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Evolution__3rd_Edition

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676 PART 5 / Macroevolution<br />

. . . or some other model<br />

The data to test the models is<br />

currently ambiguous ...<br />

. . . and subject to active statistical<br />

analysis<br />

diversity, as the logistic model assumes, then that limit has not yet been reached. 2<br />

Secondly, mass extinctions have been less important for the history of diversity. Diversity<br />

now would be much the same if no mass extinctions had occurred. Other models<br />

beside those by Sepkoski and Benton have also been proposed (see Miller 1998).<br />

Which model is correct? The question has been difficult to answer, because of limitations<br />

in the data. Even Sepkoski’s compilation has gaps and biases. Jackson & Johnson<br />

(2001), for instance, investigated Sepkoski’s data for tropical Bryozoa. They found a<br />

huge underestimate of the diversity of this regional taxon for the Pliocene. The reason<br />

was simply that Europe and North America were no longer tropical in the Pliocene.<br />

Most paleontologists are European or North American, and most of them work locally.<br />

Thus, the high diversity of tropical bryozoan fauna has been much better studied for<br />

earlier times, when Europe and North America were tropical, than for the Pliocene,<br />

when they were temperate. If Sepkoski’s data are adjusted for this bias, Jackson and<br />

Johnson suggest it fits better with the exponential model. However, the main point is<br />

that we need a database that has been more systematically corrected for bias. The two<br />

main kinds of bias come from the amount of rock preserved from different time intervals,<br />

and the amount of that preserved rock that has been studied by paleontologists.<br />

Geographic and taxonomic biases (as paleontologists study some regions, and some<br />

taxa, more than others) interact with these two main kinds of bias.<br />

A new database is being compiled by a team of paleobiologists, and is being housed at<br />

the University of California at Santa Barbara. The new database aims to correct for<br />

biases, by appropriate statistical corrections to the raw data. The preliminary results are<br />

remarkable (Figure 23.15c). The estimated global species diversity seems to show little<br />

change from the Paleozoic to the Oligocene. If the result holds up as the database is<br />

developed, it will suggest that diversity has a tighter limit than had previously been<br />

suspected. Speciation and extinction may have been in balance for much of the past<br />

500 million years, with mass extinctions having had little effect on global species<br />

diversity. That such a dramatically different picture can be produced now highlights<br />

the importance of statistical corrections to the data. The main difference between<br />

Figure 23.15a and 23.15c is due to the statistical corrections for bias.<br />

In summary, we have seen how there is an active research program that aims to<br />

describe the history of global species diversity. The main problems lie in data compilation,<br />

and correction for biases and gaps. Paleobiologists can be found who support at<br />

least three models of history: a logistic increase to a Paleozoic plateau, followed by a<br />

steady increase; steady exponential increase; and a prolonged plateau. The influence<br />

of mass extinctions on diversity is uncertain. It is also uncertain whether modern life<br />

subdivides ecological niches more finely than earlier life did. These uncertainties exist<br />

not because the problems have been forgotten about, but because of a multipronged<br />

modern attack by research paleobiologists.<br />

2 Ultimately, species diversity will be limited, among sexual creatures, by the time it takes to find a mate.<br />

As species split and split, the numbers of individuals per species will go down (because the total biomass on<br />

Earth is limited by the energy input from the sun). As the members of a species become rarer, and sparser, the<br />

energetic cost of finding a mate will ultimately become prohibitive. Hybridization, despite its genetic costs<br />

(Section 14.4, p. 389) will eventually be favored.<br />

..

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