Chemical ionization mass spectrometry of pristane.
Chemical ionization mass spectrometry of pristane
Engineering topics
Publications and source records attributed to Oro, J..
Chemical ionization mass spectrometry of pristane
Gas chromatography-mass spectrometry system for analysis of organic compounds on moon and planetary surfaces
High resolution gas chromatography combined with mass spectrometry applied to analysis of pyrolysis products of isoprene from 300 to 1000 degrees C
Gas chromatographic and mass spectrometric analysis of chlamydospores of Ustilago maydis, U. nuda and Sphacelotheca reiliana for hydrocarbon content
Aromatic hydrocarbon synthesis by passing methane through silica gel at high temperature
Paraffinic hydrocarbons composition in Orgueil, Murray, Mokoia and other meteorites identified by gas chromatography
Gas chromatography and mass spectrometry of acetonitrile, furan, pyrrole, paraffins, and other aromatic organic compounds of biological significance
According to Oparin, Mendeleev thought that the origin of petroleum was the result of the hydrolysis of iron carbides by superheated steam under pressure from the deep interior of the Earth through geological formations where the metal carbides exist. As early as 1877, Mendeleev described the reaction leading to the synthesis of hydrocarbons according to the general equation 3Fe(sub m)C(sub n) + mH2O yields mFe3O4 + C(sub 3n)H(sub 8m). Other experimental studies on the production of hydrocarbons from cast iron have been reported. Because of the possibility that hydrocarbons may have been trapped within the carbon matrix of the cast iron, which usually has a high content of carbon, we have studied the reaction of pure iron carbide with deuterium chloride and deuterated water. This was done in order to distinguish any newly formed deuterated hydrocarbons from any possible impurities of trapped hydrocarbons. The experiments were carried out by simply allowing iron carbide to react with concentrated deuterium chloride in D2O. The volatile hydrocarbon fraction examined by gas chromatography-mass spectrometry (GC/MS), using a Finnigan 1020/OWA instrument. contained low molecular weight hydrocarbons in a range C3 to C7. Lower molecular weight hydrocarbons were not detected by GC/MS because the MS scanning mode was preset above mass 40 to exclude components of air. The identified hydrocarbons are similar to those obtained under prebiotic conditions using high frequency discharge. The hydrocarbons found in common were propane, butane, pentane, 3-methylpentane, hexane, and heptane. The percent yields decline with increasing carbon number (propane 11%, n-heptane 1%). Similar results have been obtained by the direct treatment of metal carbides by pulse laser vaporization mass spectrometry. These results show that the hydrolysis of iron carbides may have been a significant source of hydrocarbons on the primitive Earth. There appears to be a predominance of straight chain isomers, which may have been important in the prebiotic synthesis of membrane-forming compounds.
Contamination of carbonaceous chondrites by ordinary viable microorganisms, isolating three types of bacteria on various meteorites
Chromatographic study of free amino acids on human fingers as contamination factor in microanalysis of such acids on meteorites
Hydrocarbons of biological origin in Gunflint iron formation sediments from shore of Lake Superior that are two billion years old, examining alkane distribution
Gas chromatographic/mass spectrometric technique applied to analysis of paraffinic hydrocarbons from pasture plants
Prebiological organic synthesis stages and mechanisms prior to and during formation of Earth, noting extraterrestrial organic matter
Nonenzymatic synthesis of nucleic acid components and abiogenesis of neurines, pyrimidines, pentosribose and deoxyribose
Organic synthesis processes, which may have occurred in the primitive earth atmosphere or in comets, produced in the laboratory by methods of electric discharge, uv light and ionizing radiation
Organic chemistry and synthesis of biochemical compounds found in universe
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