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February 26 - March 12, 2018
Bergmann’s Rule, named for the nineteenth-century German biologist who described it, refers to the tendency for size to increase with latitude among individuals within a species or among closely related species.
Natural selection has no foresight—it won’t favor a detrimental feature just because it is an early step on a path leading to an ultimately superior condition. Rather, for a feature to evolve by natural selection, every step along the way must be an improvement on what came before it—natural selection will never favor a worse condition, even if it’s only a transient evolutionary phase.
The prevalence of convergence among closely related populations and species is easy to understand. Close relatives tend to be similar genetically, so selection is likely to have the same genetic systems on which to work. Moreover, relatives tend to be similar in many phenotypic attributes. Because of these similarities, closely related species and populations share the same evolutionary predispositions, more likely to evolve in some ways than in others. Some evolutionary biologists refer to these predispositions as constraints or evolutionary biases. These biases could operate in a number of
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“Against this backdrop of parallelism, or repeatability, the longer the LTEE has been running, the more we see that each population really is following its own path,” he said, “and both sets of forces—the random and the predictable, as it were—together give rise to what we call history.”
So, can we predict evolution? In the short-term, yes, to some extent. But the longer the passage of time and the more different the ancestors or conditions, the less likely we are to prognosticate successfully. Dinosauroid? I don’t think so. Perry the Platypusoid? Alas, no. Were we destined to be here? Hardly.

