Results of I-Xe analyses have been obtained from meteorite samples that experienced different extents of thermal processing in the early Solar System in order to help characterise the movements of iodine and xenon in the early Solar System and constrain the timing of these movem…
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This dissertation presents the results and implications of the isotopic and elemental analyses of presolar silicate grains from the primitive chondrites, Acfer 094, SAH 97096, and ALHA77307. Oxygen-anomalous, C-anomalous, and N-anomalous grains were identified by O, C, and N iso…
Much of what is known about the early solar system’s history, processes, and conditions are determined through the study of airless bodies. Like their terrestrial counterparts, the geologic materials of airless bodies contain information about their formative environment; these …