Imagine a hypothetical scenario. Imagine you are traveling through space and come across Earth for the first time … what would you be most struck by? Would it be the water that gives our planet the nickname ‘blue-marble’? I doubt it. We’ve now found water on the moon (Saal et al., 2008), on several other planets in our own solar system (Carr et al., 1998; Malin and Edgett, 2000), and a single survey of the Milky Way found>270 planets in the so-called “habitable zone,” warm enough for liquid water (Borucki et al., 2011). Would you instead be struck by the mountains, canyons and other geological features that are most visible from space? Again, it’s doubtful. Geologists tell us there are few, if any, landforms that are wholly unique to Earth (Baker, 2008; Dietrich and Perron, 2006), and you probably would have seen them all before. Based on our current understanding of the universe, the only thing a space-traveler is likely to be struck by, and the one thing that appears to be fundamentally unique to Earth, is its remarkable variety of life.
Ever since the first prokaryotic cells evolved more than 3 billion years ago, the diversity of life on Earth has steadily increased, punctuated by only a handful of extinction events. Our best guess is there are perhaps 9 million forms of eukaryotic organisms on this planet (Mora et al., 2011). The number of prokaryotic organisms is largely unknown, but a single hydrothermal vent on the bottom of the ocean can harbor an astounding 37,000 unique types of microbes (Huber et al., 2007).
While the great variety of life is perhaps the most striking feature of Earth, loss of this biodiversity is one of the most striking forms of environmental change in the Anthopocene. The percentage of species that have gone extinct ranges from < 1% to 13% of described taxa depending on the group considered (Barnosky et al., 2011). But rates of extinction are occurring orders of magnitude faster than what is ‘normal’ in the fossil record. Projections suggest that if these high rates of extinction continue, biodiversity loss could equal or exceed the five prior mass extinctions (loss of 75% or more of known taxa) in 240 to 540 years (Barnosky et al., 2011).
So what? What does it matter if we lose 75% of all life forms on the planet over the next few centuries? Will Earth become any less hospitable for humans? Will this planet still be able provide people with the food, water, air, and other goods and services needed to survive and prosper? Won’t evolution simply replace all of that lost diversity with life forms that are more fit for a human dominated planet? And if evolution does compensate for extinctions in the Anthropocene, what ecological roles will those newly evolved species play?
These are pressing questions as we ponder what future Earth will be like. The variety of life that has evolved over 3.6-billion years is a catalog of biological resources from which we produce nearly all of the goods and services needed for humanity to prosper (Daily et al., 1997; MEA, 2005; Cardinale et al., 2012). If we are to have any hope of predicting how human domination of the planet will impact our own prosperity in an era that will have fewer biological options, we must develop a general theory of Earth’s biodiversity that can predict both the causes as well as the consequences of biological variation.
Fortunately, biologists have made great strides on developing models that simultaneously explain three dimensions of biodiversity: (a) the evolutionary origin of biodiversity, (b) the ecological maintenance of biodiversity, and (c) the ecosystem-level function of biodiversity. Below I describe one set of evolutionary and ecological models that are beginning to show remarkably consistency in form. These models are by no means the only descriptions of how diversity originates, why species coexist, or how diversity influences ecosystem function. But the particular models discussed here do have a common thread that suggests biologists from different sub-disciplines are, in some instances, converging on a suite of equations, all with similar terms that collectively predict the origin, maintenance, and function of biodiversity.
One of Darwin’s most influential ideas was that species originate by the process of natural selection (Darwin, 1859). Though deceivingly simple, it took biologists more than a century to confirm (Coyne and Orr, 2004). One form of natural selection that has now been well documented is ecological speciation (Schluter, 2001). Ecological speciation begins when individuals in a population exhibit variation in their phenotype along an ecological niche axis that corresponds to their use of limiting resources (e.g., space, food, mates) in space or time (Fig. 1A inset, solid red and blue distributions represent individuals that vary in phenotype along a hypothetical niche axis). Examples include Darwin’s finches that vary in beak morphologies that influence the size of seeds they can eat (Grant and Grant, 2006), or body shapes of Stickleback fishes that influence feeding success in the benthic verses pelagic habitat of lakes (Schluter and McPhail, 1992).
When phenotypic variation among individuals occurs along a niche axis with two or more adaptive peaks (Fig. 1A inset, red and blue lines show a ‘fitness landscape’ with adaptive peaks on y-axis), a population can undergo divergent selection, splitting into two populations composed of individuals that each achieve maximal fitness at different values along the niche axis (Schluter, 2001). When divergent selection among individuals becomes sufficiently strong, reproductive isolation can occur, and the population can split into two ecologically distinct species that each use limiting resources (space, food, mates, etc.) differently in space or time.
Models of ecological speciation assume that ecological opportunities lead to niche differences among individuals in a population, and that fitness differences on an adaptive landscape create a selection pressure for individuals to diverge into distinct species. Niche and fitness differences are the same terms now being used by ecologists to explain how species coexist after they evolve. The ecological theory described next suggests that if fitness differences among individuals evolve faster than niche differences, then long-term coexistence of two populations undergoing ecological speciation is not possible (Fig. 1, trajectory to sister taxa A, B). If, however, niche differences evolve faster than fitness differences, coexistence can occur after ecological speciation (Fig. 1, trajectory leading to sister taxa C, D). Thus, the evolutionary trajectory of divergence of niche and fitness differences among individuals determines whether species coexist after reproductive isolation occurs.
Historically, ecologists have assumed that after species evolve, the only thing that can maintain diversity and allow species to coexist is niche differences (Chase and Leibold, 2003). Indeed, common wisdom has long been that evolutionary divergence must cause species to use limiting resources differently in space or time or, if not, competitive exclusion and extinction of the inferior species is inevitable (Gause, 1934). This niche theory of biodiversity was challenged in 2001 when Hubbell (2001) published his Unified Neutral Theory of Biodiversity, arguing that biodiversity is not maintained by niche differences, but rather, by species being so similar to each other that their competitive interactions are ‘neutral’. When interactions are neutral, meaning that competing with an individual of one’s own species has the same consequence as competing with an individual of another species, then species diversity is maintained by a simple balance between speciation rates and random walks to extinction (called ecological ‘drift’ as an analogy to genetic drift).
It has been argued that Neutral Theory is the limiting case of Chesson’s (2000) more general theory of biodiversity (Adler et al., 2007). Chesson showed that most models of species coexistence can be partitioned into two forces that jointly determine whether two species stably coexist. The first force, which Chesson called ‘stabilizing’, represent various forms of traditional niche differences, all of which cause species to limit their own growth rates more strongly than they limit the growth of other species (Fig. 1, x-axis). All niche differences lead to frequency dependent growth such that species have a per capita growth advantage when they are rare in a community. The second force, which Chesson called ‘equalizing’, minimize fitness differences among species (Fig. 1, y-axis). Fitness differences stem from variation in biological traits that would influence the outcome of competition even if species had no niche differences among them (Adler et al., 2007). These traits are the same as those that influence individual reproductive success, such as the per capita population growth rate (Carroll et al., 2011; HilleRisLambers et al., 2012; Narwani et al., 2013).
Chesson showed that for species to stably coexist, niche differences must be larger than fitness differences (Fig. 1, area below 45° line dissecting graph). Thus, if the diverging populations that lead to sister taxa evolve niche differences more rapidly than fitness differences, the ecological species that result should also exhibit long-term, stable coexistence (Fig. 1, trajectories for species C, D and E, F). If, however, diverging populations that lead to sister taxa evolve fitness differences more rapidly than niche differences, the individuals or species that are inferior competitors will go extinct, and diversity will not be maintained over ecological time-frames (Fig. 1, trajectory for species A, B).
Chesson’s theory opens the door for a common set of equations that link concepts in ecological speciation to the ecological maintenance of diversity in competitive communities. Chesson’s theory has also recently been used to show how species coexistence can predict the efficiency of resource use, and production of biomass in communities that control the functioning of ecosystems.
Over the past several decades, there has been a concerted effort to merge concepts in community and ecosystem ecology into common conceptual and theoretical frameworks (Loreau, 2010; Chapin et al., 1997). While community ecology has historically focused on explaining patterns of biodiversity, distributions of populations, and species interactions, ecosystem ecology has focused on explaining the fluxes of energy and the cycles of elements that limit the productivity of life. An increasing number of topics like ‘ecological stoichiometry’ (Sterner and Elser, 2002), ‘ecosystem engineering’ (Jones et al., 1994), ‘trophic cascades’ (Estes et al., 2011) and ‘biodiversity and ecosystem functioning’ (Naeem, 2002), have formed at the intersection of these two fields, emphasizing that the composition and diversity of species in communities not only respond to, but also directly control, fluxes of energy and matter.
A recent sequence of publications have taken theories of species coexistence from community ecology and used these to explain how biodiversity should impact ecosystem-level processes. Tilman et al. (1997) and Loreau (2004) were among first to use traditional models of niche differentiation to show how this force that contributes to coexistence translates mathematically to the sequestration of carbon or nutrients and production of biomass in ecosystems. More recently, Carroll et al. (2011) took a classic model of competition — the MacArthur niche model — and showed how coexistence in this model could be translated into Chesson’s niche differences (ND), and fitness differences (FD). While ND allow diverse communities to capture resources more efficiently and produce more overall biomass, the magnitude of ND required for species to coexist depends on the magnitude of FD that hasten competitive exclusion. As such, the balance of ND and FD that influence competitive coexistence also control the efficiency and productivity of entire communities, with the greatest ecosystem functioning occurring when ND are large relative to FD (Fig. 1, colors from yellow to red indicate increasingly efficient and productive communities).
Use of Chesson’s theory of coexistence to examine how both niche and fitness differences influence ecosystem functioning (Carroll et al., 2011) opens the door for a common set of equations that not only predict the maintenance of biodiversity in ecological time, but also the functional role of biodiversity in controlling the efficiency and productivity of ecosystems.
I have argued that for select modes of evolution (ecological speciation) and certain types of communities (competitive), we are well-within reach of a set of models that simultaneously explain the origin, maintenance, and function of biodiversity. There are, however, still many challenges we face in formalizing these models and extending them to biodiversity more broadly. Therefore, I end with four proposed research foci for the near future:
These four steps are essential short-term goals if we are to predict the causes and consequences of biological change in an era of human domination of the planet. Should we achieve these goals and move closer to a general model of biodiversity, we may yet navigate the Anthropocene in a way that curbs the current tide of extinction, and protects our biological prosperity into the future.
© 2013 Cardinale. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
I thank C. Miller and A. Narwani for comments that improved this article, and the U.S. National Science Foundation’s DIMENSIONS of Biodiversity program for funding (DEB-1046121).
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