Chronology of SNC meteorites

Computer Science – Emerging Technologies

Scientific paper

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Lead Isotopes, Mars (Planet), Meteoritic Composition, Neodymium Isotopes, Planetary Evolution, Strontium Isotopes, Chronology, Magma, Planetary Geology, Radioactive Age Determination, Samarium Isotopes, Meteorites, Snc Meteorites, Chronology, Models, Geochemistry, Evolution, Isotopic Ratios, Crystallization, Age, Metamorphism, Magmatic Processes, Shock Effects, Petrography, Samples, Meteorite, Antarctic Meteorites, Alha77009, Alh Meteorites, Formation, Origin, Differentiation, Melting, Parent Material, Diag

Scientific paper

A model is presented for the geochemical evolution of Mars which is constrained by the isotope systematics of Pb, Nd, and Sr determined for SCN meteorites. The young magmatic crystallization ages of SCNs may indicate that these meteorites do in fact stem from Mars. Internal ages of U-Pb and Pb-Pb systematics strongly suggest that they are the result of two magmatic processes. In addition, shock metamorphism is implied from observed petrographic shock features.

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