Using Microbial Microcosms to Study Host–parasite Coevolution
© Springer Science+Business Media, LLC 2009
Published: 10 November 2009
Microbial microcosm experiments with bacteria and their viral parasites allow us to observe host–parasite coevolution in action. Laboratory populations of microbes evolve rapidly, thanks to their short generation times and huge population sizes. By taking advantage of a “living fossil record” stored in the laboratory freezer, we can directly compare the fitness of hosts and parasites with their actual evolutionary ancestors. Such experiments demonstrate that host–parasite coevolution is an important evolutionary force and a cause of strong and divergent natural selection.
KeywordsMicrocosm experiments Host–parasite coevolution Experimental evolution
One of the insights of Red Queen thinking was that host–parasite coevolution should drive very rapid evolution, so rapid in fact that biologists could expect to observe it occurring now. There is just one small problem with studying coevolution in nature: to really understand the nitty-gritty requires time travel! This is because the ideal experiment uses a “time-shift” such that host and parasite genotypes from the present day can be confronted with parasite or host genotypes from the past and future (Gandon et al. 2008; Gaba and Ebert 2009). Such time-shift experiments allow experimenters to make direct measurements of how both the infectivity of parasites and the resistance of hosts evolve through time. One solution to the time travel dilemma is to use laboratory populations of microbes which can be cryogenically stored in a freezer; these stored populations remain viable in suspended animation and form a “living fossil record” of evolutionary ancestors waiting to be defrosted at a later date (Buckling and Rainey 2002a; Brockhurst et al. 2003). A further advantage of using laboratory populations of microbes is their short generation times and large population sizes, which favor very rapid evolution that is observable over the course of a few days (Elena and Lenski 2003; Jessup et al. 2004; Buckling et al. 2009). In this article, I discuss how evolutionary biologists have used laboratory populations of microbes to study host–parasite coevolution.
Microcosms: The World in a Test Tube
As you would expect in the world of the Red Queen, bacteria do not sit idly by while phages decimate them but, rather, have evolved an array of sophisticated defense mechanisms. These range from genetic mutations that change their surface molecules, thereby preventing phage attachment to internal mechanisms blocking phage replication and apoptotic cell-death postinfection to prevent further spread of the phages to neighboring cells (Allison and Klaenhammer 1998). Fortunately, it is easy to keep populations of bacteria and phages in the laboratory to study their coevolutionary arms-race in detail: all you need are test tubes containing liquid growth medium, an incubator, and a freezer to store the living fossil record. Each replicate population can be founded with genetically identical individuals (both bacteria and phages reproduce asexually, producing clones of themselves); but with millions of individuals per milliliter and genetic mutations arising from errors in the copying of DNA from generation to generation, natural selection soon has plenty to work with and evolutionary change in both species can be observed over the course of a few days!
Fluctuation or Escalation?
Two main models of host–parasite coevolution have been proposed, each corresponding to patterns seen in different host–parasite interactions in nature (Woolhouse et al. 2002). One proposes that host and parasite populations cycle through different resistance and infectivity genotypes through time, but that each genotype is a specialist only capable of resisting or infecting one genotype of the other species. The other proposes that new infectivity and resistance genotypes sweep through the population; repeated selective sweeps lead to the evolution of generalist hosts and parasites, which can resist or infect a progressively wider range of genotypes. The first model predicts genotype frequencies to fluctuate through time but for resistance and infectivity ranges to remain constant; whereas the second model predicts repeated fixation of new genotypes and escalation of resistance and infectivity ranges (Woolhouse et al. 2002).
Coevolution in Space
One of the most significant recent developments in our understanding of host–parasite coevolution in nature is the realization that coevolutionary interactions are often played out over large geographic scales. The importance of space in the coevolutionary process is captured in the Geographic Mosaic Theory (Thompson 2005). This comprises three components: (a) selection mosaics, which arise from each different population patch wandering off on its own coevolutionary trajectory; (b) coevolutionary hotspots and coldspots, such that the strength of selection arising from coevolution often varies between population patches; and (c) gene-flow, where dispersal of individuals can lead to mixing of the gene pools from different population patches. To test for differences in the trajectory of coevolution among populations, we need not a time-shift, but a “space-shift” experiment where bacteria are confronted with phages from other populations at the same time step. If we do this with our coevolving laboratory populations, we see that bacteria are more resistant to phages from the same population than to phages from other populations (Buckling and Rainey 2002a; Morgan et al. 2005). This suggests that each population is indeed following its own slightly different coevolutionary trajectory, thereby creating selection mosaics.
It is surprisingly easy to alter the strength of coevolutionary selection to generate relative coevolutionary hotspots and coldspots in our laboratory populations. One way to do this is to increase the amount of nutrients in the growth medium, which effectively lowers the cost for bacteria of investing some of their resources in antiphage defenses (Lopez-Pascua and Buckling 2008). This change allows bacteria to more readily evolve resistance, which in turn imposes selection for novel infectivity genotypes in the phage, thus spurring on the rate of coevolution. Another way is to periodically shake the test tubes while they are being incubated. This has the effect of increasing the frequency with which bacteria and phage encounter one another; if bacteria encounter infectious phage more often, this increases natural selection for resistance, which in turn increases selection for novel infectivity in the phage, thereby accelerating coevolution (Brockhurst et al. 2003).
So what effect does dispersal (and therefore, gene flow) between different test tube populations have on coevolution between bacteria and phage? In general, dispersal between test tubes accelerates coevolution but only up to a point (Morgan et al. 2007; Vogwill et al. 2008). The reason for this relates to Fisher’s Fundamental Theorem of Natural Selection: “The rate of increase in fitness of any organism at any time is equal to its genetic variance in fitness at that time” (Fisher 1930). Dispersal between populations on divergent coevolutionary trajectories increases the genetic diversity within populations upon which natural selection can act, thereby increasing the rate of evolution in both bacteria and phage (Morgan et al. 2007; Vogwill et al. 2008). However, dispersal is a double-edged sword because too much can homogenize genetic variation across all populations, reducing the benefits of dispersal, and causing the rate of coevolution to drop off at very high levels of dispersal (Vogwill et al. 2008). An interesting experimental twist is to allow moderate dispersal between relative coevolutionary hotspots and coldspots. When this occurs, we observe a pacemaker effect overriding local ecological conditions, such that dispersal from hotter spots to colder spots speeds up coevolution in the colder spot, whereas dispersal from colder spots to hotter spots slows down coevolution in the hotter spot (Vogwill et al. 2009).
Escape and Radiate Coevolution
Coevolution with parasites can also affect the evolution of other ecologically important traits in hosts. One interesting possibility is that evolutionary escape from parasite attack could open up a range of previously inaccessible ecological opportunities, thereby allowing diversification of the host so-called “escape and radiate coevolution” (Ehrlich and Raven 1964). In the absence of phage, P. fluorescens diversifies in laboratory test tubes into three types distinguishable by their heritable colony morphologies on agar plates and their niche preferences within the liquid medium (Rainey and Travisano 1998). Wrinkly spreaders live at the air–liquid interface, smooths live in the liquid broth, and fuzzy spreaders inhabit the murky depths at the bottom of the test tube. These types are each specialists in their preferred niche, and all three can stably coexist within the same population. When phages are added to populations of P. fluorescens, they prevent the diversification of the bacteria by reducing bacterial abundance and weakening resource competition (Buckling and Rainey 2002b). However, once bacteria evolve high levels of resistance, they are able to “escape and radiate” into the three colony types to take advantage of the ecological opportunities available in the test tube. The bacteria’s success is short-lived, however, and phages rapidly evolve to overcome bacterial resistance, thereby reducing bacterial colony type diversity once more (Buckling and Hodgson 2007).
The coevolutionary interactions between bacteria and phage exhibit much of the complexities and nuances anticipated from theory. The hypotheses investigated experimentally in microcosms are of broad relevance to our understanding of host–parasite interactions in general, yet have proved difficult to test in natural populations. Microbial microcosms, therefore, provide an opportunity to observe coevolution in action and serve as an essential stepping stone between theory and the natural world.
I am grateful to John Thompson and one anonymous reviewer for helpful comments on the manuscript.
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