1 00:00:00,280 --> 00:00:02,960 Speaker 1: Brought to you by the reinvented two thousand twelve Camray. 2 00:00:03,160 --> 00:00:08,920 Speaker 1: It's ready. Are you get in touch with technology? With 3 00:00:09,039 --> 00:00:18,040 Speaker 1: tech Stuff from how stuff works dot com. Hello again, everyone, 4 00:00:18,079 --> 00:00:20,320 Speaker 1: and welcome to tech stuff. My name is Chris Poulette 5 00:00:20,320 --> 00:00:23,000 Speaker 1: and I am an editor at how stuff works dot com. 6 00:00:23,000 --> 00:00:26,440 Speaker 1: Sitting across from me, as always, is senior writer Jonathan Strickland. 7 00:00:26,640 --> 00:00:28,680 Speaker 1: The governor and I aren't even in the same party. 8 00:00:28,720 --> 00:00:30,520 Speaker 1: If this turns out to be a false alarm, he'll 9 00:00:30,520 --> 00:00:32,320 Speaker 1: make me out to be the biggest fool west of 10 00:00:32,360 --> 00:00:37,800 Speaker 1: the Mississippi. Hey, nice Mississippi. Yeah, you know what. That's 11 00:00:37,800 --> 00:00:42,040 Speaker 1: the site of several faults, actually one great, big fault. 12 00:00:42,040 --> 00:00:44,680 Speaker 1: There are lots of faults everywhere, and it's not my fault. No, 13 00:00:45,159 --> 00:00:47,400 Speaker 1: before we get into whose fault it is, let's talk 14 00:00:47,400 --> 00:00:51,120 Speaker 1: about listener mail. By the way, this is not his fault. 15 00:00:56,680 --> 00:01:00,520 Speaker 1: This listener mail comes from Joe, and Joe says earthquake. No, 16 00:01:00,680 --> 00:01:03,040 Speaker 1: just kidding. I live in Christchurch, New Zealand, and I've 17 00:01:03,080 --> 00:01:05,320 Speaker 1: been through two major earthquakes and I was wondering if 18 00:01:05,319 --> 00:01:08,000 Speaker 1: you could do a podcast on how they measure earthquakes. 19 00:01:08,319 --> 00:01:13,880 Speaker 1: Cheers Joe, Joe, we're very glad that you are okay. Definitely, 20 00:01:13,959 --> 00:01:16,640 Speaker 1: so definitely, So that was a scary situation if you 21 00:01:16,680 --> 00:01:20,360 Speaker 1: don't know. Um uh, just a few weeks ago, as 22 00:01:20,360 --> 00:01:24,080 Speaker 1: I when we're recording this, in very late February two eleven, 23 00:01:24,200 --> 00:01:28,400 Speaker 1: there was a pretty significant earthquake, to say the very least, 24 00:01:28,560 --> 00:01:32,600 Speaker 1: that hit New Zealand. Um and uh, you know, several 25 00:01:32,600 --> 00:01:35,880 Speaker 1: people lost their lives as a result of this. Um 26 00:01:35,959 --> 00:01:40,520 Speaker 1: And of course these things are very damaging, both to 27 00:01:40,840 --> 00:01:44,480 Speaker 1: people and property. So it's a it would be nice 28 00:01:44,520 --> 00:01:46,560 Speaker 1: if we could do a lot of prediction and give 29 00:01:46,600 --> 00:01:48,640 Speaker 1: you a heads up from when these things are coming, 30 00:01:48,760 --> 00:01:51,720 Speaker 1: but I'm afraid at this point about the best we 31 00:01:51,760 --> 00:01:53,880 Speaker 1: can do is let you know how big they were 32 00:01:54,000 --> 00:01:57,840 Speaker 1: and maybe get an idea of what you might expect 33 00:01:57,880 --> 00:02:01,520 Speaker 1: from an aftershock. Yeah. As it turns out, predicting an 34 00:02:01,520 --> 00:02:06,680 Speaker 1: earthquake is not exact science, but we have learned quite 35 00:02:06,720 --> 00:02:09,840 Speaker 1: a bit about earthquakes. And before we get too far 36 00:02:09,880 --> 00:02:12,239 Speaker 1: into this, I should just point out that a couple 37 00:02:12,320 --> 00:02:16,320 Speaker 1: of our sister podcasts have covered similar topics. Stuff you 38 00:02:16,320 --> 00:02:19,079 Speaker 1: Should Know has done an entire episode on how earthquakes work. 39 00:02:19,120 --> 00:02:21,680 Speaker 1: It's actually one of their older episodes, but it's it's excellent, 40 00:02:21,760 --> 00:02:24,800 Speaker 1: so you can listen to that if you are interested 41 00:02:24,880 --> 00:02:28,280 Speaker 1: in the topic and the stuff of Genius did an 42 00:02:28,320 --> 00:02:34,160 Speaker 1: episode about an early pioneer in seismology, which and we'll 43 00:02:34,160 --> 00:02:35,720 Speaker 1: talk about him in a little bit, just because it's 44 00:02:36,120 --> 00:02:38,760 Speaker 1: it's too cool not to talk about, right, Oh yeah, yeah, 45 00:02:38,800 --> 00:02:42,880 Speaker 1: definitely so so an earthquake. You know, we most of 46 00:02:42,960 --> 00:02:45,919 Speaker 1: us probably know exactly what someone means when they say earthquake. 47 00:02:45,960 --> 00:02:48,520 Speaker 1: It's it's an event in which the ground is shaking 48 00:02:48,680 --> 00:02:54,359 Speaker 1: right right, the earth thing. Yeah, yeah, Um, they can 49 00:02:54,360 --> 00:02:58,880 Speaker 1: be caused from from many many different related types of 50 00:02:58,960 --> 00:03:03,760 Speaker 1: movement in the Earth. Um, it's pretty well, uh, pretty 51 00:03:03,760 --> 00:03:06,320 Speaker 1: well known at this point that the Earth's crust is 52 00:03:06,320 --> 00:03:10,440 Speaker 1: made up of many plates, and there are different kinds 53 00:03:10,720 --> 00:03:14,920 Speaker 1: of they're they're moving in different ways. Um. I'm going 54 00:03:15,000 --> 00:03:19,160 Speaker 1: back to my undergraduate days when I actually took a 55 00:03:19,200 --> 00:03:22,560 Speaker 1: geology class, which I found fascinating but didn't go into 56 00:03:22,560 --> 00:03:26,200 Speaker 1: it obviously as a career field. But um, in some cases, 57 00:03:26,200 --> 00:03:29,400 Speaker 1: one plate is going underneath another plate. In other cases, 58 00:03:29,440 --> 00:03:32,240 Speaker 1: they're rubbing against one another in a and you know 59 00:03:32,320 --> 00:03:34,480 Speaker 1: along you know, one is going north while the other 60 00:03:34,520 --> 00:03:38,160 Speaker 1: is going south. And and gradually what happens is tension 61 00:03:38,160 --> 00:03:41,800 Speaker 1: builds up. I'm oversimplifying here, but tension builds up, and 62 00:03:42,200 --> 00:03:46,160 Speaker 1: when the tension is released, that causes an earthquake. And 63 00:03:46,200 --> 00:03:48,440 Speaker 1: they can be you know, small enough that you don't 64 00:03:48,440 --> 00:03:51,080 Speaker 1: even notice it. Um. But some of the equipment we're 65 00:03:51,080 --> 00:03:56,000 Speaker 1: going to talk about today can detect that. Of course, others, um, 66 00:03:56,120 --> 00:03:59,400 Speaker 1: like the earthquake in New Zealand and and famous earthquakes 67 00:03:59,440 --> 00:04:05,840 Speaker 1: like in Haiti and uh in California, in Japan, um 68 00:04:06,000 --> 00:04:08,480 Speaker 1: and and my favorite fault, the New Madrid fault in 69 00:04:08,480 --> 00:04:10,600 Speaker 1: the middle of the United States. Again, that would be 70 00:04:10,640 --> 00:04:14,880 Speaker 1: the one near Mississippi and all the others around it. Um. 71 00:04:14,920 --> 00:04:18,680 Speaker 1: You know, those can can be very very serious. So uh, 72 00:04:18,680 --> 00:04:22,080 Speaker 1: you know, scientists have been trying to figure out for 73 00:04:22,920 --> 00:04:26,560 Speaker 1: a long time, we'll say a very very very long 74 00:04:26,600 --> 00:04:31,640 Speaker 1: time millennia in fact, yes, exactly how to measure the 75 00:04:31,680 --> 00:04:36,440 Speaker 1: effect of the earth shaking. So let's talk about what 76 00:04:36,560 --> 00:04:38,480 Speaker 1: actually happens and then we can talk about how we 77 00:04:38,880 --> 00:04:42,080 Speaker 1: how we measure it. Now you gave a good overview. Yeah, there's, 78 00:04:42,200 --> 00:04:44,680 Speaker 1: like I said, that's just a nutshell, very very very 79 00:04:44,720 --> 00:04:48,080 Speaker 1: basic version, right, Yeah, three basic ways that plates move 80 00:04:48,120 --> 00:04:50,720 Speaker 1: against each other. Right, they either move apart, or they 81 00:04:50,800 --> 00:04:53,720 Speaker 1: move together, or they slide against each other. Right, that's 82 00:04:53,720 --> 00:04:56,000 Speaker 1: about it. The by the way, if you're talking about 83 00:04:56,040 --> 00:05:00,680 Speaker 1: a plate going underneath another, that's called subducting. Um, just 84 00:05:00,720 --> 00:05:04,760 Speaker 1: so you guys know. And when plates, when plates meet, uh, 85 00:05:04,800 --> 00:05:09,960 Speaker 1: it pushes rock and dirt together. That's what actually forms mountains. Besides, 86 00:05:10,120 --> 00:05:12,920 Speaker 1: there's also volcanic mountains, so there's some mountains that are 87 00:05:12,920 --> 00:05:15,559 Speaker 1: formed through volcanic activity. But in general, mountains are formed 88 00:05:15,880 --> 00:05:18,400 Speaker 1: when two plates pressed up against each other and they 89 00:05:18,480 --> 00:05:25,400 Speaker 1: crinkle essentially. Um. Now, when these these uh, these events happen, 90 00:05:25,480 --> 00:05:27,320 Speaker 1: these these plate events. By the way, there are other 91 00:05:27,360 --> 00:05:31,159 Speaker 1: things that can cause an earthquake, like an explosion can 92 00:05:31,200 --> 00:05:36,000 Speaker 1: cause the essentially a localized earthquake, and meteoric impact can 93 00:05:36,080 --> 00:05:38,040 Speaker 1: cause an earthquake, that kind of thing. But most of 94 00:05:38,040 --> 00:05:41,360 Speaker 1: them are caused by these these plate movements. Um. There's 95 00:05:41,360 --> 00:05:44,080 Speaker 1: about eight thousand of them each day, and most of 96 00:05:44,080 --> 00:05:48,200 Speaker 1: them are uh beneath our level of being able to 97 00:05:48,240 --> 00:05:50,679 Speaker 1: perceive them. And of course lots of them are happening 98 00:05:50,720 --> 00:05:54,400 Speaker 1: in places where there's really little to know human habitat there, 99 00:05:54,440 --> 00:05:58,000 Speaker 1: so we wouldn't necessarily notice it even if it were 100 00:05:58,160 --> 00:06:01,360 Speaker 1: a significant earthquake, because one is there, right, might be 101 00:06:01,440 --> 00:06:05,080 Speaker 1: under the ocean or anything like that. Um. And like 102 00:06:05,120 --> 00:06:07,039 Speaker 1: you were saying, where the plates meet, that's a fault. 103 00:06:07,800 --> 00:06:10,240 Speaker 1: That's you know, any place where two two plates are meeting, 104 00:06:10,240 --> 00:06:14,080 Speaker 1: that's a fault. When when there is an earthquake, energy 105 00:06:14,240 --> 00:06:19,040 Speaker 1: radiates out from the center of that earthquake in seismic waves. Yes, 106 00:06:19,680 --> 00:06:22,240 Speaker 1: and these waves are what you would you know, when 107 00:06:22,279 --> 00:06:24,080 Speaker 1: you think of a wave, that's what we're talking about. 108 00:06:24,160 --> 00:06:29,119 Speaker 1: It's energy moving in a wavelength. There's there's a peak 109 00:06:29,320 --> 00:06:32,960 Speaker 1: and there's a trough through this wave. And uh, there's 110 00:06:33,000 --> 00:06:35,960 Speaker 1: actually two waves that move out from an earthquake. Yes, 111 00:06:36,000 --> 00:06:39,560 Speaker 1: he's talking about the PEA wave in which those those 112 00:06:39,560 --> 00:06:43,159 Speaker 1: waves move in the direction that they're they're being propagated. 113 00:06:43,800 --> 00:06:47,880 Speaker 1: Um and then the S wave, which is perpendicular to that, right, 114 00:06:47,920 --> 00:06:51,240 Speaker 1: And the PEA wave moves faster than the S wave. 115 00:06:51,320 --> 00:06:54,880 Speaker 1: It actually goes about between one to five miles per second. 116 00:06:55,360 --> 00:06:58,800 Speaker 1: It tends to be one point seven times faster than 117 00:06:58,920 --> 00:07:01,680 Speaker 1: the than the S wave. So this has become a 118 00:07:01,800 --> 00:07:06,640 Speaker 1: key for us to figure out where earthquakes are originating. Right, 119 00:07:06,720 --> 00:07:10,200 Speaker 1: because you measure the time between the primary wave and 120 00:07:10,240 --> 00:07:13,120 Speaker 1: the secondary wave, and that will tell you, in general 121 00:07:13,360 --> 00:07:15,840 Speaker 1: how far away the focus is. It doesn't tell you 122 00:07:15,880 --> 00:07:18,760 Speaker 1: the direction. It will just tell you. You know, you 123 00:07:18,800 --> 00:07:20,800 Speaker 1: feel a shaking, and then you feel a second shaking. 124 00:07:20,840 --> 00:07:23,680 Speaker 1: You take the time between that, you do a little calculation. 125 00:07:23,680 --> 00:07:26,320 Speaker 1: You figured, all right, so the center of this earthquake 126 00:07:26,560 --> 00:07:29,640 Speaker 1: is fifty miles away, but it could literally be fifty 127 00:07:29,640 --> 00:07:34,600 Speaker 1: miles in any direction on the surface. You can discount 128 00:07:34,640 --> 00:07:37,240 Speaker 1: the directions that are directly below you and directly above you, 129 00:07:37,320 --> 00:07:42,440 Speaker 1: and all that like anything in the air, not gonna matter. Um. 130 00:07:42,480 --> 00:07:46,440 Speaker 1: So that's that's the basics of earthquakes. We'll talk a 131 00:07:46,440 --> 00:07:48,800 Speaker 1: little bit about the measuring. Let's let's let's take a 132 00:07:48,840 --> 00:07:52,760 Speaker 1: little walk back into history by a couple of millennia. 133 00:07:52,920 --> 00:07:54,760 Speaker 1: This is the guy that we were talking about and 134 00:07:54,800 --> 00:08:00,560 Speaker 1: the stuff of genius who came up with an interesting seismoscope. Now, 135 00:08:00,560 --> 00:08:05,240 Speaker 1: a seismoscope is a an instrument, any instrument that indicates 136 00:08:05,240 --> 00:08:08,120 Speaker 1: that motion has occurred. But it does not give you 137 00:08:08,840 --> 00:08:12,800 Speaker 1: more information than that, right right. It can't necessarily tell 138 00:08:12,800 --> 00:08:17,320 Speaker 1: you where it was coming from. It can't necessarily tell you, um, 139 00:08:17,960 --> 00:08:20,160 Speaker 1: it can't give you like a reading over a duration 140 00:08:20,160 --> 00:08:23,520 Speaker 1: of time, it just tells you, hey, stuff moved around. 141 00:08:24,160 --> 00:08:28,000 Speaker 1: So basically, if you've seen Jurassic Park, when that dinosaur 142 00:08:28,080 --> 00:08:30,800 Speaker 1: is coming up on you and you watch the motion 143 00:08:30,960 --> 00:08:33,000 Speaker 1: in the glass of water, in the glass of water, 144 00:08:33,200 --> 00:08:36,760 Speaker 1: that wop. Yes, it's a very primitive seismoscope, but as 145 00:08:36,800 --> 00:08:42,199 Speaker 1: slightly and I stress slightly more sophisticated seismoscope was invented 146 00:08:42,360 --> 00:08:46,440 Speaker 1: by a Chinese philosopher named Chong Hang Yes, and one 147 00:08:46,480 --> 00:08:50,319 Speaker 1: thirty two. Yeah, one thirty two a d Yes, that's 148 00:08:50,320 --> 00:08:52,520 Speaker 1: not that, that's not one thirty two in the afternoon. 149 00:08:52,640 --> 00:08:57,120 Speaker 1: That's the year. Um No, Chang hangg came up with 150 00:08:57,160 --> 00:09:01,200 Speaker 1: this really cool design. And we we've actually seen examples 151 00:09:01,320 --> 00:09:05,640 Speaker 1: of this and you know, uh, not just it's it's 152 00:09:05,679 --> 00:09:08,800 Speaker 1: not just a theory that these things actually existed. Though 153 00:09:08,840 --> 00:09:13,160 Speaker 1: they're they're actual, the way they worked is somewhat of 154 00:09:13,160 --> 00:09:15,280 Speaker 1: a mystery. We've got a couple of ideas of how 155 00:09:15,280 --> 00:09:17,520 Speaker 1: they could have worked, but but we'll get to that. 156 00:09:17,640 --> 00:09:20,960 Speaker 1: So basically, what you had was a wine jar. Yes, 157 00:09:21,040 --> 00:09:23,040 Speaker 1: it was. It was cylinder. You know, think of it 158 00:09:23,080 --> 00:09:25,960 Speaker 1: as a sort of cylindrical shape standing on in so 159 00:09:26,160 --> 00:09:29,959 Speaker 1: like a jar. Yes, six ft in diameter, so we're 160 00:09:30,000 --> 00:09:32,079 Speaker 1: not talking like a little jar, No, this would be 161 00:09:32,120 --> 00:09:34,840 Speaker 1: a big jar. And mounted to the jar on the 162 00:09:34,920 --> 00:09:39,000 Speaker 1: jar were eight dragon head spouts that faced in the 163 00:09:39,000 --> 00:09:42,000 Speaker 1: cardinal directions. Yes, and that would be at the very 164 00:09:42,040 --> 00:09:45,000 Speaker 1: top of the jar from what from what I understand, 165 00:09:45,240 --> 00:09:48,400 Speaker 1: it can be anywhere from the above the middle to 166 00:09:48,520 --> 00:09:51,360 Speaker 1: the top of anything on the top half of the jar. 167 00:09:51,520 --> 00:09:53,920 Speaker 1: Is that's because I've actually seen pictures of these. There 168 00:09:53,920 --> 00:09:56,640 Speaker 1: are images of these on the Internet of various people 169 00:09:56,679 --> 00:10:00,200 Speaker 1: have made recreations of these things. Um. So within that 170 00:10:00,320 --> 00:10:04,680 Speaker 1: each dragon's mouth there's essentially a marble or stone, and 171 00:10:05,040 --> 00:10:08,640 Speaker 1: so those are balanced within the mouths of the dragons. 172 00:10:09,040 --> 00:10:13,960 Speaker 1: And then underneath the dragon mouths are these little ceramic 173 00:10:14,080 --> 00:10:17,320 Speaker 1: frogs with open mouths. And the idea here is that 174 00:10:17,360 --> 00:10:20,480 Speaker 1: if there's an earthquake that is significant enough for it 175 00:10:20,559 --> 00:10:24,920 Speaker 1: to set this seis muscope off, it'll rattle the pebbles, 176 00:10:25,000 --> 00:10:27,200 Speaker 1: and the pebbles that are facing the direction that the 177 00:10:27,200 --> 00:10:31,000 Speaker 1: earthquake is coming from, uh would theoretically fall out the 178 00:10:31,040 --> 00:10:33,720 Speaker 1: dragon's mouth into the frog mouth. So then you could 179 00:10:33,800 --> 00:10:36,240 Speaker 1: look in and say, all right, this is coming from 180 00:10:36,360 --> 00:10:40,840 Speaker 1: somewhere the north northeast region. Um, it doesn't tell you 181 00:10:40,840 --> 00:10:45,040 Speaker 1: how far away it's gonna the earthquake was. But let's 182 00:10:45,040 --> 00:10:49,400 Speaker 1: say that you're in ancient China and you are overseeing 183 00:10:49,480 --> 00:10:54,000 Speaker 1: a large amount of land. Communication is not fast. But 184 00:10:54,160 --> 00:10:57,800 Speaker 1: seeing something like that happened, you could say, well, now 185 00:10:57,840 --> 00:11:00,400 Speaker 1: I know that there's some problems to the north of us. 186 00:11:00,679 --> 00:11:04,480 Speaker 1: I should expect some people to come and ask me 187 00:11:04,559 --> 00:11:09,160 Speaker 1: for help, or maybe I should send Uh perhaps it 188 00:11:09,200 --> 00:11:11,760 Speaker 1: came from the direction that an enemy is in. Perhaps 189 00:11:11,840 --> 00:11:14,520 Speaker 1: you would want to send a group of troops out 190 00:11:14,559 --> 00:11:17,200 Speaker 1: there to see, like, hey, were they weakened enough for 191 00:11:17,280 --> 00:11:19,679 Speaker 1: us to kind of come in and mop up? Right? 192 00:11:19,720 --> 00:11:23,760 Speaker 1: So this isn't this isn't just a diversion, uh, you know, 193 00:11:23,840 --> 00:11:25,559 Speaker 1: just something that you do for fun. They really had 194 00:11:25,559 --> 00:11:29,360 Speaker 1: a practical use. Now, now, the point where I said 195 00:11:29,559 --> 00:11:32,000 Speaker 1: it might be a bit of a mystery is that 196 00:11:33,120 --> 00:11:36,520 Speaker 1: we're not sure what was inside the jar. There are 197 00:11:36,559 --> 00:11:40,120 Speaker 1: some who think that the jar had perhaps a pendulum 198 00:11:40,160 --> 00:11:43,319 Speaker 1: suspended from the top of the jar. That so it's 199 00:11:43,360 --> 00:11:45,800 Speaker 1: it's actually you know, the base of the weight of 200 00:11:45,840 --> 00:11:48,360 Speaker 1: the pendulum would be inside the jar. That's funny that 201 00:11:48,400 --> 00:11:49,880 Speaker 1: you have mentioned that, because I have the feeling that 202 00:11:49,920 --> 00:11:52,320 Speaker 1: will come up again. Yes, and this is because you 203 00:11:52,360 --> 00:11:56,120 Speaker 1: need an inertial mass in most of these seismoscopes. You 204 00:11:56,200 --> 00:11:59,320 Speaker 1: need something that is not going to move in relation 205 00:11:59,440 --> 00:12:02,560 Speaker 1: to the rest of the instrument because one of the 206 00:12:02,559 --> 00:12:05,800 Speaker 1: big challenges of measuring earthquakes, I mean it sounds silly, 207 00:12:05,800 --> 00:12:08,240 Speaker 1: but it's true, is that you have to design a 208 00:12:08,320 --> 00:12:11,800 Speaker 1: tool that can measure something even when the uh the 209 00:12:11,800 --> 00:12:15,680 Speaker 1: tool itself is moving right like, you know, if the 210 00:12:15,679 --> 00:12:18,040 Speaker 1: earth is quaking and the tool is on the earth, 211 00:12:18,640 --> 00:12:21,520 Speaker 1: then how do you get a reliable measurement. Well, this 212 00:12:21,679 --> 00:12:24,520 Speaker 1: idea of an inertial mass becomes very important with later 213 00:12:24,960 --> 00:12:30,840 Speaker 1: size seismometers. So um, yeah, there was one possibility. Another 214 00:12:30,880 --> 00:12:34,000 Speaker 1: possibility was a reverse pendulum. And a reverse pendulum is 215 00:12:34,040 --> 00:12:37,760 Speaker 1: essentially a flexible pole with a weight at the end 216 00:12:37,760 --> 00:12:40,720 Speaker 1: of it. The weight is on the top right, And 217 00:12:40,760 --> 00:12:45,480 Speaker 1: the idea here is that a significant UH quake would 218 00:12:45,480 --> 00:12:48,520 Speaker 1: cause the pendulum to swing, perhaps hitting the inside of 219 00:12:48,520 --> 00:12:52,360 Speaker 1: the jar, and that's what would then cause the stone 220 00:12:52,400 --> 00:12:55,600 Speaker 1: in that dragon's mouth to fall into the the frog's mouth, 221 00:12:56,280 --> 00:13:02,040 Speaker 1: and then it's six more weeks of winter. Uh, okay, stuff, 222 00:13:02,040 --> 00:13:06,640 Speaker 1: I'm a little bit I'm on cold medication. So yeah, 223 00:13:07,520 --> 00:13:10,920 Speaker 1: And in doing some research I read in in Britannica 224 00:13:11,000 --> 00:13:16,239 Speaker 1: that in Italy in the seventeenth century, um a seismoscope. 225 00:13:16,280 --> 00:13:19,679 Speaker 1: They're used spilling water to show you know what was 226 00:13:19,720 --> 00:13:23,000 Speaker 1: going on, whether there was an earthquake taking place. And 227 00:13:23,920 --> 00:13:26,960 Speaker 1: another they also used a lot of mercury. I know 228 00:13:27,040 --> 00:13:29,319 Speaker 1: that's probably not a surprise, but yeah, a cup of mercury, 229 00:13:29,320 --> 00:13:31,920 Speaker 1: which would be would probably be a pretty good indicator 230 00:13:32,080 --> 00:13:35,600 Speaker 1: given its color. Um. Yeah, too bad, you'd be crazy 231 00:13:35,679 --> 00:13:37,720 Speaker 1: by the time the earthquake hit. Now see you're getting 232 00:13:37,760 --> 00:13:40,080 Speaker 1: into the tiny details that are just just ruined them 233 00:13:40,160 --> 00:13:43,880 Speaker 1: the magic for me. Um and uh. And then there 234 00:13:43,920 --> 00:13:48,920 Speaker 1: was a Luigi Palmieri who had a seized seismometer to detect, 235 00:13:49,440 --> 00:13:51,760 Speaker 1: you know, the motion during an earthquake. He had a 236 00:13:51,760 --> 00:13:56,440 Speaker 1: series of use you shaped tubes that again used mercury. Um. 237 00:13:56,480 --> 00:13:58,840 Speaker 1: And then there was a clock hooked up to that 238 00:13:58,920 --> 00:14:02,560 Speaker 1: and um, what would happen is the motion would cause 239 00:14:02,800 --> 00:14:08,079 Speaker 1: an electrical clock to stop and to start a recording drum. Um. Basically, 240 00:14:08,080 --> 00:14:10,160 Speaker 1: there was a float on top of the mercury and 241 00:14:10,200 --> 00:14:13,480 Speaker 1: the drum was keeping track of the floats motion as 242 00:14:13,480 --> 00:14:15,440 Speaker 1: it moved. It would tell you the time and intensity 243 00:14:15,480 --> 00:14:19,080 Speaker 1: of the earthquake. That makes it more that. That's why 244 00:14:19,120 --> 00:14:22,120 Speaker 1: we would refer to that as a seismoment or even 245 00:14:22,160 --> 00:14:27,120 Speaker 1: a seismograph, because seismograph essentially that that graph means to draw, 246 00:14:27,760 --> 00:14:31,120 Speaker 1: but it's it's essentially meaning that you are recording the 247 00:14:31,200 --> 00:14:34,360 Speaker 1: event of the earthquake and there's some element of time 248 00:14:34,440 --> 00:14:38,560 Speaker 1: there or you can actually see the earthquakes movements over 249 00:14:38,640 --> 00:14:41,360 Speaker 1: time and be able to say this is when it started, 250 00:14:41,400 --> 00:14:44,440 Speaker 1: this is when it ended, and um. And that's what 251 00:14:44,520 --> 00:14:48,000 Speaker 1: sets it apart from the seismoscopes, which essentially just tell you, hey, 252 00:14:48,040 --> 00:14:50,880 Speaker 1: something's moving out there, yes, which you know a lot 253 00:14:50,920 --> 00:14:54,760 Speaker 1: of us can do on a good day. I can 254 00:14:54,800 --> 00:14:58,960 Speaker 1: do it. The rabbits, they're agitated. So let's let's talk 255 00:14:59,000 --> 00:15:01,640 Speaker 1: a little bit about what it takes to get uh. 256 00:15:01,960 --> 00:15:05,320 Speaker 1: One of some of the challenges in creating a seismic graph, Well, 257 00:15:05,320 --> 00:15:09,520 Speaker 1: there's one very big challenge, which is to overcome friction. 258 00:15:10,400 --> 00:15:14,160 Speaker 1: That's a big one because see, and in a seismograph, 259 00:15:14,520 --> 00:15:17,680 Speaker 1: in a lot of cases, especially the earlier seismographs, you 260 00:15:17,680 --> 00:15:22,360 Speaker 1: would want to use a marketing device, a pen and 261 00:15:22,440 --> 00:15:26,240 Speaker 1: a piece of paper essentially, um and uh. The problem 262 00:15:26,360 --> 00:15:30,480 Speaker 1: is that the in order to be sensitive, the pen 263 00:15:30,600 --> 00:15:32,920 Speaker 1: is marking on the paper right right to record the 264 00:15:32,920 --> 00:15:36,520 Speaker 1: Earth's motion UM. But the problem is that it has 265 00:15:36,560 --> 00:15:39,200 Speaker 1: to overcome the friction of the pen on the paper 266 00:15:39,360 --> 00:15:42,040 Speaker 1: right and if it's a very very subtle quake, then 267 00:15:42,560 --> 00:15:44,720 Speaker 1: the friction may be too great for the pen to 268 00:15:44,800 --> 00:15:49,160 Speaker 1: move UM. And that that is a very big challenge. 269 00:15:49,200 --> 00:15:51,120 Speaker 1: It it doesn't seem like it would be that big, 270 00:15:51,160 --> 00:15:54,040 Speaker 1: but if you think about it, uh, you know, if 271 00:15:54,080 --> 00:15:57,040 Speaker 1: you had a UM I would imagine too for older 272 00:15:57,440 --> 00:16:01,640 Speaker 1: pens before ballpoint type technology it's created. If you had 273 00:16:01,680 --> 00:16:05,280 Speaker 1: something like some of these UM seismographs where it was 274 00:16:05,320 --> 00:16:08,840 Speaker 1: constantly moving UM, when the paper was constantly moving under 275 00:16:08,840 --> 00:16:11,200 Speaker 1: the pen, I'm not sure how you would distribute inc 276 00:16:11,360 --> 00:16:13,800 Speaker 1: to it unless it worked sort of like a fountainin 277 00:16:13,800 --> 00:16:15,480 Speaker 1: And I didn't actually research that. I wish I had 278 00:16:15,520 --> 00:16:20,120 Speaker 1: because now I'm kind of intrigued the podcast. But yeah, 279 00:16:20,160 --> 00:16:24,880 Speaker 1: I mean that the seismograph is not a twentieth century innovation, 280 00:16:25,080 --> 00:16:28,360 Speaker 1: and you know the ballpoint pen, well it wasn't either, 281 00:16:28,520 --> 00:16:32,640 Speaker 1: but the seismograph goes back farther. So another big challenge 282 00:16:32,840 --> 00:16:36,320 Speaker 1: is that you have to you have to segregate the 283 00:16:36,400 --> 00:16:41,400 Speaker 1: seismograph from other structures. Yes, So for example, here in 284 00:16:41,440 --> 00:16:43,920 Speaker 1: our building, it wouldn't do us much good to have 285 00:16:43,960 --> 00:16:47,840 Speaker 1: a seismograph here because the vibrations that we would create 286 00:16:47,960 --> 00:16:51,080 Speaker 1: in the building, the vibrations from traffic passing outside. The 287 00:16:51,080 --> 00:16:53,080 Speaker 1: seismograph would pick all that up and we get a 288 00:16:53,120 --> 00:16:56,080 Speaker 1: lot of false readings, false positives. Yeah, if you've ever 289 00:16:56,120 --> 00:16:57,720 Speaker 1: been on the top floor of a parking deck when 290 00:16:57,720 --> 00:17:00,880 Speaker 1: people are leaving at rush hour, I mean you'll feel 291 00:17:01,000 --> 00:17:04,480 Speaker 1: the motion of the cars moving and sometimes they'll you know, 292 00:17:04,560 --> 00:17:06,240 Speaker 1: you can bounce around a little bit, depending on the 293 00:17:06,240 --> 00:17:09,840 Speaker 1: parking deck. So the key to having a very good 294 00:17:09,840 --> 00:17:13,480 Speaker 1: seismograph is finding a way so that you can you 295 00:17:13,480 --> 00:17:17,040 Speaker 1: can connect it to the bedrock of whatever region you're in. 296 00:17:17,960 --> 00:17:21,119 Speaker 1: I will I will try to do flint stones. I 297 00:17:21,240 --> 00:17:25,400 Speaker 1: hated that cartoon really, Yeah, despised it with the heat 298 00:17:25,400 --> 00:17:27,480 Speaker 1: of a thousand exploding suns. Well, we won't get into 299 00:17:27,520 --> 00:17:31,200 Speaker 1: that um. But yes, you have to connect it to 300 00:17:31,240 --> 00:17:33,360 Speaker 1: the bedrock and then once sits connect to the bed 301 00:17:33,560 --> 00:17:37,880 Speaker 1: bedrock and and completely separate from other buildings. So it's 302 00:17:37,880 --> 00:17:45,840 Speaker 1: not getting essentially uh pollution really because vibration vibration, then 303 00:17:45,880 --> 00:17:49,359 Speaker 1: you can be more more sure that the readings you 304 00:17:49,400 --> 00:17:52,040 Speaker 1: get reflect what's actually going on with the Earth as 305 00:17:52,040 --> 00:17:58,359 Speaker 1: opposed to localized events. And it's interesting, this idea of 306 00:17:58,400 --> 00:18:02,040 Speaker 1: the inertial mass ends up being really really important. Yes, 307 00:18:02,440 --> 00:18:06,200 Speaker 1: and there's it's it's funny because um pendulums have been 308 00:18:06,280 --> 00:18:11,080 Speaker 1: used for a very very very long time in UH 309 00:18:11,200 --> 00:18:16,720 Speaker 1: seismological circles. UM. Because if you have a pendulum hanging 310 00:18:16,880 --> 00:18:21,200 Speaker 1: and and it's free of vibration pollution, then um, it's 311 00:18:21,240 --> 00:18:23,719 Speaker 1: just going to hang there until something acts on it 312 00:18:23,840 --> 00:18:27,000 Speaker 1: because of the laws of inertia. Basically, an object at 313 00:18:27,040 --> 00:18:31,080 Speaker 1: rest tends to stay at rest. Um. But there's something 314 00:18:31,119 --> 00:18:33,960 Speaker 1: else too. You also have to have a damper because 315 00:18:34,000 --> 00:18:36,879 Speaker 1: of the laws of inertia, because an object in motion 316 00:18:37,080 --> 00:18:39,600 Speaker 1: tends to stay in motion. So you have to have 317 00:18:39,720 --> 00:18:43,280 Speaker 1: both if you're going to have an accurate UH seismometer, 318 00:18:43,840 --> 00:18:48,679 Speaker 1: because you if once the pendulum starts to move with 319 00:18:48,840 --> 00:18:51,960 Speaker 1: the earth as it starts to shake, it will continue 320 00:18:52,000 --> 00:18:55,199 Speaker 1: to do that. And from from what i've from what 321 00:18:55,280 --> 00:18:59,040 Speaker 1: I understand, you need some kind of dampening material in 322 00:18:59,160 --> 00:19:02,119 Speaker 1: order for it to get an accurate representation of how 323 00:19:02,240 --> 00:19:06,119 Speaker 1: much the Earth is moving, which is kind of funny. 324 00:19:06,119 --> 00:19:08,480 Speaker 1: I wouldn't necessarily have thought about that, but yes, the 325 00:19:08,520 --> 00:19:11,120 Speaker 1: pendulum is just gonna keep swinging and you'll you really 326 00:19:11,160 --> 00:19:13,680 Speaker 1: won't have an idea and it's okay, well, this is it. 327 00:19:13,760 --> 00:19:15,920 Speaker 1: Was it a serious earthquake or was it a very 328 00:19:16,000 --> 00:19:18,800 Speaker 1: very mild earthquake? And you can tell both from the 329 00:19:18,800 --> 00:19:23,199 Speaker 1: pendulum moving and the inertial damper that's that stops it 330 00:19:23,240 --> 00:19:26,679 Speaker 1: from moving as much. Right, Uh. One one way to 331 00:19:26,760 --> 00:19:31,440 Speaker 1: imagine there are a couple of different variations on the 332 00:19:31,480 --> 00:19:34,239 Speaker 1: seize mobter basic design. But one way to imagine it 333 00:19:34,280 --> 00:19:39,280 Speaker 1: is imagine you've got a stand and from the stand 334 00:19:39,400 --> 00:19:43,919 Speaker 1: hangs a very very sense of spring, a very tight spring, 335 00:19:43,920 --> 00:19:45,800 Speaker 1: and there's a weight on the end of that spring, 336 00:19:45,840 --> 00:19:48,160 Speaker 1: so it's above the ground. It's just it's hanging there. 337 00:19:48,880 --> 00:19:51,600 Speaker 1: It's not moving up and down. It's it's at rest. 338 00:19:51,760 --> 00:19:54,159 Speaker 1: It's just the weight is hanging from the spring, not 339 00:19:54,240 --> 00:19:56,960 Speaker 1: moving at all. There is a pen attached to the weight, 340 00:19:58,000 --> 00:20:00,800 Speaker 1: and the pens the top of the pen is or 341 00:20:00,840 --> 00:20:06,639 Speaker 1: the the ink is rested the nib thank you like 342 00:20:06,760 --> 00:20:10,520 Speaker 1: words gone, Jonathan. The ap upset. The nib of the 343 00:20:10,560 --> 00:20:13,879 Speaker 1: pen is resting against a piece of paper that's on 344 00:20:14,080 --> 00:20:17,960 Speaker 1: a spool that's constantly turning giving fresh paper to the pen. 345 00:20:19,840 --> 00:20:23,560 Speaker 1: So when there's an earthquake, if there's up and down motion, 346 00:20:23,600 --> 00:20:27,119 Speaker 1: this is, you know, a vertical seismometer. There are different kinds, 347 00:20:27,160 --> 00:20:33,639 Speaker 1: so the weight tends to stay still. Uh. You're you 348 00:20:33,680 --> 00:20:35,720 Speaker 1: have to step outside the context of the Earth, which 349 00:20:35,760 --> 00:20:37,159 Speaker 1: is kind of weird to say, but you have to 350 00:20:37,200 --> 00:20:40,480 Speaker 1: do it. Like the Earth, the the mass is maintaining 351 00:20:40,520 --> 00:20:43,720 Speaker 1: its space, uh, and then the the everything else is 352 00:20:43,720 --> 00:20:48,560 Speaker 1: moving up and down in relation to the weight. And 353 00:20:48,600 --> 00:20:51,760 Speaker 1: that's the basis for most seismometers. There's also a kind 354 00:20:51,800 --> 00:20:57,199 Speaker 1: where it's similar except the the it's it's a horizontal seismometer, 355 00:20:57,320 --> 00:21:02,680 Speaker 1: in which there's a imagine a stand. Okay, but now 356 00:21:02,720 --> 00:21:07,120 Speaker 1: you've got a long pole that sticks out halfway through 357 00:21:07,160 --> 00:21:12,240 Speaker 1: the stand, right, So it's a horizontal pole that's connected. 358 00:21:12,280 --> 00:21:14,760 Speaker 1: It's got a it's got a hinge on it so 359 00:21:14,800 --> 00:21:17,200 Speaker 1: it can move left and right in relation to the stand. 360 00:21:18,400 --> 00:21:21,919 Speaker 1: And then there's also a spring attached from the top 361 00:21:22,080 --> 00:21:25,760 Speaker 1: of the stand to the the far end of the pole. Right. 362 00:21:25,880 --> 00:21:28,960 Speaker 1: All right, You've got you've got your weight there at 363 00:21:28,960 --> 00:21:30,959 Speaker 1: the far end of the pole. And again you've got 364 00:21:31,000 --> 00:21:34,000 Speaker 1: your pen attached to it. The pen's nib is against 365 00:21:34,000 --> 00:21:37,399 Speaker 1: the paper. Now, when there's an earthquake that does side 366 00:21:37,440 --> 00:21:41,240 Speaker 1: to side motion, the lever can swing to the left 367 00:21:41,240 --> 00:21:43,600 Speaker 1: and to the right. The the spring acts as the 368 00:21:43,680 --> 00:21:47,920 Speaker 1: dampener it amount because it's it's a high tension spring. 369 00:21:48,640 --> 00:21:53,000 Speaker 1: So the weight will move back and forth again again. Really, 370 00:21:53,040 --> 00:21:56,600 Speaker 1: the the paper is moving back and forth against the weight. Uh. 371 00:21:56,680 --> 00:22:01,520 Speaker 1: And that's how you get your readings for horizontal waves. UM. Now, 372 00:22:01,840 --> 00:22:05,400 Speaker 1: a good seismometer actually has will have a three axes 373 00:22:06,280 --> 00:22:10,120 Speaker 1: UH detector on it. Yes, Now, what do you were 374 00:22:10,160 --> 00:22:11,640 Speaker 1: just I'm sorry, go ahead, and I was gonna say 375 00:22:11,640 --> 00:22:14,359 Speaker 1: what you were describing before was the strained seismograph if 376 00:22:14,400 --> 00:22:18,000 Speaker 1: I'm not mistaken. Yes, Um, from from some of the 377 00:22:18,040 --> 00:22:20,639 Speaker 1: research that I had done, I understand that it really 378 00:22:20,680 --> 00:22:25,520 Speaker 1: you really need to measure basically, just for the simplification 379 00:22:25,720 --> 00:22:27,480 Speaker 1: of this and and the fact that we're trying to 380 00:22:27,520 --> 00:22:31,359 Speaker 1: describe it in an UH in an audio track, left 381 00:22:31,400 --> 00:22:34,280 Speaker 1: to right, up and down, so I'm not up and 382 00:22:34,320 --> 00:22:37,600 Speaker 1: down but left and right, north to south. Uh. So 383 00:22:37,640 --> 00:22:40,240 Speaker 1: you have two different directions, and X axis and y 384 00:22:40,320 --> 00:22:43,199 Speaker 1: axis you're measuring those two and then you do have 385 00:22:43,320 --> 00:22:47,800 Speaker 1: a vertical access to UM. And you're you have pendulums 386 00:22:47,800 --> 00:22:50,680 Speaker 1: for each of those three and so really we should 387 00:22:50,680 --> 00:22:52,880 Speaker 1: say instead of left right, we should say north south 388 00:22:52,960 --> 00:22:57,440 Speaker 1: east west. Sorry, yes, that's much better, UM and UM 389 00:22:57,840 --> 00:23:02,440 Speaker 1: And yes, so I totally lost my train of thought. Sorry, 390 00:23:02,480 --> 00:23:04,200 Speaker 1: but yes, you have to have the three axes to 391 00:23:04,240 --> 00:23:07,480 Speaker 1: be able to detect, uh, what kind of earthquake is 392 00:23:07,560 --> 00:23:09,360 Speaker 1: hitting you, like, what kind of waves are moving through 393 00:23:09,359 --> 00:23:13,320 Speaker 1: the ground. Yes, And they have found another way to 394 00:23:13,480 --> 00:23:18,240 Speaker 1: solve the pen on paper UH problem because some optical 395 00:23:18,359 --> 00:23:23,639 Speaker 1: seismographs use mirrors to reflect light onto photosensitive paper has 396 00:23:23,680 --> 00:23:28,240 Speaker 1: mounted on the drum. Now there the drum in in UH. 397 00:23:28,440 --> 00:23:32,639 Speaker 1: Seismographs that use a drum of paper basically have a 398 00:23:33,800 --> 00:23:35,800 Speaker 1: if you think about it as a recording point that 399 00:23:36,000 --> 00:23:40,880 Speaker 1: is gradually moving around the drum. So it starts it. 400 00:23:40,560 --> 00:23:44,000 Speaker 1: It's sort of like a recording drum that you might 401 00:23:44,480 --> 00:23:50,119 Speaker 1: see UM in those early audio recorders or a version 402 00:23:50,200 --> 00:23:52,920 Speaker 1: of the long playing vinyl record. It starts at one 403 00:23:52,960 --> 00:23:56,560 Speaker 1: point and gradually goes in a spiral around as the 404 00:23:56,640 --> 00:24:00,560 Speaker 1: drum goes So it's recording the movement of the as 405 00:24:00,840 --> 00:24:06,040 Speaker 1: time goes on, and the the fact that it is moving. UM. 406 00:24:06,720 --> 00:24:11,919 Speaker 1: And distance to shows you roughly when those uh, those 407 00:24:11,960 --> 00:24:16,400 Speaker 1: seismological waves are taking place. UM, And I think that's 408 00:24:16,440 --> 00:24:20,119 Speaker 1: really that the optical seismograph is an elegant solution to 409 00:24:21,119 --> 00:24:24,400 Speaker 1: the problem. Of course, es since you're using photosensitive paper, 410 00:24:24,440 --> 00:24:26,439 Speaker 1: that means you also have to be recording this in 411 00:24:26,480 --> 00:24:28,639 Speaker 1: the dark. Yeah, there are there are quite a few 412 00:24:29,160 --> 00:24:35,160 Speaker 1: seismic uh seismoscopes and seismommits that no longer use pen 413 00:24:35,280 --> 00:24:39,480 Speaker 1: or paper at all. They're just using various sensors, so 414 00:24:39,560 --> 00:24:41,919 Speaker 1: that I mean, there's some where they have the paper 415 00:24:42,160 --> 00:24:44,600 Speaker 1: counterpart as well to show off to the public whenever 416 00:24:44,600 --> 00:24:46,280 Speaker 1: the public wants to watch it, because it's a lot 417 00:24:46,280 --> 00:24:49,200 Speaker 1: more interesting to see the pen against paper, especially since 418 00:24:49,240 --> 00:24:53,360 Speaker 1: that's such an iconic image for size seismographs. I remember 419 00:24:53,480 --> 00:24:56,639 Speaker 1: seeing the little needle like pens, you know then and 420 00:24:56,760 --> 00:25:01,200 Speaker 1: watching the paper tape scroll through any united is scratching 421 00:25:01,760 --> 00:25:06,400 Speaker 1: seismology and light detectors many so it is a very 422 00:25:06,440 --> 00:25:09,240 Speaker 1: it is there is something very satisfying about seeing that. 423 00:25:09,320 --> 00:25:11,240 Speaker 1: But the truth is is that a lot of the 424 00:25:11,280 --> 00:25:14,960 Speaker 1: modern ones just use sensors. Now, let's talk about um 425 00:25:15,840 --> 00:25:18,800 Speaker 1: identifying where the focus of an earthquake is, because here's 426 00:25:18,840 --> 00:25:23,440 Speaker 1: another thing. You can have the most advanced seismicograph or 427 00:25:23,520 --> 00:25:26,720 Speaker 1: seismometer in the world, and it's not necessarily going to 428 00:25:26,760 --> 00:25:29,440 Speaker 1: tell you where the focus is. What it's gonna tell 429 00:25:29,480 --> 00:25:32,840 Speaker 1: you is how far away the earthquake is, right, and 430 00:25:33,080 --> 00:25:35,560 Speaker 1: we're how far away the focus of the earthquake is right. 431 00:25:35,600 --> 00:25:39,760 Speaker 1: And I think that's um that's sort of a frustrating 432 00:25:39,880 --> 00:25:43,160 Speaker 1: point for geologists because as much as they know, they 433 00:25:43,200 --> 00:25:49,320 Speaker 1: still have difficulty um being pinpoint accurate too. And they're 434 00:25:49,359 --> 00:25:51,919 Speaker 1: they're very good at what they do, but they're very 435 00:25:51,920 --> 00:25:55,840 Speaker 1: good at measuring, yes, But there I think the material 436 00:25:56,320 --> 00:25:59,640 Speaker 1: inside the earth is difficult for them. Makes it makes 437 00:25:59,640 --> 00:26:03,400 Speaker 1: life because when you talk about the epicent of the earthquake, 438 00:26:03,400 --> 00:26:04,800 Speaker 1: you're not saying, well, you know it's down at the 439 00:26:04,800 --> 00:26:07,160 Speaker 1: corner of Fifth and Maine. You also have to figure 440 00:26:07,160 --> 00:26:10,560 Speaker 1: out how deep within the earth it is. And that 441 00:26:10,680 --> 00:26:14,080 Speaker 1: also it's you know, once it gets down to a 442 00:26:14,160 --> 00:26:17,760 Speaker 1: certain point, it's very very it's sort of is a fustcutory. 443 00:26:17,840 --> 00:26:22,320 Speaker 1: You can't really tell as accurately as you would like to. Um. Yeah, 444 00:26:22,359 --> 00:26:24,480 Speaker 1: and then that just that just makes these tools the 445 00:26:24,600 --> 00:26:28,320 Speaker 1: more accurate they become. There's still an element of difficulty, 446 00:26:28,760 --> 00:26:32,119 Speaker 1: and and and to make matters even more difficult. Um, 447 00:26:32,240 --> 00:26:36,960 Speaker 1: the primary waves and secondary waves have different different traits. 448 00:26:37,320 --> 00:26:41,480 Speaker 1: Primary waves can move through anything. They move through solids, liquids, 449 00:26:41,480 --> 00:26:44,880 Speaker 1: and gas. Secondary waves, however, can only move through solids. 450 00:26:45,520 --> 00:26:49,800 Speaker 1: So once they hit the liquid center, the delicious liquid 451 00:26:49,800 --> 00:26:52,320 Speaker 1: center of the Earth, that they don't go any further 452 00:26:52,359 --> 00:26:57,960 Speaker 1: than that. Um. But you know, there are there seismographs 453 00:26:57,960 --> 00:27:01,040 Speaker 1: out there that are sensitive enough to, at least in theory, 454 00:27:01,119 --> 00:27:03,320 Speaker 1: detect an earthquake even if it's happening on the other 455 00:27:03,400 --> 00:27:07,560 Speaker 1: side of the world. So how do earthquake scientists figure 456 00:27:07,560 --> 00:27:11,080 Speaker 1: out where the epicenter of an earthquake is. They have 457 00:27:11,160 --> 00:27:16,480 Speaker 1: to consult multiple seismic graphs, and they they do it 458 00:27:16,560 --> 00:27:19,359 Speaker 1: with three of them. And this is going to be 459 00:27:19,400 --> 00:27:23,080 Speaker 1: familiar to anyone who has done any kind of navigation. UM. 460 00:27:23,200 --> 00:27:25,960 Speaker 1: The reason here is that, like I said before, that 461 00:27:26,080 --> 00:27:28,679 Speaker 1: you measure the difference between the primary wave that the 462 00:27:28,680 --> 00:27:30,840 Speaker 1: time it takes a primary wave and a secondary wave 463 00:27:30,880 --> 00:27:32,760 Speaker 1: to hit you, and that's how you can figure out 464 00:27:33,119 --> 00:27:36,360 Speaker 1: how far away the thing is. Right. Well, that creates 465 00:27:37,160 --> 00:27:41,640 Speaker 1: a sphere, a virtual sphere around the seismic graph. Okay, 466 00:27:41,920 --> 00:27:44,679 Speaker 1: let's say that we know that the epicenter of the 467 00:27:44,720 --> 00:27:49,200 Speaker 1: earthquake is twenty five miles away from our seismic graph, 468 00:27:49,320 --> 00:27:51,600 Speaker 1: So that's twenty five miles in every direction. We we 469 00:27:51,640 --> 00:27:55,080 Speaker 1: don't know the origin of this. Now, of course, you 470 00:27:55,119 --> 00:27:56,680 Speaker 1: can go ahead and say, all right, it's not gonna 471 00:27:56,680 --> 00:28:00,520 Speaker 1: be the sky, but at any rate, can imagine that. 472 00:28:01,640 --> 00:28:04,560 Speaker 1: So you then call up your buddy who's a couple 473 00:28:04,560 --> 00:28:07,240 Speaker 1: of cities away, and say, hey, we just had an earthquake. 474 00:28:07,240 --> 00:28:09,399 Speaker 1: Do you guys have an earthquake registered on there too? 475 00:28:09,400 --> 00:28:12,040 Speaker 1: And he says, yeah, yeah, it's seventy five miles away. Well, 476 00:28:12,080 --> 00:28:15,280 Speaker 1: now you take the intersection of your sphere and their 477 00:28:15,359 --> 00:28:18,800 Speaker 1: sphere at every point where it's you know where where 478 00:28:18,840 --> 00:28:22,320 Speaker 1: those two spheres connect, and say, okay, the epicenter is 479 00:28:22,320 --> 00:28:24,600 Speaker 1: somewhere in here. Then you call up a third well, 480 00:28:24,640 --> 00:28:27,280 Speaker 1: a third person. It's your second buddy. You call up 481 00:28:27,280 --> 00:28:30,160 Speaker 1: your second buddy, he's in another city. He said, hey, 482 00:28:30,240 --> 00:28:32,640 Speaker 1: we have an earthquake. Do you guys notice anything? So, yeah, 483 00:28:32,680 --> 00:28:35,840 Speaker 1: it was thirty miles away. And you take those three uh, 484 00:28:36,000 --> 00:28:38,040 Speaker 1: those those three measurements, and that's going to give you 485 00:28:38,080 --> 00:28:41,000 Speaker 1: a point on the map. It'll actually give you two 486 00:28:41,120 --> 00:28:43,640 Speaker 1: you'll get two connections that it could possibly be, but 487 00:28:43,680 --> 00:28:44,920 Speaker 1: one of them is going to be in the sky, 488 00:28:45,880 --> 00:28:48,240 Speaker 1: and that means you can count that one out. The 489 00:28:48,240 --> 00:28:51,320 Speaker 1: one that's in the earth. That's the epicenter of the 490 00:28:51,320 --> 00:28:56,720 Speaker 1: earthquake's triliteration. Okay, I'll try it. No, no, no no, that's 491 00:28:56,840 --> 00:28:59,840 Speaker 1: t r I. But yeah, it's you know, it's this 492 00:29:00,040 --> 00:29:02,480 Speaker 1: idea of it's something that we've used, like I said, 493 00:29:02,480 --> 00:29:05,600 Speaker 1: in navigation, where you it's like triangulating. It's the same 494 00:29:05,640 --> 00:29:08,920 Speaker 1: sort of principles that you need three points and from 495 00:29:08,920 --> 00:29:11,760 Speaker 1: those three points, once you've made the measurements, you can 496 00:29:11,760 --> 00:29:16,520 Speaker 1: figure out where that epicenter is. Yeah, and that's that's important. 497 00:29:16,560 --> 00:29:21,360 Speaker 1: That's why so many scientists, especially around the uh what 498 00:29:21,520 --> 00:29:24,040 Speaker 1: is known as the Ring of Fire, an area of 499 00:29:24,080 --> 00:29:28,080 Speaker 1: intense geologic activity. They're scientists all over the world who 500 00:29:28,160 --> 00:29:32,959 Speaker 1: have access to this kind of equipment and that's so 501 00:29:33,080 --> 00:29:37,840 Speaker 1: very important to determining um. There are a lot of 502 00:29:37,840 --> 00:29:39,959 Speaker 1: things that that go into this in addition to just 503 00:29:40,040 --> 00:29:43,960 Speaker 1: the earthquake and finding out where the epicenter is. Because 504 00:29:44,280 --> 00:29:47,920 Speaker 1: if you have earthquakes, say off the coast in the 505 00:29:47,920 --> 00:29:53,480 Speaker 1: middle of the ocean, they might produce tsunami and uh, 506 00:29:53,680 --> 00:29:56,800 Speaker 1: knowing roughly where the epicenter is can give you an 507 00:29:56,840 --> 00:30:01,320 Speaker 1: idea of where you might expect to see a tsunami 508 00:30:01,440 --> 00:30:05,520 Speaker 1: and and roughly how long you might have until you 509 00:30:05,560 --> 00:30:11,040 Speaker 1: would expect it on shore. UM. So that's very very important, UM, 510 00:30:11,160 --> 00:30:14,920 Speaker 1: and is really really useful in enable you know, in 511 00:30:15,080 --> 00:30:17,560 Speaker 1: enabling people to do that. UM. And you can use 512 00:30:17,800 --> 00:30:21,360 Speaker 1: you can use a seismological equipment to do all kinds 513 00:30:21,360 --> 00:30:23,920 Speaker 1: of other things too. They use it in patroleum exploration, 514 00:30:24,760 --> 00:30:28,440 Speaker 1: monitoring volcanic activity. Of course, these these two are actually 515 00:30:28,520 --> 00:30:32,520 Speaker 1: very very closely related. UM. That's because sound will move 516 00:30:32,560 --> 00:30:35,480 Speaker 1: at a different speed depending upon the medium it's moving through. 517 00:30:36,200 --> 00:30:39,840 Speaker 1: And by knowing the speeds that sound moves in and 518 00:30:39,880 --> 00:30:43,800 Speaker 1: the various medium or media that it can that you 519 00:30:43,840 --> 00:30:47,640 Speaker 1: could possibly encounter, you can start to narrow down like, oh, 520 00:30:47,800 --> 00:30:51,000 Speaker 1: this is a likely place for oil versus this it 521 00:30:51,080 --> 00:30:53,160 Speaker 1: is unlikely that we would find oil it were we 522 00:30:53,240 --> 00:30:55,880 Speaker 1: to drill here. And we talked about a little bit 523 00:30:55,880 --> 00:30:59,000 Speaker 1: about that in our Auto Tune podcast. Yeah yeah, and 524 00:30:59,040 --> 00:31:03,600 Speaker 1: the oil drilling episode two. UM. So yeah, these are 525 00:31:03,640 --> 00:31:06,920 Speaker 1: these are certainly very important devices and UM, you know, 526 00:31:07,880 --> 00:31:09,520 Speaker 1: can you think of anything else that we need to. Yeah, 527 00:31:09,560 --> 00:31:12,520 Speaker 1: let's let's talk really quickly about the Richter scale. Oh, 528 00:31:12,520 --> 00:31:14,680 Speaker 1: the Richter scale, we haven't even touched on that. So 529 00:31:14,920 --> 00:31:17,480 Speaker 1: Richter scale is you may have heard about the Richter scale, 530 00:31:17,600 --> 00:31:19,920 Speaker 1: about that being a way of measuring the magnitude of 531 00:31:19,960 --> 00:31:23,960 Speaker 1: an earthquake. The Richter scale is a scale in which 532 00:31:24,560 --> 00:31:30,320 Speaker 1: each whole number is uh ten times more powerful. I 533 00:31:30,320 --> 00:31:33,200 Speaker 1: guess you could say or has a magnitude of ten 534 00:31:33,280 --> 00:31:37,440 Speaker 1: times the previous whole number. So a magnitude to earthquake 535 00:31:37,960 --> 00:31:42,320 Speaker 1: has ten times the magnitude of a one earthquake excellent, 536 00:31:42,400 --> 00:31:45,720 Speaker 1: and three would have ten times that the two and um, 537 00:31:45,800 --> 00:31:50,680 Speaker 1: So these numbers get big really quickly. Anything below of 538 00:31:50,760 --> 00:31:53,680 Speaker 1: four is pretty much a minor earthquake, and in fact 539 00:31:53,880 --> 00:31:58,000 Speaker 1: three or lower you're not likely to feel. Anything that's 540 00:31:58,040 --> 00:32:00,400 Speaker 1: a seven or higher is a major earth wake. That's 541 00:32:00,440 --> 00:32:03,080 Speaker 1: that's going to cause lots of damage should it hit 542 00:32:03,120 --> 00:32:08,320 Speaker 1: any populated area. Um and some serious side effects can 543 00:32:08,360 --> 00:32:10,920 Speaker 1: happen to We're talking about things like a fissure opening 544 00:32:11,000 --> 00:32:15,200 Speaker 1: up and magma pouring out, or the tsunami, as Chris 545 00:32:15,240 --> 00:32:18,240 Speaker 1: was mentioned, that could also be a byproduct. Those are 546 00:32:18,320 --> 00:32:19,959 Speaker 1: those are the really bad ones. Anything that's in the 547 00:32:20,000 --> 00:32:22,800 Speaker 1: six to seven range is still bad bad, it's just 548 00:32:22,840 --> 00:32:25,840 Speaker 1: not considered a major earthquake. Now, that's not the only 549 00:32:25,880 --> 00:32:28,360 Speaker 1: scale we used to measure earthquakes, or at least not 550 00:32:28,360 --> 00:32:32,280 Speaker 1: the effects of earthquakes. Do you know of the Marcali scale? No, 551 00:32:32,440 --> 00:32:37,640 Speaker 1: I don't, Okay, So the Richter scale is more it's scientific, right, 552 00:32:37,720 --> 00:32:40,800 Speaker 1: you are actually taking measurements of the earthquake and you're saying, 553 00:32:40,800 --> 00:32:44,280 Speaker 1: based upon this magnitude, this is how powerful this earthquake was. 554 00:32:44,920 --> 00:32:48,200 Speaker 1: So it's a scientific measurement. The Marcali scale is more 555 00:32:48,280 --> 00:32:52,560 Speaker 1: of a subjective measurement. Marcali scale is the scale of 556 00:32:52,760 --> 00:32:59,240 Speaker 1: damage done by an earthquake. Now, for earthquakes where where 557 00:32:59,280 --> 00:33:03,200 Speaker 1: you can feel the earth shaking, but but it's not 558 00:33:03,320 --> 00:33:05,840 Speaker 1: strong enough to actually damage anything. That would be a 559 00:33:05,920 --> 00:33:11,280 Speaker 1: category two on the Mercaulli scale. So one would be 560 00:33:11,320 --> 00:33:14,280 Speaker 1: an earthquake you couldn't even feel. Now it goes up 561 00:33:14,320 --> 00:33:17,360 Speaker 1: to all the way up to twelve. That's a quake 562 00:33:17,400 --> 00:33:21,160 Speaker 1: that's so powerful that's doing major structural damage in the area. 563 00:33:21,360 --> 00:33:23,520 Speaker 1: So let's look, I'm gonna finish up here with one 564 00:33:23,600 --> 00:33:25,960 Speaker 1: other thing that we we talked that I wanted to 565 00:33:25,960 --> 00:33:30,480 Speaker 1: talk about. There was a discussion recently online about the 566 00:33:30,480 --> 00:33:36,280 Speaker 1: possibility that solar flares could somehow induce earthquakes and predict earthquakes. Yes, 567 00:33:36,320 --> 00:33:38,880 Speaker 1: we we had a solar flare not too long ago, 568 00:33:38,960 --> 00:33:41,520 Speaker 1: and then there was the earthquake in christ Church, and 569 00:33:41,600 --> 00:33:45,040 Speaker 1: so some have said that that that the solar flare 570 00:33:45,080 --> 00:33:49,040 Speaker 1: in in effect predicted the earthquake. I'm not so quick 571 00:33:49,080 --> 00:33:52,440 Speaker 1: to jump on this. I've done some research, alcoholic preliminary. 572 00:33:52,720 --> 00:33:55,520 Speaker 1: I've done some preliminary research into this, and I can't 573 00:33:55,600 --> 00:34:01,120 Speaker 1: find any um accepted scientific study that really points to 574 00:34:01,200 --> 00:34:05,120 Speaker 1: a connection. There's some that seemed to say there's some 575 00:34:05,200 --> 00:34:09,560 Speaker 1: sort of uh connection there, but nothing that's actually, you know, 576 00:34:09,719 --> 00:34:12,759 Speaker 1: really like, nothing that that really grabs me and says 577 00:34:12,880 --> 00:34:16,400 Speaker 1: this is this is proof. Most of it seems circumstantial. 578 00:34:16,400 --> 00:34:18,640 Speaker 1: A lot of it has confirmation bias written all over it, 579 00:34:18,640 --> 00:34:21,840 Speaker 1: which is a logical fallacy. And I was trying to 580 00:34:21,840 --> 00:34:24,839 Speaker 1: search around to find because I saw things saying that 581 00:34:24,840 --> 00:34:29,440 Speaker 1: that that the solar flare did in effect predict the 582 00:34:29,520 --> 00:34:32,880 Speaker 1: earthquake in christ Church. One of them, one of the 583 00:34:32,960 --> 00:34:36,799 Speaker 1: sources I found made at error that I just wanted 584 00:34:36,800 --> 00:34:38,239 Speaker 1: to point out. And I'm not saying that this is 585 00:34:38,280 --> 00:34:42,160 Speaker 1: necessarily the the crux of the entire argument, or that 586 00:34:42,239 --> 00:34:45,040 Speaker 1: this is the source. But it was a blog that 587 00:34:45,040 --> 00:34:51,120 Speaker 1: that quoted a NASA UM scientist, and you think, okay, 588 00:34:51,239 --> 00:34:54,160 Speaker 1: NASA people, they know a lot about solar flares. Well, 589 00:34:54,200 --> 00:34:57,960 Speaker 1: the quote was the total energy in a space quake, which, 590 00:34:58,000 --> 00:35:00,960 Speaker 1: by the way, that's what happens when the energy from 591 00:35:00,960 --> 00:35:04,680 Speaker 1: a solar flare and encounters the Earth's magnetosphere. The total 592 00:35:04,760 --> 00:35:08,359 Speaker 1: energy in a spacequake can rival that of a magnitude 593 00:35:08,440 --> 00:35:13,680 Speaker 1: five or six earthquake. Now, the blogger chose to interpret 594 00:35:13,760 --> 00:35:19,480 Speaker 1: this as saying that space quakes cause magnitude five or 595 00:35:19,560 --> 00:35:23,719 Speaker 1: six earthquakes. That's not the case. What the scientist said 596 00:35:23,920 --> 00:35:27,800 Speaker 1: was that the amount of energy is equivalent to an earthquake, 597 00:35:27,880 --> 00:35:31,480 Speaker 1: not that one causes the other. Right, And I made 598 00:35:31,520 --> 00:35:35,799 Speaker 1: a I just made up an analogy that said, if 599 00:35:35,840 --> 00:35:39,920 Speaker 1: we said that a redwood, fully mature redwood falling in 600 00:35:40,000 --> 00:35:42,400 Speaker 1: the forest and hitting the ground had the same amount 601 00:35:42,440 --> 00:35:44,879 Speaker 1: of of energy to it, the same amount of force 602 00:35:44,960 --> 00:35:48,560 Speaker 1: to it that a locomotive moving at seventy five miles 603 00:35:48,640 --> 00:35:51,160 Speaker 1: per hour has, we would not say that a tree 604 00:35:51,239 --> 00:35:53,960 Speaker 1: falling in the forest causes the locomotive to go seventy 605 00:35:54,000 --> 00:35:56,919 Speaker 1: five miles per hour. There's no connection between the two 606 00:35:56,960 --> 00:35:59,400 Speaker 1: other than the fact that the magnitude of the energy 607 00:35:59,520 --> 00:36:02,920 Speaker 1: is the same. Aim. So now I'm not saying that 608 00:36:03,000 --> 00:36:05,680 Speaker 1: there is no connection. I'm saying I can't find any 609 00:36:05,719 --> 00:36:09,640 Speaker 1: scientific study that gives me a very definitive answer, or 610 00:36:09,640 --> 00:36:14,600 Speaker 1: even a semi definitive answer. So but from the geologists 611 00:36:14,600 --> 00:36:18,640 Speaker 1: that I referenced, most of them seem skeptical, saying that 612 00:36:19,000 --> 00:36:24,040 Speaker 1: really earthquakes mostly that mostly are caused by these plate movements, 613 00:36:24,080 --> 00:36:29,520 Speaker 1: which are not affected by magnetic phenomena. Okay, I just 614 00:36:29,520 --> 00:36:34,919 Speaker 1: wanted to head that off a well, let's clarified nicely. Yeah, well, 615 00:36:35,280 --> 00:36:37,200 Speaker 1: I didn't write a blog post this time. At least 616 00:36:37,920 --> 00:36:41,880 Speaker 1: I've been doing that. Jonathan responds to people who have 617 00:36:41,960 --> 00:36:44,160 Speaker 1: no interest in what he has to say. I guess 618 00:36:44,200 --> 00:36:45,879 Speaker 1: that's what blogging is all about, really, when I get 619 00:36:45,880 --> 00:36:49,240 Speaker 1: down to it. Okay, so let's wrap this up, guys. Uh, 620 00:36:49,520 --> 00:36:53,600 Speaker 1: that's our our discussion on seismology and seismological equipment. If 621 00:36:53,600 --> 00:36:56,200 Speaker 1: you have any questions or you want to share some stories, 622 00:36:56,239 --> 00:36:58,920 Speaker 1: if you've been in an earthquake and you got some 623 00:36:58,920 --> 00:37:02,240 Speaker 1: some tales to hell. You can let us know on 624 00:37:02,239 --> 00:37:06,120 Speaker 1: Facebook and Twitter are handled. There is tech Stuff hs W, 625 00:37:06,480 --> 00:37:08,560 Speaker 1: or you can shoot us an email. That address is 626 00:37:08,760 --> 00:37:11,120 Speaker 1: tech stuff at how stuff works dot com and Chris 627 00:37:11,120 --> 00:37:15,160 Speaker 1: and I will taught to you again really soon. For 628 00:37:15,280 --> 00:37:17,640 Speaker 1: more on this and thousands of other topics, visit how 629 00:37:17,680 --> 00:37:20,360 Speaker 1: stuff works dot com. So learn more about the podcast, 630 00:37:20,560 --> 00:37:23,080 Speaker 1: click on the podcast icon in the upper right corner 631 00:37:23,120 --> 00:37:27,240 Speaker 1: of our homepage. The how Stuff Works iPhone app has arrived. 632 00:37:27,360 --> 00:37:34,600 Speaker 1: Download it today on iTunes, brought to you by the 633 00:37:34,640 --> 00:37:38,000 Speaker 1: reinvented two thousand twelve camera. It's ready, are you