{"id":34481,"date":"2023-11-01T23:41:00","date_gmt":"2023-11-01T22:41:00","guid":{"rendered":"https:\/\/karmaka.de\/?p=34481"},"modified":"2023-11-01T23:47:50","modified_gmt":"2023-11-01T22:47:50","slug":"moon-forming-impactor-as-a-source-of-earths-basal-mantle-anomalies","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=34481","title":{"rendered":"Moon-forming impactor as a source of Earth\u2019s basal mantle anomalies"},"content":{"rendered":"\n<p>Qian Yuan, Mingming Li, Steven J. Desch, Byeongkwan Ko, Hongping Deng, Edward J. Garnero, Travis S. J. Gabriel, Jacob A. Kegerreis, Yoshinori Miyazaki, Vincent Eke &amp; Paul D. Asimow<\/p>\n\n\n\n<p>Nature, Volume 623, pages 95\u201399<br>Published: 01 November 2023<\/p>\n\n\n\n<p><a href=\"https:\/\/www.nature.com\/articles\/s41586-023-06589-1\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;Seismic images of Earth\u2019s interior have revealed two continent-sized anomalies with low seismic velocities, known as the large low-velocity provinces (LLVPs), in the lowermost mantle1. The LLVPs are often interpreted as intrinsically dense heterogeneities that are compositionally distinct from the surrounding mantle2. Here we show that LLVPs may represent buried relics of Theia mantle material (TMM) that was preserved in proto-Earth\u2019s mantle after the Moon-forming giant impact3. Our canonical giant-impact simulations show that a fraction of Theia\u2019s mantle could have been delivered to proto-Earth\u2019s solid lower mantle. We find that TMM is intrinsically 2.0\u20133.5% denser than proto-Earth\u2019s mantle based on models of Theia\u2019s mantle and the observed higher FeO content of the Moon. Our mantle convection models show that dense TMM blobs with a size of tens of kilometres after the impact can later sink and accumulate into LLVP-like thermochemical piles atop Earth\u2019s core and survive to the present day. The LLVPs may, thus, be a natural consequence of the Moon-forming giant impact. Because giant impacts are common at the end stages of planet accretion, similar mantle heterogeneities caused by impacts may also exist in the interiors of other planetary bodies.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Qian Yuan, Mingming Li, Steven J. Desch, Byeongkwan Ko, Hongping Deng, Edward J. Garnero, Travis S. J. Gabriel, Jacob A. Kegerreis, Yoshinori Miyazaki, Vincent Eke &amp; Paul D. Asimow Nature, Volume 623, pages 95\u201399Published: 01&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[112,115],"tags":[1857,2659,1665,114],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/34481"}],"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=34481"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/34481\/revisions"}],"predecessor-version":[{"id":34482,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/34481\/revisions\/34482"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=34481"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=34481"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=34481"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}