Walton, Erin L.Aizon, Jannah2021-06-042022-05-312022-05-312021https://hdl.handle.net/20.500.14078/2318Presented on April 26, 2021 at Student Research Day held virtually at MacEwan University in Edmonton, Alberta, and on May 3-4, 2021 at the Undergraduate Research in Science Conference of Alberta (URSCA) held at Concordia University of Edmonton.The study of meteorites is crucial to understanding the geological evolution of our early solar system. In this study, we observe optical and chemical properties of two diogenite meteorites (Northwest Africa 7464 and 10268) that originated from the second-largest asteroid, 4 Vesta. By studying the mechanical deformation and transformation features of feldspar, olivine and pyroxene grains within the samples, we are able to constrain the shock stage of each meteorite. Northwest Africa 7464 and 10268 were both observed using a scanning electron microscope, an energy dispersive X-ray spectrometer, an electron microprobe, a petrographic microscope and a Raman spectrometer. Northwest Africa 7464 exhibits weak mosaicism and planar fractures in pyroxene, as well as, undulatory extinction and planar fractures in olivine. These features suggest a weakly shocked S3 meteorite consistent with a shock pressure of between 5-15 GPa. Northwest Africa 10268 contains opaque shock veins associated with the diaplectic plagioclase glass, maskelynite. This host rock exhibits strong mosaicism and undulatory extinction in pyroxene, as well as, twinning in crystalline feldspar. These features are consistent with a moderately shocked S4 meteorite, experiencing a shock pressure of between 15-30 GPa. These results give insight on shock pressure and temperature conditions that occur on 4 Vesta.3.36MBPDFenAll Rights Reservedmeteoritesshock pressureStudent Presentation