Shock compaction heating and collisional processes in the production of type 3 ordinary chondrites: Lessons from the (nearly) unique L3 chondrite melt breccia Northwest Africa 8709-Reference-Cited by-同舟云学术

Shock compaction heating and collisional processes in the production of type 3 ordinary chondrites: Lessons from the (nearly) unique L3 chondrite melt breccia Northwest Africa 8709

Published:2020-09 Issue:9 Volume:55 Page:2117-2140
ISSN:1086-9379
Container-title:Meteoritics & Planetary Science
language:en
Short-container-title:Meteorit Planet Sci

Author:

Ruzicka Alex M.¹^ORCID,Friedrich Jon M.²³^ORCID,Hutson Melinda L.¹,Strasser Juliette W.²,Macke Robert J.⁴^ORCID,Rivers Mark L.⁵,Greenwood Richard C.⁶,Ziegler Karen⁷,Pugh Richard N.¹

Affiliation:

1. Department of Geology and Cascadia Meteorite Laboratory Portland State University 17 Cramer Hall, 1721 SW Broadway Portland Oregon97201USA

2. Department of Chemistry Fordham University 441 East Fordham Road Bronx New York10458USA

3. Department of Earth and Planetary Sciences American Museum of Natural History 79th Street at Central Park West New York City New York10024USA

4. Vatican Observatory Vatican CityV‐00120Italy

5. Center for Advanced Radiation Sources University of Chicago Argonne Illinois60439USA

6. Planetary Sciences Research Institute The Open University Walton Hall Milton KeynesMK7 6AAUK

7. Institute of Meteoritics University of New Mexico Albuquerque New Mexico87131USA

Funder

National Aeronautics and Space Administration

Portland State University

U.S. Department of Energy

Henry Luce Foundation

Publisher

Wiley

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.13567

Reference75 articles.

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2. Impact history of the Chelyabinsk meteorite: Electron microprobe and LA-ICP-MS study of sulfides and metals

3. Experiments on the consolidation of chondrites and the formation of dense rims around chondrules

4. The formation and chronology of the PAT 91501 impact-melt L chondrite with vesicle–metal–sulfide assemblages

5. Shock stage distribution of 2280 ordinary chondrites—Can bulk chondrites with a shock stage of S6 exist as individual rocks?

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