Science. 1971 Feb 5;171(3970):474-7. doi: 10.1126/science.171.3970.474.
Total carbon in the Apollo 12 sample 12023 fines was 110 micrograms per gram of sample with a carbon isotopic abundance delta(13)C (relative to the Pee Dee belemnite standard) of +12 per mil. Hydrolysis of the fines with deuterium chloride yielded undeuterated methane along with deuterated hydrocarbons, thus confirming the presence of 7 to 21 micrograms of carbon per gram of sample as carbide and about 2 micrograms of carbon per gram of sample as indigenous methane. After vacuum pyrolysis of the fines to 1100 degrees C the following gases were detected in the relative abundance: carbon monoxide carbon dioxide methane. Variations of the delta(13)C value with the pyrolysis temperature indicated the presence of carbon with more than one range of isotopic values. The observed delta(13)C value of +14 per mil for lunar carbide is much higher than that of carbide in meteorites. These results suggest that lunar carbide is either indigenous to the moon or a meteoritic contribution that has been highly fractionated isotopically.
阿波罗 12 号样本 12023 细粉中的总碳含量为每克样品 110 微克,碳同位素丰度 δ(13)C(相对于 Pee Dee 箭石标准)为+12‰。用重氯化氘将细粉水解,得到未氘化的甲烷和氘化烃,从而证实每克样品中有 7 至 21 微克碳作为碳化钙,以及约 2 微克碳作为本地产甲烷。将细粉真空热解至 1100°C 后,在相对丰度中检测到以下气体:一氧化碳、二氧化碳、甲烷。δ(13)C 值随热解温度的变化表明存在具有多种同位素值范围的碳。观测到的月球碳化钙的 δ(13)C 值为+14‰,远高于陨石中碳化钙的值。这些结果表明,月球碳化钙要么是月球本土的,要么是经过高度同位素分馏的陨石贡献。