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Journal Articles

Argon retentivity of carbonaceous materials; Feasibility of kerogen as a carrier phase of Q-noble gases in primitive meteorites

Osawa, Takahito; Hirao, Norie; Takeda, Nobuyori*; Baba, Yuji

Earth Planets and Space, 61(8), p.1003 - 1011, 2009/10

 Times Cited Count:4 Percentile:12.37(Geosciences, Multidisciplinary)

To verify that kerogen is a carrier phase of Q-noble gases, XAS and XPS using synchrotron radiation were carried on for kerogens (coals) and carbon allotropes that had been bombarded by 3-keV Ar ions, and the Ar retentivities of the two materials were compared. This comparison of the estimated Ar concentrations in the target materials revealed that carbon allotropes (graphite, fullerene, carbon nanotube, and diamond) have a much higher Ar retentivity than kerogens. This unexpected result clearly shows that the terrestrial kerogens tested in our study are not suitable as a carrier phase of Ar and, consequently, that phase Q may not be similar to the terrestrial kerogen tested. If heavy noble gases are really concentrated in carbonaceous components of primitive meteorites, phase Q may have a more ordered structure than terrestrial kerogen based on the fact that the greatest difference between terrestrial kerogen and carbon allotropes is the degree of order of the molecular structure.

Oral presentation

Noble gas retentivity of carbon allotropes and kerogen; Feasibility of kerogen as phase Q

Osawa, Takahito; Hirao, Norie; Takeda, Nobuyori*; Baba, Yuji

no journal, , 

To verify that kerogen is a carrier phase of Q-noble gases, X-ray absorption spectroscopy (XAS) and X-ray photoelectron spectroscopy (XPS) using synchrotron radiation were carried out for type II and III kerogens and carbon allotropes which had been bombarded by 3 keV Ar, Kr, and Xe ions, and noble gas retentivities of the materials were compared. Ar concentrations was estimated from XPS and XAS. Kr and Xe concentrations were estimated by the peak areas of Kr3p3/2 and Xe3d5/2 in XPS. The concentrations were used as indexes of the relative retentivity of noble gases. Our investigation shows that the surface concentrations of carbon allotropes (0.40-0.79 atom%) are much higher than those of kerogens (0.04-0.08 atom%). This unexpected result clearly shows that the terrestrial kerogens are inferior to other carbon materials in noble gas retentivity, and thus, phase Q might not be similar to terrestrial kerogen, especially coals tested in this work.

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