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Structural studies on HCN oligomers.

NMR spectral studies on the HCN oligomers suggest the presence of carboxamide and urea groupings. The release of CO2, H2O, HCN, CH3CN, HCONH2 and pyridine on pyrolysis is consistent with the presence of these groupings as well as carboxylic acid groups. No basic primary amine groupings could be detected with fluorescamine. Hydrazinolysis of the HCN oligomers releases 10% of the amino acids normally released by acid hydrolysis. The oligomers give a positive biuret test but this is not due to the presence of peptide bonds. There is no conclusive evidence for the presence of peptide bonds in the HCN oligomers. No diglycine was detected on partial hydrolysis of the HCN oligomers at pH 8.5 suggesting that HCN oligomers were not a source of prebiotic peptides.

Amino Acids↗

Origin of organic compounds on the primitive earth and in meteorites.

The role and relative contributions of different forms of energy to the synthesis of amino acids and other organic compounds on the primitive earth, in the parent bodies or carbonaceous chondrites, and in the solar nebula are examined. A single source of energy or a single process would not account for all the organic compounds synthesized in the solar system. Electric discharges appear to produce amino acids more efficiently than other sources of energy and the composition of the synthesized amino acids is qualitatively similar to those found in the Murchison meteorite. Ultraviolet light is also likely to have played a major role in prebiotic synthesis. Although the energy in the sun's spectrum that can be absorbed by the major constituents of the primitive atmosphere is not large, reactive trace components such as H2S and formaldehyde absorb at longer wavelengths where greater amounts of energy are available and produce amino acids by reactions involving hot hydrogen atoms. The thermal reaction of CO + H2 + NH3 on Fischer-Tropsch catalysts generates intermediates that lead to amino acids and other organic compounds that have been found in meteorites. However, this synthesis appears to be less efficient than electric discharges and to require a special set of reaction conditions. It should be emphasized that after the reactive organic intermediates are generated by the above processes, the subsequent reactions which produce the more complete biochemical compounds are low temperature homogenous reactions occurring in an aqueous environment.

Amino Acids↗

Photochemical reactions in interstellar grains photolysis of CO, NH3, and H2O.

A simulation of the organic layer accreted onto interstellar dust particles was prepared by slow deposition of a CO:NH2:H2O gas mixture on an Al block at 10 K, with concomitant irradiation with vacuum UV. The residues were analyzed by GC-MS, HPLC, and near IR; a reaction pathway leading from NH3 to complex alcohol, fatty acid, and amide products in 27 stages is postulated. The astronomical relevance and significance of the observations are discussed.

Ammonia↗

Estimates of the maximum time required to originate life.

Fossils of the oldest microorganisms exist in 3.5 billion year old rocks and there is indirect evidence that life may have existed 3.8 billion years ago (3.8 Ga). Impacts able to destroy life or interrupt prebiotic chemistry may have occurred after 3.5 Ga. If large impactors vaporized the oceans, sterilized the planets, and interfered with the origination of life, life must have originated in the time interval between these impacts which increased with geologic time. Therefore, the maximum time required for the origination of life is the time that occurred between sterilizing impacts just before 3.8 Ga or 3.5 Ga, depending upon when life first appeared on Earth. If life first originated 3.5 Ga, and impacts with kinetic energies between 2 x 10(34) and 2 x 10(35) were able to vaporize the oceans, using the most probable impact flux, we find that the maximum time required to originate life would have been 67 to 133 million years (My). If life first originated 3.8 Ga, the maximum time to originate life was 2.5 to 11 My. Using a more conservative estimate for the flux of impacting objects before 3.8 Ga, we find a maximum time of 25 My for the same range of impactor kinetic energies. The impact model suggest that it is possible that life may have originated more than once.

Earth, Planet↗

Phosphorylation of glyceric acid in aqueous solution using trimetaphosphate.

The phosphorylation of glyceric acid is an interesting prebiotic reaction because it converts a simple, potentially prebiotic organic molecule into phosphate derivatives that are central to carbohydrate metabolism. We find that 0.05 M glyceric acid in the presence of 0.5 M trimetaphosphate in alkaline solution gives a mixture of 2- and 3-phosphoglyceric acids in combined yields of up to 40%.

Deuterium Oxide↗

Potentially prebiotic syntheses of condensed phosphates.

In view of the importance of a prebiotic source of high energy phosphates, we have investigated a number of potentially prebiotic processes to produce condensed phosphates from orthophosphate and cyclic trimetaphosphate from tripolyphosphate. The reagents investigated include polymerizing nitriles, acid anhydrides, lactones, hexamethylene tetramine and carbon suboxide. A number of these processes give substantial yields of pyrophosphate from orthophosphate and trimetaphosphate from tripolyphosphate. Although these reactions may have been applicable in local areas, they are not sufficiently robust to have been of importance in the prebiotic open ocean.

4-Butyrolactone↗

Enantioselective autocatalysis. IV. Implications for parity violation effects.

Historically, parity violation at the contemporary biomolecular level (i.e., only L-amino acids in proteins and D-sugars in DNA and RNA) has been postulated to be the inevitable result of parity violations at the elementary particle level, involving either beta-decay electrons or parity violating energy differences (PVEDs) between enantiomers. These two chiral biases have in turn allegedly impressed a small but persistent chirality onto prebiotic chemistry which, after appropriate amplification, has culminated in our contemporary homochiral biopolymers. Experiments and controversies pertaining to the efficacy of these two chiral biases are reviewed briefly, with the conclusions that: a) there is no experimental evidence supporting the capability of beta-decay electrons or other spin-polarized chiral particles to generate chiral molecules, and b) only theoretical calculations, but no experimental evidence, support the allegation of a causal relation between PVEDs and biomolecular homochirality. We here attempt to examine the latter allegation experimentally. Spontaneous resolution under racemization conditions (SRURC) during the crystallization of the bromofluoro-1,4-benzodiazepinooxazole derivative I is capable of affording products of high enantiomeric purity. This process, which involves very efficient stereoselective autocatalysis, has now been examined statistically. If PVED effects are operative, the SRURC of racemic I should provide, either exclusively or with a strong and consistent bias, only one enantiomer of crystalline I. However, crystallization experiments of racemic I showed no bias in its SRURC, leading to the conclusion that PVED effects are ineffective in dictating a preferred chirality in this system. Several earlier experiments in the literature leading to a similar conclusion as to the inefficacy of PVED effects in promoting a preferred chirality are noted.

Amino Acids↗

The influence of prebiotic-type organic molecules on the crystallization of Al and Mg hydroxides.

It is now well accepted that clays could have concentrated prebiotic organic molecules, protected them from UV radiation and served as templates and catalysts in their prebiotic evolution. A complementary question is: How did prebiotic organics in the oceans, in ground water, or in hydrothermal solutions affect the formation and inorganic evolution of oxides, hydroxides, and clay minerals? In this study predominantly amorphous Al oxyhydroxides (Al gels) and crystalline Mg hydroxyoxides were synthesized, and then crystallized and recrystallized respectively, to Al and Mg hydroxides via wet and dry (w/d) cycling using both water and organic solutions. The products that resulted were examined using IR spectroscopy and X-ray diffraction (XRD). XRD scans of the products formed by w/d cycling of the Al gels with either water or 0.1 M aqueous solutions of methanol or formaldehyde showed that bayerite (alpha Al2O3) was the major phase formed. The acetonitrile treated sample exhibited the most defined XRD peaks, and no crystalline phase could be observed by XRD of the 0.1 M formamide solution treated sample. Cycling the Mg hydroxyoxide with water, or 0.1 M solutions of methanol, formamide, formaldehyde, or acetonitrile resulted in the formation of brucite (Mg(OH)2) (in varying amounts) and of three unidentified phases. One unidentified phase, 'phase II', was observed in the formaldehyde cycled sample (and tentatively identified in the methanol and formamide cycled samples), 'phase III' in the formamide and formaldehyde cycled sample, and 'phase IV' in only the formaldehyde. XRD peaks with a spacing of approximately 11.5 Angstrom (assigned to phase III) suggest intercalation of formamide and formaldehyde into the interlayer spaces of the brucite. Phosphate treatment, prior to w/d cycling with water, and also with the above mentioned organics, while totally preventing subsequent formation of any crystalline Al hydroxide, enhanced the formation of Mg phases, shown by XRD data. Formation of brucite was impeded only by w/d cycling using concentrated methanol solution, but even these effects were reversible. The XRD scans of the products resulting from the aqueous and organic solution cycling treatments of the Mg starting materials showed peaks due to brucite and three unidentified phases. Only the brucite is evident in oriented sample XRD scans of the Mg starting material when treated with methanol, formamide, and acetonitrile. In random powder sample XRD scans of the Mg starting material treated with: 1) methanol--the unidentified phase 11 is evident, 2) formamide--phase II and III are seen, and 3) formaldehyde--phases II, III, and IV are evident.

Acetonitriles↗

Formate ester formation in amide solutions.

Simple aliphatic alcohols, deoxynucleosides and nucleosides undergo reaction with formamide yielding formate esters. Formate ester formation was observed to occur slowly at 100 degrees C and more rapidly at 130 degrees C. As expected, formate esters were hydrolyzed to the alcohol and formic acid upon heating in aqueous solution. It was proposed to study the possibility that formate esters are formed initially in amide solvents, followed by displacement of formate by dihydrogen phosphate ion to form monophosphate esters. Experiments are described which demonstrate the formation and hydrolysis of formate esters, as well as their lack of reaction with hydrogen phosphate ion. Formate esters are not intermediates in the phosphorylation of nucleosides in formamide. Their formation has been observed and such an esterification is a side reaction during the phosphorylation of nucleosides in formamide.

Adenosine↗

Oligomerization of negatively-charged amino acids by carbonyldiimidazole.

The carbonyldiimidazole-induced oligomerizations of aspartic acid, glutamic acid and O-phospho-serine are amongst the most efficient reported syntheses of biopolymers in aqueous solution. The dependence of the yields of products on the concentrations of reagents, the temperature and the enantiomeric composition of the substrate amino acids are reported. Catalysis by metal ions, particularly by Mg2+, is described. These reactions do not generate significant amounts of material in the size-range of several tens of residues that are thought to be needed for a polymer to function as a genetic material.

Aspartic Acid↗

2-aminopropionitrile polymer. I. The hydrolyzate of the basic fraction.

The basic fraction of a 2-aminopropionitrile polymer was subjected to acid hydrolysis and was analyzed by means of GC-MS, after trimethylsilylation. The fundamental polymer structural units were alanine, 2,2'-iminodipropionic acid, N-(1-cyanoethyl)alanine, N-ethylalanine, glycine, cyanoglycine, and 5-amino-4-carboxyimidazole residues. The last three units may be derived from hydrogen cyanide. Oligomeric combinations of these units were also detected in the hydrolyzate, due to partial hydrolysis of the polymer.

Acetaldehyde↗

Thermal synthesis and hydrolysis of polyglyceric acid.

Polyglyceric acid was synthesized by thermal condensation of glyceric acid at 80 degrees in the presence and absence of two mole percent of sulfuric acid catalyst. The acid catalyst accelerated the polymerization over 100-fold and made possible the synthesis of insoluble polymers of both L- and DL-glyceric acid by heating for less than 1 day. Racemization of L-glyceric acid yielded less than 1% D-glyceric acid in condensations carried out at 80 degrees C with catalyst for 1 day and without catalyst for 12 days. The condensation of L-glyceric acid yielded an insoluble polymer much more readily than condensation of DL-glyceric acid. Studies of the hydrolysis of poly-DL-glyceric acid revealed that it was considerably more stable under mild acidic conditions compared to neutral pH. The relationship of this study to the origin of life is discussed.

Evolution, Chemical↗

Condensation of vaporous amino acids in the presence of silica. Formation of bi- and tricyclic amidines.

Amino acids (alanine, valine, norvaline, leucine, and 2-aminoisobutyric acid) were subjected to repeated (5-9 times) sublimation in the presence of silica at temperature of 220-240 degrees C. The major amino acid condensation products were diketopiperazines (DKPs) in yields of 27-89%. Mixtures of by-products have been isolated from the DKPs by means of chloroform extraction. On the basis of fast atom bombardment mass spectrometric studies of the mixtures it is proposed that under these conditions further dehydration proceeds resulting in bicyclic (BCA) and tricyclic (TCA) amidine derivatives of DKPs; the BCA formation has been confirmed by means of IR and 1H NMR spectroscopy in the case of 2-aminoisobutyric acid. During the sublimation, thermal destruction of the cyclic products was also observed accompanied by the cycle degradation and cleavage of alkyl substituents. The BCAs and TCAs are considered as possible sources of linear di- and tripeptides.

Amidines↗

The spark discharge synthesis of amino acids from various hydrocarbons.

The spark discharge synthesis of amino acids using an atmosphere of CH4 + N2 + H2O + NH3 has been investigated with variable pNH3. The amino acids produced using higher hydrocarbons (ethane, ethylene, acetylene, propane, butane, and isobutane) instead of CH4 were also investigated. There was considerable range in the absolute yields of amino acids, but the yields relative to glycine (or alpha-amino-n-butyric acid) were more uniform. The relative yields of the C3 to C6 aliphatic alpha-amino acids are nearly the same (with a few exceptions) with all the hydrocarbons. The glycine yields are more variable. The precursors to the C3-C6 aliphatic amino acids seem to be produced in the same process, which is separate from the synthesis of glycine precursors. It may be possible to use these relative yields as a signature for a spark discharge synthesis provided corrections can be made for subsequent decomposition events (e.g. in the Murchison meteorite).

Acetylene↗

Prebiotic formation of 'energy-rich' thioesters from glyceraldehyde and N-acetylcysteine.

The 'energy-rich' thioester, N-acetyl-S-lactoylcysteine, is formed from low concentrations of glyceraldehyde and N-acetylcysteine under anaerobic conditions at ambient temperature in aqueous solutions of sodium phosphate (pH 7.0). Reactions with 2 mM glyceraldehyde, 2 mM N-acetylcysteine, and 500 mM sodium phosphate (pH 7.0) convert about 3%/day of the glyceraldehyde to lactoyl thioester. The formation of lactoyl thioester in similar reactions with 500 mM imidazole hydrochloride (pH 7.0) is supported by the thiol-dependence of lactate formation, which is 3-fold greater in the presence of thiol (0.11%/day) than in the absence of thiol (0.04%/day). The formation of lactoyl thioester is thought to proceed by the phosphate (or imidazole)-catalyzed dehydration of glyceraldehyde to give pyruvaldehyde, which adds to the thiol to form a hemithioacetal that rearranges to the thioester. A limited amount of a second thioester, N-acetyl-S-glyceroyl-cycsteine, is also formed at the beginning of these reactions. The significance of these reactions to the origin of life is discussed.

Acetylcysteine↗

pH profile of the adsorption of nucleotides onto montmorillonite. I. Selected homoionic clays.

The effect of adsorbed ions and pH on the adsorption of several purine and pyrimidine nucleotides on montmorillonite was studied. The cations used to prepare homoionic montmorillonite was Na+, Mn2+, Fe3+, Co2+, Ni+, Cu2+, and Zn2+. The nucleotides studied were 5'-,3'-, and 2'-AMP, and 5'-CMP in the pH range 2 through 12. The results show that preferential adsorption amongst nucleotides and similar molecules is dependent upon pH and the nature of the substituted metal cation in the clay. At neutral pH, it was observed that 5'-AMP was more strongly adsorbed than 2'AMP, 3'-AMP, and 5'-CMP. Cu2+ and Zn2+ clays showed enhanced adsorption of 5'-AMP compared to the other cation clays studied in the pH range 4-8. Below pH 4, the adsorption is attributed to cation and anion exchange adsorption mechanisms: above pH 4, anion exchange may also occur, but the adsorption (when it occurs) likely depends on a complexation mechanism occurring between metal cation in the clay exchange site the biomolecule. It is thus proposed that homoionic clays may have played a significant role in the concentration mechanism of biomonomers in the prebiotic environment, a prerequisite step necessary for the formation of biopolymers in the remaining steps leading to the origin of life.

Adenosine Monophosphate↗