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• W1966055051 abstract "Research Article| April 01, 1987 Carbon solubility in olivine: Implications for upper mantle evolution Tracy N. Tingle; Tracy N. Tingle 1Department of Geology, University of California, Davis, California 95616 Search for other works by this author on: GSW Google Scholar Harry W. Green, II Harry W. Green, II 1Department of Geology, University of California, Davis, California 95616 Search for other works by this author on: GSW Google Scholar Author and Article Information Tracy N. Tingle 1Department of Geology, University of California, Davis, California 95616 Harry W. Green, II 1Department of Geology, University of California, Davis, California 95616 Publisher: Geological Society of America First Online: 02 Jun 2017 Online ISSN: 1943-2682 Print ISSN: 0091-7613 Geological Society of America Geology (1987) 15 (4): 324–326. https://doi.org/10.1130/0091-7613(1987)15<324:CSIOIF>2.0.CO;2 Article history First Online: 02 Jun 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn Email Permissions Search Site Citation Tracy N. Tingle, Harry W. Green; Carbon solubility in olivine: Implications for upper mantle evolution. Geology 1987;; 15 (4): 324–326. doi: https://doi.org/10.1130/0091-7613(1987)15<324:CSIOIF>2.0.CO;2 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyGeology Search Advanced Search Abstract Volcanic activity worldwide and carbonaceous phases in mantle xenoliths demonstrate that carbon is present in trace amounts in the modern mantle. We have determined that carbon solubility in olivine at 0.1 GPa and 1200 °C is below our detection limit (30 ppm by weight) but dissolves in excess of 100 ppm wt at 3.0 GPa, 1180–1530 °C. The significant solubility in mantle silicates may explain the rarity of carbonate-bearing xenoliths and the extreme age of diamonds. We propose a model in which low-pressure melting during mantle convection scavenges hydrogen and carbon from the primitive mantle and thereby reduces the content of these volatiles to below the silicate saturation limit and restricts carbonaceous and hydrous phases to the roots of continents isolated from convection. This content is PDF only. Please click on the PDF icon to access. First Page Preview Close Modal You do not have access to this content, please speak to your institutional administrator if you feel you should have access." @default.
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• W1966055051 title "Carbon solubility in olivine: Implications for upper mantle evolution" @default.
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