Cargando…
Atomic-scale age resolution of planetary events
Resolving the timing of crustal processes and meteorite impact events is central to understanding the formation, evolution and habitability of planetary bodies. However, identifying multi-stage events from complex planetary materials is highly challenging at the length scales of current isotopic tec...
Autores principales: | , , , , , , , , , |
---|---|
Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group
2017
|
Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5477514/ https://www.ncbi.nlm.nih.gov/pubmed/28548083 http://dx.doi.org/10.1038/ncomms15597 |
_version_ | 1783244809326034944 |
---|---|
author | White, L. F. Darling, J. R. Moser, D. E. Reinhard, D. A. Prosa, T. J. Bullen, D. Olson, D. Larson, D. J. Lawrence, D. Martin, I. |
author_facet | White, L. F. Darling, J. R. Moser, D. E. Reinhard, D. A. Prosa, T. J. Bullen, D. Olson, D. Larson, D. J. Lawrence, D. Martin, I. |
author_sort | White, L. F. |
collection | PubMed |
description | Resolving the timing of crustal processes and meteorite impact events is central to understanding the formation, evolution and habitability of planetary bodies. However, identifying multi-stage events from complex planetary materials is highly challenging at the length scales of current isotopic techniques. Here we show that accurate U-Pb isotopic analysis of nanoscale domains of baddeleyite can be achieved by atom probe tomography. Within individual crystals of highly shocked baddeleyite from the Sudbury impact structure, three discrete nanostructural domains have been isolated yielding average (206)Pb/(238)U ages of 2,436±94 Ma (protolith crystallization) from homogenous-Fe domains, 1,852±45 Ma (impact) from clustered-Fe domains and 1,412±56 Ma (tectonic metamorphism) from planar and subgrain boundary structures. Baddeleyite is a common phase in terrestrial, Martian, Lunar and asteroidal materials, meaning this atomic-scale approach holds great potential in establishing a more accurate chronology of the formation and evolution of planetary crusts. |
format | Online Article Text |
id | pubmed-5477514 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2017 |
publisher | Nature Publishing Group |
record_format | MEDLINE/PubMed |
spelling | pubmed-54775142017-07-03 Atomic-scale age resolution of planetary events White, L. F. Darling, J. R. Moser, D. E. Reinhard, D. A. Prosa, T. J. Bullen, D. Olson, D. Larson, D. J. Lawrence, D. Martin, I. Nat Commun Article Resolving the timing of crustal processes and meteorite impact events is central to understanding the formation, evolution and habitability of planetary bodies. However, identifying multi-stage events from complex planetary materials is highly challenging at the length scales of current isotopic techniques. Here we show that accurate U-Pb isotopic analysis of nanoscale domains of baddeleyite can be achieved by atom probe tomography. Within individual crystals of highly shocked baddeleyite from the Sudbury impact structure, three discrete nanostructural domains have been isolated yielding average (206)Pb/(238)U ages of 2,436±94 Ma (protolith crystallization) from homogenous-Fe domains, 1,852±45 Ma (impact) from clustered-Fe domains and 1,412±56 Ma (tectonic metamorphism) from planar and subgrain boundary structures. Baddeleyite is a common phase in terrestrial, Martian, Lunar and asteroidal materials, meaning this atomic-scale approach holds great potential in establishing a more accurate chronology of the formation and evolution of planetary crusts. Nature Publishing Group 2017-05-26 /pmc/articles/PMC5477514/ /pubmed/28548083 http://dx.doi.org/10.1038/ncomms15597 Text en Copyright © 2017, The Author(s) http://creativecommons.org/licenses/by/4.0/ This work is licensed under a Creative Commons Attribution 4.0 International License. The images or other third party material in this article are included in the article's Creative Commons license, unless indicated otherwise in the credit line; if the material is not included under the Creative Commons license, users will need to obtain permission from the license holder to reproduce the material. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/ |
spellingShingle | Article White, L. F. Darling, J. R. Moser, D. E. Reinhard, D. A. Prosa, T. J. Bullen, D. Olson, D. Larson, D. J. Lawrence, D. Martin, I. Atomic-scale age resolution of planetary events |
title | Atomic-scale age resolution of planetary events |
title_full | Atomic-scale age resolution of planetary events |
title_fullStr | Atomic-scale age resolution of planetary events |
title_full_unstemmed | Atomic-scale age resolution of planetary events |
title_short | Atomic-scale age resolution of planetary events |
title_sort | atomic-scale age resolution of planetary events |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC5477514/ https://www.ncbi.nlm.nih.gov/pubmed/28548083 http://dx.doi.org/10.1038/ncomms15597 |
work_keys_str_mv | AT whitelf atomicscaleageresolutionofplanetaryevents AT darlingjr atomicscaleageresolutionofplanetaryevents AT moserde atomicscaleageresolutionofplanetaryevents AT reinhardda atomicscaleageresolutionofplanetaryevents AT prosatj atomicscaleageresolutionofplanetaryevents AT bullend atomicscaleageresolutionofplanetaryevents AT olsond atomicscaleageresolutionofplanetaryevents AT larsondj atomicscaleageresolutionofplanetaryevents AT lawrenced atomicscaleageresolutionofplanetaryevents AT martini atomicscaleageresolutionofplanetaryevents |