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The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters
The only martian rock samples on Earth are meteorites ejected from the surface of Mars by asteroid impacts. The locations and geological contexts of the launch sites are currently unknown. Determining the impact locations is essential to unravel the relations between the evolution of the martian int...
Autores principales: | , , , , , , , , , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Nature Publishing Group UK
2021
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8566585/ https://www.ncbi.nlm.nih.gov/pubmed/34732704 http://dx.doi.org/10.1038/s41467-021-26648-3 |
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author | Lagain, A. Benedix, G. K. Servis, K. Baratoux, D. Doucet, L. S. Rajšic, A. Devillepoix, H. A. R. Bland, P. A. Towner, M. C. Sansom, E. K. Miljković, K. |
author_facet | Lagain, A. Benedix, G. K. Servis, K. Baratoux, D. Doucet, L. S. Rajšic, A. Devillepoix, H. A. R. Bland, P. A. Towner, M. C. Sansom, E. K. Miljković, K. |
author_sort | Lagain, A. |
collection | PubMed |
description | The only martian rock samples on Earth are meteorites ejected from the surface of Mars by asteroid impacts. The locations and geological contexts of the launch sites are currently unknown. Determining the impact locations is essential to unravel the relations between the evolution of the martian interior and its surface. Here we adapt a Crater Detection Algorithm that compile a database of 90 million impact craters, allowing to determine the potential launch position of these meteorites through the observation of secondary crater fields. We show that Tooting and 09-000015 craters, both located in the Tharsis volcanic province, are the most likely source of the depleted shergottites ejected 1.1 million year ago. This implies that a major thermal anomaly deeply rooted in the mantle under Tharsis was active over most of the geological history of the planet, and has sampled a depleted mantle, that has retained until recently geochemical signatures of Mars’ early history. |
format | Online Article Text |
id | pubmed-8566585 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2021 |
publisher | Nature Publishing Group UK |
record_format | MEDLINE/PubMed |
spelling | pubmed-85665852021-11-15 The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters Lagain, A. Benedix, G. K. Servis, K. Baratoux, D. Doucet, L. S. Rajšic, A. Devillepoix, H. A. R. Bland, P. A. Towner, M. C. Sansom, E. K. Miljković, K. Nat Commun Article The only martian rock samples on Earth are meteorites ejected from the surface of Mars by asteroid impacts. The locations and geological contexts of the launch sites are currently unknown. Determining the impact locations is essential to unravel the relations between the evolution of the martian interior and its surface. Here we adapt a Crater Detection Algorithm that compile a database of 90 million impact craters, allowing to determine the potential launch position of these meteorites through the observation of secondary crater fields. We show that Tooting and 09-000015 craters, both located in the Tharsis volcanic province, are the most likely source of the depleted shergottites ejected 1.1 million year ago. This implies that a major thermal anomaly deeply rooted in the mantle under Tharsis was active over most of the geological history of the planet, and has sampled a depleted mantle, that has retained until recently geochemical signatures of Mars’ early history. Nature Publishing Group UK 2021-11-03 /pmc/articles/PMC8566585/ /pubmed/34732704 http://dx.doi.org/10.1038/s41467-021-26648-3 Text en © The Author(s) 2021 https://creativecommons.org/licenses/by/4.0/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/ (https://creativecommons.org/licenses/by/4.0/) . |
spellingShingle | Article Lagain, A. Benedix, G. K. Servis, K. Baratoux, D. Doucet, L. S. Rajšic, A. Devillepoix, H. A. R. Bland, P. A. Towner, M. C. Sansom, E. K. Miljković, K. The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title | The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title_full | The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title_fullStr | The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title_full_unstemmed | The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title_short | The Tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
title_sort | tharsis mantle source of depleted shergottites revealed by 90 million impact craters |
topic | Article |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8566585/ https://www.ncbi.nlm.nih.gov/pubmed/34732704 http://dx.doi.org/10.1038/s41467-021-26648-3 |
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