{"id":12700,"date":"2017-06-06T21:52:16","date_gmt":"2017-06-06T19:52:16","guid":{"rendered":"http:\/\/karmaka.de\/?p=12700"},"modified":"2017-06-06T21:52:16","modified_gmt":"2017-06-06T19:52:16","slug":"measuring-the-level-of-interstellar-inheritance-in-the-solar-protoplanetary-disk","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=12700","title":{"rendered":"Measuring the level of interstellar inheritance in the solar protoplanetary disk"},"content":{"rendered":"<p>Conel M. O&#8217;D. Alexander,Larry R. Nittler,Jemma Davidson,Fred J. Ciesla<\/p>\n<p>Meteoritics &#038; Planetary Science. doi: 10.1111\/maps.12891<br \/>\nFirst published: 6 June 2017<\/p>\n<p><a href=\"http:\/\/onlinelibrary.wiley.com\/doi\/10.1111\/maps.12891\/full\">LINK<\/a><\/p>\n<p>&#8220;The timing and extent to which the initial interstellar material was thermally processed provide fundamental constraints for models of the formation and early evolution of the solar protoplanetary disk. We argue that the nonsolar (solar \u039417O \u2248 \u221229\u2030) and near-terrestrial (\u039417O \u2248 0\u2030) O-isotopic compositions of the Earth and most extraterrestrial materials (Moon, Mars, asteroids, and comet dust) were established very early by heating of regions of the disk that were modestly enriched (dust\/gas \u2265 5\u201310 times solar) in primordial silicates (\u039417O \u2248 \u221229\u2030) and water-dominated ice (\u039417O \u2248 24\u2030) relative to the gas. Such modest enrichments could be achieved by grain growth and settling of dust to the midplane in regions where the levels of turbulence were modest. The episodic heating of the disk associated with FU Orionis outbursts were the likely causes of this early thermal processing of dust. We also estimate that at the time of accretion the CI chondrite and interplanetary dust particle parent bodies were composed of ~5\u201310% of pristine interstellar material. The matrices of all chondrites included roughly similar interstellar fractions. Whether this interstellar material avoided the thermal processing experienced by most dust during FU Orionis outbursts or was accreted by the disk after the outbursts ceased to be important remains to be established.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Conel M. O&#8217;D. Alexander,Larry R. Nittler,Jemma Davidson,Fred J. Ciesla Meteoritics &#038; Planetary Science. doi: 10.1111\/maps.12891 First published: 6 June 2017 LINK &#8220;The timing and extent to which the initial interstellar material was thermally processed provide&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,10,72,65,71],"tags":[200,3905,3138],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12700"}],"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=12700"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12700\/revisions"}],"predecessor-version":[{"id":12701,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12700\/revisions\/12701"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=12700"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=12700"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=12700"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}