{"id":16927,"date":"2018-12-13T18:29:28","date_gmt":"2018-12-13T17:29:28","guid":{"rendered":"http:\/\/karmaka.de\/?p=16927"},"modified":"2018-12-13T19:07:54","modified_gmt":"2018-12-13T18:07:54","slug":"iron-isotope-constraints-on-planetesimal-core-formation-in-the-early-solar-system","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=16927","title":{"rendered":"Iron Isotope Constraints on Planetesimal Core Formation in the Early Solar System"},"content":{"rendered":"\n<p>Michelle K. Jordan, HaoLan Tang, Issaku E. Kohl, Edward D. Young<\/p>\n\n\n\n<p>Geochimica et Cosmochimica Acta<\/p>\n\n\n\n<p><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/pii\/S0016703718306884\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;We determined the Fe isotope fractionation between the metal and silicate phases of two aubrite meteorites, Norton County and Mount Egerton. We find that the metallic phase is high in 57Fe\/54Fe with respect to the silicate phase, with \u039457Femetal-silicate = 0.08\u2030 \u00b1 0.04 for Mount Egerton and 0.09 \u00b1 0.02 \u2030 for Norton County. These data, combined with new measurements of 57Fe\/54Fe of IIIAB iron meteorites, are used to constrain the origins of the high 57Fe\/54Fe exhibited by all classes of iron meteorites. We find that if the parent bodies of the iron meteorites had chondritic bulk 57Fe\/54Fe values, their cores must have been unusually small (\u2264 8% by mass). Relaxing the constraint that the bodies were chondritic in their bulk iron isotope ratios allows for larger core mass fractions commensurate with usual expectations. In this case, the elevated 57Fe\/54Fe values of iron meteorites are due in part to evaporation of melt during the accretion stages of the parent bodies and not solely the result of metal-silicate differentiation.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Michelle K. Jordan, HaoLan Tang, Issaku E. Kohl, Edward D. Young Geochimica et Cosmochimica Acta LINK &#8220;We determined the Fe isotope fractionation between the metal and silicate phases of two aubrite meteorites, Norton County and&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[28,38,1038,214,420],"tags":[4779,1826,1541,807,3858,257,1262],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16927"}],"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=16927"}],"version-history":[{"count":2,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16927\/revisions"}],"predecessor-version":[{"id":16929,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16927\/revisions\/16929"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=16927"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=16927"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=16927"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}