1 00:00:00 --> 00:00:04 And, we're going to make a major shift. You're going to feel like 2 00:00:04 --> 00:00:09 this is a whole different class compared to what we were talking 3 00:00:09 --> 00:00:14 about last time, because were jumping from the 4 00:00:14 --> 00:00:19 biogeochemical cycles, or looking at the biosphere as 5 00:00:19 --> 00:00:23 essentially a large biochemical machine, to studying individual 6 00:00:23 --> 00:00:28 populations of organisms, and the communities that they make 7 00:00:28 --> 00:00:33 up when they come together. So, before we were really talking 8 00:00:33 --> 00:00:38 about organisms as they function in the biosphere. 9 00:00:38 --> 00:00:44 Mentally, we're grinding them all up and thinking of them as a 10 00:00:44 --> 00:00:49 collective biochemistry basically. And now we are going to stop 11 00:00:49 --> 00:00:54 grinding them up, mentally, and think of them as 12 00:00:54 --> 00:00:59 individual organisms. So, the next series of lectures, 13 00:00:59 --> 00:01:05 we're going to talk about population ecology. 14 00:01:05 --> 00:01:12 If you remember the first lecture I gave we talked about the hierarchy 15 00:01:12 --> 00:01:19 of organization within ecological systems, and then we are going to 16 00:01:19 --> 00:01:26 talk about competition between organisms with a population, 17 00:01:26 --> 00:01:33 and between organisms of different species, and were going to talk 18 00:01:33 --> 00:01:40 about predation, and mutualism. These are all interactions between 19 00:01:40 --> 00:01:47 organisms that affect the fitness of organisms. And then we'll, 20 00:01:47 --> 00:01:54 at the end, talk about community structure. So this is sort of the 21 00:01:54 --> 00:02:01 outline for the rest of my lectures, not for this lecture. 22 00:02:01 --> 00:02:11 So, today we are going to talk about properties of populations. 23 00:02:11 --> 00:02:22 We're going to analyze how we measure growth rate, 24 00:02:22 --> 00:02:32 growth and death in populations, and this will include populations 25 00:02:32 --> 00:02:43 that have an age structure, and populations that don't. 26 00:02:43 --> 00:02:47 And this is all in preparation for the next lecture where we will talk 27 00:02:47 --> 00:02:52 about human population growth. So, in this field of population 28 00:02:52 --> 00:02:56 ecology, which is as I told you in the first lecture, 29 00:02:56 --> 00:03:01 and some universities you could take three courses in population ecology, 30 00:03:01 --> 00:03:06 and you could get a Ph.D. in population ecology. 31 00:03:06 --> 00:03:11 I mean, this is a whole field that we're going to cover in two lectures. 32 00:03:11 --> 00:03:16 But what population ecologists worry about fundamentally, 33 00:03:16 --> 00:03:21 well, they don't worry about it. This is what they study, is what 34 00:03:21 --> 00:03:27 regulates the density of populations? Obviously, it's a function of how 35 00:03:27 --> 00:03:32 fast they're growing, the birth rate, and how fast they're 36 00:03:32 --> 00:03:37 dying, the death rate. But what are the factors that 37 00:03:37 --> 00:03:41 actually influence those rates? Is it competition with other 38 00:03:41 --> 00:03:45 organisms? Is it the entire structure of the community? 39 00:03:45 --> 00:03:49 Is it the availability of food? Is it the various abiotic 40 00:03:49 --> 00:03:53 properties of the environment: temperature, etc. 41 00:03:53 --> 00:03:57 So, they analyze these and basically try to model the 42 00:03:57 --> 00:04:02 population growth as a function of these various parameters. 43 00:04:02 --> 00:04:06 The other questions they ask, is how are populations distributed 44 00:04:06 --> 00:04:10 in the environment? Are they clustered? 45 00:04:10 --> 00:04:14 Are they evenly distributed? This has specific meanings about 46 00:04:14 --> 00:04:19 their ecology. And, the other thing that people 47 00:04:19 --> 00:04:23 are really fascinated by, which is a really tough question, 48 00:04:23 --> 00:04:27 is why are some species' populations extremely abundant, while 49 00:04:27 --> 00:04:32 others are rare? And one of the discussions we always 50 00:04:32 --> 00:04:36 have in my lab, we work on an organism that's 51 00:04:36 --> 00:04:40 extremely abundant, this prochlorococcus, 52 00:04:40 --> 00:04:44 which I told you briefly about, is the most abundant photosynthetic 53 00:04:44 --> 00:04:49 cell on the planet. So, my students tend to keep saying 54 00:04:49 --> 00:04:53 why is it so successful? And I keep saying, it's successful 55 00:04:53 --> 00:04:57 but there are thousands of other species who are also successful. 56 00:04:57 --> 00:05:02 Abundance does not equal success. Endurance equals success. 57 00:05:02 --> 00:05:07 If you're here in the next generation, you're successful. 58 00:05:07 --> 00:05:13 If you're not, if your species is disappearing, then you're not 59 00:05:13 --> 00:05:19 successful. So, speaking of abundance, 60 00:05:19 --> 00:05:25 let's talk about how we measure abundance, population ecologists. 61 00:05:25 --> 00:05:30 And this is just one example. Obviously, for microorganisms, 62 00:05:30 --> 00:05:35 or some microorganisms it's really easy because they're tiny relative 63 00:05:35 --> 00:05:40 to their habitats. So for the prochlorococcus that we 64 00:05:40 --> 00:05:44 work on, there are 10^5 cells per milliliter. So, 65 00:05:44 --> 00:05:49 we can go take a milliliter of water and measure how many cells there. 66 00:05:49 --> 00:05:54 But for some organisms, larger ones, that are widely distributed, 67 00:05:54 --> 00:05:59 it's not that easy. So, one method is mark and recapture. 68 00:05:59 --> 00:06:04 That's used a lot for things like birds and butterflies. 69 00:06:04 --> 00:06:09 For a bird, the mark would be putting a band on the bird. 70 00:06:09 --> 00:06:14 For a butterfly, they often take a magic marker and put a mark on the 71 00:06:14 --> 00:06:19 wing. Well, that's largely what they do. You try to mark 72 00:06:19 --> 00:06:24 individuals in some way that would not influence their survivorship 73 00:06:24 --> 00:06:29 rate. So, if N equals the population size, 74 00:06:29 --> 00:06:34 that is, that's our unknown, what we're going to do is capture, 75 00:06:34 --> 00:06:39 say, for butterflies or moths, you use a butterfly net, or moths 76 00:06:39 --> 00:06:44 you can use a light to track them; for birds, you put up these big mist 77 00:06:44 --> 00:06:49 nets. They fly into them; they get tangled up a little bit but they 78 00:06:49 --> 00:06:54 don't get hurt. Then you band them, 79 00:06:54 --> 00:06:59 and that we let them go. That's the way you mark them. 80 00:06:59 --> 00:07:07 So, we're going to say n1 equals the total number of marked individuals 81 00:07:07 --> 00:07:15 released. So you capture them, you mark them, you release them. 82 00:07:15 --> 00:07:24 n2 is equal to, and then you go out sometime later and you recapture as 83 00:07:24 --> 00:07:32 many individuals as you can find, and this would be the total number 84 00:07:32 --> 00:07:41 [SIREN] that doesn't sound like a fire drill, does it? 85 00:07:41 --> 00:07:50 I assume we're good to go here. So, n2 is the total number of 86 00:07:50 --> 00:08:00 recaptured. And we're going to say m2 is equal to the numbers 87 00:08:00 --> 00:08:09 recaptured that are marked. OK, and then we assume that the 88 00:08:09 --> 00:08:18 fraction of the recaptured that are marked represent the fraction in the 89 00:08:18 --> 00:08:27 total population that was marked. So, we say m2 over n2 is equal to 90 00:08:27 --> 00:08:34 n1 over N. And the number that we're looking 91 00:08:34 --> 00:08:40 for, population size, is equal to n1, n2 divided by m2. 92 00:08:40 --> 00:08:45 So, of course, this assumes that there's no effect of the marking of 93 00:08:45 --> 00:08:51 the individuals. It assumes that there's no bias in 94 00:08:51 --> 00:08:56 the trapping for the marked or not marked individuals. 95 00:08:56 --> 00:09:02 There's all kinds of assumptions that underlie this. 96 00:09:02 --> 00:09:07 It's a start for assessing the population size. 97 00:09:07 --> 00:09:13 OK, so how do we measure population growth? We're going to first start 98 00:09:13 --> 00:09:19 with looking at populations that have age structure. 99 00:09:19 --> 00:09:25 Now, I hope you printed out the slides that were on the Web, 100 00:09:25 --> 00:09:31 because I'm depending on these overheads a lot for this lecture 101 00:09:31 --> 00:09:37 because we wouldn't get through any of it if I wrote all this 102 00:09:37 --> 00:09:44 stuff on the board. So, we're going to talk about 103 00:09:44 --> 00:09:53 populations that have an age structure. And the data I'm going 104 00:09:53 --> 00:10:03 to show you here is for human populations. 105 00:10:03 --> 00:10:12 But this applies to any population that has differential birth and 106 00:10:12 --> 00:10:21 death rates as a function of the age of the organism, 107 00:10:21 --> 00:10:30 OK? So, in these populations if birth rate and death rate are high, 108 00:10:30 --> 00:10:40 the population is dominated by young people. 109 00:10:40 --> 00:11:00 And, we'll look at this in a minute. And, if B and D are low, 110 00:11:00 --> 00:11:06 dominated by old people, or older I should say, since I now 111 00:11:06 --> 00:11:12 fit into the old category. OK, so here's a typical population 112 00:11:12 --> 00:11:19 age distribution for developed countries, where each slice here, 113 00:11:19 --> 00:11:25 these are females on the right, males on the left, 114 00:11:25 --> 00:11:32 and each slice is an age category: zero to 10 years, 10 to 20. 115 00:11:32 --> 00:11:36 And you can see that in these kinds of populations, 116 00:11:36 --> 00:11:41 you have a fairly even age distribution. Long periods of no 117 00:11:41 --> 00:11:45 net growth in a population lead to this. In these developed countries, 118 00:11:45 --> 00:11:50 and we're going to examine why this is, there's basically an even 119 00:11:50 --> 00:11:55 replacement rate of children for adults. And one of the things we 120 00:11:55 --> 00:11:59 worry about when you see this kind of age distribution, 121 00:11:59 --> 00:12:04 although it's good in terms of population growth, 122 00:12:04 --> 00:12:09 is when you have few young people and a lot of older people, 123 00:12:09 --> 00:12:13 who's going to take care of them, which is what's behind the Social 124 00:12:13 --> 00:12:18 Security crisis. But we won't get into that. 125 00:12:18 --> 00:12:23 Since you're the young people and I'm the old people, 126 00:12:23 --> 00:12:28 I don't want to dwell on that. OK, so what demographers do for 127 00:12:28 --> 00:12:33 human populations is project what the population will look like in the 128 00:12:33 --> 00:12:38 future based on the reproductive rates of the present. 129 00:12:38 --> 00:12:42 And you can see for the US here, it's reasonably stable if you look 130 00:12:42 --> 00:12:47 at these three snapshots. We're going to go backwards 131 00:12:47 --> 00:12:52 starting with 1950, and show you what the population has 132 00:12:52 --> 00:12:57 been doing since 1950. And I'm just going to walk through 133 00:12:57 --> 00:13:02 this. You only have one in your handouts, but I'll show you how it's 134 00:13:02 --> 00:13:07 moving along. Moving along, you can think of this 135 00:13:07 --> 00:13:13 as generations moving through the population. And this is the date up 136 00:13:13 --> 00:13:19 here. So, this is 1950, 1955, you can see this red cohort. 137 00:13:19 --> 00:13:25 A cohort is a group of individuals that were born at roughly the same 138 00:13:25 --> 00:13:31 time. So, you can see that red cohort there. And we are going 139 00:13:31 --> 00:13:37 along, 1965. This lip here, that we can now see, is the postwar 140 00:13:37 --> 00:13:42 baby boom. That's what I'm a member of. 141 00:13:42 --> 00:13:47 If you can see it in this bulge in this population. 142 00:13:47 --> 00:13:53 And now were marching along. Here's my cohort, and I just put 143 00:13:53 --> 00:13:58 these lines on to keep you oriented. And here comes you guys. I think 144 00:13:58 --> 00:14:03 those are you guys, 1985. That's roughly right, 145 00:14:03 --> 00:14:09 because I never know when I've last updated these slides. 146 00:14:09 --> 00:14:14 So, and here you go. See, here's the big bulge of all of 147 00:14:14 --> 00:14:19 these baby boomers that you guys are going to have to take care of. 148 00:14:19 --> 00:14:24 And now, we can actually see an echo. This is what's called the 149 00:14:24 --> 00:14:29 baby boom echo. These are the kids of the baby 150 00:14:29 --> 00:14:34 boomers, which is you guys. But you can only see that as we 151 00:14:34 --> 00:14:40 march through it. So, here we are at 2020. 152 00:14:40 --> 00:14:46 But you get the impression that it's a fairly stable, 153 00:14:46 --> 00:14:52 now, even age distribution in the US and these developed countries. 154 00:14:52 --> 00:14:58 Oops, here we go a little but more. Sorry. 2035, 2045, OK. 155 00:14:58 --> 00:15:03 Now, in less developed countries, the birth rate's high and the death 156 00:15:03 --> 00:15:09 rate's low. We see a much different age distribution. 157 00:15:09 --> 00:15:14 And here's Uganda, with a very high reproductive rate 158 00:15:14 --> 00:15:20 showing the projections to 2050. And here, we can march through from 159 00:15:20 --> 00:15:25 1970. You can see that this huge expansion, do you know what that 160 00:15:25 --> 00:15:31 noise is? OK. Does anybody have a hypothesis for 161 00:15:31 --> 00:15:37 what that noise is that we could test? 162 00:15:37 --> 00:15:40 Oh, OK, I guess we can't do anything about that. OK, 163 00:15:40 --> 00:15:44 so here's Uganda. And you can see the dramatic 164 00:15:44 --> 00:15:48 difference in a population where there is large birthrates, 165 00:15:48 --> 00:15:52 and reducing death rates. And we're going to get into analyzing that in 166 00:15:52 --> 00:15:56 the next lecture. I just want to show you this here 167 00:15:56 --> 00:16:00 so you have a feeling for what we are talking about in age 168 00:16:00 --> 00:16:04 structured populations. So, let's now look at how are going 169 00:16:04 --> 00:16:09 to analyze these populations to try to quantify growth rates or 170 00:16:09 --> 00:16:14 replacement rates. And to do this, we set up life 171 00:16:14 --> 00:16:19 tables. And this is basically what insurance agencies do for human 172 00:16:19 --> 00:16:24 populations. But we do the same thing for populations of ecological 173 00:16:24 --> 00:16:30 interests. We use the same techniques. 174 00:16:30 --> 00:16:34 In this lecture, going to use a unicorn is my example, 175 00:16:34 --> 00:16:39 because I can make up the numbers because they don't exist. 176 00:16:39 --> 00:16:44 But in a textbook there are examples for real organisms like 177 00:16:44 --> 00:16:49 lizards and things like that. OK, so we need to define an age 178 00:16:49 --> 00:16:54 interval, X, and then this is the number of intervals in the original 179 00:16:54 --> 00:16:59 cohort. Again, a cohort is a group of individuals 180 00:16:59 --> 00:17:04 that are born within a defined age interval. 181 00:17:04 --> 00:17:08 I mean, I think of you guys as a cohort. DX is the number dying 182 00:17:08 --> 00:17:13 during that interval. All of this is on the Web. 183 00:17:13 --> 00:17:18 These slides are on the Web. So, you don't need to write it down, 184 00:17:18 --> 00:17:23 but you can. And, NX is that number of individuals 185 00:17:23 --> 00:17:28 surviving to age X. LX is the portion of individuals 186 00:17:28 --> 00:17:33 surviving to age X. So, that's just equal to NX divided 187 00:17:33 --> 00:17:39 by N0. And, we're going to look at a table that shows this in a minute. 188 00:17:39 --> 00:17:45 And MX is something that's measured. It's the per capita 189 00:17:45 --> 00:17:51 births during age interval X to X plus one. And this is also called 190 00:17:51 --> 00:17:57 age-specific fecundity. And you can think of it as the 191 00:17:57 --> 00:18:03 number of female offspring produced per female in a particular 192 00:18:03 --> 00:18:11 age category. OK, is everybody comfortable with 193 00:18:11 --> 00:18:21 that? So, with these definitions, we're going to build a life table 194 00:18:21 --> 00:18:31 that will allow us to actually calculate some things of interest. 195 00:18:31 --> 00:18:37 And, what do we want to calculate? We want to calculate the 196 00:18:37 --> 00:18:50 survivorship probability, 197 00:18:50 --> 00:19:02 LX. We want to calculate the net replacement rate. 198 00:19:02 --> 00:19:10 No it's not really a rate, net replacement of population per 199 00:19:10 --> 00:19:19 generation, which we are calling R0. It's basically the number of 200 00:19:19 --> 00:19:27 children people have to replace who's there per generation. 201 00:19:27 --> 00:19:36 And then, for now, this is what we are going to look at. 202 00:19:36 --> 00:19:48 And to do that, we are going to generate what's 203 00:19:48 --> 00:20:00 called a cohort life table. And to do this, we follow a cohort 204 00:20:00 --> 00:20:11 of individuals throughout lifetime. Or, we can also generate a static 205 00:20:11 --> 00:20:19 life table because it's not that easy sometimes to have a group of 206 00:20:19 --> 00:20:27 organisms that are born at the same time to follow them throughout their 207 00:20:27 --> 00:20:34 entire lifetime. So there is a static life table of 208 00:20:34 --> 00:20:40 taking a snapshot at one time of the population, and calculating the age 209 00:20:40 --> 00:20:47 structure. So, you take a snapshot, 210 00:20:47 --> 00:20:53 and we look at the age structure. And, we are going to do this in a 211 00:20:53 --> 00:21:00 second so it will make more sense. OK, so we've defined our terms. 212 00:21:00 --> 00:21:06 And now, we are going to start by calculating LX. 213 00:21:06 --> 00:21:13 So, this is a cohort life table for unicorns. We're going to start out 214 00:21:13 --> 00:21:19 with a hundred baby unicorns that we have in our imaginary unicorn pen. 215 00:21:19 --> 00:21:26 So, this is a cohort size of 100. And, we find that after a year there 216 00:21:26 --> 00:21:34 are 50 of them left. 50 of them die in the first year. 217 00:21:34 --> 00:21:42 So, the probability here, the proportion surviving is 0. 218 00:21:42 --> 00:21:50 , NX over N0, and then a year later, .4, .3, and then by four years older, 219 00:21:50 --> 00:21:58 no unicorns left. They don't live very long. 220 00:21:58 --> 00:22:06 All right, so this is what's called the survivorship probability, 221 00:22:06 --> 00:22:12 and what we can do is look at there. Different types of organisms have 222 00:22:12 --> 00:22:16 different, what we call, survivorship curves. And this is 223 00:22:16 --> 00:22:20 discussed in your textbook. We'll just describe the extremes. 224 00:22:20 --> 00:22:25 These are just theoretical survivorship curves. 225 00:22:25 --> 00:22:29 But some organisms have a very high probability of survival as a 226 00:22:29 --> 00:22:34 function of age until they reach an old age. 227 00:22:34 --> 00:22:40 And then, they have a very low probability of survival. 228 00:22:40 --> 00:22:46 There are other organisms whose survivorship probability drops very 229 00:22:46 --> 00:22:53 fast, right after they're born. But if they make it through that 230 00:22:53 --> 00:22:59 interval, they're pretty good to go. And then there are some that have a 231 00:22:59 --> 00:23:08 steady probability of dying. So, where are humans, 232 00:23:08 --> 00:23:20 do you think, on this? Two? No, but that's OK. 233 00:23:20 --> 00:23:32 Let me ask you the other way; where our frogs, do you think? 234 00:23:32 --> 00:23:37 Yeah, OK, so you got that image. Tons of frogs' eggs: everybody eats 235 00:23:37 --> 00:23:42 them. Or for that matter, the video I showed towards the end 236 00:23:42 --> 00:23:47 of the last class where there were all those eggs of, 237 00:23:47 --> 00:23:53 what was that? Remember all those eggs that everybody was eating? 238 00:23:53 --> 00:23:58 Herring, thank you. So, any organism that puts out just tons of 239 00:23:58 --> 00:24:03 fertilized eggs, and knowing that most of them will 240 00:24:03 --> 00:24:09 be eaten, but some of them will survive, falls here. 241 00:24:09 --> 00:24:14 And, humans actually fall here. Any organism that has a high 242 00:24:14 --> 00:24:19 investment in the care of offspring, they have few offspring but they 243 00:24:19 --> 00:24:24 invest a lot into the care of those offspring, would fall here. 244 00:24:24 --> 00:24:30 And then this, actually birds and things fall here. 245 00:24:30 --> 00:24:34 So, here's some real but idealized survivorship curves. 246 00:24:34 --> 00:24:38 These are humans. And males and females are different. 247 00:24:38 --> 00:24:42 I'm not sure whether we understand that completely yet. 248 00:24:42 --> 00:24:46 Does anybody know whether that's socially constructed? 249 00:24:46 --> 00:24:51 Now that there's more women experiencing equal stress in the 250 00:24:51 --> 00:24:55 workplace as there are men that will probably even out. 251 00:24:55 --> 00:24:59 But, I think there are more women born, or girl babies. 252 00:24:59 --> 00:25:03 Anyway, there's some interesting biology behind this, 253 00:25:03 --> 00:25:07 but I don't know. I don't remember. 254 00:25:07 --> 00:25:11 And, here's grass, of course grass spew out all these 255 00:25:11 --> 00:25:14 seeds everywhere, and very few of them survive, 256 00:25:14 --> 00:25:18 also these frogs, etc. and birds are commonly like this, 257 00:25:18 --> 00:25:22 where they're somewhere in between. Why do we care so much about 258 00:25:22 --> 00:25:25 survivorship curves? Who cares? Well, I mean they're 259 00:25:25 --> 00:25:29 inherently interesting to population ecologists, but there are 260 00:25:29 --> 00:25:33 also uses for them. For example, if you want to conserve 261 00:25:33 --> 00:25:38 a species, if you're worried about a species going extinct, 262 00:25:38 --> 00:25:44 you want to figure out whether it's better to conserve the young ones or 263 00:25:44 --> 00:25:49 the old ones. For example, turtle species, you would pick a 264 00:25:49 --> 00:25:54 certain age group where the probability of survival is high, 265 00:25:54 --> 00:26:00 and decide to target the conservation of that age group. 266 00:26:00 --> 00:26:05 So, let's continue with, we are building our life table here. 267 00:26:05 --> 00:26:11 So, we have the survivorship probability, but what we really want 268 00:26:11 --> 00:26:17 to get at is understanding whether or not the population that we are 269 00:26:17 --> 00:26:23 describing is replacing itself with each generation. 270 00:26:23 --> 00:26:29 So, maybe we should define, when R0 is equal to one, that meets 271 00:26:29 --> 00:26:35 the population is exactly replacing itself. 272 00:26:35 --> 00:26:45 So, this is replacing, so the actual growth rate of the 273 00:26:45 --> 00:26:55 population would be steady. If R0 is less than one, the number 274 00:26:55 --> 00:27:02 of individuals is declining. And R0 of greater than one, 275 00:27:02 --> 00:27:08 it's increasing. So, we want to know for our unicorns what that is. 276 00:27:08 --> 00:27:14 And to get to that, we have to know something about the birth rates. 277 00:27:14 --> 00:27:20 So, MX is the average offspring per female of age X. 278 00:27:20 --> 00:27:26 So, this is called the age-specific fecundity. And that's something 279 00:27:26 --> 00:27:32 that's a known property of the population. 280 00:27:32 --> 00:27:41 Whoops, oh, my, my, my, my, I'm missing a slide. 281 00:27:41 --> 00:27:50 Oh, there we go. They're out of order. OK, so we have MX. 282 00:27:50 --> 00:28:00 So, how do we calculate R0? Well, R0 is the sum of LX MX. 283 00:28:00 --> 00:28:17 With the sum of the survivorship 284 00:28:17 --> 00:28:25 times the age-specific fecundity, and in this case, it sums up to 285 00:28:25 --> 00:28:33 three. So, what's happening to our unicorn population? It's growing. 286 00:28:33 --> 00:28:39 Yeah, we are getting three unicorns in each generation for every one 287 00:28:39 --> 00:28:46 that existed before. So, in our imaginary unit of our 288 00:28:46 --> 00:28:53 population, we're going to be knee deep in unicorns pretty fast. 289 00:28:53 --> 00:29:00 OK, so I forgot my watch, so I have to look at my computer. 290 00:29:00 --> 00:29:06 What if we can't follow cohort? Oh, thank you. 291 00:29:06 --> 00:29:11 How do we create the same kind of analysis for a population that we 292 00:29:11 --> 00:29:16 can't follow through time, but can only look at as a snapshot? 293 00:29:16 --> 00:29:22 OK, this is where we go to the slide. If you don't have it in your 294 00:29:22 --> 00:29:27 handout, it doesn't matter. I just got off the web this morning. 295 00:29:27 --> 00:29:32 I couldn't find a skeleton of the 296 00:29:32 --> 00:29:37 unicorn because, of course, that's totally imaginary, 297 00:29:37 --> 00:29:42 but I found a mastodon. So, just imagine that this is a unicorn, 298 00:29:42 --> 00:29:47 and I couldn't find a unicorn horn, so this is a sheep's. But, all 299 00:29:47 --> 00:29:52 these principles apply. I just discovered Images in Google, 300 00:29:52 --> 00:29:57 which is really exciting. So, you're going to get subjected 301 00:29:57 --> 00:30:02 to this for awhile. So, OK, so what you can do, 302 00:30:02 --> 00:30:06 and this has actually been done with mountain sheep, 303 00:30:06 --> 00:30:11 is you go out you find dead sheep, you find skeletons of sheep that 304 00:30:11 --> 00:30:15 have died for whatever causes. And you go out, and you sample 305 00:30:15 --> 00:30:19 until you have, say, 100 skeletons. 306 00:30:19 --> 00:30:24 And that's your cohort that you're looking at, at one point in time. 307 00:30:24 --> 00:30:28 And from their horn, you can actually tell how old they 308 00:30:28 --> 00:30:33 were when they died. You can count the number of rings, 309 00:30:33 --> 00:30:38 so that's what's here, annual horn rings. This is for a dall mountain 310 00:30:38 --> 00:30:43 sheep. So, you can say well now it died when it was two. 311 00:30:43 --> 00:30:47 That one died when it was 10. That one died when it was whatever 312 00:30:47 --> 00:30:52 age. And then you can create the same kind of life table, 313 00:30:52 --> 00:30:57 a static life table, where you have a hundred skeletons. 314 00:30:57 --> 00:31:02 That is your cohort. You look at the number dying of age 315 00:31:02 --> 00:31:06 zero to one, the number of one year olds, the number that died when they 316 00:31:06 --> 00:31:11 were one year old, the number that died when they were 317 00:31:11 --> 00:31:16 a two-year-old etc. And so, from these data, 318 00:31:16 --> 00:31:20 these are the data that you collected, you can calculate this 319 00:31:20 --> 00:31:25 column, NX, so NX is DX, or NX minus DX equals NX plus one. 320 00:31:25 --> 00:31:30 Does that make sense? I can never tell whether. 321 00:31:30 --> 00:31:35 I know if I write this on the board it might be easier, 322 00:31:35 --> 00:31:40 but it's so obvious isn't it? We are just saying that this is the 323 00:31:40 --> 00:31:45 number that died at the age. This is the number you started with, 324 00:31:45 --> 00:31:50 so that's how many are going to have that age, that age, 325 00:31:50 --> 00:31:55 and that age. And then, once you have this column, 326 00:31:55 --> 00:32:00 your proportion surviving LX, you can calculate LX. LX equals NX 327 00:32:00 --> 00:32:05 divided by N0, OK? So, we are doing exactly the same 328 00:32:05 --> 00:32:10 thing as we did before. It's just that we're getting the NX 329 00:32:10 --> 00:32:15 column instead of getting it by following the cohort. 330 00:32:15 --> 00:32:20 We're getting it by calculating it based on how old dead organisms were 331 00:32:20 --> 00:32:25 when they died. And in my ecology class that I 332 00:32:25 --> 00:32:30 teach, some years we actually go out to the Mount Auburn Cemetery. 333 00:32:30 --> 00:32:37 And you can do this from human gravestones. You can go to the 334 00:32:37 --> 00:32:44 cemetery, and pick out a number of gravestones, and see the age at 335 00:32:44 --> 00:32:51 which humans died. You create yourself a cohort, 336 00:32:51 --> 00:32:58 and you can create a life table. And you can do that for different 337 00:32:58 --> 00:33:06 eras, and see how replacements have changed. 338 00:33:06 --> 00:33:13 OK, now so that's the analysis for populations that have an age 339 00:33:13 --> 00:33:21 structure. Now we are going to go more into simpler type of population, 340 00:33:21 --> 00:33:29 and that is a population with a stable age distribution. 341 00:33:29 --> 00:33:46 And to do this, 342 00:33:46 --> 00:33:51 you're going to help me, and we're going to use your calculus 343 00:33:51 --> 00:33:55 that you've all been studying. So, instead of the unicorn now, 344 00:33:55 --> 00:34:00 have your imaginary population be a population of microbes 345 00:34:00 --> 00:34:06 that divide in half. They multiplied by dividing in half. 346 00:34:06 --> 00:34:12 So, each one of these is a microbe that's dividing in half. 347 00:34:12 --> 00:34:18 This is your mental image. This is what's called exponential 348 00:34:18 --> 00:34:25 growth. It's obvious how that happens. And we're going to model 349 00:34:25 --> 00:34:31 this population, we're going to first assume 350 00:34:31 --> 00:34:42 unlimited resources. OK, so we're going to say that the 351 00:34:42 --> 00:34:56 rate of population increase is equal to the average birth rate minus the 352 00:34:56 --> 00:35:11 average death rate times the number of cells. 353 00:35:11 --> 00:35:19 OK, so we are going to now turn this into math, and that is to say the 354 00:35:19 --> 00:35:28 dN/dt, the increase in population where N is the population number is 355 00:35:28 --> 00:35:36 equal to the birth rate minus the death rate times N which is the 356 00:35:36 --> 00:35:46 number of cells, OK? And then, we're going to let B minus 357 00:35:46 --> 00:35:58 D, the birth rate minus the death rate, be what we call r. 358 00:35:58 --> 00:36:08 And, this is what's called the intrinsic rate of increase of a 359 00:36:08 --> 00:36:19 population. OK, what are the units of r? 360 00:36:19 --> 00:36:30 One over time, exactly, time to the minus one. 361 00:36:30 --> 00:36:36 So, let's look at that more carefully. And also, 362 00:36:36 --> 00:36:43 it's a little misleading to say it's the rate of increase because r can 363 00:36:43 --> 00:36:49 be positive or negative, however it turns out. It can be 364 00:36:49 --> 00:36:56 positive or negative, but that's what it's called. 365 00:36:56 --> 00:37:02 So, we have the dN/dt equals rN. We're substituting r in this 366 00:37:02 --> 00:37:09 equation for one over N times dN/dt equals r. 367 00:37:09 --> 00:37:15 OK, so ours has the unit time to the minus one. And so, 368 00:37:15 --> 00:37:21 let's ask a question. Given N0 I give you the population 369 00:37:21 --> 00:37:27 density at some time which we're going to call T equals zero. 370 00:37:27 --> 00:37:33 Given a population growing according to this, 371 00:37:33 --> 00:37:39 which is exponential growth, what if we want to know the 372 00:37:39 --> 00:37:45 population, what N is at any time T? 373 00:37:45 --> 00:37:51 We want an equation that will give us, given N0 what would the 374 00:37:51 --> 00:37:57 population density be at some time, T? What do you have to do to this 375 00:37:57 --> 00:38:03 to get that? Yeah, so who wants to do that for me? 376 00:38:03 --> 00:38:10 Come on. You guys did this freshman year. It's the easiest thing there 377 00:38:10 --> 00:38:17 is, right? Every class I've had has had somebody who was willing to come 378 00:38:17 --> 00:38:24 up and do this. OK, so we'll just add a T there. 379 00:38:24 --> 00:38:31 So, N at sometime T is equally to N0 e to the rT. 380 00:38:31 --> 00:38:38 And so, We could say, then, r equals natural log of NT 381 00:38:38 --> 00:38:46 minus natural log of N0 divided by T. And I like to write it that way 382 00:38:46 --> 00:38:53 because then, we know what this looks like, right? 383 00:38:53 --> 00:39:01 Let's plot that. This is N and this is T. What does 384 00:39:01 --> 00:39:08 that look like? I know this is really rudimentary 385 00:39:08 --> 00:39:14 but remember we're modeling population growth. 386 00:39:14 --> 00:39:20 So here, if we plot the log of N, and this is what we do with cultures 387 00:39:20 --> 00:39:26 of microorganisms. That's a flask. Those are a lot of 388 00:39:26 --> 00:39:33 microbes in there. And what we do is we sample it at 389 00:39:33 --> 00:39:39 various points in time, and if you take the log we get a 390 00:39:39 --> 00:39:46 nice straight line that we can draw a regression through. 391 00:39:46 --> 00:39:53 And what's the slope of that line equal to? r. Exactly. 392 00:39:53 --> 00:40:00 The growth rate in the units: N to the minus one. 393 00:40:00 --> 00:40:12 OK, what's the Y intercept? N0. OK, now suppose we want to 394 00:40:12 --> 00:40:25 calculate the doubling time of the population, the time it 395 00:40:25 --> 00:40:37 takes to double. How would we do that? 396 00:40:37 --> 00:40:48 Let's first define it. It's the time, T, that it takes for 397 00:40:48 --> 00:40:59 NT to equal to N0, right? If we start with N0 the 398 00:40:59 --> 00:41:10 population doubles. Then, that's the time at NT. 399 00:41:10 --> 00:41:22 So, we want to solve for that T for the time it takes for the 400 00:41:22 --> 00:41:33 population to double. Since natural log of NT over N0 401 00:41:33 --> 00:41:45 equals rT, then the natural log of, sorry, 2N0 over N0 equals rT, and T 402 00:41:45 --> 00:41:57 equals the natural log of two divided by r equals our 403 00:41:57 --> 00:42:05 doubling time. Does that make sense? 404 00:42:05 --> 00:42:09 I'll put this out there so you can see it better. 405 00:42:09 --> 00:42:14 What's the natural log of two? 0.69, thank you, always a handy 406 00:42:14 --> 00:42:18 thing to have in our repertoire. So, that's just the way, it's 407 00:42:18 --> 00:42:23 easier to think about the time it takes for a population to double 408 00:42:23 --> 00:42:26 often, then the instantaneous growth rate.