 | Dionnet, Z., Aleon-Toppani, A., Baklouti, D., Borondics, F., Brisset, F., Djouadi, Z., Sandt, C., Brunetto, R. (2018) Organic and mineralogic heterogeneity of the Paris meteorite followed by FTIR hyperspectral imaging. Meteoritics & Planetary Science, 53 (12) 2608-2623 doi:10.1111/maps.13178 | Journal (article/letter/editorial) | | Organic and mineralogic heterogeneity of the Paris meteorite followed by FTIR hyperspectral imaging Z. DIONNET... Universite Paris-Sud, Universite Paris-Saclay, B^ at. 121, 91405 Orsay Cedex, France 2 Synchrotron...Saint-Aubin, France 3 Institut de Chimie Moleculaire et des Materiaux dâOrsay, Universite Paris Sud, Universite...Universite Paris-Saclay, 91405 Orsay Cedex, France * Corresponding author. E-mail: zelia.dionnet@u-psud...measurements at the micron scale on a fragment of the Paris carbonaceous chondrite, supported by Raman and SEM-EDS |  | Hewins, Roger H., Bourot-Denise, MichĂšle, Zanda, Brigitte, Leroux, Hugues, Barrat, Jean-Alix, Humayun, Munir, Göpel, Christa, Greenwood, Richard C., Franchi, Ian A., Pont, Sylvain, Lorand, Jean-Pierre, CournĂšde, CĂ©cile, Gattacceca, JĂ©rĂŽme, Rochette, Pierre, Kuga, MaĂŻa, Marrocchi, Yves, Marty, Bernard (2014) The Paris meteorite, the least altered CM chondrite so far. Geochimica et Cosmochimica Acta, 124. 190-222 doi:10.1016/j.gca.2013.09.014 | Journal (article/letter/editorial) | | (2014) 190â222 www.elsevier.com/locate/gca The Paris meteorite, the least altered CM chondrite so far Roger...Laboratoire de MineÌralogie et Cosmochimie du MuseÌum, MNHN and CNRS UMR 7202, 75005 Paris, France b Department...8207, F-59655 Villeneuve dâAscq, France d UniversiteÌ EuropeÌenne de Bretagne and CNRS UMR 6538, U.B.O-I...O-I.U.E.M., 29280 PlouzaneÌ Cedex, France e Department of Earth, Ocean and Atmospheric Science and National...USA f Institut de Physique du Globe de Paris, Sorbonne Paris CiteÌ, UniversiteÌ Paris Diderot, UMR 7154 |  | Zanetta, P.-M., Le Guillou, C., Leroux, H., Zanda, B., Hewins, R.H., Lewin, E., Pont, S. (2019) Modal abundance, density and chemistry of micrometer-sized assemblages by advanced electron microscopy: Application to chondrites. Chemical Geology, 514. 27-41 doi:10.1016/j.chemgeo.2019.03.025 | Journal (article/letter/editorial) | | Lille, France ; 2. IMPMC, Sorbonne UniversitĂ©, MNHN, UPMC Paris 06, UMR CNRS 7590, 75005 Paris, France...NJ 08854, USA ; 4. Observatoire de Paris, IMCCE, 75014 Paris, France ; 5. ISTerre (OSUG : Univ. Grenoble...Grenoble Alpes & INSU-CNRS), Grenoble, France. (Pierre.marie.zanetta@gmail.com) US CR Keywords: Hyperspy;...applied to three well-known chondrites (Murchison, Paris and Orgueil), showing heterogeneous grain sizes...Orgueil meteorite, one section of the Murchison meteorite and one section of the Paris meteorite provided |  | Jacquet, Emmanuel, Barrat, Jean-Alix, Beck, Pierre, Caste, Florent, Gattacceca, JĂ©rĂŽme, Sonzogni, Corinne, Gounelle, Matthieu (2016) Northwest Africa 5958: A weakly altered CM-related ungrouped chondrite, not a CI3. Meteoritics & Planetary Science, 51 (5) 851-869 doi:10.1111/maps.12628 | Journal (article/letter/editorial) | | Matthieu GOUNELLE1,8 1 Institut de Mineralogie de Physique des Materiaux et de Cosmochimie, CNRS & Museum...dâHistoire Naturelle, UMR 7202, 57 rue Cuvier, 75005 Paris, France 2 Canadian Institute for Theoretical Astrophysics... UMR 6538, Universite Europeenne de Bretagne, Bretagne, France 4 CNRS UMR 6538 (Domaines Oceaniques)...Plouzane Cedex, France 5 1 Univ. Grenoble Alpes, Institut de Planetologie et dâAstrophysique de Grenoble (IPAG)...(IPAG), F-38000 Grenoble, France 6 CNRS, IPAG, F-38000 Grenoble, France 7 CEREGE UM 34, CNRS/Universite |  | Cuvillier, Priscille, Chaumard, NoĂ«l, Leroux, Hugues, Zanda, Brigitte, Hewins, Roger H., Jacob, Damien, Devouard, Bertrand (2018) A TEM study of exsolution in Ca-rich pyroxenes from the Paris and Renazzo chondrites: Determination of type I chondrule cooling rates. Meteoritics & Planetary Science, 53 (3) 482-492 doi:10.1111/maps.13032 | Journal (article/letter/editorial) | | study of exsolution in Ca-rich pyroxenes from the Paris and Renazzo chondrites: Determination of type I...Villeneuve dâAscq, France Institut de Mineralogie, de Physique des Materiaux, et de Cosmochimie (IMPMC)...dâHistoire Naturelle, UPMC Universite Paris 06, IRD & CNRS, 75005 Paris, France 3 WiscSIMS, Department of Geoscience...USA 5 Institut de Mecanique Celeste et de Calcul des Ephemerides, Observatoire de Paris, 77 Av. Denfert...Denfert Rochereau, F-75014 Paris Cedex, France 6 Aix-Marseille Universite, CNRS, IRD, CEREGE UM34, 13545 |  | | Journal (article/letter/editorial) | | com/locate/gca GEMS-like material in the matrix of the Paris meteorite and the early stages of alteration of CM chondrites...Villeneuve dâAscq, France Institut de MineÌralogie, de Physique des MateÌriaux, et de Cosmochimie (IMPMC)...UPMC UniversiteÌ Paris 06, UMR CNRS 7590, IRD UMR 206, 57 rue Cuvier, 75231 Paris, France Received 26 July...Available online 28 September 2015 Abstract The Paris meteorite is a weakly altered CM chondrite that has been...the CM parent body. The study of the matrix of Paris has been conducted by analytical transmission electron |  | Pignatelli, Isabella, Marrocchi, Yves, Vacher, Lionel. G., Delon, RĂ©mi, Gounelle, Matthieu (2016) Multiple precursors of secondary mineralogical assemblages in CM chondrites. Meteoritics & Planetary Science, 51 (4) 785-805 doi:10.1111/maps.12625 | Journal (article/letter/editorial) | | 4 1 Universite de Lorraine, CRPG, UMR 7358, Vandoeuvre-les-Nancy F-54501, France 2 CNRS, CRPG UMR...y F-54501, France 3 IMPMC, MNHM, UPMC, UMR CNRS 7590, 61 rue Buffon, 75005 Paris, France 4 Institut Universitaire...Universitaire de France, Maison des Universites, 103 boulevard Saint-Michel, 75005 Paris, France * Corresponding...tochilinite/cronstedtite intergrowths (TCIs) in Paris, a new CM chondrite considered to be the least altered...the absence of Mg-bearing secondary minerals in Paris TCIs suggests that the Mg content increases during |  | Marrocchi, Yves, Gounelle, Matthieu, Blanchard, Ingrid, Caste, Florent, Kearsley, Anton T. (2014) The Paris CM chondrite: Secondary minerals and asteroidal processing. Meteoritics & Planetary Science, 49 (7) 1232-1249 doi:10.1111/maps.12329 | Journal (article/letter/editorial) | | 1232â1249 (2014) doi: 10.1111/maps.12329 The Paris CM chondrite: Secondary minerals and asteroidal...KEARSLEY7 1 Universite de Lorraine, CRPG, UMR 7358, Vandoeuvre les Nancy, F-54501, France 2 CNRS, CRPG UMR...Vandoeuvre les Nancy, F-54501, France 3 Laboratoire de Mineralogie et de Cosmochimie du Museum, MNHN...and CNRS, UMR 7202, 75005 Paris, France 4 Institut Universitaire de France, Maison des Universites,...Saint-Michel, 75005 Paris, France 5 Institut de Physique du Globe de Paris, Sorbonne Paris Cite, Universite |  | Ebert, Samuel, Bischoff, Addi, Harries, Dennis, Lentfort, Sarah, Barrat, JeanâAlix, Pack, Andreas, Gattacceca, JĂ©rĂŽme, Visser, Robbin, SchmidâBeurmann, Peter, Kimpel, Stephan (2019) Northwest Africa 11024âA heated and dehydrated unique carbonaceous (CM) chondrite. Meteoritics & Planetary Science, 54 (2) 328-356 doi:10.1111/maps.13212 | Journal (article/letter/editorial) | | Germany 3 Institut Universitaire Europeen de la Mer, Universite de Bretagne Occidentale, Place Nicolas Copernic...Copernic, F-29280 Plouzane Cedex, France 4 Geowissenschaftliches Zentrum, Universit⏠at G⏠ottingen,...Universite, IRD, INRA, College de France, CEREGE, Aix-en-Provence, France 6 Institut f⏠ur Geologische...dehydrated the sample. We suggest to classify the meteorite NWA 11024 as the first type 3 CM chondrite similar...ordinary chondrites Monahans (H5) and Villalbeto de la Pena (L6) are affected by asteroidal water. Furthermore |  | Pignatelli, Isabella, Marrocchi, Yves, Mugnaioli, Enrico, Bourdelle, Franck, Gounelle, Matthieu (2017) Mineralogical, crystallographic and redox features of the earliest stages of fluid alteration in CM chondrites. Geochimica et Cosmochimica Acta, 209. 106-122 doi:10.1016/j.gca.2017.04.017 | Journal (article/letter/editorial) | | UMR 7358, CNRS - UniversitĂ© de Lorraine, 54500 Vandoeuvre-lĂšs-Nancy, France Dipartimento di Scienze Fisiche... 5 6 LGCgE, UniversitĂ© de Lille 1, SN 5, 59655 Villeneuve d'Ascq, France IMPMC, MNHN, UPMC, UMR CNRS...7590, 61 rue Buffon, 75005 Paris, France Institut Universitaire de France, Maison des UniversitĂ©s, 103...103 bd. Saint-Michel, 75005 Paris, *Corresponding author: Isabella Pignatelli (isabella.pignatelli@univ-lorraine...CM2) down to heavily altered (i.e., CM 1) . The Paris chondrite is considered the least altered CM and |  | VerdierâPaoletti, Maximilien J., Marrocchi, Yves, Vacher, Lionel G., Gattacceca, JĂ©rĂŽme, Gurenko, Andrey, Sonzogni, Corinne, Gounelle, Matthieu (2019) Testing the genetic relationship between fluid alteration and brecciation in
CM
chondrites. Meteoritics & Planetary Science, 54 (8) 1692-1709 doi:10.1111/maps.13306 | Journal (article/letter/editorial) | | UPMC, UMR CNRS 7590, 61 rue Buffon, 75005 Paris, France Department of Terrestrial Magnetism, Carnegie...CRPG, CNRS, Universite de Lorraine, UMR 7358, Vandoeuvre les Nancy F-54501, France 4 Department of Physics...Univ, IRD, Coll France, CEREGE, Aix-en-Provence, France 6 Institut Universitaire de France, Maison des Universites...Universites, 103 bd. Saint-Michel, 75005 Paris, France * Corresponding author. E-mail: mverdier@carnegiescience...2012). To a few exceptions, like the Y-791198 and Paris INTRODUCTION Mighei-like chondrites (CM) represent |  | | Journal (article/letter/editorial) | | (2015) doi: 10.1111/maps.12482 An American on Paris: Extent of aqueous alteration of a CM chondrite...2014; revision accepted 02 June 2015) AbstractâParis is the least aqueously altered CM chondrite identified...apparently brecciated meteorite may be subtype 2.9. The suite of CAIs in Paris includes 19% spinelâpyroxene...have found a few rare occurrences of melilite in Paris CAIs. Because melilite is highly susceptible to...chondrules and CAIs were admixed. Also present in Paris are a few amoeboid olivine inclusions (AOI) consisting |  | | Journal (article/letter/editorial) | | revision accepted 26 September 2019) AbstractâMeteorite Hills (MET) 01075 is unique among the CM carbonaceous...that has not been previously recorded by this meteorite group. MET 01075 is composed of aqueously altered...CAI that also contains spinel, perovskite, and diopside together with Fe-rich phyllosilicate and calcite...describe sodalite in the CM carbonaceous chondrite Meteorite Hills (MET) 01075. This mineral has not been previously...(jadeite), Mg (periclase), Al (corundum), Si (diopside), S (pyrite), K (orthoclase), Ca (wollastonite) |  | Marinova, Maya, Leroux, Hugues, Cuvillier, Priscille, Gloter, Alexandre, Jacob, Damien (2020) STEM-EELS Investigation of Planar Defects in Olivine in the Allende Meteorite. Minerals, 11 (1) 35 doi:10.3390/min11010035 | Journal (article/letter/editorial) | | Investigation of Planar Defects in Olivine in the Allende Meteorite Maya Marinova 1, *, Hugues Leroux 2, *, Priscille...2638-IMEC-Institut Michel-EugĂšne Chevreul, F-59000 Lille, France Univ. Lille, CNRS, INRAE, Centrale Lille, UMR 8207-UMET-UnitĂ©...Lille, France; priscille.cuvillier@edf.fr (P.C.); damien.jacob@univ-lille.fr (D.J.) UniversitĂ© Paris-Saclay...Laboratoire de Physique des Solides (LPS), 91405 Orsay, France; alexandre.gloter@universite-paris-saclay.fr...EDFâIndustrial Direction, NPP of Chinon-BP23, 37420 Avoine, France. Abstract: The present study focuses on a detailed |  | | Journal (article/letter/editorial) | | MOÌSSBAUER SPECTROSCOPY OF OLIVINES FROM THE DâORBIGNY METEORITE Y. A. Abdu1, M. E. Varela2 and F. C. Hawthorne1...(d13C approximately 0 to +5&) lining vugs in the meteorite. There are also diïŹerences in magmatic carbon...of the Meteoritical Society: Abstracts 5022 METEORITE IMPACT CRATERS IN SOUTH AMERICA: A BRIEF REVIEW...discoveries. The following possible and conïŹrmed meteorite impact structures have been reported for this...iron-nickel Apollo-type asteroid (meteorite type IA) and plenty of meteorite specimens survived the impact |  | | Journal (article/letter/editorial) | | Buffon, 75005 Paris, France, (jerome.aleon@mnhn.fr), 2IAS, UMR 8617, CNRS, Univ. Paris-Saclay, 91405...Orsay cedex, France, 3GEOPS, CNRS UMR 8148, Univ Paris-Saclay, 91405 Orsay cedex, France, 4Dept of Earth...5 ICMMO, CNRS UMR 8182, Univ. Paris-Saclay, 91405 Orsay cedex, France. Introduction: Chondritic meteorites...ICCMO and ENS Paris and Electron Probe MicroAnalysis at the CAMPARIS facility in Paris. O and Mg isotopes...50 in the National Museum of Natural History in Paris, respectively. Results: UH154-11 has a fine-grained |  | Langbroek, Marco, Jenniskens, Peter, Kriegsman, Leo M., Nieuwenhuis, Henk, De Kort, Niek, Kuiper, Jacob, Van Westrenen, Wim, Zolensky, Michael E., Ziegler, Karen, Yin, QingâZhu, Sanborn, Matthew E., Wimpenny, Josh, Yamakawa, Akane, De Vet, Sebastiaan J., Meier, Matthias M. M., Welten, Kees C., Nishiizumi, Kunihiko, Caffee, Marc W., Burton, Aaron S., Dworkin, Jason P., Glavin, Daniel P., Wu, Qinghao, Zare, Richard N., Ruf, Alexander, Harir, Mourad, SchmittâKopplin, Philippe, , (2019) The CM carbonaceous chondrite regolith Diepenveen. Meteoritics & Planetary Science, 54 (7) 1431-1461 doi:10.1111/maps.13297 | Journal (article/letter/editorial) | | 3*, Leo M. KRIEGSMAN 1,4, Henk NIEUWENHUIS 5, Niek DE KORT 6, Jacob KUIPER 7, Wim VAN WESTRENEN Michael...WIMPENNY 11,12, Akane YAMAKAWA 11,13, Sebastiaan J. DE VET 1,6, Matthias M. M. MEIER 14,15, Kees C. WELTEN...Philippe SCHMITT-KOPPLIN 20,21, The Diepenveen Meteorite Consortium 8 , , 11 18 , 1 Department of... 3731 GA, De Bilt, the Netherlands 8 Department of Earth Sciences, Vrije Universiteit, De Boelelaan 1085...chondrites like Cochabamba (Kurat and Kracher 1975) and Paris (Hewins et al. 2014), Diepenveen has a known provenance |  | Rubin, Alan E., Breen, John P., Isa, Junko, Tutorow, Sean (2017) NWA 10214-An LL3 chondrite breccia with an assortment of metamorphosed, shocked, and unique chondrite clasts. Meteoritics & Planetary Science, 52 (2) 372-390 doi:10.1111/maps.12797 | Journal (article/letter/editorial) | | Slab of the NWA 10214 LL3 chondrite breccia. The meteorite contains numerous well-defined chondrules and...can be viewed at wileyonlinelibrary.com.) The meteorite has been significantly weathered. Most of the...thin section of NWA 10214, we estimate that the meteorite contains ~2â3 vol% metallic Fe-Ni, corresponding...exhibit some patchy Fe-Mg zoning. Because the meteorite contains LL5 and LL6 clasts (see below), the whole...indicate that the host is subtype 3.6â3.9. The meteorite has been very weakly shocked. Most of the coarse |  | | Journal (article/letter/editorial) | | University, Aix en Provence, France. mail : aboulahris@cerege.fr . 3UniversitĂ© de Tunis El Manar ,FacultĂ©...Science Tunis, Tunisia, 4 Meteorite Laboratory Lehmweg Gifhorn, Germany, 5 Meteorite Recon MĂŒhlendamm Hamburg...calculation of meteorite flux is possible [4]. Following previous estimation of meteorite flux based on...result of a meteorite shower. Their age, whatever the event is, is very recent. Salar de Antofalla. The...ANALYSIS (INAA) FOR ELEMENTAL COMPOSITION OF FRESH METEORITE FALL IN ORISSA, INDIA (2003). B. Adur, H.B. Mali |  | | Journal (article/letter/editorial) | | CARBONACEOUS-CHONDRITE INCLUSIONS FROM THE KAPOETA METEORITE: EVIDENCE FOR THE EXISTENCE OF NANODIAMONDS WITH...Waterloo, ON, Canada. Kapoeta is an achondrite meteorite that belongs to the howardite group, which along...nanodiamonds in CC material from the Kapoeta meteorite by Fourier-transform infrared (FTIR) and Raman...nanodiamonds and amorphous carbon found in this meteorite. References: [1] Zolensky M. E. et al. 1996. Meteoritics...State. Samples provided by the JSCâs Antarctic meteorite curatorial facility. 5214.pdf 76th Annual Meteoritical |  | | Journal (article/letter/editorial) | | parent bodies are sampled by the group. This meteorite is composed of rimmed chondrules, chondrule fragments...CV-CK-CO field. Other distinctive properties of this meteorite include the presence of abundant refractory inclusions...mildly altered CMs including Yamato (Y) 791198, Paris, Elephant Morraine (EET) 96029 and Jbilet Winselwan...chondrite parent bodies with CM-affinities. This meteorite has come to our attention because its bulk chemical...1992). LEW 85311 is classified as CM2 (Antarctic Meteorite Newsletter 2008, vol. 31). This study used three |  | | Journal (article/letter/editorial) | | CRPG, CNRS, UniversitĂ© de Lorraine, UMR 7358, Vandoeuvre-les-Nancy, F-54501, France a r t i c l e i n...performed at Centre de Recherches PĂ©trographiques et GĂ©ochimiques (CRPGCNRS, Nancy, France) using a JEOL JSM-6510...SX-100 electron microprobe at the University of Paris VI. Electron microprobe analyses of silicates were...standard materials (San Carlos olivine, magnetite, diopside, and fayalite) to: (i) deïŹne the mass fractionation...of iron meteorites derived from a carbonaceous meteorite reservoir to a late addition of W- and Mo-bearing |  | | Journal (article/letter/editorial) | | H. HEWINS1,3 1 Institut de Mineralogie, de Physique des Materiaux et de Cosmochimie, Sorbonne Universites...Universite Paris 06, UMR CNRS 7590, IRD, UMR 206, CP 52, 57 rue Cuvier, 75231 Paris Cedex 05, France 2 Department...the systematics of exsolution of pigeonite from diopside, while Humayun (2012) estimated cooling rates...the Museum national dâHistoire naturelle (MNHN, Paris). This fragment of Renazzo was scanned using a 100...performed at the Institut de Mineralogie, de Physique des Materiaux et de Cosmochimie (IMPMC, Universite |  | | Journal (article/letter/editorial) | | Schrader1,2* and Jemma Davidson3 1 Center for Meteorite Studies, School of Earth and Space Exploration...480-965-0720 Email: devin.schrader@asu.edu Center for Meteorite Studies School of Earth and Space Exploration...3 Electron Annexes) Key Words: CM chondrite, meteorite, chondrule, olivine, accretion, relict, aqueous... Queen Alexandra Range (QUE) 99177 (CR2) and Meteorite Hills (MET) 00426 (CR2) (e.g., Brearley, 1993;...thermally altered pre-accretionary minerals in more meteorite groups, it may be necessary (depending on scientific |  | Lee, Martin R., Lindgren, Paula, King, Ashley J., Greenwood, Richard C., Franchi, Ian A., Sparkes, Robert (2016) Elephant Moraine 96029, a very mildly aqueously altered and heated CM carbonaceous chondrite: Implications for the drivers of parent body processing. Geochimica et Cosmochimica Acta, 187. 237-259 doi:10.1016/j.gca.2016.05.008 | Journal (article/letter/editorial) | | and the fine-grained matrix indicates that this meteorite was aqueously altered in its parent body. Features...whilst still in the parent body regolith, the meteorite was heated to ~400â600 °C by impacts or solar...and water/hydroxyl contents, suggests that the meteorite contains lithologies that have undergone different...minerals are a major constituent of the finegrained meteorite matrix, and also occur within chondrules, calcium-...the CR3 and CO3 meteorites and the ungrouped meteorite Acfer 094, the matrix and fine-grained rims of |
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