Carbon and energy yields in prebiotic syntheses using atmospheres containing CH4, CO and CO2

Yields based on carbon are usually reported in prebiotic experiments, while energy yields (moles cal^–1) are more useful in estimating the yields of products that would have been obtained from the primitive atmosphere of the earth. Energy yields for the synthesis of HCN and H₂CO from a spark discharge were determined for various mixtures of CH₄, CO, CO₂, H₂, H₂O, N₂ and NH₃. The maximum yields of HCN and H₂CO from CH₄, CO, and CO₂ as carbon sources are about 4×10^–8 moles cal^–1.     

Nitrogen Fixation By Corona Discharge On The Early Precambrian Earth

We report the first experimental study of nitrogen fixation by corona discharge on the anoxic primitive Earth. The energy yields of nitric oxide (NO) and nitrous oxide (N₂O) were experimentally determined over a wide range of CO₂-N₂ mixtures simulating the evolution of the Earth's atmosphere during the Hadean and Archean eras (from 4.5 ba to 2.5 ba). NO, the principal form of fixed nitrogen in lightning and coronal discharge in early Earth, is produced ten times less efficiently in the latter type of electrical discharge with an estimated maximum annual production rate of the order of 10¹⁰ g yr⁻¹. For N₂O the maximum production rate was estimated to be ∼10⁹ g yr⁻¹. These low rates of syntheses indicate that corona discharges as point discharges on the clouds and ground did not play a significant role in the overall pool of reactive nitrogen needed for the emergence and sustainability of life.     

Carbon and energy yields in prebiotic syntheses using atmospheres containing CH4, CO and CO2

Yields based on carbon are usually reported in prebiotic experiments, while energy yields (moles cal-1) are more useful in estimating the yields of products that would have been obtained from the primitive atmosphere of the earth. Energy yields for the synthesis of HCN and H2CO from a spark discharge were determined for various mixtures of CH4, CO, CO2, H2, H2O, N2 and NH3. The maximum yields of HCN and H2CO from CH4, CO, and CO2 as carbon sources are about 4 X 10(-8) moles cal-1.     

Rates of fixation by lightning of carbon and nitrogen in possible primitive atmospheres

A thermochemical-hydrodynamic model of the production of trace species by electrical discharges has been used to estimate the rates of fixation of C and N by lightning in the primitive atmosphere. Calculations for various possible mixtures of CH₄, CO₂, N₂, H₂, and H₂O reveal that the prime species produced were probably HCN and NO and that the key parameter determining the rates of fixation was the ratio of C atoms to O atoms in the atmosphere. Atmospheres with C more abundant than O have large HCN fixation rates, in excess of 10¹⁷ molecules J^–1, but small NO yields. However, when O is more abundant than C, the NO fixation rate approaches 10¹⁷ molecules J^–1 while the HCN yield is small. The implications for the evolution of life are discussed.     

Quantum Yields of Decomposition and Homo-Dimerization of Solid <Emphasis Type="SmallCaps">L</Emphasis>-Alanine Induced by 7.2 eV Vacuum Ultraviolet Light Irradiation: An Estimate of the Half-Life of <Emphasis Type="SmallCaps">L</Emphasis>-Alanine on the Surface of Space Objects

One of the leading hypotheses regarding the origin of prebiotic molecules on primitive Earth is that they formed from inorganic molecules in extraterrestrial environments and were delivered by meteorites, space dust and comets. To evaluate the availability of extraterrestrial amino acids, it is necessary to examine their decomposition and oligomerization rates as induced by extraterrestrial energy sources, such as vacuum ultraviolet (VUV) and X-ray photons and high energy particles. This paper reports the quantum yields of decomposition ((8.2 ± 0.7) × 10⁻² photon⁻¹) and homo-dimerization ((1.2 ± 0.3) × 10⁻³ photon⁻¹) and decomposition of the dimer (0.24 ± 0.06 photon⁻¹) of solid l-alanine (Ala) induced by VUV light with an energy of 7.2 eV. Using these quantum yields, the half-life of l-Ala on the surface of a space object in the present earth orbit was estimated to be about 52 days, even when only photons with an energy of 7.2 eV emitted from the present Sun were considered. The actual half-life of solid l-Ala on the surface of a space object orbit around the present day Earth would certainly be much shorter than our estimate, because of the added effect of photons and particles of other energies. Thus, we propose that l-Ala needs to be shielded from solar VUV in protected environments, such as the interior of a meteorite, within a time scale of days after synthesis to ensure its arrival on the primitive Earth.     

Enhanced Synthesis of Alkyl Amino Acids in Miller’s 1958 H<Subscript>2</Subscript>S Experiment

Stanley Miller’s 1958 H₂S-containing experiment, which included a simulated prebiotic atmosphere of methane (CH₄), ammonia (NH₃), carbon dioxide (CO₂), and hydrogen sulfide (H₂S) produced several alkyl amino acids, including the α-, β-, and γ-isomers of aminobutyric acid (ABA) in greater relative yields than had previously been reported from his spark discharge experiments. In the presence of H₂S, aspartic and glutamic acids could yield alkyl amino acids via the formation of thioimide intermediates. Radical chemistry initiated by passing H₂S through a spark discharge could have also enhanced alkyl amino acid synthesis by generating alkyl radicals that can help form the aldehyde and ketone precursors to these amino acids. We propose mechanisms that may have influenced the synthesis of certain amino acids in localized environments rich in H₂S and lightning discharges, similar to conditions near volcanic systems on the early Earth, thus contributing to the prebiotic chemical inventory of the primordial Earth.     

Kinetics of CO conversion into H<Subscript>2</Subscript> by <Emphasis Type="Italic">Carboxydothermus hydrogenoformans</Emphasis>

The objective of this study was to improve the biological water–gas shift reaction for producing hydrogen (H₂) by conversion of carbon monoxide (CO) using an anaerobic thermophilic pure strain, Carboxydothermus hydrogenoformans. Specific hydrogen production rates and yields were investigated at initial biomass densities varying from 5 to 20 mg volatile suspended solid (VSS) L⁻¹. Results showed that the gas–liquid mass transfer limits the CO conversion rate at high biomass concentrations. At 100-rpm agitation and at CO partial pressure of 1 atm, the optimal substrate/biomass ratio must exceed 5 mol CO g⁻¹ biomass VSS in order to avoid gas–liquid substrate transfer limitation. An average H₂ yield of 94 ± 3% and a specific hydrogen production rate of ca. 3 mol g⁻¹ VSS day⁻¹ were obtained at initial biomass densities between 5 and 8 mg VSS⁻¹. In addition, CO bioconversion kinetics was assessed at CO partial pressure from 0.16 to 2 atm, corresponding to a dissolved CO concentration at 70°C from 0.09 to 1.1 mM. Specific bioactivity was maximal at 3.5 mol CO g⁻¹ VSS day⁻¹ for a dissolved CO concentration of 0.55 mM in the culture. This optimal concentration is higher than with most other hydrogenogenic carboxydotrophic species.     

The Effects of Ferrous and other Ions on the Abiotic Formation of Biomolecules using Aqueous Aerosols and Spark Discharges

It has been postulated that the oceans on early Earth had a salinity of 1.5 to 2 times the modern value and a pH between 4 and 10. Moreover, the presence of the banded iron formations shows that Fe⁺² was present in significant concentrations in the primitive oceans. Assuming the hypotheses above, in this work we explore the effects of Fe⁺² and other ions in the generation of biomolecules in prebiotic simulation experiments using spark discharges and aqueous aerosols. These aerosols have been prepared using different sources of Fe⁺², such as FeS, FeCl₂ and FeCO₃, and other salts (alkaline and alkaline earth chlorides and sodium bicarbonate at pH = 5.8). In all these experiments, we observed the formation of some amino acids, carboxylic acids and heterocycles, involved in biological processes. An interesting consequence of the presence of soluble Fe⁺² was the formation of Prussian Blue, Fe₄[Fe(CN)₆]₃, which has been suggested as a possible reservoir of HCN in the initial prebiotic conditions on the Earth.     

Production Of Low Molecular Weight Hydrocarbons By Volcanic Eruptions On Early Mars

Methane and other larger hydrocarbons have been proposed as possible greenhouse gases on early Mars. In this work we explore if volcanic processes may have been a source for such molecules based on theoretical and experimental considerations. Geologic evidence and numerical simulations indicate that explosive volcanism was widely distributed throughout Mars. Volcanic lightning is typically produced in such explosive volcanism. Therefore this geologic setting was studied to determine if lightning could be a source for hydrocarbons in volcanic plumes. Volcanic lightning was simulated by focusing a high-energy infrared laser beam inside of a Pyrex reactor that contained the proposed volcanic gas mixture composed of 64% CH₄, 24% H₂, 10% H₂O and 2% N₂, according to an accretion model and the nitrogen content measured in Martian meteorites. The analysis of products was performed by gas chromatography coupled to infrared and mass spectroscopy. Eleven hydrocarbons were identified among the products, of which acetylene (C₂H₂) was the most abundant. A thermochemical model was used to determine which hydrocarbons could arise only from volcanic heat. In this case, acetylene and ethylene are formed at magmatic temperatures. Our results indicate that explosive volcanism may have injected into the atmosphere of early Mars ∼6×10¹² g yr⁻¹ of acetylene, and ∼2×10¹² g yr⁻¹ of 1,3-butadiyne, both produced by volcanic lightning, ∼5×10¹¹ g yr⁻¹ of ethylene produced by volcanic heat, and 10¹³ g yr⁻¹ of methane.     

Nitric oxide,hydrogen cyanide and ethylene are required in the control of germination and undisturbed development of young apple seedlings

Reactive oxygen species (ROS) and reactive nitrogen species (RNS) are emerging as important regulators of plant development (germination, flowering, senescence), acting as secondary messengers in cooperation with classical phytohormones. Apple seeds are dormant, unless they undergo a 3 month long cold stratification. Deep dormancy of isolated apple embryos can also be broken by short pre-treatment with HCN or NO with the effect associated with enhanced ethylene synthesis. Non-dormant embryos germinate well and young seedlings grown from non-dormant embryos do not exhibit any morphological anomalies, such as asymmetric growth and greening of cotyledons. One of the aims of this work was to investigate the correlation between RNS- mediated (HCN- and NO-dependent) dormancy removal and ROS (H₂O₂ and O₂^−•) accumulation in the embryos. The beneficial effect of NO and HCN on germination of dormant apple embryos has been associated with marked increases in H₂O₂ and O₂^−• concentration in the embryos at early germination stages. We also analyzed growth of young seedlings developed from embryos pre-treatment with HCN or NO or exposed to ethylene (ethephone) and its precursor 1-aminocyclopropane-1-carboxylic acid (ACC). ACC and ethephone removed all morphological anomalies of the seedlings (asymmetric growth and greening of cotyledons) but the radicle growth was rather slight. We propose that accumulation of ROS provoked by HCN and NO pre-treatment is required for embryo germination “sensu stricto”, while ethylene is required for post-germination seedling growth.     

Biohydrogen production from carbon monoxide and water byRhodopseudomonas palustris P4

A reactor-scale hydrogen (H₂) productionvia the water-gas shift reaction of carbon monoxide (CO) and water was studied using the purple nonsulfur bacterium,Rhodopseudomonas palustris P4. The experiment was conducted in a two-step process: an aerobic/chemoheterotrophic cell growth step and a subsequent anaerobic H₂ production step. Important parameters investigated included the agitation speed, inlet CO concentration and gas retention time. P4 showed a stable H₂ production capability with a maximum activity of 41 mmol H₂ g cell⁻¹h⁻¹ during the continuous reactor operation of 400 h. The maximal volumetric H₂ production rate was estimated to be 41 mmol H₂ L¹h⁻¹, which was about nine-fold and fifteen-fold higher than the rates reported for the photosynthetic bacteriaRhodospirillum rubrum andRubrivivax gelatinosus, respectively. This is mainly attributed to the ability of P4 to grow to a high cell density with a high specific H₂ production activity. This study indicates that P4 has an outstanding potential for a continuous H₂ productionvia the water-gas shift reaction once a proper bioreactor system that provides a high rate of gas-liquid mass transfer is developed.     

Succinate is the controller of O<Stack><Subscript>2</Subscript><Superscript>−</Superscript></Stack>/H<Subscript>2</Subscript>O<Subscript>2</Subscript> release at mitochondrial complex I : negative modulation by malate,positive by cyanide

Mitochondrial production of H₂O₂ is low with NAD substrates (glutamate/pyruvate, 3 and 2 mM) (G/P) and increases over ten times upon further addition of succinate, with the formation of a sigmoidal curve (semimaximal value at 290 μM, maximal H₂O₂ production at 600 μM succinate). Malate counteracts rapidly the succinate induced increased H₂O₂ release and moves the succinate dependent H₂O₂ production curve to the right. Nitric oxide (NO) and carbon monoxide (CO) are cytochrome c oxidase inhibitors which increase mitochondrial ROS production. Cyanide (CN⁻) was used to mimic NO and CO. In the presence of G/P and succinate (300 μM), CN⁻ progressively increased the H₂O₂ release rate, starting at 1.5 μM. The succinate dependent H₂O₂ production curve was moved to the left by 30 μM CN⁻. The V_max was little modified. We conclude that succinate is the controller of mitochondrial H₂O₂ production, modulated by malate and CN⁻. We propose that succinate promotes an interaction between Complex II and Complex I, which activates O₂⁻ production.     

H<Subscript>2</Subscript> enrichment from synthesis gas by <Emphasis Type="Italic">Desulfotomaculum</Emphasis><Emphasis Type="Italic">carboxydivorans</Emphasis> for potential applications in synthesis gas purification and biodesulfurization

Desulfotomaculum carboxydivorans, recently isolated from a full-scale anaerobic wastewater treatment facility, is a sulfate reducer capable of hydrogenogenic growth on carbon monoxide (CO). In the presence of sulfate, the hydrogen formed is used for sulfate reduction. The organism grows rapidly at 200 kPa CO, pH 7.0, and 55°C, with a generation time of 100 min, producing nearly equimolar amounts of H₂ and CO₂ from CO and H₂O. The high specific CO conversion rates, exceeding 0.8 mol CO (g protein)⁻¹ h⁻¹, makes this bacterium an interesting candidate for a biological alternative of the currently employed chemical catalytic water–gas shift reaction to purify synthesis gas (contains mainly H₂, CO, and CO₂). Furthermore, as D. carboxydivorans is capable of hydrogenotrophic sulfate reduction at partial CO pressures exceeding 100 kPa, it is also a good candidate for biodesulfurization processes using synthesis gas as electron donor at elevated temperatures, e.g., in biological flue gas desulfurization. Although high maximal specific sulfate reduction rates (32 mmol (g protein)⁻¹ h⁻¹) can be obtained, its sulfide tolerance is rather low and pH dependent, i.e., maximally 9 and 5 mM sulfide at pH 7.2 and pH 6.5, respectively.     

Enantiodifferent Proton Exchange in Alanine and Asparagine in the Presence of H 2 17 O

Using Time Domain ¹H Nuclear Magnetic Resonance with H₂¹⁷O (H₂¹⁷O-TD-¹HNMR), we found [H₂¹⁷O]- and pH-controlled chiral differences in proton exchange properties in alanine (Ala) and asparagine (Asn). To minimize and equalize chemical impurities, Asn enantiomers were purified by crystallization from racemic solution. At <0.1 M H₂¹⁷O, a shift in isoelectric pH (pI) occurred, ~1.14 kJ mol⁻¹ l-d-Asn ΔΔG ^o′ in the 5.91–6.42 pH range. One potential source for this asymmetry is the enantio-different magnetic moments (lμ↑ ≠ dμ↓) produced by neutral ring currents in the chiral center, leading to enantio-different nuclear spin organization and charge distribution in the amino group. At ≥pI, dissimilar interactions may occur in the hydration of the amino group with H₂¹⁷O (NH₂/H₂¹⁷O ≠ NH₂/H₂¹⁶O; NH₃ ⁺/H₂¹⁷O ≠ NH₂/H₂¹⁷O; l-*C-NH₂/H₂¹⁷O ≠ d-*C-NH₂/H₂¹⁷O). As lμ↑ ≠ dμ↓, the l-*C-amino and the d-*C-amino groups are diastereo spin-isomers. The nuclear spin of ¹⁷O may be parallel or antiparallel with the ortho-¹H¹H pair; hence two ortho-H₂¹⁷O molecules exist, also diastereo spin-isomers. As the pK of H₂¹⁷O is different from H₂¹⁶O, dissimilarities between l-*C- and d-*C-amino groups are converted into proton exchange differences. During H₂¹⁷O-TD-¹HNMR, the H₂¹⁷O molecule is a “probe” of the state of the amino group. Regarding prebiotic evolution: prebiotic chirality may not require stochastic symmetry breaking or preexisting chiral conditions; chemical chiral effects due to lμ↑ ≠ dμ↓ are small and need chiral amplification to generate an enantiomeric excess significant for prebiotic evolution; and prebiotic symmetry breaking was homochiral because the effect of lμ↑ and dμ↓ on the amino group should be similar in all alpha amino acids.     

Electrical energy sources for organic synthesis on the early earth

In 1959, Miller and Urey (Science 130, 245) published their classic compilation of energy sources for indigenous prebiotic organic synthesis on the early Earth. Much contemporary origins of life research continues to employ their original estimates for terrestrial energy dissipation by lightning and coronal discharges, 2 × 10¹⁹ J yr^–1 and 6 × 10¹⁹ J yr^–1, respectively. However, more recent work in terrestrial lightning and point discharge research suggests that these values are overestimates by factors of about 20 and 120, respectively. Calculated concentrations of amino acids (or other prebiotic organic products) in the early terrestrial oceans due to electrical discharge sources may therefore have been equally overestimated. A review of efficiencies for those experiments that provide good analogues to naturally-occurring lightning and coronal discharges suggests that lightning energy yields for organic synthesis (nmole J^–1) are about one order of magnitude higher than those for coronal discharge. Therefore organic production by lightning may be expected to have dominated that due to coronae on early Earth. Limited data available for production of nitric oxide in clouds suggests that coronal emission within clouds, a source of energy heretofore too uncertain to be included in the total coronal energy inventory, is insufficient to change this conclusion. Our recommended valves for lightning and coronal discharge dissipation rates on the early Earth are, respectively, 1 × 10¹⁸ J yr^–1 and 5 × 10¹⁷ J yr^–1.     

Time- and space-resolved Monte Carlo study of water radiolysis for photon,electron and ion irradiation

Time-dependent yields of the most important products of water radiolysis , ^•OH, H^•, H₃O⁺, H₂, OH⁻ and H₂O₂ have been calculated for ⁶⁰Co-photons, electrons, protons, helium- and carbon-ions incident onto water. G values have been evaluated for the interval from 1 ps to 1 μs after initial energy deposition as a function of time, as well as after 1 ns and at the end of the chemical stage as a function of linear energy transfer (LET), covering an interval from approximately 0.2 up to 750 keV/μm by means of different particle types. In this work, the modules of the biophysical Monte Carlo track structure code PARTRAC dealing with the simulation of prechemical and chemical stages have been improved to extend interaction data sets for heavier ions. Among other newly selected parameter values, the thermalisation distance between the point of generation and hydration of subexcitation electrons has been adopted from recent data in the literature. As far as data from the literature are available, good agreement has been found with the calculated time- and LET-dependent yields in this work, supporting the selection of the revised parameter values.     

A Monte-Carlo step-by-step simulation code of the non-homogeneous chemistry of the radiolysis of water and aqueous solutions—Part II: calculation of radiolytic yields under different conditions of LET,pH, and temperature

The importance of the radiolysis of water in the initial events following irradiation of biological systems has motivated considerable theoretical and experimental work in the field of radiation chemistry of water and aqueous systems. These studies include Monte-Carlo simulations of the radiation track structure and of the non-homogeneous chemical stage, which have been successfully used to calculate the yields of radiolytic species (H^·, ^·OH, H₂, H₂O₂, e_aq⁻, …). Most techniques used for the simulation of the non-homogeneous chemical stage such as the independent reaction time (IRT) technique and diffusion kinetics methods do not calculate the time evolution of the positions of the radiolytic species. This is a major limitation to their extension to the simulation of the irradiation of radiobiological systems. Step-by-step (SBS) simulation programs provide such information, but they are very demanding in term of computer power and storage capacity. Recent improvements in computer performance now allow the regular use of the SBS method in radiation chemistry simulations. In the first of a series of two papers, the SBS method has been reviewed in details and the implementation of a SBS code has been discussed. In this second paper, the results of several studies are presented: (1) the time evolution of the radiolytic yields from the formation of the radiation track to 10⁻⁶ s; (2) the effect of pH on yields (pH ~ 0.4–7.0); (3) the effect of proton energy (and LET) on yields (300 MeV-0.1 MeV), and iv) the effect of the ion type (¹H⁺, ⁴He²⁺, ¹²C⁶⁺) on yields. Nonbiological applications, i.e., the study of the temperature on the yields (about 25–300°C) and the simulation of the time evolution of G(Fe³⁺) in the Fricke dosimeter are also discussed.     

Actual and potential rates of hydrogen photoproduction by continuous culture of the purple non-sulphur bacterium Rhodobacter capsulatus

The influence of (NH₄)₂SO₄ concentration and dilution rate (D) on actual and potential H₂ photoproduction has been studied in ammonium-limited chemostat cultures of Rhodobacter capsulatus B10. The actual H₂ production in a photobioreactor was maximal (approx. 80 ml h⁻¹l⁻¹) at D = 0.06 h⁻¹ and 4 mM (NH₄)₂SO₄. However, it was lower than the potential H₂ evolution (calculated from hydrogen evolution rates in incubation vials), which amounted to 100–120 ml h⁻¹ l⁻¹ at D = 0.03–0.08 h⁻¹. Taking into account the fact that H₂ production in the photobioreactor under these conditions was not limited by light or lactate, another limiting (inhibiting) factor should be sought. One possibility is an inhibition of H₂ production by the H₂ accumulated in the gas phase. This is apparent from the non-linear kinetics of H₂ evolution in the vials or from its inhibition by the addition of H₂; initial rates were restored in both cases after the vials had been refilled with argon. The actual H₂ production in the photobioreactor at D = 0.06 h⁻¹ was shown to increase from approximately 80 ml h⁻¹ l⁻¹ to approximately 100 ml h⁻¹ l⁻¹ under an argon flow at 100 ml min⁻¹. Under maximal H₂ production rates in the photobioreactor, up to 30% of the lactate feedstock was utilised for H₂ production and 50% for biomass synthesis. Received: 22 April 1997 / Received revision: 14 July 1997 / Accepted: 27 July 1997     

Carbonylation and other metal-catalysed C?C coupling reactions used in industry

The formation of new carbon-carbon bonds is probably the most fundamental reaction in organic chemistry. Many of the most selective and energy efficient reactions today involve the use of metals and their complexes as promoters. Key routes to C−C bond formation involve carbonylation (using CO) and coupling reactions (of olefins, dienes, and arenes) following an activation step. The largest carbonylation reactions in volume terms are the hydrogenation of CO, to make long chain hydrocarbons for diesel fuel (over supported Fe, Co, Ru or Rh metal catalysts; the Fischer-Tropsch reaction) or, over a Cu−ZnO catalyst, to make methanol. Many of the important carbonylations are homogeneously catalysed, using soluble complexes of the late transition metals, such as Co, Rh, Ir, or Pd. The carbonylation of methanol to acetic acid, MeOH+CO→MeCOOH was originally developed using a Co/I⁻ catalyst; improvements in conditions (better energy use and selectivity), led by mechanistic considerations resulted in, first the Rh/I⁻ (Monsanto) and more recently, the Ir/I⁻ (BP, Cativa) processes. The hydroformylation of olefins,e.g., MeCH=CH₂+H₂+CO→MeCH₂CH₂CHO+MeCH(CHO)CH₃ was also originally developed using a soluble cobalt catalyst, but again the use of rhodium catalysts (bearing phosphine ligands) has largely superseded the older processes. Even newer technologies, for example involvingsupported homogeneous catalysts, now promise still cleaner and more selective processes. Direct coupling reactions include Friedel-Crafts type processes, for example, C₆H₆+CH₂=CHR→C₆H₅−C₂H₄R Zeolites are now the strong acid catalysts employed heterogeneously rather than the previously used AlCl₃ or HF; the new catalysts are much more environmentally friendly (?greener?) as they do not involve halides which cause corrosion and undesirable side reactions. Valuable highly selective reactions include the Cr-catalysed oligomerization of ethylene to 1-hexene or 1-octene, and of butadiene to cyclo-octadiene or cyclo-dodecatriene, over Ni catalysts. Palladium catalysed coupling and carbonylation reactions have made key steps much more environmentally acceptable in the syntheses of the important anti-inflammatory pharmaceuticalsibuprofen andnaproxen.

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Riassunto   Carbonilazione ed altri accoppiamenti C−C catalizzati da metalli impiegati nell'industria. La formazione di nuovi legami carbonio-carbonio è forse la reazione più fondamentale in chimica organica. Molte delle reazioni più selettive ed energeticamente efficienti implicano oggi l'impiego di metalli e loro complessi come promotori. Le vie chiave per la formazione di legami C−C sono la carbonilazione (mediante CO) e le reazioni di accoppiamento (di olefine, dieni ed areni) precedute da uno stadio di attivazione. Le maggiori reazioni di carbonilazione in termini di volume sono l'idrogenazione del CO per la produzione di idrocarburi a lunga catena destinati all'impiego come combustibili Diesel (su catalizzatiri metallici supportati a base di Fe, Co, Ru o Rh; reazione di Fischer-Tropsch) o di metanolo su catalizzatore Cu−ZnO. Molte tra le più importanti carbonilazioni avvengono su catalizzatori in fase omogenea costituiti da complessi solubili di metalli alla fine di una serie di transizione come Co, Rh, Ir e Pd. La carbonilazione del metanolo ad acido acetico MeOH+CO→MeCOOH venne originariamente sviluppata usando un catalizzatore Co/I⁻; il miglioramento delle condizioni (miglior uso dell'energia e maggior selettività) sulla base di considerazioni meccanicistiche condusse in un primo tempo al catalizzatore Rh/I⁻ (processo Monsanto) e più recentemente al catalizzatore Ir/I⁻ (processo BP, Cativa). L'idroformilazione delle olefine, per esempio: MeCH=CH₂+H₂+CO→MeCH₂CH₂CHO+MeCH(CHO)CH₃ venne anch'essa sviluppata originariamente usando un complesso solubile del cobalto, ma di nuovo l'uso dei catalizzatori a base di rodio (contenenti leganti fosfinici) ha largamente superato i processi più vecchi. Anche le nuove technologie basate su catalizzatori omogenei supportati promettono ora processi ancora più puliti e selettivi. Le reazioni di accoppiamento diretto comprendono i processi di tipo Friedel-Crafts, per esempio: C₆H₆+CH₂=CHR→C₆H₅−C₂H₄R. Le zeoliti rappresentano ora i catalizzatori fortemente acidi impiegati in fase etrogenea al posto di AlCl₃ od HF usati in precedenza; i nuovi catalizzatori sono molto più compatibili ambientalmente (?più verdi?) in quanto non contengono alogenuri che possono provocare corrosioni ed altre reazioni secondarie non desiderate. Pregevoli reazioni ad alta selettività comprendono l'oligomerizzazione dell'etilene ad 1-esene od 1-ottene catalizzata dal cromo o del butadiene a cicloottadiene o ciclododecatriene catalizzata dal nichel. Attraverso reazioni di accoppiamento e carbonilazione catalizzate dal palladio sono stati realizzati passaggi chiave molto più accettabili ambientalmente nella sintesi degli importanti composti farmaceuticiibuprofen enaproxen.

     

Intracellular pH regulation and buffer capacity in CO2/HCO− 3-buffered media in cultured epithelial cells from rainbow trout gills

The influence of a CO₂/HCO⁻ ₃-buffered medium on intracellular pH regulation of gill pavement cells from freshwater rainbow trout was examined in monolayers grown in primary culture on glass coverslips; intracellular pH (pH_i) was monitored by continuous spectrofluorometric recording from cells loaded with 2′,7′-bis(2-carboxyethyl)-5(6)-carboxy-fluoroscein. When cells in HEPES-buffered medium at normal pH=7.70 were transferred to normal CO₂/HCO⁻ ₃-buffered medium {P _CO2=3.71 mmHg, [HCO⁻ ₃]= 6.1 mmol l⁻¹, extracellular pH (pH_e)=7.70}, they exhibited a brief acidosis but subsequently regulated the same pHi (∼7.41) as in HEPES. Buffer capacity (β) increased by the expected amount (5.5–8.0 slykes) based on intracellular [HCO⁻ ₃], and was unaffected by most drugs and treatments. However, after transfer to high P _CO2=11.15 mmHg, [HCO⁻ ₃]= 18.2 mmol l⁻¹ at the same pH_e=7.70, the final regulated pHi was elevated (∼7.53). The rate of correction of alkalosis caused by washout of this high P _CO2, high-HCO⁻ ₃ medium was unaffected by removal of extracellular Cl⁻. Removal of extracellular Na⁺ lowered resting pH_i and greatly inhibited the rate of pH_i recovery from acidosis. Bafilomycin A₁ (3 μmol l⁻¹) had no effect on these responses. However amiloride (0.2 mmol l⁻¹) inhibited recovery from acidosis caused by washout of an ammonia prepulse, but did not affect resting pH_i, the latter differing from the response in HEPES where amiloride also lowered resting pH_i. Similarly 4-acetamido-4′- isothiocyanatostilbene-2,2′-disulfonic acid, sodium salt (0.1 mmol l⁻¹) did not affect resting pH_i but slowed the rate of recovery from acidosis, though to a lesser extent than amiloride. Removal of extracellular Cl⁻ also slowed the rate of recovery but greatly increased β by an unknown mechanism; when this was taken into account, H⁺ extrusion rate was unaffected. These results are consistent with the presence of Na⁺-(HCO⁻ ₃)_N co-transport and/or Na⁺-dependent HCO⁻ ₃/Cl⁻ exchange, in addition to Na⁺/H⁺ exchange, as mechanisms contributing to “housekeeping” pH_i regulation in gill cells in CO₂/HCO⁻ ₃ media, whereas only Na⁺/H⁺ exchange is seen in HEPES. Both Na⁺-independent Cl⁻/HCO⁻ ₃ exchange and V-type H⁺-ATPase mechanisms appear to be absent from these cells cultured in isotonic media. Accepted: 30 November 1999