{"id":2434,"date":"2014-11-25T17:57:39","date_gmt":"2014-11-25T16:57:39","guid":{"rendered":"http:\/\/karmaka.de\/?page_id=2434"},"modified":"2021-07-19T10:23:06","modified_gmt":"2021-07-19T08:23:06","slug":"paris","status":"publish","type":"page","link":"https:\/\/karmaka.de\/?page_id=2434","title":{"rendered":"Paris"},"content":{"rendered":"
<\/div>\n

PARIS<\/span><\/strong><\/p>\n

THIS PAGE WILL BE UPDATED VERY SOON.<\/strong><\/p>\n

Meteoritical Bulletin *<\/strong><\/a>:<\/strong><\/p>\n

Paris<\/p>\n

19\u00b047.139\u2019N, 55\u00b051.21\u2019E<\/p>\n

Unknown location Find: 2001 Carbonaceous chondrite (CM)<\/p>\n

History: This sample was in an auction box lot bought by Jean-Jacques Corr\u00e9 at the Hotel des Ventes in Paris. The box was part of the estate of Jean Simon Colonna-Cimera, an “Ing\u00e9nieur des Mines,” who supervised mines in foreign countries and in the French Colonies. Corr\u00e9 thought that the stone might be a meteorite but kept it for 7 years before attempting to have it identified. Physical characteristics: One complete, fresh stone weighing 1.370 kg and covered with a very black fusion crust (Fig. 6). Petrography: (M. Bourot-Denise, B. Zanda, MNHNP): The stone contains abundant metal and refractory inclusions up to 800 \u03bcm in size. The chondrules (up to 1 mm in size) are well preserved, although their mesostases are altered to phyllosilicates. The finegrained matrix is heterogeneous and contains zones with abundant sulfides (pyrrhotite and pentlandite), zones with magnetites, and zones with PCPs. Geochemistry: Olivine (Fa0.2\u201355, CaO = 0.35, Cr2O3 = 0.35); low-Ca pyroxene (Fs0.6\u20134.4). Minor phases: kamacite (average: Ni = 5.5, Co = 0.22), tochilinite, pyrrhotite, pentlandite, magnetite (pure Fe3O4); calcite and PCPs (average: FeO = 52, SiO2 = 12, S = 9). (EPMA and expressed in wt%). Oxygen isotopes: \u03b418O=3.34\u2030, \u03b417O= -1.37\u2030. Classification: Carbonaceous chondrite (CM), no signs of terrestrial weathering or shock (chondrules are perfectly spherical). Chondrules are more abundant and phyllosilicates less abundant than in CM2s. PCP averages 4.51 for FeO\u2044SiO2 and 0.77 for S\u2044SiO2, well out of the ranges defined by Rubin et al. (2007), making Paris significantly less aqueously altered than any known CM2. Oxygen isotopes also place it toward the least hydrated end of CM chondrites. Specimens: The mass of 1.275 kg and one thin section are on deposit at MNHNP.<\/div><\/div>\n

Oxygen isotope plot:<\/strong><\/span><\/p>\n

\"\"<\/a><\/p>\n

Scientific literature:<\/strong><\/span><\/p>\n

Paris vs. Murchison: Impact of hydrothermal alteration on organic matter in CM chondrites<\/strong>
\nV. Vinogradoff, C. Le Guillou, S. Bernard, L. Binet, P. Cartigny, A.J. Brearley, L. Remusat
\nGeochimica et Cosmochimica Acta
\nIn Press, Accepted Manuscript, Available online 12 June 2017
\nabstract<\/strong><\/a><\/p>\n

Mineralogical, crystallographic and redox features of the earliest stages of fluid alteration in CM chondrites<\/strong>
\nIsabella Pignatelli, Yves Marrocchi, Enrico Mugnaioli, Franck Bourdelle, Matthieu Gounelle
\nGeochimica et Cosmochimica Acta
\nAvailable online 19 April 2017
\nabstract<\/strong><\/a><\/p>\n

Non Destructive IR Micro-Imaging of the Paris Meteorite<\/strong>
\nZ. Dionnet, A. Al\u00e9on-Toppani, F. Borondics, R. Brunetto, Z. Djouadi, D. Troadec
\n48th Lunar and Planetary Science Conference (2017), Abstract #1466
\nabstract<\/strong><\/a><\/p>\n

Oxygen Isotope Systematics of Chondrules from the Paris CM2 Chondrite<\/strong>
\nN. Chaumard, C. Defouilloy, N. T. Kita, A. Hertwig
\n48th Lunar and Planetary Science Conference (2017), Abstract #1610
\nabstract<\/strong><\/a><\/p>\n

Water in type I chondrules of Paris CM chondrite<\/strong>
\nA. Stephant, L. Remusat, F. Robert
\nGeochimica et Cosmochimica Acta
\nIn Press, Accepted Manuscript, Available online 25 November 2016
\nabstract<\/strong><\/a><\/p>\n

Inward Radial Mixing of Interstellar Water Ices in the Solar Protoplanetary Disk<\/strong>
\nLionel G. Vacher, Yves Marrocchi, Maximilien J. Verdier-Paoletti, Johan Villeneuve, and Matthieu Gounelle
\nThe Astrophysical Journal Letters, Volume 827, Number 1, published 2016 August 2
\nabstract<\/strong><\/a><\/p>\n

GEMS-like material in the matrix of the Paris meteorite and the early stages of alteration of CM chondrites<\/strong>
\nH. Leroux, P. Cuvillier, B. Zanda, R.H. Hewins
\nIn Press, Accepted Manuscript, Available online 28 September 2015
\nabstract<\/strong><\/a><\/p>\n

An American on Paris: Extent of aqueous alteration of a CM chondrite and the petrography of its refractory and amoeboid olivine inclusions<\/strong>
\nRubin, A. E.
\nMeteoritics & Planetary Science. doi: 10.1111\/maps.12482
\nabstract<\/strong><\/a><\/p>\n

The Insoluble Organic Matter of the Paris CM Chondrite<\/strong>
\nVinogradoff V., Remusat L., Bernard S., Le Guillou C.
\n78th Annual Meeting of the Meteoritical Society (2015)
\nBerkeley, USA, July 27-31 2015
\nPDF (abstract)<\/strong><\/a><\/p>\n

The amino acid and hydrocarbon contents of the Paris meteorite:
\nInsights into the most primitive CM chondrite<\/strong>
\nZita Martins, Paola Modica, Brigitte Zanda and Louis Le Sergeant d\u2019Hendecourt
\nMeteoritics & Science Planetary<\/em> 1-18 (2015)
\nArticle first published online: 20 APR 2015 | DOI: 10.1111\/maps.12442
\nPDF<\/strong><\/a><\/p>\n

Oxygen Isotopic Composition of an Unusual Clast in the Paris CM Meteorite<\/strong>
\nMostefaoui, S.; Caillet Komorowski, C.; Boudouma, O.; Godard, G.; Fialin, M.
\n77th Annual Meeting of the Meteoritical Society, held September 7–12, 2014 in Casablanca, Morocco. LPI Contribution No. 1800, id.5267 (09\/2014)
\nPDF LINK<\/strong><\/a><\/p>\n

The Paris CM chondrite: Secondary minerals and asteroidal processing<\/strong>
\nMarrocchi, Yves; Gounelle, Matthieu; Blanchard, Ingrid; Caste, Florent; Kearsley, Anton T.
\nMeteoritics & Planetary Science, Volume 49, Issue 7, pages 1232\u20131249, July 2014
\nLINK<\/strong><\/a><\/p>\n

A TEM Study of Exsolution in Ca-Rich Pyroxenes from the Paris Meteorite: Determination of Type I Chondrule Cooling Rates<\/strong>
\nCuvillier, P.; Chaumard, N.; Leroux, H.; Zanda, B.; Hewins, R. H.; Jacob, D.; Devouard, B.
\n45th Lunar and Planetary Science Conference, held 17-21 March, 2014 at The Woodlands, Texas. LPI Contribution No. 1777, p.1711
\nPDF LINK<\/strong><\/a><\/p>\n

Sub-Micrometer Composition Fields of Acfer 094 and Paris Matrices<\/strong>
\nLeroux, H.; Cuvillier, P.; Zanda, B.; Hewins, R. H.
\n45th Lunar and Planetary Science Conference, held 17-21 March, 2014 at The Woodlands, Texas. LPI Contribution No. 1777, p.1706 (03\/2014)
\nPDF LINK<\/strong><\/a><\/p>\n

Degree of Aqueous Alteration in CM2 Paris and the Petrography of its Refractory and Amoeboid Olivine Inclusions<\/strong>
\nRubin, A. E.
\n45th Lunar and Planetary Science Conference, held 17-21 March, 2014 at The Woodlands, Texas. LPI Contribution No. 1777, p.1130 (03\/2014)
\nPDF LINK<\/strong><\/a><\/p>\n

The Paris meteorite, the least altered CM chondrite so far<\/strong>
\nHewins, Roger H.; Bourot-Denise, Mich\u00e8le; Zanda, Brigitte; Leroux, Hugues; Barrat, Jean-Alix; Humayun, Munir; G\u00f6pel, Christa; Greenwood, Richard C.; Franchi, Ian A.; Pont, Sylvain; and 7 coauthors
\nGeochimica et Cosmochimica Acta, Volume 124, 1 January 2014, Pages 190\u2013222
\nPDF LINK<\/strong><\/a><\/p>\n

Correlated Petrologic and Mg-Isotopic Studies of an Unusual Igneous Fragment in the Paris CM Chondrite<\/strong>
\nCaillet Komorowski, C.; Mostefaoui, S.; Boudouma, O.; Godard, G.; Fialin, M.
\n76th Annual Meeting of the Meteoritical Society, held July 29-August 7, 2013 in Edmonton, Canada. Published in Meteoritics and Planetary Science Supplement, id.5199 (09\/2013)
\nPDF LINK<\/strong><\/a><\/p>\n

The Soluble Organic Content of the Paris Meteorite — The Most Primitive CM Chondrite<\/strong>
\nMartins, Z.; Modica, P.; Sephton, M. A.; Zanda, B.; d’Hendecourt, L. 76th Annual Meeting of the Meteoritical Society, held July 29-August 7, 2013 in Edmonton, Canada. Published in Meteoritics and Planetary Science Supplement, id.5115 (09\/2013)
\nPDF LINK<\/strong><\/a><\/p>\n

A TEM Investigation of the Fine-Grained Matrix of the Paris CM Chondrite<\/strong>
\nLeroux, H.; Cuvillier, P.; Zanda, B.; Hewins, R. H.
\n44th Lunar and Planetary Science Conference, held March 18-22, 2013 in The Woodlands, Texas. LPI Contribution No. 1719, p.1528 (03\/2013)
\nPDF LINK<\/strong><\/a><\/p>\n

Hydrogen Isotopic Compositions and Water Contents in Type I Chondrules of Paris CM Chondrite<\/strong>
\nStephant, A.; R\u00e9musat, L.; Robert, F.
\n44th Lunar and Planetary Science Conference, held March 18-22, 2013 in The Woodlands, Texas. LPI Contribution No. 1719, p.1560 (03\/2013)
\nPDF LINK<\/strong><\/a><\/p>\n

Hydrocarbon Materials of Likely Interstellar Origin from the Paris Meteorite<\/strong>
\nS. Merouane, Z. Djouadi, L. Le Sergeant d’Hendecourt, B. Zanda, and J. Borg
\nThe Astrophysical Journal, Volume 756, Number 2
\nLINK (open access)<\/strong><\/a><\/p>\n

Cluster Ion Imaging of the \u2019\u2019Paris\u2019\u2019 Meteorite<\/strong>
\nM. Noun, B. Nsouli , D. Baklouti , R. Brunetto, F. Jamme, C. Sandt , P. Dumas , L. d\u2019Hendecourt, and S. Della-Negra
\nPDF LINK<\/strong><\/a><\/p>\n

VIDEO<\/strong><\/span><\/p>\n

‘Paris’ presented by B. Zanda in the French evening news 20 heures<\/em> on channel France 2<\/em> (2 February 2010)<\/strong>
\nVIDEO<\/strong><\/a><\/p>\n

B. Zanda talks about ‘Paris’ in her presentation
\nLes m\u00e9t\u00e9orites, t\u00e9moins de la formation du Soleil et des plan\u00e8tes <\/em>
\nduring Les Mardis de l’Espace des sciences<\/em> on 15 December 2009 (20:32 – 22:33 min.)<\/strong>
\nVIDEO<\/strong><\/a><\/p>\n

AUDIO<\/strong><\/span><\/p>\n

La m\u00e9t\u00e9orite Paris : mieux conna\u00eetre l\u2019\u00e2ge du syst\u00e8me solaire ?<\/strong>
\nAvec les cosmochimistes Brigitte Zanda et Matthieu Gounelle au Mus\u00e9um National d\u2019Histoire Naturelle
\nCanal Acad\u00e9mie (16:49 min.)
\nAUDIO<\/strong><\/a><\/p>\n","protected":false},"excerpt":{"rendered":"

PARIS THIS PAGE WILL BE UPDATED VERY SOON. Meteoritical Bulletin *: Oxygen isotope plot: Scientific literature: Paris vs. Murchison: Impact of hydrothermal alteration on organic matter in CM chondrites V. Vinogradoff, C. Le Guillou, S….<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":64,"menu_order":0,"comment_status":"open","ping_status":"open","template":"page-template-wide.php","meta":{"footnotes":""},"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/pages\/2434"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=2434"}],"version-history":[{"count":33,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/pages\/2434\/revisions"}],"predecessor-version":[{"id":28432,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/pages\/2434\/revisions\/28432"}],"up":[{"embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/pages\/64"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=2434"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}