{"id":4793,"date":"2015-05-22T22:53:44","date_gmt":"2015-05-22T20:53:44","guid":{"rendered":"http:\/\/karmaka.de\/?p=4793"},"modified":"2015-06-01T22:58:00","modified_gmt":"2015-06-01T20:58:00","slug":"organic-matter-evolution-on-asteroids-new-clues-from-paris","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=4793","title":{"rendered":"Organic Matter Evolution on Asteroids: New Clues from Paris"},"content":{"rendered":"<p>Remusat L, Vinogradoff V, Le Guillou C &#038; Bernard S<\/p>\n<p>Goldschmidt 2015, Prague, 16-21 August 2015<\/p>\n<p><a href=\"http:\/\/goldschmidt.info\/2015\/uploads\/abstracts\/origPDFs\/5155.pdf\" target=\"_blank\"><strong>PDF (abstract)<\/strong><\/a><\/p>\n<div class=\"su-quote su-quote-style-default\"><div class=\"su-quote-inner su-u-clearfix su-u-trim\">The Paris meteorite is the least altered CM carbonaceous<br \/>\nchondrite,  as  witnessed  by  the  presence  of  unaltered  metal<br \/>\ngrains  and  amorphous  silicate,  usually  absent  in  CM<br \/>\nchondrites  [1].  Its  O-isotopes  are  intermediate  between<br \/>\naltered CM and the thermally metamorphosed CO chondrites.<br \/>\nChondritic  organics  have  most  likely  a  multi-stage  history<br \/>\nthat  remains  complex  to  disentangle,  but  Paris  provides  a<br \/>\nunique opportunity to assess the specific role of parent body<br \/>\nprocesses on their evolution. Therefore, we have studied the<br \/>\ninsoluble  organic  matter  (IOM)  of  Paris  and  compared  it  to<br \/>\nIOM from Murchison and other CMs. By focusing on a single<br \/>\nchondrite group, we can rule out possible precursor influence<br \/>\nthat  we  encountered  in  a  previous  study  of  IOM  in<br \/>\ncarbonaceous chondrites from different groups [2].<br \/>\nWe obtained a \u201cbulk\u201d IOM of Paris by HF\/HCl digestion<br \/>\nof a large sample (>10g) of matrix isolated by the freeze-thaw<br \/>\nmethod  [1].  The  bulk  C,  H  and  N-isotope  compositions  of<br \/>\nParis  IOM  fall  among  the  heaviest  CM  chondrites.<br \/>\nNanoSIMS images of H and N-isotopes reveal numerous hot<br \/>\nspots.  D-rich  hot  spots  in  Paris  span  the  same  range  as  in<br \/>\nMurchison,  however  15 N-rich  hot  spots  are  significantly<br \/>\nheavier (mean value at 550\u2030, max at 1000\u2030), albeit lighter<br \/>\nthan in Bells [3]. The Raman signature points to a disordered<br \/>\nmaterial,  similar  to  type  1  and  2  chondrites  [4].  FTIR,<br \/>\nXANES and NMR reveal that Paris is intermediate between<br \/>\nCR2  and  CM2  IOMs.  In  particular,  they  show  that  the<br \/>\naliphatic\/aromatic  carbon  ratio   is  larger  in  Paris  than  in<br \/>\nMurchison.<br \/>\nOverall,  it  appears  that  during  aqueous  alteration  on  the<br \/>\nCM  parent  body,  IOM  underwent  some  degree  of<br \/>\naromatization in addition to slight D\/H decrease and a more<br \/>\nsignificant  15 N-rich hot spot depletion. Coupled hydrous and<br \/>\nthermal  effects  could  explain  this  evolution.  Paris  IOM<br \/>\nappears  primitive  with  respects  to  other  CM  and  could<br \/>\nresemble to the organic matter that accreted on the CM parent<br \/>\nbody. <\/div><\/div>\n","protected":false},"excerpt":{"rendered":"<p>Remusat L, Vinogradoff V, Le Guillou C &#038; Bernard S Goldschmidt 2015, Prague, 16-21 August 2015 PDF (abstract)<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,18,576],"tags":[106,105,743,1807,304],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4793"}],"collection":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/types\/post"}],"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=4793"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4793\/revisions"}],"predecessor-version":[{"id":4794,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4793\/revisions\/4794"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=4793"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=4793"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=4793"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}