Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites
Abstract The behavior of rare earth elements ( REE s) during hot desert weathering of meteorites is investigated. Ordinary chondrites ( OC s) from Atacama (Chile) and Lut (Iran) deserts show different variations in REE composition during this process. Inductively coupled plasma–mass spectrometry ( I...
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crwiley:10.1111/maps.12894 2023-12-03T10:14:06+01:00 Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites Pourkhorsandi, Hamed D'Orazio, Massimo Rochette, Pierre Valenzuela, Millarca Gattacceca, Jérôme Mirnejad, Hassan Sutter, Brad Hutzler, Aurore Aboulahris, Maria CONICYT-FONDECYT 2017 http://dx.doi.org/10.1111/maps.12894 https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fmaps.12894 https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.12894 https://onlinelibrary.wiley.com/doi/full-xml/10.1111/maps.12894 en eng Wiley http://onlinelibrary.wiley.com/termsAndConditions#vor Meteoritics & Planetary Science volume 52, issue 9, page 1843-1858 ISSN 1086-9379 1945-5100 Space and Planetary Science Geophysics journal-article 2017 crwiley https://doi.org/10.1111/maps.12894 2023-11-09T14:14:45Z Abstract The behavior of rare earth elements ( REE s) during hot desert weathering of meteorites is investigated. Ordinary chondrites ( OC s) from Atacama (Chile) and Lut (Iran) deserts show different variations in REE composition during this process. Inductively coupled plasma–mass spectrometry ( ICP ‐ MS ) data reveal that hot desert OC s tend to show elevated light REE concentrations, relative to OC falls. Chondrites from Atacama are by far the most enriched in REE s and this enrichment is not necessarily related to their degree of weathering. Positive Ce anomaly of fresh chondrites from Atacama and the successive formation of a negative Ce anomaly with the addition of trivalent REE s are similar to the process reported from Antarctic eucrites. In addition to REE s, Sr and Ba also show different concentrations when comparing OC s from different hot deserts. The stability of Atacama surfaces and the associated old terrestrial ages of meteorites from this region give the samples the necessary time to interact with the terrestrial environment and to be chemically modified. Higher REE contents and LREE ‐enriched composition are evidence of contamination by terrestrial soil. Despite their low degrees of weathering, special care must be taken into account while working on the REE composition of Atacama meteorites for cosmochemistry applications. In contrast, chondrites from the Lut desert show lower degrees of REE modification, despite significant weathering signed by Sr content. This is explained by the relatively rapid weathering rate of the meteorites occurring in the Lut desert, which hampers the penetration of terrestrial material by forming voluminous Fe oxide/oxyhydroxides shortly after the meteorite fall. Article in Journal/Newspaper Antarc* Antarctic Wiley Online Library (via Crossref) Antarctic Meteoritics & Planetary Science 52 9 1843 1858 |
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Wiley Online Library (via Crossref) |
op_collection_id |
crwiley |
language |
English |
topic |
Space and Planetary Science Geophysics |
spellingShingle |
Space and Planetary Science Geophysics Pourkhorsandi, Hamed D'Orazio, Massimo Rochette, Pierre Valenzuela, Millarca Gattacceca, Jérôme Mirnejad, Hassan Sutter, Brad Hutzler, Aurore Aboulahris, Maria Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
topic_facet |
Space and Planetary Science Geophysics |
description |
Abstract The behavior of rare earth elements ( REE s) during hot desert weathering of meteorites is investigated. Ordinary chondrites ( OC s) from Atacama (Chile) and Lut (Iran) deserts show different variations in REE composition during this process. Inductively coupled plasma–mass spectrometry ( ICP ‐ MS ) data reveal that hot desert OC s tend to show elevated light REE concentrations, relative to OC falls. Chondrites from Atacama are by far the most enriched in REE s and this enrichment is not necessarily related to their degree of weathering. Positive Ce anomaly of fresh chondrites from Atacama and the successive formation of a negative Ce anomaly with the addition of trivalent REE s are similar to the process reported from Antarctic eucrites. In addition to REE s, Sr and Ba also show different concentrations when comparing OC s from different hot deserts. The stability of Atacama surfaces and the associated old terrestrial ages of meteorites from this region give the samples the necessary time to interact with the terrestrial environment and to be chemically modified. Higher REE contents and LREE ‐enriched composition are evidence of contamination by terrestrial soil. Despite their low degrees of weathering, special care must be taken into account while working on the REE composition of Atacama meteorites for cosmochemistry applications. In contrast, chondrites from the Lut desert show lower degrees of REE modification, despite significant weathering signed by Sr content. This is explained by the relatively rapid weathering rate of the meteorites occurring in the Lut desert, which hampers the penetration of terrestrial material by forming voluminous Fe oxide/oxyhydroxides shortly after the meteorite fall. |
author2 |
CONICYT-FONDECYT |
format |
Article in Journal/Newspaper |
author |
Pourkhorsandi, Hamed D'Orazio, Massimo Rochette, Pierre Valenzuela, Millarca Gattacceca, Jérôme Mirnejad, Hassan Sutter, Brad Hutzler, Aurore Aboulahris, Maria |
author_facet |
Pourkhorsandi, Hamed D'Orazio, Massimo Rochette, Pierre Valenzuela, Millarca Gattacceca, Jérôme Mirnejad, Hassan Sutter, Brad Hutzler, Aurore Aboulahris, Maria |
author_sort |
Pourkhorsandi, Hamed |
title |
Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
title_short |
Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
title_full |
Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
title_fullStr |
Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
title_full_unstemmed |
Modification of <scp>REE</scp> distribution of ordinary chondrites from Atacama (Chile) and Lut (Iran) hot deserts: Insights into the chemical weathering of meteorites |
title_sort |
modification of <scp>ree</scp> distribution of ordinary chondrites from atacama (chile) and lut (iran) hot deserts: insights into the chemical weathering of meteorites |
publisher |
Wiley |
publishDate |
2017 |
url |
http://dx.doi.org/10.1111/maps.12894 https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fmaps.12894 https://onlinelibrary.wiley.com/doi/pdf/10.1111/maps.12894 https://onlinelibrary.wiley.com/doi/full-xml/10.1111/maps.12894 |
geographic |
Antarctic |
geographic_facet |
Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_source |
Meteoritics & Planetary Science volume 52, issue 9, page 1843-1858 ISSN 1086-9379 1945-5100 |
op_rights |
http://onlinelibrary.wiley.com/termsAndConditions#vor |
op_doi |
https://doi.org/10.1111/maps.12894 |
container_title |
Meteoritics & Planetary Science |
container_volume |
52 |
container_issue |
9 |
container_start_page |
1843 |
op_container_end_page |
1858 |
_version_ |
1784261178016399360 |