{"id":12803,"date":"2017-06-13T00:41:11","date_gmt":"2017-06-12T22:41:11","guid":{"rendered":"http:\/\/karmaka.de\/?p=12803"},"modified":"2017-06-13T00:41:11","modified_gmt":"2017-06-12T22:41:11","slug":"age-of-jupiter-inferred-from-the-distinct-genetics-and-formation-times-of-meteorites","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=12803","title":{"rendered":"Age of Jupiter inferred from the distinct genetics and formation times of meteorites"},"content":{"rendered":"<p>Thomas S. Kruijer, Christoph Burkhardt, Gerrit Budde, and Thorsten Kleine<\/p>\n<p>PNAS2017 ; published ahead of print June 12, 2017, doi:10.1073\/pnas.1704461114 <\/p>\n<p><a href=\"http:\/\/www.pnas.org\/content\/early\/2017\/06\/06\/1704461114.abstract\" target=\"_blank\"><strong>LINK<\/strong><\/a><\/p>\n<p>&#8220;The age of Jupiter, the largest planet in our Solar System, is still unknown. Gas-giant planet formation likely involved the growth of large solid cores, followed by the accumulation of gas onto these cores. Thus, the gas-giant cores must have formed before dissipation of the solar nebula, which likely occurred within less than 10 My after Solar System formation. Although such rapid accretion of the gas-giant cores has successfully been modeled, until now it has not been possible to date their formation. Here, using molybdenum and tungsten isotope measurements on iron meteorites, we demonstrate that meteorites derive from two genetically distinct nebular reservoirs that coexisted and remained spatially separated between \u223c1 My and \u223c3\u20134 My after Solar System formation. The most plausible mechanism for this efficient separation is the formation of Jupiter, opening a gap in the disk and preventing the exchange of material between the two reservoirs. As such, our results indicate that Jupiter\u2019s core grew to \u223c20 Earth masses within <1 My, followed by a more protracted growth to \u223c50 Earth masses until at least \u223c3\u20134 My after Solar System formation. Thus, Jupiter is the oldest planet of the Solar System, and its solid core formed well before the solar nebula gas dissipated, consistent with the core accretion model for giant planet formation. \"\n<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Thomas S. Kruijer, Christoph Burkhardt, Gerrit Budde, and Thorsten Kleine PNAS2017 ; published ahead of print June 12, 2017, doi:10.1073\/pnas.1704461114 LINK &#8220;The age of Jupiter, the largest planet in our Solar System, is still unknown&#8230;.<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[214],"tags":[1874,2267,2572,3930,1735],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12803"}],"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=12803"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12803\/revisions"}],"predecessor-version":[{"id":12804,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/12803\/revisions\/12804"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=12803"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=12803"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=12803"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}