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Evolution__3rd_Edition

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656 PART 5 / Macroevolution<br />

Extinction rates could show a<br />

continuous or a two-peaked<br />

distribution<br />

In fact, they look fairly continuous<br />

...<br />

. . . and may fit a power law<br />

Mass extinctions may not have<br />

distinct causes<br />

p per time unit. Then, many time intervals have a small number of species going extinct,<br />

and a few have many species going extinct. (Because if the chance that one goes extinct<br />

is p, the chance that two go extinct is p 2 , the chance that three go extinct is p 3 and so on.)<br />

The different extinction rates observed at different times are simply due to chance effects.<br />

Alternatively, mass extinctions could be a distinct kind of event, with a distinct kind<br />

of cause from extinctions at other times. Then the extinction rates at times of mass<br />

extinction should be unpredictable, and distinct from the extinction rates at other<br />

times. For instance, suppose mass extinctions are caused by large asteroid impacts.<br />

Extinction rates would then occur at a certain rate between large asteroid impacts, and<br />

at a distinct, higher rate during and immediately after an impact. Unlike the random<br />

model, the frequency distribution will not be continuous. Mass extinctions will (or might)<br />

have a distinct peak (Figure 23.6b). When Alvarez’s explanation for the Cretaceous–<br />

Tertiary mass extinction became widely accepted in the early and mid-1980s, some<br />

paleobiologists suggested that there are two macroevolutionary regimes. <strong>Evolution</strong><br />

may alternate between “normal” periods with a “background” extinction rate, and mass<br />

extinctions. Extinctions would have different causes at the two times: asteroids (perhaps)<br />

for the mass extinctions and competition (perhaps) for the periods in between.<br />

The distribution of extinction rates can be used to test between these ideas. Figure<br />

23.6c shows one early study by Raup (1986). The extinction rates appear to fit the random,<br />

Poisson distribution. The rate during the Cretaceous–Tertiary mass extinction may be<br />

an exception, however, being above the curve. The generally good fit to the Poisson distribution<br />

supports the view that variations in extinction rate are mainly random, and<br />

that the history of life does not have two distinct macroevolutionary regimes.<br />

More recently, the frequency distribution of extinction rates has been analyzed<br />

further to see whether it fits a “power law.” A power law here refers to a family of<br />

mathematical equations that describe distributions like those in Figure 23.6. In particular,<br />

paleobiologists are interested in whether the distribution of extinction rates<br />

is “fractal,” showing “self-similarity.” “Self-similarity” and “fractal” are two ways of<br />

saying the same thing. A distribution shows self-similarity if its pattern on a large scale<br />

is an expanded version of its pattern on a small scale, that is the pattern is the same at<br />

all scales. For instance, the frequency distribution of extinction rates between 1 and<br />

10 species per million years will show some pattern. If the pattern for extinction rates<br />

between 10 and 100 species per million years is the same, but multiplied up by a certain<br />

amount, then the whole distribution shows self-similarity.<br />

Solé et al. (1997) performed an analysis of this sort. They found that the distribution<br />

of extinction rates in a large compilation of fossil data appeared to be fractal a to show<br />

self-similarity. Extinction rate data are noisy, however, because of the many sources of<br />

error in the data. Tests of this sort are not all that strong.<br />

If the distribution of extinction rates does show self-similarity, it is tempting to take<br />

the reasoning a step further. If extinction rates are fractal, the differences in extinction<br />

rates between different times are random and unpredictable. It would then be a mistake<br />

to ask what the “cause” or even “causes” of mass extinctions is, or are. Mass extinctions<br />

may not have a different cause from the periods when extinction rates are lower.<br />

Consider, for instance, a simple model of extinctions that gives rise to fractal extinction<br />

rates. The species in an ecosystem have a certain degree of interdependence.<br />

Predators depend on prey; herbivores depend on food plants. If a food plant goes<br />

..

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