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Silica-rich volcanism in the early solar system dated at 4.565 Ga
The ranges in chemical composition of ancient achondrite meteorites are key to understanding the diversity and geochemical evolution of planetary building blocks. These achondrites record the first episodes of volcanism and crust formation, the majority of which are basaltic. Here we report data on...
Autores principales: | , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Nature Publishing Group UK
2018
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6072707/ https://www.ncbi.nlm.nih.gov/pubmed/30072693 http://dx.doi.org/10.1038/s41467-018-05501-0 |
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author | Srinivasan, Poorna Dunlap, Daniel R. Agee, Carl B. Wadhwa, Meenakshi Coleff, Daniel Ziegler, Karen Zeigler, Ryan McCubbin, Francis M. |
author_facet | Srinivasan, Poorna Dunlap, Daniel R. Agee, Carl B. Wadhwa, Meenakshi Coleff, Daniel Ziegler, Karen Zeigler, Ryan McCubbin, Francis M. |
author_sort | Srinivasan, Poorna |
collection | PubMed |
description | The ranges in chemical composition of ancient achondrite meteorites are key to understanding the diversity and geochemical evolution of planetary building blocks. These achondrites record the first episodes of volcanism and crust formation, the majority of which are basaltic. Here we report data on recently discovered volcanic meteorite Northwest Africa (NWA) 11119, which represents the first, and oldest, silica-rich (andesitic to dacitic) porphyritic extrusive crustal rock with an Al–Mg age of 4564.8 ± 0.3 Ma. This unique rock contains mm-sized vesicles/cavities and phenocrysts that are surrounded by quench melt. Additionally, it possesses the highest modal abundance (30 vol%) of free silica (i.e., tridymite) compared to all known meteorites. NWA 11119 substantially widens the range of volcanic rock compositions produced within the first 2.5–3.5 million years of Solar System history, and provides direct evidence that chemically evolved crustal rocks were forming on planetesimals prior to the assembly of the terrestrial planets. |
format | Online Article Text |
id | pubmed-6072707 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2018 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-60727072018-08-06 Silica-rich volcanism in the early solar system dated at 4.565 Ga Srinivasan, Poorna Dunlap, Daniel R. Agee, Carl B. Wadhwa, Meenakshi Coleff, Daniel Ziegler, Karen Zeigler, Ryan McCubbin, Francis M. Nat Commun Article The ranges in chemical composition of ancient achondrite meteorites are key to understanding the diversity and geochemical evolution of planetary building blocks. These achondrites record the first episodes of volcanism and crust formation, the majority of which are basaltic. Here we report data on recently discovered volcanic meteorite Northwest Africa (NWA) 11119, which represents the first, and oldest, silica-rich (andesitic to dacitic) porphyritic extrusive crustal rock with an Al–Mg age of 4564.8 ± 0.3 Ma. This unique rock contains mm-sized vesicles/cavities and phenocrysts that are surrounded by quench melt. Additionally, it possesses the highest modal abundance (30 vol%) of free silica (i.e., tridymite) compared to all known meteorites. NWA 11119 substantially widens the range of volcanic rock compositions produced within the first 2.5–3.5 million years of Solar System history, and provides direct evidence that chemically evolved crustal rocks were forming on planetesimals prior to the assembly of the terrestrial planets. Nature Publishing Group UK 2018-08-02 /pmc/articles/PMC6072707/ /pubmed/30072693 http://dx.doi.org/10.1038/s41467-018-05501-0 Text en © The Author(s) 2018 Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/. |
spellingShingle | Article Srinivasan, Poorna Dunlap, Daniel R. Agee, Carl B. Wadhwa, Meenakshi Coleff, Daniel Ziegler, Karen Zeigler, Ryan McCubbin, Francis M. Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title | Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title_full | Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title_fullStr | Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title_full_unstemmed | Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title_short | Silica-rich volcanism in the early solar system dated at 4.565 Ga |
title_sort | silica-rich volcanism in the early solar system dated at 4.565 ga |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC6072707/ https://www.ncbi.nlm.nih.gov/pubmed/30072693 http://dx.doi.org/10.1038/s41467-018-05501-0 |
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