you know what, those those rings 123 00:06:54,120 --> 00:06:56,960 Speaker 2: and those moons have gravitational pulls, So why don't we 124 00:06:57,080 --> 00:07:00,520 Speaker 2: just let it work its magic on the space and 125 00:07:00,600 --> 00:07:03,320 Speaker 2: let it pull it a little bit in whatever direction 126 00:07:03,480 --> 00:07:05,960 Speaker 2: it's going to go in and that will result in 127 00:07:06,000 --> 00:07:09,159 Speaker 2: these little bitty changes to its trajectory and we can 128 00:07:09,200 --> 00:07:13,000 Speaker 2: measure those and that'll allow us to find out the 129 00:07:13,000 --> 00:07:15,200 Speaker 2: mass of this thing using magic. 130 00:07:15,640 --> 00:07:19,320 Speaker 1: Right, Yeah, they could detect fractions of a millimeter per 131 00:07:19,400 --> 00:07:23,160 Speaker 1: second increases in acceleration. That's how sensitive the stuff that 132 00:07:23,280 --> 00:07:27,720 Speaker 1: Cassini was sending back Cassini Huyggens. Sure, it sounds like 133 00:07:27,880 --> 00:07:33,040 Speaker 1: Jerry lewis saying Cassini, Cassini, Huygens exactly. Hey, So what 134 00:07:33,080 --> 00:07:35,280 Speaker 1: they were doing was they were figuring out the mass 135 00:07:35,320 --> 00:07:41,320 Speaker 1: of the rings by figuring out how much the probe 136 00:07:41,360 --> 00:07:46,480 Speaker 1: resisted the pull of Saturn itself. Yeah, okay, And then 137 00:07:46,520 --> 00:07:49,000 Speaker 1: by figuring out the mass of the rings, they could 138 00:07:49,040 --> 00:07:52,200 Speaker 1: make a pretty good guess at the age of the rings, right, 139 00:07:52,280 --> 00:07:55,520 Speaker 1: because less mass would be younger, more mass would be older. 140 00:07:55,560 --> 00:07:57,760 Speaker 1: Because this is a These things are spinning in a 141 00:07:57,880 --> 00:08:00,840 Speaker 1: very tight orbit around Saturn. They're not like these solid things. 142 00:08:01,160 --> 00:08:03,040 Speaker 1: It's kind of like an asteroid belt, but there's so 143 00:08:03,200 --> 00:08:06,720 Speaker 1: much stuff in there that they actually appear as rings. 144 00:08:07,320 --> 00:08:09,800 Speaker 2: An solo couldn't even navigate that asteroidery. 145 00:08:09,360 --> 00:08:12,360 Speaker 1: Not a chance. And so the longer that they are around, 146 00:08:12,360 --> 00:08:16,400 Speaker 1: the more space stuff they're going to attract. So there 147 00:08:16,400 --> 00:08:19,040 Speaker 1: would be more masks, the older they were, less mass, 148 00:08:19,080 --> 00:08:21,120 Speaker 1: the younger they were. But what they found out was 149 00:08:21,520 --> 00:08:24,200 Speaker 1: that the predictions were way off, that what they came 150 00:08:24,280 --> 00:08:27,280 Speaker 1: up with was just didn't make any sense. And what 151 00:08:27,360 --> 00:08:30,120 Speaker 1: they figured out how to explain it was actually taught 152 00:08:30,160 --> 00:08:32,840 Speaker 1: them a lot about what's going on inside of Saturn. 153 00:08:33,480 --> 00:08:38,160 Speaker 2: Yeah, as they figured out in the end, that was because, 154 00:08:38,240 --> 00:08:40,120 Speaker 2: like we said, it was being altered by the tug 155 00:08:40,720 --> 00:08:44,160 Speaker 2: of gravity, but it was also being altered by these 156 00:08:44,200 --> 00:08:47,960 Speaker 2: big flows of material in that atmosphere at the equator, 157 00:08:48,520 --> 00:08:51,959 Speaker 2: which was about six thousand miles deep, and they were 158 00:08:52,000 --> 00:08:55,240 Speaker 2: moving slower, about four percent slower than the upper atmosphereic 159 00:08:55,320 --> 00:08:58,560 Speaker 2: clouds that we could see. And that was sort of 160 00:08:58,600 --> 00:09:01,680 Speaker 2: the discrepancy. It was that they did not know about 161 00:09:01,760 --> 00:09:03,720 Speaker 2: and therefore couldn't predict right. 162 00:09:04,640 --> 00:09:06,960 Speaker 1: So once they figured out that the mass of the 163 00:09:07,040 --> 00:09:10,440 Speaker 1: rings are actually much lower than they thought, they took 164 00:09:10,480 --> 00:09:15,800 Speaker 1: some other measurement from I can't remember, some sort of waves. 165 00:09:16,360 --> 00:09:18,440 Speaker 1: I guess gravitation always, but I don't think that's what 166 00:09:18,480 --> 00:09:23,200 Speaker 1: it was. Yes, they had a measurement from before that 167 00:09:23,200 --> 00:09:25,920 Speaker 1: they're like, that is way low. There must be some 168 00:09:26,000 --> 00:09:28,280 Speaker 1: hidden mass in there that we're not detecting from the 169 00:09:28,400 --> 00:09:32,079 Speaker 1: density waves. And when they did the calculations they figured 170 00:09:32,120 --> 00:09:35,200 Speaker 1: out Nope, that was actually a pretty good estimate. These 171 00:09:35,200 --> 00:09:37,800 Speaker 1: things are not as massive as you think, so they're 172 00:09:37,800 --> 00:09:43,880 Speaker 1: made up of fairly light stuff. And because it's not massive, 173 00:09:44,679 --> 00:09:47,880 Speaker 1: and because the rings are still very bright, it suggests 174 00:09:47,880 --> 00:09:50,679 Speaker 1: that there's not a lot of rocky crud mixed in there, 175 00:09:50,720 --> 00:09:54,200 Speaker 1: which suggests that they're fairly young. So they estimate that 176 00:09:54,240 --> 00:09:57,760 Speaker 1: the age of Saturn's rings are between one hundred and 177 00:09:57,920 --> 00:09:59,120 Speaker 1: ten million years. 178 00:09:58,920 --> 00:10:03,240 Speaker 2: Old, Yeah, which is way off. Initially they said anywhere 179 00:10:03,240 --> 00:10:05,839 Speaker 2: it depends, but from four point five billion years to 180 00:10:05,960 --> 00:10:09,360 Speaker 2: maybe like thirty million years. 181 00:10:09,160 --> 00:10:13,640 Speaker 1: Right, yeah, but so yeah, they figured it out what 182 00:10:13,679 --> 00:10:15,960 Speaker 1: they think figured And by the way, I want to 183 00:10:16,000 --> 00:10:20,760 Speaker 1: do a whole episode on Saturn. But they they both 184 00:10:21,080 --> 00:10:23,280 Speaker 1: that they believe. No, it's gonna be great. Remember our 185 00:10:23,360 --> 00:10:28,200 Speaker 1: Venus episode was really fun. Yeah, So what they believe 186 00:10:28,480 --> 00:10:31,080 Speaker 1: is that either the rings are made up of an 187 00:10:31,320 --> 00:10:37,120 Speaker 1: icy comet that got caught in Saturn's orbit and was 188 00:10:37,160 --> 00:10:40,920 Speaker 1: basically pulled apart by the gravity of Saturn and it 189 00:10:40,960 --> 00:10:43,400 Speaker 1: turned into spread out into a ring. So what you're 190 00:10:43,400 --> 00:10:46,200 Speaker 1: seeing is a super spread out comet, Whi's pretty cool. 191 00:10:46,320 --> 00:10:49,800 Speaker 1: It's also possible it's Moon that the same fate happened 192 00:10:49,800 --> 00:10:55,199 Speaker 1: to it just kind of crumbled and came apart, but the. 193 00:10:54,760 --> 00:10:55,760 Speaker 2: Kin might say it's beach. 194 00:10:56,480 --> 00:11:01,280 Speaker 1: The upside of it is that we're going to do 195 00:11:01,320 --> 00:11:03,600 Speaker 1: an episode on Saturday, and so look for that one day. 196 00:11:04,000 --> 00:11:06,520 Speaker 2: Yeah, And the upside is that this could I mean, 197 00:11:06,520 --> 00:11:10,440 Speaker 2: if it was an arrant comment, that could happen again 198 00:11:10,600 --> 00:11:13,840 Speaker 2: to another planet. So there could potentially, in another you know, 199 00:11:14,160 --> 00:11:17,160 Speaker 2: twenty thirty million years, be another one of our beloved 200 00:11:17,160 --> 00:11:18,520 Speaker 2: planets with their own rings. 201 00:11:18,600 --> 00:11:22,040 Speaker 1: That's right, And I sent upside on that upshot of course, 202 00:11:22,360 --> 00:11:24,800 Speaker 1: of course, and that of course means short stuff is app. 203 00:11:28,160 --> 00:11:31,040 Speaker 2: Stuff you should know is a production of iHeartRadio. For 204 00:11:31,120 --> 00:11:35,319 Speaker 2: more podcasts my heart Radio, visit the iHeartRadio app, Apple Podcasts, 205 00:11:35,440 --> 00:11:42,360 Speaker 2: or wherever you listen to your favorite shows