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• W2085383657 abstract "Research Article| June 01, 2006 Aqueous Processes Recorded by Martian Meteorites: Analyzing Martian Water on Earth Laurie A. Leshin; Laurie A. Leshin 1Sciences and Exploration Directorate NASA Goddard Space Flight Center Greenbelt, MD 20771, USA E-mail: laurie.leshin@nasa.gov Search for other works by this author on: GSW Google Scholar Edward Vicenzi Edward Vicenzi 2Department of Mineral Sciences National Museum of National History Smithsonian Institution Washington, DC 20560, USA E-mail: vicenzi@volcano.si.edu Search for other works by this author on: GSW Google Scholar Author and Article Information Laurie A. Leshin 1Sciences and Exploration Directorate NASA Goddard Space Flight Center Greenbelt, MD 20771, USA E-mail: laurie.leshin@nasa.gov Edward Vicenzi 2Department of Mineral Sciences National Museum of National History Smithsonian Institution Washington, DC 20560, USA E-mail: vicenzi@volcano.si.edu Publisher: Mineralogical Society of America First Online: 09 Mar 2017 Online ISSN: 1811-5217 Print ISSN: 1811-5209 © 2006 by the Mineralogical Society of America Elements (2006) 2 (3): 157–162. https://doi.org/10.2113/gselements.2.3.157 Article history First Online: 09 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation Laurie A. Leshin, Edward Vicenzi; Aqueous Processes Recorded by Martian Meteorites: Analyzing Martian Water on Earth. Elements 2006;; 2 (3): 157–162. doi: https://doi.org/10.2113/gselements.2.3.157 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 Abstract Martian meteorites have delivered to Earth water molecules and minerals produced by aqueous processes on Mars. The study of these samples, using powerful analytical instrumentation, provides a basis for understanding aqueous activity on Mars. Although most analyses are at the scale of microns, the conclusions reached have important implications for large-scale aqueous processes. Secondary minerals, such as clays, salts, and carbonates, are present at some level in all Martian meteorite subtypes and are especially important in the nakhlites and ALH84001. Light element stable isotope analyses show evidence for mixing between atmosphere and magmatic fluids into a crustal reservoir, and that this crustal water was not in equilibrium with the host rocks. The mineralogical and isotopic data present a fairly consistent picture of the aqueous history of Mars: low levels of aqueous alteration are generally present but extensive aqueous processes are probably limited in space and time. 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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