Investigation of Antarctic Micrometeorites and Selected Carbonaceous Chondrites by Raman Spectroscopy, Electron Microscopy and Mass Spectrometry

• Main Authors: Merouane, Sihane, Günther, Stefanie, Chitarra, Olivia, Stenzel, Oliver, Hilchenbach, Martin, Engrand, Cecile, Tarcea, N.
• Other Authors: Max-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research (MPS), Max-Planck-Gesellschaft, Geowissenschaftliches Zentrum Göttingen (GZG), Georg-August-University = Georg-August-Universität Göttingen, Institut des Sciences Moléculaires d'Orsay (ISMO), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Friedrich-Schiller-Universität = Friedrich Schiller University Jena Jena, Germany
• Format: Conference Object
• Language: English
• Published: HAL CCSD 2018
• Subjects: [SDU]Sciences of the Universe [physics]; Antarctic; Antarc*
• Online Access: https://hal.science/hal-02395348

International audience Concordia Antarctic micrometeorites (MMs) are micrometer-sized particles collected in Antarctic snow that are likely originating from asteroids and comets [1,2]. These samples, coming from primitive bodies (i.e. that have suffered low secondary processes), may have preserved information of the early stages of the Solar system. We analyzed three MMs from the Concordia collection (DC06-07-54, DC06-07-162 and DC06-09-249) and com- pare their mineralogical and elemental composition as well as the nature of their organic material with five selected carbonaceous chondrites with the goal of classifying them among meteorites families.