{"id":7988,"date":"2016-03-09T18:32:36","date_gmt":"2016-03-09T17:32:36","guid":{"rendered":"http:\/\/karmaka.de\/?p=7988"},"modified":"2016-03-09T18:37:40","modified_gmt":"2016-03-09T17:37:40","slug":"pallasite-paleomagnetism-quiescence-of-a-core-dynamo","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=7988","title":{"rendered":"Pallasite paleomagnetism: Quiescence of a core dynamo"},"content":{"rendered":"<p>Claire I.O. Nichols, James F.J. Bryson, Julia Herrero-Albillos, Florian Kronast, Francis Nimmo, Richard J. Harrison<\/p>\n<p>Earth and Planetary Science Letters<br \/>\nVolume 441, 1 May 2016, Pages 103\u2013112<br \/>\nAvailable online 9 March 2016<\/p>\n<p><a href=\"http:\/\/www.sciencedirect.com\/science\/article\/pii\/S0012821X16300541\" target=\"_blank\"><strong>LINK (open access)<\/strong><\/a><\/p>\n<p>&#8220;Recent paleomagnetic studies of two Main Group pallasites, the Imilac and Esquel, have found evidence for a strong, late-stage magnetic field on the parent body. It has been hypothesized that this magnetic field was generated by a core dynamo, driven by compositional convection during core solidification. Cooling models suggest that the onset of core solidification occurred \u223c200 Ma after planetary accretion. Prior to core solidification, a core dynamo may have been generated by thermal convection; however a thermal dynamo is predicted to be short-lived, with a duration of \u223c10 Ma to \u223c40 Ma after planetary accretion. These models predict, therefore, a period of quiescence between the thermally driven dynamo and the compositionally driven dynamo, when no core dynamo should be active. To test this hypothesis, we have measured the magnetic remanence recorded by the Marjalahti and Brenham pallasites, which based on cooling-rate data locked in any magnetic field signals present \u223c95 Ma to \u223c135 Ma after planetary accretion, before core solidification began. The cloudy zone, a region of nanoscale tetrataenite islands within a Fe-rich matrix was imaged using X-ray photoemission electron microscopy. The recovered distribution of magnetisation within the cloudy zone suggests that the Marjalahti and Brenham experienced a very weak magnetic field, which may have been induced by a crustal remanence, consistent with the predicted lack of an active core dynamo at this time. We show that the transition from a quiescent period to an active, compositionally driven dynamo has a distinctive paleomagnetic signature, which may be a crucial tool for constraining the time of core solidification on differentiated bodies, including Earth.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Claire I.O. Nichols, James F.J. Bryson, Julia Herrero-Albillos, Florian Kronast, Francis Nimmo, Richard J. Harrison Earth and Planetary Science Letters Volume 441, 1 May 2016, Pages 103\u2013112 Available online 9 March 2016 LINK (open access)&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[2583,219,810,2580,764],"tags":[2582,2584,2061,930,929,2585,2581,590,1894],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/7988"}],"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=7988"}],"version-history":[{"count":2,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/7988\/revisions"}],"predecessor-version":[{"id":7991,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/7988\/revisions\/7991"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=7988"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=7988"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=7988"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}