{"id":5043,"date":"2015-06-19T07:43:39","date_gmt":"2015-06-19T05:43:39","guid":{"rendered":"http:\/\/karmaka.de\/?p=5043"},"modified":"2015-06-21T13:39:37","modified_gmt":"2015-06-21T11:39:37","slug":"pb-pb-dating-of-individual-chondrules-from-the-cba-chondrite-gujba-assessment-of-the-impact-plume-formation-model","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=5043","title":{"rendered":"Pb-Pb dating of individual chondrules from the CBa chondrite Gujba: Assessment of the impact plume formation model"},"content":{"rendered":"<p>Bollard, J., Connelly, J. N. and Bizzarro, M.<\/p>\n<p>Meteoritics &#038; Planetary Science. doi: 10.1111\/maps.12461<\/p>\n<p><a href=\"http:\/\/onlinelibrary.wiley.com\/doi\/10.1111\/maps.12461\/abstract\" 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\">The CB chondrites are metal-rich meteorites with characteristics that sharply distinguish them from other chondrite groups. Their unusual chemical and petrologic features and a young formation age of bulk chondrules dated from the CBa chondrite Gujba are interpreted to reflect a single-stage impact origin. Here, we report high-precision internal isochrons for four individual chondrules of the Gujba chondrite to probe the formation history of CB chondrites and evaluate the concordancy of relevant short-lived radionuclide chronometers. All four chondrules define a brief formation interval with a weighted mean age of 4562.49 \u00b1 0.21 Myr, consistent with its origin from the vapor-melt impact plume generated by colliding planetesimals. Formation in a debris disk mostly devoid of nebular gas and dust sets an upper limit for the solar protoplanetary disk lifetime at 4.8 \u00b1 0.3 Myr. Finally, given the well-behaved Pb-Pb systematics of all four chondrules, a precise formation age and the concordancy of the Mn-Cr, Hf-W, and I-Xe short-lived radionuclide relative chronometers, we propose that Gujba may serve as a suitable time anchor for these systems.<\/div><\/div>\n","protected":false},"excerpt":{"rendered":"<p>Bollard, J., Connelly, J. N. and Bizzarro, M. Meteoritics &#038; Planetary Science. doi: 10.1111\/maps.12461 LINK<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[584,56,148,582,72,68],"tags":[1426,1644,1643,1645,649,274,1848,762],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/5043"}],"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=5043"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/5043\/revisions"}],"predecessor-version":[{"id":5044,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/5043\/revisions\/5044"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=5043"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=5043"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=5043"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}