{"id":16917,"date":"2018-12-10T21:43:48","date_gmt":"2018-12-10T20:43:48","guid":{"rendered":"http:\/\/karmaka.de\/?p=16917"},"modified":"2018-12-10T21:43:50","modified_gmt":"2018-12-10T20:43:50","slug":"an-aqueously-altered-carbon-rich-ceres","status":"publish","type":"post","link":"https:\/\/karmaka.de\/?p=16917","title":{"rendered":"An aqueously altered carbon-rich Ceres"},"content":{"rendered":"\n<p>S. Marchi, A. Raponi, T. H. Prettyman, M. C. De Sanctis, J. Castillo-Rogez, C. A. Raymond, E. Ammannito, T. Bowling, M. Ciarniello, H. Kaplan, E. Palomba, C. T. Russell, V. Vinogradoff &amp; N. Yamashita <\/p>\n\n\n\n<p>Nature Astronomy (2018) <\/p>\n\n\n\n<p><a href=\"https:\/\/www.nature.com\/articles\/s41550-018-0656-0\" target=\"_blank\" rel=\"noreferrer noopener\"><strong>LINK<\/strong><\/a><\/p>\n\n\n\n<p class=\"justify-text\">&#8220;The surface mineralogy of dwarf planet Ceres appears to be dominated by products of rock\u2013fluid interactions, such as phyllosilicates\u2014some of which are NH4-bearing\u2014and carbonates1,2,3. Elemental concentrations derived from the inferred mineral mixing fractions, however, do not match measurements of H, C, K and Fe on Ceres4. A complicating factor in assessing Ceres\u2019s unique surface composition is the secular accretion of asteroids typical of chondritic compositions. Here we show that Ceres\u2019s mineral and elemental data can be explained by the presence of carbonaceous chondritic-like materials (~50\u201360\u2009vol%), possibly due to infalling asteroids, admixed with aqueously altered endogenic materials that contain higher-than-chondritic concentrations of carbon. We find that Ceres\u2019s surface may contain up to 20\u2009wt% of carbon, which is more than five times higher than in carbonaceous chondrites. The coexistence of phyllosilicates, magnetite, carbonates and a high carbon content implies rock\u2013water alteration played an important role in promoting widespread carbon chemistry. These findings unveil pathways for the synthesis of organic matter, with implications for their transport across the Solar System.&#8221;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>S. Marchi, A. Raponi, T. H. Prettyman, M. C. De Sanctis, J. Castillo-Rogez, C. A. Raymond, E. Ammannito, T. Bowling, M. Ciarniello, H. Kaplan, E. Palomba, C. T. Russell, V. Vinogradoff &amp; N. Yamashita Nature&#8230;<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[9,167,1700,8],"tags":[3273,701,1868,994,330],"_links":{"self":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16917"}],"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=16917"}],"version-history":[{"count":1,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16917\/revisions"}],"predecessor-version":[{"id":16918,"href":"https:\/\/karmaka.de\/index.php?rest_route=\/wp\/v2\/posts\/16917\/revisions\/16918"}],"wp:attachment":[{"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=16917"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=16917"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/karmaka.de\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=16917"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}