{"id":317,"date":"2014-08-19T11:01:14","date_gmt":"2014-08-19T09:01:14","guid":{"rendered":"http:\/\/karmaka.de\/?p=317"},"modified":"2014-10-21T21:42:31","modified_gmt":"2014-10-21T19:42:31","slug":"solar-system-chemical-abundances-corrected-for-systematics","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=317","title":{"rendered":"Solar system chemical abundances corrected for systematics"},"content":{"rendered":"<div style=\"width: 810px\" class=\"wp-caption alignleft\"><a href=\"http:\/\/upload.wikimedia.org\/wikipedia\/commons\/e\/e6\/SolarSystemAbundances.png\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/upload.wikimedia.org\/wikipedia\/commons\/e\/e6\/SolarSystemAbundances.png\" alt=\"\" width=\"800\" height=\"357\" \/><\/a><p class=\"wp-caption-text\"><strong>(STOCK IMAGE) Numerical data from: Katharina Lodders (2003). &#8220;SOLAR SYSTEM ABUNDANCES AND CONDENSATION TEMPERATURES OF THE ELEMENTS&#8221;. The Astrophysical Journal 591: 1220\u20131247<\/strong><\/p><\/div>\n<p>Guillermo Gonzalez<\/p>\n<p>MNRAS (September 1, 2014) 443 (1): L99-L103. doi: 10.1093\/mnrasl\/slu083<br \/>\nFirst published online July 10, 2014<\/p>\n<p><a href=\"http:\/\/arxiv.org\/abs\/1406.0480\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<p><a href=\"http:\/\/arxiv.org\/pdf\/1406.0480v1.pdf\"><strong>PDF-LINK<\/strong><\/a><\/p>\n<blockquote><p>It has been assumed that CI chondrite meteorites are<br \/>\nthe least affected by fractionation processes, given their<br \/>\nhigher volatile\/refractory ratio than other meteorite classes<br \/>\n(Lodders et al. 2009). However, it had not been demon-<br \/>\nstrated that the CI chondrites are completely lacking in<br \/>\nfractionation effects for elements more refractory than H,<br \/>\nC, N and O relative to the primordial state. If our \fnding is<br \/>\nconrrmed, then a mechanism for this fractionation will need<br \/>\nto be sought.<\/p><\/blockquote>\n","protected":false},"excerpt":{"rendered":"<p>Guillermo Gonzalez MNRAS (September 1, 2014) 443 (1): L99-L103. doi: 10.1093\/mnrasl\/slu083 First published online July 10, 2014 LINK PDF-LINK It has been assumed that CI chondrite meteorites are the least affected by fractionation processes, given&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[156,71,142],"tags":[],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/317"}],"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=317"}],"version-history":[{"count":2,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/317\/revisions"}],"predecessor-version":[{"id":319,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/317\/revisions\/319"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=317"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=317"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=317"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}