1970
DOI: 10.1016/0016-7037(70)90105-5
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Light hydrocarbon gases, C13, and origin of organic matter in carbonaceous chondrites

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Cited by 71 publications
(24 citation statements)
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“…These data suggest that effective blank production is reduced when rock fragments are present in the ball mill and that repeated shaking in the presence of rock powder results in less blank production. A similar observation by Belsky and Kaplan (1970), in which gas amounts decreased with repeated crushing of previously crushed material, was interpreted by them as an indication that the released gases were indigenous to the rock and not produced by impact within the crushing device. Such an effect may be due t o a reduction in med-metal impact within the crusher, possibly because of cushioning by the rock powder, so that blank generation is reduced compared with the-empty ball-mill runs.…”
Section: Blank Productionmentioning
confidence: 63%
“…These data suggest that effective blank production is reduced when rock fragments are present in the ball mill and that repeated shaking in the presence of rock powder results in less blank production. A similar observation by Belsky and Kaplan (1970), in which gas amounts decreased with repeated crushing of previously crushed material, was interpreted by them as an indication that the released gases were indigenous to the rock and not produced by impact within the crushing device. Such an effect may be due t o a reduction in med-metal impact within the crusher, possibly because of cushioning by the rock powder, so that blank generation is reduced compared with the-empty ball-mill runs.…”
Section: Blank Productionmentioning
confidence: 63%
“…The abundance and stable C-isotopic composition of bulk C within the stony meteorites is well characterised (e.g., Otting and Zahringer, 1967;Belsky and Kaplan, 1970;Smith and Kaplan, 1970;…”
Section: Discussionmentioning
confidence: 99%
“…These studies detected a large number of aromatic and alkyl aromatic compounds ranging from naphthalene to coronene and, in many Table 11 Carbon and hydrogen isotope data for individual volatile alkanes (Butterworth et al, 2004;Yuen et al, 1984) and normal alkanes (Sephton et al, 2001a) cases, high-molecular-weight compounds dominated. Aromatic hydrocarbons can be liberated by heating meteorites at temperatures at or below 300 C. Such thermally extracted compounds, ranging from benzene to pyrene, were detected by mass spectrometry (Hayes and Biemann, 1968;Muenow et al, 1971;Studier et al, 1965Studier et al, , 1968; GC (Belsky and Kaplan, 1970;Levy et al, 1970) and GC-MS . The analyses of Allende (CV3) shortly after its fall revealed small amounts of aromatic contamination, which consisted mainly of a phenyl alkane structure.…”
Section: Solvent and Thermal Extractsmentioning
confidence: 99%