{"id":17925,"date":"2019-02-25T21:49:48","date_gmt":"2019-02-25T20:49:48","guid":{"rendered":"http:\/\/karmaka.de\/?p=17925"},"modified":"2019-02-25T21:49:49","modified_gmt":"2019-02-25T20:49:49","slug":"dissipation-of-the-solar-systems-debris-disk-recorded-in-primitive-meteorites","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=17925","title":{"rendered":"Dissipation of the Solar System\u2019s debris disk recorded in primitive meteorites"},"content":{"rendered":"\n<p>Jamie D. Gilmour &amp; Michal J. Filtness<\/p>\n\n\n\n<p>Nature Astronomy, 1\u20136<br>\nPublished: 25 February 2019<\/p>\n\n\n\n<p><a href=\"https:\/\/www.nature.com\/articles\/s41550-019-0696-0\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;Many newly formed Sun-like stars show evidence of debris disks composed of dust generated through destructive collisions among residual planetesimals. These are inferred to survive at a detectable level over the first ~100\u2009Myr of their parent star\u2019s lifetime. We hypothesize that the most primitive meteorites were processed as a result of impacts as our Solar System\u2019s debris disk dissipated, rather than as a result of heat generated by decay of 26Al. We show how the iodine\u2013xenon (I\u2013Xe) record from chondrules in the Chainpur meteorite supports this hypothesis, and use it to constrain the decline in the impact rate. We demonstrate that it is the creation of I\u2013Xe sites during compaction that is recorded by the chondrule dataset. We show that, to account for the broader I\u2013Xe record from primitive material, a consistent picture requires that the dissipation of our Solar System\u2019s debris disk had a timescale of around 40\u201350\u2009Myr in this period. Against this backdrop, the late addition of siderophiles to the Earth in a single large impact may represent a rare phenomenon in planetary system formation that has been anthropically selected.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Jamie D. Gilmour &amp; Michal J. Filtness Nature Astronomy, 1\u20136 Published: 25 February 2019 LINK &#8220;Many newly formed Sun-like stars show evidence of debris disks composed of dust generated through destructive collisions among residual planetesimals&#8230;.<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[56,72,24,7,71],"tags":[238,3071,1839,3701,378,1816,1452,1807,1592,1850],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17925"}],"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=17925"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17925\/revisions"}],"predecessor-version":[{"id":17926,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/17925\/revisions\/17926"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=17925"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=17925"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=17925"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}