Noble Gases in Meteorites - Trapped Components

Abstract

Research Article| January 01, 2002 Noble Gases in Meteorites – Trapped Components Ulrich Ott Ulrich Ott Max-Planck-Institut für Chemie (Otto-Hahn-Institut), Becherweg 27, D-55128 Mainz, Germany, ott@mcph-mainz.mpg.de Search for other works by this author on: GSW Google Scholar Reviews in Mineralogy and Geochemistry (2002) 47 (1): 71–100. https://doi.org/10.2138/rmg.2002.47.3 Article history first online: 13 Jul 2017 Cite View This Citation Add to Citation Manager Share Icon Share MailTo Twitter LinkedIn Tools Icon Tools Get Permissions Search Site Citation Ulrich Ott; Noble Gases in Meteorites – Trapped Components. Reviews in Mineralogy and Geochemistry 2002;; 47 (1): 71–100. doi: https://doi.org/10.2138/rmg.2002.47.3 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 Fundamental insights in the field of cosmochemistry have come from the study of the abundances and isotopic compositions of trapped noble gases. A case in point is the discovery of presolar grains in primitive meteorites: isotope abundance anomalies in noble gases were known long before the discovery of presolar grains such as nanodiamonds, silicon carbide and graphite, and it was the search for the carrier phases of these anomalies that ultimately led to the identification and isolation of these types of grains (e.g., Anders and Zinner 1993; Ott 1993). Starting with the work of John Reynolds and his... You do not have access to this content, please speak to your institutional administrator if you feel you should have access.