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Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites
Nakhlite meteorites are ~1.4 to 1.3 Ga old igneous rocks, aqueously altered on Mars ~630 Ma ago. We test the theory that water-rock interaction was impact driven. Electron backscatter diffraction demonstrates that the meteorites Miller Range 03346 and Lafayette were heterogeneously deformed, leading...
Autores principales: | , , , , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
American Association for the Advancement of Science
2019
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6726442/ https://www.ncbi.nlm.nih.gov/pubmed/31517047 http://dx.doi.org/10.1126/sciadv.aaw5549 |
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author | Daly, L. Lee, M. R. Piazolo, S. Griffin, S. Bazargan, M. Campanale, F. Chung, P. Cohen, B. E. Pickersgill, A. E. Hallis, L. J. Trimby, P. W. Baumgartner, R. Forman, L. V. Benedix, G. K. |
author_facet | Daly, L. Lee, M. R. Piazolo, S. Griffin, S. Bazargan, M. Campanale, F. Chung, P. Cohen, B. E. Pickersgill, A. E. Hallis, L. J. Trimby, P. W. Baumgartner, R. Forman, L. V. Benedix, G. K. |
author_sort | Daly, L. |
collection | PubMed |
description | Nakhlite meteorites are ~1.4 to 1.3 Ga old igneous rocks, aqueously altered on Mars ~630 Ma ago. We test the theory that water-rock interaction was impact driven. Electron backscatter diffraction demonstrates that the meteorites Miller Range 03346 and Lafayette were heterogeneously deformed, leading to localized regions of brecciation, plastic deformation, and mechanical twinning of augite. Numerical modeling shows that the pattern of deformation is consistent with shock-generated compressive and tensile stresses. Mesostasis within shocked areas was aqueously altered to phyllosilicates, carbonates, and oxides, suggesting a genetic link between the two processes. We propose that an impact ~630 Ma ago simultaneously deformed the nakhlite parent rocks and generated liquid water by melting of permafrost. Ensuing water-rock interaction focused on shocked mesostasis with a high density of reactive sites. The nakhlite source location must have two spatially correlated craters, one ~630 Ma old and another, ejecting the meteorites, ~11 Ma ago. |
format | Online Article Text |
id | pubmed-6726442 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2019 |
publisher | American Association for the Advancement of Science |
record_format | MEDLINE/PubMed |
spelling | pubmed-67264422019-09-12 Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites Daly, L. Lee, M. R. Piazolo, S. Griffin, S. Bazargan, M. Campanale, F. Chung, P. Cohen, B. E. Pickersgill, A. E. Hallis, L. J. Trimby, P. W. Baumgartner, R. Forman, L. V. Benedix, G. K. Sci Adv Research Articles Nakhlite meteorites are ~1.4 to 1.3 Ga old igneous rocks, aqueously altered on Mars ~630 Ma ago. We test the theory that water-rock interaction was impact driven. Electron backscatter diffraction demonstrates that the meteorites Miller Range 03346 and Lafayette were heterogeneously deformed, leading to localized regions of brecciation, plastic deformation, and mechanical twinning of augite. Numerical modeling shows that the pattern of deformation is consistent with shock-generated compressive and tensile stresses. Mesostasis within shocked areas was aqueously altered to phyllosilicates, carbonates, and oxides, suggesting a genetic link between the two processes. We propose that an impact ~630 Ma ago simultaneously deformed the nakhlite parent rocks and generated liquid water by melting of permafrost. Ensuing water-rock interaction focused on shocked mesostasis with a high density of reactive sites. The nakhlite source location must have two spatially correlated craters, one ~630 Ma old and another, ejecting the meteorites, ~11 Ma ago. American Association for the Advancement of Science 2019-09-04 /pmc/articles/PMC6726442/ /pubmed/31517047 http://dx.doi.org/10.1126/sciadv.aaw5549 Text en Copyright © 2019 The Authors, some rights reserved; exclusive licensee American Association for the Advancement of Science. No claim to original U.S. Government Works. Distributed under a Creative Commons Attribution License 4.0 (CC BY). http://creativecommons.org/licenses/by/4.0/ This is an open-access article distributed under the terms of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/4.0/) , which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. |
spellingShingle | Research Articles Daly, L. Lee, M. R. Piazolo, S. Griffin, S. Bazargan, M. Campanale, F. Chung, P. Cohen, B. E. Pickersgill, A. E. Hallis, L. J. Trimby, P. W. Baumgartner, R. Forman, L. V. Benedix, G. K. Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title | Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title_full | Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title_fullStr | Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title_full_unstemmed | Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title_short | Boom boom pow: Shock-facilitated aqueous alteration and evidence for two shock events in the Martian nakhlite meteorites |
title_sort | boom boom pow: shock-facilitated aqueous alteration and evidence for two shock events in the martian nakhlite meteorites |
topic | Research Articles |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6726442/ https://www.ncbi.nlm.nih.gov/pubmed/31517047 http://dx.doi.org/10.1126/sciadv.aaw5549 |
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