Hypervelocity collision and water-rock interaction in space preserved in the Chelyabinsk ordinary chondrite

1Eizo Nakamura et al. (>10)
Proceedings of the Japan Academy, Series B 95, 165-177 Link to Article [https://doi.org/10.2183/pjab.95.013]
1The Pheasant Memorial Laboratory for Geochemistry and Cosmochemistry, Institute for Planetary Materials, Okayama University

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STXM-XANES analyses of Murchison meteorite samples captured by aerogel after hypervelocity impacts: A potential implication of organic matter degradation for micrometeoroid collection experiments

1Yoko Kebukawa et al. (>10)
Geochemical Journal 53, 53-67 Link to Article [https://doi.org/10.2343/geochemj.2.0549]
1Faculty of Engineering, Yokohama National University

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Probing the chemical and mineralogical characteristics of the Martian meteorite NWA 7397 through μRaman and μXRF non-destructively

1Bruno Leonardo do Nascimento-Dias,2Douglas Galante,1,3Davi Oliveira,1,3 Marcelino Anjos
International Journal of Astrobiology 18, 73-78 Link to Article [https://doi.org/10.1017/S1473550418000022]
1University of state of Rio of Janeiro, Rio de Janeiro, Brazil
2Brazilian Synchrotron Light Laboratory, Brazilian Center for Research in Energy and Materials, Campinas, Brazil
3Federal University of Rio de Janeiro, Rio de Janeiro, Brazil

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CanMars mission Science Team operational results: Implications for operations and the sample selection process for Mars Sample Return (MSR)

1Christy M.Caudill et al. (>10)
Planetary and Space Science (in Press) Link to Article [https://doi.org/10.1016/j.pss.2019.04.004]
1Centre for Planetary Science and Exploration / Dept. Earth Sciences, University of Western Ontario, 1151, Richmond St, London, ON, N6A 3K7, Canada

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Nanometre-scale infrared chemical imaging of organic matter in ultra-carbonaceous Antarctic micrometeorites (UCAMMs)

1Jérémie Mathurin,2Emmanuel Dartois,2Thomas Pino,3Cécile Engrand,3Jean Duprat,1Ariane Deniset-Besseau,4Ferenc Borondics,4Christophe Sandt,1 Alexandre Dazzi
Astronomy & Astrophysics 622, A160 Link to Article [https://doi.org/10.1051/0004-6361/201833957]
1Laboratoire de Chimie Physique, CNRS, Université Paris Sud, Université Paris-Saclay, 91405 Orsay Cedex, France
2Institut des sciences moléculaires d’Orsay, CNRS, Université Paris Sud, Université Paris-Saclay, 91405 Orsay, France
3Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM), CNRS/IN2P3, Université Paris Sud, Université Paris-Saclay, 91405 Orsay, France
4Synchrotron Soleil, L’Orme des Merisiers, BP 48 Saint Aubin, 91192 Gif-sur-Yvette Cedex, France

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Chemical composition of planet building blocks as predicted by stellar population synthesis

1N. Cabral,1N. Lagarde,1C. Reylé,1A. Guilbert-Lepoutre,1A. C. Robin
Astronomy & Astrophysics 622, A49 Link to Article [https://doi.org/10.1051/0004-6361/201833750]
1Institut UTINAM, CNRS UMR6213, Université Bourgogne Franche-Comté, OSU THETA Franche-Comté-Bourgogne, Observatoire de Besançon, BP 1615, 25010 Besançon Cedex, France

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