{"id":11363,"date":"2017-01-29T15:10:51","date_gmt":"2017-01-29T14:10:51","guid":{"rendered":"http:\/\/karmaka.de\/?p=11363"},"modified":"2017-01-29T15:10:51","modified_gmt":"2017-01-29T14:10:51","slug":"a-magmatic-origin-for-silica-rich-glass-inclusions-hosted-in-porphyritic-magnesian-olivines-in-chondrules-an-experimental-study","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=11363","title":{"rendered":"A magmatic origin for silica-rich glass inclusions hosted in porphyritic magnesian olivines in chondrules: an experimental study"},"content":{"rendered":"<p>Fran\u00e7ois Faure, Laurent Tissandier, L\u00e9a Florentin, Karine Devineau<\/p>\n<p>Geochimica et Cosmochimica Acta<br \/>\nIn Press, Accepted Manuscript, Available online 29 January 2017<\/p>\n<p><a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S0016703717300480\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<p>&#8220;Rare silica-rich glass inclusions (69 < SiO2 < 82 wt.%) are described within magnesian olivines of porphyritic Type IA chondrules. These glass inclusion compositions are clearly out of equilibrium with their host Mg-olivines and their presence within the olivines is generally attributed to an unclear secondary process such as a late interaction with nebular gases. We performed dynamic crystallisation experiments that demonstrate that these Si-rich glass inclusions are actually magmatic in origin and were trapped inside olivines that crystallized slowly from a magma with a CI, i.e. solar, composition. Their silica-rich compositions are the consequence of the small volumes of inclusions, which inhibit the nucleation of secondary crystalline phase (Ca-poor pyroxene) but allow olivine to continue to crystallize metastably on the walls of the inclusions. We suggest that Si-rich glass inclusions could be the only reliable relicts of what were the first magmas of the solar system, exhibiting a CI, i.e. non-fractionated, composition.\"\n<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Fran\u00e7ois Faure, Laurent Tissandier, L\u00e9a Florentin, Karine Devineau Geochimica et Cosmochimica Acta In Press, Accepted Manuscript, Available online 29 January 2017 LINK &#8220;Rare silica-rich glass inclusions (69 < SiO2 < 82 wt.%) are described within...\n<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[56,578],"tags":[1839,3277,3565,3564],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/11363"}],"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=11363"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/11363\/revisions"}],"predecessor-version":[{"id":11364,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/11363\/revisions\/11364"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=11363"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=11363"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=11363"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}