{"id":4177,"date":"2015-03-25T14:58:15","date_gmt":"2015-03-25T13:58:15","guid":{"rendered":"http:\/\/karmaka.de\/?p=4177"},"modified":"2015-03-25T16:19:11","modified_gmt":"2015-03-25T15:19:11","slug":"early-stages-of-core-segregation-recorded-by-fe-isotopes-in-an-asteroidal-mantle","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=4177","title":{"rendered":"Early stages of core segregation recorded by Fe isotopes in an asteroidal mantle"},"content":{"rendered":"<p>J.A. Barrat, O. Rouxel, K. Wang, F. Moynier, A. Yamaguchi, A. Bischoff, J. Langlade<\/p>\n<p>Earth and Planetary Science Letters<br \/>\nVolume 419, 1 June 2015, Pages 93\u2013100<\/p>\n<p><a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S0012821X15001697\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<div class=\"su-quote su-quote-style-default\"><div class=\"su-quote-inner su-u-clearfix su-u-trim\"><\/div><\/div>Ureilite meteorites are achondrites that are debris of the mantle of a now disrupted differentiated asteroid rich in carbon. They provide a unique opportunity to study the differentiation processes of such a body. We analyzed the iron isotopic compositions of 30 samples from the Ureilite Parent Body (UPB) including 29 unbrecciated ureilites and one ureilitic trachyandesite (ALM-A) which is at present the sole large crustal sample of the UPB. The \u03b456Fe of the whole rocks fall within a restricted range, from 0.01 to 0.11\u2030, with an average of +0.056\u00b10.008\u2030+0.056\u00b10.008\u2030, which is significantly higher than that of chondrites. We show that this difference can be ascribed to the segregation of S-rich metallic melts at low degrees of melting at a temperature close to the Fe\u2013FeS eutectic, and certainly before the onset of the melting of the silicates (View the MathML source<1100\u00b0C), in agreement with the marked S depletions, and the siderophile element abundances of the ureilites. These results point to an efficient segregation of S-rich metallic melts during the differentiation of small terrestrial bodies.[\/su_quote]\n","protected":false},"excerpt":{"rendered":"<p>J.A. Barrat, O. Rouxel, K. Wang, F. Moynier, A. Yamaguchi, A. Bischoff, J. Langlade Earth and Planetary Science Letters Volume 419, 1 June 2015, Pages 93\u2013100 LINK Ureilite meteorites are achondrites that are debris of&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[28,77,39],"tags":[781,1854,462,237,245,1163],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4177"}],"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=4177"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4177\/revisions"}],"predecessor-version":[{"id":4178,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/4177\/revisions\/4178"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=4177"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=4177"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=4177"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}