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Evolution__3rd_Edition

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..<br />

Several models could explain why<br />

extinction rates fit a power law ...<br />

. . . but the facts remain uncertain<br />

CHAPTER 23 / Extinction and Radiation 657<br />

extinct, the herbivores that depend on it will go extinct too, and then the predators that<br />

depend on the herbivore. Thus if one species in an ecologically connected web of<br />

species goes extinct, it will take out a number of other species too. The number taken<br />

out depends on the number of interdependent species.<br />

Over time, the degree of interconnectivity in an ecosystem may change. Sometimes<br />

many species depend on one another. At other times, ecological relations are more diffuse<br />

and few species strongly depend on one another. If one species accidentally goes<br />

extinct at a time of strong, extensive interconnectedness, many species will follow it to<br />

extinction. If one species accidentally goes extinct at a time of weak interconnectedness,<br />

few species will follow it. The same initial cause (the accidental loss of one species) can<br />

trigger a range of extinction rates, depending on the state of the ecosystem.<br />

For this model to produce a fractal pattern of extinction rates, we would need<br />

to assume that the degree of interconnectedness in ecosystems evolves more or less at<br />

random, wandering up and down over time. Then if accidents happen at a steady rate,<br />

the resulting frequency distribution of extinction rates would be fractal in the way<br />

that appears to be observed.<br />

The “ecosystem connectedness” model is not the only one that could explain the<br />

(tentative) observations. Another simple model could propose that almost all extinctions<br />

are caused by asteroid impacts. Asteroids vary in size, and small asteroid impacts<br />

probably cause fewer extinctions than large asteroid impacts. Then if the size distribution<br />

of asteroids fits a power law, the frequency distribution of the resulting extinctions<br />

will also fit a power law. 1<br />

More realistically, various causes of extinction such as asteroids and volcanic eruptions<br />

may interact with the condition of the ecosystem to determine the extinction rate.<br />

A more complex model could be produced. However, the point of the models here is<br />

to show that various factors could explain the observations. What the processes have<br />

in common is that they do not posit a distinct set of causes for mass extinctions as<br />

opposed to extinctions at other times. If extinction rates do fit a power law, we are led to<br />

think of causes for extinction rates that operate in much the same way over time.<br />

However, not all paleobiologists are agreed that extinction rates do fit a power law.<br />

There could be life yet in the search for a distinct set of causes for mass extinctions. This<br />

area of research, like several others in this chapter, will progress along with the quality<br />

of the fossil databases.<br />

23.5 Changes in the quality of the sedimentary record<br />

through time are associated with changes in the<br />

observed extinction rate<br />

So far we have treated changes in extinction rates, and particularly the high extinction<br />

rates at times of mass extinction, as real. Factors such as asteroid impacts and<br />

1 In the next section we look at the possibility that fluctuations in the sedimentary record may explain<br />

changes in the observed extinction rate. If the processes determining sedimentation rates are fractal, this factor<br />

too could produce extinction rates that fit a power law.

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