 | 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 |  | 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 |  | | 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 |  | 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...contains glass and/or quench crystallites, and a gehlenite-bearing calcium- and aluminium-rich inclusion...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- |  | | Journal (article/letter/editorial) | | aqueous alteration and thermal metamorphism in the meteorite parent bodies. To verify this hypothesis, we performed...following experiments. Hydrothermal experiments of gehlenite (Al-rich melilite) and plagioclase (An48) were...and 14 with a uniform Na concentration. In the gehlenite experiments, various amounts of SiO2 were added...10/6 mixtures of gehlenite/SiO2 at pH 7, 13, and14, and from a 10/10 mixture of gehlenite/SiO2 and plagioclase...hydroxycancrinite, were produced from the 10/6 mixture of gehlenite/SiO2, and fabriesite from plagioclase. Isothermal |  | | 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...describe sodalite in the CM carbonaceous chondrite Meteorite Hills (MET) 01075. This mineral has not been previously...from pure standards of minerals present in the meteorite for 30 min. Phase quantification used an XRD pattern...MT75-1, we first discuss the history of its host meteorite with a focus on the three most obvious effects |  | | Journal (article/letter/editorial) | | Chaussidon a, Christa Göpel c, Typhoon Lee d a Centre de Recherches PĂ©trographiques et GĂ©ochimiques, CNRS...des Pauvres, BP20, 54501 Vandoeuvre-lĂšs-Nancy, France Institute of Astronomy and Astrophysics, Academia...Institut de Physique du Globe, Sorbonne Paris CitĂ©, Univ Paris Diderot, CNRS UMR 7154, F-75005 Paris, France...inclusions extracted from CM2 meteorites Murchion and Paris were measured with a Cameca 1280 HR2 ion microprobe...hand-picked from an acid residue of the Murchison meteorite prepared at the University of Chicago (Courtesy |  | | Journal (article/letter/editorial) | | Superimposed Processes in Chondrules of the Ochansk Meteorite A. I. Bakhtin, R. Kh. Sungatullin, A. V. Gusev..... 6199 A Multi-Technique Analysis of the Paris Meteorite to Characterize its Organic Content âIn Situâ............................. 6230 Influence of Meteorite Structure on Nanotubes and Nanocrystals Synthesis...Heat and Aqueous Alteration Experienced by the Paris CM Chondrite L. Bonal, P. Beck, T. Nakamura, Y....Material F. E. Brenker, L. Vincze, B. Vekemans, E. de Pauw, B. Tkalcec, and G. Falkenberg ............ |  | | Journal (article/letter/editorial) | | Zanda3. 1Ecole Normale SupeÌrieure de Lyon, 69007 Lyon, France. E-mail: albarede@ens-lyon.fr. 2American...3MuseÌum National dâHistoire Naturelle, 75005 Paris, France. Introduction: Very few measurements of natural...isotopic variability in troilite within a same meteorite, our data are consistent with literature results:...E. Charon1,4. 1CSNSM, CNRS/IN2P3, Orsay Campus, France. E-mail: Jerome.Aleon@csnsm.in2p3.fr. 2Department...Geoinstitut, Bayreuth, Germany. 4Laboratoire de GeÌologie, ENS Paris, France. 5367 PARENT BODY MODIFICATION OF |  | | Journal (article/letter/editorial) | | Meteoritical Society (2015) 5231.pdf THE MINNESOTA METEORITE MYSTERY: TWO UNRELATED VERY FLAT IRONS E. C. Alexander...of the Arlington site. It was identified as a meteorite by the first author in June 2013 and named High...meteorites described here, the only other iron meteorite with a similar shape is Tawallah Valley, a IVB...â 2.16 g/cm3) is 93 ppm relative to the bulk meteorite and AO comprises 38 % of the parent fraction AL...Introduction: ALM-A (Almahata Sitta trachyandesitic meteorite) is a 24.2 gram SiO2-rich volcanic rock from the |  | | 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 |  | | 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) | | spinel+forsterite objects from the CM chondrite Paris. We note that at least one RMN from LT1 is dominated...was found in a CAI in the Isheyevo CH/CB-like meteorite (Grokhovsky 2006; Meibom et al. 2007). Osbornite...anorthite, and Al,Ti clinopyroxene. In the Paris meteorite, which is believed to be the most pristine...hibonite, perovskite, and grossite) with a mantle of gehlenite which is overlain by anorthite and diopside/fassaite...anorthite, Per = perovskite, Mel = melilite, Geh = gehlenite, Cpx = clinopyroxene, Hib = hibonite, Cor = corundum |  | | Journal (article/letter/editorial) | | features may be preserved. Most prominently, CM Paris reveals some of these pre-accretionary features...FIB sections retrieved from the matrix of each meteorite using a Talos F200X. All observations were conducted...records similar degrees of thermal metamorphism as Paris and QUE 97990 [e.g., 14], while LAP 02333 has been... [14] Schrader & Davidson (submitted) GCA. METEORITE MATERIAL MODEL FOR STRUCTURAL PROPERTIES Parul...needed to achieve this objective. At present, the meteorite material found on earth are the only objects from |  | | Journal (article/letter/editorial) | | OF THE METALLIC PHASES IN THE ALMAHATA SITTA METEORITE (FRAGMENT#051). Y. A. Abdu1, A. M. Gismelseed2...Khartoum, Sudan. Introduction: The Almahata Sitta meteorite fall was unique because asteroid 2008 TC3, the...alwmark@geol.lu.se), 2Centro de Astrobiologia (INTA-CSIC), 28850 Torrejon de Ardoz, Spain, 3University of...the event reported the presence of the following de novo geomorphological features in the impact area...funnel-like hole in the ground at the end of the de novo dry groove conventionally named âdry riverâ; |  | | Journal (article/letter/editorial) | | the IMACNMNC, including 17 from the Allende CV3 meteorite (Ma, 2015a) and high-pressure phases such as bridgmanite...shannonite peridot; chrysolite paqueite perrierite gehlenite melilite pumpellyite thortveitite wadsleyite cyclosilicates...ïŹuor-richterite forsterite galena galileiite gehlenite geikielite gentnerite (not approved) gersdorfïŹte...Ca pyroxene (diopside), forsterite, enstatite, gehlenite (Ca2 Al(Si,Al) 2 O7 ), Ă„kermanite (Ca2 Al(Si,Al)...sources plausibly responsible for the bulk of meteorite metamorphism and melting: (1) the decay of shortlived |
|
