My primary research interests focus on the origin and evolution of elements in the Galaxy and planetary materials within the early Solar System through a variety of isotopic anomalies (radiogenic, spallogenic and nucleosynthetic) preserved in meteoritic components. These isotopically anomalous signals, revealed through analyses of samples by Secondary Ion Mass Spectrometry (SIMS), provide information about the astrophysical environment in which the Solar System formed, the timescales of high temperature processing and chemical evolution during the earliest stages of the Solar System formation, and nucleosynthetic processes inside stars.