| タイトル | Isotope Ratio Monitoring Gas Chromatography Mass Spectrometry (IRM-GCMS) |
| 本文（外部サイト） | http://hdl.handle.net/2060/19890016975 |
| 著者（英） | Hayes, J. M.; Studley, A.; Freeman, K. H.; Ricci, S. A. |
| 著者所属（英） | Indiana Univ. |
| 発行日 | 1989-03-01 |
| 言語 | eng |
| 内容記述 | On Earth, the C-13 content of organic compounds is depleted by roughly 13 to 23 permil from atmospheric carbon dioxide. This difference is largely due to isotope effects associated with the fixation of inorganic carbon by photosynthetic organisms. If life once existed on Mars, then it is reasonable to expect to observe a similar fractionation. Although the strongly oxidizing conditions on the surface of Mars make preservation of ancient organic material unlikely, carbon-isotope evidence for the existence of life on Mars may still be preserved. Carbon depleted in C-13 could be preserved either in organic compounds within buried sediments, or in carbonate minerals produced by the oxidation of organic material. A technique is introduced for rapid and precise measurement of the C-13 contents of individual organic compounds. A gas chromatograph is coupled to an isotope-ratio mass spectrometer through a combustion interface, enabling on-line isotopic analysis of isolated compounds. The isotope ratios are determined by integration of ion currents over the course of each chromatographic peak. Software incorporates automatic peak determination, corrections for background, and deconvolution of overlapped peaks. Overall performance of the instrument was evaluated by the analysis of a mixture of high purity n-alkanes of know isotopic composition. Isotopic values measured via IRM-GCMS averaged withing 0.55 permil of their conventionally measured values. |
| NASA分類 | INORGANIC AND PHYSICAL CHEMISTRY |
| レポートNO | 89N26346 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/141282 |
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