Shock effects in feldspars: An overview

Author:

Pickersgill* Annemarie E.1,Jaret Steven J.2,Pittarello Lidia3,Fritz Jörg4,Harris R. Scott5

Affiliation:

1. School of Geographical & Earth Sciences, University of Glasgow, Gregory Building, Lilybank Gardens, Glasgow G12 8QQ, UK

2. Department of Earth and Planetary Sciences, American Museum of Natural History, New York, New York 10024, USA

3. Natural History Museum Vienna, Department of Mineralogy and Petrography, Burgring 7, A-1010 Vienna, Austria

4. Saalbau Weltraum Projekt, Liebigstraße 6, 64646 Heppenheim, Germany, and Zentrum für Rieskrater und Impaktforschung Nördlingen (ZERIN), Vordere Gerbergasse 3, 86720 Nördlingen, Germany

5. Department of Space Sciences, Fernbank Science Center, 156 Heaton Park Drive, Atlanta, Georgia 30307, USA

Abstract

ABSTRACT Feldspars are the dominant mineral in the crust of most terrestrial planetary bodies, including Earth, Earth’s moon, and Mars, as well as in asteroids, and thus in meteorites. These bodies have experienced large numbers of hypervelocity impact events, and so it is important to have a robust understanding of the effects of shock waves exerted on feldspars. However, due to their optical complexity and susceptibility to weathering, feldspars are underutilized as shock barometers and indicators of hypervelocity impact. Here, we provide an overview of the work done on shocked feldspars so far, in an effort to better frame the current strengths and weaknesses of different techniques, and to highlight some gaps in the literature.

Publisher

Geological Society of America

Reference209 articles.

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2. Shock compression of feldspars;Ahrens;Journal of Geophysical Research,1969

3. Shock compression of a recrystallized anorthositic rock from Apollo 15;Ahrens;Proceedings of the 4th Lunar Science Conference: Geochimica et Cosmochimica Acta,1973

4. High-pressure structure of anorthite;Angel;The American Mineralogist,1988

5. Feldspars at high pressure;Angel,1994

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