Hydrogen Cyanide Production due to Mid-Size Impacts in a Redox-Neutral N2-Rich Atmosphere

Cyanide compounds are amongst the most important molecules of the origin of life. Here, we demonstrate the importance of mid-size (0.1–1 km in diameter) hence frequent meteoritic impacts to the cyanide inventory on the early Earth. Subsequent aerodynamic ablation and chemical reactions with the ambient atmosphere after oblique impacts were investigated by both impact and laser experiments. A polycarbonate projectile and graphite were used as laboratory analogs of meteoritic organic matter. Spectroscopic observations of impact-generated ablation vapors show that laser irradiation to graphite within an N₂-rich gas can produce a thermodynamic environment similar to that produced by oblique impacts. Thus, laser ablation was used to investigate the final chemical products after this aerodynamic process. We found that a significant fraction (>0.1 mol%) of the vaporized carbon is converted to HCN and cyanide condensates, even when the ambient gas contains as much as a few hundred mbar of CO₂. As such, the column density of cyanides after carbon-rich meteoritic impacts with diameters of 600 m would reach ~10 mol/m² over ~10² km² under early Earth conditions. Such a temporally and spatially concentrated supply of cyanides may have played an important role in the origin of life.     

Photosynthesis in the Archean Era

The earliest reductant for photosynthesis may have been H₂. The carbon isotope composition measured in graphite from the 3.8-Ga Isua Supercrustal Belt in Greenland is attributed to H₂-driven photosynthesis, rather than to oxygenic photosynthesis as there would have been no evolutionary pressure for oxygenic photosynthesis in the presence of H₂. Anoxygenic photosynthesis may also be responsible for the filamentous mats found in the 3.4-Ga Buck Reef Chert in South Africa. Another early reductant was probably H₂S. Eventually the supply of H₂ in the atmosphere was likely to have been attenuated by the production of CH₄ by methanogens, and the supply of H₂S was likely to have been restricted to special environments near volcanos. Evaporites, possible stromatolites, and possible microfossils found in the 3.5-Ga Warrawoona Megasequence in Australia are attributed to sulfur-driven photosynthesis. Proteobacteria and protocyanobacteria are assumed to have evolved to use ferrous iron as reductant sometime around 3.0 Ga or earlier. This type of photosynthesis could have produced banded iron formations similar to those produced by oxygenic photosynthesis. Microfossils, stromatolites, and chemical biomarkers in Australia and South Africa show that cyanobacteria containing chlorophyll a and carrying out oxygenic photosynthesis appeared by 2.8 Ga, but the oxygen level in the atmosphere did not begin to increase until about 2.3 Ga.     

Additional criterion for the determination of the handedness of 21 helices in crystals of bile acids: Crystal structure of a tert‐butylphenyl derivative of cholic acid

[3β,5β,7α,12α]‐3‐(4‐t‐Butylbenzoilamine)‐7,12‐dihydroxycholan‐24‐oic acid was synthesized and recrystallized from chlorobenzene and acetone. Orthorhombic P2₁2₁2₁ and monoclinic P2₁ crystals were obtained, respectively, and both crystals include solvent and water molecules with a 1:1:1 stoichiometry. In the second case, there are two nonequivalent molecules of the steroid in the unit cell. In both crystals, a crossing structure results for the molecular packing, stabilized by hydrogen bonds between the steroid molecules. In the second crystal, water links steroid molecules of the same type, which are not directly connected through hydrogen bonds. The steroid molecules define helicoidal assemblies along 2₁ screw axes. The handedness in the crystal in chlorobenzene is unambiguously defined by following the criterion proposed by Miyata et al., as the steroids are in a belly‐to‐belly disposition around the axis. This motif does not appear in the crystal in acetone, and other criterion is required. On the basis of the fact that a staircase and its banister have the same handedness and using the crystal in chlorobenzene as reference, the additional criterion has been established. According to it, in the absence of a belly‐to‐belly orientation, the handedness must be defined by keeping the bile acid with its right side oriented toward the axis. Pitch angles of the helices and tilt angles of the molecules are also determined. Chirality, 2011. © 2011 Wiley‐Liss, Inc.     

Mineral Radioactivity in Sands as a Mechanism for Fixation of Organic Carbon on the Early Earth

Irradiation of organic molecules by mineral radioactivity is a feasible alternative to cosmic irradiation to precipitate solid organic carbon-rich matter on the early Earth. Radioactive (uranium- and thorium-rich) minerals have been concentrated at the Earth's surface, and accumulated accretionary coatings of carbon due to irradiation, since early Archean times. The organic accretion process could have occurred at the surface or in the sub-surface, and is independent of a terrestrial or extraterrestrial source for the carbon.     

Extended High Circular Polarization in the Orion Massive Star Forming Region: Implications for the Origin of Homochirality in the Solar System

We present a wide-field (∼6′ × 6′) and deep near-infrared (K _s band: 2.14 μm) circular polarization image in the Orion nebula, where massive stars and many low-mass stars are forming. Our results reveal that a high circular polarization region is spatially extended (∼0.4 pc) around the massive star-forming region, the BN/KL nebula. However, other regions, including the linearly polarized Orion bar, show no significant circular polarization. Most of the low-mass young stars do not show detectable extended structure in either linear or circular polarization, in contrast to the BN/KL nebula. If our solar system formed in a massive star-forming region and was irradiated by net circularly polarized radiation, then enantiomeric excesses could have been induced, through asymmetric photochemistry, in the parent bodies of the meteorites and subsequently delivered to Earth. These could then have played a role in the development of biological homochirality on Earth.     

Effect of Pyrolysis Temperature on Chemical and Surface Properties of Biochar of Rapeseed (Brassica napus L.)

The biochar is an important carbon-rich product that is generated from biomass sources through pyrolysis. Biochar (charcoal) can be both used directly as a potential source of solid biofuels and as soil amendments for barren lands. The aim of this study was investigate influence of pyrolysis temperature on the physicochemical properties and structure of biochar. The biochars were produced by pyrolysis of rapeseed (Brassica napus L.) using a fixed-bed reactor at different pyrolysis temperatures (400–700°C). The produced biochars were characterized by proximate and elemental analysis, Brunauer–Emmett–Teller (BET) surface area, particle size distributions, scanning electron microscopy (SEM), Fourier transform infrared (FTIR) spectroscopy. The results showed that both chemical and surface properties of the biochars were significantly affected by the pyrolysis temperature. Aromatic hydrocarbons, hydroxyl and carbonyl compounds were the majority components of the biochar. The biochar obtained at 700°C had a high fixed carbon content (66.16%) as well as a high heating value, and therefore it could be used as solid fuel, precursor in the activated carbons manufacture (specific surface area until 25.38 m² g^?1), or to obtain category-A briquettes.     

Catalytic reactions in the solar nebula: Implications for interstellar molecules and organic compounds in meteorites

Organic compounds in meteorites seem to have formed by Fischer-Tropsch-type, catalytic reactions of CO, H₂, and NH₃ in the solar nebula, at 360–400K and (4–10)×10^–6 atm. The onset of these reactions was triggered by the formation of catalytically active grains of magnetite and serpentine at these temperatures.Laboratory experiments show that the Fischer-Tropsch reaction gives a large kineticisotope fractionation of C¹²/C¹³, duplicating the hitherto unexplained fractionation in meteorites. All of the principal compound classes in meteorites are produced by this reaction, or a variant involving a brief excursion to higher temperatures. (1) normal, mono-, and dimethylalkanes (2)arenes andalkylarenes; (3) dimericisoprenoids from C₉ to C₁₄; (4)purines andpyrimidines, such as adenine, guanine, uracil, thymine, xanthine, etc.; (5)amino acids, including tyrosine and histidine; (6)porphyrin-like pigments; (7) aromaticpolymer with –OH and –COOH groups.These reactions may also have played a major role in the evolution of life: first, by converting carbon to a sufficiently non-volatile form to permit its accretion by the inner planets; second, by synthesizing organic compounds on the primitive planets whenever CO, H₂, NH₃, and clay or magnetite particles came together at the right temperature. Similar reactions in other solar nebulae may be the source of interstellar molecules, as first suggested by G. H. Herbig. Ten of the twelve polyatomic interstellar molecules have in fact been seen in these syntheses or in meteorites.This paper is a revised and abridged version of the author's article inScience 182 (1973), 781.     

Production of poly(3-hydroxyalkanoates) by a bacterium of the genus Alcaligenes utilizing long-chain fatty acids

Summary The synthesis of poly(3-hydroxyalkanoates) [P(3HA)] by a new Alcaligenes species was investigated. The new species was grown on various carbon sources such as n-alkanoic acids of carbon numbers ranging from C₂ to C₂₂, plant oils and animal fats, and accumulated P(3HA) within the cells. When the bacterium was cultured in mineral media containing sodium salts of n-alkanoic acids, the homopolymer of poly(3-hydroxybutyrate) [P(3HB)] was produced from n-alkanoates of even carbon numbers, whereas the copolymer of 3-hydroxybutyrate and 3-hydroxyvalerate units [P(3HB-co-3HV)] was produced from n-alkanoates of odd carbon numbers. Relatively high yields of both dry cells and P(3HA) were obtained by the use of n-alkanoates from C₁₂ to C₁₆ as the sole carbon source. Correspondence to: Y. Doi     

Sulphur oxidation by a Streptomyces sp. growing in a carbon-deficient medium and autoclaved soil

Streptomyces colonies, apparently all of the same species, were isolated from a range of soils using a polysulphide medium lacking an organic carbon source. Growth on this medium, and clearing of the otherwise white, opaque overlay, suggested that the organisms were capable of growing autotrophically. However, investigation of one of these isolates showed that it was unable to fix ¹⁴CO₂ and did not possess the enzyme ribulose bisphosphate carboxylase, showing that it was incapable of autotrophic growth. The isolate oxidized elemental sulphur, thiosulphate and tetrathionate to sulphate in vitro in carbon-deficient medium, and also oxidized elemental sulphur to sulphate when inoculated into autoclaved soil supplemented with sulphur. It also oxidized polysulphide when growing on Czapek Dox and plate count agars. The isolate can therefore grow heterotrophically in both carbon-rich media and in media lacking organic carbon — presumably by scavenging organic carbon from the laboratory atmosphere. The possible role of these organisms in sulphur oxidation in soils is commented upon.     

Overview of the physiological ecology of carbon metabolism in seagrasses

The small but diverse group of angiosperms known as seagrasses form submersed meadow communities that are among the most productive on earth. Seagrasses are frequently light-limited and, despite access to carbon-rich seawaters, they may also sustain periodic internal carbon limitation. They have been regarded as C3 plants, but many species appear to be C3–C4 intermediates and/or have various carbon-concentrating mechanisms to aid the Rubisco enzyme in carbon acquisition. Photorespiration can occur as a C loss process that may protect photosynthetic electron transport during periods of low CO₂ availability and high light intensity. Seagrasses can also become photoinhibited in high light (generally>1000 μE m⁻² s⁻¹) as a protective mechanism that allows excessive light energy to be dissipated as heat. Many photosynthesis–irradiance curves have been developed to assess light levels needed for seagrass growth. However, most available data (e.g. compensation irradiance I_c) do not account for belowground tissue respiration and, thus, are of limited use in assessing the whole-plant carbon balance across light gradients. Caution is recommended in use of I_k (saturating irradiance for photosynthesis), since seagrass photosynthesis commonly increases under higher light intensities than I_k; and in estimating seagrass productivity from H_sat (duration of daily light period when light equals or exceeds I_k) which varies considerably among species and sites, and which fails to account for light-limited photosynthesis at light levels less than I_k. The dominant storage carbohydrate in seagrasses is sucrose (primarily stored in rhizomes), which generally forms more than 90% of the total soluble carbohydrate pool. Seagrasses with high I_c levels (suggesting lower efficiency in C acquisition) have relatively low levels of leaf carbohydrates. Sucrose-P synthase (SPS, involved in sucrose synthesis) activity increases with leaf age, consistent with leaf maturation from carbon sink to source. Unlike terrestrial plants, SPS apparently is not light-activated, and is positively influenced by increasing temperature and salinity. This response may indicate an osmotic adjustment in marine angiosperms, analogous to increased SPS activity as a cryoprotectant response in terrestrial non-halophytic plants. Sucrose synthase (SS, involved in sucrose metabolism and degradation in sink tissues) of both above- and belowground tissues decreases with tissue age. In belowground tissues, SS activity increases under low oxygen availability and with increasing temperatures, likely indicating increased metabolic carbohydrate demand. Respiration in seagrasses is primarily influenced by temperature and, in belowground tissues, by oxygen availability. Aboveground tissues (involved in C assimilation and other energy-costly processes) generally have higher respiration rates than belowground (mostly storage) tissues. Respiration rates increase with increasing temperature (in excess of 40°C) and increasing water-column nitrate enrichment (Z. marina), which may help to supply the energy and carbon needed to assimilate and reduce nitrate. Seagrasses translocate oxygen from photosynthesizing leaves to belowground tissues for aerobic respiration. During darkness or extended periods of low light, belowground tissues can sustain extended anerobiosis. Documented alternate fermentation pathways have yielded high alanine, a metabolic ‘strategy’ that would depress production of the more toxic product ethanol, while conserving carbon skeletons and assimilated nitrogen. In comparison to the wealth of information available for terrestrial plants, little is known about the physiological ecology of seagrasses in carbon acquisition and metabolism. Many aspects of their carbon metabolism — controls by interactive environmental factors; and the role of carbon metabolism in salt tolerance, growth under resource-limited conditions, and survival through periods of dormancy — remain to be resolved as directions in future research. Such research will strengthen the understanding needed to improve management and protection of these environmentally important marine angiosperms.     

What factors are responsible for the greater yield of ATP per carbon atom when fatty acids are completely oxidised to CO2 and water compared with glucose?

Some current textbooks of biochemistry present calculations which indicate that when palmitic or stearic acid is completely oxidised to CO₂ and water, more molecules of ATP are produced per carbon atom than when glucose is similarly oxidised. This greater yield of ATP is not due to ATP produced as a result of the β-oxidative process, but rather due to the increased yield of acetyl-CoA molecules produced from fatty acids (3 acetyl-CoA molecules per 6 carbon atoms) compared with that produced from glucose (2 acetyl-CoA molecules per 6 carbon atoms).     

Preferential solvation and association constants of 2-exo and 2-endo norbornyl chlorides in water–acetone mixtures

Molecular dynamics simulations of 2-exo and 2-endo norbornyl chlorides are performed in water–acetone mixtures to investigate the role of preferential solvation on the dissociation process of norbornyl chlorides. Increase in the association constants between carbon (C2) and chloride (Cl) of norbornyl chlorides with an increase in mole fraction of acetone supports the experimental data for the corresponding decrease in the rates of solvolysis for both exo and endo norbornyl chlorides. When the mole fraction of water is increased in water–acetone mixtures, acetone molecules are replaced by water molecules around C2 as well as Cl of norbornyl chloride. Preferential solvation by water is analysed using running coordination numbers and excess coordination numbers around C2 and Cl.     

Biochemical complexity of serum HLA class I molecules

Human serum was found to contain a variety of class I-like molecules by Western blotting with anti-class I heavy chain reagents: major bands usually are observed around M _r 44 000, 40 000, and 35 000–37 000. HLA-A24-positive individuals are distinguished by higher serum levels of M _r 44 000 and 40 000 class I-like molecules than those found in HLA-A24-negative individuals. The M _r 44 000 serum molecules are probably intact class I molecules that have been shed from the cell membrane, because they contain both a transmembrane segment (TM), as deduced from detergent-binding experiments, and a cytoplasmic tail (CT), as inferred from reactivity with an antipeptide serum specific for the cytoplasmic domain of class I antigens (RaCT). The M _r 35 000 and 37 000 molecules contain neither a TM nor a CT region and therefore are probably proteolytic breakdown products of cellular and/or serum M _r 44 000 molecules, although the existence of Q10-like molecules in man cannot be ruled out. The M _r 40 000 molecules do not contain a TM region. M _r 40 000 molecules reactive with the RaCT serum were found in the minority (2/13) of sera tested. We conclude that alternative splicing resulting in a precise excision of the TM exon plays a minor role in the generation of serum HLA class I antigens.Abbreviations used in this paper B2m beta-2 microglobulin - BSA bovine serum albumin - EBV-BLCL Epstein-Barr virus-transformed B lymphoblastoid cell line - mAb monoclonal antibody - SDS-PAGE sodium dodecyl sulfate-polyacrylamide gel electrophoresis - TCA trichloroacetic acid     

Towards an explanation of carboxylation/oxygenation bifunctionality in Rubisco. Transition structure for the carboxylation reaction of 2,3,4-pentanetriol

We construct a theoretical model of the transition structure for the carboxylation reaction of ribulose-1,5-biphosphate catalyzed by Rubisco. This is a first-order saddle point on the energy hypersurface for the nucleophilic attack of carbon dioxide on CH₃-(CHOH)₃-CH₃ at the C2 center.Ab initio analytical gradients methods at a 4-31G basis set level are used.The carbon framework and oxygens of the stationary structure superpose with the corresponding atoms of 2-carboxyarabinitol-1,5-biphosphate, which is a transition state analog that has recently been highly refined with X-ray methods. The hydroxyl group in C3 iscis to the C2 oxygen. The C3 center is somewhat pyramidized, the dienol O2-C2-C3-O3 is not planar.The geometry of the transition state allows for simple explanations of both the enolization of Rubisco's substrate ribulose-1,5-biphosphate, O₃PO-CH2-CO-(CHOH)₂-CH₂-OPO₃ and oxygenation reaction. The former is due to the pyramidal deformation at C3 and out of plane of O2-C2-C3-O3 framework: the enoliation is intramolecular and is probably enhanced by proton tunnelling. The latter is related with the fact that a rotation around an ethylene-like bond brings the triplet state down in energy. The reactive skeleton has a stationary geometry in the triplet state not very different from the one obtained in the global transition structure. There, the triplet is only 9 kcal/mol above the singlet. The spin densities at C2 and C3 centers clearly indicate the place where oxygenation will take place.     

Megabenthic commmunities in the waters around Svalbard

 Composition and distribution of megabenthic communities around Svalbard were investigated in June/July 1991 with 20 Agassiz trawl and 5 bottom trawl hauls in depths between 100 and 2100 m. About 370 species, ranging from sponges to fish, were identified in the catches. Species numbers per station ranged from 21 to 86. Brittle stars, such as Ophiacantha bidentata, Ophiura sarsi and Ophiocten sericeum, were most important in terms of constancy and relative abundance in the catches. Other prominent faunal elements were eunephthyid alcyonarians, bivalves, shrimps, sea stars and fish (Gadidae, Zoarcidae, Cottidae). Multivariate analyses of the species and environmental data sets showed that the spatial distribution of the megabenthos was characterized by a pronounced depth zonation: abyssal, bathyal, off-shore shelf and fjordic communities were discriminated. However, a gradient in sediment properties, especially the organic carbon content, seemed to superimpose on the bathymetric pattern. Both main factors are interpreted as proxies of the average food availability, which is, hence, suggested to have the strongest influence in structuring megabenthic communities off Svalbard. Received: 28 April 1995/Accepted: 18 November 1995     

The synthesis of amino acids and sugars on an inorganic template from constituents of the prebiotic atmosphere

Inelastic Electron Tunnelling Spectroscopy (IETS) has been used to identify the reaction products present on an alumina surface when it is exposed to likely components of the earth's prebiotic atmosphere. The alumina barrier of Al-AlO _x -Pb tunnelling junctions have been exposed to water; aqueous ammonia; wet carbon monoxide gas and to aqueous formaldehyde vapour under normal atmospheric conditions at room temperature. The water spectrum shows strong coincidence with that of a genuine sample of formic acid. It is proposed that atmospheric CO₂ is involved in this surface catalyzed reaction. The aqueous ammonia spectrum is assigned as an amino acid species produced from ammonia, water and atmospheric carbon dioxide. This spectrum compares very closely with the tunnelling spectrum of a genuine sample of glycine. The wet carbon monoxide spectrum and the aqueous formaldehyde spectrum have been produced by an infusion doping process. These spectra of CO and aqueous formaldehyde are assigned as a sugar like polymer or a sugar formed on the alumina surface. A tunnelling spectrum of D(–) fructose has been produced to aid this assignment. The role of an inorganic template such as alumina in the original prebiotic synthesis of amino acids and sugars is considered.     

Fermentation of hardwood hemicellulose hydrolysate byPachysolen tannophilus,candida shehatae andPichia stipitis

Summary Hardwood hemicellulose hydrolysate has been utilized as a substrate for ethanol production. Among the three different yeasts tested, the best performances have been obtained, in decreasing order, usingPachysolen tannophilus, Candida shehatae andPichia stipitis. Several pretreatments of this raw material have been studied to improve ethanol yields; in one such pretreatment a strain ofP. tannophilus produced ethanol with a yield of 0.29 g_ethanol/g_sugars (g_P/g_S); which is only 15% less than the values observed with synthetic media. Neither aeration nor acetone addition improved the fermentation of this substrate; in fact, only a marked stimulation of biomass growth has been observed at the expense of both ethanol and xylitol production.     

Yeast mutants without phosphofructokinase activity can still perform glycolysis and alcoholic fermentation

Summary Mutants of Saccharomyces cerevisiae without detectable phosphofructokinase activity were isolated. They were partly recessive and belonged to two genes called PFK1 and PFK2. Mutants with a defect in only one of the two genes could not grow when they were transferred from a medium with a nonfermentable carbon source to a medium with glucose and antimycin A, an inhibitor of respiration. However, the same mutants could grow when antimycin A was added to such mutants after they had been adapted to the utilization of glucose. Double mutants with defects in both genes could not grow at all on glucose as the sole carbon source. Mutants with a single defect in gene PFK1 or PFK2 could form ethanol on a glucose medium. However, in contrast to wild-type cells, there was a lag period of about 2 h before ethanol could be formed after transfer from a medium with only nonfermentable carbon sources to a glucose medium. Wild-type cells under the same conditions started to produce ethanol immediately. Mutants with defects in both PFK genes could not form ethanol at all. Mutants without phosphoglucose isomerase or triosephosphate isomerase did not form ethanol either. Double mutants without phosphofructokinase and phosphoglucose isomerase accumulated large amounts of glucose-6-phosphate on a glucose medium. This suggested that the direct oxidation of glucose-6-phosphate could not provide a bypass around the phosphofructokinase reaction. On the other hand, the triosephosphate isomerase reaction was required for ethanol production. Experiments with uniformly labeled glucose and glucose labeled in positions 3 and 4 were used to determine the contribution of the different carbon atoms of glucose to the fermentative production of CO₂. With only fermentation operating, only carbon atoms 3 and 4 should contribute to CO₂ production. However, wild-type cells produced significant amounts of radioactivity from other carbon atoms and pfk mutants generated CO₂ almost equally well from all six carbon atoms of glucose. This suggested that phosphofructokinase is a dispensable enzyme in yeast glycolysis catalyzing only part of the glycolytic flux.     

Direct Observation of Spin-Trapped Carbon Dioxide Radicals in Hepatocytes Exposed to Carbon Tetrachloride

Carbon dioxide radical adducts of the spin trapping agent, α-phenyl N-t-butyl nitrone (PBN), have been observed to occur in the urine and bile of rats exposed to carbon tetrachloride as well as in perfusates of liver in which the perfusion medium contained carbon tetrachloride (Connor er al., J. Biol. Chem., 261, 4542, (1986)). The carbon dioxide adduct was proven to be derived from CCI, by use of 13-C-labelled compound. These adducts were not observed in the liver itself suggesting that they might be rapidly secreted from the liver. However, using isolated hepatocytes, we have demonstrated that the carbon dioxide radical adduct can be observed directly in the liver cells as it is formed. Since this water-soluble adduct cannot be extracted by non-aqueous solvents such as chloroform or toluene, its formation in liver in vivo or in perfused livers was not detected. Lowering the oxygen tension in the system diminished the intensity of production of the carbon dioxide adduct, consistent with the adduct being produced as a result of ·OOCCl₃ generation. It is not clear the extent to which this adduct is formed as a result of the ·CO₂ radical or is produced by metabolic oxidation of the trichloromethyl radical adduct of PBN per se to the carbon dioxide radical adduct. The intensity of the signal of the carbon dioxide radical adduct suggests that adduct conversion may be the route of formation since it seems unlikely that a sufficient amount of the halocarbon could be metabolized to ·COCl or ·CO₂ radicals to generate a signal of the magnitude involved. The ·CO₂ adduct is readily observed in intact hepatocytes, but the ·CCl₃ adduct is not (although we know the ·CCl₃ adduct has been produced in these cells), indicating that the ·CO₂ adduct is present in considerable abundance compared to the ·CCl₃ adduct.     

Preparation of Carbon Nanosheets at Room Temperature

Amphiphilic molecules equipped with a reactive, carbon-rich "oligoyne" segment consisting of conjugated carbon-carbon triple bonds self-assemble into defined aggregates in aqueous media and at the air-water interface. In the aggregated state, the oligoynes can then be carbonized under mild conditions while preserving the morphology and the embedded chemical functionalization. This novel approach provides direct access to functionalized carbon nanomaterials. In this article, we present a synthetic approach that allows us to prepare hexayne carboxylate amphiphiles as carbon-rich siblings of typical fatty acid esters through a series of repeated bromination and Negishi-type cross-coupling reactions. The obtained compounds are designed to self-assemble into monolayers at the air-water interface, and we show how this can be achieved in a Langmuir trough. Thus, compression of the molecules at the air-water interface triggers the film formation and leads to a densely packed layer of the molecules. The complete carbonization of the films at the air-water interface is then accomplished by cross-linking of the hexayne layer at room temperature, using UV irradiation as a mild external stimulus. The changes in the layer during this process can be monitored with the help of infrared reflection-absorption spectroscopy and Brewster angle microscopy. Moreover, a transfer of the carbonized films onto solid substrates by the Langmuir-Blodgett technique has enabled us to prove that they were carbon nanosheets with lateral dimensions on the order of centimeters.