Abstract
The activation-polymerization-epimerization-depolymerization (APED) model of Plasson et al. has recently been proposed as a mechanism for the evolution of homochirality on prebiotic Earth. The dynamics of the APED model in two-dimensional spatially-extended systems is investigated for various realistic reaction parameters. It is found that the APED system allows for the formation of isolated homochiral proto-domains surrounded by a racemate. A diffusive slowdown of the APED network induced, for example, through tidal motion or evaporating pools and lagoons leads to the stabilization of homochiral bounded structures as expected in the first self-assembled protocells.
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Introduction
While much progress has been made in understanding the many aspects related to the origin of terrestrial life, a coherent framework of events leading up to first life is still beyond reach. Current theories of the origin of life typically address one of its aspects. For example, investigations may focus on prebiotic chemistry as in the Miller experiment (Miller 1955) and related follow-up studies (Rode 1999) or on the formation of the first cellular membranes as in the work of Deamer and collaborators (Deamer et al. 2002; Morowitz et al. 1988). Here we attempt to combine a recent scenario for the onset of homochirality in peptide systems with models describing the formation of localized cell-like proto-domains in an effort to synthesize some of the ideas presented in the literature into a cohesive framework.
A critical step in the emergence of life was the advent of cellular membranes. Membranous boundaries are a key component of all modern cells and are required for processes such as speciation, energy capture, and metabolic catalytic reactions (Monnard and Deamer 2002). “Minimum protocells”—membrane vesicles capable of self-replication—have been proposed by Morowitz et al. as a possible first step toward functioning cells fitted for self-replication and Darwinian evolution (Morowitz et al. 1988). The appeal of this membrane-first, lipid-world scenario is the ability of such boundary structures to thermodynamically separate their contents from the external environment: the interior of the membrane provides a closed microenvironment for chemical reactions while the exterior environment provides free energy and nutrients (Morowitz et al. 1988). This view is supported by numerous studies focusing on the formation of lipid membrane-vesicles from prebiotically relevant ingredients: vesicle formation has been demonstrated for a variety of amphiphilic compounds (Deamer 2002; Deamer and Dworkin 2005; Monnard and Deamer 2002, Lonchin et al. 1999; Berclaz et al. 2001a, b including formation of boundary structures from organic molecules found in the Murchison meteorite (Deamer 1985).
In contrast to the perspective provided by proponents of the lipid-world scenario (Segrè et al. 2002), self-organization of short peptides has recently been proposed as a possible alternative to lipid self-organization for formation of the first protocellular membrane structures (Fishkis 2007; Santoso et al. 2002). Although phospholipids are the primary components of modern cellular membranes, it is unlikely that such compounds were prevalent enough on the early Earth to be major components of the very first membranes (Deamer et al. 2002; Lazcano and Miller 1996). As pointed out by Fishkis (2007), the first cellular membranes may have consisted of polypeptides, possibly in conjunction with other prebiotic amphiphilic molecules. This idea is supported by findings indicating that short peptides can aggregate into fibrils, microtubes, and vesicles (Reches and Gazit 2004, 2006; Santoso et al. 2002; Vauthey et al 2002).
The notion of a “peptide-first” origin of life where polypeptides self-organize into protocellular structures is not new. Earlier work by Fox and coworkers (Fox 1973, 1980) addressed the formation of proteinoid microspheres from self-organizing amino acids. It was found that heated amino acids can self-order in copolymerization reactions and self-organize when in contact with water to form protocells (also referred to as minimal or pre-contemporary cells (Fox 1973)). These protocells can feature many of the properties common to life: metabolism, growth, reproduction and response to stimuli in the environment (Fox et al. 1995). They are also capable of evolving to more modern cells—including the initiation of a nucleic acid coding system (Fox et al. 1995). However, the polypeptides in these studies are composed of mixed L- and D-amino acids with no mention of how a microsphere might evolve toward a homochiral contemporary cell with exclusively L-amino acids (Fox 1973).
Apart from studies of the origins of the first cellular boundaries, the origin of life’s chiral signature, i.e. dextrorotatory sugars and levorotatory amino acids, has been a longstanding question in studies of abiogenesis (Bonner 1996). The first breakthrough in understanding biomolecular chiral symmetry-breaking occurred with the influential work of Frank (1953), where autocatalysis and some form of mutual antagonism were identified as sufficient ingredients for obtaining molecular homochirality. Since then, many “Frank models” have been proposed, each providing its own description of chiral symmetry breaking. These models range from the early work on bifurcation models by Kondepudi and Nelson (1983) and Avetisov and Goldanskii (1993) to more recent investigations of crystallization (Saito and Hyuga 2005; Viedma 2005), and chiral selection in polymerization (Sandars 2003; Saito and Hyuga 2005). One of the better known models is that of Sandars (2003; Brandenburg and Multamäki (2004; Wattis and Coveney (2005; Gleiser and Walker (2008), where the mutual antagonism is provided by enantiomeric cross-inhibition in template-directed polycondensation of polynucleotides (Joyce et al. 1984). Although this model provides a theoretically elegant description of how homochirality might emerge in a RNA world, the autocatalytic reactions necessary for chiral symmetry breaking to be observed in such a system are presently only demonstrated for a few non-biological molecules (Blackmond 2004; Soai et al. 1995) and would be trying to achieve with even very simple organic molecules (Joyce 1991).
A more recent proposal, describing the emergence of homochirality in an early peptide world has been provided by Plasson et al. (2004). A prebiotically relevant reaction network consisting of activation, polymerization, epimerization, and depolymerization (APED) of chiral peptides was shown to allow self-conversion of all chiral subunits to a single handedness. As discussed by Plasson et al., and later by Brandenburg et al. (2007), the APED model is distinct from the class of Frank models in that symmetry breaking in APED mimics autocatalysis without any of the molecules actually possessing catalytic behavior. The APED system therefore represents what may be the first in a class of models which are not dependent on autocatalysis—a beneficial feature given that direct autocatalysis is not believed to be possible with short nucleotides or short peptides (Brandenburg et al. 2007).
Another attractive feature of the APED model is that it describes a mass-conserving, closed, recycled system of reversible chemical reactions allowing complete conversion of all chiral subunits to a single chirality: in other words, with continual input of energy, the APED system provides a description of emergent chirality, where one may begin with a closed near-racemic system of left and right-handed deactivated monomers and end with a nearly homochiral system of monomers and dimers. It is this feature that makes the model appealing—it provides a bottom-up approach to the onset of homochirality.
A bottom-up approach to the origins of life, based on increased complexification from primordial prebiotic precursors (Frank 1953; Miller 1955; Lazcano and Miller 1996; Avetisov and Goldanskii 1993; Sandars 2003; Brandenburg and Multamäki 2004; Gleiser and Walker 2008; Rode 1999) is usually contrasted with top-down methods aimed at reducing cells to the minimal ingredients necessary to still be deemed living (Rasmussen et al. 2004; Szostak et al. 2001). Although there is no doubt that both approaches are fundamentally sound and worth pursuing, very little work has been done in trying to bridge the gap between the two, that is, in trying to go from chemistry to biology. Our goal in the present manuscript is to take the first steps in this direction, by providing a workable closed chemical model which evolves dynamically through its own self-interactions towards precursors of cell-like homochiral structures surrounded by a racemic environment. By “cell-like” we mean spatially-bounded structures with contents differentiated from the exterior and with a hint of proto-metabolic activity. We do not attempt here to model full cell-like behavior, including transmembrane ionic transport activity and division with transmission of genetic information. Our goal is to provide the possible first steps toward more complex and realistic cell-like behavior including homochiral biochemistry.
For this end, we will introduce spatial dynamics to the APED model and obtain the reaction rates allowing for the emergence of localized homochiral domains. We will see that both tube-like and spherical domains are possible, depending on the details of the dynamics. We begin our discussion with a description of some of the key features of the APED model in the section “The Model”. We then introduce spatial dynamics and discuss our findings in the “Results” section. In the “Discussion” we make contact with proto-cellular abiogenesis in light of the work by Fox and colleagues (Fox 1973, 1980; Fox et al. 1995) and by Fishkis (2007), highlighting peptides as a potentially crucial ingredient in the first protocells. We also briefly discuss the consequences of our work to future searches of extraterrestrial stereochemistry.
The Model
The polymerization reactions in the original work of Plasson et al. were limited to dimerizations (Plasson et al. 2004): a relevant truncation given that dipeptides have been identified in the Murchison meteorite (Meierhenrich et al. 2004). We follow this simplification here, since solving the coupled network of reaction equations becomes quite complex when spatial dynamics are included. The set of APED reactions limited to dimerizations is:
supplemented by the complementary reactions with \(L \leftrightarrow D\). By convention (Plasson et al. 2004), the reacting amino acid is on the left side of a polymer chain. Here a and b are the activation and deactivation rates of monomers, respectively. The rates p and h describe the respective rates of polymerization and depolymerization of homochiral dimers, while e describes the rate of epimerization of heterochiral dimers. The rates αp, βh, and γe then correspond to the complementary stereospecific reactions rates for polymerization and depolymerization of heterochiral dimers and epimerization of homochiral dimers, respectively, where α, β, and γ quantify the degree of stereoselectivity. An important feature of the model is that the system is closed with respect to mass flux and maintains a constant total concentration of amino acids and peptides,
Successful symmetry breaking in APED systems requires stereospecific reactions, i.e., α, β, γ ≠ 1. Studying the case of complete stereoselectivity for depolymerization and epimerization reactions (β = γ = 0), Plasson et al. found that the system allows four types of fixed points, labeled asymmetric, symmetric, dead, and unstable. The behavior of the system is thus governed by the nonzero stereoselectivity parameter, α, and the conserved total mass through the parameter c. Together, these two parameters control the type of fixed point. In all cases, if c is below a critical value, no dimers ever form. This is the (racemic) dead solution. The existence of these low concentration dead solutions becomes important when we study spatially extended systems. A stereoselectivity favoring formation of homochiral dimers (α < 1) was found to be essential in producing stable homochiral solutions (Brandenburg et al. 2007; Plasson et al. 2004) even in the relevant case of increased stereoselective pressure due to the presence of nonzero β and γ. Therefore, in this work we will restrict our investigations to the case α < 1.
As pointed out by Plasson et al., the model can be applied to realistic systems of amino acid derivatives (Plasson et al. 2004). Although amino acids have been shown to be synthesized under a variety of prebiotically relevant conditions (Miller 1955; Rode 1999), this fact alone is not enough to guarantee the eventual emergence of peptide chemistry or life: free amino acids are notoriously poor reactants. Therefore, the limiting factor in primitive peptide synthesis is most likely not the formation of the amino acids but, instead, their eventual activation.
The most commonly cited potential prebiotic activations of stable amino acid derivatives lead to the formation of N −carboxyanhydrides of α-amino acids (Commeyras et al. 2002; Huber and Wächtershäuser 1998; Leman et al. 2004). NCAs have several features that make them highly amenable to building a desirable prebiotic chemistry (i.e. a homochiral chemistry) based on the APED set of reactions (Plasson et al. 2004):
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1.
NCAs are very reactive amino acid derivatives, which easily permit the formation of peptides in aqueous solutions.
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2.
The polymerization of NCAs is stereoselective, favoring the formation of homochiral peptides.
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3.
The chemistry of NCAs promotes the recycling of products.
There exists a wide range of models based on the chemistry of NCAs with different energy sources for activation. Potential compounds that may have acted as sources of energy to activate amino acids on the primitive Earth include nitrogen oxides, as in the primary pump model of Commeyras and coworkers (Boiteau et al. 2001; Commeyras et al. 2002); CO, familiar from the work of Wächtershäuser and collaborators (Huber and Wächtershäuser 1998; Huber et al. 2003; Wächtershäuser et al. 1992); or COS, as in the model of Leman et al. (2004). Such sources of chemical energy would have existed on the early Earth, possibly in large quantities due to increased geological activity during the Hadean era such as outgassing from volcanos. For a NCA-driven APED chemistry, these activating compounds provide the necessary free energy required for the system to have operated in a primordial environment (Plasson et al. 2004; Plasson and Bersini 2008).
Results
The introduction of spatial dependence permits the net enantiomeric excess (ee) to evolve in space as well as time, thereby unveiling new and interesting dynamics in the APED system. We establish a spatiotemporal reaction-diffusion network from the rate equations derived from Eq. 1 by following the usual procedure in the phenomenological treatment of phase transitions outlined below. Systems with either spatially homogeneous and inhomogeneous concentrations are investigated separately.
Introducing Spatial Dependence
Spatial dependence was introduced following the usual procedure in the phenomenological treatment of phase transitions (Gunton et al. 1983; Langer 1992) by rewriting total derivatives as \(d/dt \rightarrow \partial / \partial t - k_{1,2} \nabla ^2\) in the rate equations derived from Eq. 1. This established a reaction-diffusion network with diffusion constants k 1 and k 2 describing the molecular diffusion of monomers and dimers respectively. It is convenient to introduce the dimensionless diffusion constants κ 1,2 = k 1,2/ κ, where κ is a dimensionful diffusion rate which we scale out of the network equations (typically we set κ 1 = 2κ 2). Some values of physically relevant diffusion rates are κ = 10 − 9 m2s − 1 for molecular diffusion in water and κ = 10 − 5 m2s − 1 for air (Cotterill 2002). The corresponding rate equations were then made dimensionless by scaling all concentrations [U] (with U being any monomer or dimer in the network) such that the dimensionless concentrations are written as \(u = \frac{p}{a} [U]\). This allowed us to scale the reaction rate p out of the network equations and to write all other network reaction rates in terms of dimensionless ratios with a (see below). Here we have chosen a as our tunable parameter as it is dependent on activation by consumption of fuel compounds from the primordial environment and is therefore more flexible than other model parameters (Plasson and Bersini 2008). We also introduce the dimensionless time and space variables t 0 ≡ a t and \(x_0 \equiv \sqrt{a/\kappa} ~~ x \). One may then recover dimensionful values for a particular choice of the rate a and the diffusion coefficient κ. The dimensionless rate equations corresponding to Eq. 1 (with b = 0) were found to be, with \(l \equiv \frac{p}{a} [L]\), \(d\equiv \frac{p}{a}[D]\), etc.:
and the corresponding four equations obtained with \(l \leftrightarrow d\). The dimensionless reaction rates η and ε are defined as η ≡ h/a and ε ≡ e/a and \({\scriptstyle \nabla_0^2}\) is the dimensionless Laplacian (in \({\scriptstyle 2d}\), \({\scriptstyle \nabla_0^2 = \partial^2 / \partial x^2 + \partial^2 / \partial y^2}\)). For the work presented here we have chosen values of κ 1 and κ 2 such that κ 1 = 2 κ 2.
We also note that the global ee, defined by Plasson et al. as a measure of the net asymmetry, is given by
where c is given in Eq. 2. The net enantiomeric excess we cite in this work is then found by spatial averaging, i.e.,
where A is the area.
Numerical Simulations with Stochastic Initial Conditions
The numerical implementation utilized a finite-difference leapfrog algorithm with spatial step δx = 0.2 and temporal step δt = 0.005. Periodic boundary conditions were adopted on a 5122 square lattice in two dimensions. Near-racemic initial conditions were prepared in a two step process. First, a racemic lattice configuration was established using the analytic form of the symmetric steady-state solution to the network equations in Eq. 3 (with b = 0), found as a function of the total concentration c, given in Eq. 2. The dependence of the analytic solution on the total mass allowed us to use the distribution of c(x) over the lattice to determine whether we would study a homogeneous or inhomogeneous system. For homogeneous systems, we set a uniform concentration \(c({\bf x}) = \langle c({\bf x}) \rangle > c_{\rm crit} = 1.5\) such that symmetry breaking would be observed everywhere in the system (here c crit is given for the case α = 0.35). For inhomogeneous systems, initial high concentration regions (i.e. regions where c > c crit), or bubbles, were established with Gaussian profiles such that \(c({\bf x}, 0) = {\cal C}\exp[-(x^2 + y^2)/R^2]\) where \({\cal C}\) is the total concentration of amino acids and peptides at the bubble’s core (\({\cal C} > c_{\rm crit}\)), and R is the radius of the bubble. Outside of the bubbles, the concentration was set to zero. The final step was to create stochastic initial conditions via a generalized spatiotemporal Langevin equation. We added a Gaussian white noise term, ξ(x, y, t), with zero mean and two-point correlation function \(\langle \xi({\bf x'}, t') \xi({\bf x}, t) \rangle = \theta^2 \delta (t' -t)\delta ({\bf x'} -{\bf x})\), to the rate equations. The equations of motion, u(x, y, t) from Eq. 3 with the added noise terms were then solved with simple quadratic potentials, V(u) = (1/2) u 2 and low noise (θ 2 = 0.002) until the volume-averaged enantiomeric excess achieved a steady-state Gaussian distribution centered on the racemic state. By steady-state we mean \(d \langle ee(t) \rangle /dt \approx 0\), where \(\langle ee \rangle\) is given by Eq. 5. Once the near-racemic initial condition was established, the noise (ξ(x, y, t)) was turned off and the system was then set to evolve deterministically.
Homogeneous Systems and Chiral Domains
We first consider the formation of chiral domains in systems with homogeneous concentrations (i.e. \(c(\textbf{x},t)=\) constant). With a near-racemic initial distribution, a typical spatial volume \({\cal V} \gg \lambda^2\), where λ is the correlation length, will coarsen into domains of left and right-handed chiralities (Brandenburg and Multamäki 2004; Gleiser and Thorarinson 2006; Gleiser 2007). This occurs after a long induction period where activated monomers of both chiral species accumulate in the system. During the induction period, the ee (given in Eq. 4) remains small; however, once a sufficient concentration of activated monomers has been achieved we begin to observe regions of growing enantiomeric excess. Results demonstrating the evolution of \(\langle ee \rangle\) are shown in Fig. 1 for a number of runs (the dashed lines in the figure correspond to the two sample systems of Fig. 2). We present data for both the unrealistic case of complete stereoselectivity of depolymerization and epimerization reactions (β = γ = 0) and for more realistic nonzero parameters (β, γ ≠ 0), although for the homogeneous systems of this section we restrict our analysis to β = γ = 0. We note that the results are qualitatively similar even if with realistic parameters the final ee never reaches a complete homochiral state (see Plasson et al. 2004). As discussed in the introduction, other polymerization models describing the onset of homochirality yield similar results for the evolution of the spatially averaged \(\langle ee \rangle\) (Gleiser and Walker 2008) without the activation period which is typical of the APED model.
We have observed two types of domain evolution, as shown in Fig. 2. In the top row, domains of both chiralities percolate (i.e. permeate the entire volume) through the volume and the system reaches a steady-state consisting of two domains with opposing chirality separated by a thin domain wall. In the bottom row, only one chiral domain percolates and the system eventually evolves toward homochirality. The parameters chosen here (β = γ = 0 with α = 0.3, ε = η = a, and b = 0) allow for near complete conversion to homochirality: within a single domain, the net ee ≥ 99 %.
Quite interestingly, the domain wall or ring-like structure surrounding the homochiral domains consists of a racemic mixture of monomers and dimers including large concentrations of the heterodimers DL and LD, as shown in Fig. 3. This is very suggestive of a physical barrier isolating the inside of the homochiral domain and is true both when only one chirality percolates (bottom-right snapshot), and when both chiralities percolate (top-right snapshot), where one observes the formation of tubular domains. These situations are suggestive of micelle vesicles and bilayer membranes, observed in emerging self-assembled structures of amphiphiles (Deamer et al. 2002). It is thus of great interest to examine the possibility of assembling similar structures in an inhomogeneous context, such that homochiral protodomains may become surrounded by a racemate.
Inhomogeneous Systems: The Role of Non-Uniform Concentration
The examples discussed thus far have maintained a uniform concentration over the entire lattice. We now consider the more realistic dynamics of systems with spatially-dependent concentrations (\(c(\textbf{x},t) \neq \) constant). In this case, starting from stochastic near-racemic initial conditions, regions where chiral symmetry breaking occurs and regions where a racemate is maintained should emerge dynamically. Holding all reaction parameters fixed, the previous results indicate that we should observe this separation in systems where some regions have concentrations above and others below a critical, parameter-dependent value (see section “The Model”). Accordingly, our simulations show that the spatially-extended APED system naturally develops chiral protocell-like structures surrounded by a racemate, as shown in Fig. 4.
Left to evolve diffusively, the high-concentration protocellular domains containing an enantiomeric excess (Fig. 4 lower panel) would eventually shrink away. However, we must recall that in prebiotic Earth reactor pools were submitted to environmental disturbances ranging from mild (e.g. tides, evaporating lagoons) to severe (e.g. volcanic eruptions, meteoritic impacts). Both kinds of disturbances affected the evolution of chirality in early Earth (Gleiser et al. 2008). Recent studies of life’s origins have focused on molecular interactions in the context of changing tides (Boiteau et al. 2001; Bywater and Conde–Frieboes 2005; Commeyras et al. 2002; Lathe 2004, 2005) or evaporating pools and lagoons (Robertson and Miller 1995) as ways to enhance the concentrations of reactants. From a modeling perspective, their effect can be mimicked by a time-dependent modulation in the diffusion rates.
To simulate such processes, we started the system’s evolution with a fast diffusion coefficient (κ 2 = 0.1, corresponding to molecular diffusion slightly slower than that in water with dimensionful values) followed by evolution with a very slow diffusion rate (\(\kappa_2 = 10^{-6}\)) such as might occur for molecules diffusing on dry clay, a rocky surface, or on a beach. The initial conditions were set such that the lattice had, on average, a low concentration of amino acids and peptides: \(\langle c({\bf x}) \rangle < c_{\rm crit}\), where c crit = 1.5 for the systems studied. Bubbles with higher concentrations, c(x) > c crit, were interspersed on the lattice (see section “Numerical Simulations with Stochastic Initial Conditions”). The results of a sample run are shown in Fig. 4. The stereoselectivities have been set such that α = 0.35, β = 0.2, and γ = 0.3 as in the “real system” parameters from Plasson et al. (2004), with the non-stereoselective reaction rates set to the dimensionless values ε = η = 10 and b = 0 (a and p have been scaled out of the network equations - see section “Introducing Spatial Dependence”). Since the epimerization rate on the N-terminal is of the same order as the hydrolysis rate for NCAs (Plasson et al. 2004), we have set ε = η (i.e. e = h).
The top left snapshot in Fig. 4 shows a near-racemic distribution with regions of higher reactant concentration barely visible. In this simulation, the tide would ebb or the lagoon evaporate between the two leftmost snapshots in the bottom row. Following the drying of the tidal pool or lagoon, regions with total reactant concentration initially above critical are seen to coarsen into domains with high \(\langle ee \rangle\) surrounded by a near-racemic environment.
As with the homogeneous case, we also investigated if the near-homochiral domains were surrounded by a ring-like structure rich in heterodimers LD and DL. In Fig. 5, we see that, indeed, such rings do appear. The net concentrations are sensitive to the parameters β and γ and tend to be suppressed for high values. The figure shows a simulation with the values β = 0.001 and γ = 0.001. Also, as in Fig. 4, the diffusion was sharply reduced to simulate a tidal ebb: in this case, the tide would ebb prior to the snapshots shown in Fig. 5. Our results show that for small nonzero values of β and γ (typically < 0.05) the near-homochiral domains are surrounded by racemic boundary structures.
Toward Smaller Protodomains
For suitable choices of our tuneable parameter a—a measure of the energy input into the reactor pool, we can recover physically relevant, dimensionful values for the timescale and spatial extent. Here we focus on the inhomogeneous case as it offers a realistic example of a spatially-extended prebiotic system. Taking a = 10 − 8 s − 1 as in the real system parameters of Plasson et al., the hydrolysis rate assumes the value h = 10 a = 10 − 7 s − 1 indicative of either high or low pH conditions (Plasson et al. 2004; Smith and Hanson 1998). Using the dimensionless space and time variables, x 0 = 102.4 and t 0 = 225 from the simulation, the physical space and time scales are x = 35 m and t = 713 y, respectively, not unreasonable values for a small pond that after evaporating for hundreds of years leaves chiral domains behind. Increasing a will decrease the physical size and timescales of the simulation. If, instead, we take a = 10 − 6 s − 1, we obtain x = 3.2 m and t = 7.1 y, indicating faster time scales for evaporation of smaller lagoons or pools. A changing tide on the order of hours in microscopic protocellular domains is harder to achieve with presently accepted values of the reaction parameters. However, we have completed additional simulations on 1282 square lattices using parameters dt = 0.0001 and dx = 0.05 where proto-domains with diameters of centimeters and timescales of years were achieved for a = 10 − 5s − 1. Please note that these dimensions are not due to fundamental restrictions on the chemistry involved but due to the limitations of our numerical simulations.
Discussion
Our results demonstrate that for suitable parameter choices, the APED model exhibits chiral symmetry breaking leading to homochiral (or near-homochiral) domains in spatially extended systems. The results are qualitatively similar to those for other bottom-up polymerization models describing the onset of homochirality where domains of opposite chirality form and compete for dominance (Brandenburg and Multamäki 2004; Gleiser and Walker 2008), although here the model allows for the possibility of complete conversion of all chiral subunits for suitable parameter choices. A key point is that symmetry breaking in APED systems is sensitive to the total mass: processes, environmental or otherwise, which acted to accumulate prebiotic compounds would have favored the emergence of homochirality.
As discussed in the introduction, self-organization of short peptides has previously been proposed as a possible mechanism for formation of the first protocellular membranes (Fishkis 2007; Fox 1973, 1980). In the context of the results presented here, this implies that in regions where homochiral peptides are formed, one may observe spontaneous emergence of peptide vesicles. In fact, a compelling feature of polypeptide self-organization is that homochiral polypeptides have the propensity to form β-sheets while racemic mixtures will not exhibit such structural conformation (Brack 1979). For molecules consisting of homochiral and heterochiral segments, structural formation entails aggregation of stable homochiral β-sheets surrounded by less stable and disordered heterochiral segments (Brack 1979); furthermore, when subjected to mild hydrolysis, the more stable homochiral sheets are enriched by the residual fraction. These mechanisms may play a significant role in structural formation within the near-homochiral regions shown in Fig. 3. It is therefore plausible that formation of β-sheets will be enhanced in homochiral regions, consistent with favoring vesicle formation in regions with high ee, although there is no experimental proof of this correlation. In this scenario, homochiral, high concentration regions are preferentially selected to evolve into primitive protocellular structures.
Self-organized homochiral protocellular structures could potentially share many features in common with modern cellular life. Encapsulation of macromolecules has been discussed in the context of lipid membranes via dehydration–rehydration processes (Deamer et al. 2002); it is possible that such processes may have operated in peptide membranes as well (Fishkis 2007). Short peptides have been shown to exhibit catalytic activity under prebiotic conditions (Shen et al. 1990). In addition, a potential energy source for the protocell could be the chemical energy of activated amino acids (Fishkis 2007) that would still be present in the system at steady state. In fact, the APED model has been described as a protometabolic pattern (Plasson et al. 2004). At the very least, peptide protocells represent feasible prototypes displaying rudimentary features of modern cellular life (Fox 1973; Fishkis 2007). In light of the work presented here, this may now be extended to include homochiral protocells in the context of the APED model. We stress that our work says nothing of more complex cell behavior, such as nutrient exchange across cellular membranes and cell division. But it does provide a framework to study the emergence of isolated homochiral domains within a promising peptide model, possibly a first step toward the formation of rudimentary cell-like structures in early Earth.
We also note that in the absence of a specific chiral bias, the net enantiomeric excess in the APED model, and in many models of chiral symmetry breaking, is random and may be attributable to amplification of stochastic fluctuations about the initial near-racemic state (Dunitz 1996) due to environmental influences (Gleiser et al. 2008) which may or may not induce turbulence (Brandenburg and Multamäki 2004). Therefore, as shown in Fig. 4, isolated regions can develop opposite chirality. This raises the possibility of having life forms of opposing chirality competing for resources on the early Earth (Brandenburg and Multamäki 2004). Extending this scenario to other potentially life-bearing planetary platforms, and consistent with the difficulties of using parity violation in the weak interactions as a consistent chiral bias (Gleiser 2007), our results suggests the existence of stereochemistry of opposing chirality, and possibly life, elsewhere in the universe (Castelvecchi 2007; Gleiser et al. 2008). It is hopeful that proposed robotic missions such as the Titan Organics Explorer, if funded, will be equipped to analyze enantioenriched organic compounds (Welch and Lunine 2001) shedding light on this fundamental question.
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Acknowledgements
This work was supported in part by a National Science Foundation Grant PHY-0757124. We thank R. Plasson and Axel Brandenburg for many interesting suggestions and comments. SW thanks NORDITA in Stockholm for their kind hospitality during the initial stages of this work.
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Gleiser, M., Walker, S.I. Toward Homochiral Protocells in Noncatalytic Peptide Systems. Orig Life Evol Biosph 39, 479–493 (2009). https://doi.org/10.1007/s11084-009-9166-5
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DOI: https://doi.org/10.1007/s11084-009-9166-5