4.5 Article

Clay mineral evolution

期刊

AMERICAN MINERALOGIST
卷 98, 期 11-12, 页码 2007-2029

出版社

MINERALOGICAL SOC AMER
DOI: 10.2138/am.2013.4425

关键词

Clay minerals; biominerals; weathering; diagenesis; Mars mineralogy

资金

  1. National Science Foundation
  2. NASA Astrobiology Institute
  3. Deep Carbon Observatory
  4. Carnegie Institution of Washington, D.C.

向作者/读者索取更多资源

Changes in the mechanisms of formation and global distribution of phyllosilicate clay minerals through 4.567 Ga of planetary evolution in our solar system reflect evolving tectonic, geochemical, and biological processes. Clay minerals were absent prior to planetesimal formation similar to 4.6 billion years ago but today are abundant in all near-surface Earth environments. New clay mineral species and modes of clay mineral paragenesis occurred as a consequence of major events in Earth's evolution notably the formation of a mafic crust and oceans, the emergence of granite-rooted continents, the initiation of plate tectonics and subduction, the Great Oxidation Event, and the rise of the terrestrial biosphere. The changing character of clay minerals through time is thus an important part of Earth's mineralogical history and exemplifies the principles of mineral evolution.

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