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• W2912157437 abstract "Research Article| February 01, 2019 The Origin and Differentiation of Planet Mercury Bernard Charlier; Bernard Charlier Department of Geology, University of Liege, 4000 Sart Tilman, Belgium E-mail: b.charlier@uliege.be Search for other works by this author on: GSW Google Scholar Olivier Namur Olivier Namur Department of Earth and Environmental Sciences, KU Leuven, 3001 Leuven, Belgium E-mail: olivier.namur@kuleuven.be Search for other works by this author on: GSW Google Scholar Author and Article Information Bernard Charlier Department of Geology, University of Liege, 4000 Sart Tilman, Belgium Olivier Namur Department of Earth and Environmental Sciences, KU Leuven, 3001 Leuven, Belgium E-mail: b.charlier@uliege.be E-mail: olivier.namur@kuleuven.be Publisher: Mineralogical Society of America First Online: 11 Feb 2019 Online Issn: 1811-5217 Print Issn: 1811-5209 Copyright © 2019 by the Mineralogical Society of AmericaMineralogical Society of America Elements (2019) 15 (1): 9–14. https://doi.org/10.2138/gselements.15.1.9 Article history First Online: 11 Feb 2019 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Bernard Charlier, Olivier Namur; The Origin and Differentiation of Planet Mercury. Elements 2019;; 15 (1): 9–14. doi: https://doi.org/10.2138/gselements.15.1.9 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 SocietyElements Search Advanced Search Unique physical and chemical characteristics of Mercury have been revealed by measurements from NASA's MESSENGER spacecraft. The closest planet to our Sun is made up of a large metallic core that is partially liquid, a thin mantle thought to be formed by solidification of a silicate magma ocean, and a relatively thick secondary crust produced by partial melting of the mantle followed by volcanic eruptions. However, the origin of the large metal/silicate ratio of the bulk planet and the conditions of accretion remain elusive. Metal enrichment may originate from primordial processes in the solar nebula or from a giant impact that stripped most of the silicate portion of a larger planet leaving Mercury as we know it today. 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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• W2912157437 title "The Origin and Differentiation of Planet Mercury" @default.
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