Abstract
The emergence of biochemical homochirality was a key step in the origin of life, yet prebiotic mechanisms for chiral separation are not well constrained. Here we demonstrate a geochemically plausible scenario for chiral separation of amino acids by adsorption on mineral surfaces. Crystals of the common rock-forming mineral calcite (CaCO3), when immersed in a racemic aspartic acid solution, display significant adsorption and chiral selectivity of d- and l-enantiomers on pairs of mirror-related crystal-growth surfaces. This selective adsorption is greater on crystals with terraced surface textures, which indicates that d- and l-aspartic acid concentrate along step-like linear growth features. Thus, selective adsorption of linear arrays of d- and l-amino acids on calcite, with subsequent condensation polymerization, represents a plausible geochemical mechanism for the production of homochiral polypeptides on the prebiotic Earth.
One of life's most distinctive biochemical signatures is its strong selectivity for chiral molecular species, notably l-amino acids and d-sugars. Prebiotic synthesis reactions, with the possible exception of some interstellar processes, yield essentially equal amounts of l- and d-enantiomers (1–4). A significant challenge in origin-of-life research, therefore, is to identify natural mechanisms for the homochiral selection, concentration, and polymerization of molecules from an initially racemic mixture (5, 6). Symmetry breaking on a chirally selective mineral surface offers a viable scenario for the origin of life; according to Lahav (5), “if a selective adsorption of chiral amino acids . . . on certain crystal faces were observed, then the problem of biological homochirality would be possible to comprehend.”
Effective chiral selectivity by a crystal requires at least three noncolinear configuration-dependent points of interaction between the molecule and an acentric mineral surface (7). Most previous experimental studies of adsorption of organic molecules on mineral surfaces have focused on the symmetry-breaking effects of right- vs. left-handed quartz, which is the most common acentric mineral (8). However, recent studies, which report minimal adsorption of organic molecules by quartz in an aqueous environment, cast doubt on any significant role of quartz in prebiotic chiral selectivity (6). Centric minerals, although seldom studied for their chiral selectivity, also have the potential for symmetry breaking (5, 9, 10). Indeed, any general crystal face with a surface structure that does not possess mirror symmetry has the potential for enantioselectivity. Crystal faces that meet these conditions are displayed by most common rock-forming minerals (11, 12).
We chose calcite (CaCO3; rhombohedral space group Rc) for adsorption experiments for three reasons. First and foremost, calcite was one of the most abundant marine minerals in the Archaean era. Thick limestone (calcium carbonate) formations are common in Archaean terranes, including the oldest known sedimentary formations (13). Sumner (14) has proposed that before 2.5 billion years ago, massive calcite deposits “precipitated as crystals directly on the sea floor.” Carbonate-rich formations, furthermore, often partially dissolve and reprecipitate under mildly acidic or hydrothermal conditions, and the [211] trigonal scalenohedral is the most commonly observed crystal form in vein and vug coatings. Calcite crystal surfaces would thus have been widely present in prebiotic environments.
A second, more pragmatic reason for employing calcite is that it is readily available in large (>10 cm) crystals with prominent [211] trigonal scalenohedral crystal forms, commonly referred to as “dog-tooth” crystals (12). Pairs of adjacent scalenohedral faces, for example (211) and (31), possess surface structures that are related by mirror symmetry (Fig. 1) and thus have the potential for chiral selectivity.
A third reason for using calcite in studies of chiral separation is its well documented tendency to adsorb amino acids. Biomineralized calcite is strongly bonded to proteins in the shells of many invertebrates (15, 16). Surface-growth topology of calcite, furthermore, may be affected strongly by the presence of L- vs. d-amino acids (17)—a phenomenon that underscores calcite's potential for chiral selectivity.
Experimental Methods
As a test of chirally selective adsorption, we immersed four calcite crystals for 24 h in a 0.05 M solution of racemic aspartic acid, which is strongly adsorbed onto calcite (14, 15). Crystal nos. 1, 3, and 4 are pale golden calcite from the Gordonville–Elmwood Mine (Carthage, TN). Crystal no. 2 is a pale golden calcite from Joplin, MO. Maximum crystal dimensions ranged from 11 to 18 cm, whereas surface areas of crystal faces selected for study range from 6 to 36 cm2. Each crystal displays at least one termination with no significant development of surfaces other than faces of the [211] form, although not all faces are well developed on all crystals. Three types of faces, R, L, and C, were studied. The R and L denote enantiomeric scalenohedral faces, which have the potential for chiral selectivity (Fig. 1). The R-type faces are equivalent to (211), whereas L-type faces are equivalent to (31). The C denotes a rhombohedral cleavage face equivalent to (101); these faces have a centric surface structure that should not selectively adsorb l- or d-amino acids, and thus can serve as an experimental control. The initial assignment of an index to a calcite face is somewhat arbitrary, owing to the rhombohedral symmetry. We assign indices in the same sense as Dana (12). Note, however, that once one face is assigned indices, the indices of all other faces are defined completely.
We cleaned each crystal successively with deionized water, methanol, methylene chloride, methanol, and deionized distilled water for two cycles. Each face was then etched for 20 seconds in 0.02 M HCl and rinsed in HPLC-grade water. After this thorough surface cleaning, we immersed each crystal in a separate 0.05 M solution of racemic aspartic acid. After 24 h, each crystal was removed from its aspartic acid solution and washed by immersion in HPLC-grade, distilled deionized water. We subsequently removed adsorbed aspartic acid from each individual crystal face by holding the face horizontally, pipetting 0.02 M HCl onto the face for 20 sec, and then collecting the acid wash in the same pipet. We repeated this procedure three times on 3 successive days for each face.
The d/l-aspartic acid values were measured by gas chromatography of N-trifluoroacetyl isopropyl ester derivatives, with a Chirasil-val 50-m × 0.25-mm i.d. column (Alltech Associates) and a nitrogen–phosphorus detector in a Hewlett–Packard 5890 series II gas chromatograph. Derivatization followed the methods of Goodfriend (18), except that the esterification step was carried out for 60 min and the fully derivatized samples were dried under a nitrogen stream rather than low vacuum. Maximum aspartic acid adsorption, estimated by comparison with GC peak areas of a concentration series of standard solutions, was ≈1 nmol/cm2. No other amino acids were detected in any of our GC analyses; therefore, contamination by environmental l-amino acids is not a significant factor in these experiments.
Results
The d/l values for three sets of acid-wash experiments on 23 different crystal faces are recorded in Table 1. The d/l values for 12 acid-wash experiments on four different (101)-type cleavage faces (denoted C) range from 0.9889 ± 0.0051 to 1.0025 ± 0.0051, with a mean value of 0.9964—consistent with the 0.9948 ± 0.0015 d/l value observed for the aspartic acid experimental solution.
Table 1.
Crystal no. | Indices | Face type | d/l (1) | d/l (2) | d/l (3) |
---|---|---|---|---|---|
1 | (2 1 3̄ 1) | R | 1.0020(25) | 1.0123(12) | 1.0365(19) |
(3 1̄2̄ 1) | L | 0.9922(2) | 0.9978(15) | 0.9857(12) | |
(1 3̄ 2 1) | R | 1.0053(20) | — | 1.0029(34) | |
(1̄2̄ 3 1) | L | 0.9398(16) | — | 0.9991(34) | |
(3̄ 2 1 1) | R | 0.9904(28) | 1.0062(45) | — | |
(2̄ 3 1̄ 1) | L | 0.9894(10) | 0.9918(37) | 0.8960(49) | |
2 | (2 1 3̄ 1) | R | 1.0004(51) | 1.0042(51) | — |
(3 1̄2̄ 1) | L | 0.9850(51) | 0.9908(51) | 0.9594(36) | |
(1 3̄ 2 1) | R | 0.9957(51) | 0.9974(51) | 1.0113(27) | |
(1̄2̄ 3 1) | L | 1.0036(51) | 0.9800(23) | 0.9930(51) | |
(3̄ 2 1 1) | R | 0.9984(2) | 1.0001(51) | 0.9996(51) | |
(2̄ 3 1̄ 1) | L | 0.9925(51) | 0.9695(23) | 0.9811(24) | |
(0 1 1̄1̄) | C | 0.9889(51) | 1.0025(51) | 0.9972(25) | |
3 | (2 1 3̄ 1) | R | 1.0011(51) | 0.9986(51) | 0.9852(8) |
(3 1̄2̄ 1) | L | — | 0.9979(51) | 0.9288(51) | |
(1̄2̄ 3 1) | L | 0.9942(51) | 1.0028(51) | 0.9470(12) | |
(2̄ 3 1̄ 1) | L | 1.0028(51) | 0.9993(51) | 0.9938(51) | |
(0 1 1̄1̄) | C | 1.0024(51) | 0.9928(51) | 1.0002(51) | |
(1 1̄ 0 1̄) | C | 0.9917(51) | 0.9988(51) | 0.9936(51) | |
4 | (2 1 3̄ 1) | R | 0.9955(51) | 0.9935(51) | 0.9860(29) |
(1̄2̄ 3 1) | L | 1.0038(51) | — | 0.9952(51) | |
(2̄ 3 1̄ 1) | L | 1.0026(51) | 1.0013(6) | 0.9675(31) | |
(1 1̄ 0 1̄) | C | 0.9975(51) | 0.9972(51) | 0.9937(12) |
The analytical error of d/l-aspartic acid values, based on 3–6 (mean of 3.6) replicate injections of 15 samples, averaged 0.0051 or 0.52% of the d/l value. For samples analyzed only once, this value is taken as the error of the measurement. For samples analyzed two or more times, the standard error of the measurements is used as the measure of analytical error.
Two crystals (nos. 1 and 2) with finely terraced, chevron-like growth textures on [211]-type scalenohedral faces display significant chiral selectivity (Fig. 2 and Table 1). Faces of the same handedness as (211), which are designated R in Fig. 2 and Table 1, selectively adsorb d-aspartic acid. The mean value of d/l from 15 separate acid-wash experiments (Table 1) is 1.0042, with a maximum observed value in a single acid wash of 1.0365 ± 0.0019. Of these 15 d/l values, 14 are greater than the 0.9948 value of the experimental solution.
The opposite pattern is observed for mirror-related (31)-type faces (designated L in Fig. 2 and Table 1), which selectively adsorb l-aspartic acid. The mean d/l value for 17 acid-wash experiments range is 0.9792, with a minimum observed value of 0.8960 ± 0.0049. Of these 17 d/l values, 14 are less than the 0.9948 value of the experimental solution.
The maximum observed chiral excess of ≈10% is a lower limit for calcite chiral selectivity, because each acid wash may incorporate some of the 0.05 M racemic aspartic acid solution. This solution, trapped in microscopic cracks and pits on the calcite surface, cannot be removed fully by the water rinse, but it may be extracted in part during the acid-wash process. Less than a microliter of this racemic experimental solution would overwhelm the nanomolar amounts of adsorbed amino acid. Microscopically localized chiral excess of d- and l-aspartic acid may thus be many times greater than the bulk values reported here.
In contrast, adsorption of aspartic acid on the other two crystals (nos. 3 and 4 in Table 1), which possess mirror-smooth scalenohedral faces, is approximately racemic in 17 of 20 acid-wash experiments on scalenohedral faces. Three single experiments yielded l-aspartic acid excesses (d/l < 0.97) from L-type faces, but no other systematic trends are evident.
Conclusions
This study of calcite–aspartic acid interactions points to the need for additional experimental and theoretical studies. The contrast in behavior between crystals with different surface-growth textures underscores the need for these studies. Experiments with racemic mixtures of other amino acids, as well as sugars and nucleotides, will also be of importance in understanding the extent and relevance of these effects. Preliminary experiments reveal that d- and l-alanine display selective adsorption behavior similar to aspartic acid, whereas d- and l-valine and lysine may not be adsorbed selectively on calcite.
Many other mineral–molecule pairs also have the potential for chirally selective adsorption. Large natural crystals with enantiomeric faces occur commonly for the evaporite minerals gypsum (hydrous calcium sulfate) and barite (barium sulfate), as well as apatite (calcium phosphate). Significantly, chiral amino acids affect the growth morphology of gypsum crystals (19), so chiral selectivity by gypsum may be expected also. All of the major rock-forming minerals in basalt, including pyroxenes, feldspars, and olivines, also may display enantiomorphic pairs of faces (12).
These experiments have implications for origin-of-life scenarios. The Archaean Earth had substantial, although presumably dilute, inventories of racemic amino acids, both from exogenous sources (20, 21) and from prebiotic synthesis (22, 23). This study demonstrates that calcite and other minerals may have provided a mechanism for concentrating and chirally selecting these amino acids.
These results may also point to a possible mechanism for prebiotic synthesis of homochiral polypeptides. Chirally selective adsorption occurs preferentially on calcite surfaces with terraced growth features. This phenomenon suggests that local, highly selective concentration of d- and l-enantiomers may arise along step-like features, with calcite serving as a template for linear arrays of homochiral amino acids. Such a configuration may promote homochiral polymerization (24–26), which is a key step in the synthesis of self-replicating peptides (27, 28). We suggest that mineral-mediated chiral selectivity, in conjunction with homochiral polymerization, may thus provide a link between prebiotic synthesis and the RNA/protein world.
Acknowledgments
We thank L. Becker, G. Cody, J. Cronin, D. Deamer, R. Downs, W. Huntress, A. Knoll, M. McCarthy, M. Singer, J. Szostak, N. Tuross, P. Unrau, and H. Yang for useful discussions and constructive reviews of the manuscript. R. Filley, M. Grosso, and M. Horan contributed to the development of analytical procedures. This work was supported by the National Aeronautics and Space Administration Astrobiology Institute, the National Science Foundation, and the Carnegie Institution of Washington.
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