Deuterium exchange rate between D3+ and organic CH bonds: Implication for D enrichment in meteoritic IOM

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The rate of the transfer of deuterium from D3+ to the three types (benzylic, aliphatic and aromatic) of bonds of 2-Ethylnaphthalene (and Methylnaphthalene) has been measured in the laboratory. The D/H ratio of each bond was calculated from the mass spectrum of the different isotopomers produced in the source of the GC mass spectrometer. The relations between the D/H ratio of the different isotopomers allow to calculate the internal isotopic fractionation factors (αi-j = (D/H)i/(D/H)j) between the 3 bonds: αBenzylic-Aromatic = 1.99 ± 0.38 and αAliphatic-Aromatic = 1.22 ± 0.39. Isotopic exchange rate constants are ⩾2.2 × 10-7±0.4 s-1, determined at room temperature for 10-3 g of 2-Ethylnaphthalene in contact with 5 × 1012 cm-3 of D3+. These results are compatible with those measured in the insoluble organic matter (IOM) isolated from the Orgueil meteorite (Remusat et al., 2006), i.e., αBenzylic-Aromatic = 1.96 ± 0.05 and αAliphatic-Aromatic = 1.35 ± 0.05. Using the calculated dust and H2D+ densities from the models of deuterium chemistry in protostellar disks, the duration needed to enrich the IOM up to its measured D/H ratio is ⩽104±1 s. These laboratory results are in agreement with a late deuteration of the insoluble organic matter taking place in the solar T-Tauri disk by interaction of the organic dust with H2D+.

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