Gas–Solid Interactions on Venus and Other Solar System Bodies

Research Article| November 01, 2018 Gas–Solid Interactions on Venus and Other Solar System Bodies Mikhail Yu. Zolotov Mikhail Yu. Zolotov School of Earth and Space Exploration, Arizona State University, Tempe AZ 85287, USA Search for other works by this author on: GSW Google Scholar Reviews in Mineralogy and Geochemistry (2018) 84 (1): 351–392. https://doi.org/10.2138/rmg.2018.84.10 Article history first online: 09 Nov 2018 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Mikhail Yu. Zolotov; Gas–Solid Interactions on Venus and Other Solar System Bodies. Reviews in Mineralogy and Geochemistry 2018;; 84 (1): 351–392. doi: https://doi.org/10.2138/rmg.2018.84.10 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 SocietyReviews in Mineralogy and Geochemistry Search Advanced Search Gas–solid reactions on solar system bodies occur in the vicinity of their surfaces and in their interiors where gases are liberated through magma degassing or thermal devolatilization. The reactions are driven by chemical disequilibria created by exogenic (erosion, impacts) and endogenic processes (tectonics, magmatism) that change the composition of gas–solid systems and/or alter temperature and pressure conditions. Typically, the disequilibria are caused by a supply of fresh rocks to a body’s surface, degassing into an atmosphere, transport of gases through rocks, and gas–solid mixing in volcanic and impact environments. On bodies with atmospheres (Venus, Earth, Mars and Titan), gas–solid reactions... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.