A neon-E rich phase in Orgueil - Results obtained on density separates

Computer Science

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Carbonaceous Chondrites, Density Measurement, Galactic Evolution, Meteoritic Composition, Neon Isotopes, Chemical Analysis, Solar System, Spallation, Models, Spallation, Grains, Cosmogenic Elements, Meteorites, Neon, Data, Carbonaceous Chondrites, Orgueil Meteorite, Phases, Density, Irradiation, Argon, Techniques, Enrichment, Temperatures, Spinel, Carbon, Rare Gases, Experiments, Procedure, Isotopes, Isotopic Ratios, In Situ Measurements, Composition, Samples, Meteorite, Q Value, Origin, Helium, Concentrati

Scientific paper

A stepwise heating technique was used on eight density separates from the neon-E rich phase G4j of the carbonaceous chondrite Orgueil to measure He, Ne and Ar. The density separation technique was found to further enrich the Ne-E carrier phases, allowing the Ne-E to be identified as virtually pure Ne-22. At least two separable carrier phases exist: (1) the l-carrier phase, which releases its Ne-E at temperatures below 900 C and is heavily enriched in the low-density separate; and (2) the h-carrier phase. The h-carrier is found to be highly retentive, with release temperatures above 900 C, and is associated with higher-density material. It is concluded that Ne-E and its carrier phases are probably of presolar origin.

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