Noble-gas-rich separates from ordinary chondrites

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Chondrites, Meteoritic Composition, Rare Gases, Etchants, Isotope Separation

Scientific paper

Acid resistant residues were prepared by HCl-HF demineralization of three H-type ordinary chondrites. These residues were found to contain a large proportion of the planetary type trapped Ar, Kr, and Xe of the meteorites. The similarity of these acid residues to those from carbonaceous chondrites and LL type ordinary chondrites suggests that the same phase carries the trapped noble gases in all these diverse meteorite types. Because the H group represents a large fraction of all meteorites, this result indicates that the gas rich carrier phase is as universal as the trapped noble-gas component itself.

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